Revolution 1318

Observation start: 2013-07-30T04:56 = MJD 56503.206
Total Observation GTI = 12461 seconds

ISGRI

1318np_isgri_mosa1.png1318np_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 1700-377           255.982  -37.845 0.5  347.752   +2.176   44.6   0.6  77.6   12.9   0.4  32.8
4U 1735-444           264.847  -44.441 5.6  346.101   -7.052    2.7   0.6   4.4    0.0   0.0   0.0
AX J1700.2-4220       254.962  -42.350 6.8  343.712   +0.033    1.3   0.4   3.5    0.0   0.0   0.0
GPS 1742-326          266.311  -32.721 5.8  356.727   -1.904   38.8   9.2   4.2    0.0   0.0   0.0
GX 340+0              251.430  -45.615 2.3  339.577   -0.072    3.8   0.3  11.9    0.0   0.0   0.0
GX 349+2              256.394  -36.428 3.3  349.079   +2.772    5.5   0.7   7.8    0.0   0.0   0.0
H 1538-522            235.621  -52.397 3.1  327.425   +2.146    4.2   0.5   8.3    0.0   0.0   0.0
H 1636-536            250.204  -53.768 1.5  332.892   -4.816    7.0   0.4  18.6    3.3   0.3  12.3
H 1702-429            256.578  -43.006 2.1  343.917   -1.309    4.8   0.4  12.9    1.4   0.0   5.2
H 1705-440            257.199  -44.089 2.7  343.319   -2.318    3.7   0.4   9.9    0.0   0.0   0.0
IGR J15479-4529       236.949  -45.459 5.1  332.390   +7.087    2.1   0.4   4.8    0.0   0.0   0.0
IGR J16195-4945       244.937  -49.809 4.5  333.534   +0.267    1.8   0.3   5.6    0.0   0.0   0.0
IGR J16293-4603       247.191  -45.957 5.8  337.340   +1.891    1.3   0.0   4.2    0.0   0.0   0.0
IGR J16318-4848       247.947  -48.818 2.1  335.613   -0.447    3.5   0.3  12.7    1.3   0.2   5.9
OAO 1657-415          255.210  -41.655 0.4  344.373   +0.316   41.4   0.4 103.5   12.9   0.3  45.8
SGR 1627-41           248.880  -47.663 5.1  336.883   -0.118    1.5   0.3   4.8    0.0   0.0   0.0
XTE J1701-407         255.299  -40.867 5.0  345.035   +0.748    2.0   0.0   5.0    0.0   0.0   0.0

JEM-X

1318np_jemx_mosa1.png1318np_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  
==================== ========  ======= ======== ======== ====== ===== ===== ====== ===== =====
4U 1630-47            248.519  -47.396  336.915   +0.242    0.1   0.0  57.3   0.0   0.0    1.8 
GX 340+0              251.454  -45.607  339.594   -0.080    0.6   0.0 183.6   0.1   0.0   39.7 
H 1624-490            247.022  -49.190  334.926   -0.262    0.1   0.0  31.0   0.0   0.0    4.5 
H 1705-440            257.240  -44.100  343.328   -2.349    0.5   0.0  24.3   0.1   0.0    5.2 

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