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.
CITATION STYLE
Sakamoto, T., Oda, R., Mihara, T., Yoshida, A., Arimoto, M., Barthelmy, S. D., … Serino, M. (2016, June 1). Swift/BAT and MAXI/GSC broadband transient monitor. Publications of the Astronomical Society of Japan. Oxford University Press. https://doi.org/10.1093/pasj/psv130
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