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                          Compton Observatory

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

                      (Earth Occultation Monitoring)

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            Data for: Jun. 15, 1997 thru Jun. 17, 1997   TJD 10614-10616

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

  CYGX-1        10614        0.29        -2.0        65.9
                10615        0.29                    73.7
                10616        0.29                    66.5

  CRAB          10614        0.32        -2.2        56.7
                10615        0.31                    55.5
                10616        0.32                    61.2

  SCOX-1        10614        0.14        -5.0        10.1
                10615        0.16                    11.7
                10616        0.17                    11.8

  GRS1915+105   10614        0.06        -2.8         8.6
                10615        0.06                     6.6
                10616        0.08                    11.3

  4U1700-377    10614        0.08        -3.0         8.1
                10615        0.04                     3.1

  1E1740-29     10614        0.05        -2.5         6.1
                10615        0.07                     7.5
                10616        0.07                     6.3

  GX1+4         10614        0.06        -3.0         5.6

  VELAX-1       10614        0.06        -3.7         4.9

  GROJ1744-28   10614        0.10        -4.2         4.7
                10615        0.08                     4.0

  GRS1758-258   10614        0.03        -2.0         4.3
                10616        0.03                     3.2

  SMCX-1        10614        0.02        -2.0         3.9
                10615        0.01                     3.1

  CYGX-3        10614        0.03        -3.3         3.8


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

           **Detection Significance, = Flux/Sigma

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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).