------------------------------------------------------------------------------- Compton Observatory ***************** BATSE Bright Source Report ***************** (Earth Occultation Monitoring) ------------------------------------------------------------------------------- Data for: Jan. 20, 1997 thru Jan. 23, 1997 TJD 10468-10471 Source TJD Flux Spectral Signif** Comments (ph/cm^2 sec, Index* 20-100 keV) (20-100 keV) CRAB 10468 0.31 -2.2 52.9 10469 0.31 49.2 10470 0.33 58.1 10471 0.32 55.6 CYGX-1 10468 0.29 -2.0 16.0 10469 0.21 8.3 10470 0.27 35.7 10471 0.27 29.7 GROJ1744-28 10468 0.55 -4.2 15.5 10469 0.58 19.3 10470 0.61 26.4 10471 0.51 13.1 GRS1915+105 10468 0.20 -2.8 12.6 10469 0.12 9.8 10470 0.13 12.2 10471 0.16 12.8 SCOX-1 10468 0.14 -5.0 10.3 10469 0.18 13.6 10470 0.18 13.6 10471 0.15 11.5 4U1700-377 10468 0.12 -3.0 9.4 10470 0.06 4.2 10471 0.06 3.6 VELAX-1 10468 0.09 -3.7 8.0 10469 0.09 7.4 10470 0.09 9.7 10471 0.09 9.0 GX339-4 10468 0.06 -2.4 6.5 10469 0.03 3.5 10470 0.04 4.1 10471 0.08 7.9 NGC4151 10468 0.03 -2.0 5.4 10469 0.02 3.2 10470 0.02 3.9 10471 0.02 3.7 HERX-1 10468 0.06 -4.4 4.6 1E1740-29 10468 0.07 -2.5 3.5 Confusion with 10470 0.07 3.3 CGRO J1744-28 likely AQLX-1 10469 0.03 -2.0 2.5 Possible source confusion 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 data are of a preliminary nature and should only be used for planning observational programs, and are not intended for publication. Please do not distribute this report beyond your local team. For additional information, contact B. A. Harmon (harmon@ssl.msfc.nasa.gov).