-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Dec. 12, 1997 thru Dec. 14, 1997 TJD 10794-10796 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10794 0.31 -2.2 81.9 10795 0.31 79.4 10796 0.31 74.1 CYGX-1 10794 0.30 -2.0 68.6 10795 0.28 71.0 10796 0.28 63.6 SCOX-1 10794 0.20 -5.0 12.3 10795 0.15 10.3 10796 0.24 16.5 1E1740-29 10794 0.11 -2.5 11.9 10795 0.11 15.1 10796 0.06 7.6 4U1700-377 10794 0.10 -3.0 10.7 10795 0.07 5.4 GS1354-645 10794 0.08 -2.5 8.8 10795 0.08 7.7 GX301-2 10794 0.21 -4.4 7.1 10795 0.07 4.2 10796 0.11 4.9 GRS1758-258 10794 0.04 -2.0 5.7 10795 0.03 4.4 GX339-4 10794 0.05 -2.4 5.6 10795 0.05 5.7 10796 0.06 6.4 GRS1915+105 10794 0.04 -2.8 4.2 10796 0.03 3.8 3C273 10794 0.01 -1.6 4.2 CYGX-3 10794 0.05 -3.3 4.1 CEN_A 10794 0.02 -1.9 3.5 10795 0.02 4.7 OAO1657-415 10795 0.06 -3.4 3.6 10796 0.10 5.5 Notes: * Spectral index for power law fit to photon number spectrum (photons/cm^2-s) in 20-100 keV band **Detection Significance, = Flux/Sigma -------------------------------------------------------------------------------- The information given above comes from the quick-look analysis performed daily on data obtained from the Burst and Transient Source Experiment (BATSE). The typical sensitivity of these measurements using the Earth occultation technique (one-day integration) is ~100 mCrab. Be aware that sources within about 22 degrees of the orbital poles are not occulted by the Earth; therefore, some bright sources may not show up in the daily averages. These quick-look science results are freely available, but should be considered preliminary. Please use with caution. For additional information, contact B.A. Harmon (harmon@sslmor.msfc.nasa.gov).