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...
Main Authors: | , , , , , , , , , , , , , , , , |
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SPIE
2018
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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. |
first_indexed | 2024-09-23T09:49:57Z |
format | Article |
id | mit-1721.1/114869 |
institution | Massachusetts Institute of Technology |
last_indexed | 2024-09-23T09:49:57Z |
publishDate | 2018 |
publisher | SPIE |
record_format | dspace |
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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