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Peer-reviewed

Astro-H/Hitomi data analysis, processing, and archive

L. Angelini, Y. Terada, M. Dutka, J. R. Eggen, I. Harrus, Robert Hill, H. A. Krimm, Michael Loewenstein, Eric D. Miller, Masayoshi Nobukawa, Kristin Rutkowski, Andrew J. Sargent, Makoto Sawada, H. Takahashi, Hiroya Yamaguchi, Tahir Yaqoob

Journal of Astronomical Telescopes Instruments and Systems · 2018

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Summary

Astro-H is the x-ray/gamma-ray mission led by Japan with international participation, launched on February 17, 2016. Soon after launch, Astro-H was renamed Hitomi. 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. On March 27, 2016, JAXA lost contact with the satellite and, on April 28, they announced the cessation of the efforts to restore mission operations. Hitomi collected about one month’s worth of data with its instruments. 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. These activities have been a collaborative effort shared between scientists and software

Source type
Peer-reviewed study
DOI
10.1117/1.jatis.4.1.011207
Catalogue ID
SNmoic29yz-e035dv
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