Revolution 1454

Observation start: 2014-09-09T15:06 = MJD 56909.63
Total Observation GTI = 14625 seconds

ISGRI

1454ss_isgri_mosa1.png1454ss_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            273.750  -12.106 2.2   18.012   +2.415    4.2   0.3  12.5    3.2   0.2  13.3
AX J1736.4-2910       264.123  -29.067 4.9  358.833   +1.624   21.0   4.2   5.0    0.0   0.0   0.0
GRS 1758-258          270.306  -25.754 1.5    4.501   -1.370   12.7   0.7  18.4    9.5   0.5  20.7
GX 1+4                263.028  -24.766 3.8    1.929   +4.769    9.1   1.4   6.6    0.0   0.0   0.0
GX 17+2               274.001  -14.031 1.1   16.434   +1.284    8.5   0.3  27.7    0.0   0.0   0.0
GX 9+1                270.464  -20.506 3.9    9.134   +1.100    2.8   0.4   6.5    0.0   0.0   0.0
Ginga 1826-24         277.364  -23.801 0.9    9.267   -6.087   19.6   0.5  37.5    8.0   0.4  22.2
H 1820-303            275.823  -30.399 4.0    2.717   -7.857   27.5   4.3   6.4    0.0   0.0   0.0
HETE J1900.1-2455     285.069  -24.921 3.9   11.317  -12.900    6.4   1.0   6.4    3.2   0.6   5.1
IGR J18193-2542       274.876  -25.662 4.5    6.563   -4.937    3.6   0.7   5.6    0.0   0.0   0.0
NEW_1                 273.343  -12.152 0.0   17.782   +2.743    2.3   0.0   6.8    0.0   0.0   0.0
NEW_2                 274.403  -12.616 4.2   17.866   +1.612    1.9   0.3   6.0    0.0   0.0   0.0
NEW_3                 271.826  -12.829 4.1   16.474   +3.717    2.1   0.3   6.2    0.0   0.0   0.0
NEW_4                 273.261  -13.948 5.3   16.165   +1.955    1.4   0.3   4.7    0.0   0.0   0.0
SAX J1818.6-1703      274.633  -17.032 1.9   14.083   -0.676    5.0   0.3  14.5    2.0   0.3   8.1
SLX 1744-300          266.844  -30.100 3.9  359.204   -0.931   41.5   6.4   6.5    0.0   0.0   0.0
SWIFT J1753.5-0127    268.395   -1.490 3.9   24.877  +12.144    7.1   1.1   6.5    5.4   0.8   7.1
XTE J1748-288         266.976  -28.365 4.0    0.748   -0.132   14.6   0.0   6.2    0.0   0.0   0.0
XTE J1855-026         283.905   -2.572 4.3   31.118   -2.103    5.4   0.9   5.8    0.0   0.0   0.0

JEM-X

1454ss_jemx_mosa1.png1454ss_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 13+1               273.630  -17.153   13.519   +0.109    0.3   0.0  84.7   0.0   0.0   12.1 
GX 17+2               274.011  -14.031   16.439   +1.275    0.7   0.0 232.8   0.1   0.0   67.4 

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