SWIFT/BAT Detections of Hard X-ray Sources: IV

Details SWIFT/BAT Detections of Hard X-ray Sources: IV SWIFT/BAT Detections of Hard X-ray Sources: IV

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..697....1a&link_type=abstract

The Astronomer's Telegram, #697

Astronomy and Astrophysics

Astronomy

15

X-Ray, Gamma Ray, Agn, Binaries

Scientific paper

We report on the first detection of hard X-rays (15-150 keV) from further 3 sources with the Swift Burst Alert Telescope (BAT), and subsequent follow-up observations with the Swift X-ray Telescope (XRT; 0.5-10 keV). In contrast Tueller et al. (ATEL #668, #669) and Kennea et al. (ATEL #677), BAT data from May-Nov 2005 have been used. Sources are named by their SWIFT/BAT name/position. The XRT position is accurate to a few arcsec, but can be off the BAT position by about 3 arcmin (90%).

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