Revolution 1127: Observation start 2012-01-06T02:45 = MJD 55932.115
Total Observation GTI = 39134 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-1 299.598 +35.206 0.5 0.000 +0.000 147.5 1.86 79.4 90.9 1.33 68.6
Cyg X-3 308.103 +40.957 0.7 0.000 +0.000 40.4 0.75 53.7 8.8 0.58 15.1
EXO 2030+375 308.101 +37.631 0.0 0.000 +0.000 5.3 0.00 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 A(cps) sigma
==================== ============= ============= ============= =============
gam Cas 1.4164658E+01 6.0717052E+01 1.3520861E-01 5.3205514E+00
Cas A 3.5087079E+02 5.8827469E+01 4.5394823E-01 2.2059271E+01
3A 2206+543 3.3198856E+02 5.4520733E+01 1.8264125E-01 1.0516994E+01
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