Revolution 1227

Observation start: 2012-10-30T14:51 = MJD 56230.619
Total Observation GTI = 24797 seconds

ISGRI

1227ss_isgri_mosa1.png1227ss_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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
2EG J1825-1307        276.568  -13.661 5.2   17.935   -0.740    1.1   0.2   4.8    0.0   0.0   0.0
3A 1850-087           283.292   -8.716 5.1   25.356   -4.344    1.2   0.2   4.8    0.0   0.0   0.0
4U 1812-12            273.784  -12.094 1.3   18.038   +2.391    5.9   0.3  23.3    3.2   0.2  16.8
AX J1838.0-0655       279.571   -6.938 5.2   25.261   -0.252    1.0   0.2   4.7    0.0   0.0   0.0
AX J1907.8+0803       286.884   +8.020 6.6   41.899   +0.101    8.9   2.4   3.6    0.0   0.0   0.0
GX 17+2               274.009  -14.042 1.3   16.428   +1.272    6.0   0.3  22.2    0.0   0.0   0.0
GX 3+1                266.962  -26.635 0.0    2.223   +0.773  129.8   0.0   4.0    0.0   0.0   0.0
GX 5-1                270.332  -25.138 4.7    5.047   -1.085   17.6   3.3   5.3    0.0   0.0   0.0
GX 9+1                270.290  -20.594 5.0    8.976   +1.198    3.0   0.6   5.0    0.0   0.0   0.0
Ginga 1826-24         277.365  -23.786 2.1    9.281   -6.080   17.9   1.4  12.8    8.6   0.9   9.1
Ginga 1843+009        281.388   +0.768 0.0   32.945   +1.660    1.3   0.0   4.2    0.0   0.0   0.0
IGR J17536-2339       268.323  -23.686 0.0    5.388   +1.225    6.6   0.0   4.0    0.0   0.0   0.0
IGR J19173+0747       289.281   +7.782 5.1   42.787   -2.114   16.8   3.5   4.8    0.0   0.0   0.0
SAX J1806.5-2215      271.668  -22.220 4.3    8.191   -0.717    4.3   0.7   5.9    0.0   0.0   0.0
SGR 1806-20           272.146  -20.397 5.9   10.000   -0.220    2.1   0.5   4.2    0.0   0.0   0.0
SWIFT J1753.5-0127    268.361   -1.457 1.1   24.890  +12.189   13.8   0.5  28.6    8.4   0.3  24.1
SWIFT J1910.2-0546    287.608   -5.800 1.3   29.908   -6.856    8.3   0.4  23.4    5.2   0.3  20.4
XTE J1855-026         283.848   -2.637 2.9   31.034   -2.082    2.6   0.3   9.0    1.4   0.2   6.5

JEM-X

1227ss_jemx_mosa1.png1227ss_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               274.004  -14.038   16.430   +1.279  142.3   5.1  28.0  22.2   3.3    6.7 

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