Revolution 1049a: Observation start 2011-05-17T06:
59 = MJD 55698.292
Total Observation GTI = 37023 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 ~ 207 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 103 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-1 135.534 -40.557 0.5 263.062 +3.931 38.6 0.50 77.5 4.2 0.40 10.4
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 with j_ima_src_locator
in 3-10 keV energy band.
.
Source Name RA dec l b A(cps) +/-
==================== ======== ======== ======== ======== ====== =====
Go back to the INTEGRAL Galactic bulge home page