-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Apr. 4, 1997 thru Apr. 6, 1997 TJD 10542-10544 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10542 0.33 -2.2 72.6 10543 0.33 57.8 10544 0.31 54.3 CYGX-1 10542 0.24 -2.0 51.0 10543 0.25 55.3 10544 0.33 64.0 GX301-2 10542 0.22 -4.4 14.8 10543 0.16 12.3 10544 0.16 12.8 GROJ1744-28 10542 0.17 -4.2 14.1 10543 0.19 14.0 10544 0.13 9.6 VELAX-1 10542 0.11 -3.7 14.1 10543 0.06 6.4 SCOX-1 10542 0.17 -5.0 14.0 10543 0.11 5.4 4U1700-377 10542 0.09 -3.0 11.6 10543 0.06 5.3 GX339-4 10542 0.07 -2.4 10.5 10543 0.05 5.0 10544 0.07 4.8 GRS1915+105 10542 0.05 -2.8 7.7 10543 0.11 12.3 10544 0.07 7.7 GX1+4 10542 0.06 -3.0 6.8 10543 0.05 4.7 NGC4151 10542 0.02 -2.0 5.1 10544 0.02 3.4 3C273 10542 0.01 -1.6 4.5 CYGX-3 10542 0.03 -3.3 3.0 10543 0.04 4.1 10544 0.08 7.5 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).