-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: May. 12, 1997 thru May. 14, 1997 TJD 10580-10582 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CYGX-1 10580 0.35 -2.0 87.3 10581 0.33 80.0 10582 0.35 85.5 CRAB 10580 0.33 -2.2 74.4 10581 0.33 63.7 10582 0.32 72.2 SCOX-1 10580 0.15 -5.0 14.3 10581 0.19 16.0 10582 0.16 14.5 1E1740-29 10580 0.10 -2.5 12.6 probable 10581 0.11 16.5 source 10582 0.08 12.8 interference GRS1915+105 10580 0.08 -2.8 12.5 10581 0.08 12.5 10582 0.08 12.8 4U1700-377 10580 0.08 -3.0 8.2 10581 0.08 7.7 10582 0.07 6.0 GRS1758-258 10580 0.04 -2.0 6.5 10581 0.03 5.3 10582 0.03 4.2 GX339-4 10580 0.03 -2.4 5.0 10581 0.05 7.5 10582 0.06 8.1 CYGX-3 10580 0.04 -3.3 4.7 10581 0.03 3.1 OAO1657-415 10581 0.05 -3.4 4.3 10582 0.07 5.8 VELAX-1 10581 0.12 -3.7 3.8 NGC4151 10582 0.02 -2.0 4.3 GX301-2 10582 0.08 -4.4 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).