Revolution 1610: Observation start 2015-11-14T09:35 = MJD 57340.4
Total Observation GTI = 30502 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 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
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Vela X-1 135.520 -40.544 0.8 263.046 +3.932 26.3 0.60 43.7 6.3 0.40 15.6
H 0614+091 94.307 +9.173 0.0 200.858 -3.323 7.9 0.00 5.6 0.0 0.00 0.0
JEM-X

JEM-X1 and JEM-X2 significance mosaic images in 3-10 keV energy band.
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
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