Revolution 1511

Observation start: 2015-02-24T19:51 = MJD 57077.827
Total Observation GTI = 12179 seconds

ISGRI

1511ss_isgri_mosa1.png1511ss_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   +/- A(cps)  +/-   sig  B(cps)  +/-   sig  
==================== ========  ======= === ====== ===== ===== ====== ===== =====
2EG J1825-1307        276.634  -13.638 6.2   1.1   0.3   3.9    0.0   0.0   0.0
3EG J1744-0310        266.034   -3.822 0.0   3.8   0.0   4.4    0.0   0.0   0.0
3EG J1810-1032        272.441  -10.419 0.0   1.5   0.0   4.6    0.0   0.0   0.0
4U 1807-10            272.727  -10.870 7.4   1.0   0.3   3.2    0.0   0.0   0.0
4U 1812-12            273.778  -12.096 1.9   4.4   0.3  14.5    2.4   0.2  10.6
AX J1742.6-2901       265.610  -29.033 0.0  24.5   0.0   4.5    0.0   0.0   0.0
GRO J1750-27          267.329  -26.596 2.4  15.1   1.4  11.1    0.0   0.0   0.0
GRS 1739-278          265.696  -27.846 6.8   7.4   2.1   3.6    0.0   0.0   0.0
GRS 1758-258          270.305  -25.738 1.8  11.8   0.8  15.0    6.4   0.5  12.0
GX 1+4                262.978  -24.742 2.6  14.8   1.4  10.3    0.0   0.0   0.0
GX 13+1               273.552  -17.083 4.7   1.6   0.3   5.2    0.0   0.0   0.0
GX 17+2               274.004  -14.034 0.8  12.2   0.3  43.0    0.0   0.0   0.0
GX 9+1                270.418  -20.533 4.7   2.0   0.4   5.3    0.0   0.0   0.0
Ginga 1826-24         277.370  -23.795 0.8  19.8   0.5  40.5    7.4   0.3  21.6
H 1745-203            267.220  -20.364 1.0  16.3   0.5  29.7    4.7   0.4  12.3
HESS J1834-087        278.769   -8.772 6.1   1.3   0.3   4.0    0.0   0.0   0.0
HETE J1900.1-2455     285.068  -24.865 2.9   7.5   0.8   9.2    2.8   0.6   4.8
IGR J17586-2129       269.670  -21.361 5.4   2.0   0.4   4.5    0.0   0.0   0.0
IGR J18027-2016       270.743  -20.297 0.0   1.4   0.0   3.9    0.0   0.0   0.0
IGR J18079-0921       272.047   -9.382 6.9   1.2   0.3   3.5    0.0   0.0   0.0
IGR J18129-0649       273.282   -6.839 5.6   1.6   0.4   4.4    0.0   0.0   0.0
IGR J18151-1052       273.772  -10.757 5.9   1.3   0.0   4.1    0.0   0.0   0.0
PDS 456               262.038  -14.306 5.5   3.7   0.8   4.4    0.0   0.0   0.0
RX J1744.7-2713       266.167  -27.337 5.3   7.1   1.5   4.7    0.0   0.0   0.0
SAX J1806.5-2215      271.634  -22.230 3.5   3.3   0.5   7.4    1.7   0.3   5.1
SNR 021.5-00.9        278.457  -10.625 4.7   1.6   0.3   5.2    1.0   0.2   4.6

JEM-X

1511ss_jemx_mosa1.png1511ss_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   A(cps)  +/-   sig  B(cps)  +/-   sig  
==================== ========  ======= ====== ===== ===== ====== ===== =====
GX 13+1               273.635  -17.157  31.1   0.5  60.8   2.1   0.3    8.4 
GX 17+2               274.003  -14.035 113.0   0.4 309.6  21.8   0.2  122.1 

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