Revolution 2316a: Observation start 2021-01-03T03:37 = MJD 59217.151
Total Observation GTI = 60590 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
3A 0114+650 19.497 +65.304 1.3 125.703 +2.575 3.2 0.14 22.8 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
==================== ============= ============= ============= =============
Cas A 3.5084869E+02 5.8823318E+01 8.1465160E-04 2.0605494E+01
3A 0114+650 1.9523735E+01 6.5300064E+01 1.0971314E-03 2.8176325E+01
Gam Cas 1.4182437E+01 6.0723164E+01 6.8358652E-04 1.9326445E+01
4U 0022+63 6.2912211E+00 6.4168526E+01 2.0370366E-04 5.2035089E+00
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