-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: May. 4, 1997 thru May. 7, 1997 TJD 10572-10575 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10572 0.33 -2.2 71.3 10573 0.34 67.9 10574 0.32 50.8 10575 0.34 68.4 CYGX-1 10572 0.44 -2.0 31.6 10573 0.36 51.0 10574 0.32 53.2 10575 0.31 59.2 SCOX-1 10572 0.16 -5.0 12.3 10573 0.14 10.7 10574 0.16 14.7 10575 0.19 18.3 GRS1915+105 10572 0.13 -2.8 10.5 10573 0.11 11.0 10574 0.13 15.2 10575 0.11 9.8 GX339-4 10572 0.05 -2.4 6.3 10573 0.06 7.3 10574 0.04 5.4 HERX-1 10572 0.05 -4.4 6.2 10573 0.07 7.7 NGC4151 10572 0.02 -2.0 4.9 10573 0.02 4.6 10574 0.02 3.8 1E1740-29 10572 0.04 -2.5 4.3 10573 0.08 9.1 10574 0.06 4.9 possible source 10575 0.11 5.6 interference 4U1700-377 10572 0.06 -3.0 3.7 10573 0.04 3.1 10574 0.04 3.2 VELAX-1 10573 0.14 -3.7 9.5 10574 0.10 6.6 10575 0.08 6.5 3C273 10573 0.02 -1.6 5.3 CYGX-3 10574 0.04 -3.3 3.7 10575 0.03 4.1 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).