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                          Compton Observatory

   *****************   BATSE Bright Source Report   *****************

                      (Earth Occultation Monitoring)

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            Data for: Jun. 24, 1997 thru Jun. 25, 1997   TJD 10623-10624

  Source        TJD          Flux      Spectral    Signif**   Comments
                        (ph/cm^2 sec,   Index*
                         20-100 keV)  (20-100 keV)

  CRAB          10623        0.33        -2.2        70.3
                10624        0.33                    83.8

  SCOX-1        10623        0.17        -5.0        17.5
                10624        0.14                    14.6

  1E1740-29     10623        0.07        -2.5         8.6
                10624        0.05                     6.1

  GRS1915+105   10623        0.08        -2.8         8.5
                10624        0.07                     6.2

  GRS1758-258   10623        0.03        -2.0         4.8
                10624        0.02                     3.2

  NGC4151       10623        0.02        -2.0         4.1
                10624        0.02                     4.4

  VELAX-1       10623        0.04        -3.7         3.7
                10624        0.09                     9.8

  CYGX-1        10624        0.28        -2.0        31.2

  4U1700-377    10624        0.11        -3.0        10.3

  GX339-4       10624        0.05        -2.4         5.9

  Notes:   * Spectral index for power law fit to photon number spectrum
             (photons/cm^2-s) in 20-100 keV band

           **Detection Significance, = Flux/Sigma

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  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).