Astro-H data analysis, processing and archive

Astro-H (Hitomi) is an X-ray/Gamma-ray mission led by Japan with international participation, launched on February 17, 2016. The payload consists of four different instruments (SXS, SXI, HXI and SGD) that operate simultaneously to cover the energy range from 0.3 keV up to 600 keV. This paper present...

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Main Authors: Angelini, Lorella, Terada, Yukitatsu, Loewenstein, Michael, Yamaguchi, Hiroya, Yaqoob, Tahir, Krimm, Hans, Harrus, Ilana, Takahashi, Hiromitsu, Nobukawa, Masayoshi, Sawada, Makoto, Witthoeft, Michael, Rutkowski, Kristin, Sargent, Andrew, Hill, Robert S., Dutka, Michael, Eggen, Joseph, Miller, Eric D
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Published: SPIE 2018
Online Access:http://hdl.handle.net/1721.1/114869
https://orcid.org/0000-0002-3031-2326
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author Angelini, Lorella
Terada, Yukitatsu
Loewenstein, Michael
Yamaguchi, Hiroya
Yaqoob, Tahir
Krimm, Hans
Harrus, Ilana
Takahashi, Hiromitsu
Nobukawa, Masayoshi
Sawada, Makoto
Witthoeft, Michael
Rutkowski, Kristin
Sargent, Andrew
Hill, Robert S.
Dutka, Michael
Eggen, Joseph
Miller, Eric D
author2 MIT Kavli Institute for Astrophysics and Space Research
author_facet MIT Kavli Institute for Astrophysics and Space Research
Angelini, Lorella
Terada, Yukitatsu
Loewenstein, Michael
Yamaguchi, Hiroya
Yaqoob, Tahir
Krimm, Hans
Harrus, Ilana
Takahashi, Hiromitsu
Nobukawa, Masayoshi
Sawada, Makoto
Witthoeft, Michael
Rutkowski, Kristin
Sargent, Andrew
Hill, Robert S.
Dutka, Michael
Eggen, Joseph
Miller, Eric D
author_sort Angelini, Lorella
collection MIT
description Astro-H (Hitomi) is an X-ray/Gamma-ray mission led by Japan with international participation, launched on February 17, 2016. The payload consists of four different instruments (SXS, SXI, HXI and SGD) that operate simultaneously to cover the energy range from 0.3 keV up to 600 keV. This paper presents the analysis software and the data processing pipeline created to calibrate and analyze the Hitomi science data along with the plan for the archive and user support. These activities have been a collaborative effort shared between scientists and software engineers working in several institutes in Japan and USA.
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spelling mit-1721.1/1148692022-09-30T17:09:30Z Astro-H data analysis, processing and archive Angelini, Lorella Terada, Yukitatsu Loewenstein, Michael Yamaguchi, Hiroya Yaqoob, Tahir Krimm, Hans Harrus, Ilana Takahashi, Hiromitsu Nobukawa, Masayoshi Sawada, Makoto Witthoeft, Michael Rutkowski, Kristin Sargent, Andrew Hill, Robert S. Dutka, Michael Eggen, Joseph Miller, Eric D MIT Kavli Institute for Astrophysics and Space Research Miller, Eric D Astro-H (Hitomi) is an X-ray/Gamma-ray mission led by Japan with international participation, launched on February 17, 2016. The payload consists of four different instruments (SXS, SXI, HXI and SGD) that operate simultaneously to cover the energy range from 0.3 keV up to 600 keV. This paper presents the analysis software and the data processing pipeline created to calibrate and analyze the Hitomi science data along with the plan for the archive and user support. These activities have been a collaborative effort shared between scientists and software engineers working in several institutes in Japan and USA. 2018-04-23T15:40:40Z 2018-04-23T15:40:40Z 2016-06 2018-03-16T14:08:33Z Article http://purl.org/eprint/type/ConferencePaper http://hdl.handle.net/1721.1/114869 Angelini, Lorella, et al. "Astro-H Data Analysis, Processing and Archive." Proceedings Volume 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, 29 June - 1 July, 2016, Edinburgh, Scotland, edited by Jan-Willem A. den Herder et al., SPIE, 2016, p. 990514. © 2016 SPIE https://orcid.org/0000-0002-3031-2326 http://dx.doi.org/10.1117/12.2234429 Proceedings Volume 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf SPIE SPIE
spellingShingle Angelini, Lorella
Terada, Yukitatsu
Loewenstein, Michael
Yamaguchi, Hiroya
Yaqoob, Tahir
Krimm, Hans
Harrus, Ilana
Takahashi, Hiromitsu
Nobukawa, Masayoshi
Sawada, Makoto
Witthoeft, Michael
Rutkowski, Kristin
Sargent, Andrew
Hill, Robert S.
Dutka, Michael
Eggen, Joseph
Miller, Eric D
Astro-H data analysis, processing and archive
title Astro-H data analysis, processing and archive
title_full Astro-H data analysis, processing and archive
title_fullStr Astro-H data analysis, processing and archive
title_full_unstemmed Astro-H data analysis, processing and archive
title_short Astro-H data analysis, processing and archive
title_sort astro h data analysis processing and archive
url http://hdl.handle.net/1721.1/114869
https://orcid.org/0000-0002-3031-2326
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