-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Jul. 14, 1997 thru Jul. 16, 1997 TJD 10643-10645 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10643 0.33 -2.2 77.3 10644 0.34 68.4 10645 0.33 65.9 CYGX-1 10643 0.26 -2.0 66.4 10644 0.28 66.7 10645 0.34 84.9 SCOX-1 10643 0.14 -5.0 17.9 10644 0.19 19.6 10645 0.16 12.9 1E1740-29 10643 0.07 -2.5 14.2 10644 0.08 14.2 10645 0.07 12.2 GRS1915+105 10643 0.05 -2.8 6.8 10644 0.03 4.5 10645 0.03 5.1 4U1630-47 10643 0.04 -3.0 6.4 GX1+4 10643 0.04 -3.0 6.1 10644 0.04 5.2 10645 0.05 7.7 CYGX-3 10643 0.05 -3.3 6.0 10644 0.04 4.6 10645 0.06 6.0 NGC4151 10643 0.02 -2.0 3.8 10644 0.03 5.0 4U1700-377 10644 0.11 -3.0 9.7 10645 0.12 10.1 GX301-2 10644 0.06 -4.4 4.6 NGC5548 10644 0.02 -2.0 4.1 10645 0.02 4.2 SMCX-1 10644 0.03 -2.0 3.5 GX339-4 10644 0.03 -2.4 3.3 Possible source 10645 0.05 4.9 confusion CEN_A 10644 0.01 -1.9 3.3 10645 0.01 3.1 VELAX-1 10645 0.18 -3.7 9.2 MRK421 10645 0.01 -2.0 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).