Swift/BAT and MAXI/GSC broadband transient monitor

Takanori Sakamoto; Ryoma Oda; Tatehiro Mihara; Atsumasa Yoshida; Makoto Arimoto; Scott D. Barthelmy; Nobuyuki Kawai; Hans A. Krimm; Satoshi Nakahira; Motoko Serino

doi:10.1093/pasj/psv130

Swift/BAT and MAXI/GSC broadband transient monitor

Takanori Sakamoto, Ryoma Oda, Tatehiro Mihara, Atsumasa Yoshida, Makoto Arimoto, Scott D. Barthelmy, Nobuyuki Kawai, Hans A. Krimm, Satoshi Nakahira, Motoko Serino

研究成果: Review article › 査読

1 被引用数 (Scopus)

抄録

We present a newly developed broadband transient monitor using the Swift Burst Alert Telescope (BAT) and the MAXI Gas Slit Camera (GSC) data. Our broadband transient monitor keeps vigil for high-energy transient sources from 2 keV to 200 keV in seven energy bands by combining the BAT (15-200 keV) and the GSC (2-20 keV) data. Currently, daily and 90-minute (one orbit) averaged light curves are available for 106 high-energy transient sources. This transient monitor is available to the public through our web server, http://yoshidalab.mydns.jp/bat-gsc-trans-mon/, for wider use by the community. We discuss a daily sensitivity of our monitor and possible future improvements on our pipeline.

本文言語	English
ページ（範囲）	S21-S211
ジャーナル	Publications of the Astronomical Society of Japan
巻	68
DOI	https://doi.org/10.1093/pasj/psv130
出版ステータス	Published - 2016 6月 1
外部発表	はい

ASJC Scopus subject areas

天文学と天体物理学
宇宙惑星科学

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10.1093/pasj/psv130

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引用スタイル

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title = "Swift/BAT and MAXI/GSC broadband transient monitor",

abstract = "We present a newly developed broadband transient monitor using the Swift Burst Alert Telescope (BAT) and the MAXI Gas Slit Camera (GSC) data. Our broadband transient monitor keeps vigil for high-energy transient sources from 2 keV to 200 keV in seven energy bands by combining the BAT (15-200 keV) and the GSC (2-20 keV) data. Currently, daily and 90-minute (one orbit) averaged light curves are available for 106 high-energy transient sources. This transient monitor is available to the public through our web server, http://yoshidalab.mydns.jp/bat-gsc-trans-mon/, for wider use by the community. We discuss a daily sensitivity of our monitor and possible future improvements on our pipeline.",

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author = "Takanori Sakamoto and Ryoma Oda and Tatehiro Mihara and Atsumasa Yoshida and Makoto Arimoto and Barthelmy, {Scott D.} and Nobuyuki Kawai and Krimm, {Hans A.} and Satoshi Nakahira and Motoko Serino",

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month = jun,

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doi = "10.1093/pasj/psv130",

language = "English",

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T1 - Swift/BAT and MAXI/GSC broadband transient monitor

AU - Sakamoto, Takanori

AU - Oda, Ryoma

AU - Mihara, Tatehiro

AU - Yoshida, Atsumasa

AU - Arimoto, Makoto

AU - Barthelmy, Scott D.

AU - Kawai, Nobuyuki

AU - Krimm, Hans A.

AU - Nakahira, Satoshi

AU - Serino, Motoko

PY - 2016/6/1

Y1 - 2016/6/1

N2 - We present a newly developed broadband transient monitor using the Swift Burst Alert Telescope (BAT) and the MAXI Gas Slit Camera (GSC) data. Our broadband transient monitor keeps vigil for high-energy transient sources from 2 keV to 200 keV in seven energy bands by combining the BAT (15-200 keV) and the GSC (2-20 keV) data. Currently, daily and 90-minute (one orbit) averaged light curves are available for 106 high-energy transient sources. This transient monitor is available to the public through our web server, http://yoshidalab.mydns.jp/bat-gsc-trans-mon/, for wider use by the community. We discuss a daily sensitivity of our monitor and possible future improvements on our pipeline.

AB - We present a newly developed broadband transient monitor using the Swift Burst Alert Telescope (BAT) and the MAXI Gas Slit Camera (GSC) data. Our broadband transient monitor keeps vigil for high-energy transient sources from 2 keV to 200 keV in seven energy bands by combining the BAT (15-200 keV) and the GSC (2-20 keV) data. Currently, daily and 90-minute (one orbit) averaged light curves are available for 106 high-energy transient sources. This transient monitor is available to the public through our web server, http://yoshidalab.mydns.jp/bat-gsc-trans-mon/, for wider use by the community. We discuss a daily sensitivity of our monitor and possible future improvements on our pipeline.

KW - binaries: general

KW - methods: data analysis

KW - stars: activity

KW - stars: black holes

KW - stars: jets

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U2 - 10.1093/pasj/psv130

DO - 10.1093/pasj/psv130

M3 - Review article

AN - SCOPUS:84973349183

SN - 0004-6264

VL - 68

SP - S21-S211

JO - Publications of the Astronomical Society of Japan

JF - Publications of the Astronomical Society of Japan

ER -

Swift/BAT and MAXI/GSC broadband transient monitor

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