Revolution 1225

Observation start: 2012-10-25T10:27 = MJD 56225.436
Total Observation GTI = 12435 seconds

ISGRI

1225ss_isgri_mosa1.png1225ss_isgri_mosa2.png

ISGRI significance mosaic images in Galactic coordinates. Left: ISGRI 18-40 keV. Right: 40-100 keV. The scaling is zscale limiting the significance to the range of 4 to 20. Sources detected > 6σ 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, of all 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. The table is constructed from the isgri_mosa_res.fits file - fluxes in the mosaic output are known to be systematically ~10% lower than in the ScW light-curves (see known issues). The systematic noise increases towards the edge of the field of view and NEW sources towards the border of the image may be spurious.

ISGRI detected sources 18-40 keV (A) and 40-100 keV (B):

Source Name             RA       dec   +/-    l        b     A(cps)  +/-   sig  B(cps)  +/-   sig  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
4U 1812-12            273.783  -12.090 2.0   18.042   +2.394    4.5   0.3  13.4    2.3   0.3   8.8
AX J1748.7-2709       267.229  -27.152 6.3    1.902   +0.302   18.8   4.9   3.9    8.8   3.1   2.8
AX J1753.5-2745       268.481  -27.796 0.0    1.917   -0.981   32.2   0.0   4.3    0.0   0.0   0.0
GRS 1758-258          270.378  -25.709 0.0    4.572   -1.404    7.2   0.0   4.6    0.0   0.0   0.0
GX 13+1               273.663  -17.122 2.6   13.562   +0.097    3.8   0.4  10.1    0.0   0.0   0.0
GX 17+2               274.008  -14.040 2.1   16.430   +1.274    4.1   0.3  13.0    0.0   0.0   0.0
GX 5-1                270.245  -25.077 4.2    5.062   -0.987    9.3   1.5   6.1    0.0   0.0   0.0
GX 9+1                270.339  -20.629 0.0    8.968   +1.141    3.0   0.0   5.5    0.0   0.0   0.0
Ginga 1826-24         277.374  -23.798 1.5    9.275   -6.094   16.8   0.9  19.3    5.6   0.6   9.1
IGR J18179-1621       274.514  -16.471 5.8   14.522   -0.310    1.3   0.0   4.2    0.0   0.0   0.0
IGR J18532+0416       283.328   +4.347 5.9   37.015   +1.565    8.8   2.1   4.2    0.0   0.0   0.0
NEW_1                 290.088   +4.249 3.5   40.028   -4.467   39.8   5.5   7.3    9.9   1.9   5.1
SAX J1806.5-2215      271.593  -22.290 4.4    8.096   -0.692    3.4   0.6   5.7    2.3   0.5   5.2
SWIFT J1753.5-0127    268.367   -1.472 1.9   24.879  +12.177    9.6   0.7  14.5    7.5   0.5  14.8
SWIFT J1816.7-1613    274.177  -16.240 5.8   14.572   +0.084    1.5   0.4   4.2    0.0   0.0   0.0
SWIFT J1910.2-0546    287.604   -5.797 1.6   29.908   -6.852    9.7   0.6  17.2    6.6   0.4  16.0
Swift J174510.8-2624  266.308  -26.423 1.5    2.100   +1.384   80.0   4.1  19.5   28.2   2.6  10.9
XTE J1855-026         283.865   -2.663 4.9   31.019   -2.108    2.4   0.5   5.0    0.0   0.0   0.0

JEM-X

1225ss_jemx_mosa1.png1225ss_jemx_mosa2.png

Combined JEM-X1/2 significance mosaic images in Galactic coordinates. Left: 3-10 keV. Right: 10-25 keV. Sources labeled were detected in the 3-10 keV image > 5σ and are listed in the table below. Fluxes are extracted at the known catalog position of the source (i.e. no fitting of the source position is done), with mosaic_spec, in two bands: A = 3-10 keV (1 Crab ~ 173 cps) and B = 10-25 keV (1 Crab ~ 71 cps).

JEM-X detected sources in 3-10 keV (A) and 10-25 keV (B):

Source Name             RA       dec      l        b     A(cps)  +/-   sig  B(cps)  +/-   sig  
==================== ========  ======= ======== ======== ====== ===== ===== ====== ===== =====
GX 17+2               274.003  -14.033   16.434   +1.282  144.4   1.1 125.7  14.7   0.6   24.9 

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