Revolution 2664: Observation start 2023-07-17T22:58 = MJD 60142.957
Total Observation GTI = 46527 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
Cyg X-1 299.589 +35.200 0.3 71.333 +3.067 45.6 0.15 294.3 40.2 0.17 236.1
Cyg X-3 308.105 +40.961 0.7 79.847 +0.703 6.1 0.12 51.5 4.3 0.14 31.7
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
==================== ============= ============= ============= =============
Cyg X-3 3.0810938E+02 4.0955734E+01 1.0935110E-02 1.7819313E+02
Cyg X-1 2.9958817E+02 3.5197021E+01 2.4973666E-02 4.1808804E+01
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