-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Aug. 18, 1997 thru Aug. 21, 1997 TJD 10678-10681 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10678 0.32 -2.2 62.5 10679 0.31 64.3 10680 0.32 64.8 10681 0.32 63.6 CYGX-1 10678 0.32 -2.0 24.6 10679 0.28 29.6 10680 0.33 56.6 10681 0.30 50.8 SCOX-1 10678 0.15 -5.0 8.7 10679 0.17 9.5 10680 0.15 7.9 10681 0.11 5.6 GRS1915+105 10678 0.07 -2.8 8.3 10679 0.05 4.3 10680 0.04 4.6 10681 0.09 10.7 4U1700-377 10678 0.08 -3.0 7.1 10680 0.06 3.5 GRS1758-258 10678 0.03 -2.0 4.8 10681 0.04 5.1 GX1+4 10678 0.10 -3.0 4.1 GX339-4 10678 0.03 -2.4 3.6 10679 0.05 5.9 10680 0.04 4.9 10681 0.04 5.4 NGC4151 10678 0.01 -2.0 3.1 1E1740-29 10679 0.07 -2.5 6.0 10680 0.07 6.7 10681 0.05 4.5 HERX-1 10679 0.04 -4.4 3.7 3C273 10679 0.01 -1.6 3.1 VELAX-1 10680 0.04 -3.7 3.5 10681 0.18 13.6 SMCX-1 10680 0.01 -2.0 3.1 CYGX-3 10681 0.06 -3.3 5.8 OAO1657-415 10681 0.11 -3.4 5.1 CEN_A 10681 0.03 -1.9 4.3 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).