Revolution 2809: Observation start 2024-08-08T07:39 = MJD 60530.319
Total Observation GTI = 48265 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
4U 2238+60 339.882 61.280 2.0 339.415 +61.019 9.2 0.6 15.0 0.8 0.1 8.0
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
==================== ============= ============= ============= =============
4U 2238+60 3.3985406E+02 6.1271889E+01 1.2092970E-03 3.0063309E+01
3A 2206+543 3.3198126E+02 5.4515415E+01 6.7104097E-04 2.0939089E+01
Cas A 3.5083078E+02 5.8808746E+01 1.1868837E-03 1.4444850E+01
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