J 2018

Hitomi (ASTRO-H) X-ray Astronomy Satellite

TAKAHASHI, T.; M. KOKUBUN; K. MITSUDA; RL KELLEY; T. OHASHI et al.

Základní údaje

Originální název

Hitomi (ASTRO-H) X-ray Astronomy Satellite

Autoři

TAKAHASHI, T.; M. KOKUBUN; K. MITSUDA; RL KELLEY; T. OHASHI; F. AHARONIAN; H. AKAMATSU; F. AKIMOTO; S.W. ALLEN; N. ANABUKI; L. ANGELINI; K. ARNAUD; M. ASAI; M. AUDARD; H. AWAKI; M. AXELSSON; P. AZZARELLO; C. BALUTA; A. BAMBA; N. BANDO; MW BAUTZ; T. BIALAS; R. BLANDFORD; K. BOYCE; LW BRENNEMAN; GV BROWN; E. BULBUL; EM CACKETT; E. CANAVAN; M. CHERNYAKOVA; MP CHIAO; PS COPPI; E. COSTANTINI; SO DELL; M. DIPIRRO; C. DONE; T. DOTANI; J. DOTY; K. EBISAWA; ME ECKART; T. ENOTO; Y. EZOE; A.C. FABIAN; C. FERRIGNO; AR FOSTER; R. FUJIMOTO; Y. FUKAZAWA; S. FUNK; A. FURUZAWA; M. GALEAZZI; LC GALLO; P. GANDHI; K. GILMORE; M. GIUSTINI; A. GOLDWURM; Gu LY; M. GUAINAZZI; D. HAAS; Y. HABA; K. HAGINO; K. HAMAGUCHI; IM HARRUS; I. HATSUKADE; T. HAYASHI; K. HAYASHI; K. HAYASHIDA; JW DEN HERDER; JS HIRAGA; K. HIROSE; A. HORNSCHEMEIER; A. HOSHINO; JP HUGHES; Y. ICHINOHE; R. IIZUKA; H. INOUE; Y. INOUE; K. ISHIBASHI; M. ISHIDA; K. ISHIKAWA; K. ISHIMURA; Y. ISHISAKI; M. ITOH; M. IWAI; N. IWATA; N. IYOMOTO; C. JEWELL; J. KAASTRA; T. KALLMAN; T. KAMAE; E. KARA; J. KATAOKA; S. KATSUDA; J. KATSUTA; M. KAWAHARADA; N. KAWAI; T. KAWANO; S. KAWASAKI; D. KHANGULYAN; CA KILBOURNE; M. KIMBALL; A. KING; T. KITAGUCHI; S. KITAMOTO; T. KITAYAMA; T. KOHMURA; S. KONAMI; T. KOSAKA; A. KOUJELEV; K. KOYAMA; S. KOYAMA; P. KRETSCHMAR; HA KRIMM; A. KUBOTA; H. KUNIEDA; P. LAURENT; SH LEE; MA LEUTENEGGER; O. LIMOUSIN; M. LOEWENSTEIN; KS LONG; D. LUMB; G. MADEJSKI; Y. MAEDA; D. MAIER; K. MAKISHIMA; M. MARKEVITCH; C. MASTERS; H. MATSUMOTO; K. MATSUSHITA; D. MCCAMMON; D. MCGUINNESS; BR MCNAMARA; M. MEHDIPOUR; J. MIKO; ED MILLER; JM MILLER; S. MINESHIGE; K. MINESUGI; I. MITSUISHI; T. MIYAZAWA; T. MIZUNO; H. MORI; K. MORI; F. MOROSO; H. MOSELEY; T. MUENCH; K. MUKAI; H. MURAKAMI; T. MURAKAMI; RF MUSHOTZKY; H. NAGANO; R. NAGINO; T. NAKAGAWA; H. NAKAJIMA; T. NAKAMORI; T. NAKANO; S. NAKASHIMA; K. NAKAZAWA; Y. NAMBA; C. NATSUKARI; Y. NISHIOKA; KK NOBUKAWA; M. NOBUKAWA; H. NODA; M. NOMACHI; H. ODAKA; H. OGAWA; M. OGAWA; K. OGI; M. OHNO; M. OHTA; T. OKAJIMA; A. OKAMOTO; T. OKAZAKI; N. OTA; M. OZAKI; F. PAERELS; S. PALTANI; A. PARMAR; R. PETRE; C. PINTO; J. DE PLAA; M. POHL; J. PONTIUS; FS PORTER; K. POTTSCHMIDT; B. RAMSEY; C. REYNOLDS; H. RUSSELL; S. SAFI-HARB; S. SAITO; K. SAKAI; S. SAKAI; H. SAMESHIMA; T. SASAKI; G. SATO; K. SATO; R. SATO; Y. SATO; M. SAWADA; N. SCHARTEL; PJ SERLEMITSOS; H. SETA; Y. SHIBANO; M. SHIDA; M. SHIDATSU; T. SHIMADA; K. SHINOZAKI; P. SHIRRON; A. SIMIONESCU; C. SIMMONS; RK SMITH; G. SNEIDERMAN; Y. SOONG; L. STAWARZ; Y. SUGAWARA; S. SUGITA; H. SUGITA; A. SZYMKOWIAK; H. TAJIMA; H. TAKAHASHI; S. TAKEDA; Y. TAKEI; T. TAMAGAWA; T. TAMURA; K. TAMURA; T. TANAKA; Y. TANAKA; YT TANAKA; MS TASHIRO; Y. TAWARA; Y. TERADA; Y. TERASHIMA; F. TOMBESI; H. TOMIDA; Y. TSUBOI; M. TSUJIMOTO; H. TSUNEMI; TG TSURU; H. UCHIDA; H. UCHIYAMA; Y. UCHIYAMA; S. UEDA; Y. UEDA; S. UENO; S. UNO; CM URRY; E. URSINO; CP DE VRIES; A. WADA; S. WATANABE; T. WATANABE; Norbert WERNER; DR WIK; DR WILKINS; BJ WILLIAMS; S. YAMADA; T. YAMADA; H. YAMAGUCHI; K. YAMAOKA; NY YAMASAKI; M. YAMAUCHI; S. YAMAUCHI; T. YAQOOB; Y. YATSU; D. YONETOKU; A. YOSHIDA; T. YUASA; I. ZHURAVLEVA a A. ZOGHBI

Vydání

JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS, BELLINGHAM, SPIE-SOC PHOTO-OPTICAL INSTRUMENTATION ENGINEERS, 2018, 2329-4124

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Spojené státy

Utajení

není předmětem státního či obchodního tajemství

Odkazy

Impakt faktor

Impact factor: 3.143

Označené pro přenos do RIV

Ano

Kód RIV

RIV/00216224:14310/18:00103908

Organizační jednotka

Přírodovědecká fakulta

EID Scopus

Klíčová slova anglicky

x-ray; hard x-ray; gamma ray; x-ray astronomy; gamma-ray astronomy; microcalorimeter
Změněno: 10. 11. 2022 12:37, Mgr. Marie Novosadová Šípková, DiS.

Anotace

V originále

The Hitomi (ASTRO-H) mission is the sixth Japanese x-ray astronomy satellite developed by a large international collaboration, including Japan, USA, Canada, and Europe. The mission aimed to provide the highest energy resolution ever achieved at E > 2 keV, using a microcalorimeter instrument, and to cover a wide energy range spanning four decades in energy from soft x-rays to gamma rays. After a successful launch on February 17, 2016, the spacecraft lost its function on March 26, 2016, but the commissioning phase for about a month provided valuable information on the onboard instruments and the spacecraft system, including astrophysical results obtained from first light observations. The paper describes the Hitomi (ASTRO-H) mission, its capabilities, the initial operation, and the instruments/spacecraft performances confirmed during the commissioning operations for about a month. (C) The Authors. Published by SPIE under a Creative Commons Attribution 3.0 Unported License.