Revolution 1917: Observation start 2018-02-07T05:45 = MJD 58156.24
Total Observation GTI = 28505 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
AX J1620.1-5002 245.108 -50.030 1.8 333.458 +0.033 5.4 0.36 15.2 2.3 0.32 7.3
4U 1626-67 247.926 -67.448 3.2 321.761 -13.042 3.4 0.41 8.2 0.0 0.00 0.0
Circinus Galaxy 213.374 -65.323 3.0 311.364 -3.803 2.2 0.26 8.8 0.0 0.00 0.0
4U 1543-624 236.922 -62.563 3.6 321.740 -6.317 1.4 0.20 7.1 0.0 0.00 0.0
IGR J16318-4848 247.997 -48.818 3.9 335.636 -0.470 3.4 0.53 6.5 0.0 0.00 0.0
GX 301-2 186.672 -62.740 4.4 300.102 -0.005 8.2 0.00 5.6 0.0 0.00 0.0
JEM-X Detected Sources 3-10 keV
Note: Sources labelled 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
==================== ============= ============= ============= =============
Cir X-1 2.3016214E+02 -5.7163757E+01 5.9752655E-04 8.4750671E+00
PSR B1509-58 2.2846629E+02 -5.9126678E+01 4.8646715E-04 6.0515046E+00
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