Revolution 1048b: Observation start 201
1-05-16T08:28 = MJD 55697.353
Total Observation GTI = 40680 seconds
ISGRI


ISGRI significance mosaic images. Top: ISGRI 18-40 keV. Bottom: 40-100 keV
Sources dete
cted > 10σ in each band are marked on the image. The table below lists the fitted position, and statistical position
al uncertainty in arcmin returned by the mosaic step of OSA9
, of all the sources detected in the 18 - 40 keV
range (band A: 1 Crab ~ 176 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 88 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
Vela X-1 135.501 -40.565 1.4 263.052 +3.908 10.0 0.50 19.9 0.0 0.00 0.0
4U 0813-38 123.759 -38.760 5.6 256.130 -2.172 1.3 0.30 4.3 0.0 0.00 0.0
JEM-X

JEM-X1 and JEM-X2 significance mos
aic images in 3-10 keV energy band.
Note: Sources labelled were detected in the 3-10 keV image > 5σ and are l
isted in the table below. Fluxes are extracted at the known catalogue position of the source (i.e. no fitting of the sour
ce position is done), with j_ima_src_locator
in 3-10 keV energy band.
Source Name RA dec A(cps) sigma
==================== ============= ============= ============= =============
3EG J0747-3412 1.2086077E+02 -3.5113445E+01 9.8218091E-02 4.9672689E+00
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