-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Dec. 22, 1997 thru Dec. 24, 1997 TJD 10804-10806 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10804 0.31 -2.2 80.4 10805 0.31 74.6 10806 0.32 81.7 CYGX-1 10804 0.26 -2.0 63.9 10805 0.25 56.7 10806 0.24 60.1 SCOX-1 10804 0.14 -5.0 11.7 10805 0.16 11.2 10806 0.26 18.5 1E1740-29 10804 0.05 -2.5 10.1 10805 0.05 9.5 10806 0.05 9.5 GS1354-645 10804 0.05 -2.5 7.8 10805 0.06 9.6 10806 0.07 10.5 GX1+4 10804 0.04 -3.0 6.3 10806 0.02 3.0 GRS1915+105 10804 0.04 -2.8 5.7 10805 0.05 6.2 10806 0.03 3.6 GX301-2 10804 0.06 -4.4 4.7 10805 0.06 4.4 CYGX-3 10804 0.03 -3.3 3.6 10806 0.03 3.5 GS1826-238 10805 0.02 -3.0 3.9 Possible source 10806 0.03 5.9 confusion CEN_A 10805 0.02 -1.9 3.4 VELAX-1 10805 0.03 -3.7 3.2 10806 0.13 16.1 GX339-4 10806 0.07 -2.4 6.8 4U1700-377 10806 0.05 -3.0 3.7 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).