Revolution 2717: Observation start 2023-12-07T03:38 = MJD 60285.152
Total Observation GTI = 75930 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 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 J16024-6107 240.638 -61.168 0.0 323.992 -6.376 3721 0.00 57.8 0.0 0.00 0.0
GX 301-2 186.666 -62.775 0.7 300.103 -0.039 5.9 0.12 50.1 1.1 0.15 7.4
IGR J16056-6110 241.521 -61.174 0.0 324.307 -6.664 2346 0.00 22.2 0.0 0.00 0.0
Cen X-3 170.323 -60.628 1.7 292.097 +0.333 1.9 0.12 16.3 0.0 0.00 0.0
4U 1323-62 201.670 -62.197 3.3 307.029 +0.394 1.3 0.17 7.9 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 1.7030975E+02 -6.0622852E+01 1.5967960E-02 2.7790744E+02
GX 301-2 1.8664517E+02 -6.2768837E+01 6.7616198E-03 1.4589113E+02
1H 1254-690 1.9442807E+02 -6.9286781E+01 2.1545598E-03 3.7488346E+01
1E 1145.1-6141 1.7686989E+02 -6.1959541E+01 6.3425465E-04 1.6648232E+01
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