INTEGRAL Galactic Plane Scanning
Revolution 1051a: Observation start 2011-05-23T08:17 = MJD 55704.346
Total Observation GTI = 30615 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 ~ 207 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 103 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-1 299.589 +35.203 0.2 71.336 +3.069 183.3 0.44 416.3 94.5 0.34 279.1 GRS 1915+105 288.796 +10.948 0.3 45.367 -0.216 93.3 0.41 229.3 0.0 0.00 0.0 Cyg X-3 308.098 +40.959 0.7 79.842 +0.706 25.7 0.48 53.8 6.5 0.37 17.3 EXO 2030+375 308.050 +37.642 1.4 77.149 -1.230 11.1 0.55 20.1 0.0 0.00 0.0 4U 1909+07 287.710 +7.633 3.4 41.933 -0.804 3.1 0.41 7.6 0.0 0.00 0.0 3A 2206+543 331.967 +54.547 3.5 100.612 -1.077 4.7 0.63 7.4 0.0 0.00 0.0 SS 433 287.918 +5.001 3.6 39.693 -2.202 2.7 0.38 7.1 0.0 0.00 0.0 IGR J19113+1533 287.806 +15.595 4.4 49.041 +2.790 2.6 0.44 5.7 0.0 0.00 0.0
JEM-X
JEM-X1 and JEM-X2 significance mosaic images in 3-10 keV energy band.
Note: Sources labelled were detected in the 3-10 keV image > 5σ and are listed in the table below. Fluxes are extracted at the known catalogue position of the source with
j_ima_src_locator in 3-10 keV energy band. .
Source Name RA dec l b A(cps) +/- ==================== ======== ======== ======== ======== ====== ===== Cyg X-1 299.589 +35.203 71.336 +3.069 17.39 0.06 IGR J19254+1047 294.404 +13.730 46.413 -2.509 0.12 0.02