Swift/BAT monitoring of Fermi/LAT sources

Hans A. Krimm; Scott D. Barthelmy; Neil Gehrels; Jack Tueller; Wayne H. Baumgartner; Jay R. Cummings; Taka Sakamoto; Edward E. Fenimore; David M. Palmer; Craig B. Markwardt; Gerald K. Skinner; Michael Stamatikos

arXiv · 0912.3498

Swift/BAT monitoring of Fermi/LAT sources

Hans A. Krimm·Scott D. Barthelmy·Neil Gehrels·Jack Tueller·Wayne H. Baumgartner·Jay R. Cummings·Taka Sakamoto·Edward E. Fenimore·David M. Palmer·Craig B. Markwardt·Gerald K. Skinner·Michael Stamatikos

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Abstract

The Swift Burst Alert Telescope (BAT) hard X-ray transient monitor tracks more than 700 galactic and extragalactic sources on time scales ranging from a single Swift pointing (approximately 20 minutes) to one day. The monitored sources include all objects from the Fermi LAT bright source list which are either identified or which have a 95% error confidence radius of less than eight arc minutes. We report on the detection statistics of these sources in the BAT monitor both before and after the launch of Fermi.

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Hans A. Krimm, Scott D. Barthelmy, Neil Gehrels, Jack Tueller, Wayne H. Baumgartner, Jay R. Cummings, Taka Sakamoto, Edward E. Fenimore, David M. Palmer, Craig B. Markwardt, Gerald K. Skinner, Michael Stamatikos. 2009-12-17. Swift/BAT monitoring of Fermi/LAT sources. https://arxiv.org/abs/0912.3498

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