Revolution 2448: Observation start 2021-12-21T03:19 = MJD 59569.139
Total Observation GTI = 48321 seconds
ISGRI
![2448_isgri_mosa1.jpg](2448_isgri_mosa1.jpg)
![2448_isgri_mosa2.jpg](2448_isgri_mosa2.jpg)
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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GX 301-2 186.661 -62.764 1.2 300.100 -0.029 3.2 0.13 24.9 0.0 0.00 0.0
Circinus Galaxy 213.405 -65.308 4.2 311.381 -3.793 1.2 0.20 5.9 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
==================== ============= ============= ============= =============
GX 301-2 1.8664407E+02 -6.2771656E+01 2.9192888E-03 6.2784199E+01
1H 1254-690 1.9443459E+02 -6.9285965E+01 2.1899864E-03 2.3587854E+01
4U 1323-62 2.0166957E+02 -6.2141949E+01 4.4595424E-04 8.7083063E+00
4U 1210-64 1.8329414E+02 -6.4874039E+01 5.4003857E-04 8.3218355E+00
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