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Swift/BAT and MAXI/GSC Broadband Transient Monitor

We present the newly developed broadband transient monitor using the Swift Burst Alert Telescope (BAT) and the MAXI Gas Slit Camera (GSC) data. Our broadband transient monitor monitors 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, the daily and the 90-minute (one orbit) averaged light curves are available for 106 high energy transient sources. Our broadband transient monitor is available to the public through our web server, http://yoshidalab.mydns.jp/bat_gsc_trans_mon/, for a wider use by the community. We discuss the daily sensitivity of our monitor and possible future improvements to our pipeline.

preprint2015arXivOpen access
Takanori SakamotoRyoma OdaTatehiro MiharaAtsumasa YoshidaMakoto ArimotoScott D. BarthelmyNobuyuki KawaiHans A. KrimmSatoshi NakahiraMotoko Serino
astro-ph.HE
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Open access10 authors1 topic
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Authors

Takanori SakamotoRyoma OdaTatehiro MiharaAtsumasa YoshidaMakoto ArimotoScott D. BarthelmyNobuyuki KawaiHans A. KrimmSatoshi NakahiraMotoko Serino

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