INTEGRAL Galactic Plane Scanning

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

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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