Revolution 2565: Observation start 2022-10-29T04:47 = MJD 59881.2
Total Observation GTI = 42320 seconds
ISGRI
![2565_isgri_mosa1.jpg](2565_isgri_mosa1.jpg)
![2565_isgri_mosa2.jpg](2565_isgri_mosa2.jpg)
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 OSA10.2
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 208 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 100 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
IGR J11435-6109 176.079 -61.159 3.7 294.926 +0.665 1.2 0.18 7.0 0.0 0.00 0.0
GX 301-2 186.710 -62.704 3.1 300.116 +0.034 3.2 0.38 8.3 2.2 0.46 4.9
1E 1145.1-6141 176.864 -61.915 3.9 295.478 +0.027 1.2 0.19 6.4 0.0 0.00 0.0
Vela X-1 135.564 -40.487 4.4 263.025 +3.994 34.4 6.11 5.6 0.0 0.00 0.0
Vela Pulsar 128.921 -45.266 4.8 263.659 -2.793 5.1 0.00 5.2 0.0 0.00 0.0
4U 1036-56 159.487 -56.829 3.9 285.410 +1.431 0.7 0.11 6.4 0.0 0.00 0.0
JEM-X Detected Sources 3-10 keV
Sources 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
==================== ============= ============= ============= =============
Cen X-3 1.7032150E+02 -6.0615227E+01 1.8428889E-03 1.8472673E+01
4U 1036-56 1.5939790E+02 -5.6799332E+01 4.6845229E-04 1.3027045E+01
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