INTEGRAL Galactic Plane Scanning
Revolution 1059a: Observation start 2011-06-16T02:52 = MJD 55728.12
Total Observation GTI = 57090 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-1 299.586 +35.202 0.3 71.334 +3.070 103.0 0.36 288.0 63.2 0.28 226.5 Cyg X-3 308.112 +40.958 0.5 79.848 +0.697 26.9 0.36 74.9 5.8 0.29 19.9 H 0115+634 19.645 +63.748 0.6 125.928 +1.034 22.7 0.36 63.7 0.0 0.00 0.0 GRS 1915+105 288.792 +10.949 0.6 45.366 -0.213 62.2 0.96 65.0 0.0 0.00 0.0 Cyg X-2 326.081 +38.337 2.3 87.284 -11.258 6.6 0.56 11.7 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 (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 ==================== ======== ======== ======== ======== ====== ===== Cyg X-3 308.103 +40.956 79.842 +0.702 9.71 154.7 Cyg X-1 299.587 +35.203 71.335 +3.070 59.6 77.48 H 0115+634 19.6363 +63.738 125.92 +1.025 3.66 80.40 gam Cas 14.1718 +60.707 123.57 -2.148 0.19 10.06 3A 2206+543 332.012 +54.474 100.59 -1.151 0.21 59.35