-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Oct. 16, 1997 thru Oct. 18, 1997 TJD 10737-10739 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10737 0.31 -2.2 76.2 10738 0.31 76.0 10739 0.32 76.8 CYGX-1 10737 0.34 -2.0 71.4 10738 0.33 85.3 10739 0.38 88.4 SCOX-1 10737 0.23 -5.0 15.0 10738 0.24 9.0 10739 0.16 7.5 VELAX-1 10737 0.09 -3.7 8.7 10738 0.10 8.3 4U1700-377 10737 0.16 -3.0 8.1 10738 0.11 10.1 10739 0.03 3.5 1E1740-29 10737 0.11 -2.5 6.1 Possible source 10738 0.08 8.2 confusion 10739 0.07 7.4 GX339-4 10737 0.07 -2.4 4.7 10738 0.05 6.5 10739 0.05 6.3 CYGX-3 10737 0.04 -3.3 4.3 10738 0.05 5.3 10739 0.05 5.5 GRS1915+105 10737 0.09 -2.8 3.1 10738 0.10 7.5 10739 0.07 5.4 OAO1657-415 10738 0.11 -3.4 5.4 GRS1758-258 10738 0.03 -2.0 3.6 Possible source 10739 0.04 4.4 confusion HERX-1 10738 0.04 -4.4 3.4 10739 0.04 3.5 CEN_A 10738 0.02 -1.9 3.2 NGC4151 10738 0.02 -2.0 3.2 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).