-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Feb. 19, 1998 thru Feb. 22, 1998 TJD 10863-10866 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CYGX-1 10863 0.29 -2.0 72.0 10864 0.33 85.8 10865 0.30 75.4 10866 0.30 75.0 CRAB 10863 0.31 -2.2 71.6 10864 0.31 70.6 10865 0.32 62.9 10866 0.32 66.0 4U1630-47 10863 0.08 -3.0 11.6 10864 0.09 12.6 10865 0.09 13.9 10866 0.09 14.3 SCOX-1 10863 0.15 -5.0 10.4 10864 0.10 5.9 10865 0.21 15.9 10866 0.11 6.3 4U1700-377 10863 0.07 -3.0 9.3 10864 0.07 9.6 10865 0.03 4.1 10866 0.14 18.1 CYGX-3 10863 0.07 -3.3 9.0 10864 0.05 6.5 10865 0.05 6.2 10866 0.05 6.9 VELAX-1 10863 0.07 -3.7 7.8 10864 0.07 8.0 10865 0.08 8.2 10866 0.06 7.3 OAO1657-415 10863 0.07 -3.4 6.2 10864 0.06 5.0 10865 0.04 4.1 1E1740-29 10863 0.06 -2.5 5.8 10864 0.07 6.9 10865 0.05 4.8 GX301-2 10863 0.17 -4.4 5.6 10865 0.08 4.8 CEN_A 10863 0.02 -1.9 4.9 10864 0.01 3.1 10866 0.02 4.8 3C279 10863 0.01 -2.0 3.1 GS1826-238 10864 0.03 -3.0 4.5 Possible Source 10866 0.03 3.9 Confusion NGC4151 10864 0.01 -2.0 3.0 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).