-------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) -------------------------------------------------------------------------------- Data for: May. 18, 1997 thru May. 21, 1997 TJD 10586-10589 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CYGX-1 10586 0.32 -2.0 89.1 10587 0.35 98.3 10588 0.32 64.0 10589 0.34 54.2 CRAB 10586 0.33 -2.2 84.8 10587 0.32 85.6 10588 0.33 79.8 10589 0.34 70.9 SCOX-1 10586 0.17 -5.0 16.1 10587 0.21 20.4 10588 0.16 17.6 10589 0.14 15.9 GX301-2 10586 0.16 -4.4 11.0 10587 0.14 8.5 10588 0.10 6.9 GRS1915+105 10586 0.06 -2.8 10.3 10587 0.07 11.8 10588 0.09 16.2 10589 0.10 22.2 GX339-4 10586 0.06 -2.4 9.6 10587 0.04 4.2 10588 0.06 7.6 10589 0.06 7.3 VELAX-1 10586 0.09 -3.7 9.1 10587 0.07 8.1 GX1+4 10586 0.05 -3.0 6.7 10587 0.03 4.8 10588 0.04 6.1 10589 0.04 6.1 1E1740-29 10586 0.04 -2.5 6.2 10587 0.04 6.8 10588 0.04 7.9 10589 0.04 8.8 CYGX-3 10586 0.03 -3.3 3.7 10587 0.03 3.2 4U1700-377 10589 0.04 -3.0 3.4 OAO1657-415 10589 0.07 -3.4 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).