15 July 2016 Astro-H data analysis, processing and archive
Author Affiliations +
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.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Lorella Angelini, Lorella Angelini, Yukitatsu Terada, Yukitatsu Terada, Michael Loewenstein, Michael Loewenstein, Eric D. Miller, Eric D. Miller, Hiroya Yamaguchi, Hiroya Yamaguchi, Tahir Yaqoob, Tahir Yaqoob, Hans Krimm, Hans Krimm, Ilana Harrus, Ilana Harrus, Hiromitsu Takahashi, Hiromitsu Takahashi, Masayoshi Nobukawa, Masayoshi Nobukawa, Makoto Sawada, Makoto Sawada, Michael Witthoeft, Michael Witthoeft, Kristin Rutkowski, Kristin Rutkowski, Andrew Sargent, Andrew Sargent, Robert S. Hill, Robert S. Hill, Michael Dutka, Michael Dutka, Joseph Eggen, Joseph Eggen, } "Astro-H data analysis, processing and archive", Proc. SPIE 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, 990514 (15 July 2016); doi: 10.1117/12.2234429; https://doi.org/10.1117/12.2234429


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