Hitomi (ASTRO-H) X-ray Astronomy Satellite

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F18%3A00103908" target="_blank" >RIV/00216224:14310/18:00103908 - isvavai.cz</a>

Výsledek na webu

<a href="https://www.spiedigitallibrary.org/journals/Journal-of-Astronomical-Telescopes-Instruments-and-Systems/volume-4/issue-02/021402/Hitomi-ASTRO-H-X-ray-Astronomy-Satellite/10.1117/1.JATIS.4.2.021402.full" target="_blank" >https://www.spiedigitallibrary.org/journals/Journal-of-Astronomical-Telescopes-Instruments-and-Systems/volume-4/issue-02/021402/Hitomi-ASTRO-H-X-ray-Astronomy-Satellite/10.1117/1.JATIS.4.2.021402.full</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1117/1.JATIS.4.2.021402" target="_blank" >10.1117/1.JATIS.4.2.021402</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Hitomi (ASTRO-H) X-ray Astronomy Satellite

Popis výsledku v původním jazyce

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 &gt; 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.

Název v anglickém jazyce

Hitomi (ASTRO-H) X-ray Astronomy Satellite

Popis výsledku anglicky

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 &gt; 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.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

—

Návaznosti

S - Specificky vyzkum na vysokych skolach

Rok uplatnění

2018

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS

ISSN

2329-4124

e-ISSN

—

Svazek periodika

4

Číslo periodika v rámci svazku

2

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

13

Strana od-do

„021402-1“-„021402-13“

Kód UT WoS článku

000439235200002

EID výsledku v databázi Scopus

2-s2.0-85062992860