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Otomo M, Osawa SI, Suzuki K, Kakinuma K, Ukishiro K, Suzuki H, Niizuma K, Narita N, Nakasato N, Tominaga T. Bilateral and asymmetrical localization of language function identified by the superselective infusion of propofol in an epilepsy patient with a mild malformation of cortical development: illustrative case. J Neurosurg Case Lessons 2023; 6:CASE23451. [PMID: 38145562 PMCID: PMC10751223 DOI: 10.3171/case23451] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/19/2023] [Accepted: 11/16/2023] [Indexed: 12/27/2023]
Abstract
BACKGROUND Atypical localization of language function can result in unexpected postsurgical deficits after cortical resection, but it is difficult to predict the risk in the presurgical evaluation. The authors experienced a rare case of the bilateral and independent existence of different components of language function identified by segmented evaluation of anatomical anterior and posterior language areas using the superselective infusion of propofol. OBSERVATIONS A 32-year-old right-handed female presented with drug-resistant epilepsy. Comprehensive epilepsy evaluation suggested that the epileptic foci involved the whole left frontal lobe but provided less evidence of structural abnormality. To estimate the extent of functional deterioration likely to be caused by an extended left frontal lobectomy, the authors evaluated segmented cortical function in the ipsi- and contralateral hemispheres by the superselective infusion of propofol into the branches of the intracranial artery. The results revealed bilateral and asymmetrical localization of language function because the patient presented with different components of aphasia in each hemisphere. Based on the authors' assessment of her functional tolerance, an extended left frontal lobectomy was performed and resulted in neurological deficits within the anticipated range. LESSONS An accurate understanding of the correlations between vascular and functional anatomy and the highly specific evaluation of language function provides more advanced presurgical assessment, allowing more tailored planning of cortical resection.
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Affiliation(s)
| | | | | | | | | | - Hiroyoshi Suzuki
- Department of Pathology, Sendai Medical Center, Sendai, Miyagi, Japan
| | - Kuniyasu Niizuma
- Departments of Neurosurgery
- Neurosurgical Engineering and Translational Neuroscience, Tohoku University Graduate School of Medicine, Sendai, Miyagi, Japan
- Department of Neurosurgical Engineering and Translational Neuroscience, Graduate School of Biomedical Engineering, Tohoku University, Sendai, Miyagi, Japan; and
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
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Luque R, Osborn HP, Leleu A, Pallé E, Bonfanti A, Barragán O, Wilson TG, Broeg C, Cameron AC, Lendl M, Maxted PFL, Alibert Y, Gandolfi D, Delisle JB, Hooton MJ, Egger JA, Nowak G, Lafarga M, Rapetti D, Twicken JD, Morales JC, Carleo I, Orell-Miquel J, Adibekyan V, Alonso R, Alqasim A, Amado PJ, Anderson DR, Anglada-Escudé G, Bandy T, Bárczy T, Barrado Navascues D, Barros SCC, Baumjohann W, Bayliss D, Bean JL, Beck M, Beck T, Benz W, Billot N, Bonfils X, Borsato L, Boyle AW, Brandeker A, Bryant EM, Cabrera J, Carrazco-Gaxiola S, Charbonneau D, Charnoz S, Ciardi DR, Cochran WD, Collins KA, Crossfield IJM, Csizmadia S, Cubillos PE, Dai F, Davies MB, Deeg HJ, Deleuil M, Deline A, Delrez L, Demangeon ODS, Demory BO, Ehrenreich D, Erikson A, Esparza-Borges E, Falk B, Fortier A, Fossati L, Fridlund M, Fukui A, Garcia-Mejia J, Gill S, Gillon M, Goffo E, Gómez Maqueo Chew Y, Güdel M, Guenther EW, Günther MN, Hatzes AP, Helling C, Hesse KM, Howell SB, Hoyer S, Ikuta K, Isaak KG, Jenkins JM, Kagetani T, Kiss LL, Kodama T, Korth J, Lam KWF, Laskar J, Latham DW, Lecavelier des Etangs A, Leon JPD, Livingston JH, Magrin D, Matson RA, Matthews EC, Mordasini C, Mori M, Moyano M, Munari M, Murgas F, Narita N, Nascimbeni V, Olofsson G, Osborne HLM, Ottensamer R, Pagano I, Parviainen H, Peter G, Piotto G, Pollacco D, Queloz D, Quinn SN, Quirrenbach A, Ragazzoni R, Rando N, Ratti F, Rauer H, Redfield S, Ribas I, Ricker GR, Rudat A, Sabin L, Salmon S, Santos NC, Scandariato G, Schanche N, Schlieder JE, Seager S, Ségransan D, Shporer A, Simon AE, Smith AMS, Sousa SG, Stalport M, Szabó GM, Thomas N, Tuson A, Udry S, Vanderburg AM, Van Eylen V, Van Grootel V, Venturini J, Walter I, Walton NA, Watanabe N, Winn JN, Zingales T. A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067. Nature 2023; 623:932-937. [PMID: 38030780 DOI: 10.1038/s41586-023-06692-3] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/02/2023] [Accepted: 09/28/2023] [Indexed: 12/01/2023]
Abstract
Planets with radii between that of the Earth and Neptune (hereafter referred to as 'sub-Neptunes') are found in close-in orbits around more than half of all Sun-like stars1,2. However, their composition, formation and evolution remain poorly understood3. The study of multiplanetary systems offers an opportunity to investigate the outcomes of planet formation and evolution while controlling for initial conditions and environment. Those in resonance (with their orbital periods related by a ratio of small integers) are particularly valuable because they imply a system architecture practically unchanged since its birth. Here we present the observations of six transiting planets around the bright nearby star HD 110067. We find that the planets follow a chain of resonant orbits. A dynamical study of the innermost planet triplet allowed the prediction and later confirmation of the orbits of the rest of the planets in the system. The six planets are found to be sub-Neptunes with radii ranging from 1.94R⊕ to 2.85R⊕. Three of the planets have measured masses, yielding low bulk densities that suggest the presence of large hydrogen-dominated atmospheres.
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Affiliation(s)
- R Luque
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA.
| | - H P Osborn
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - A Leleu
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
| | - E Pallé
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- Departamento de Astrofisica, Universidad de La Laguna, La Laguna, Tenerife, Spain
| | - A Bonfanti
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - O Barragán
- Sub-department of Astrophysics, Department of Physics, University of Oxford, Oxford, UK
| | - T G Wilson
- Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews, St Andrews, UK
- Department of Physics, University of Warwick, Coventry, UK
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
| | - C Broeg
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - A Collier Cameron
- Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews, St Andrews, UK
| | - M Lendl
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
| | - P F L Maxted
- Astrophysics Group, Lennard Jones Building, Keele University, Keele, UK
| | - Y Alibert
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - D Gandolfi
- Dipartimento di Fisica, Universita degli Studi di Torino, Torino, Italy
| | - J-B Delisle
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
| | - M J Hooton
- Cavendish Laboratory, University of Cambridge, Cambridge, UK
| | - J A Egger
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
| | - G Nowak
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- Departamento de Astrofisica, Universidad de La Laguna, La Laguna, Tenerife, Spain
- Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Toruń, Poland
| | - M Lafarga
- Department of Physics, University of Warwick, Coventry, UK
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
| | - D Rapetti
- NASA Ames Research Center, Moffett Field, CA, USA
- Research Institute for Advanced Computer Science, Universities Space Research Association, Washington, DC, USA
| | - J D Twicken
- NASA Ames Research Center, Moffett Field, CA, USA
- SETI Institute, Mountain View, CA, USA
| | - J C Morales
- Institut de Ciencies de l'Espai (ICE-CSIC), Bellaterra, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), Barcelona, Spain
| | - I Carleo
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- INAF - Osservatorio Astrofisico di Torino, Pino Torinese, Italy
| | - J Orell-Miquel
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- Departamento de Astrofisica, Universidad de La Laguna, La Laguna, Tenerife, Spain
| | - V Adibekyan
- Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, Porto, Portugal
- Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, Porto, Portugal
| | - R Alonso
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- Departamento de Astrofisica, Universidad de La Laguna, La Laguna, Tenerife, Spain
| | - A Alqasim
- Mullard Space Science Laboratory, University College London, Dorking, UK
| | - P J Amado
- Instituto de Astrofísica de Andalucía (IAA-CSIC), Granada, Spain
| | - D R Anderson
- Department of Physics, University of Warwick, Coventry, UK
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
| | - G Anglada-Escudé
- Institut de Ciencies de l'Espai (ICE-CSIC), Bellaterra, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), Barcelona, Spain
| | - T Bandy
- European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Noordwijk, The Netherlands
| | | | | | - S C C Barros
- Instituto de Astrofisica e Ciencias do Espaco, Universidade do Porto, Porto, Portugal
- Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto, Porto, Portugal
| | - W Baumjohann
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - D Bayliss
- Department of Physics, University of Warwick, Coventry, UK
| | - J L Bean
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | - M Beck
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
| | - T Beck
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
| | - W Benz
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - N Billot
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
| | - X Bonfils
- Université Grenoble Alpes, CNRS, IPAG, Grenoble, France
| | - L Borsato
- INAF - Osservatorio Astronomico di Padova, Padova, Italy
| | - A W Boyle
- Department of Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - A Brandeker
- Department of Astronomy, Stockholm University, AlbaNova University Center, Stockholm, Sweden
| | - E M Bryant
- Department of Physics, University of Warwick, Coventry, UK
- Mullard Space Science Laboratory, University College London, Dorking, UK
| | - J Cabrera
- Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany
| | - S Carrazco-Gaxiola
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de México, Mexico
- Department of Physics and Astronomy, Georgia State University, Atlanta, GA, USA
- RECONS Institute, Chambersburg, PA, USA
| | - D Charbonneau
- Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA
| | - S Charnoz
- Université de Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France
| | - D R Ciardi
- Department of Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - W D Cochran
- McDonald Observatory, The University of Texas, Austin, TX, USA
- Center for Planetary Systems Habitability, The University of Texas, Austin, TX, USA
| | - K A Collins
- Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA
| | - I J M Crossfield
- Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
| | - Sz Csizmadia
- Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany
| | - P E Cubillos
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
- INAF - Osservatorio Astrofisico di Torino, Pino Torinese, Italy
| | - F Dai
- Department of Astronomy, California Institute of Technology, Pasadena, CA, USA
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - M B Davies
- Centre for Mathematical Sciences, Lund University, Lund, Sweden
| | - H J Deeg
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- Departamento de Astrofisica, Universidad de La Laguna, La Laguna, Tenerife, Spain
| | - M Deleuil
- Aix Marseille Univ., CNRS, CNES, LAM, Marseille, France
| | - A Deline
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
| | - L Delrez
- Astrobiology Research Unit, Université de Liège, Liège, Belgium
- Space sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège, Liège, Belgium
| | - O D S Demangeon
- Instituto de Astrofisica e Ciencias do Espaco, Universidade do Porto, Porto, Portugal
- Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto, Porto, Portugal
| | - B-O Demory
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - D Ehrenreich
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
- Centre Vie dans l'Univers, Faculté des sciences, Université de Genève, Genève 4, Switzerland
| | - A Erikson
- Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany
| | - E Esparza-Borges
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- Departamento de Astrofisica, Universidad de La Laguna, La Laguna, Tenerife, Spain
| | - B Falk
- Space Telescope Science Institute, Baltimore, MD, USA
| | - A Fortier
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - L Fossati
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - M Fridlund
- Leiden Observatory, University of Leiden, Leiden, The Netherlands
- Onsala Space Observatory, Department of Space, Earth and Environment, Chalmers University of Technology, Onsala, Sweden
| | - A Fukui
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- Komaba Institute for Science, The University of Tokyo, Tokyo, Japan
| | - J Garcia-Mejia
- Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA
| | - S Gill
- Department of Physics, University of Warwick, Coventry, UK
| | - M Gillon
- Astrobiology Research Unit, Université de Liège, Liège, Belgium
| | - E Goffo
- Dipartimento di Fisica, Universita degli Studi di Torino, Torino, Italy
- Thüringer Landessternwarte Tautenburg, Tautenburg, Germany
| | - Y Gómez Maqueo Chew
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de México, Mexico
| | - M Güdel
- Department of Astrophysics, University of Vienna, Vienna, Austria
| | - E W Guenther
- Thüringer Landessternwarte Tautenburg, Tautenburg, Germany
| | - M N Günther
- European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Noordwijk, The Netherlands
| | - A P Hatzes
- Thüringer Landessternwarte Tautenburg, Tautenburg, Germany
| | - Ch Helling
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - K M Hesse
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - S B Howell
- NASA Ames Research Center, Moffett Field, CA, USA
| | - S Hoyer
- Aix Marseille Univ., CNRS, CNES, LAM, Marseille, France
| | - K Ikuta
- Department of Multi-Disciplinary Sciences, Graduate School of Arts and Sciences, The University of Tokyo, Tokyo, Japan
| | - K G Isaak
- European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Noordwijk, The Netherlands
| | - J M Jenkins
- NASA Ames Research Center, Moffett Field, CA, USA
| | - T Kagetani
- Department of Multi-Disciplinary Sciences, Graduate School of Arts and Sciences, The University of Tokyo, Tokyo, Japan
| | - L L Kiss
- Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, Hungary
- Institute of Physics, ELTE Eötvös Loránd University, Budapest, Hungary
| | - T Kodama
- Komaba Institute for Science, The University of Tokyo, Tokyo, Japan
| | - J Korth
- Lund Observatory, Division of Astrophysics, Department of Physics, Lund University, Lund, Sweden
| | - K W F Lam
- Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany
| | - J Laskar
- IMCCE, UMR8028 CNRS, Observatoire de Paris, PSL Univ., Sorbonne Univ., Paris, France
| | - D W Latham
- Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA
| | - A Lecavelier des Etangs
- Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, Paris, France
| | - J P D Leon
- Department of Multi-Disciplinary Sciences, Graduate School of Arts and Sciences, The University of Tokyo, Tokyo, Japan
| | - J H Livingston
- Astrobiology Center, Tokyo, Japan
- National Astronomical Observatory of Japan, Tokyo, Japan
- Department of Astronomical Science, The Graduate University for Advanced Studies, SOKENDAI, Tokyo, Japan
| | - D Magrin
- INAF - Osservatorio Astronomico di Padova, Padova, Italy
| | - R A Matson
- United States Naval Observatory, Washington, DC, USA
| | - E C Matthews
- Max Planck Institute for Astronomy, Heidelberg, Germany
| | - C Mordasini
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - M Mori
- Department of Multi-Disciplinary Sciences, Graduate School of Arts and Sciences, The University of Tokyo, Tokyo, Japan
| | - M Moyano
- Instituto de Astronomía, Universidad Católica del Norte, Antofagasta, Chile
| | - M Munari
- INAF - Osservatorio Astrofisico di Catania, Catania, Italy
| | - F Murgas
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- Departamento de Astrofisica, Universidad de La Laguna, La Laguna, Tenerife, Spain
| | - N Narita
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- Komaba Institute for Science, The University of Tokyo, Tokyo, Japan
- Astrobiology Center, Tokyo, Japan
| | - V Nascimbeni
- INAF - Osservatorio Astronomico di Padova, Padova, Italy
| | - G Olofsson
- Department of Astronomy, Stockholm University, AlbaNova University Center, Stockholm, Sweden
| | - H L M Osborne
- Mullard Space Science Laboratory, University College London, Dorking, UK
| | - R Ottensamer
- Department of Astrophysics, University of Vienna, Vienna, Austria
| | - I Pagano
- INAF - Osservatorio Astrofisico di Catania, Catania, Italy
| | - H Parviainen
- Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain
- Departamento de Astrofisica, Universidad de La Laguna, La Laguna, Tenerife, Spain
| | - G Peter
- Institute of Optical Sensor Systems, German Aerospace Center (DLR), Berlin, Germany
| | - G Piotto
- INAF - Osservatorio Astronomico di Padova, Padova, Italy
- Dipartimento di Fisica e Astronomia "Galileo Galilei", Universita degli Studi di Padova, Padova, Italy
| | - D Pollacco
- Department of Physics, University of Warwick, Coventry, UK
| | - D Queloz
- Cavendish Laboratory, University of Cambridge, Cambridge, UK
- Department of Physics, ETH Zurich, Zurich, Switzerland
| | - S N Quinn
- Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA
| | - A Quirrenbach
- Landessternwarte, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany
| | - R Ragazzoni
- INAF - Osservatorio Astronomico di Padova, Padova, Italy
- Dipartimento di Fisica e Astronomia "Galileo Galilei", Universita degli Studi di Padova, Padova, Italy
| | - N Rando
- European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Noordwijk, The Netherlands
| | - F Ratti
- European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Noordwijk, The Netherlands
| | - H Rauer
- Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany
- Zentrum für Astronomie und Astrophysik, Technische Universität Berlin, Berlin, Germany
- Institut für Geologische Wissenschaften, Freie Universität Berlin, Berlin, Germany
| | - S Redfield
- Astronomy Department, Wesleyan University, Middletown, CT, USA
- Van Vleck Observatory, Wesleyan University, Middletown, CT, USA
| | - I Ribas
- Institut de Ciencies de l'Espai (ICE-CSIC), Bellaterra, Spain
- Institut d'Estudis Espacials de Catalunya (IEEC), Barcelona, Spain
| | - G R Ricker
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - A Rudat
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - L Sabin
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ensenada, Mexico
| | - S Salmon
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
| | - N C Santos
- Instituto de Astrofisica e Ciencias do Espaco, Universidade do Porto, Porto, Portugal
- Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto, Porto, Portugal
| | - G Scandariato
- INAF - Osservatorio Astrofisico di Catania, Catania, Italy
| | - N Schanche
- Center for Space and Habitability, University of Bern, Bern, Switzerland
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - J E Schlieder
- NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - S Seager
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA
- Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - D Ségransan
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
| | - A Shporer
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - A E Simon
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
| | - A M S Smith
- Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany
| | - S G Sousa
- Instituto de Astrofisica e Ciencias do Espaco, Universidade do Porto, Porto, Portugal
| | - M Stalport
- Space sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège, Liège, Belgium
| | - Gy M Szabó
- Gothard Astrophysical Observatory, ELTE Eötvös Loránd University, Szombathely, Hungary
- HUN-REN-ELTE Exoplanet Research Group, Szombathely, Hungary
| | - N Thomas
- Space Research and Planetary Sciences, Physics Institute, University of Bern, Bern, Switzerland
| | - A Tuson
- Cavendish Laboratory, University of Cambridge, Cambridge, UK
| | - S Udry
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
| | - A M Vanderburg
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - V Van Eylen
- Mullard Space Science Laboratory, University College London, Dorking, UK
| | - V Van Grootel
- Space sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège, Liège, Belgium
| | - J Venturini
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
| | - I Walter
- Institute of Optical Sensor Systems, German Aerospace Center (DLR), Berlin, Germany
| | - N A Walton
- Institute of Astronomy, University of Cambridge, Cambridge, UK
| | - N Watanabe
- Department of Multi-Disciplinary Sciences, Graduate School of Arts and Sciences, The University of Tokyo, Tokyo, Japan
| | - J N Winn
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
| | - T Zingales
- Dipartimento di Fisica e Astronomia "Galileo Galilei", Universita degli Studi di Padova, Padova, Italy
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Naponiello L, Mancini L, Sozzetti A, Bonomo AS, Morbidelli A, Dou J, Zeng L, Leinhardt ZM, Biazzo K, Cubillos PE, Pinamonti M, Locci D, Maggio A, Damasso M, Lanza AF, Lissauer JJ, Collins KA, Carter PJ, Jensen ELN, Bignamini A, Boschin W, Bouma LG, Ciardi DR, Cosentino R, Crossfield I, Desidera S, Dumusque X, Fiorenzano AFM, Fukui A, Giacobbe P, Gnilka CL, Ghedina A, Guilluy G, Harutyunyan A, Howell SB, Jenkins JM, Lund MB, Kielkopf JF, Lester KV, Malavolta L, Mann AW, Matson RA, Matthews EC, Nardiello D, Narita N, Pace E, Pagano I, Palle E, Pedani M, Seager S, Schlieder JE, Schwarz RP, Shporer A, Twicken JD, Winn JN, Ziegler C, Zingales T. Author Correction: A super-massive Neptune-sized planet. Nature 2023; 623:E6. [PMID: 37863962 DOI: 10.1038/s41586-023-06748-4] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/22/2023]
Affiliation(s)
- Luca Naponiello
- Department of Physics, University of Rome "Tor Vergata", Rome, Italy.
- Department of Physics and Astronomy, University of Florence, Florence, Italy.
- Department of Physics, Sapienza University of Rome, Rome, Italy.
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy.
| | - Luigi Mancini
- Department of Physics, University of Rome "Tor Vergata", Rome, Italy
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
- Max Planck Institute for Astronomy, Heidelberg, Germany
| | | | - Aldo S Bonomo
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | - Alessandro Morbidelli
- Laboratoire Lagrange, Université Cote d'Azur, CNRS, Observatoire de la Côte d'Azur, Nice, France
| | - Jingyao Dou
- School of Physics, H.H. Wills Physics Laboratory, University of Bristol, Bristol, UK
| | - Li Zeng
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA
- Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA
| | - Zoe M Leinhardt
- School of Physics, H.H. Wills Physics Laboratory, University of Bristol, Bristol, UK
| | - Katia Biazzo
- INAF - Rome Astronomical Observatory, Monte Porzio Catone, Italy
| | - Patricio E Cubillos
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | | | - Daniele Locci
- INAF - Palermo Astronomical Observatory, Palermo, Italy
| | | | - Mario Damasso
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | | | - Jack J Lissauer
- NASA Ames Research Center, Moffett Field, CA, USA
- Department of Earth and Planetary Sciences, Stanford University, Stanford, CA, USA
| | - Karen A Collins
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA
| | - Philip J Carter
- School of Physics, H.H. Wills Physics Laboratory, University of Bristol, Bristol, UK
| | - Eric L N Jensen
- Department of Physics & Astronomy, Swarthmore College, Swarthmore, PA, USA
| | | | - Walter Boschin
- Fundación Galileo Galilei - INAF, Tenerife, Spain
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- Departamento de Astrofísica, Universidad de La Laguna (ULL), Tenerife, Spain
| | - Luke G Bouma
- NASA Exoplanet Science Institute - Caltech/IPAC, Pasadena, CA, USA
| | - David R Ciardi
- NASA Exoplanet Science Institute - Caltech/IPAC, Pasadena, CA, USA
| | | | - Ian Crossfield
- Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
| | | | - Xavier Dumusque
- Observatoire de Genève, Université de Genève, Versoix, Switzerland
| | | | - Akihiko Fukui
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- Komaba Institute for Science, The University of Tokyo, Tokyo, Japan
| | - Paolo Giacobbe
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | - Crystal L Gnilka
- NASA Ames Research Center, Moffett Field, CA, USA
- NASA Exoplanet Science Institute - Caltech/IPAC, Pasadena, CA, USA
| | | | - Gloria Guilluy
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | | | | | | | - Michael B Lund
- NASA Exoplanet Science Institute - Caltech/IPAC, Pasadena, CA, USA
| | - John F Kielkopf
- Department of Physics and Astronomy, University of Louisville, Louisville, KY, USA
| | | | - Luca Malavolta
- INAF - Padova Astronomical Observatory, Padova, Italy
- Department of Physics and Astronomy, University of Padova, Padova, Italy
| | - Andrew W Mann
- Department of Physics and Astronomy, The University of North Carolina at Chapel Hill, Chapel Hill, NC, USA
| | | | | | | | - Norio Narita
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- Komaba Institute for Science, The University of Tokyo, Tokyo, Japan
- Astrobiology Center, Osawa, Mitaka, Japan
| | - Emanuele Pace
- Department of Physics and Astronomy, University of Florence, Florence, Italy
| | | | - Enric Palle
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- Departamento de Astrofísica, Universidad de La Laguna (ULL), Tenerife, Spain
| | - Marco Pedani
- Fundación Galileo Galilei - INAF, Tenerife, Spain
| | - Sara Seager
- Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | | | | | - Avi Shporer
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Joseph D Twicken
- NASA Ames Research Center, Moffett Field, CA, USA
- SETI Institute, Mountain View, CA, USA
| | - Joshua N Winn
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
| | - Carl Ziegler
- Department of Physics, Engineering & Astronomy, Stephen F. Austin State University, Nacogdoches, TX, USA
| | - Tiziano Zingales
- INAF - Padova Astronomical Observatory, Padova, Italy
- Department of Physics and Astronomy, University of Padova, Padova, Italy
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4
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Naponiello L, Mancini L, Sozzetti A, Bonomo AS, Morbidelli A, Dou J, Zeng L, Leinhardt ZM, Biazzo K, Cubillos PE, Pinamonti M, Locci D, Maggio A, Damasso M, Lanza AF, Lissauer JJ, Collins KA, Carter PJ, Jensen ELN, Bignamini A, Boschin W, Bouma LG, Ciardi DR, Cosentino R, Crossfield I, Desidera S, Dumusque X, Fiorenzano AFM, Fukui A, Giacobbe P, Gnilka CL, Ghedina A, Guilluy G, Harutyunyan A, Howell SB, Jenkins JM, Lund MB, Kielkopf JF, Lester KV, Malavolta L, Mann AW, Matson RA, Matthews EC, Nardiello D, Narita N, Pace E, Pagano I, Palle E, Pedani M, Seager S, Schlieder JE, Schwarz RP, Shporer A, Twicken JD, Winn JN, Ziegler C, Zingales T. A super-massive Neptune-sized planet. Nature 2023; 622:255-260. [PMID: 37648866 DOI: 10.1038/s41586-023-06499-2] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/15/2023] [Accepted: 07/28/2023] [Indexed: 09/01/2023]
Abstract
Neptune-sized planets exhibit a wide range of compositions and densities, depending on factors related to their formation and evolution history, such as the distance from their host stars and atmospheric escape processes. They can vary from relatively low-density planets with thick hydrogen-helium atmospheres1,2 to higher-density planets with a substantial amount of water or a rocky interior with a thinner atmosphere, such as HD 95338 b (ref. 3), TOI-849 b (ref. 4) and TOI-2196 b (ref. 5). The discovery of exoplanets in the hot-Neptune desert6, a region close to the host stars with a deficit of Neptune-sized planets, provides insights into the formation and evolution of planetary systems, including the existence of this region itself. Here we show observations of the transiting planet TOI-1853 b, which has a radius of 3.46 ± 0.08 Earth radii and orbits a dwarf star every 1.24 days. This planet has a mass of 73.2 ± 2.7 Earth masses, almost twice that of any other Neptune-sized planet known so far, and a density of 9.7 ± 0.8 grams per cubic centimetre. These values place TOI-1853 b in the middle of the Neptunian desert and imply that heavy elements dominate its mass. The properties of TOI-1853 b present a puzzle for conventional theories of planetary formation and evolution, and could be the result of several proto-planet collisions or the final state of an initially high-eccentricity planet that migrated closer to its parent star.
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Affiliation(s)
- Luca Naponiello
- Department of Physics, University of Rome "Tor Vergata", Rome, Italy.
- Department of Physics and Astronomy, University of Florence, Florence, Italy.
- Department of Physics, Sapienza University of Rome, Rome, Italy.
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy.
| | - Luigi Mancini
- Department of Physics, University of Rome "Tor Vergata", Rome, Italy
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
- Max Planck Institute for Astronomy, Heidelberg, Germany
| | | | - Aldo S Bonomo
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | - Alessandro Morbidelli
- Laboratoire Lagrange, Université Cote d'Azur, CNRS, Observatoire de la Côte d'Azur, Nice, France
| | - Jingyao Dou
- School of Physics, H.H. Wills Physics Laboratory, University of Bristol, Bristol, UK
| | - Li Zeng
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA
- Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA
| | - Zoe M Leinhardt
- School of Physics, H.H. Wills Physics Laboratory, University of Bristol, Bristol, UK
| | - Katia Biazzo
- INAF - Rome Astronomical Observatory, Monte Porzio Catone, Italy
| | - Patricio E Cubillos
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | | | - Daniele Locci
- INAF - Palermo Astronomical Observatory, Palermo, Italy
| | | | - Mario Damasso
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | | | - Jack J Lissauer
- NASA Ames Research Center, Moffett Field, CA, USA
- Department of Earth and Planetary Sciences, Stanford University, Stanford, CA, USA
| | - Karen A Collins
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA
| | - Philip J Carter
- School of Physics, H.H. Wills Physics Laboratory, University of Bristol, Bristol, UK
| | - Eric L N Jensen
- Department of Physics & Astronomy, Swarthmore College, Swarthmore, PA, USA
| | | | - Walter Boschin
- Fundación Galileo Galilei - INAF, Tenerife, Spain
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- Departamento de Astrofísica, Universidad de La Laguna (ULL), Tenerife, Spain
| | - Luke G Bouma
- NASA Exoplanet Science Institute - Caltech/IPAC, Pasadena, CA, USA
| | - David R Ciardi
- NASA Exoplanet Science Institute - Caltech/IPAC, Pasadena, CA, USA
| | | | - Ian Crossfield
- Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
| | | | - Xavier Dumusque
- Observatoire de Genève, Université de Genève, Versoix, Switzerland
| | | | - Akihiko Fukui
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- Komaba Institute for Science, The University of Tokyo, Tokyo, Japan
| | - Paolo Giacobbe
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | - Crystal L Gnilka
- NASA Ames Research Center, Moffett Field, CA, USA
- NASA Exoplanet Science Institute - Caltech/IPAC, Pasadena, CA, USA
| | | | - Gloria Guilluy
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | | | | | | | - Michael B Lund
- NASA Exoplanet Science Institute - Caltech/IPAC, Pasadena, CA, USA
| | - John F Kielkopf
- Department of Physics and Astronomy, University of Louisville, Louisville, KY, USA
| | | | - Luca Malavolta
- INAF - Padova Astronomical Observatory, Padova, Italy
- Department of Physics and Astronomy, University of Padova, Padova, Italy
| | - Andrew W Mann
- Department of Physics and Astronomy, The University of North Carolina at Chapel Hill, Chapel Hill, NC, USA
| | | | | | | | - Norio Narita
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- Komaba Institute for Science, The University of Tokyo, Tokyo, Japan
- Astrobiology Center, Osawa, Mitaka, Japan
| | - Emanuele Pace
- Department of Physics and Astronomy, University of Florence, Florence, Italy
| | | | - Enric Palle
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- Departamento de Astrofísica, Universidad de La Laguna (ULL), Tenerife, Spain
| | - Marco Pedani
- Fundación Galileo Galilei - INAF, Tenerife, Spain
| | - Sara Seager
- Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | | | | | - Avi Shporer
- Department of Physics, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Joseph D Twicken
- NASA Ames Research Center, Moffett Field, CA, USA
- SETI Institute, Mountain View, CA, USA
| | - Joshua N Winn
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
| | - Carl Ziegler
- Department of Physics, Engineering & Astronomy, Stephen F. Austin State University, Nacogdoches, TX, USA
| | - Tiziano Zingales
- INAF - Padova Astronomical Observatory, Padova, Italy
- Department of Physics and Astronomy, University of Padova, Padova, Italy
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5
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Peterson MS, Benneke B, Collins K, Piaulet C, Crossfield IJM, Ali-Dib M, Christiansen JL, Gagné J, Faherty J, Kite E, Dressing C, Charbonneau D, Murgas F, Cointepas M, Almenara JM, Bonfils X, Kane S, Werner MW, Gorjian V, Roy PA, Shporer A, Pozuelos FJ, Socia QJ, Cloutier R, Dietrich J, Irwin J, Weiss L, Waalkes W, Berta-Thomson Z, Evans T, Apai D, Parviainen H, Pallé E, Narita N, Howard AW, Dragomir D, Barkaoui K, Gillon M, Jehin E, Ducrot E, Benkhaldoun Z, Fukui A, Mori M, Nishiumi T, Kawauchi K, Ricker G, Latham DW, Winn JN, Seager S, Isaacson H, Bixel A, Gibbs A, Jenkins JM, Smith JC, Chavez JP, Rackham BV, Henning T, Gabor P, Chen WP, Espinoza N, Jensen ELN, Collins KI, Schwarz RP, Conti DM, Wang G, Kielkopf JF, Mao S, Horne K, Sefako R, Quinn SN, Moldovan D, Fausnaugh M, Fűűrész G, Barclay T. A temperate Earth-sized planet with tidal heating transiting an M6 star. Nature 2023; 617:701-705. [PMID: 37198481 DOI: 10.1038/s41586-023-05934-8] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/08/2021] [Accepted: 03/08/2023] [Indexed: 05/19/2023]
Abstract
Temperate Earth-sized exoplanets around late-M dwarfs offer a rare opportunity to explore under which conditions planets can develop hospitable climate conditions. The small stellar radius amplifies the atmospheric transit signature, making even compact secondary atmospheres dominated by N2 or CO2 amenable to characterization with existing instrumentation1. Yet, despite large planet search efforts2, detection of low-temperature Earth-sized planets around late-M dwarfs has remained rare and the TRAPPIST-1 system, a resonance chain of rocky planets with seemingly identical compositions, has not yet shown any evidence of volatiles in the system3. Here we report the discovery of a temperate Earth-sized planet orbiting the cool M6 dwarf LP 791-18. The newly discovered planet, LP 791-18d, has a radius of 1.03 ± 0.04 R⊕ and an equilibrium temperature of 300-400 K, with the permanent night side plausibly allowing for water condensation. LP 791-18d is part of a coplanar system4 and provides a so-far unique opportunity to investigate a temperate exo-Earth in a system with a sub-Neptune that retained its gas or volatile envelope. On the basis of observations of transit timing variations, we find a mass of 7.1 ± 0.7 M⊕ for the sub-Neptune LP 791-18c and a mass of [Formula: see text] for the exo-Earth LP 791-18d. The gravitational interaction with the sub-Neptune prevents the complete circularization of LP 791-18d's orbit, resulting in continued tidal heating of LP 791-18d's interior and probably strong volcanic activity at the surface5,6.
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Affiliation(s)
- Merrin S Peterson
- Department of Physics and Trottier Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
| | - Björn Benneke
- Department of Physics and Trottier Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada.
| | - Karen Collins
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | - Caroline Piaulet
- Department of Physics and Trottier Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
| | - Ian J M Crossfield
- Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
| | - Mohamad Ali-Dib
- Department of Physics and Trottier Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
- Center for Astro, Particle and Planetary Physics (CAP3), New York University Abu Dhabi, Abu Dhabi, United Arab Emirates
| | | | - Jonathan Gagné
- Planetarium of Rio Tinto Alcan and Institute for Research on Exoplanets, University of Montréal, Montreal, Quebec, Canada
| | | | - Edwin Kite
- Department of the Geological Sciences, University of Chicago, Chicago, IL, USA
| | - Courtney Dressing
- Department of Astronomy, University of California - Berkeley, Berkeley, CA, USA
| | - David Charbonneau
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | - Felipe Murgas
- Instituto de Astrofísica de Canarias, La Laguna, Spain
| | - Marion Cointepas
- Institute of Planetology and Astrophysics of Grenoble, Grenoble, France
| | | | - Xavier Bonfils
- Institute of Planetology and Astrophysics of Grenoble, Grenoble, France
| | - Stephen Kane
- Department of Earth and Planetary Sciences, University of California, Riverside, CA, USA
| | - Michael W Werner
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Varoujan Gorjian
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Pierre-Alexis Roy
- Department of Physics and Trottier Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
| | - Avi Shporer
- Department of Physics and Kavli Institute of Astronomy, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Francisco J Pozuelos
- Institute of Astrophysics of Andalucía (IAA-CSIC), Glorieta de la Astronomía s, Granada, Spain
- Astrobiology Research Unit, University of Liège, Liège, Belgium
| | | | - Ryan Cloutier
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
- Department of Physics and Astronomy, McMaster University, Ontario, Hamilton, Canada
| | | | - Jonathan Irwin
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | | | - William Waalkes
- Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO, USA
| | - Zach Berta-Thomson
- Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO, USA
| | - Thomas Evans
- Department of Physics and Kavli Institute of Astronomy, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Daniel Apai
- Steward Observatory, Tucson, AZ, USA
- Lunar and Planetary Laboratory, The University of Arizona, Tucson, AZ, USA
| | | | - Enric Pallé
- Instituto de Astrofísica de Canarias, La Laguna, Spain
| | - Norio Narita
- Instituto de Astrofísica de Canarias, La Laguna, Spain
- Komaba Institute for Science, The University of Tokyo Komaba, Meguro, Tokyo, Japan
- Astrobiology Center, Osawa, Mitaka, Tokyo, Japan
| | - Andrew W Howard
- Department of Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - Diana Dragomir
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - Khalid Barkaoui
- Astrobiology Research Unit, University of Liège, Liège, Belgium
- Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, Cadi Ayyad University, Marrakech, Morocco
| | - Michaël Gillon
- Astrobiology Research Unit, University of Liège, Liège, Belgium
| | - Emmanuel Jehin
- Space Sciences, Technologies and Astrophysics Research (STAR), Institute, University of Liège, Liège, Belgium
| | - Elsa Ducrot
- Astrobiology Research Unit, University of Liège, Liège, Belgium
| | - Zouhair Benkhaldoun
- Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, Cadi Ayyad University, Marrakech, Morocco
| | - Akihiko Fukui
- Instituto de Astrofísica de Canarias, La Laguna, Spain
- Komaba Institute for Science, The University of Tokyo Komaba, Meguro, Tokyo, Japan
| | - Mayuko Mori
- Department of Astronomy, Graduate School of Science, The University of Tokyo, Hongo, Bunkyoku, Tokyo, Japan
| | - Taku Nishiumi
- Astrobiology Center, Osawa, Mitaka, Tokyo, Japan
- Department of Astronomical Science, The Graduated University for Advanced Studies, Sokendai, Osawa, Mitaka, Tokyo, Japan
- Department of Multi-Disciplinary Sciences, Graduate School of Arts and Sciences, The University of Tokyo, Komaba, Meguro, Tokyo, Japan
| | - Kiyoe Kawauchi
- Instituto de Astrofísica de Canarias, La Laguna, Spain
- Department of Multi-Disciplinary Sciences, Graduate School of Arts and Sciences, The University of Tokyo, Komaba, Meguro, Tokyo, Japan
| | - George Ricker
- Department of Physics and Kavli Institute of Astronomy, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - David W Latham
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | - Joshua N Winn
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
| | - Sara Seager
- Department of Physics and Kavli Institute of Astronomy, Massachusetts Institute of Technology, Cambridge, MA, USA
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA
- Department of Aeronautics and Astronautics, MIT, Cambridge, MA, USA
| | - Howard Isaacson
- Department of Astronomy, University of California - Berkeley, Berkeley, CA, USA
| | | | - Aidan Gibbs
- Department of Astronomy, University of California, Los Angeles, Los Angeles, CA, USA
| | | | | | | | - Benjamin V Rackham
- Department of Physics and Kavli Institute of Astronomy, Massachusetts Institute of Technology, Cambridge, MA, USA
| | | | - Paul Gabor
- Vatican Observatory Research Group, University of Arizona, Tucson, AZ, USA
| | - Wen-Ping Chen
- Graduate Institute of Astronomy, National Central University, Taoyuan, Taiwan
| | | | - Eric L N Jensen
- Department of Physics and Astronomy, Swarthmore College, Swarthmore, PA, USA
| | | | - Richard P Schwarz
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | - Dennis M Conti
- American Association of Variable Star Observers, Cambridge, MA, USA
| | - Gavin Wang
- Tsinghua International School, Beijing, China
| | - John F Kielkopf
- Department of Physics and Astronomy, University of Louisville, Louisville, KY, USA
| | - Shude Mao
- National Astronomical Observatories of China, Chinese Academy of Sciences, Beijing, China
| | - Keith Horne
- SUPA Physics and Astronomy, University of St. Andrews, Fife, UK
| | | | - Samuel N Quinn
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | | | - Michael Fausnaugh
- Department of Physics and Kavli Institute of Astronomy, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Gábor Fűűrész
- Department of Physics and Kavli Institute of Astronomy, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Thomas Barclay
- NASA Goddard Space Flight Center, Greenbelt, MD, USA
- University of Maryland, Baltimore County, Baltimore, MD, USA
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Narita N, Terada N, Nomura K, Sakamoto S, Hatakeyama S, Kato T, Matsui Y, Inokuchi J, Yokomizo A, Tabata K, Shiota M, Kimura T, Kojima T, Inoue T, Mizowaki T, Sugimoto M, Kitamura H, Kamoto T, Nishiyama H, Habuchi T. Survival outcomes in octogenarian patients with de novo metastatic prostate cancer: Propensity score matching and net overall survival analyses. Eur Urol 2023. [DOI: 10.1016/s0302-2838(23)01223-x] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/12/2023]
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7
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Sato Y, Osawa S, Narita N, Tominaga T. Double-lumen Carotid Plaque Associated with Severe Stenosis Treated with Staged Angioplasty: A Case Report. NMC Case Rep J 2022; 8:359-365. [PMID: 35079489 PMCID: PMC8769422 DOI: 10.2176/nmccrj.cr.2020-0205] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/03/2020] [Accepted: 09/11/2020] [Indexed: 11/20/2022] Open
Abstract
Double-lumen carotid plaque is a rare pathological condition, and only few reports about this condition have been recorded in the literature. However, no study has used endovascular therapy (EVT) for the treatment of double-lumen carotid plaque. Herein, we present a unique case of double-lumen carotid plaque associated with severe stenosis that was successfully treated with staged angioplasty (SAP). Moreover, a literature review of its pathology and other treatment options has been conducted. SAP is a two-stage carotid artery stenting (CAS) that can prevent hyperperfusion syndrome after revascularization. In this study, a 62-year-old man developed walking disturbance and left hemiparesis. Magnetic resonance imaging (MRI) revealed ischemic lesions in the watershed area of the right hemisphere and an irregular plaque in the right cervical internal carotid artery (ICA). Ultrasonography showed 84% stenosis in the area and a double lumen distal to the stenosis in the right ICA. Digital subtraction angiography (DSA) revealed a double-lumen plaque with 70% stenosis based on the North American Symptomatic Carotid Endarterectomy Trial criteria. SAP was performed after medication therapy and rehabilitation, and the surgery was uneventful. A double-lumen carotid plaque associated with severe stenosis is a rare condition with a high risk of emboli and stroke. In an unstable lesion, carotid endarterectomy is the first option. However, since the patient in this case was at high risk for general anesthesia, SAP was performed. Hence, if an appropriate device is used, EVT can be a safe treatment strategy for unstable and atypical plaques as in this case.
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Affiliation(s)
- Yoshimichi Sato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Shinichiro Osawa
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Miyagi, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Miyagi, Japan
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8
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Katsuki M, Narita N, Watanabe O, Cai S, Ishida N, Tominaga T. Endoscopically Treated Subacute Subdural Hematoma Presenting Postoperative Cerebral Hyperperfusion Syndrome: Chronological Changes of Cerebral Blood Flow on Arterial Spin Labeling and Subcortical Low Intensity on Fluid-attenuated Inversion Recovery Images. NMC Case Rep J 2022; 8:457-464. [PMID: 35079504 PMCID: PMC8769462 DOI: 10.2176/nmccrj.cr.2020-0400] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/26/2020] [Accepted: 01/04/2021] [Indexed: 11/24/2022] Open
Abstract
Subacute subdural hematoma (SASDH) is a neurotraumatic entity. There are few reports of chronological changes of cerebral blood flow (CBF) on arterial spin labeling (ASL) and subcortical low intensity (SCLI) on fluid-attenuated inversion recovery (FLAIR) images of magnetic resonance imaging (MRI) observations from the injury onset, deterioration, to post-surgery. We reported a SASDH patient presenting postoperative cerebral hyperperfusion (CHP) syndrome with chronological changes of those findings. An 85-year-old woman fell and presented right ASDH. She was treated conservatively due to no neurological deficits. On day 3, ASL image revealed increased CBF against brain compression. On day 7, the CBF was normalized on ASL image, but SCLI was confirmed. On day 14, SCLI was strengthened. Then she developed left hemiparesis due to brain compression by SASDH. Considering age and comorbidities, we performed endoscopic hematoma removal under local anesthesia, and her neurological deficits improved after the surgery. On postoperative day 1, she newly presented left upper limb paresis. MRI revealed increased CBF and enhanced SCLI. We diagnosed CHP syndrome, and antihypertensive treatment improved the symptoms gradually. However, SCLI had been consistently observed, and CBF easily changed depending on the blood pressure, suggesting dysfunction of the CBF autoregulation. We showed the endoscopically treated SASDH patient with CBF’s chronological changes on ASL images and SCLI on FLAIR images. Long-time brain compression would lead to dysfunction of the CBF autoregulation, and we should be careful about CHP syndrome after the endoscopic surgery for SASDH.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan.,Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Miyagi, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Ohmi Watanabe
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Siqi Cai
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Naoya Ishida
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Miyagi, Japan
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9
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Lam KWF, Csizmadia S, Astudillo-Defru N, Bonfils X, Gandolfi D, Padovan S, Esposito M, Hellier C, Hirano T, Livingston J, Murgas F, Smith AMS, Collins KA, Mathur S, Garcia RA, Howell SB, Santos NC, Dai F, Ricker GR, Vanderspek R, Latham DW, Seager S, Winn JN, Jenkins JM, Albrecht S, Almenara JM, Artigau E, Barragán O, Bouchy F, Cabrera J, Charbonneau D, Chaturvedi P, Chaushev A, Christiansen JL, Cochran WD, De Meideiros JR, Delfosse X, Díaz RF, Doyon R, Eigmüller P, Figueira P, Forveille T, Fridlund M, Gaisné G, Goffo E, Georgieva I, Grziwa S, Guenther E, Hatzes AP, Johnson MC, Kabáth P, Knudstrup E, Korth J, Lewin P, Lissauer JJ, Lovis C, Luque R, Melo C, Morgan EH, Morris R, Mayor M, Narita N, Osborne HLM, Palle E, Pepe F, Persson CM, Quinn SN, Rauer H, Redfield S, Schlieder JE, Ségransan D, Serrano LM, Smith JC, Šubjak J, Twicken JD, Udry S, Van Eylen V, Vezie M. GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star. Science 2021; 374:1271-1275. [PMID: 34855492 DOI: 10.1126/science.aay3253] [Citation(s) in RCA: 7] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
[Figure: see text].
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Affiliation(s)
- Kristine W F Lam
- Centre for Astronomy and Astrophysics, Technical University Berlin, 10585 Berlin, Germany.,Institute of Planetary Research, German Aerospace Center, 12489 Berlin, Germany
| | - Szilárd Csizmadia
- Institute of Planetary Research, German Aerospace Center, 12489 Berlin, Germany
| | - Nicola Astudillo-Defru
- Departamento de Matemática y Física Aplicadas, Universidad Católica de la Santísima Concepción, Concepción, Chile
| | - Xavier Bonfils
- Université Grenoble Alpes, Centre national de la recherche scientifique, Institut de Planétologie et d'Astrophysique de Grenoble, F-38000 Grenoble, France
| | - Davide Gandolfi
- Dipartimento di Fisica, Università degli Studi di Torino, I-10125, Torino, Italy
| | - Sebastiano Padovan
- Institute of Planetary Research, German Aerospace Center, 12489 Berlin, Germany.,WorkGroup Solutions GmbH at European Organisation for the Exploitation of Meteorological Satellites, 64295 Darmstadt, Germany
| | | | - Coel Hellier
- Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK
| | - Teruyuki Hirano
- Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo, Japan
| | | | - Felipe Murgas
- Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
| | - Alexis M S Smith
- Institute of Planetary Research, German Aerospace Center, 12489 Berlin, Germany
| | - Karen A Collins
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | - Savita Mathur
- Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
| | - Rafael A Garcia
- Institut de Recherche sur les Lois Fondamentales de l'Universe, Commissariat à l'Énergie Atomique et aux énergies alternatives, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France.,Astrophysique, Instrumentation et modélisation, Commissariat à l'Énergie Atomique et aux énergies alternatives, Centre National de la recherche scientifique, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France
| | | | - Nuno C Santos
- Instituto de Astrofísica e Ciênciasdo Espaço, Universidade do Porto, Centro de Astrofísica da Universidade do Porto, 4150-762 Porto, Portugal.,Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, 4169-007 Porto, Portugal
| | - Fei Dai
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - George R Ricker
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Roland Vanderspek
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - David W Latham
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | - Sara Seager
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA.,Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA.,Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Joshua N Winn
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
| | | | - Simon Albrecht
- Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark
| | - Jose M Almenara
- Université Grenoble Alpes, Centre national de la recherche scientifique, Institut de Planétologie et d'Astrophysique de Grenoble, F-38000 Grenoble, France
| | - Etienne Artigau
- Université Grenoble Alpes, Centre national de la recherche scientifique, Institut de Planétologie et d'Astrophysique de Grenoble, F-38000 Grenoble, France
| | - Oscar Barragán
- Subdepartment of Astrophysics, Department of Physics, University of Oxford, Oxford, OX1 3RH, UK
| | - François Bouchy
- Geneva Observatory, University of Geneva, 1290 Versoix, Switzerland
| | - Juan Cabrera
- Université Grenoble Alpes, Centre national de la recherche scientifique, Institut de Planétologie et d'Astrophysique de Grenoble, F-38000 Grenoble, France
| | - David Charbonneau
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | | | - Alexander Chaushev
- Centre for Astronomy and Astrophysics, Technical University Berlin, 10585 Berlin, Germany
| | | | - William D Cochran
- Center for Planetary Systems Habitability and McDonald Observatory, The University of Texas, Austin, TX, USA
| | - José R De Meideiros
- Departamento de Física, Universidade Federal do Rio Grande do Norte, 59072-970 Natal, RN, Brazil
| | - Xavier Delfosse
- Université Grenoble Alpes, Centre national de la recherche scientifique, Institut de Planétologie et d'Astrophysique de Grenoble, F-38000 Grenoble, France
| | - Rodrigo F Díaz
- International Center for Advanced Studies and Instituto de Ciencias Físicas (Consejo Nacional de Investigaciones Científicas y Técnicas), Escuela de Ciencia y Tecnología - Universidad Nacional de San Martín, Campus Miguelete, Buenos Aires, Argentina
| | - René Doyon
- Institut de Recherche sur les Exoplantes, Dpartement de Physique, Universit de Montral, Montral, QC, H3C 3J7, Canada
| | - Philipp Eigmüller
- Institute of Planetary Research, German Aerospace Center, 12489 Berlin, Germany
| | - Pedro Figueira
- Instituto de Astrofísica e Ciênciasdo Espaço, Universidade do Porto, Centro de Astrofísica da Universidade do Porto, 4150-762 Porto, Portugal.,European Southern Observatory, Vitacura, Santiago, Chile
| | - Thierry Forveille
- Université Grenoble Alpes, Centre national de la recherche scientifique, Institut de Planétologie et d'Astrophysique de Grenoble, F-38000 Grenoble, France
| | - Malcolm Fridlund
- Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, 439 92 Onsala, Sweden.,Leiden Observatory, University of Leiden, 2300 RA, Leiden, Netherlands
| | - Guillaume Gaisné
- Université Grenoble Alpes, Centre national de la recherche scientifique, Institut de Planétologie et d'Astrophysique de Grenoble, F-38000 Grenoble, France
| | - Elisa Goffo
- Dipartimento di Fisica, Università degli Studi di Torino, I-10125, Torino, Italy.,Thüringer Landessternwarte Tautenburg, D-07778 Tautenberg, Germany
| | - Iskra Georgieva
- Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, 439 92 Onsala, Sweden
| | - Sascha Grziwa
- Rheinisches Institut für Umweltforschung an der Universität zu Köln, D-50931 Köln, Germany
| | - Eike Guenther
- Thüringer Landessternwarte Tautenburg, D-07778 Tautenberg, Germany
| | - Artie P Hatzes
- Thüringer Landessternwarte Tautenburg, D-07778 Tautenberg, Germany
| | | | - Petr Kabáth
- Astronomical Institute, Czech Academy of Sciences, 25165 Ondřejov, Czech Republic
| | - Emil Knudstrup
- Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark
| | - Judith Korth
- Rheinisches Institut für Umweltforschung an der Universität zu Köln, D-50931 Köln, Germany.,Department of Space, Earth and Environment, Astronomy and Plasma Physics, Chalmers University of Technology, 412 96 Gothenburg, Sweden
| | - Pablo Lewin
- The Maury Lewin Astronomical Observatory, Glendora, CA, USA
| | - Jack J Lissauer
- NASA Ames Research Center, Moffett Field, CA, USA.,Geological Sciences Department, Stanford University, CA, USA
| | - Christophe Lovis
- Geneva Observatory, University of Geneva, 1290 Versoix, Switzerland
| | - Rafael Luque
- Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
| | - Claudio Melo
- European Southern Observatory, Vitacura, Santiago, Chile
| | - Edward H Morgan
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Robert Morris
- NASA Ames Research Center, Moffett Field, CA, USA.,Search for Extraterrestrial Intelligence Institute, Mountain View, CA, USA
| | - Michel Mayor
- Geneva Observatory, University of Geneva, 1290 Versoix, Switzerland
| | - Norio Narita
- Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain.,Komaba Institute for Science, The University of Tokyo, Tokyo, Japan.,Japan Science and Technology Agency, Precursory Research for Embryonic Science and Technology, Tokyo, Japan.,Astrobiology Center, Tokyo, Japan
| | - Hannah L M Osborne
- Mullard Space Science Laboratory, University College London, Dorking, Surrey, RH5 6NT, UK
| | - Enric Palle
- Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
| | - Francesco Pepe
- Geneva Observatory, University of Geneva, 1290 Versoix, Switzerland
| | - Carina M Persson
- Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, 439 92 Onsala, Sweden
| | - Samuel N Quinn
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | - Heike Rauer
- Centre for Astronomy and Astrophysics, Technical University Berlin, 10585 Berlin, Germany.,Institute of Planetary Research, German Aerospace Center, 12489 Berlin, Germany.,Institute of Geological Sciences, Freie Universität Berlin, D-12249 Berlin, Germany
| | - Seth Redfield
- Astronomy Department and Van Vleck Observatory, Wesleyan University, Middletown, CT, USA
| | | | - Damien Ségransan
- Geneva Observatory, University of Geneva, 1290 Versoix, Switzerland
| | - Luisa M Serrano
- Dipartimento di Fisica, Università degli Studi di Torino, I-10125, Torino, Italy
| | - Jeffrey C Smith
- NASA Ames Research Center, Moffett Field, CA, USA.,Search for Extraterrestrial Intelligence Institute, Mountain View, CA, USA
| | - Ján Šubjak
- Astronomical Institute, Czech Academy of Sciences, 25165 Ondřejov, Czech Republic.,Astronomical Institute of Charles University, 180 00 Prague, Czech Republic
| | - Joseph D Twicken
- NASA Ames Research Center, Moffett Field, CA, USA.,Search for Extraterrestrial Intelligence Institute, Mountain View, CA, USA
| | - Stéphane Udry
- Geneva Observatory, University of Geneva, 1290 Versoix, Switzerland
| | - Vincent Van Eylen
- Mullard Space Science Laboratory, University College London, Dorking, Surrey, RH5 6NT, UK
| | - Michael Vezie
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
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10
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Katsuki M, Narita N, Ozaki D, Sato Y, Jia W, Nishizawa T, Kochi R, Sato K, Kawamura K, Ishida N, Watanabe O, Cai S, Shimabukuro S, Yasuda I, Kinjo K, Yokota K. Deep Learning-Based Functional Independence Measure Score Prediction After Stroke in Kaifukuki (Convalescent) Rehabilitation Ward Annexed to Acute Care Hospital. Cureus 2021; 13:e16588. [PMID: 34466308 PMCID: PMC8396410 DOI: 10.7759/cureus.16588] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Journal Information] [Subscribe] [Scholar Register] [Accepted: 07/23/2021] [Indexed: 01/11/2023] Open
Abstract
Introduction Prediction models of functional independent measure (FIM) score after kaifukuki (convalescent) rehabilitation ward (KRW) are needed to decide the treatment strategies and save medical resources. Statistical models were reported, but their accuracies were not satisfactory. We made such prediction models using the deep learning (DL) framework, Prediction One (Sony Network Communications Inc., Tokyo, Japan). Methods Of the 559 consecutive stroke patients, 122 patients were transferred to our KRW. We divided our 122 patients’ data randomly into halves of training and validation datasets. Prediction One made three prediction models from the training dataset using (1) variables at the acute care ward admission, (2) those at the KRW admission, and (3) those combined (1) and (2). The models’ determination coefficients (R2), correlation coefficients (rs), and residuals were calculated using the validation dataset. Results Of the 122 patients, the median age was 71, length of stay (LOS) in acute care ward 23 (17-30) days, LOS in KRW 53 days, total FIM scores at the admission of KRW 85, those at discharge 108. The mean FIM gain and FIM efficiency were 19 and 0.417. All patients were discharged home. Model (1), (2), and (3)’s R2 were 0.794, 0.970, and 0.972. Their mean residuals between the predicted and actual total FIM scores were -1.56±24.6, -4.49±17.1, and -2.69±15.7. Conclusion Our FIM gain and efficiency were better than national averages of FIM gain 17.1 and FIM efficiency 0.187. We made DL-based total FIM score prediction models, and their accuracies were superior to those of previous statistically calculated ones. The DL-based FIM score prediction models would save medical costs and perform efficient stroke and rehabilitation medicine.
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Affiliation(s)
- Masahito Katsuki
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN.,Neurosurgery, Itoigawa General Hospital, Itoigawa, JPN
| | - Norio Narita
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
| | - Dan Ozaki
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
| | | | - Wenting Jia
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
| | | | | | - Kanako Sato
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
| | | | - Naoya Ishida
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
| | - Ohmi Watanabe
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
| | - Siqi Cai
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
| | | | - Iori Yasuda
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
| | - Kengo Kinjo
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
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11
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Yasuda I, Katsuki M, Narita N. A Case of Traumatic Cerebrospinal Fluid Rhinorrhea Successfully Treated Using Intravenous Factor XIII Administration. Cureus 2021; 13:e15633. [PMID: 34306845 PMCID: PMC8278359 DOI: 10.7759/cureus.15633] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Accepted: 06/14/2021] [Indexed: 11/23/2022] Open
Abstract
Traumatic cerebrospinal fluid (CSF) rhinorrhea occurs around 2% of severe head trauma. We should find the fistula and surgically seal it or perform conservative therapy with bed rest with/without lumbar spinal CSF drainage. However, the fistula may not be identified, and treatment may sometimes be challenging. Blood coagulation factor XIII (factor XIII) is one of the blood coagulation factors. It also promotes fibroblast proliferation during the wound healing process. We herein reported a traumatic CSF rhinorrhea patient who was successfully treated using intravenous (IV) factor XIII administration. This report would contribute to the effectiveness of factor XIII administration in the treatment of traumatic CSF rhinorrhea. A 58-year-old man fell from a height of 1.5 meters and hit his forehead. He presented with numbness in both upper limbs but no paresis. Neck magnetic resonance imaging (MRI) revealed cervical spinal cord injury without a cervical vertebral or cranial fracture. He was conservatively treated and discharged after three months. He had been aware of rhinorrhea since the trauma but was treated as allergic rhinitis. A year after the trauma, he was diagnosed with traumatic CSF rhinorrhea. We confirmed a bit of rhinorrhea despite the seven-day bedrest, so we intravenously administered 240 international units of factor XIII every day for 10 days. After 10 days, there was no rhinorrhea at all, and the patient was discharged on the 28th day. He has had no recurrence of rhinorrhea after a three-month follow-up. Factor XIII administration might be useful to treat traumatic CSF rhinorrhea.
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Affiliation(s)
- Iori Yasuda
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
| | - Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN.,Department of Neurosurgery, Itoigawa General Hospital, Itoigawa, JPN
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
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12
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Katsuki M, Yasuda I, Narita N, Ozaki D, Sato Y, Kato Y, Jia W, Nishizawa T, Kochi R, Sato K, Kawamura K, Ishida N, Watanabe O, Cai S, Shimabukuro S, Yokota K. Chronic subdural hematoma in patients over 65 years old: Results of using a postoperative cognitive evaluation to determine whether to permit return to driving. Surg Neurol Int 2021; 12:212. [PMID: 34084639 PMCID: PMC8168661 DOI: 10.25259/sni_186_2021] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/22/2021] [Accepted: 04/08/2021] [Indexed: 12/13/2022] Open
Abstract
Background: Chronic subdural hematoma (CSDH) is usually associated with good recovery with burr hole irrigation and postoperative drainage under local anesthesia. In Japan, traffic accidents by the elderly drivers over 65 years old are severely increasing, and there is no consensus on whether or not to return to driving after CSDH treatment. We perform a postoperative cognitive assessment. We retrospectively investigated the return-to-driving rate and associated factors. Methods: Of the 45 patients over 65 y.o. and who had usually driven, 30 patients wished to drive again. We performed tests composed of Mini-Mental State Examination (MMSE), line cancellation and line bisection task, Kohs block design test, trail making test (TMT)-A and B, Kana-hiroi test, Rey-Osterrieth complex figure test, and behavioral assessment of the dysexecutive syndrome, in order. When all tests’ scores were better than the cutoff values, we let patients drive again. When some of the scores were worse than the cutoff values, we reevaluated the patients at the outpatient every month. If the patients’ scores could not improve at the outpatient, we recommended them to stop driving. Results: Nineteen of 30 patients could return to driving. Worse MMSE, Kohs block design test, TMT-A, TMT-B scores, higher age, dementia, or consciousness disturbance as chief complaints were associated with driving disability. Conclusion: CSDH is known as treatable dementia. However, we should perform an objective cognitive assessment before discharge because only 63% of the patients over 65 y.o. who wished to drive could return to driving.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Iori Yasuda
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Dan Ozaki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Yoshimichi Sato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Yuya Kato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Wenting Jia
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Taketo Nishizawa
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Ryuzaburo Kochi
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Kanako Sato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Kokoro Kawamura
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Naoya Ishida
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Ohmi Watanabe
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Siqi Cai
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Shinya Shimabukuro
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Kenichi Yokota
- Department of Rehabilitation, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
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13
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Katsuki M, Narita N, Sugawara K, Cai S, Shimabukuro S, Watanabe O, Ishida N, Tominaga T. A case with bilateral thalamic infarction manifesting mutism - Cerebral blood flow and neural fibers evaluation. Surg Neurol Int 2021; 12:84. [PMID: 33767888 PMCID: PMC7982103 DOI: 10.25259/sni_874_2020] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/04/2020] [Accepted: 02/09/2021] [Indexed: 11/04/2022] Open
Abstract
Background: Acute bilateral thalamic infarction is rare, and occlusion of the artery of percheron (AOP) may be one of its reasons. AOP occlusion results in an acute disturbance of consciousness, but mutism due to AOP occlusion is rare. We described a mutism patient with bilateral thalamic infarction presumably due to AOP occlusion. We also performed cerebral blood flow (CBF) evaluation by N-isopropyl-p-[123I]-iodoamphetamine single-photon emission computed tomography (123I-IMP-SPECT) as well as neural fiber evaluation by diffusion tensor tractography, discussing the mechanism of mutism. Case Description: A 92-year-old woman presented a gradual deterioration of consciousness. Diffusion-weighted images revealed high-intensity areas at the bilateral thalami, and we diagnosed AOP occlusion. We administered a recombinant tissue plasminogen activator. On day 14, her Glasgow Coma Scale score was 11 (E4V1M6), and she did not present any apparent paresis. She was mute but cognitively alert, although she could communicate by nodding or facial expression. 123I-IMP-SPECT showed CBF increase in the bilateral cerebellum and CBF decrease in the infarcted bilateral thalami and frontal lobes. Diffusion tensor tractography revealed the bilateral dentatothalamo-cortical tracts (DTCs). However, the tracts terminated at the parieto-occipital cortex, but not at the frontal cortex. She still had mutism on day 30. Conclusion: We reported the bilateral thalamic infarction patient presumably due to AOP occlusion, who presented mutism. The discontinuity of the bilateral DTCs resulted in her mutism, and our results supported the hypothesis that the cerebellum plays a significant role in uttering, associated with the bilateral DTCs.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Kazuya Sugawara
- Department of Radiological Technology, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Siqi Cai
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Shinya Shimabukuro
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Ohmi Watanabe
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Naoya Ishida
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Miyagi, Japan
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14
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Trifonov T, Caballero JA, Morales JC, Seifahrt A, Ribas I, Reiners A, Bean JL, Luque R, Parviainen H, Pallé E, Stock S, Zechmeister M, Amado PJ, Anglada-Escudé G, Azzaro M, Barclay T, Béjar VJS, Bluhm P, Casasayas-Barris N, Cifuentes C, Collins KA, Collins KI, Cortés-Contreras M, de Leon J, Dreizler S, Dressing CD, Esparza-Borges E, Espinoza N, Fausnaugh M, Fukui A, Hatzes AP, Hellier C, Henning T, Henze CE, Herrero E, Jeffers SV, Jenkins JM, Jensen ELN, Kaminski A, Kasper D, Kossakowski D, Kürster M, Lafarga M, Latham DW, Mann AW, Molaverdikhani K, Montes D, Montet BT, Murgas F, Narita N, Oshagh M, Passegger VM, Pollacco D, Quinn SN, Quirrenbach A, Ricker GR, Rodríguez López C, Sanz-Forcada J, Schwarz RP, Schweitzer A, Seager S, Shporer A, Stangret M, Stürmer J, Tan TG, Tenenbaum P, Twicken JD, Vanderspek R, Winn JN. A nearby transiting rocky exoplanet that is suitable for atmospheric investigation. Science 2021; 371:1038-1041. [PMID: 33674491 DOI: 10.1126/science.abd7645] [Citation(s) in RCA: 19] [Impact Index Per Article: 6.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/10/2020] [Accepted: 02/02/2021] [Indexed: 11/02/2022]
Abstract
Spectroscopy of transiting exoplanets can be used to investigate their atmospheric properties and habitability. Combining radial velocity (RV) and transit data provides additional information on exoplanet physical properties. We detect a transiting rocky planet with an orbital period of 1.467 days around the nearby red dwarf star Gliese 486. The planet Gliese 486 b is 2.81 Earth masses and 1.31 Earth radii, with uncertainties of 5%, as determined from RV data and photometric light curves. The host star is at a distance of ~8.1 parsecs, has a J-band magnitude of ~7.2, and is observable from both hemispheres of Earth. On the basis of these properties and the planet's short orbital period and high equilibrium temperature, we show that this terrestrial planet is suitable for emission and transit spectroscopy.
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Affiliation(s)
- T Trifonov
- Max-Planck-Institut für Astronomie, D-69117 Heidelberg, Germany.
| | - J A Caballero
- Centro de Astrobiología (Consejo Superior de Investigaciones Científicas - Instituto Nacional de Técnica Aeroespacial), E-28692 Villanueva de la Cañada, Madrid, Spain
| | - J C Morales
- Institut de Ciències de l'Espai (Consejo Superior de Investigaciones Científicas), E-08193 Bellaterra, Barcelona, Spain.,Institut d'Estudis Espacials de Catalunya, E-08034 Barcelona, Spain
| | - A Seifahrt
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637, USA
| | - I Ribas
- Institut de Ciències de l'Espai (Consejo Superior de Investigaciones Científicas), E-08193 Bellaterra, Barcelona, Spain.,Institut d'Estudis Espacials de Catalunya, E-08034 Barcelona, Spain
| | - A Reiners
- Institut für Astrophysik, Georg-August-Universität, D-37077 Göttingen, Germany
| | - J L Bean
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637, USA
| | - R Luque
- Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
| | - H Parviainen
- Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
| | - E Pallé
- Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
| | - S Stock
- Landessternwarte, Zentrum für Astronomie der Universität Heidelberg, D-69117 Heidelberg, Germany
| | - M Zechmeister
- Institut für Astrophysik, Georg-August-Universität, D-37077 Göttingen, Germany
| | - P J Amado
- Instituto de Astrofísica de Andalucía (Consejo Superior de Investigaciones Científicas), E-18008 Granada, Spain
| | - G Anglada-Escudé
- Institut de Ciències de l'Espai (Consejo Superior de Investigaciones Científicas), E-08193 Bellaterra, Barcelona, Spain.,Institut d'Estudis Espacials de Catalunya, E-08034 Barcelona, Spain
| | - M Azzaro
- Centro Astronómico Hispano-Alemán, Observatorio de Calar Alto, E-04550 Gérgal, Almería, Spain
| | - T Barclay
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.,University of Maryland, Baltimore County, Baltimore, MD 21250, USA
| | - V J S Béjar
- Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
| | - P Bluhm
- Landessternwarte, Zentrum für Astronomie der Universität Heidelberg, D-69117 Heidelberg, Germany
| | - N Casasayas-Barris
- Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
| | - C Cifuentes
- Centro de Astrobiología (Consejo Superior de Investigaciones Científicas - Instituto Nacional de Técnica Aeroespacial), E-28692 Villanueva de la Cañada, Madrid, Spain
| | - K A Collins
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA 02138, USA
| | - K I Collins
- Department of Physics and Astronomy, George Mason University, Fairfax, VA 22030, USA
| | - M Cortés-Contreras
- Centro de Astrobiología (Consejo Superior de Investigaciones Científicas - Instituto Nacional de Técnica Aeroespacial), E-28692 Villanueva de la Cañada, Madrid, Spain
| | - J de Leon
- Department of Astronomy, Graduate School of Science, University of Tokyo, Tokyo 113-0033, Japan
| | - S Dreizler
- Institut für Astrophysik, Georg-August-Universität, D-37077 Göttingen, Germany
| | - C D Dressing
- Astronomy Department, University of California at Berkeley, Berkeley, CA 94720, USA
| | - E Esparza-Borges
- Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
| | - N Espinoza
- Space Telescope Science Institute, Baltimore, MD 21218, USA
| | - M Fausnaugh
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
| | - A Fukui
- Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo, Tokyo 113-0033, Japan.,Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
| | - A P Hatzes
- Thüringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany
| | - C Hellier
- Astrophysics Group, Keele University, Staffordshire ST5 5BG, UK
| | - Th Henning
- Max-Planck-Institut für Astronomie, D-69117 Heidelberg, Germany
| | - C E Henze
- NASA Ames Research Center, Moffett Field, CA 94035, USA
| | - E Herrero
- Institut de Ciències de l'Espai (Consejo Superior de Investigaciones Científicas), E-08193 Bellaterra, Barcelona, Spain.,Institut d'Estudis Espacials de Catalunya, E-08034 Barcelona, Spain
| | - S V Jeffers
- Institut für Astrophysik, Georg-August-Universität, D-37077 Göttingen, Germany.,Max-Planck-Institut für Sonnensystemforschung, D-37077, Göttingen, Germany
| | - J M Jenkins
- NASA Ames Research Center, Moffett Field, CA 94035, USA
| | - E L N Jensen
- Department of Physics and Astronomy, Swarthmore College, Swarthmore, PA 19081, USA
| | - A Kaminski
- Landessternwarte, Zentrum für Astronomie der Universität Heidelberg, D-69117 Heidelberg, Germany
| | - D Kasper
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637, USA
| | - D Kossakowski
- Max-Planck-Institut für Astronomie, D-69117 Heidelberg, Germany
| | - M Kürster
- Max-Planck-Institut für Astronomie, D-69117 Heidelberg, Germany
| | - M Lafarga
- Institut de Ciències de l'Espai (Consejo Superior de Investigaciones Científicas), E-08193 Bellaterra, Barcelona, Spain.,Institut d'Estudis Espacials de Catalunya, E-08034 Barcelona, Spain
| | - D W Latham
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA 02138, USA
| | - A W Mann
- Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, NC 27599, USA
| | - K Molaverdikhani
- Landessternwarte, Zentrum für Astronomie der Universität Heidelberg, D-69117 Heidelberg, Germany
| | - D Montes
- Departamento de Física de la Tierra y Astrofísica and Instituto de Física de Partículas y del Cosmos, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain
| | - B T Montet
- School of Physics, University of New South Wales, Sydney NSW 2052, Australia
| | - F Murgas
- Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
| | - N Narita
- Komaba Institute for Science, University of Tokyo, Tokyo 153-8902, Japan.,Japan Science and Technology Agency, Precursory Research for Embryonic Science and Technology, Tokyo 153-8902, Japan.,Astrobiology Center, Tokyo 181-8588, Japan.,Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain
| | - M Oshagh
- Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
| | - V M Passegger
- Hamburger Sternwarte, Universität Hamburg, D-21029 Hamburg, Germany.,Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USA
| | - D Pollacco
- Department of Physics, University of Warwick, Coventry CV4 7AL, UK
| | - S N Quinn
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA 02138, USA
| | - A Quirrenbach
- Landessternwarte, Zentrum für Astronomie der Universität Heidelberg, D-69117 Heidelberg, Germany
| | - G R Ricker
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
| | - C Rodríguez López
- Instituto de Astrofísica de Andalucía (Consejo Superior de Investigaciones Científicas), E-18008 Granada, Spain
| | - J Sanz-Forcada
- Centro de Astrobiología (Consejo Superior de Investigaciones Científicas - Instituto Nacional de Técnica Aeroespacial), E-28692 Villanueva de la Cañada, Madrid, Spain
| | - R P Schwarz
- Patashnick Voorheesville Observatory, Voorheesville, NY 12186, USA
| | - A Schweitzer
- Hamburger Sternwarte, Universität Hamburg, D-21029 Hamburg, Germany
| | - S Seager
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.,Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.,Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
| | - A Shporer
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
| | - M Stangret
- Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.,Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
| | - J Stürmer
- Landessternwarte, Zentrum für Astronomie der Universität Heidelberg, D-69117 Heidelberg, Germany
| | - T G Tan
- Perth Exoplanet Survey Telescope, Perth WA 6010, Australia
| | - P Tenenbaum
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
| | - J D Twicken
- Search for Extraterrestrial Intelligence Institute, Mountain View, CA 94043, USA.,NASA Ames Research Center, Moffett Field, CA 94035, USA
| | - R Vanderspek
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
| | - J N Winn
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA
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15
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Katsuki M, Narita N, Yasuda I, Tominaga T. Lance-Adams Syndrome Treated by Perampanel in the Acute Term. Cureus 2021; 13:e13761. [PMID: 33842137 PMCID: PMC8022676 DOI: 10.7759/cureus.13761] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
Abstract
Lance-Adams syndrome (LAS) is chronic post-hypoxic myoclonus after a hypoxic encephalopathy. Recently, the report on LAS in the chronic term treated by perampanel (PER) is increasing. However, PER’s efficacy in the “acute term” has not been reported. Here, we report an LAS patient who markedly improved when PER was added to his existing treatment regime in the acute term. The 65-year-old patient presented with a return of spontaneous circulation after cardiopulmonary arrest. He developed myoclonus on the admission day, and it led to tonic-clonic convulsion. We started levetiracetam 3000 mg/day, lacosamide 400 mg/day, general anesthesia using midazolam 180 mg/day, dexmedetomidine 1000 μg/day, and fentanyl 1.2 mg/day. We could stop the convulsions after 18 h from the onset. We tried to reduce sedatives, but his convulsion recurred. We added PER 2 mg/day for three days, PER 4 mg/day for next four days, then used PER 8 mg/day and we could gradually reduce the sedatives. Single-photon emission computed tomography on day 40 showed cerebral blood flow (CBF) increase at the bilateral anterior lobes of the cerebellum, medial temporal lobes, and supplementary motor and premotor areas, while CBF decrease at the brain surface of the frontal, parietal, and temporal lobes. The myoclonus disappeared since day 12, and he was transferred to another rehabilitation hospital on day 56. The optimal treatment strategy has not been established for LAS, but our case suggested that PER could be one of the choices to treat LAS in the acute term.
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Affiliation(s)
| | - Norio Narita
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
| | - Iori Yasuda
- Neurosurgery, Kesennuma City Hospital, Kesennuma, JPN
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16
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Katsuki M, Narita N, Sasaki K, Sato Y, Suzuki Y, Mashiyama S, Tominaga T. Standard values for temporal muscle thickness in the Japanese population who undergo brain check-up by magnetic resonance imaging. Surg Neurol Int 2021; 12:67. [PMID: 33767871 PMCID: PMC7982108 DOI: 10.25259/sni_3_2021] [Citation(s) in RCA: 6] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/02/2021] [Accepted: 02/09/2021] [Indexed: 02/07/2023] Open
Abstract
BACKGROUND Skeletal muscle mass is an important factor for various diseases' outcomes. The psoas muscle cross-sectional area on the abdominal computed tomography (CT), gait speed, and handgrip strength is used to measure it. However, it is difficult to measure the neurological patients' muscle mass or function because (1) we do not perform abdominal CT. (2) Such patients have impaired consciousness, gait disturbance, paresis, and need of rest. Temporal muscle thickness (TMT) on magnetic resonance imaging (MRI) is now attractive for skeletal muscle volume indicator, but the reference values are not established. We herein investigated the standard value of the Japanese TMT using the brain check-up database by MRI. METHODS We retrospectively investigated 360 Japanese individuals from two institutions between 2017 and 2019. We measured TMT on the T1-weighted images in the previously reported way. The associations between TMT and other variables were analyzed. RESULTS TMT of 214 women and 146 men, ranging from 35 to 84 years old, was investigated. TMT ranged from 3.69 to 16.90 mm. Mean TMT values were significantly higher in men compared to women except for the over 70-year-old cohort. TMT was correlated to weight and body mass index in both sexes. CONCLUSION This is the first retrospective study on the standard TMT values from the Japanese brain check-up database. Our results were just reference values, but these would be useful for further investigation in other neurosurgical and neurological diseases regarding muscle volume or sarcopenia.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Keisuke Sasaki
- Department of Neurosurgery, Iwaki City Medical Center, Iwaki, Fukushima, Japan
| | - Yoshimichi Sato
- Department of Neurosurgery, Iwaki City Medical Center, Iwaki, Fukushima, Japan
| | - Yasuhiro Suzuki
- Department of Neurosurgery, Iwaki City Medical Center, Iwaki, Fukushima, Japan
| | - Shoji Mashiyama
- Department of Neurosurgery, Iwaki City Medical Center, Iwaki, Fukushima, Japan
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Miyagi, Japan
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17
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Katsuki M, Narita N, Sato K, Kochi R, Nishizawa T, Kawamura K, Ishida N, Watanabe O, Cai S, Shimabukuro S, Tominaga T. Where to make burr hole for endoscopic hematoma removal against intracerebral hemorrhage at the basal ganglia to increase the hematoma removal rate - Comparison between trans-forehead and along-the-long-axis approaches. Surg Neurol Int 2021; 12:41. [PMID: 33598357 PMCID: PMC7881520 DOI: 10.25259/sni_887_2020] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/08/2020] [Accepted: 01/13/2021] [Indexed: 11/04/2022] Open
Abstract
Background: Endoscopic hematoma removal is performed to treat intracerebral hemorrhage (ICH) at the basal ganglia. In our hospital, young neurosurgical trainees perform it for the only 1st to the 3rd time. We perform a “trans-forehead approach” and hypothesized that our technique would contribute to higher hematoma removal rate and easiness despite their inexperience. We compared our dataset with an open dataset with along-the-long-axis approaches using pre- and intraoperative neuronavigation by well-trained neurosurgeons and tested the utility of our trans-forehead approach. Methods: We retrospectively investigated our 17 consecutive patients with hypertensive ICH who underwent endoscopic hematoma removal using the trans-forehead approach. We obtained the open dataset and compared our data with the 12 patients from the open dataset using the inverse probability weighting method. Operative time, hematoma removal rate, postoperative hematoma volume, Glasgow Coma Scale (GCS) on day 7, and modified Rankin Scale (mRS) at 6 months were assessed as outcomes. Results: The median age was 68 (interquartile range; 58–78) years. Median postoperative hematoma volume, removal rate, operative time, GCS on day 7, and mRS at 6 months were 9 (2–24) mL, 90 (79–98)%, 53 (41–80) min, 13 (12–13), and 4 (2–5), respectively. The weighted generalized estimating equations revealed that operative time was shorter in the along-the-long-axis group, but other items were not significantly different between the two approaches. Conclusion: The hematoma removal rate of endoscopic hematoma removal with the trans-forehead approach by young trainees was not different from that of the along-the-long-axis approach by well-trained neurosurgeons using neuronavigation.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Japan
| | - Kanako Sato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Japan
| | - Ryuzaburo Kochi
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Japan
| | - Taketo Nishizawa
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Japan
| | - Kokoro Kawamura
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Japan
| | - Naoya Ishida
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Japan
| | - Ohmi Watanabe
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Japan
| | - Siqi Cai
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Japan
| | | | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Miyagi, Japan
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18
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Watanabe O, Narita N, Katsuki M, Ishida N, Cai S, Otomo H, Yokota K. Prediction Model of Deep Learning for Ambulance Transports in Kesennuma City by Meteorological Data. Open Access Emerg Med 2021; 13:23-32. [PMID: 33536798 PMCID: PMC7850460 DOI: 10.2147/oaem.s293551] [Citation(s) in RCA: 4] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/23/2020] [Accepted: 01/14/2021] [Indexed: 12/15/2022] Open
Abstract
PURPOSE With the aging population in Japan, the prediction of ambulance transports is needed to save the limited medical resources. Some meteorological factors were risks of ambulance transports, but it is difficult to predict in a classically statistical way because Japan has 4 seasons. We tried to make prediction models for ambulance transports using the deep learning (DL) framework, Prediction One (Sony Network Communications Inc., Tokyo, Japan), with the meteorological and calendarial variables. MATERIALS AND METHODS We retrospectively investigated the daily ambulance transports and meteorological data between 2017 and 2019. First, to confirm their association, we performed classically statistical analysis. Second, to test the DL framework's utility for ambulance transports prediction, we made 3 prediction models for daily ambulance transports (total daily ambulance transports more than 5 or not, cardiopulmonary arrest (CPA), and trauma) using meteorological and calendarial factors and evaluated their accuracies by internal cross-validation. RESULTS During the 1095 days of 3 years, the total ambulance transports were 5948, including 240 CPAs and 337 traumas. Cardiogenic CPA accounted for 72.3%, according to the Utstein classification. The relation between ambulance transports and meteorological parameters by polynomial curves were statistically obtained, but their r2s were small. On the other hand, all DL-based prediction models obtained satisfactory accuracies in the internal cross-validation. The areas under the curves obtained from each model were all over 0.947. CONCLUSION We could statistically make polynomial curves between the meteorological variables and the number of ambulance transport. We also preliminarily made DL-based prediction models. The DL-based prediction for daily ambulance transports would be used in the future, leading to solving the lack of medical resources in Japan.
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Affiliation(s)
- Ohmi Watanabe
- Kesennuma City Hospital, Kesennuma, Miyagi988-0181, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi988-0181, Japan
| | - Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi988-0181, Japan
| | - Naoya Ishida
- Kesennuma City Hospital, Kesennuma, Miyagi988-0181, Japan
| | - Siqi Cai
- Kesennuma City Hospital, Kesennuma, Miyagi988-0181, Japan
| | - Hiroshi Otomo
- Department of Surgery, Kesennuma City Hospital, Kesennuma, Miyagi988-0181, Japan
| | - Kenichi Yokota
- Department of Surgery, Kesennuma City Hospital, Kesennuma, Miyagi988-0181, Japan
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Katsuki M, Narita N, Ishida N, Watanabe O, Cai S, Ozaki D, Sato Y, Kato Y, Jia W, Nishizawa T, Kochi R, Sato K, Tominaga T. Preliminary development of a prediction model for daily stroke occurrences based on meteorological and calendar information using deep learning framework (Prediction One; Sony Network Communications Inc., Japan). Surg Neurol Int 2021; 12:31. [PMID: 33598347 PMCID: PMC7881509 DOI: 10.25259/sni_774_2020] [Citation(s) in RCA: 7] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/29/2020] [Accepted: 01/07/2021] [Indexed: 12/13/2022] Open
Abstract
BACKGROUND Chronologically meteorological and calendar factors were risks of stroke occurrence. However, the prediction of stroke occurrences is difficult depending on only meteorological and calendar factors. We tried to make prediction models for stroke occurrences using deep learning (DL) software, Prediction One (Sony Network Communications Inc., Tokyo, Japan), with those variables. METHODS We retrospectively investigated the daily stroke occurrences between 2017 and 2019. We used Prediction One software to make the prediction models for daily stroke occurrences (present or absent) using 221 chronologically meteorological and calendar factors. We made a prediction models from the 3-year dataset and evaluated their accuracies using the internal cross-validation. Areas under the curves (AUCs) of receiver operating characteristic curves were used as accuracies. RESULTS The 371 cerebral infarction (CI), 184 intracerebral hemorrhage (ICH), and 53 subarachnoid hemorrhage patients were included in the study. The AUCs of the several DL-based prediction models for all stroke occurrences were 0.532-0.757. Those for CI were 0.600-0.782. Those for ICH were 0.714-0.988. CONCLUSION Our preliminary results suggested a probability of the DL-based prediction models for stroke occurrence only by meteorological and calendar factors. In the future, by synchronizing a variety of medical information among the electronic medical records and personal smartphones as well as integrating the physical activities or meteorological conditions in real time, the prediction of stroke occurrence could be performed with high accuracy, to save medical resources, to have patients care for themselves, and to perform efficient medicine.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Naoya Ishida
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Ohmi Watanabe
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Siqi Cai
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Dan Ozaki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Yoshimichi Sato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Yuya Kato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Wenting Jia
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Taketo Nishizawa
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Ryuzaburo Kochi
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Kanako Sato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University, Sendai, Miyagi, Japan
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Katsuki M, Ozaki D, Narita N, Ishida N, Watanabe O, Cai S, Shimabukuro S, Tominaga T. Unilateral posterior reversible encephalopathy syndrome characterized with a long and gradually exacerbating course over 3 years and that presented propofol infusion syndrome - A case report. Surg Neurol Int 2021; 12:19. [PMID: 33500834 PMCID: PMC7827507 DOI: 10.25259/sni_853_2020] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/29/2020] [Accepted: 12/25/2020] [Indexed: 12/13/2022] Open
Abstract
Background: Posterior reversible encephalopathy syndrome (PRES) is characterized by acute neurological symptoms and vasogenic edema, and most patients wholly recover. We report a unilateral PRES patient characterized by a gradual onset followed by propofol infusion syndrome (PRIS) due to general anesthesia therapy. Case Description: A 32-year-old woman had ovarian dysfunction treated by Kaufmann’s treatment for 17 years. Three years ago, she developed seizures, and photophobia and myoclonus sometimes occurred. This time, she had strong photophobia and nausea for 3 months and then developed tonic-clonic seizures for 3 min. Her blood pressure and laboratory test on admission were all within normal limits. She presented no neurological deficits at admission, but the T2-weighted image (T2WI) showed a high-intensity area (HIA), and arterial spin labeling (ASL) image described cerebral blood flow (CBF) increase in the left parieto-occipital region. We diagnosed PRES and started anticonvulsants, antihypertensive, and steroid pulse therapy. However, her aphasia and neuroimaging findings worsened, so we started general anesthesia treatment with propofol on day 29. On day 32, she suddenly developed multiple organ dysfunctions due to PRIS. After intensive care with other sedatives over 2 months, the systemic status and neurological symptoms gradually improved almost as before the onset. On day 90, HIA in the T2WI in the lesion became small, and CBF was severely downregulated in the ASL image. Conclusion: Unilateral PRES’s pathophysiology and the association with the female hormone remain unknown. Some patients undergo gradual onset and long-term courses, and we should care for PRIS during PRES treatment.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Dan Ozaki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Naoya Ishida
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Ohmi Watanabe
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Siqi Cai
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Shinya Shimabukuro
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Aobaku, Sendai, Miyagi, Japan
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21
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Katsuki M, Narita N, Sugawara K, Ishida N, Tominaga T. Musician developed right putaminal hemorrhage but conserved absolute pitch ability -Case report. Clin Neurol Neurosurg 2021; 202:106521. [PMID: 33571783 DOI: 10.1016/j.clineuro.2021.106521] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/18/2020] [Revised: 01/22/2021] [Accepted: 01/23/2021] [Indexed: 12/01/2022]
Abstract
Absolute pitch (AP) is known as the ability to recognize and label the pitch chroma of a given tone without external reference. The neural mechanism and its asymmetry of AP musicians remain unclear. We herein report a 41-year-old AP musician who developed a right putaminal hemorrhage. On a postoperative day 5, a fluid-attenuated inversion recovery image revealed the rest of the hematoma and edematous lesion at the right white matter between the Heschl's gyrus and other cortices. Diffusion tensor tractography with the region of interest at the Heschl's gyrus was performed. In the left hemisphere, the anterior part of the arcuate fiber and middle longitudinal fasciculus were observed. However, these connections were absent in the right hemisphere, but her AP ability was maintained. Our case suggested that the fibers from the right Heschl's gyrus to the right frontal lobe via the right ventral stream is not associated with AP.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, 988-0181, Japan; Composer and Singer Song Writer, Cuty KATSKI Music Office, Niigata, Niigata, 950-0028, Japan.
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, 988-0181, Japan.
| | - Kazuya Sugawara
- Department of Radiological Technology, Kesennuma City Hospital, Kesennuma, Miyagi, 988-0181, Japan.
| | - Naoya Ishida
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, 988-0181, Japan.
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Miyagi, 980-8574, Japan.
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22
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Katsuki M, Narita N, Ishida N, Sugawara K, Watanabe O, Ozaki D, Sato Y, Kato Y, Jia W, Tominaga T. Usefulness of 3 Tesla Ultrashort Echo Time Magnetic Resonance Angiography (UTE-MRA, SILENT-MRA) for Evaluation of the Mother Vessel after Cerebral Aneurysm Clipping: Case Series of 19 Patients. Neurol Med Chir (Tokyo) 2021; 61:193-203. [PMID: 33504734 PMCID: PMC7966203 DOI: 10.2176/nmc.oa.2020-0336] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/11/2022] Open
Abstract
It is important to assess the cerebral arteries near the clip after cerebral aneurysm clipping. Contrast-enhanced computed tomography angiography has side effects of contrast medium and radiation exposure. Time-of-flight magnetic resonance angiography (TOF-MRA) is a fast and non-invasive method, but clip-induced artifact limits the assessment around the clip. Recently, 3 tesla MRA with ultrashort echo time called SILENT MRA (GE Healthcare Life Sciences, UK) has been reported to have the potential to overcome these disadvantages. We herein present consecutive 19 cerebral aneurysm patients treated by clipping and evaluated using SILENT MRA. The 19 patients (15 women and 4 men) underwent TOF-MRA and SILENT MRA during the same scan session. Two neurosurgeons independently assessed the visibility of the mother vessel at the clipping site in TOF-MRA and SILENT MRA. We also investigated the factors related to visibility in SILENT MRA. All patients’ mother vessels were not described in TOF-MRA, and that of 16 patients (84%) were described in SILENT MRA. Overall agreement was 100% in the two neurosurgeons, and the fixed marginal kappa = 1.00 (95% CI: 0.36–1.00). Univariate analysis revealed that larger aneurysm dome and long clip blade length contributed to the visibility of the mother vessel in SILENT MRA. (p = 0.023, 0.007, each). In conclusion, SILENT MRA can be applied for the assessment of the arteries and aneurysm neck remnants near the clip. Using clips with long blade and ligation with its tip would be related to the visibility of the mother vessels in SILENT MRA.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Naoya Ishida
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Kazuya Sugawara
- Department of Radiological Technology, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Ohmi Watanabe
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Dan Ozaki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Yoshimichi Sato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Yuya Kato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Wenting Jia
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Miyagi, Japan
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23
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Katsuki M, Narita N, Matsumori Y, Ishida N, Watanabe O, Cai S, Tominaga T. Preliminary development of a deep learning-based automated primary headache diagnosis model using Japanese natural language processing of medical questionnaire. Surg Neurol Int 2020; 11:475. [PMID: 33500813 PMCID: PMC7827501 DOI: 10.25259/sni_827_2020] [Citation(s) in RCA: 20] [Impact Index Per Article: 5.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/16/2020] [Accepted: 12/10/2020] [Indexed: 12/12/2022] Open
Abstract
Background Primary headaches are widespread and costly public health problems. However, there are insufficient medical resources for their treatment in Japan due to two reasons. First, the numbers of headache specialists and clinics remain insufficient. Second, neurologists and neurosurgeons mainly treat headaches in Japan. However, they mainly work as general stroke neurologists, so they cannot focus on primary headache treatment. To solve these problems, we preliminarily developed a deep learning (DL)-based automated diagnosis model from patients' Japanese unstructured sentences in the medical questionnaire using a DL framework. We hypothesized that the model would reduce the time and burden on both doctors and patients and improve their quality of life. Methods We retrospectively investigated our primary headache database and developed a diagnosis model using the DL framework (Prediction One, Sony Network Communications Inc., Japan). We used age, sex, date, and embedding layer made by the medical questionnaire's natural language processing (NLP). Results Eight hundred and forty-eight primary headache patients (495 women and 353 men) are included. The median (interquartile range) age was 59 (40-74). Migraine accounted for 46%, tension-type headache for 47%, trigeminal autonomic cephalalgias for 5%, and other primary headache disorders for 2%. The accuracy, mean precision, mean recall, and mean F value of the developed diagnosis model were 0.7759, 0.8537, 0.6086, and 0.6353, which were satisfactory. Conclusion The DL-based diagnosis model for primary headaches using the raw medical questionnaire's Japanese NLP would be useful in performing efficient medical practice after ruling out the secondary headaches.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | | | - Naoya Ishida
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Ohmi Watanabe
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Siqi Cai
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Aobaku, Sendai, Miyagi, Japan
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24
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Vanderburg A, Rappaport SA, Xu S, Crossfield IJM, Becker JC, Gary B, Murgas F, Blouin S, Kaye TG, Palle E, Melis C, Morris BM, Kreidberg L, Gorjian V, Morley CV, Mann AW, Parviainen H, Pearce LA, Newton ER, Carrillo A, Zuckerman B, Nelson L, Zeimann G, Brown WR, Tronsgaard R, Klein B, Ricker GR, Vanderspek RK, Latham DW, Seager S, Winn JN, Jenkins JM, Adams FC, Benneke B, Berardo D, Buchhave LA, Caldwell DA, Christiansen JL, Collins KA, Colón KD, Daylan T, Doty J, Doyle AE, Dragomir D, Dressing C, Dufour P, Fukui A, Glidden A, Guerrero NM, Guo X, Heng K, Henriksen AI, Huang CX, Kaltenegger L, Kane SR, Lewis JA, Lissauer JJ, Morales F, Narita N, Pepper J, Rose ME, Smith JC, Stassun KG, Yu L. A giant planet candidate transiting a white dwarf. Nature 2020; 585:363-367. [PMID: 32939071 DOI: 10.1038/s41586-020-2713-y] [Citation(s) in RCA: 67] [Impact Index Per Article: 16.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/16/2020] [Accepted: 07/15/2020] [Indexed: 11/09/2022]
Abstract
Astronomers have discovered thousands of planets outside the Solar System1, most of which orbit stars that will eventually evolve into red giants and then into white dwarfs. During the red giant phase, any close-orbiting planets will be engulfed by the star2, but more distant planets can survive this phase and remain in orbit around the white dwarf3,4. Some white dwarfs show evidence for rocky material floating in their atmospheres5, in warm debris disks6-9 or orbiting very closely10-12, which has been interpreted as the debris of rocky planets that were scattered inwards and tidally disrupted13. Recently, the discovery of a gaseous debris disk with a composition similar to that of ice giant planets14 demonstrated that massive planets might also find their way into tight orbits around white dwarfs, but it is unclear whether these planets can survive the journey. So far, no intact planets have been detected in close orbits around white dwarfs. Here we report the observation of a giant planet candidate transiting the white dwarf WD 1856+534 (TIC 267574918) every 1.4 days. We observed and modelled the periodic dimming of the white dwarf caused by the planet candidate passing in front of the star in its orbit. The planet candidate is roughly the same size as Jupiter and is no more than 14 times as massive (with 95 per cent confidence). Other cases of white dwarfs with close brown dwarf or stellar companions are explained as the consequence of common-envelope evolution, wherein the original orbit is enveloped during the red giant phase and shrinks owing to friction. In this case, however, the long orbital period (compared with other white dwarfs with close brown dwarf or stellar companions) and low mass of the planet candidate make common-envelope evolution less likely. Instead, our findings for the WD 1856+534 system indicate that giant planets can be scattered into tight orbits without being tidally disrupted, motivating the search for smaller transiting planets around white dwarfs.
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Affiliation(s)
- Andrew Vanderburg
- Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA. .,Department of Astronomy, The University of Texas at Austin, Austin, TX, USA.
| | - Saul A Rappaport
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Siyi Xu
- NSF's NOIRLab/Gemini Observatory, Hilo, HI, USA
| | - Ian J M Crossfield
- Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
| | - Juliette C Becker
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Bruce Gary
- Hereford Arizona Observatory, Hereford, AZ, USA
| | - Felipe Murgas
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain.,Departamento Astrofísica, Universidad de La Laguna (ULL), Tenerife, Spain
| | - Simon Blouin
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - Thomas G Kaye
- Raemor Vista Observatory, Sierra Vista, AZ, USA.,Laboratory for Space Research, The University of Hong Kong, Hong Kong, China
| | - Enric Palle
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain.,Departamento Astrofísica, Universidad de La Laguna (ULL), Tenerife, Spain
| | - Carl Melis
- Center for Astrophysics and Space Sciences, University of California, San Diego, San Diego, CA, USA
| | - Brett M Morris
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - Laura Kreidberg
- Max Planck Institute for Astronomy, Heidelberg, Germany.,Center for Astrophysics
- Harvard & Smithsonian, Cambridge, MA, USA
| | - Varoujan Gorjian
- NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Caroline V Morley
- Department of Astronomy, The University of Texas at Austin, Austin, TX, USA
| | - Andrew W Mann
- Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, NC, USA
| | - Hannu Parviainen
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain.,Departamento Astrofísica, Universidad de La Laguna (ULL), Tenerife, Spain
| | - Logan A Pearce
- Steward Observatory, University of Arizona, Tucson, AZ, USA
| | - Elisabeth R Newton
- Department of Physics and Astronomy, Dartmouth College, Hanover, NH, USA
| | - Andreia Carrillo
- Department of Astronomy, The University of Texas at Austin, Austin, TX, USA
| | - Ben Zuckerman
- Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA, USA
| | - Lorne Nelson
- Department of Physics and Astronomy, Bishop's University, Sherbrooke, Quebec, Canada
| | - Greg Zeimann
- Hobby-Eberly Telescope, University of Texas, Austin, Austin, TX, USA
| | - Warren R Brown
- Center for Astrophysics
- Harvard & Smithsonian, Cambridge, MA, USA
| | - René Tronsgaard
- DTU Space, National Space Institute, Technical University of Denmark, Kongens Lyngby, Denmark
| | - Beth Klein
- Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA, USA
| | - George R Ricker
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Roland K Vanderspek
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - David W Latham
- Center for Astrophysics
- Harvard & Smithsonian, Cambridge, MA, USA
| | - Sara Seager
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA.,Department of Earth and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA.,Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Joshua N Winn
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
| | | | - Fred C Adams
- Physics Department, University of Michigan, Ann Arbor, MI, USA.,Astronomy Department, University of Michigan, Ann Arbor, MI, USA
| | - Björn Benneke
- Départment de Physique, Université de Montréal, Montreal, Quebec, Canada.,Institut de Recherche sur les Exoplanètes (iREx), Université de Montréal, Montreal, Quebec, Canada
| | - David Berardo
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Lars A Buchhave
- DTU Space, National Space Institute, Technical University of Denmark, Kongens Lyngby, Denmark
| | - Douglas A Caldwell
- NASA Ames Research Center, Moffett Field, CA, USA.,SETI Institute, Mountain View, CA, USA
| | | | - Karen A Collins
- Center for Astrophysics
- Harvard & Smithsonian, Cambridge, MA, USA
| | - Knicole D Colón
- Exoplanets and Stellar Astrophysics Laboratory (Code 667), NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Tansu Daylan
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | | | - Alexandra E Doyle
- Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, Los Angeles, CA, USA
| | - Diana Dragomir
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - Courtney Dressing
- Department of Astronomy, University of California, Berkeley, Berkeley, CA, USA
| | - Patrick Dufour
- Départment de Physique, Université de Montréal, Montreal, Quebec, Canada.,Institut de Recherche sur les Exoplanètes (iREx), Université de Montréal, Montreal, Quebec, Canada
| | - Akihiko Fukui
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain.,Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo, Tokyo, Japan
| | - Ana Glidden
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA.,Department of Earth and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Natalia M Guerrero
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Xueying Guo
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Kevin Heng
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - Andreea I Henriksen
- DTU Space, National Space Institute, Technical University of Denmark, Kongens Lyngby, Denmark
| | - Chelsea X Huang
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Lisa Kaltenegger
- Carl Sagan Institute, Cornell University, Ithaca, NY, USA.,Department of Astronomy and Space Sciences, Ithaca, NY, USA
| | - Stephen R Kane
- Department of Earth and Planetary Sciences, University of California, Riverside, Riverside, CA, USA
| | - John A Lewis
- Center for Astrophysics
- Harvard & Smithsonian, Cambridge, MA, USA
| | | | - Farisa Morales
- NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.,Department of Physics and Astronomy, Moorpark College, Moorpark, CA, USA
| | - Norio Narita
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain.,Astrobiology Center, Tokyo, Japan.,PRESTO, JST, Tokyo, Japan.,National Astronomical Observatory of Japan, Tokyo, Japan.,Komaba Institute for Science, The University of Tokyo, Tokyo, Japan
| | - Joshua Pepper
- Department of Physics, Lehigh University, Bethlehem, PA, USA
| | - Mark E Rose
- NASA Ames Research Center, Moffett Field, CA, USA
| | - Jeffrey C Smith
- NASA Ames Research Center, Moffett Field, CA, USA.,SETI Institute, Mountain View, CA, USA
| | - Keivan G Stassun
- Department of Physics and Astronomy, Vanderbilt University, Nashville, TN, USA.,Department of Physics, Fisk University, Nashville, TN, USA
| | - Liang Yu
- Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA.,ExxonMobil Upstream Integrated Solutions, Spring, TX, USA
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25
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Katsuki M, Narita N, Ozaki D, Sato Y, Iwata S, Tominaga T. Three tesla magnetic resonance angiography with ultrashort echo time describes the arteries near the cerebral aneurysm with clip and the peripheral cerebral arteries. Surg Neurol Int 2020; 11:224. [PMID: 32874727 PMCID: PMC7451165 DOI: 10.25259/sni_329_2020] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/02/2020] [Accepted: 07/01/2020] [Indexed: 12/18/2022] Open
Abstract
Background: The assessment of the clipped cerebral aneurysm and the cerebral arteries after the treatment of subarachnoid hemorrhage (SAH) is important to find aneurysm regrowth or postoperative cerebral vasospasm. Usually, contrast-enhanced computed tomography angiography is performed for the evaluation of the arteries, but it has side effects of contrast medium. Time-of-flight magnetic resonance angiography (MRA) is a fast and non-invasive method, but clip-induced artifact limits assessment of the artery in the vicinity of the clip. 1.5T MRA with ultrashort echo time (UTE) reduces metal artifact, but the obtained image is too rough to evaluate the aneurysm remnant, and the description range is too narrow to assess the cerebral vasospasm. We routinely use SIGNA Pioneer 3.0T (GE Healthcare Life Sciences, Buckinghamshire, England) and perform SILENT SCAN with UTE-MRA for the postoperative assessment of the clipped aneurysm and cerebral arteries for SAH patients treated by clipping. It has better image quality and describes arteries with a wide description range, so it possesses the potential to overcome the disadvantages of 1.5T UTE-MRA. Case Description: We presented a representative SAH patient who postoperatively underwent 3.0T UTE- MRA after clipping. The artery near the clipped aneurysm was evaluated in detail, and the cerebral arteries were described from the main trunk to the peripheral parts with a wide description range, which enabled the assessment of cerebral vasospasm. Conclusion: 3.0T UTE-MRA may be helpful for the usual assessment of the arteries after clipping and cerebral vasospasm in the future.
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Affiliation(s)
- Masahito Katsuki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi
| | - Dan Ozaki
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi
| | - Yoshimichi Sato
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi
| | - Saki Iwata
- Department of Radiological Technology, Sapporo City General Hospital, Sapporo, Hokkaido, Japan
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Miyagi
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26
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Plavchan P, Barclay T, Gagné J, Gao P, Cale B, Matzko W, Dragomir D, Quinn S, Feliz D, Stassun K, Crossfield IJM, Berardo DA, Latham DW, Tieu B, Anglada-Escudé G, Ricker G, Vanderspek R, Seager S, Winn JN, Jenkins JM, Rinehart S, Krishnamurthy A, Dynes S, Doty J, Adams F, Afanasev DA, Beichman C, Bottom M, Bowler BP, Brinkworth C, Brown CJ, Cancino A, Ciardi DR, Clampin M, Clark JT, Collins K, Davison C, Foreman-Mackey D, Furlan E, Gaidos EJ, Geneser C, Giddens F, Gilbert E, Hall R, Hellier C, Henry T, Horner J, Howard AW, Huang C, Huber J, Kane SR, Kenworthy M, Kielkopf J, Kipping D, Klenke C, Kruse E, Latouf N, Lowrance P, Mennesson B, Mengel M, Mills SM, Morton T, Narita N, Newton E, Nishimoto A, Okumura J, Palle E, Pepper J, Quintana EV, Roberge A, Roccatagliata V, Schlieder JE, Tanner A, Teske J, Tinney CG, Vanderburg A, von Braun K, Walp B, Wang J, Wang SX, Weigand D, White R, Wittenmyer RA, Wright DJ, Youngblood A, Zhang H, Zilberman P. A planet within the debris disk around the pre-main-sequence star AU Microscopii. Nature 2020; 582:497-500. [PMID: 32581383 PMCID: PMC7323865 DOI: 10.1038/s41586-020-2400-z] [Citation(s) in RCA: 82] [Impact Index Per Article: 20.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/16/2019] [Accepted: 03/17/2020] [Indexed: 11/09/2022]
Affiliation(s)
- Peter Plavchan
- Department of Physics and Astronomy, George Mason University, Fairfax, VA, USA.
| | - Thomas Barclay
- Center for Space Sciences and Technology, University of Maryland Baltimore County (UMBC), Baltimore, MD, USA.,Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Jonathan Gagné
- Institute for Research on Exoplanets, Département de Physique, Université de Montréal, Montréal, Quebec, Canada
| | - Peter Gao
- Department of Astronomy, University of California, Berkeley, CA, USA
| | - Bryson Cale
- Department of Physics and Astronomy, George Mason University, Fairfax, VA, USA
| | - William Matzko
- Department of Physics and Astronomy, George Mason University, Fairfax, VA, USA
| | - Diana Dragomir
- Massachusetts Institute of Technology, Cambridge, MA, USA.,Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - Sam Quinn
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
| | - Dax Feliz
- Department of Physics and Astronomy, Vanderbilt University, Nashville, TN, USA
| | - Keivan Stassun
- Department of Physics and Astronomy, Vanderbilt University, Nashville, TN, USA
| | - Ian J M Crossfield
- Massachusetts Institute of Technology, Cambridge, MA, USA.,Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
| | | | - David W Latham
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
| | - Ben Tieu
- Department of Physics and Astronomy, George Mason University, Fairfax, VA, USA
| | | | - George Ricker
- Massachusetts Institute of Technology, Cambridge, MA, USA
| | | | - Sara Seager
- Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Joshua N Winn
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
| | | | - Stephen Rinehart
- Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | | | - Scott Dynes
- Massachusetts Institute of Technology, Cambridge, MA, USA
| | - John Doty
- Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Fred Adams
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
| | - Dennis A Afanasev
- Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Chas Beichman
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.,NASA Exoplanet Science Institute, California Institute of Technology, Pasadena, CA, USA
| | - Mike Bottom
- Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI, USA
| | - Brendan P Bowler
- Department of Astronomy, University of Texas at Austin, Austin, TX, USA
| | | | - Carolyn J Brown
- University of Southern Queensland, Centre for Astrophysics, Toowoomba, Queensland, Australia
| | - Andrew Cancino
- Department of Physics, Astronomy and Materials Science, Missouri State University, Springfield, MO, USA
| | - David R Ciardi
- NASA Exoplanet Science Institute, California Institute of Technology, Pasadena, CA, USA
| | - Mark Clampin
- Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Jake T Clark
- University of Southern Queensland, Centre for Astrophysics, Toowoomba, Queensland, Australia
| | - Karen Collins
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
| | - Cassy Davison
- Department of Physics and Astronomy, Georgia State University, Atlanta, GA, USA
| | | | - Elise Furlan
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Eric J Gaidos
- Department of Earth Sciences, University of Hawaii at Manoa, Honolulu, HI, USA
| | - Claire Geneser
- Department of Physics and Astronomy, Mississippi State University, Starkville, MS, USA
| | - Frank Giddens
- Department of Physics, Astronomy and Materials Science, Missouri State University, Springfield, MO, USA
| | - Emily Gilbert
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | - Ryan Hall
- Department of Physics and Astronomy, Georgia State University, Atlanta, GA, USA
| | | | | | - Jonathan Horner
- University of Southern Queensland, Centre for Astrophysics, Toowoomba, Queensland, Australia
| | - Andrew W Howard
- Department of Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - Chelsea Huang
- Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Joseph Huber
- Department of Physics, Astronomy and Materials Science, Missouri State University, Springfield, MO, USA
| | - Stephen R Kane
- Department of Earth and Planetary Sciences, University of California, Riverside, CA, USA
| | | | - John Kielkopf
- Department of Physics and Astronomy, University of Louisville, Louisville, KY, USA
| | - David Kipping
- Department of Astronomy, Columbia University, New York, NY, USA
| | - Chris Klenke
- Department of Physics, Astronomy and Materials Science, Missouri State University, Springfield, MO, USA
| | - Ethan Kruse
- Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Natasha Latouf
- Department of Physics and Astronomy, George Mason University, Fairfax, VA, USA
| | | | - Bertrand Mennesson
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Matthew Mengel
- University of Southern Queensland, Centre for Astrophysics, Toowoomba, Queensland, Australia
| | - Sean M Mills
- Department of Astronomy, California Institute of Technology, Pasadena, CA, USA
| | - Tim Morton
- Astronomy Department, University of Florida, Gainesville, FL, USA
| | - Norio Narita
- Department of Astronomy, The University of Tokyo, Tokyo, Japan.,JST, PRESTO, Tokyo, Japan.,Astrobiology Center, NINS, Tokyo, Japan.,National Astronomical Observatory of Japan, NINS, Tokyo, Japan.,Instituto de Astrofisica de Canarias (IAC), La Laguna, Tenerife, Spain
| | - Elisabeth Newton
- Department of Physics and Astronomy, Dartmouth College, Hanover, NH, USA
| | - America Nishimoto
- Department of Physics, Astronomy and Materials Science, Missouri State University, Springfield, MO, USA
| | - Jack Okumura
- University of Southern Queensland, Centre for Astrophysics, Toowoomba, Queensland, Australia
| | - Enric Palle
- Instituto de Astrofisica de Canarias (IAC), La Laguna, Tenerife, Spain
| | - Joshua Pepper
- Department of Physics, Lehigh University, Bethlehem, PA, USA
| | - Elisa V Quintana
- Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Aki Roberge
- Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Veronica Roccatagliata
- Dipartimento di Fisica "Enrico Fermi", Universita' di Pisa, Pisa, Italy.,INAF-Osservatorio Astrofisico di Arcetri, Firenze, Italy.,INFN, Sezione di Pisa, Pisa, Italy
| | - Joshua E Schlieder
- Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Angelle Tanner
- Department of Physics and Astronomy, Mississippi State University, Starkville, MS, USA
| | - Johanna Teske
- Observatories of the Carnegie Institution for Science, Pasadena, CA, USA
| | - C G Tinney
- Exoplanetary Science at UNSW, School of Physics, UNSW Sydney, New South Wales, Australia
| | - Andrew Vanderburg
- Department of Astronomy, University of Texas at Austin, Austin, TX, USA
| | | | - Bernie Walp
- NASA Infrared Telescope Facility, Hilo, HI, USA
| | - Jason Wang
- Department of Astronomy, University of California, Berkeley, CA, USA.,Department of Astronomy, California Institute of Technology, Pasadena, CA, USA
| | | | - Denise Weigand
- Department of Physics, Astronomy and Materials Science, Missouri State University, Springfield, MO, USA
| | - Russel White
- Department of Physics and Astronomy, Georgia State University, Atlanta, GA, USA
| | - Robert A Wittenmyer
- University of Southern Queensland, Centre for Astrophysics, Toowoomba, Queensland, Australia
| | - Duncan J Wright
- University of Southern Queensland, Centre for Astrophysics, Toowoomba, Queensland, Australia
| | - Allison Youngblood
- Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Hui Zhang
- School of Astronomy and Space Science, Key Laboratory of Ministry of Education, Nanjing University, Nanjing, China
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27
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Kato T, Higuma T, Yokota T, Kudo N, Yokono Y, Senoo M, Narita N, Endo T, Nishizaki F, Shibutani S, Hanada K, Tomita H. P856Incidence and Outcomes of irregular protrusion after stent implantation in patients with acute myocardial infarction: An in in vivo optical coherence tomography study. Eur Heart J 2019. [DOI: 10.1093/eurheartj/ehz747.0454] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
Abstract
Background
Irregular protrusion, a protrusion of material with an irregular surface into the lumen of the vessel after stent implantation, can only be identified by optical coherence tomography (OCT). A previous study demonstrated that irregular protrusion after stent implantation was an independent predictor of 1-year major adverse cardiac events (MACE) in CAD patients. However, the true incidence and prognostic significance of irregular protrusion after stenting in patients with ST-segment elevation myocardial infarction (STEMI) have not previously examined.
Aims
The aims of this study were the following: 1) to evaluate the incidence of irregular protrusion detected by OCT in STEMI patients after stenting; and 2) to compare the long-term outcomes between patients with and without irregular protrusion.
Methods and results
A total of 210 STEMI patients who had post-procedure OCT imaging after coronary stenting within 12 hours after symptom onset were studied. We divided them into two groups: those with irregular protrusion (n=159) and those without (n=51) after stenting. There were no significant differences in baseline characteristics between the 2 groups except that peak CK-MB levels were higher in patients with irregular protrusion than those without (289 (137–563) vs. 260 (63–349) U/L, p<0.05). During mean follow-up period of 298 days, the overall incidence of MACE defined as cardiac death, target vessel-related myocardial infarction, and target lesion revascularization was 15.3%. Kaplan-Meier curve showed that the incidence of MACE did not differ between patients with and without irregular protrusion (14.7% vs. 17.7%, p=0.53 by Log-rank).
Conclusions
Irregular protrusion after stent implantation was detected in three-fourth of STEMI patients. Although patients with irregular protrusion had a greater myocardial damage, it did not influence clinical outcomes.
Acknowledgement/Funding
Donation course from Abbott Japan
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Affiliation(s)
- T Kato
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
| | - T Higuma
- St. Marianna University, Cardiology, Kawasaki, Japan
| | - T Yokota
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
| | - N Kudo
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
| | - Y Yokono
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
| | - M Senoo
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
| | - N Narita
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
| | - T Endo
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
| | - F Nishizaki
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
| | - S Shibutani
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
| | - K Hanada
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
| | - H Tomita
- Hirosaki University Graduate School of Medicine, Hirosaki, Japan
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28
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Narita M, Hanada K, Yokono Y, Narita N, Senoo M, Kimura Y, Ichikawa H, Shimada M, Tanaka M, Osanai T, Okumura K, Tomita H. P938A direct factor Xa inhibitor, rivaroxaban, attenuates cardiac hypertrophy and fibrosis in renin-overexpressing hypertensive mice. Eur Heart J 2018. [DOI: 10.1093/eurheartj/ehy564.p938] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
Affiliation(s)
- M Narita
- Hirosaki University Graduate School of Medicine, Cardiology and Nephrology, Hirosaki, Japan
| | - K Hanada
- Hirosaki University Graduate School of Medicine, Cardiology and Nephrology, Hirosaki, Japan
| | - Y Yokono
- Hirosaki University Graduate School of Medicine, Cardiology and Nephrology, Hirosaki, Japan
| | - N Narita
- Hirosaki University Graduate School of Medicine, Cardiology and Nephrology, Hirosaki, Japan
| | - M Senoo
- Hirosaki University Graduate School of Medicine, Cardiology and Nephrology, Hirosaki, Japan
| | - Y Kimura
- Hirosaki University Graduate School of Medicine, Cardiology and Nephrology, Hirosaki, Japan
| | - H Ichikawa
- Hirosaki University Graduate School of Medicine, Cardiology and Nephrology, Hirosaki, Japan
| | - M Shimada
- Hirosaki University Graduate School of Medicine, Cardiology and Nephrology, Hirosaki, Japan
| | - M Tanaka
- Hirosaki University Graduate School of Medicine, Cardiology and Nephrology, Hirosaki, Japan
| | - T Osanai
- Hirosaki University, Graduate School of Health Sciences, Hirosaki, Japan
| | - K Okumura
- Saiseikai Kumamoto Hospital, Cardiology, Kumamoto, Japan
| | - H Tomita
- Hirosaki University Graduate School of Medicine, Cardiology and Nephrology, Hirosaki, Japan
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29
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Meadows VS, Reinhard CT, Arney GN, Parenteau MN, Schwieterman EW, Domagal-Goldman SD, Lincowski AP, Stapelfeldt KR, Rauer H, DasSarma S, Hegde S, Narita N, Deitrick R, Lustig-Yaeger J, Lyons TW, Siegler N, Grenfell JL. Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment. Astrobiology 2018; 18:630-662. [PMID: 29746149 PMCID: PMC6014580 DOI: 10.1089/ast.2017.1727] [Citation(s) in RCA: 51] [Impact Index Per Article: 8.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/12/2017] [Accepted: 12/15/2017] [Indexed: 05/04/2023]
Abstract
We describe how environmental context can help determine whether oxygen (O2) detected in extrasolar planetary observations is more likely to have a biological source. Here we provide an in-depth, interdisciplinary example of O2 biosignature identification and observation, which serves as the prototype for the development of a general framework for biosignature assessment. Photosynthetically generated O2 is a potentially strong biosignature, and at high abundance, it was originally thought to be an unambiguous indicator for life. However, as a biosignature, O2 faces two major challenges: (1) it was only present at high abundance for a relatively short period of Earth's history and (2) we now know of several potential planetary mechanisms that can generate abundant O2 without life being present. Consequently, our ability to interpret both the presence and absence of O2 in an exoplanetary spectrum relies on understanding the environmental context. Here we examine the coevolution of life with the early Earth's environment to identify how the interplay of sources and sinks may have suppressed O2 release into the atmosphere for several billion years, producing a false negative for biologically generated O2. These studies suggest that planetary characteristics that may enhance false negatives should be considered when selecting targets for biosignature searches. We review the most recent knowledge of false positives for O2, planetary processes that may generate abundant atmospheric O2 without a biosphere. We provide examples of how future photometric, spectroscopic, and time-dependent observations of O2 and other aspects of the planetary environment can be used to rule out false positives and thereby increase our confidence that any observed O2 is indeed a biosignature. These insights will guide and inform the development of future exoplanet characterization missions. Key Words: Biosignatures-Oxygenic photosynthesis-Exoplanets-Planetary atmospheres. Astrobiology 18, 630-662.
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Affiliation(s)
- Victoria S. Meadows
- Department of Astronomy, University of Washington, Seattle, Washington
- NASA Astrobiology Institute, Virtual Planetary Laboratory Team, Seattle, Washington
| | - Christopher T. Reinhard
- School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, Georgia
- NASA Astrobiology Institute, Alternative Earths Team, Riverside, California
| | - Giada N. Arney
- NASA Astrobiology Institute, Virtual Planetary Laboratory Team, Seattle, Washington
- Planetary Systems Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland
| | - Mary N. Parenteau
- NASA Astrobiology Institute, Virtual Planetary Laboratory Team, Seattle, Washington
- NASA Ames Research Center, Exobiology Branch, Mountain View, California
| | - Edward W. Schwieterman
- NASA Astrobiology Institute, Virtual Planetary Laboratory Team, Seattle, Washington
- NASA Astrobiology Institute, Alternative Earths Team, Riverside, California
- Department of Earth Sciences, University of California, Riverside, California
- NASA Postdoctoral Program, Universities Space Research Association, Columbia, Maryland
- Blue Marble Space Institute of Science, Seattle, Washington
| | - Shawn D. Domagal-Goldman
- NASA Astrobiology Institute, Virtual Planetary Laboratory Team, Seattle, Washington
- Planetary Environments Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland
| | - Andrew P. Lincowski
- Department of Astronomy, University of Washington, Seattle, Washington
- NASA Astrobiology Institute, Virtual Planetary Laboratory Team, Seattle, Washington
| | - Karl R. Stapelfeldt
- NASA Exoplanet Exploration Program, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, California
| | - Heike Rauer
- German Aerospace Center, Institute of Planetary Research, Extrasolar Planets and Atmospheres, Berlin, Germany
| | - Shiladitya DasSarma
- Department of Microbiology and Immunology, School of Medicine, University of Maryland, Baltimore, Maryland
- Institute of Marine and Environmental Technology, University System of Baltimore, Maryland
| | - Siddharth Hegde
- Carl Sagan Institute, Cornell University, Ithaca, New York
- Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, New York
| | - Norio Narita
- Department of Astronomy, The University of Tokyo, Tokyo, Japan
- Astrobiology Center, NINS, Tokyo, Japan
- National Astronomical Observatory of Japan, NINS, Tokyo, Japan
| | - Russell Deitrick
- Department of Astronomy, University of Washington, Seattle, Washington
- NASA Astrobiology Institute, Virtual Planetary Laboratory Team, Seattle, Washington
| | - Jacob Lustig-Yaeger
- Department of Astronomy, University of Washington, Seattle, Washington
- NASA Astrobiology Institute, Virtual Planetary Laboratory Team, Seattle, Washington
| | - Timothy W. Lyons
- NASA Astrobiology Institute, Alternative Earths Team, Riverside, California
- Department of Earth Sciences, University of California, Riverside, California
| | - Nicholas Siegler
- NASA Exoplanet Exploration Program, Jet Propulsion Laboratory/California Institute of Technology, Pasadena, California
| | - J. Lee Grenfell
- German Aerospace Center, Institute of Planetary Research, Extrasolar Planets and Atmospheres, Berlin, Germany
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30
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Narita N, Ishii T, Kamiya K. Dissociation between physical and cognitive demands in Occlusal Dysesthesia. J Neurol Sci 2017. [DOI: 10.1016/j.jns.2017.08.745] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/26/2022]
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31
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Takizawa K, Minagawa J, Tamura M, Kusakabe N, Narita N. Red-edge position of habitable exoplanets around M-dwarfs. Sci Rep 2017; 7:7561. [PMID: 28790357 PMCID: PMC5548919 DOI: 10.1038/s41598-017-07948-5] [Citation(s) in RCA: 13] [Impact Index Per Article: 1.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/30/2016] [Accepted: 07/07/2017] [Indexed: 11/09/2022] Open
Abstract
One of the possible signs of life on distant habitable exoplanets is the red-edge, which is a rise in the reflectivity of planets between visible and near-infrared (NIR) wavelengths. Previous studies suggested the possibility that the red-edge position for habitable exoplanets around M-dwarfs may be shifted to a longer wavelength than that for Earth. We investigated plausible red-edge position in terms of the light environment during the course of the evolution of phototrophs. We show that phototrophs on M-dwarf habitable exoplanets may use visible light when they first evolve in the ocean and when they first colonize the land. The adaptive evolution of oxygenic photosynthesis may eventually also use NIR radiation, by one of two photochemical reaction centers, with the other center continuing to use visible light. These “two-color” reaction centers can absorb more photons, but they will encounter difficulty in adapting to drastically changing light conditions at the boundary between land and water. NIR photosynthesis can be more productive on land, though its evolution would be preceded by the Earth-type vegetation. Thus, the red-edge position caused by photosynthetic organisms on habitable M-dwarf exoplanets could initially be similar to that on Earth and later move to a longer wavelength.
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Affiliation(s)
- Kenji Takizawa
- Astrobiology Center, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan.,National Institute for Basic Biology, National Institutes of Natural Sciences, 38 Nishigonaka, Myodaiji, Okazaki, Aichi, 444-8585, Japan
| | - Jun Minagawa
- National Institute for Basic Biology, National Institutes of Natural Sciences, 38 Nishigonaka, Myodaiji, Okazaki, Aichi, 444-8585, Japan
| | - Motohide Tamura
- Astrobiology Center, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan.,Department of Astronomy, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan.,National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan
| | - Nobuhiko Kusakabe
- Astrobiology Center, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan.,National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan
| | - Norio Narita
- Astrobiology Center, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan. .,Department of Astronomy, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan. .,National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan.
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32
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Ichikawa H, Narita M, Nishizaki K, Kimura Y, Seno M, Narita N, Yonekura M, Tanaka M, Shimada M, Osanai T, Okumura K, Tomita H. P4489Rivaroxaban, a direct factor Xa inhibitor, ameliorates angiotensin II-induced renal damage through inhibition of protease-activated receptor pathway-mediated inflammatory response. Eur Heart J 2017. [DOI: 10.1093/eurheartj/ehx504.p4489] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/13/2022] Open
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33
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Shimoda Y, Murakami K, Narita N, Tominaga T. Fourth Ventricle Outlet Obstruction with Expanding Space on the Surface of Cerebellum. World Neurosurg 2017; 100:711.e1-711.e5. [PMID: 28153613 DOI: 10.1016/j.wneu.2017.01.088] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/04/2016] [Revised: 01/19/2017] [Accepted: 01/23/2017] [Indexed: 11/18/2022]
Abstract
BACKGROUND Hydrocephalus is classified as noncommunicating and communicating based on whether all ventricular and subarachnoid spaces are communicating. Although the diagnosis between the two different states is crucial, it is difficult in certain conditions. In particular, communicating hydrocephalus and noncommunicating hydrocephalus owing to fourth ventricle outlet obstruction are highly misdiagnosed. We describe a case of fourth ventricle outlet obstruction of unknown origin that was initially misdiagnosed as communicating hydrocephalus. CASE DESCRIPTION A 66-year-old woman with gait disturbance and incontinence caused by hydrocephalus underwent ventriculoperitoneal shunt surgery. After 9 months, her fourth ventricle became enlarged and could not be controlled by lowering the shunt pressure. Magnetic resonance imaging (MRI) demonstrated obstruction at the foramen of Magendie, foramina of Luschka, and the cerebral aqueduct. Endoscopic surgery for aqueduct plasty with third ventriculostomy was planned. Because the aqueduct was observed to open spontaneously, only the standard third ventriculostomy was performed. When MRI findings were reviewed retrospectively, an unnatural space was observed between the lower cranial nerves and cerebellar hemisphere that grew along with the fourth ventricular enlargement. This space was determined by MRI cisternography to be the cystic membrane ballooning out from the foramen of Luschka. The primary hydrocephalus likely resulted from fourth ventricle outlet obstruction. CONCLUSIONS Enlargement of the whole ventricular system with an expanded space between the lower cranial nerves and cerebellar hemisphere can be caused by fourth ventricle outlet obstruction. In such cases, preoperative evaluation of anatomic architecture and cerebrospinal fluid obstruction using MRI cisternography is essential and leads to a successful endoscopic strategy.
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Affiliation(s)
- Yoshiteru Shimoda
- Department of Neurosurgery, Kesen-numa City Hospital, Miyagi, Japan; Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Japan.
| | - Kensuke Murakami
- Department of Neurosurgery, Sendai Medical Center, Sendai, Japan
| | - Norio Narita
- Department of Neurosurgery, Kesen-numa City Hospital, Miyagi, Japan
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University Graduate School of Medicine, Sendai, Japan
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34
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Chonan M, Narita N, Tominaga T. Total regression of brain metastases in non-small cell lung cancer patients harboring EGFR mutations treated with gefitinib without radiotherapy: two case reports. BMC Res Notes 2016; 9:2. [PMID: 26724810 PMCID: PMC4698324 DOI: 10.1186/s13104-015-1834-0] [Citation(s) in RCA: 9] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/18/2015] [Accepted: 12/21/2015] [Indexed: 12/13/2022] Open
Abstract
Background Gefitinib is an epidermal growth factor receptor tyrosine kinase inhibitor. Clinical trials have reported its effectiveness in the treatment of brain metastases from non-small cell lung cancer by overcoming the blood–brain barrier. Gefitinib is generally regarded as a relatively safe agent, and several reports have described its efficacy in patients with epidermal growth factor receptor mutation-positive non-small cell lung cancer and a poor performance status. Case presentation We herein described two patients with brain metastasis from non-small cell lung cancer who achieved the total regression of metastasis with the administration of gefitinib. A 70-year-old Japanese woman was referred to our hospital with a severe cough. Brain magnetic resonance imaging revealed a metastatic lesion in the left temporal lobe. The tumor was positive for an epidermal growth factor receptor L858R mutation in exon 21 using the peptide nucleic acid-locked nucleic acid polymerase chain reaction clamp method. She was treated with 250 mg gefitinib per day, and, 1 month later, the primary lesion and brain metastasis had totally resolved. A 58-year-old Japanese woman was referred to our hospital with nausea and headache. Brain magnetic resonance imaging revealed a metastatic lesion in the left cerebellar hemisphere and meningeal dissemination. The tumor was positive for the epidermal growth factor receptor L858R mutation in exon 21. She was treated with 250 mg gefitinib per day, and, 3 weeks later, the primary lesion, brain metastasis, and meningeal dissemination had completely resolved. Conclusion We successfully treated two lung cancer patients with brain metastasis using gefitinib. Gefitinib therapy may be a suitable treatment for brain metastasis in lung cancer with an epidermal growth factor receptor mutation, particularly in elderly patients with a poor performance status.
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Affiliation(s)
- Masashi Chonan
- Department of Neurosurgery, Iwaki Kyoritsu Hospital, 16 Kusehara, Uchigo Mimaya-machi, Iwaki, Fukushima, 973-8555, Japan.
| | - Norio Narita
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Miyagi, Japan.
| | - Teiji Tominaga
- Department of Neurosurgery, Tohoku University School of Medicine, Sendai, Miyagi, Japan.
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Narisawa A, Narita N, Tominaga T, Iwasaki M, Jin K, Nakasato N. Remote Epilepsy Clinic using a Video Conferencing System. ACTA ACUST UNITED AC 2014. [DOI: 10.7887/jcns.23.136] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/23/2022]
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Tensho K, Aoki T, Morioka S, Narita N, Kato H, Saito N. Snapping pes syndrome after total knee arthroplasty. Knee Surg Sports Traumatol Arthrosc 2014; 22:192-4. [PMID: 23263260 DOI: 10.1007/s00167-012-2352-4] [Citation(s) in RCA: 11] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 08/10/2012] [Accepted: 12/10/2012] [Indexed: 11/30/2022]
Abstract
Snapping syndrome rarely occurs at the knee joint. This is the first report of snapping pes syndrome after total knee arthroplasty. Surgeons should be aware of the presence of such a case and pay attention to the fact that snapping symptoms could be caused by a residual bony prominence and a change in alignment after total knee arthroplasty.
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Affiliation(s)
- K Tensho
- Department of Orthopedic Surgery, Shinshu University School of Medicine, Asahi 3-1-1, Matsumoto, Nagano, 390-8621, Japan
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Tamai H, Ishida K, Murakami K, Narita N, Tominaga T, Fuse N. Compression neuropathy caused by cancer metastasis to the optic nerve canal. BMC Res Notes 2013; 6:546. [PMID: 24359676 PMCID: PMC3878198 DOI: 10.1186/1756-0500-6-546] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/29/2012] [Accepted: 12/18/2013] [Indexed: 11/10/2022] Open
Abstract
Background Cancerous cells are known to metastasize to different ocular structures. This happens especially to the choroid in males with lung cancer and females with breast cancer. However, we observed two cases of cancerous metastasis to the optic canal region. Both cases showed only a progressive decrease in vision without any other remarkable ophthalmological symptoms or abnormalities in the affected eye. Case presentation Two females, a 60-year-old and a 73-year-old, came to our hospital because of progressive loss of vision. These patients showed no remarkable symptoms or signs in their eyes except visual acuity loss. Several ophthalmoscopic examinations, such as slit lamp microscopy and fundoscopy, showed no abnormal changes in their affected eye but magnetic resonance imaging indicated a massive legion around the optic nerve. Conclusion It is possible for cancer to metastasize to the optic canal region and the existence of primary tumors should be considered.
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Affiliation(s)
- Hiroshi Tamai
- Department of Ophthalmology, Kesennuma City Hospital, 184 Tanaka, Kesennuma, Miyagi 988-0052, Japan.
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Shibahara I, Osawa SI, Kon H, Morita T, Nakasato N, Tominaga T, Narita N. Increase in the number of patients with seizures following the Great East-Japan Earthquake. Epilepsia 2013; 54:e49-52. [PMID: 23294222 DOI: 10.1111/epi.12070] [Citation(s) in RCA: 26] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Accepted: 11/06/2012] [Indexed: 11/28/2022]
Abstract
In the afternoon of March 11, 2011, Kesennuma City was hit by the Great East-Japan Earthquake and a devastating tsunami. The purpose of this retrospective study is to document possible changes in the number of patients with distinct neurologic diseases seeking treatment following this disaster. Because of Kesennuma's unique geographical location, the city was isolated by the disaster, allowing for a study with relatively limited population selection bias. Patients admitted for neurologic emergencies from January 14 to May 5 in 2011 (n = 117) were compared with patients in the corresponding 16-week periods in 2008-2010 (n = 323). The number of patients with unprovoked seizures was significantly higher during the 8-week period after the earthquake (n = 13) than during the same periods in 2008 (n = 6), 2009 (n = 3), and 2010 (no patients) (p = 0.0062). In contrast, the number of patients treated for other neurologic diseases such as stroke, trauma, and tumors remained unchanged. To our knowledge, this is the first report of an increase in the number of patients with seizures following a life-threatening natural disaster. We suggest that stress associated with life-threatening situations may enhance seizure generation.
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Affiliation(s)
- Ichiyo Shibahara
- Department of Neurosurgery, Kesennuma City Hospital, Kesennuma, Japan.
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Kubo S, Yamada T, Osawa Y, Ito Y, Narita N, Fujieda S. Cytosine-phosphate-guanosine-DNA induces CD274 expression in human B cells and suppresses T helper type 2 cytokine production in pollen antigen-stimulated CD4-positive cells. Clin Exp Immunol 2012; 169:1-9. [PMID: 22670772 DOI: 10.1111/j.1365-2249.2012.04585.x] [Citation(s) in RCA: 15] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/15/2023] Open
Abstract
Co-stimulatory molecules are important for regulating T cell activation and immune response. CD274 [programmed death ligand 1 (PD-L1), B7-H1] has emerged as an important immune modulator that can block T cell receptor signalling. We have investigated whether PD-L1 and other co-stimulatory ligands could be expressed in human B cells stimulated by cytosine-phosphate-guanosine (CpG)-DNA. CpG-DNA strongly induced the co-inhibitory molecule ligand, PD-L1, of human B cells. Results show that nuclear factor-kappa B (NF-κB) signalling is involved directly in CpG-DNA-induced PD-L1 expression in human B cells. We sought to determine the effect of CpG-DNA-treated B cells on T helper type 2 (Th2) cytokine production in Cry j 1 (Japanese pollen antigen)-stimulated human CD4-positive cells from patients with seasonal allergic rhinitis caused by Japanese cedar pollen. CpG-DNA-treated B cells reduced Cry j 1-induced interleukin (IL)-5 and IL-13 production in CD4-positive cells. When the binding of PD-1 to PD-L1 was inhibited by PD-1-immunoglobulin (Ig), this chimera molecule reversed the previously described reductions in IL-5 and IL-13 production. In contrast, the CpG B-treated B cells increased both interferon (IFN)-γ and IL-12 production in the presence of Cry j 1-stimulated CD4-positive cells. CpG-DNA simultaneously reduced the expression of B7RP-1 [also known as inducible co-stimulator ligand (ICOSL), B7-H2] and the ligand of CD30 (CD30L). These results indicate that CpG-DNA induces co-inhibitory molecule ligand PD-L1 expression in human B cells and PD-L1 can suppress Th2 cytokine production in Cry j 1-stimulated CD4-positive cells, while CpG-DNA increased Th1 cytokine production and reduced the expression of co-stimulatory molecule ligands that can promote Th2 inflammatory responses.
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Affiliation(s)
- S Kubo
- Department of Otorhinolaryngology, University of Fukui, Japan
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Narita N, Kumar N, Cherkas PS, Chiang CY, Dostrovsky JO, Coderre TJ, Sessle BJ. Systemic pregabalin attenuates sensorimotor responses and medullary glutamate release in inflammatory tooth pain model. Neuroscience 2012; 218:359-66. [PMID: 22609939 DOI: 10.1016/j.neuroscience.2012.05.016] [Citation(s) in RCA: 22] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/03/2012] [Revised: 04/18/2012] [Accepted: 05/04/2012] [Indexed: 11/16/2022]
Abstract
Our previous studies have demonstrated that application of inflammatory irritant mustard oil (MO) to the tooth pulp induces medullary glutamate release and central sensitization in the rat medullary dorsal horn (MDH), as well as nociceptive sensorimotor responses in craniofacial muscles in rats. There is recent evidence that anticonvulsant drugs such as pregabalin that influence glutamatergic neurotransmission are effective in several pain states. The aim of this study was to examine whether systemic administration of pregabalin attenuated glutamate release in the medulla as well as these nociceptive effects reflected in increased electromyographic (EMG) activity induced by MO application to the tooth pulp. Male adult rats were anesthetized with isofluorane (1.0-1.2%), and jaw and tongue muscle EMG activities were recorded by needle electrodes inserted bilaterally into masseter and anterior digastric muscles and into the genioglossus muscle, and also the medullary release of glutamate was assessed by in vivo microdialysis. Pregabalin or vehicle control (isotonic saline) was administered 30 min before the pulpal application of MO or vehicle control (mineral oil). Application of mineral oil to the maxillary first molar tooth pulp produced no change in baseline EMG activity and glutamate release. However, application of MO to the pulp significantly increased both the medullary release of glutamate and EMG activity in the jaw and tongue muscles for several minutes. In contrast, pre-medication with pregabalin, but not vehicle control, significantly and dose-dependently attenuated the medullary glutamate release and EMG activity in these muscles after MO application to the tooth pulp (analysis of variance (ANOVA), p<0.05). These results suggest that pregabalin may attenuate the medullary release of glutamate and associated nociceptive sensorimotor responses in this acute inflammatory pulpal pain model, and that it may prove useful for the treatment of orofacial inflammatory pain states.
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Affiliation(s)
- N Narita
- Nihon University School of Dentistry at Matsudo, Department of Removable Prosthodontics, 2-870-1, Sakaecho-Nishi, Matsudo, Chiba 271-8587, Japan.
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Narita N. Good Combination of the Rossiter-McLaughlin Measurements and Direct Imaging Observations. EPJ Web of Conferences 2011. [DOI: 10.1051/epjconf/20101105004] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
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Murakami T, Narita N, Shibata T, Nakagaki H, Koga H, Nishimuta M. Influence of beverage and food consumption on fluoride intake in Japanese children aged 3-5 years. Caries Res 2009; 43:382-6. [PMID: 19696482 DOI: 10.1159/000235646] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/28/2008] [Accepted: 07/13/2009] [Indexed: 11/19/2022] Open
Abstract
This study was conducted to estimate the relative contribution of particular foods and drinks to dietary fluoride intake in 94 preschool Japanese children in low-fluoride areas. The mean daily fluoride intake from all beverages (548 +/- 162 g) was 0.108 mg (SD = 0.082), accounting for 37% of the total dietary fluoride; tea beverages showed the highest value, 0.093 mg (SD = 0.081), 32%. That from staple food and side dishes was 0.183 mg (SD = 0.146), 63%, followed by cereals (12%), fish (8%) and bean products (5%). In conclusion, the contribution of beverages excluding tea to dietary fluoride intake is small in Japanese children.
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Affiliation(s)
- T Murakami
- Department of Preventive Dentistry and Dental Public Health, School of Dentistry, Aichi-Gakuin University, Chikusa-ku, Nagoya, Japan.
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Abstract
Heartworm caval syndrome (CS) occurred in three dogs under 2 years of age. A 23-month-old dog was recovered by surgical and medical treatments, but the other 2 dogs (15 and 21 months old) died. Necropsy demonstrated 12 heartworms in the 15-month-old dog and 8 worms in the 21-month-old dog. Histopathologically, pulmonary arterial embolism caused by dead worms and thrombi were observed in these cases. The findings suggested that CS could develop regardless of canine age and worm burden if pulmonary arterial embolism related to worm death or thrombus formation were induced.
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Affiliation(s)
- Yuichi Hidaka
- Department of Veterinary Surgery, Faculty of Agriculture, Miyazaki University, Miyazaki, Japan
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Hashimoto K, Tomitaka S, Narita N, Minabe Y, Iyo M, Fukui S. Induction of heat shock protein (HSP)-70 in posterior cingulate and retrosplenial cortex of rat brain by dizocilpine and phencyclidine: lack of protective effects of sigma receptor ligands. Addict Biol 2003; 1:61-70. [PMID: 12893487 DOI: 10.1080/1355621961000124696] [Citation(s) in RCA: 30] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/27/2022]
Abstract
The role of sigma receptors in the induction of heat shock protein (HSP)-70 by non-competitive N-methyl-Daspartate (NMDA) receptor antagonists (+)-MK-801 (dizocilpine) and phencyclidine (PCP) was studied. HSP-70 is induced in the posterior cingulate and retrosplenial cortex of rat brain 24 hours after a single administration of dizocilpine (1 mg/kg) or PCP (50 mg/kg). The induction of heat shock protein HSP-70 by dizocilpine or PCP was attenuated partially by pre-treatment with the antipsychotic drug haloperidol (3 mg/kg, i.p., 15 minutes previously). However, pre-treatment with high potent and selective sigma receptor ligands, 4-phenyl-4-(1-phenylbutyl)piperidine (4-PPBP, 3 mg/kg, i.p., 15 minutes previously) and N,N-dipropyl-2-[4-methoxy-3-(2-phenylethoxy)phenyl]-ethylamine monohydrochloride) (NE-100, 3 mg/kg, i.p., 15 minutes previously) did not alter the induction of HSP-70 by dizocilpine or PCP. These findings suggest that sigma receptors may not play a significant role in the induction of HSP-70 by non-competitive NMDA receptor antagonists dizocilpine and PCP, and that protective effects of haloperidol on induction of HSP-70 protein by dizocilpine or PCP may be due to other effect(s) except sigma receptors.
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Affiliation(s)
- K Hashimoto
- Division of Cortical Function Disorder, National Institute of Neuroscience, National Center of Neurology and Psychiatry, Kodaira, Tokyo
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Higashida K, Narita N, Tanaka M, Morikawa T, Miura Y, Onodera R. Crack tip dislocations in silicon characterized by highvoltage electron microscopy. ACTA ACUST UNITED AC 2002. [DOI: 10.1080/01418610210141307] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/27/2022]
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Kiiveri S, Liu J, Westerholm-Ormio M, Narita N, Wilson DB, Voutilainen R, Heikinheimo M. Transcription factors GATA-4 and GATA-6 during mouse and human adrenocortical development. Endocr Res 2002; 28:647-50. [PMID: 12530677 DOI: 10.1081/erc-120016980] [Citation(s) in RCA: 16] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/03/2022]
Abstract
Our earlier work implicates transcription factors GATA-4 and GATA-6 in the murine adrenal. We have now studied their expression during mouse and human adrenal development in detail. GATA-4 and GATA-6 mRNAs are readily detectable from embryonic day 15 in mouse and gestational week 19 in human adrenal cortex. In postnatal adrenal, GATA-4 expression is down-regulated, whereas GATA-6 mRNA and protein continue to be abundantly present. In a human adrenocortical cell line NCI-H295R, GATA-6 mRNA is up-regulated by cAMP. This cell line does not express GATA-4. Our findings suggest that GATA-6 expression is hormonally controlled, and required throughout adrenal development from fetal to adult age. GATA-4, on the other hand, may serve a role in fetal adrenal gene regulation.
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Affiliation(s)
- S Kiiveri
- Children's Hospital, P.O. Box 63, 00014, University of Helsinki, Finland
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Murakami T, Narita N, Nakagaki H, Shibata T, Robinson C. Fluoride intake in Japanese children aged 3-5 years by the duplicate-diet technique. Caries Res 2002; 36:386-90. [PMID: 12459609 DOI: 10.1159/000066537] [Citation(s) in RCA: 11] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/19/2022] Open
Abstract
This study was conducted to determine the fluoride intakes in 94 preschool children aged 3, 4 and 5 (n = 30, 30, 34, respectively) residing in Yokkaichi, Mie Prefecture (< 0.16 ppm F water supply). The parents duplicated all the diets that their children ingested on 3 separate days during a 1-year period. The acid-diffusible fluoride in the diet was isolated by the acid-diffusion technique and measured with a fluoride electrode. The mean daily fluoride intakes from diet alone by children aged 3, 4 and 5 were 0.30 mg (n = 29, SD 0.19), 0.28 mg (n = 30, SD 0.19) and 0.30 mg (n = 34, SD 0.19), respectively. The total estimated mean values from diet and dentifrice were 0.35 mg (n = 29, SD 0.22, range 0.13-1.00), 0.33 mg (n = 30, SD 0.19, range 0.13-0.86) and 0.39 mg (n = 34, SD 0.18, range 0.18-1.01), respectively. It was concluded that the mean (+/-SD) total fluoride from diet and dentifrice in 3- to 5-year-old Japanese children was 0.35 +/- 0.19 mg/day (0.021 +/- 0.012 mg/kg body weight).
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Affiliation(s)
- T Murakami
- Department of Preventive Dentistry and Dental Public Health, School of Dentistry, Nagoya, Japan.
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Tezuka T, Narita N. Hydroxylation of benzene with .alpha.-azohydroperoxide. A novel route for generation of hydroxyl radical and its reaction in anhydrous media. J Am Chem Soc 2002. [DOI: 10.1021/ja00518a053] [Citation(s) in RCA: 23] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/29/2022]
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