Revolution 1257

Observation start: 2013-01-29T19:59 = MJD 56321.833
Total Observation GTI = 13641 seconds

ISGRI

1257np_isgri_mosa1.png1257np_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           255.983  -37.835 0.8  347.760   +2.181   64.6   1.4  44.8   21.1   0.9  22.8
AX J1651.0-4403       252.830  -44.077 5.7  341.393   +0.159    1.8   0.4   4.3    0.0   0.0   0.0
Cir X-1               230.171  -57.169 1.3  322.118   +0.035   10.9   0.5  23.3    3.2   0.4   8.7
GX 340+0              251.470  -45.604 4.4  339.603   -0.086    2.0   0.4   5.7    0.0   0.0   0.0
H 1538-522            235.569  -52.387 3.0  327.405   +2.174    2.8   0.3   8.8    0.0   0.0   0.0
H 1636-536            250.186  -53.741 2.0  332.905   -4.791    4.4   0.3  13.5    2.5   0.2  10.5
H 1705-440            257.245  -44.159 5.5  343.283   -2.386    2.6   0.6   4.5    0.0   0.0   0.0
IGR J14331-6112       218.130  -61.290 7.3  314.767   -0.762    6.6   2.0   3.3    0.0   0.0   0.0
IGR J14471-6414       221.712  -64.338 4.6  315.027   -4.212   10.6   0.0   5.4    0.0   0.0   0.0
IGR J16016-3431       240.347  -34.534 6.2  341.617  +13.706   29.2   7.4   3.9    0.0   0.0   0.0
IGR J16207-5129       245.172  -51.511 3.1  332.443   -1.048    2.4   0.3   8.3    0.0   0.0   0.0
IGR J16316-4028       247.933  -40.564 5.5  341.645   +5.196    2.6   0.0   4.5    0.0   0.0   0.0
IGR J16318-4848       247.938  -48.812 1.2  335.614   -0.438    7.8   0.3  25.3    3.1   0.2  13.5
IGR J16320-4751       248.040  -47.877 2.6  336.342   +0.151    3.1   0.3  10.2    0.0   0.0   0.0
IGR J16465-4507       251.586  -45.171 5.7  339.985   +0.133    1.7   0.4   4.3    0.0   0.0   0.0
IGR J17008-6425       255.287  -64.481 5.2  326.060  -13.534    6.8   1.4   4.7    0.0   0.0   0.0
NEW_1                 227.031  -64.034 4.2  317.224   -5.023    7.0   1.1   6.0    0.0   0.0   0.0
NEW_2                 226.157  -64.638 4.6  316.593   -5.360    8.6   1.5   5.4    0.0   0.0   0.0

JEM-X

1257np_jemx_mosa1.png1257np_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            248.495  -47.388  336.909   +0.259   78.5   1.0  74.8   2.3   0.6    4.1 
H 1624-490            247.008  -49.198  334.914   -0.260   14.7   0.4  39.2   1.6   0.3    6.4 

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