Revolution 2782b: Observation start 2024-05-27T21:30 = MJD 60457.897
Total Observation GTI = 94927 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
Vela X-1 135.558 -40.528 2.6 263.053 +3.964 2.2 0.22 10.0 2.0 0.34 5.9
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
==================== ============= ============= ============= =============
Vela X-1 1.3554752E+02 -4.0552910E+01 7.4943580E-04 1.8629007E+01
Vela Pulsar 1.2885211E+02 -4.5176632E+01 3.4611244E-04 9.6008940E+00
H 0918-549 1.4010596E+02 -5.5201183E+01 1.0929190E-03 1.5725253E+01
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