-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Sep. 19, 1997 thru Sep. 21, 1997 TJD 10710-10712 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CYGX-1 10710 0.31 -2.0 79.7 10711 0.32 82.1 Looks Active 10712 0.27 65.1 CRAB 10710 0.32 -2.2 57.3 10711 0.31 63.6 10712 0.32 58.1 GX301-2 10710 0.31 -4.4 24.3 10711 0.15 12.2 10712 0.09 6.7 VELAX-1 10710 0.29 -3.7 22.6 Maybe still has bright pulses on 10711-10712 GRS1915+105 10710 0.09 -2.8 16.0 10711 0.09 16.5 10712 0.08 14.1 HERX-1 10710 0.12 -4.4 13.4 10711 0.07 8.7 GRS0834-430 10710 0.10 -3.7 7.5 Possible Interference 10711 0.06 3.4 from Vela X-1 1E1740-29 10710 0.08 -2.5 7.0 10711 0.06 6.0 10712 0.05 5.2 GX339-4 10710 0.05 -2.4 6.5 10711 0.07 9.3 10712 0.06 8.1 SCOX-1 10710 0.14 -5.0 5.0 10711 0.27 10.8 10712 0.16 6.2 4U1700-377 10710 0.07 -3.0 4.6 10712 0.06 4.6 SAXJ0501+11 10710 0.05 -3.0 4.2 CYGX-3 10710 0.03 -3.3 3.9 10712 0.03 3.4 NGC1275 10710 0.01 -2.0 3.2 PSR1509-58 10710 0.01 -2.0 3.1 CEPX-4 10711 0.03 -3.5 3.3 CEN_A 10712 0.01 -1.9 3.8 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).