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

Research output: Contribution to journalReview article

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.

Original languageEnglish
Pages (from-to)S21-S211
JournalPublications of the Astronomical Society of Japan
Volume68
DOIs
Publication statusPublished - 2016 Jun 1
Externally publishedYes

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Keywords

  • binaries: general
  • methods: data analysis
  • stars: activity
  • stars: black holes
  • stars: jets

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Sakamoto, T., Oda, R., Mihara, T., Yoshida, A., Arimoto, M., Barthelmy, S. D., Kawai, N., Krimm, H. A., Nakahira, S., & Serino, M. (2016). Swift/BAT and MAXI/GSC broadband transient monitor. Publications of the Astronomical Society of Japan, 68, S21-S211. https://doi.org/10.1093/pasj/psv130