Revolution 1316b: Observation start 2013-07-25T08:00 = MJD 56498.334
Total Observation GTI = 53193 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-1 299.592 +35.198 0.5 71.332 +3.064 34.4 0.37 91.9 9.6 0.27 36.2
Cyg X-3 308.104 +40.956 0.5 79.842 +0.701 22.3 0.31 72.5 5.3 0.22 24.2
Cyg X-2 326.154 +38.342 2.5 87.332 -11.292 6.0 0.56 10.6 0.0 0.00 0.0
IGR J21247+5058 321.092 +50.956 3.2 93.274 +0.412 2.4 0.30 8.2 0.0 0.00 0.0
3A 0114+650 19.517 +65.328 4.0 125.709 +2.599 1.9 0.31 6.2 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 0114+650 1.9536209E+01 6.5288734E+01 2.7519578E-01 1.3719299E+01
gam Cas 1.4144072E+01 6.0717457E+01 2.2716406E-01 1.1532056E+01
Cas A 3.5087048E+02 5.8815823E+01 4.3433353E-01 2.9938232E+01
Cyg X-1 2.9959171E+02 3.5200684E+01 1.3367718E+01 3.6787317E+02
Cyg X-3 3.0810959E+02 4.0955502E+01 4.6553340E+00 1.6302808E+02
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