INTEGRAL Galactic Plane Scanning
Revolution 1055a: Observation start 1999-12-31T23:58 = MJD 51544
Total Observation GTI = 55704 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-1 299.589 +35.204 0.3 71.336 +3.069 97.2 0.34 282.2 59.4 0.27 218.8 GRS 1915+105 288.798 +10.946 0.3 45.366 -0.219 89.0 0.57 155.8 0.0 0.00 0.0 Cyg X-3 308.105 +40.960 0.5 79.846 +0.703 26.0 0.31 83.8 5.2 0.29 18.1 EXO 2030+375 308.059 +37.627 1.7 77.142 -1.245 5.5 0.34 16.0 0.0 0.00 0.0 Cyg X-2 326.169 +38.295 2.0 87.309 -11.335 6.3 0.46 13.8 0.0 0.00 0.0 IGR J21247+5058 321.084 +51.007 4.4 93.306 +0.453 1.5 0.27 5.7 0.0 0.00 0.0 4U 0027+59 7.112 +59.215 4.2 119.988 -3.526 2.1 0.35 6.0 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 (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 l b A(cps) sigma ==================== ======== ======== ======== ======== ====== ===== Cas A 350.853 58.8230 111.73 -2.129 0.490 34.6 Cyg X-1 299.587 +35.203 71.335 +3.070 53.44 148.3 Cyg X-3 308.103 +40.956 79.842 +0.702 7.374 96.4 EXO 2030+375 308.061 +37.637 77.151 -1.240 0.557 14.9