INTEGRAL Galactic Plane Scanning

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

Revolution 2649: Observation start 2023-06-08T17:31 = MJD 60103.731
Total Observation GTI = 46588 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 OSA10.2, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 208 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 100 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              135.503  -40.558 2.2  263.048   +3.913   12.3  1.00  12.3    0.0  0.00   0.0
GX 301-2              186.705  -62.765 2.7  300.120   -0.027    8.6  0.88   9.8    0.0  0.00   0.0
IGR J11502-5427       177.479  -54.517 4.5  294.003   +7.284    1.4  0.26   5.5    0.0  0.00   0.0
1E 1145.1-6141        176.954  -62.026 4.6  295.546   -0.070    1.3  0.24   5.4    0.0  0.00   0.0

JEM-X Detected Sources 3-10 keV

Sources 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.

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    Source Name             RA             dec            A(cps)          sigma  
====================   =============   =============   =============   ============= 

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