Revolution 1508

Observation start: 2015-02-16T08:44 = MJD 57069.365
Total Observation GTI = 24259 seconds

ISGRI

1508ss_isgri_mosa1.png1508ss_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  
==================== ========  ======= === ====== ===== ===== ====== ===== =====
3A 1728-169           262.982  -16.945 5.8   2.4   0.6   4.2    0.0   0.0   0.0
3A 1850-087           283.265   -8.760 4.2   1.6   0.3   6.0    0.0   0.0   0.0
4U 1812-12            273.768  -12.094 1.4   4.0   0.2  20.2    2.2   0.2  14.4
AX J1808.2-2021       272.007  -20.389 6.3   1.1   0.3   3.8    0.0   0.0   0.0
AX J1833.7-0828       278.411   -8.399 5.2   1.0   0.2   4.7    0.0   0.0   0.0
Aql X-1               287.845   +0.584 3.2  14.1   1.7   8.2    5.5   1.2   4.7
GRO J1750-27          267.341  -26.683 3.9  11.0   1.7   6.5    0.0   0.0   0.0
GRS 1758-258          270.304  -25.740 1.8  12.0   0.8  15.7    8.6   0.5  16.3
GX 1+4                263.017  -24.810 3.4  12.3   1.6   7.5    0.0   0.0   0.0
GX 13+1               273.653  -17.193 4.0   1.4   0.2   6.2    0.0   0.0   0.0
GX 17+2               274.016  -14.020 1.4   4.1   0.2  20.3    0.0   0.0   0.0
GX 5-1                270.331  -25.070 4.1   4.3   0.7   6.1    0.0   0.0   0.0
GX 9+1                270.352  -20.490 0.0   1.6   0.0   5.4    0.0   0.0   0.0
Ginga 1826-24         277.370  -23.796 0.7  20.1   0.4  49.7    7.6   0.3  26.0
H 1745-203            267.246  -20.358 3.4   3.0   0.4   7.4    1.6   0.3   5.4
HETE J1900.1-2455     285.012  -24.896 3.4   5.0   0.7   7.5    3.2   0.5   7.0
IGR J17303-0601       262.508   -5.992 4.3   5.3   0.9   5.8    0.0   0.0   0.0
IGR J17348-2045       263.700  -20.854 5.8   2.5   0.0   4.2    0.0   0.0   0.0
NEW_1                 267.562  -11.241 4.8   1.5   0.3   5.2    0.0   0.0   0.0
SAX J1806.5-2215      271.647  -22.340 4.6   1.9   0.4   5.4    0.0   0.0   0.0
SNR 021.5-00.9        278.492  -10.570 5.6   0.9   0.2   4.4    0.0   0.0   0.0
SWIFT J1753.5-0127    268.401   -1.413 3.1   4.2   0.5   8.3    2.3   0.4   6.3
XTE J1806-246         271.717  -24.535 5.4   2.3   0.5   4.5    0.0   0.0   0.0
XTE J1855-026         283.851   -2.631 2.5   4.9   0.5  10.6    0.0   0.0   0.0

JEM-X

1508ss_jemx_mosa1.png1508ss_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               273.624  -17.144  30.5   0.5  58.5   2.3   0.3    8.3 
GX 17+2               274.005  -14.040  62.7   0.2 272.6   7.9   0.1   69.3 

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