2
|
Ishihara S, Kuribayashi S, Sato K, Kudo T, Yamazaki S, Inoue T, Hazama Y, Furuya K, Nakayama T, Hachisu Y, Marubashi K, Uraoka T. A Marked Eosinophilic Infiltration in Mucosa Could Be a Better Predictive Factor for Intractable Non-Esophageal Eosinophilic Gastrointestinal Disorders. Digestion 2023; 104:348-356. [PMID: 37088071 DOI: 10.1159/000528845] [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] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 05/03/2022] [Accepted: 12/19/2022] [Indexed: 04/25/2023]
Abstract
INTRODUCTION Non-esophageal eosinophilic gastrointestinal disorders (non-EoE EGIDs) are rare, but their prevalence has recently increased. Although it has been reported that one-half of patients with non-EoE EGIDs have intractable clinical courses, their clinical features are not fully understood. METHODS This is a multicenter retrospective study in which 10 institutions in Japan participated. Clinical databases from January 1998 to December 2020 were reviewed to identify patients with non-EoE EGIDs. A total of 44 patients were identified; they were divided into two groups based on their clinical course: an intractable group and a non-intractable group. The clinical features were compared between the two groups by a logistic regression analysis. Remarkable eosinophilic infiltration (REI) was defined histologically when the maximal counts of mucosal eosinophils reached a threshold level in the respective area of biopsy. RESULTS Prevalence of drug allergy and eosinophil counts more than 500/μL (EOS), vomiting symptoms, abnormalities of the stomach, duodenum, and jejunum on computed tomography (upper gastrointestinal abnormality on computed tomography [UACT]), and REI were significantly different between the two groups. Among the factors that were potentially associated with an intractable clinical course, logistic regression revealed that REI, EOS, and UACT were significant factors. Based on an analysis of the area under the receiver operator characteristic curve, a combination of REI and EOS had the lowest Akaike's information criterion, indicating the best model to predict an intractable clinical course. CONCLUSIONS REI may predict an intractable course in patients with non-EoE EGIDs. In addition, the combination of REI and EOS was a better predictor than REI alone.
Collapse
Affiliation(s)
- Shingo Ishihara
- Department of Internal Medicine, Isesaki Municipal Hospital, Isesaki, Japan
| | - Shiko Kuribayashi
- Department of Gastroenterology and Hepatology, Gunma University Graduate School of Medicine, Maebashi, Japan
| | - Keigo Sato
- Department of Gastroenterology and Hepatology, Gunma University Graduate School of Medicine, Maebashi, Japan
| | - Tomohiro Kudo
- Department of Gastroenterology, National Hospital Organization Takasaki Medical Center, Takasaki, Japan
| | - Setsuo Yamazaki
- Department of Gastroenterology, Maebashi Red-Cross Hospital, Maebashi, Japan
| | - Teruki Inoue
- Department of Gastroenterology, Kiryu Welfare Hospital, Kiryu, Japan
| | - Yoichi Hazama
- Department of Internal Medicine, National Hospital Organization Numata National Hospital, Numata, Japan
| | - Kensuke Furuya
- Department of Gastroenterology, National Hospital Organization Shibukawa Medical Center, Shibukawa, Japan
| | - Tetsuo Nakayama
- Department of Internal Medicine, Toho Hospital, Midori, Japan
| | - Yoko Hachisu
- Department of Gastroenterology, Saiseikai Maebashi Hospital, Maebashi, Japan
| | - Kyoko Marubashi
- Department of Gastroenterology, Kusunoki Hospital, Fujioka, Japan
| | - Toshio Uraoka
- Department of Gastroenterology and Hepatology, Gunma University Graduate School of Medicine, Maebashi, Japan
| |
Collapse
|
5
|
Adams JH, Ahmad S, Allard D, Anzalone A, Bacholle S, Barrillon P, Bayer J, Bertaina M, Bisconti F, Blaksley C, Blin-Bondil S, Bobík P, Cafagna F, Campana D, Capel F, Casolino M, Cassardo C, Catalano C, Cremonini R, Dagoret-Campagne S, Danto P, del Peral L, de la Taille C, Díaz Damian A, Dupieux M, Ebersoldt A, Ebisuzaki T, Eser J, Evrard J, Fenu F, Ferrarese S, Fornaro C, Fouka M, Gorodetzky P, Guarino F, Guzman A, Hachisu Y, Haungs A, Judd E, Jung A, Karczmarczyk J, Kawasaki Y, Klimov PA, Kuznetsov E, Mackovjak S, Manfrin M, Marcelli L, Medina-Tanco G, Mercier K, Merino A, Mernik T, Miyamoto H, Morales de los Ríos JA, Moretto C, Mot B, Neronov A, Ohmori H, Olinto AV, Osteria G, Panico B, Parizot E, Paul T, Picozza P, Piotrowski LW, Plebaniak Z, Pliego S, Prat P, Prévôt G, Prieto H, Putis M, Rabanal J, Ricci M, Rojas J, Rodríguez Frías MD, Roudil G, Sáez Cano G, Sahnoun Z, Sakaki N, Sanchez JC, Santangelo A, Sarazin F, Scotti V, Shinozaki K, Silva H, Soriano JF, Suino G, Szabelski J, Toscano S, Tabone I, Takizawa Y, von Ballmoos P, Wiencke L, Wille M, Zotov M. A Review of the EUSO-Balloon Pathfinder for the JEM-EUSO Program. Space Sci Rev 2022; 218:3. [PMID: 35153338 PMCID: PMC8807436 DOI: 10.1007/s11214-022-00870-x] [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] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 03/24/2021] [Accepted: 12/31/2021] [Indexed: 06/14/2023]
Abstract
EUSO-Balloon is a pathfinder for JEM-EUSO, the mission concept of a spaceborne observatory which is designed to observe Ultra-High Energy Cosmic Ray (UHECR)-induced Extensive Air Showers (EAS) by detecting their UltraViolet (UV) light tracks "from above." On August 25, 2014, EUSO-Balloon was launched from Timmins Stratospheric Balloon Base (Ontario, Canada) by the balloon division of the French Space Agency CNES. After reaching a floating altitude of 38 km, EUSO-Balloon imaged the UV light in the wavelength range ∼290-500 nm for more than 5 hours using the key technologies of JEM-EUSO. The flight allowed a good understanding of the performance of the detector to be developed, giving insights into possible improvements to be applied to future missions. A detailed measurement of the photoelectron counts in different atmospheric and ground conditions was achieved. By means of the simulation of the instrument response and by assuming atmospheric models, the absolute intensity of diffuse light was estimated. The instrument detected hundreds of laser tracks with similar characteristics to EASs shot by a helicopter flying underneath. These are the first recorded laser tracks measured from a fluorescence detector looking down on the atmosphere. The reconstruction of the direction of the laser tracks was performed. In this work, a review of the main results obtained by EUSO-Balloon is presented as well as implications for future space-based observations of UHECRs.
Collapse
Affiliation(s)
- J. H. Adams
- University of Alabama in Huntsville, Huntsville, USA
| | - S. Ahmad
- Omega, Ecole Polytechnique, CNRS/IN2P3, Palaiseau, France
| | - D. Allard
- APC, Univ. Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Paris, France
| | - A. Anzalone
- INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, Palermo, Italy
- Istituto Nazionale di Fisica Nucleare - Sezione di Catania, Catania, Italy
| | - S. Bacholle
- APC, Univ. Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Paris, France
| | - P. Barrillon
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, Orsay, France
| | - J. Bayer
- Institute for Astronomy and Astrophysics, University of Tübingen, Tübingen, Germany
| | - M. Bertaina
- Istituto Nazionale di Fisica Nucleare - Sezione di Torino, Torino, Italy
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
| | - F. Bisconti
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
- Karlsruhe Institute of Technology, Karlsruhe, Germany
| | - C. Blaksley
- APC, Univ. Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Paris, France
| | - S. Blin-Bondil
- Omega, Ecole Polytechnique, CNRS/IN2P3, Palaiseau, France
| | - P. Bobík
- Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia
| | - F. Cafagna
- Istituto Nazionale di Fisica Nucleare - Sezione di Bari, Bari, Italy
| | - D. Campana
- Istituto Nazionale di Fisica Nucleare - Sezione di Napoli, Naples, Italy
| | - F. Capel
- KTH Royal Institute of Technology, Stockholm, Sweden
| | - M. Casolino
- RIKEN, 2-1 Hirosawa, Wako, Saitama Japan
- Istituto Nazionale di Fisica Nucleare - Sezione di Roma Tor Vergata, Roma, Italy
| | - C. Cassardo
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
| | - C. Catalano
- IRAP, Université de Toulouse, CNRS, Toulouse, France
| | - R. Cremonini
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
| | | | - P. Danto
- CNES, 18 avenue Edouard Belin, Toulouse, France
| | | | | | | | - M. Dupieux
- IRAP, Université de Toulouse, CNRS, Toulouse, France
| | - A. Ebersoldt
- Karlsruhe Institute of Technology, Karlsruhe, Germany
| | | | - J. Eser
- Colorado School of Mines, Golden, USA
| | - J. Evrard
- CNES, 18 avenue Edouard Belin, Toulouse, France
| | - F. Fenu
- Istituto Nazionale di Fisica Nucleare - Sezione di Torino, Torino, Italy
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
| | - S. Ferrarese
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
| | | | - M. Fouka
- Center of Research in Astronomy, Astrophysics, and Geophysics, Algiers, Algeria
| | - P. Gorodetzky
- APC, Univ. Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Paris, France
| | - F. Guarino
- Istituto Nazionale di Fisica Nucleare - Sezione di Napoli, Naples, Italy
- Dipartimento di Scienze Fisiche, Universitá di Napoli Federico II, Naples, Italy
| | - A. Guzman
- Institute for Astronomy and Astrophysics, University of Tübingen, Tübingen, Germany
| | - Y. Hachisu
- RIKEN, 2-1 Hirosawa, Wako, Saitama Japan
| | - A. Haungs
- Karlsruhe Institute of Technology, Karlsruhe, Germany
| | - E. Judd
- Space Sciences Laboratory, University of California, Berkeley, CA USA
| | - A. Jung
- APC, Univ. Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Paris, France
| | | | | | - P. A. Klimov
- Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow, Russia
| | - E. Kuznetsov
- University of Alabama in Huntsville, Huntsville, USA
| | - S. Mackovjak
- Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia
| | - M. Manfrin
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
| | - L. Marcelli
- Istituto Nazionale di Fisica Nucleare - Sezione di Roma Tor Vergata, Roma, Italy
| | - G. Medina-Tanco
- Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - K. Mercier
- CNES, 18 avenue Edouard Belin, Toulouse, France
| | | | - T. Mernik
- Institute for Astronomy and Astrophysics, University of Tübingen, Tübingen, Germany
| | - H. Miyamoto
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, Orsay, France
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
| | | | - C. Moretto
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, Orsay, France
| | - B. Mot
- IRAP, Université de Toulouse, CNRS, Toulouse, France
| | - A. Neronov
- ISDC Data Centre for Astrophysics, Versoix, Switzerland
| | - H. Ohmori
- RIKEN, 2-1 Hirosawa, Wako, Saitama Japan
| | | | - G. Osteria
- Istituto Nazionale di Fisica Nucleare - Sezione di Napoli, Naples, Italy
| | - B. Panico
- Istituto Nazionale di Fisica Nucleare - Sezione di Napoli, Naples, Italy
- Dipartimento di Scienze Fisiche, Universitá di Napoli Federico II, Naples, Italy
| | - E. Parizot
- APC, Univ. Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Paris, France
| | - T. Paul
- Lehman College, City University of New York, New York, USA
| | - P. Picozza
- RIKEN, 2-1 Hirosawa, Wako, Saitama Japan
- Istituto Nazionale di Fisica Nucleare - Sezione di Roma Tor Vergata, Roma, Italy
- Dipartimento di Fisica, Universitá di Roma Tor Vergata, Roma, Italy
| | | | - Z. Plebaniak
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
- National Centre for Nuclear Research, Lodz, Poland
| | - S. Pliego
- Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - P. Prat
- APC, Univ. Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Paris, France
| | - G. Prévôt
- APC, Univ. Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Paris, France
| | - H. Prieto
- Universidad de Alcalá, Madrid, Spain
| | - M. Putis
- Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia
| | - J. Rabanal
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, Orsay, France
| | - M. Ricci
- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati, Frascati, Italy
| | - J. Rojas
- Universidad Nacional Autónoma de México, Mexico City, Mexico
| | | | - G. Roudil
- IRAP, Université de Toulouse, CNRS, Toulouse, France
| | | | - Z. Sahnoun
- Center of Research in Astronomy, Astrophysics, and Geophysics, Algiers, Algeria
| | - N. Sakaki
- RIKEN, 2-1 Hirosawa, Wako, Saitama Japan
| | - J. C. Sanchez
- Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A. Santangelo
- Institute for Astronomy and Astrophysics, University of Tübingen, Tübingen, Germany
| | | | - V. Scotti
- Istituto Nazionale di Fisica Nucleare - Sezione di Napoli, Naples, Italy
- Dipartimento di Scienze Fisiche, Universitá di Napoli Federico II, Naples, Italy
| | - K. Shinozaki
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
- National Centre for Nuclear Research, Lodz, Poland
| | - H. Silva
- Universidad Nacional Autónoma de México, Mexico City, Mexico
| | | | - G. Suino
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
| | - J. Szabelski
- National Centre for Nuclear Research, Lodz, Poland
| | - S. Toscano
- ISDC Data Centre for Astrophysics, Versoix, Switzerland
| | - I. Tabone
- Dipartimento di Fisica, Universitá di Torino, Torino, Italy
| | | | | | | | - M. Wille
- ECAP, University of Erlangen-Nuremberg, Erlangen, Germany
| | - M. Zotov
- Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow, Russia
| |
Collapse
|