-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Jul. 10, 1997 thru Jul. 13, 1997 TJD 10639-10642 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10639 0.33 -2.2 82.6 10640 0.33 63.5 10641 0.35 65.9 10642 0.33 71.2 CYGX-1 10639 0.31 -2.0 77.5 10640 0.29 72.4 10641 0.27 62.0 10642 0.28 57.0 SCOX-1 10639 0.17 -5.0 17.7 10640 0.15 17.5 10641 0.19 22.1 10642 0.21 25.9 VELAX-1 10639 0.12 -3.7 9.9 10640 0.08 7.7 10641 0.17 16.6 10642 0.04 3.4 1E1740-29 10639 0.04 -2.5 8.0 10640 0.06 10.8 10641 0.04 8.3 10642 0.06 12.0 HERX-1 10639 0.09 -4.4 6.0 10640 0.08 4.2 10641 0.09 4.7 GRS1915+105 10639 0.04 -2.8 5.6 10640 0.05 7.3 10641 0.03 5.1 10642 0.05 6.8 CYGX-3 10639 0.04 -3.3 5.1 10640 0.04 4.3 10641 0.07 7.5 10642 0.08 7.7 GX1+4 10639 0.04 -3.0 4.8 10640 0.04 5.0 10641 0.03 4.8 10642 0.02 3.4 OAO1657-415 10639 0.12 -3.4 4.2 GX301-2 10639 0.06 -4.4 4.0 10640 0.08 5.8 10641 0.06 3.8 10642 0.05 3.6 CENX-3 10639 0.06 -4.5 3.5 CEN_A 10640 0.01 -1.9 3.6 NGC4151 10641 0.03 -2.0 5.8 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).