INTEGRAL Galactic Plane Scanning

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

Revolution 1826: Observation start 2017-06-11T14:24 = MJD 57915.601
Total Observation GTI = 55417 seconds

ISGRI

1826_isgri_mosa1.jpg1826_isgri_mosa2.jpg

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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
GX 301-2              186.670  -62.779 0.7  300.105   -0.043    7.1  0.15  47.5    0.0  0.00   0.0
GRO J1008-57          152.436  -58.304 0.8  283.002   -1.834   10.4  0.25  41.3    1.8  0.23   7.9
Cen X-3               170.303  -60.627 1.0  292.087   +0.331    5.5  0.17  31.4    0.0  0.00   0.0
1E 1145.1-6141        176.855  -61.980 1.8  295.490   -0.037    2.5  0.16  15.7    0.7  0.14   5.1
4U 1036-56            159.378  -56.799 2.2  285.344   +1.428    2.8  0.23  12.0    0.0  0.00   0.0
Circinus Galaxy       213.275  -65.331 2.4  311.322   -3.798    2.4  0.21  11.0    0.0  0.00   0.0
4U 1323-62            201.639  -62.162 2.8  307.020   +0.431    1.5  0.16   9.5    0.0  0.00   0.0
IGR J12349-6434       188.851  -64.499 0.0  301.207   -1.681    0.8  0.00   5.4    0.0  0.00   0.0


Go back to the INTEGRAL Galactic Plane Scanning home page