Revolution 2713: Observation start 2023-11-26T09:48 = MJD 60274.409
Total Observation GTI = 90721 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-1 135.537 -40.570 1.0 263.074 +3.925 5.6 0.17 32.7 1.4 0.21 6.7
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 1.3552628E+02 -4.0553024E+01 6.0441946E-03 3.9300602E+01
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