INTEGRAL Galactic Plane Scanning
Revolution 1241: Observation start 2012-12-11T12:21 = MJD 56272.515
Total Observation GTI = 34481 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-3 308.100 +40.958 0.5 79.843 +0.704 34.1 0.39 87.2 7.7 0.29 26.6 Cyg X-1 299.598 +35.201 0.9 71.337 +3.061 16.5 0.44 37.6 5.4 0.32 17.0 Cyg X-2 326.206 +38.347 2.9 87.366 -11.315 8.0 0.88 9.1 0.0 0.00 0.0 3A 2206+543 331.864 +54.530 3.6 100.553 -1.056 2.2 0.30 7.1 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 A(cps) sigma
==================== ============= ============= ============= =============
3A 2206+543 3.3198807E+02 5.4526047E+01 3.8460729E-01 2.8016356E+01
Cas A 3.5085974E+02 5.8819344E+01 4.5308352E-01 1.8805365E+01
Cyg X-1 2.9959311E+02 3.5202019E+01 8.1928949E+00 1.6054881E+02