INTEGRAL Galactic Plane Scanning

******************* Very Preliminary results ******************

Revolution 1365b: Observation start 2013-12-19T10:07 = MJD 56645.422
Total Observation GTI = 46930 seconds

ISGRI

1365b_isgri_mosa1.jpg1365b_isgri_mosa2.jpg

ISGRI significance mosaic images. Top: ISGRI 18-40 keV. Bottom: 40-100 keV
Sources detected > 10σ in each band are marked on the image. The table below lists the fitted position, and statistical positional uncertainty in arcmin returned by the mosaic step of OSA9, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 176 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 88 cps ) where available.

ISGRI Detected Sources 18-40 keV (A) and 40-100 keV (B)

Source Name             RA       dec   +/-    l        b     A(cps)  +/-   sig  B(cps)  +/-   sig  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
Cyg X-1               299.590  +35.204 0.4   71.337   +3.068   38.2  0.29 133.7   14.3  0.19  74.3
KS 1947+300           297.402  +30.208 0.5   66.099   +2.080   26.8  0.31  86.8    0.0  0.00   0.0
Cyg X-3               308.115  +40.955 0.5   79.846   +0.694   26.0  0.31  83.5    5.8  0.22  26.6
3A 1954+319           298.931  +32.106 1.1   68.402   +1.928   10.1  0.38  26.4    0.0  0.00   0.0
Cyg X-2               326.173  +38.341 1.8   87.342  -11.302    8.6  0.55  15.6    0.0  0.00   0.0
==================== ============= ============= ======


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