-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Mar. 2, 1997 thru Mar. 5, 1997 TJD 10509-10512 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10509 0.31 -2.2 71.0 10510 0.31 71.2 10511 0.31 74.7 10512 0.32 66.8 CYGX-1 10509 0.23 -2.0 60.6 10510 0.23 60.7 10511 0.23 60.5 10512 0.25 34.6 SCOX-1 10509 0.33 -5.0 21.9 10510 0.22 12.2 10511 0.19 10.6 10512 0.09 3.7 GRS1915+105 10509 0.12 -2.8 19.7 10510 0.09 14.1 10511 0.11 16.0 10512 0.16 15.5 GROJ1744-28 10509 0.33 -4.2 18.7 10510 0.37 20.9 10511 0.38 17.2 10512 0.32 15.1 4U1700-377 10509 0.12 -3.0 10.7 10511 0.11 7.8 10512 0.07 5.3 CENX-3 10509 0.13 -4.5 7.7 10510 0.08 4.1 1E1740-29 10509 0.04 -2.5 3.6 possible source 10510 0.06 5.2 confusion 10511 0.06 4.1 NGC4151 10509 0.02 -2.0 3.4 10510 0.02 4.9 10511 0.01 3.2 VELAX-1 10510 0.08 -3.7 7.5 10511 0.15 14.4 10512 0.07 6.0 CYGX-3 10510 0.04 -3.3 4.0 10512 0.07 5.8 CEN_A 10512 0.01 -1.9 3.1 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).