Revolution 2564: Observation start 2022-10-25T22:00 = MJD 59877.917
Total Observation GTI = 98675 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
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Vela X-1 135.526 -40.551 0.4 263.054 +3.930 13.5 0.10 141.0 3.3 0.12 28.3
Vela Pulsar 128.794 -45.149 4.3 263.512 -2.795 0.5 0.09 5.8 0.6 0.11 5.7
Cen X-3 170.153 -60.659 4.3 292.029 +0.276 3.0 0.51 5.9 0.0 0.00 0.0
H 0918-549 140.165 -55.211 4.6 275.877 -3.826 0.5 0.09 5.4 0.5 0.00 4.1
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
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