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Hamilton VE, Simon AA, Christensen PR, Reuter DC, Clark BE, Barucci MA, Bowles NE, Boynton WV, Brucato JR, Cloutis EA, Connolly HC, Hanna KLD, Emery JP, Enos HL, Fornasier S, Haberle CW, Hanna RD, Howell ES, Kaplan HH, Keller LP, Lantz C, Li JY, Lim LF, McCoy TJ, Merlin F, Nolan MC, Praet A, Rozitis B, Sandford SA, Schrader DL, Thomas CA, Zou XD, Lauretta DS. Evidence for widespread hydrated minerals on asteroid (101955) Bennu. Nat Astron 2019; 3:332-340. [PMID: 31360777 PMCID: PMC6662227 DOI: 10.1038/s41550-019-0722-2] [Citation(s) in RCA: 46] [Impact Index Per Article: 9.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/29/2019] [Accepted: 02/12/2019] [Indexed: 05/18/2023]
Abstract
Early spectral data from the Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) mission reveal evidence for abundant hydrated minerals on the surface of near-Earth asteroid (101955) Bennu in the form of a near-infrared absorption near 2.7 μm and thermal infrared spectral features that are most similar to those of aqueously altered CM carbonaceous chondrites. We observe these spectral features across the surface of Bennu, and there is no evidence of substantial rotational variability at the spatial scales of tens to hundreds of meters observed to date. In the visible and near-infrared (0.4 to 2.4 μm) Bennu's spectrum appears featureless and with a blue (negative) slope, confirming previous ground-based observations. Bennu may represent a class of objects that could have brought volatiles and organic chemistry to Earth.
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Affiliation(s)
- V. E. Hamilton
- Department of Space Studies, Southwest Research Institute, Boulder, CO, USA
| | - A. A. Simon
- NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - P. R. Christensen
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - D. C. Reuter
- NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - B. E. Clark
- Department of Physics and Astronomy, Ithaca College, Ithaca, NY, USA
| | | | - N. E. Bowles
- Department of Atmospheric, Oceanic and Planetary Physics, University of Oxford, Oxford, UK
| | - W. V. Boynton
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
| | - J. R. Brucato
- INAF-Astrophysical Observatory of Arcetri, Firenze, Italy
| | - E. A. Cloutis
- Department of Geography, University of Winnipeg, Winnipeg, Canada
| | - H. C. Connolly
- Department of Geology, Rowan University, Glassboro, NJ, USA
| | - K. L. Donaldson Hanna
- Department of Atmospheric, Oceanic and Planetary Physics, University of Oxford, Oxford, UK
| | - J. P. Emery
- Department of Earth and Planetary Science, University of Tennessee, Knoxville, TN, USA
| | - H. L. Enos
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
| | | | - C. W. Haberle
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - R. D. Hanna
- Jackson School of Geosciences, University of Texas, Austin, TX, USA
| | - E. S. Howell
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
| | - H. H. Kaplan
- Department of Space Studies, Southwest Research Institute, Boulder, CO, USA
| | - L. P. Keller
- ARES, NASA Johnson Space Center, Houston, TX USA
| | - C. Lantz
- Institut d’Astrophysique Spatiale, CNRS/Université Paris Sud, Orsay, France
| | - J.-Y. Li
- Planetary Science Institute, Tucson, AZ, USA
| | - L. F. Lim
- NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - T. J. McCoy
- Smithsonian Institution, National Museum of Natural History, Washington, D.C., USA
| | - F. Merlin
- LESIA, Observatoire de Paris, France
| | - M. C. Nolan
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
| | - A. Praet
- LESIA, Observatoire de Paris, France
| | - B. Rozitis
- Planetary and Space Sciences, The Open University, Milton Keynes, UK
| | | | - D. L. Schrader
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - C. A. Thomas
- Department of Physics and Astronomy, Northern Arizona University, Flagstaff, AZ, USA
| | - X.-D. Zou
- Planetary Science Institute, Tucson, AZ, USA
| | - D. S. Lauretta
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
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2
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Filacchione G, Raponi A, Capaccioni F, Ciarniello M, Tosi F, Capria MT, De Sanctis MC, Migliorini A, Piccioni G, Cerroni P, Barucci MA, Fornasier S, Schmitt B, Quirico E, Erard S, Bockelee-Morvan D, Leyrat C, Arnold G, Mennella V, Ammannito E, Bellucci G, Benkhoff J, Bibring JP, Blanco A, Blecka MI, Carlson R, Carsenty U, Colangeli L, Combes M, Combi M, Crovisier J, Drossart P, Encrenaz T, Federico C, Fink U, Fonti S, Fulchignoni M, Ip WH, Irwin P, Jaumann R, Kuehrt E, Langevin Y, Magni G, McCord T, Moroz L, Mottola S, Palomba E, Schade U, Stephan K, Taylor F, Tiphene D, Tozzi GP, Beck P, Biver N, Bonal L, Combe JP, Despan D, Flamini E, Formisano M, Frigeri A, Grassi D, Gudipati MS, Kappel D, Longobardo A, Mancarella F, Markus K, Merlin F, Orosei R, Rinaldi G, Cartacci M, Cicchetti A, Hello Y, Henry F, Jacquinod S, Reess JM, Noschese R, Politi R, Peter G. Seasonal exposure of carbon dioxide ice on the nucleus of comet 67P/Churyumov-Gerasimenko. Science 2016; 354:1563-1566. [DOI: 10.1126/science.aag3161] [Citation(s) in RCA: 49] [Impact Index Per Article: 6.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/08/2016] [Accepted: 10/28/2016] [Indexed: 11/02/2022]
Affiliation(s)
- G. Filacchione
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - A. Raponi
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - F. Capaccioni
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - M. Ciarniello
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - F. Tosi
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - M. T. Capria
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - M. C. De Sanctis
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - A. Migliorini
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - G. Piccioni
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - P. Cerroni
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - M. A. Barucci
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - S. Fornasier
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - B. Schmitt
- Université Grenoble Alpes, CNRS, Institut de Planetologie et d’Astrophysique de Grenoble, Grenoble, France
| | - E. Quirico
- Université Grenoble Alpes, CNRS, Institut de Planetologie et d’Astrophysique de Grenoble, Grenoble, France
| | - S. Erard
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - D. Bockelee-Morvan
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - C. Leyrat
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - G. Arnold
- Institute for Planetary Research, DLR (Deutschen Zentrums für Luft- und Raumfahrt), Berlin, Germany
| | - V. Mennella
- INAF Osservatorio di Capodimonte, Naples, Italy
| | - E. Ammannito
- Department of Earth, Planetary, and Space Sciences, University of California–Los Angeles, 603 Charles Young Drive, Los Angeles, CA 90095-1567, USA
| | - G. Bellucci
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - J. Benkhoff
- ESA (European Space Agency), European Space Research and Technology Centre, Noordwjik, Netherlands
| | - J. P. Bibring
- Institut d’Astrophysique Spatial, CNRS, Orsay, France
| | - A. Blanco
- Dipartimento di Matematica e Fisica “Ennio De Giorgi,” Università del Salento, Lecce, Italy
| | - M. I. Blecka
- Space Research Centre, Polish Academy of Sciences, Warsaw, Poland
| | - R. Carlson
- NASA JPL (Jet Propulsion Laboratory), California Institute of Technology, Pasadena, CA 91109, USA
| | - U. Carsenty
- Université Grenoble Alpes, CNRS, Institut de Planetologie et d’Astrophysique de Grenoble, Grenoble, France
| | - L. Colangeli
- ESA (European Space Agency), European Space Research and Technology Centre, Noordwjik, Netherlands
| | - M. Combes
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - M. Combi
- Space Physics Research Laboratory, The University of Michigan, Ann Arbor, MI 48109, USA
| | - J. Crovisier
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - P. Drossart
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - T. Encrenaz
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | | | - U. Fink
- Lunar Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA
| | - S. Fonti
- Dipartimento di Matematica e Fisica “Ennio De Giorgi,” Università del Salento, Lecce, Italy
| | - M. Fulchignoni
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - W.-H. Ip
- National Central University, Taipei, Taiwan
| | - P. Irwin
- Departement of Physics, Oxford University, Oxford, UK
| | - R. Jaumann
- Institute for Planetary Research, DLR (Deutschen Zentrums für Luft- und Raumfahrt), Berlin, Germany
| | - E. Kuehrt
- Institute for Planetary Research, DLR (Deutschen Zentrums für Luft- und Raumfahrt), Berlin, Germany
| | - Y. Langevin
- Institut d’Astrophysique Spatial, CNRS, Orsay, France
| | - G. Magni
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - T. McCord
- Bear Fight Institute, Winthrop, WA 98862, USA
| | - L. Moroz
- Institute for Planetary Research, DLR (Deutschen Zentrums für Luft- und Raumfahrt), Berlin, Germany
| | - S. Mottola
- Institute for Planetary Research, DLR (Deutschen Zentrums für Luft- und Raumfahrt), Berlin, Germany
| | - E. Palomba
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - U. Schade
- Helmholtz-Zentrum Berlin für Materialien und Energie, Berlin, Germany
| | - K. Stephan
- Institute for Planetary Research, DLR (Deutschen Zentrums für Luft- und Raumfahrt), Berlin, Germany
| | - F. Taylor
- Departement of Physics, Oxford University, Oxford, UK
| | - D. Tiphene
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - G. P. Tozzi
- INAF Osservatorio Astrofisico di Arcetri, Firenze, Italy
| | - P. Beck
- Université Grenoble Alpes, CNRS, Institut de Planetologie et d’Astrophysique de Grenoble, Grenoble, France
| | - N. Biver
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - L. Bonal
- Université Grenoble Alpes, CNRS, Institut de Planetologie et d’Astrophysique de Grenoble, Grenoble, France
| | | | - D. Despan
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | | | - M. Formisano
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - A. Frigeri
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - D. Grassi
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - M. S. Gudipati
- NASA JPL (Jet Propulsion Laboratory), California Institute of Technology, Pasadena, CA 91109, USA
| | - D. Kappel
- Institute for Planetary Research, DLR (Deutschen Zentrums für Luft- und Raumfahrt), Berlin, Germany
| | - A. Longobardo
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - F. Mancarella
- Dipartimento di Matematica e Fisica “Ennio De Giorgi,” Università del Salento, Lecce, Italy
| | - K. Markus
- Institute for Planetary Research, DLR (Deutschen Zentrums für Luft- und Raumfahrt), Berlin, Germany
| | - F. Merlin
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - R. Orosei
- INAF Istituto di Radioastronomia, Bologna, Italy
| | - G. Rinaldi
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - M. Cartacci
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - A. Cicchetti
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - Y. Hello
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - F. Henry
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - S. Jacquinod
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - J. M. Reess
- Laboratoire d’Études Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Paris Sciences and Letters Research University, CNRS (Centre National de la Recherche Scientifique), Sorbonne Universités, UPMC (Université Pierre et Marie Curie) Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité, France
| | - R. Noschese
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - R. Politi
- INAF-IAPS (Istituto Nazionale di AstroFisica–Istituto di Astrofisica e Planetologia Spaziali), Rome, Italy
| | - G. Peter
- Institute of Optical Sensor Systems, DLR, Berlin, Germany
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3
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Capaccioni F, Coradini A, Filacchione G, Erard S, Arnold G, Drossart P, De Sanctis MC, Bockelee-Morvan D, Capria MT, Tosi F, Leyrat C, Schmitt B, Quirico E, Cerroni P, Mennella V, Raponi A, Ciarniello M, McCord T, Moroz L, Palomba E, Ammannito E, Barucci MA, Bellucci G, Benkhoff J, Bibring JP, Blanco A, Blecka M, Carlson R, Carsenty U, Colangeli L, Combes M, Combi M, Crovisier J, Encrenaz T, Federico C, Fink U, Fonti S, Ip WH, Irwin P, Jaumann R, Kuehrt E, Langevin Y, Magni G, Mottola S, Orofino V, Palumbo P, Piccioni G, Schade U, Taylor F, Tiphene D, Tozzi GP, Beck P, Biver N, Bonal L, Combe JP, Despan D, Flamini E, Fornasier S, Frigeri A, Grassi D, Gudipati M, Longobardo A, Markus K, Merlin F, Orosei R, Rinaldi G, Stephan K, Cartacci M, Cicchetti A, Giuppi S, Hello Y, Henry F, Jacquinod S, Noschese R, Peter G, Politi R, Reess JM, Semery A. Cometary science. The organic-rich surface of comet 67P/Churyumov-Gerasimenko as seen by VIRTIS/Rosetta. Science 2015; 347:aaa0628. [PMID: 25613895 DOI: 10.1126/science.aaa0628] [Citation(s) in RCA: 266] [Impact Index Per Article: 29.6] [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
The VIRTIS (Visible, Infrared and Thermal Imaging Spectrometer) instrument on board the Rosetta spacecraft has provided evidence of carbon-bearing compounds on the nucleus of the comet 67P/Churyumov-Gerasimenko. The very low reflectance of the nucleus (normal albedo of 0.060 ± 0.003 at 0.55 micrometers), the spectral slopes in visible and infrared ranges (5 to 25 and 1.5 to 5% kÅ(-1)), and the broad absorption feature in the 2.9-to-3.6-micrometer range present across the entire illuminated surface are compatible with opaque minerals associated with nonvolatile organic macromolecular materials: a complex mixture of various types of carbon-hydrogen and/or oxygen-hydrogen chemical groups, with little contribution of nitrogen-hydrogen groups. In active areas, the changes in spectral slope and absorption feature width may suggest small amounts of water-ice. However, no ice-rich patches are observed, indicating a generally dehydrated nature for the surface currently illuminated by the Sun.
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Affiliation(s)
- F Capaccioni
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy.
| | - A Coradini
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - G Filacchione
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - S Erard
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - G Arnold
- Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Berlin, Germany
| | - P Drossart
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - M C De Sanctis
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - D Bockelee-Morvan
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - M T Capria
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - F Tosi
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - C Leyrat
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - B Schmitt
- Université Grenoble Alpes, CNRS, Institut de Planétologie et d'Astrophysique de Grenoble, Grenoble, France
| | - E Quirico
- Université Grenoble Alpes, CNRS, Institut de Planétologie et d'Astrophysique de Grenoble, Grenoble, France
| | - P Cerroni
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - V Mennella
- Osservatorio di Capodimonte, INAF, Napoli, Italy
| | - A Raponi
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - M Ciarniello
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - T McCord
- Bear Fight Institute, Winthrop, WA 98862, USA
| | - L Moroz
- Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Berlin, Germany
| | - E Palomba
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - E Ammannito
- University of California, Los Angeles, Los Angeles, CA 90095, USA
| | - M A Barucci
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - G Bellucci
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - J Benkhoff
- European Space Agency (ESA), European Space Research and Technology Centre (ESTEC), Noordwijk, Netherlands
| | - J P Bibring
- Institut d'Astrophysique Spatial, CNRS, Orsay, France
| | - A Blanco
- Dipartimento di Matematica e Fisica "Ennio De Giorgi," Università del Salento, Italy
| | - M Blecka
- Space Research Centre, Polish Academy of Sciences, Warsaw, Poland
| | - R Carlson
- NASA Jet Propulsion Laboratory, Pasadena, CA 91109, USA
| | - U Carsenty
- Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Berlin, Germany
| | - L Colangeli
- European Space Agency (ESA), European Space Research and Technology Centre (ESTEC), Noordwijk, Netherlands
| | - M Combes
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - M Combi
- Space Physics Research Laboratory, The University of Michigan, Ann Arbor, MI 48109, USA
| | - J Crovisier
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - T Encrenaz
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | | | - U Fink
- Lunar Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA
| | - S Fonti
- Dipartimento di Matematica e Fisica "Ennio De Giorgi," Università del Salento, Italy
| | - W H Ip
- National Central University, Taipei, Taiwan
| | - P Irwin
- Departement of Physics, Oxford University, Oxford, UK
| | - R Jaumann
- Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Berlin, Germany. Free University of Berlin, Institute of Geosciences, Malteserstraße 74-100, Building Haus A, 12249 Berlin, Germany
| | - E Kuehrt
- Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Berlin, Germany
| | - Y Langevin
- Institut d'Astrophysique Spatial, CNRS, Orsay, France
| | - G Magni
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - S Mottola
- Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Berlin, Germany
| | - V Orofino
- Dipartimento di Matematica e Fisica "Ennio De Giorgi," Università del Salento, Italy
| | - P Palumbo
- Università "Parthenope," Napoli, Italy
| | - G Piccioni
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - U Schade
- Helmholtz-Zentrum Berlin für Materialien und Energie, Berlin, Germany
| | - F Taylor
- Departement of Physics, Oxford University, Oxford, UK
| | - D Tiphene
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - G P Tozzi
- Osservatorio Astrofisico di Arcetri, INAF, Firenze, Italy
| | - P Beck
- Université Grenoble Alpes, CNRS, Institut de Planétologie et d'Astrophysique de Grenoble, Grenoble, France
| | - N Biver
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - L Bonal
- Université Grenoble Alpes, CNRS, Institut de Planétologie et d'Astrophysique de Grenoble, Grenoble, France
| | - J-Ph Combe
- Bear Fight Institute, Winthrop, WA 98862, USA
| | - D Despan
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - E Flamini
- Agenzia Spaziale Italiana, Rome, Italy
| | - S Fornasier
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - A Frigeri
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - D Grassi
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - M Gudipati
- NASA Jet Propulsion Laboratory, Pasadena, CA 91109, USA. Institute for Physical Science and Technology, University of Maryland, College Park, MD 20742, USA
| | - A Longobardo
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - K Markus
- Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Berlin, Germany
| | - F Merlin
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - R Orosei
- Istituto di Radioastronomia, INAF, Bologna, Italy
| | - G Rinaldi
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - K Stephan
- Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Berlin, Germany
| | - M Cartacci
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - A Cicchetti
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - S Giuppi
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - Y Hello
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - F Henry
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - S Jacquinod
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - R Noschese
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - G Peter
- Institut für Optische Sensorsysteme, DLR, Berlin, Germany
| | - R Politi
- Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica (INAF), Rome, Italy
| | - J M Reess
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
| | - A Semery
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris/CNRS/Université Pierre et Marie Curie[acute accent over last letter in "Université"]/Université Paris-Diderot, Meudon, France
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A'Hearn MF, Belton MJS, Delamere WA, Feaga LM, Hampton D, Kissel J, Klaasen KP, McFadden LA, Meech KJ, Melosh HJ, Schultz PH, Sunshine JM, Thomas PC, Veverka J, Wellnitz DD, Yeomans DK, Besse S, Bodewits D, Bowling TJ, Carcich BT, Collins SM, Farnham TL, Groussin O, Hermalyn B, Kelley MS, Kelley MS, Li JY, Lindler DJ, Lisse CM, McLaughlin SA, Merlin F, Protopapa S, Richardson JE, Williams JL. EPOXI at Comet Hartley 2. Science 2011; 332:1396-400. [DOI: 10.1126/science.1204054] [Citation(s) in RCA: 351] [Impact Index Per Article: 27.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
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Thiébaut R, Douchin V, Jung C, Merlin F, Colombel JF, Lemann M, Almer S, Tysk C, O'Morain C, Gassull M, Finkel Y, Zouali H, Pascoe L, Hugot JP. RIP2 polymorphisms in inflammatory bowel diseases. Inflamm Bowel Dis 2011; 17:1055. [PMID: 20645315 DOI: 10.1002/ibd.21406] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 01/07/2023]
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Thiébaut R, Kotti S, Jung C, Merlin F, Colombel JF, Lemann M, Almer S, Tysk C, O'Morain M, Gassull M, Binder V, Finkel Y, Pascoe L, Hugot JP. TNFSF15 polymorphisms are associated with susceptibility to inflammatory bowel disease in a new European cohort. Am J Gastroenterol 2009; 104:384-91. [PMID: 19174806 DOI: 10.1038/ajg.2008.36] [Citation(s) in RCA: 52] [Impact Index Per Article: 3.5] [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: 12/11/2022]
Abstract
OBJECTIVES Inflammatory bowel disease (IBD), e.g., Crohn's disease (CD) and ulcerative colitis (UC), is a complex genetic disorder. Tumor necrosis factor (ligand) superfamily, member 15 (TNFSF15) has been previously identified as a susceptibility gene for CD in Japanese and UK cohorts. This replication study was designed in order to confirm and further validate the role of TNFSF15 in IBD. METHODS A total of 666 IBD families (corresponding to 2,982 relatives) with European ancestry were genotyped for the rs6478108 and rs7869487 polymorphisms, which define the main TNFSF15 haplotypes previously associated with CD. An association between the main haplotypes and CD, UC and IBD was tested using the Genehunter TDT and Unphased statistics. Caspase recruitment domain 15 (CARD15)/TNFSF15 interaction and genotype/phenotype correlations were also studied. RESULTS The previously reported "high-risk" haplotype (A) was associated with IBD (P=0.001) (OR=1.25 (1.05-1.50)) and CD (P=0.02) (OR=1.31 (1.03-1.67)) whereas the "protective" (B) haplotype was significantly less transmitted to IBD and CD patients. No interaction between CARD15 and TNFSF15 was detected. We also failed to define a clinical subgroup of CD patients specifically associated with TNFSF15 haplotype A. CONCLUSIONS This study confirms that TNFSF15 or a closely linked gene is involved in the genetic predisposition to CD.
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Affiliation(s)
- R Thiébaut
- INSERM, U843, Hôpital Robert Debré, Université Paris Diderot, Paris, France
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Merlin F, Prochilo T, Kildani B, Lombardi C, Pasolini G, Bonetti F, Beretta GD. Discoid lupus erythematosus (DLE)-like lesions induced by capecitabine. Int J Colorectal Dis 2008; 23:715-6. [PMID: 18330579 DOI: 10.1007/s00384-008-0462-8] [Citation(s) in RCA: 15] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Accepted: 02/13/2008] [Indexed: 02/04/2023]
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8
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Porcaro A, Sava T, Merlin F, Romano M, Ghimenton C, Cesaro G, Cetto G, Comunale L. HORMONE REFRACTORY METASTATIC PROSTATE CANCER: DOES PSA HALVING TIME DURING DOCETAXEL TREATMENT HAVE A PROGNOSTIC ROLE? ACTA ACUST UNITED AC 2008. [DOI: 10.1016/s1569-9056(08)60639-9] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [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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9
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Merlin F, Riolfi M, Sava T, Consoli F, Griso C, Manno P, Porcaro AB, Ghimenton C, Comunale L, Cetto G. Upper urinary tract cancer: Prognostic factors for bladder tumours development and systemic relapse. J Clin Oncol 2006. [DOI: 10.1200/jco.2006.24.18_suppl.14560] [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] [Indexed: 11/20/2022] Open
Abstract
14560 Background: Transitional cell carcinomas (TCC) of the renal pelvis and ureter are relatively uncommon. An important characteristic of TCC is multifocality throughout the all urinary tract simultaneously and/or subsequently. To clarify the association between UTTCC and bladder tumors, we retrospectively analysed 86 patients with UTTCC in order to evaluate prognostic factors for recurrence and to identify risk factors for development of bladder cancers. Methods: All 86 upper tract transitional cell carcinoma patients (pts) were treated surgically between January 1988 and July 2005. Median age was 69 years (range: 34–91). We observed a male predominance (71%) and 78% of patients were heavy smokers. Forty-five (52.3%) patients had a diagnosis of bladder transitional carcinoma. The median age of this group of patients was 70 range 40–87). In fifteen cases (17%), bladder tumour occurred first than upper tract neoplasia; in 14 patients bladder and upper tract tumours were synchronous. Results: Median survival was 97 months; 49 (57%) patients are alive and 43 are disease-free. Grading, stage T, lympho-vascular invasion and squamous differentiation were significant prognostic factors for systemic relapse (p < 0.05). Twenty-eight pts (32.5%) developed subsequent transitional bladder cancer after a median time of 12 months; multifocality of primitive tumours was significant predictive factor. Invasive UTTCC were less likely associated with bladder cancer. We observed that superficial bladder cancer developed more frequently in pts with well differentiated (G1–2) primitive cancer (90% of cases), without lympho-vascular invasion and with history of heavy smoke exposition. Conclusions: In our study, T, N and G confirmed to be the most important prognostic factors for systemic relapse. Lympho-vascular invasion highly predicts metastasis. Our analysis highlights that upper urinary tract cancers seem to have different history and different pattern of association with bladder tumours, according to specific prognostic factors. The development of recurrent superficial bladder cancer is more frequently associated with small well differentiated multifocal upper tract tumours.Therefore follow-up should be oriented according to these characteristics. No significant financial relationships to disclose.
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Affiliation(s)
- F. Merlin
- University of Verona, Verona, Italy; Ospedale Civile Maggiore, Verona, Italy
| | - M. Riolfi
- University of Verona, Verona, Italy; Ospedale Civile Maggiore, Verona, Italy
| | - T. Sava
- University of Verona, Verona, Italy; Ospedale Civile Maggiore, Verona, Italy
| | - F. Consoli
- University of Verona, Verona, Italy; Ospedale Civile Maggiore, Verona, Italy
| | - C. Griso
- University of Verona, Verona, Italy; Ospedale Civile Maggiore, Verona, Italy
| | - P. Manno
- University of Verona, Verona, Italy; Ospedale Civile Maggiore, Verona, Italy
| | - A. B. Porcaro
- University of Verona, Verona, Italy; Ospedale Civile Maggiore, Verona, Italy
| | - C. Ghimenton
- University of Verona, Verona, Italy; Ospedale Civile Maggiore, Verona, Italy
| | - L. Comunale
- University of Verona, Verona, Italy; Ospedale Civile Maggiore, Verona, Italy
| | - G. Cetto
- University of Verona, Verona, Italy; Ospedale Civile Maggiore, Verona, Italy
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Fraccon AP, Sava T, Martignoni G, Pessa S, Frisinghelli M, Merlin F, Bassetto MA, Franceschi T, Sava C, Cetto GL. Postchemotherapy residual masses (rm) in testicular nonseminomatous germ cell tumor (TNSGCT): Role of prognostic factors and adjuvant chemotherapy. J Clin Oncol 2005. [DOI: 10.1200/jco.2005.23.16_suppl.4662] [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: 11/20/2022] Open
Affiliation(s)
- A. P. Fraccon
- Dept Onc Med, Verona, Italy; Pathology, Verona, Italy; Dept Onc Med, Treviso, Italy; Med Onc, Mater Salutis Hospital Legnago, Italy
| | - T. Sava
- Dept Onc Med, Verona, Italy; Pathology, Verona, Italy; Dept Onc Med, Treviso, Italy; Med Onc, Mater Salutis Hospital Legnago, Italy
| | - G. Martignoni
- Dept Onc Med, Verona, Italy; Pathology, Verona, Italy; Dept Onc Med, Treviso, Italy; Med Onc, Mater Salutis Hospital Legnago, Italy
| | - S. Pessa
- Dept Onc Med, Verona, Italy; Pathology, Verona, Italy; Dept Onc Med, Treviso, Italy; Med Onc, Mater Salutis Hospital Legnago, Italy
| | - M. Frisinghelli
- Dept Onc Med, Verona, Italy; Pathology, Verona, Italy; Dept Onc Med, Treviso, Italy; Med Onc, Mater Salutis Hospital Legnago, Italy
| | - F. Merlin
- Dept Onc Med, Verona, Italy; Pathology, Verona, Italy; Dept Onc Med, Treviso, Italy; Med Onc, Mater Salutis Hospital Legnago, Italy
| | - M. A. Bassetto
- Dept Onc Med, Verona, Italy; Pathology, Verona, Italy; Dept Onc Med, Treviso, Italy; Med Onc, Mater Salutis Hospital Legnago, Italy
| | - T. Franceschi
- Dept Onc Med, Verona, Italy; Pathology, Verona, Italy; Dept Onc Med, Treviso, Italy; Med Onc, Mater Salutis Hospital Legnago, Italy
| | - C. Sava
- Dept Onc Med, Verona, Italy; Pathology, Verona, Italy; Dept Onc Med, Treviso, Italy; Med Onc, Mater Salutis Hospital Legnago, Italy
| | - G. L. Cetto
- Dept Onc Med, Verona, Italy; Pathology, Verona, Italy; Dept Onc Med, Treviso, Italy; Med Onc, Mater Salutis Hospital Legnago, Italy
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Merlin F, Sava T, Porcaro AB, Ghimenton C, Frisinghelli M, Manno P, Griso C, Bassetto MA, Comunale L, Cetto GL. Transitional cell carcinomas of the upper urothelial tract: A retrospective analysis. J Clin Oncol 2004. [DOI: 10.1200/jco.2004.22.90140.4740] [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: 11/20/2022] Open
Affiliation(s)
- F. Merlin
- University of Verona, Verona, Italy; Unità Operativa di Urologia, Verona, Italy; Pathology, Verona, Italy
| | - T. Sava
- University of Verona, Verona, Italy; Unità Operativa di Urologia, Verona, Italy; Pathology, Verona, Italy
| | - A. B. Porcaro
- University of Verona, Verona, Italy; Unità Operativa di Urologia, Verona, Italy; Pathology, Verona, Italy
| | - C. Ghimenton
- University of Verona, Verona, Italy; Unità Operativa di Urologia, Verona, Italy; Pathology, Verona, Italy
| | - M. Frisinghelli
- University of Verona, Verona, Italy; Unità Operativa di Urologia, Verona, Italy; Pathology, Verona, Italy
| | - P. Manno
- University of Verona, Verona, Italy; Unità Operativa di Urologia, Verona, Italy; Pathology, Verona, Italy
| | - C. Griso
- University of Verona, Verona, Italy; Unità Operativa di Urologia, Verona, Italy; Pathology, Verona, Italy
| | - M. A. Bassetto
- University of Verona, Verona, Italy; Unità Operativa di Urologia, Verona, Italy; Pathology, Verona, Italy
| | - L. Comunale
- University of Verona, Verona, Italy; Unità Operativa di Urologia, Verona, Italy; Pathology, Verona, Italy
| | - G. L. Cetto
- University of Verona, Verona, Italy; Unità Operativa di Urologia, Verona, Italy; Pathology, Verona, Italy
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Sava T, Pessa S, Nicoletti L, Perin A, Fraccon AP, Merlin F, Rosa-Bian A, Fosser V, Cetto GL, Franceschi T. Nonseminomatous germ cell testicular tumors clinical stage II: Retroperitoneal lymph node dissection, chemotherapy or both? J Clin Oncol 2004. [DOI: 10.1200/jco.2004.22.90140.4746] [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: 11/20/2022] Open
Affiliation(s)
- T. Sava
- University of Verona, Verona, Italy; Ospedale Civile, Treviso, Italy; Ospedale Civile, Vicenza, Italy; Ospedale Civile, Thiene, Italy; Mater Salutis, Legnago Verona, Italy
| | - S. Pessa
- University of Verona, Verona, Italy; Ospedale Civile, Treviso, Italy; Ospedale Civile, Vicenza, Italy; Ospedale Civile, Thiene, Italy; Mater Salutis, Legnago Verona, Italy
| | - L. Nicoletti
- University of Verona, Verona, Italy; Ospedale Civile, Treviso, Italy; Ospedale Civile, Vicenza, Italy; Ospedale Civile, Thiene, Italy; Mater Salutis, Legnago Verona, Italy
| | - A. Perin
- University of Verona, Verona, Italy; Ospedale Civile, Treviso, Italy; Ospedale Civile, Vicenza, Italy; Ospedale Civile, Thiene, Italy; Mater Salutis, Legnago Verona, Italy
| | - A. P. Fraccon
- University of Verona, Verona, Italy; Ospedale Civile, Treviso, Italy; Ospedale Civile, Vicenza, Italy; Ospedale Civile, Thiene, Italy; Mater Salutis, Legnago Verona, Italy
| | - F. Merlin
- University of Verona, Verona, Italy; Ospedale Civile, Treviso, Italy; Ospedale Civile, Vicenza, Italy; Ospedale Civile, Thiene, Italy; Mater Salutis, Legnago Verona, Italy
| | - A. Rosa-Bian
- University of Verona, Verona, Italy; Ospedale Civile, Treviso, Italy; Ospedale Civile, Vicenza, Italy; Ospedale Civile, Thiene, Italy; Mater Salutis, Legnago Verona, Italy
| | - V. Fosser
- University of Verona, Verona, Italy; Ospedale Civile, Treviso, Italy; Ospedale Civile, Vicenza, Italy; Ospedale Civile, Thiene, Italy; Mater Salutis, Legnago Verona, Italy
| | - G. L. Cetto
- University of Verona, Verona, Italy; Ospedale Civile, Treviso, Italy; Ospedale Civile, Vicenza, Italy; Ospedale Civile, Thiene, Italy; Mater Salutis, Legnago Verona, Italy
| | - T. Franceschi
- University of Verona, Verona, Italy; Ospedale Civile, Treviso, Italy; Ospedale Civile, Vicenza, Italy; Ospedale Civile, Thiene, Italy; Mater Salutis, Legnago Verona, Italy
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Pegoraro C, Savio A, Beghelli S, Scarpa A, Zamboni G, Tomba A, Sabbioni R, Merlin F, Cetto GL, Pasini F. Long-term follow-up in low-grade gastric MALT lymphoma (LGGML): Effect of persistent monoclonality (m+) on outcome. J Clin Oncol 2004. [DOI: 10.1200/jco.2004.22.90140.6560] [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: 11/20/2022] Open
Affiliation(s)
- C. Pegoraro
- University of Verona, Medical Oncology, Verona, Italy; Ospedale S. Orsola, Department of Pathology, Brescia, Italy; University of Verona, Department of Pathology, Verona, Italy; Ospedale di Negrar, Gastroenterology Unit, Verona, Italy
| | - A. Savio
- University of Verona, Medical Oncology, Verona, Italy; Ospedale S. Orsola, Department of Pathology, Brescia, Italy; University of Verona, Department of Pathology, Verona, Italy; Ospedale di Negrar, Gastroenterology Unit, Verona, Italy
| | - S. Beghelli
- University of Verona, Medical Oncology, Verona, Italy; Ospedale S. Orsola, Department of Pathology, Brescia, Italy; University of Verona, Department of Pathology, Verona, Italy; Ospedale di Negrar, Gastroenterology Unit, Verona, Italy
| | - A. Scarpa
- University of Verona, Medical Oncology, Verona, Italy; Ospedale S. Orsola, Department of Pathology, Brescia, Italy; University of Verona, Department of Pathology, Verona, Italy; Ospedale di Negrar, Gastroenterology Unit, Verona, Italy
| | - G. Zamboni
- University of Verona, Medical Oncology, Verona, Italy; Ospedale S. Orsola, Department of Pathology, Brescia, Italy; University of Verona, Department of Pathology, Verona, Italy; Ospedale di Negrar, Gastroenterology Unit, Verona, Italy
| | - A. Tomba
- University of Verona, Medical Oncology, Verona, Italy; Ospedale S. Orsola, Department of Pathology, Brescia, Italy; University of Verona, Department of Pathology, Verona, Italy; Ospedale di Negrar, Gastroenterology Unit, Verona, Italy
| | - R. Sabbioni
- University of Verona, Medical Oncology, Verona, Italy; Ospedale S. Orsola, Department of Pathology, Brescia, Italy; University of Verona, Department of Pathology, Verona, Italy; Ospedale di Negrar, Gastroenterology Unit, Verona, Italy
| | - F. Merlin
- University of Verona, Medical Oncology, Verona, Italy; Ospedale S. Orsola, Department of Pathology, Brescia, Italy; University of Verona, Department of Pathology, Verona, Italy; Ospedale di Negrar, Gastroenterology Unit, Verona, Italy
| | - G. L. Cetto
- University of Verona, Medical Oncology, Verona, Italy; Ospedale S. Orsola, Department of Pathology, Brescia, Italy; University of Verona, Department of Pathology, Verona, Italy; Ospedale di Negrar, Gastroenterology Unit, Verona, Italy
| | - F. Pasini
- University of Verona, Medical Oncology, Verona, Italy; Ospedale S. Orsola, Department of Pathology, Brescia, Italy; University of Verona, Department of Pathology, Verona, Italy; Ospedale di Negrar, Gastroenterology Unit, Verona, Italy
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Litta P, Pozzan C, Sacco G, Merlin F, Saccardi C, Ambrosini A. Adenosarcoma of the ovary. A case report. EUR J GYNAECOL ONCOL 2004; 25:507-8. [PMID: 15285316] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 04/30/2023]
Abstract
Adenosarcoma of the ovary is a rare condition. We report a case of a 32-year-old patient that has been treated in our Department. The diagnosis of ovarian adenosarcoma was carried out after laparoscopy with removal of an ovarian endometriotic cyst. Laparoscopic homolateral ovariectomy was then performed and conservative treatment was decided on considering the young age, low stage and low grade of the disease. Second-look laparoscopy, clinical evaluation and ultrasound were performed for four years of follow-up. No recurrence has been detected. Conservative treatment should be proposed in fertile age with low-grade ovarian adenosarcoma, but a strict follow-up is always necessary.
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Affiliation(s)
- P Litta
- Department of Gynecological Sciences and Human Reproduction, University of Padova, Italy
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16
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Le Floch S, Guyomarch J, Merlin F, Børseth JF, Le Corre P, Lee K. Effects of oil and bioremediation on mussel (Mytilus edulis L.) growth in mudflats. Environ Technol 2003; 24:1211-1219. [PMID: 14669801 DOI: 10.1080/09593330309385663] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/24/2023]
Abstract
Mussels (Mytilus edulis L.) were exposed to crude oil during a field experiment to evaluate two bioremediation strategies (nutrient addition and nutrient addition with tilling). The mussels were placed in 4 mesocosms: Control, Oil, Oil + Nutrients, and Oil + Nutrients + Tilled. Tilling appeared to be clearly detrimental to mussel growth. Additionally, this field experiment demonstrated that at temperatures below 5 degrees C, growth was reduced to rates undetectable by the laser diffraction method. The data on mussel shell length show that this technique does offer very sensitive and useful comparative measurements of physiological function. Measurement of shell growth has the advantage over other techniques in that it is non-invasive and non-destructive and thus may be used continuously without disturbing critical physiological and biochemical functions; however, bivalve physiology is strongly linked to environmental conditions, so it is important to include such measures (i.e. seawater temperature and turbidity) in the design of the biomonitoring program. Elevated polycyclic aromatic hydrocarbon (PAH) levels reflected bioaccumulation in mussels from all the oiled mesocosms. This correlated with reduction in growth rate. Maximum reduction in growth was observed in mussels from the tilled mesocosm which contained the lowest phenanthrene and dibenzothiophene concentrations. The tilling caused an increase in suspended solids which inhibited filter feeding activity, and resulted in suppressed growth and slower intake of PAH-laden sediment.
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Affiliation(s)
- S Le Floch
- Centre de Documentation de Recherche et d'Expérimentations sur les pollutions accidentelles des eaux, Rue Alain Colas, B.P. 20413, 29604 Brest cedex, France
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17
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Litta P, Fracas M, Pozzan C, Merlin F, Saccardi C, Sacco G, Mannici D. Laparoscopic management of early stage endometrial cancer. EUR J GYNAECOL ONCOL 2003; 24:41-4. [PMID: 12691315] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 03/01/2023]
Abstract
PURPOSE OF INVESTIGATION The purpose of this study was to evaluate the feasibility of laparoscopic hysterectomy versus the transabdominal approach with systemic pelvic lymphadenectomy in early stage endometrial cancer. METHODS From January 1996 to April 2002, 59 women were treated for endometrial cancer at the Department of Gynecology in Padova, Italy (29 by the laparoscopic technique and 30 by laparotomy). Every patient underwent hysterosalpingo-oophorectomy with systemic pelvic lymphadenectomy. RESULTS Comparing the two techniques, operating time was longer and hospital stay was significantly shorter for laparoscopy; no differences were observed about the number of removed lymph nodes (range 5-33) or intra-postoperatory complications. CONCLUSION The laparoscopic approach to endometrial cancer is certainly to be considered appropriate and efficacious, even if it requires skilled surgeons and adequate oncologic training. It is important to perform pelvic lymphadenectomy in all cases of early stage cancer.
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Affiliation(s)
- P Litta
- Department of Gynaecology & Obstetrics, University of Padova, Italy
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18
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Zouali H, Lesage S, Merlin F, Cézard JP, Colombel JF, Belaiche J, Almer S, Tysk C, O'Morain C, Gassull M, Christensen S, Finkel Y, Modigliani R, Gower-Rousseau C, Macry J, Chamaillard M, Thomas G, Hugot JP. CARD4/NOD1 is not involved in inflammatory bowel disease. Gut 2003; 52:71-4. [PMID: 12477763 PMCID: PMC1773516 DOI: 10.1136/gut.52.1.71] [Citation(s) in RCA: 53] [Impact Index Per Article: 2.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 02/07/2023]
Abstract
BACKGROUND AND AIMS Inflammatory bowel diseases (IBD), including Crohn's disease (CD) and ulcerative colitis (UC), are complex genetic disorders. CARD15/NOD2, a member of the Ced4 superfamily which includes Apaf-1 and CARD4/NOD1, has recently been associated with genetic predisposition to CD but additional genetic factors remain to be identified. Because CARD4/NOD1 shares many structural and functional similarities with CARD15, we tested its putative role in IBD. PATIENTS AND METHODS The 11 exons of CARD4 were screened for the presence of variants in 63 unrelated IBD patients. The only non-private genetic variation encoding for a substitution in the peptidic chain was genotyped in 381 IBD families (235 CD, 58 UC, 81 mixed, and seven indeterminate colitis families) using a polymerase chain reaction-restriction fragment length polymorphism procedure. Genotyping data were analysed by the transmission disequilibrium test. RESULTS Five of nine sequence variations identified in the coding sequence of the gene encoded for non-conservative changes (E266K, D372N, R705Q, T787M, and T787K). Four were present in only one family. The remaining variant (E266K), which exhibited an allele frequency of 0.28, was not associated with CD, UC, or IBD. Furthermore, IBD patients carrying sequence variations in their CARD4 gene had a similar phenotype to those with a normal sequence. CONCLUSION Our results suggest that CARD4 does not play a major role in genetic susceptibility to IBD.
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Affiliation(s)
- H Zouali
- Fondation Jean Dausset-CEPH, Paris, France
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19
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Torrisi A, Del Mistro A, Onnis GL, Merlin F, Bertorelle R, Minucci D. Colposcopy, cytology and HPV-DNA testing in HIV-positive and HIV-negative women. EUR J GYNAECOL ONCOL 2000; 21:168-72. [PMID: 10843478] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/16/2023]
Abstract
In this study we examined the incidence of colposcopic-colpocytologic findings and analyzed Human Papilloma Virus (HPV)-DNA testing by Polymerase Chain Reaction (PCR) in 104 Human Immunodeficiency Virus (HIV) serous positive women (Group 1) and 218 HIV-negative women (control Groups 2 and 3). The aim of the study was to evaluate the most appropriate and efficacious diagnostic methods for screening programs for cervical cancer in HIV-positive women. For Group 1 we also considered the value of CD4+ T-lymphocytes and morphologic and molecular follow-up from 3 to 6 months. The results showed that the abnormal transformation zone (ANTZ) was present in 66.3% of the cases in Group 1 compared with 31.4% in control-Group 2 (p<0.001), and with 58.93% of the cases in control-Group 3 (p=0.257); intraepithelial squamous lesions (SIL) were found in 50% vs 5.66% (p<0.001) and vs 56.25% of the cases (p=0.433), respectively. In 28.85% of the HIV-positive patients the first cytological screening exam was not evaluable due to inflammation but in 56.67% of the cases colposcopy revealed ANTZ. The subsequent colpocytological checkup after therapy showed 10 cases (30%) of low risk squamous intraepithelial lesions (LSIL) and two cases (6.6%) of high risk squamous intraepithelial lesions (HSIL). HPV-DNA testing by PCR was positive in 53.8% of the cases in Group 1, in 6.6% in control-Group 2 and in 42% in control-Group 3. In HIV-positive patients multiple HPV genotypes were simultaneously present in 21.43% of the cases and high risk genotypes were present in 70% of the cases of HSIL. In Group 1, 36.61% of the cases had lesions of the lower genital tract. The value of CD4+ T-lympocytes was <200 cells/ml in 30% of the cases of HSIL. Our data, like those of other Authors, confirm a high incidence of HSIL, abnormal colposcopic findings, and HPV infections in HIV-positive women with respect to control-Group 2, while there was not much difference between Group 1 and control-Group 3. Such frequency again suggests that an integrated morphological diagnostic approach with colposcopy-colpocytology in the screening of immunosuppressed subjects would be worthwhile.
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Affiliation(s)
- A Torrisi
- Institute of Gynaecology and Obstetrics, University of Padua, Italy
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20
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Le Paslier MC, Pierce RJ, Merlin F, Hirai H, Wu W, Williams DL, Johnston D, LoVerde PT, Le Paslier D. Construction and characterization of a Schistosoma mansoni bacterial artificial chromosome library. Genomics 2000; 65:87-94. [PMID: 10783255 DOI: 10.1006/geno.2000.6147] [Citation(s) in RCA: 47] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/13/2022]
Abstract
A bacterial artificial chromosome (BAC) library has been established from genomic DNA isolated from the trematode parasite of human, Schistosoma mansoni. This library consists of more than 21,000 recombinant clones carrying inserts in the pBeloBAC11 vector. The mean insert size was 100 kb, representing an approximate 7.95-fold genome coverage. Library screening with eight chromosome-specific or single-copy gene probes yielded between 1 and 9 positive clones, and none of those tested was absent from the library. End sequences were obtained for 93 randomly selected clones, and 37 showed sequence identity to S. mansoni sequences (ESTs, genes, or repetitive sequences). A preliminary analysis by fluorescence in situ hybridization localized 8 clones on schistosome chromosomes 1 (2 clones), 2, 3, 5, Z, and W (3 clones). This library provides a new resource for the physical mapping and sequencing of the genome of this important human pathogen.
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21
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Bolla M, Seigneurin D, Winckel P, Marron-Charrière J, Panh MH, Pasquier D, Chédin M, Payan R, Merlin F, Venditti V. [Prognostic value of quantitative DNA analysis, expressed in integrated optical density, in a series of 415 T1-T2, N0N1, M0 UICC breast cancers]. Bull Cancer 1996; 83:687-92. [PMID: 8952641] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/03/2023]
Abstract
From June 1982 to December 1992, 415 patients less than 75 years of age, without any previous or synchronous carcinoma, suffering from an invasive breast cancer classified as T1 (52.8%), T2 (47.2%), NO (65.1%) N1(34.9%), MO according to clinical TNM staging, were enrolled in this study. The median age was 53 (28-75), and 58.8% of the patients were menopaused; 85.3% underwent a breast conservative procedure and 14.7% a modified radical mastectomy followed by postoperative irradiation. Histological axillary lymph node status, Scarff-Bloom grade and/or cytological grade, estradiol receptor content, were used to set up medical adjuvant treatment: hormonotherapy (52%) or chemotherapy (18.8%). Imprints were taken from the macroscopically visible lesion at the time of surgery, and a Feulgen staining was done on air dried smears to be analyzed using the Samba 200 cell image processor (Alcatel TITN, France). Five parameters were systematically assessed: proliferation index, DNA histogram, integrated optical density, DNA malignancy grade, and policy balance. With a median follow-up of 36 months (0-105), proliferation index (P = 0.0008), DNA histogram (P = 0.0017), integrated optical density (P = 0.018), DNA malignancy grade (P = 0.017) have a significant prognostic value on disease free survival estimated by the Kaplan-Meir method. When these parameters were included in a Cox proportional regression hazards model, Scarff-Bloom histological grading (P = 0.002), positives nodes (P = 0.02), optical integrated density (P = 0.045) were significant. Such results need to be updated with a longer follow-up, but they suggest that the mean DNA content, as measured by the integrated optical density (IOD), has to be considered when deciding on medical adjuvant treatment with respect to patients with a negative axillary clearance.
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Affiliation(s)
- M Bolla
- Service de cancérologie-radiothérapie, CHU, Grenoble, France
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22
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Bolla M, Seigneurin D, Winckel P, Marron-Charrière J, Panh MH, Pasquier D, Ch-edin M, Payan R, Merlin F, Colonna M. Prognostic value of quantitative cytometry in a series of 415 T1T2/N0N1/M0 breast cancer patients--preliminary results. Eur J Cancer 1996; 32A:1680-5. [PMID: 8983274 DOI: 10.1016/0959-8049(96)00174-8] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [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: 02/03/2023]
Abstract
Identifying prognostic markers in local regional breast carcinomas remains an important challenge today. DNA content obtained by flow cytometry, has been found to be of prognostic value; results with other methods remain less clear. This report describes DNA image cytometry patterns which are assessed with respect to disease-free survival. From June 1982 to December 1992, 415 patients under 75 years of age, without any previous or synchronous carcinoma, suffering from an invasive breast cancer classified as T1 (52.8%), T2 (47.2%), N0 (65.1%) N1 (34.9%), MO according to clinical TNM staging, were enrolled in this study. The median age was 53 (28-75) and 58.8% of the patients were premenopausal; 85.3% underwent a breast conservative procedure and 14.7% a modified radical mastectomy followed by postoperative irradiation. Histological axillary lymph node status, Scarff-Bloom grade and/or cytological grade and, oestrogen receptor content were used in decision-making for adjuvant treatment: hormonotherapy (48%) or chemotherapy (18.8%). Imprints were taken from the macroscopically visible lesion at the time of surgery, and a Feulgen staining was carried out on air dried smears to be analysed using the Samba 200 cell image processor (Alcatel TITN, France). Five parameters were systematically assessed: proliferation index; DNA histogram, integrated optical density, DNA malignancy grade, ploidy balance. With a median follow-up of 36 months (0-105), proliferation index (P = 0.0008), DNA histogram (P = 0.0017), integrated optical density (IOD) (P = 0.018) and DNA malignancy grade (P = 0.017) had a significant prognostic value on disease-free survival estimated by the Kaplan-Meier method. When these parameters were included in a Cox proportional regression hazards model, PR (P = 0.01), Scarff-Bloom histological grading (P = 0.02), axillary clearance (P = 0.04) were significant; however, in the same model, taking into account the axillary lymph node histological status, IOD was significant for pN- patients (P = 0.03), and proliferation index (P = 0.03) was significant for pN+. Such results need to be updated with a longer median follow-up, but they suggest that the mean DNA content, as measured by the integrated optical density (IOD), should be considered when deciding on medical adjuvant treatment with respect to patients with a negative axillary clearance.
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Affiliation(s)
- M Bolla
- Department of Radiotherapy, CHU de Grenoble, France
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23
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Levasseur S, Husson MO, Leitz R, Merlin F, Laurent F, Peladan F, Drocourt JL, Leclerc H, Van Hoegaerden M. Rapid detection of members of the family Enterobacteriaceae by a monoclonal antibody. Appl Environ Microbiol 1992; 58:1524-9. [PMID: 1622220 PMCID: PMC195635 DOI: 10.1128/aem.58.5.1524-1529.1992] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.2] [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: 12/27/2022] Open
Abstract
Six monoclonal antibodies directed against enterobacteria were produced and characterized. The specificity of one of these antibodies (CX9/15; immunoglobulin G2a) was studied by indirect immunofluorescence against 259 enterobacterial strains and 125 other gram-negative bacteria. All of the enterobacteria were specifically recognized, the only exception being Erwinia chrysanthemi (one strain tested). Bacteria not belonging to members of the family Enterobacteriaceae were not detected, except for Plesiomonas shigelloides (two strains tested), Aeromonas hydrophila (five strains tested), and Aeromonas sobria (one strain tested). This recognition spectrum strongly suggested that CX9/15 recognized the enterobacterial common antigen. By sodium dodecyl sulfate-polyacrylamide gel electrophoresis and Western blot (immunoblot) experiments, the six antienterobacteria antibodies presented similar specificities; they all revealed only one band with an apparent molecular weight of about 20,000 from the crude extract of an enterobacterium. The six monoclonal antibodies, and especially CX9/15, can be used to develop new tests for rapid and specific detection of enterobacteria.
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24
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Julier C, Hyer RN, Davies J, Merlin F, Soularue P, Briant L, Cathelineau G, Deschamps I, Rotter JI, Froguel P. Insulin-IGF2 region on chromosome 11p encodes a gene implicated in HLA-DR4-dependent diabetes susceptibility. Nature 1991; 354:155-9. [PMID: 1944595 DOI: 10.1038/354155a0] [Citation(s) in RCA: 266] [Impact Index Per Article: 8.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/29/2022]
Abstract
A class of alleles at the VNTR (variable number of tandem repeat) locus in the 5' region of the insulin gene (INS) on chromosome 11p is associated with increased risk of insulin-dependent diabetes mellitus (IDDM), but family studies have failed to demonstrate linkage. INS is thought to contribute to IDDM susceptibility but this view has been difficult to reconcile with the lack of linkage evidence. We thus investigated polymorphisms of INS and neighbouring loci in random diabetics, IDDM multiplex families and controls. HLA-DR4-positive diabetics showed an increased risk associated with common variants at polymorphic sites in a 19-kilobase segment spanned by the 5' INS VNTR and the third intron of the gene for insulin-like growth factor II (IGF2). As INS is the major candidate gene from this region, diabetic and control sequence were compared to identify all INS polymorphisms that could contribute to disease susceptibility. In multiplex families the IDDM-associated alleles were transmitted preferentially to HLA-DR4-positive diabetic offspring from heterozygous parents. The effect was strongest in paternal meioses, suggesting a possible role for maternal imprinting. Our results strongly support the existence of a gene or genes affecting HLA-DR4 IDDM susceptibility which is located in a 19-kilobase region of INS-IGF2. Our results also suggest new ways to map susceptibility loci in other common diseases.
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Affiliation(s)
- C Julier
- Centre d'Etude du Polymorphisme Humain, Paris, France
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25
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Lecommandeur D, Merlin F, Daussant J, Van Hoegaerden M. Monoclonal antibodies to barley alpha-amylase I: production, characterization, and application to a specific immunoassay. Hybridoma (Larchmt) 1990; 9:177-87. [PMID: 1693360 DOI: 10.1089/hyb.1990.9.177] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/28/2022]
Abstract
Monoclonal antibodies (MAbs) to barley alpha-amylase I have been produced, purified and characterized. Six are specific for the alpha-amylase I isoform, while one also reacts with alpha-amylase II. All but one recognize the antigen in solution. Topology of the MAbs was investigated by additivity in ELISA, which led us to subdivide them into four groups. An immunoassay was developed using one of these MAbs, to measure alpha-amylase I activity in an extract containing both isoforms.
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Affiliation(s)
- D Lecommandeur
- Laboratoire de Physiologie des Organes Végétaux, C.N.R.S., Meudon, France
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26
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Feinfeld DA, Verger C, Briscoe AM, Hotchkiss JL, Nurse HM, Merlin F, Nair S, Hart PM. Serum myoglobin in patients on intermittent and continuous ambulatory peritoneal dialysis. Clin Nephrol 1987; 28:144-6. [PMID: 3665208] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/06/2023] Open
Abstract
Serum myoglobin levels were determined in patients maintained on chronic peritoneal dialysis. Eleven intermittent peritoneal dialysis patients had a mean serum myoglobin of 174 +/- 29 ng/ml. In 7 patients tested serially, there was no consistent change in serum myoglobin: the mean level was 154 +/- 36 ng/ml pre-dialysis and 170 +/- 20 ng/ml post-dialysis. Seventeen patients on continuous ambulatory peritoneal dialysis had a mean serum myoglobin of 215 +/- 18 ng/ml. Two patients given oral carnitine supplements had a substantial decrease in their serum myoglobin levels. Patients on peritoneal dialysis, like those on hemodialysis, tend to have elevated serum myoglobin levels, and neither form of dialysis affects serum myoglobin concentration. This hypermyoglobinemia may be due to metabolic changes in muscle.
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Affiliation(s)
- D A Feinfeld
- Department of Medicine, Harlem Hospital Center, Columbia University College of Physicians & Surgeons, New York, NY
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27
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Lee HH, Merlin F, Germain C, Canavaggio M. [Production of anti-A, anti-B and anti-A+B monoclonal antibodies for blood grouping]. Rev Fr Transfus Immunohematol 1985; 28:613-24. [PMID: 4095438 DOI: 10.1016/s0338-4535(85)80006-4] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 01/08/2023]
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28
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Kornecki E, Lee H, Merlin F, Hershock D, Tuszynski GP, Niewiarowski S. Comparison of platelet fibrinogen receptors on intact and proteolytically-treated platelets by use of an anti-glycoprotein IIIa monoclonal antibody (MA 123). Thromb Res 1984; 34:35-49. [PMID: 6328693 DOI: 10.1016/0049-3848(84)90104-x] [Citation(s) in RCA: 13] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/19/2023]
Abstract
A murine monoclonal antibody (MA 123) was selected by screening 153 supernatants of hybridoma cells secreting anti-human platelet antibodies for their ability to inhibit the fibrinogen-induced aggregation of chymotrypsin-treated platelets. MA 123 inhibited the binding of 125I-fibrinogen to ADP-stimulated intact human platelets and to platelets treated with chymotrypsin or pronase. Moreover, it inhibited the fibrinogen-induced aggregation of these platelet suspensions. The degree of inhibition was similar in each of the three types of platelets tested. The interactions of MA 123 with the 125I-labeled surface components of intact and chymotrypsin-treated platelets were studied by immunoprecipitation using Staphylococcus aureus coated with goat anti-mouse IgG, followed by SDS-polyacrylamide gel electrophoresis and autoradiography. MA 123 precipitated the glycoprotein IIb-glycoprotein IIIa (GPIIb-GPIIIa) complex from the surface of detergent solubilized intact human platelets; and it precipitated GPIIIa from the surface of chymotrypsin-treated platelets. Partially purified GPIIIa was also immunoprecipitated by MA 123. Our data suggest that the exposure of fibrinogen receptors by ADP, chymotrypsin or pronase, is associated with alterations of GPIIIa on the platelet surface.
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