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Astro-H data analysis, processing and archive

dc.contributor.authorAngelini, Lorella
dc.contributor.authorTerada, Yukitatsu
dc.contributor.authorLoewenstein, Michael
dc.contributor.authorYamaguchi, Hiroya
dc.contributor.authorYaqoob, Tahir
dc.contributor.authorKrimm, Hans
dc.contributor.authorHarrus, Ilana
dc.contributor.authorTakahashi, Hiromitsu
dc.contributor.authorNobukawa, Masayoshi
dc.contributor.authorSawada, Makoto
dc.contributor.authorWitthoeft, Michael
dc.contributor.authorRutkowski, Kristin
dc.contributor.authorSargent, Andrew
dc.contributor.authorHill, Robert S.
dc.contributor.authorDutka, Michael
dc.contributor.authorEggen, Joseph
dc.contributor.authorMiller, Eric D
dc.date.accessioned2018-04-23T15:40:40Z
dc.date.available2018-04-23T15:40:40Z
dc.date.issued2016-06
dc.identifier.urihttp://hdl.handle.net/1721.1/114869
dc.description.abstractAstro-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.en_US
dc.publisherSPIEen_US
dc.relation.isversionofhttp://dx.doi.org/10.1117/12.2234429en_US
dc.rightsArticle 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.en_US
dc.sourceSPIEen_US
dc.titleAstro-H data analysis, processing and archiveen_US
dc.typeArticleen_US
dc.identifier.citationAngelini, 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 SPIEen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorMiller, Eric D
dc.relation.journalProceedings Volume 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Rayen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/ConferencePaperen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dc.date.updated2018-03-16T14:08:33Z
dspace.orderedauthorsAngelini, Lorella; Terada, Yukitatsu; Loewenstein, Michael; Miller, Eric D.; 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, Josephen_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-3031-2326
mit.licensePUBLISHER_POLICYen_US


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