-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: Apr. 14, 1997 thru Apr. 17, 1997 TJD 10552-10555 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CYGX-1 10552 0.30 -2.0 75.4 10553 0.25 51.8 10554 0.32 72.1 10555 0.25 60.8 CRAB 10552 0.36 -2.2 72.4 10553 0.34 71.2 10554 0.33 82.2 10555 0.33 86.8 GRS1915+105 10552 0.09 -2.8 16.8 10553 0.08 15.4 10554 0.10 15.0 10555 0.08 13.9 4U1700-377 10552 0.10 -3.0 13.5 10553 0.08 10.4 10554 0.03 3.9 10555 0.03 3.3 GX339-4 10552 0.07 -2.4 13.4 10553 0.06 11.1 10554 0.06 9.7 10555 0.06 9.4 SCOX-1 10552 0.16 -5.0 9.1 10553 0.15 8.8 10554 0.19 8.7 10555 0.18 8.0 VELAX-1 10552 0.08 -3.7 8.7 10554 0.04 3.9 10555 0.07 6.6 GROJ1744-28 10552 0.08 -4.2 8.3 10553 0.08 9.0 10554 0.08 9.0 10555 0.08 8.6 GX301-2 10552 0.04 -4.4 4.6 10553 0.04 3.6 GROJ1719-24 10552 0.02 -2.0 4.4 10553 0.04 3.5 CYGX-3 10552 0.04 -3.3 4.4 10553 0.04 4.4 10555 0.05 5.1 NGC4151 10552 0.01 -2.0 3.1 10554 0.02 3.9 OAO1657-415 10552 0.02 -3.4 3.0 10554 0.05 3.7 CENX-3 10553 0.06 -4.5 5.4 CEN_A 10553 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).