-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Jul. 28, 1997 thru Jul. 30, 1997 TJD 10657-10659 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10657 0.33 -2.2 82.6 10658 0.32 79.5 10659 0.33 79.9 CYGX-1 10657 0.33 -2.0 71.9 10658 0.31 67.2 10659 0.31 64.3 VELAX-1 10657 0.18 -3.7 18.8 10658 0.10 10.6 10659 0.09 9.7 SCOX-1 10657 0.16 -5.0 9.8 10658 0.16 9.0 10659 0.14 6.7 CYGX-3 10657 0.08 -3.3 9.2 10658 0.09 10.9 10659 0.06 6.8 GX339-4 10657 0.05 -2.4 9.0 10658 0.05 9.2 10659 0.05 7.2 1E1740-29 10657 0.05 -2.5 8.0 Possible contamination 10658 0.07 11.0 from other sources 10659 0.06 9.7 GROJ1655-40 10657 0.06 -3.2 7.9 Possible contamination 10658 0.04 3.3 from other sources OAO1657-415 10657 0.03 -3.4 4.4 GRS1915+105 10657 0.02 -2.8 3.4 10658 0.02 3.2 4U1700-377 10657 0.03 -3.0 3.3 10658 0.07 8.0 10659 0.06 6.2 GROJ1744-28 10658 0.10 -4.2 4.4 Possible contamination from other sources NGC4151 10658 0.02 -2.0 3.2 GX301-2 10659 0.08 -4.4 5.4 CENX-3 10659 0.07 -4.5 5.3 GX1+4 10659 0.04 -3.0 4.6 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).