INTEGRAL Galactic Plane Scanning

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

Revolution 1607: Observation start 2015-11-05T20:15 = MJD 57331.845
Total Observation GTI = 42024 seconds

ISGRI

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               299.593  +35.197 0.3   71.332   +3.062   65.9  0.42 155.3   36.3  0.27 133.5
Cyg X-3               308.108  +40.952 0.5   79.841   +0.696   32.9  0.41  80.0    9.0  0.26  34.4
H 0115+634             19.615  +63.735 1.0  125.916   +1.020   28.0  0.94  29.7    0.0  0.00   0.0
GRS 1915+105          288.802  +10.976 1.8   45.394   -0.209   13.4  0.84  15.9    0.0  0.00   0.0
1ES 1959+650          299.876  +65.201 4.2   98.029  +17.740   15.4  0.00   6.0    0.0  0.00   0.0
IGR J21247+5058       321.259  +50.940 4.0   93.339   +0.328    2.1  0.33   6.3    0.0  0.00   0.0

JEM-X

Fluxes are extracted at the known catalogue position of the source (i.e. no fitting of the source position is done), with j_ima_src_locator in 3-10 keV energy band.

    Source Name             RA             dec            A(cps)          sigma  
====================   =============   =============   =============   ============= 
Cas A                  3.5083041E+02   5.8822220E+01   1.7339583E-03   1.4273587E+01
Cyg X-1                2.9958600E+02   3.5201843E+01   3.3365872E-02   1.0935499E+02

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