-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Sep. 15, 1997 thru Sep. 18, 1997 TJD 10706-10709 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CYGX-1 10706 0.29 -2.0 69.4 10707 0.28 65.3 10708 0.30 80.1 10709 0.26 61.7 CRAB 10706 0.31 -2.2 50.0 10707 0.32 55.4 10708 0.32 61.4 10709 0.32 51.0 HERX-1 10706 0.10 -4.4 11.4 10707 0.08 8.7 10708 0.07 6.4 10709 0.10 8.4 4U1700-377 10706 0.11 -3.0 9.8 10707 0.17 13.8 GRS1915+105 10706 0.04 -2.8 7.4 10707 0.10 18.3 10708 0.09 15.6 10709 0.06 11.0 GX301-2 10706 0.09 -4.4 7.2 10707 0.21 15.4 10708 0.21 15.8 10709 0.30 23.1 GX339-4 10706 0.05 -2.4 6.9 10707 0.06 7.4 10708 0.03 4.7 10709 0.07 7.7 SCOX-1 10706 0.15 -5.0 6.4 10707 0.16 6.1 10708 0.18 8.2 10709 0.15 3.5 CYGX-3 10706 0.05 -3.3 5.1 10707 0.04 3.8 10708 0.05 5.7 NGC4151 10706 0.03 -2.0 4.0 GRS1758-258 10706 0.02 -2.0 3.6 10708 0.03 3.6 1E1740-29 10706 0.06 -2.5 3.1 10709 0.07 5.2 VELAX-1 10707 0.16 -3.7 10.8 10708 0.16 11.2 10709 0.15 12.8 3C273 10707 0.01 -1.6 3.4 OAO1657-415 10708 0.04 -3.4 3.1 CEN_A 10709 0.01 -1.9 3.6 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).