The Swift gamma-ray burst (GRB) observatory was launched in 2004 November, and has been continually observing the hard X-ray (14–195 keV) sky ever since with the Burst Alert Telescope (BAT). The 70 month Swift-BAT survey is the most sensitive and uniform hard X-ray all-sky survey and reaches a flux level of 1.03×10−11 erg s−1cm−2 over 50% of the sky and 1.34×10−11 erg s−1cm−2 over 90% of the sky. Swift has three co-aligned instruments for studying gamma-ray bursts and their afterglow: the Burst Alert Telescope (BAT), the X-ray Telescope (XRT), and the Ultraviolet/Optical Telescope (UVOT).

CADE only serves

• ' The Swift Gamma-Ray Burst Mission' by Gehrels, N., et al., 2004, ApJ, 611, 1005 http://adsabs.harvard.edu/abs/2004ApJ...611.1005G

• ' The 70 Month Swift-BAT All-sky Hard X-Ray Survey' by Baumgartner, W. H., et al., 2013, ApJS, 207, 19 http://adsabs.harvard.edu/abs/2013ApJS..207...19B

14-20 keV : BAT_14_20_1_512.fits Aladin

20-24 keV : BAT_20_24_1_512.fits Aladin

24-35 keV : BAT_20_35_1_512.fits Aladin

35-50 keV : BAT_35_50_1_512.fits Aladin

50-75 keV : BAT_50_75_1_512.fits Aladin

75-100 keV : BAT_75_100_1_512.fits Aladin

100-150 keV : BAT_100_150_1_512.fits Aladin

150-195 keV : BAT_150_195_1_512.fits Aladin

https://skyview.gsfc.nasa.gov/current/cgi/query.pl

https://swift.gsfc.nasa.gov/