INTEGRAL Galactic Plane Scanning

******************* Very Preliminary results ******************

Revolution 1051b: Observation start 2011-05-25T03:15 = MJD 55706.136
Total Observation GTI = 54034 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 ~ 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              135.527  -40.555 0.3  263.058   +3.929   71.8  0.27 265.5    7.7  0.21  36.6
Cen X-3               170.317  -60.624 1.3  292.093   +0.336   18.4  0.83  22.0    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 with j_ima_src_locator in 3-10 keV energy band.

Source Name             RA      dec       l        b     A(cps)  +/-  
==================== ======== ======== ======== ======== ====== ===== 
Vela X-1             135.527  -40.555  263.058   +3.929  2.53   0.04
H 0918-549           140.1102 -55.206  275.852   -3.845  0.51   0.01
Vela Pulsar          128.8360 -45.176  263.551   -2.787  0.08   0.01

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