Revolution 1265

Observation start: 2013-02-21T07:16 = MJD 56344.303
Total Observation GTI = 9958 seconds

ISGRI

1265np_isgri_mosa1.png1265np_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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
3EG J1631-4033        247.660  -40.693 0.0  341.409   +5.260    1.9   0.0   4.2    0.0   0.0   0.0
3EG J1704-4732        256.020  -47.550 7.8  340.054   -3.741    1.2   0.4   3.1    0.0   0.0   0.0
4U 1630-47            248.484  -47.429 2.4  336.874   +0.237    3.8   0.3  11.1    1.1   0.3   4.3
4U 1735-444           264.595  -44.494 4.1  345.961   -6.927    6.0   1.0   6.1    0.0   0.0   0.0
AX J1657.1-4255       254.187  -42.840 6.5  342.973   +0.176    1.8   0.0   3.7    0.0   0.0   0.0
GX 340+0              251.440  -45.628 1.5  339.571   -0.086    6.8   0.4  18.8    0.0   0.0   0.0
GX 349+2              256.460  -36.371 4.6  349.157   +2.764    7.2   1.3   5.5    0.0   0.0   0.0
H 1636-536            250.256  -53.827 6.4  332.868   -4.879    1.5   0.4   3.8    0.0   0.0   0.0
H 1702-429            256.552  -43.028 1.3  343.888   -1.306   11.4   0.5  23.4    5.4   0.4  15.0
H 1705-440            257.207  -44.082 3.7  343.329   -2.319    3.8   0.5   6.9    0.0   0.0   0.0
IGR J16318-4848       248.005  -48.897 5.4  335.582   -0.528    1.4   0.3   4.5    0.0   0.0   0.0
IGR J16320-4751       248.085  -47.870 3.9  336.368   +0.134    2.2   0.3   6.6    0.0   0.0   0.0
IGR J16393-4643       249.813  -46.647 6.5  338.062   +0.092    1.4   0.4   3.7    0.0   0.0   0.0
IGR J16479-4514       252.034  -45.161 6.5  340.198   -0.101    1.5   0.4   3.7    0.0   0.0   0.0
NEW_1                 245.201  -36.649 4.4  343.014   +9.443    4.8   0.8   5.7    0.0   0.0   0.0
NEW_2                 228.737  -45.521 3.4  327.604  +10.364    5.9   0.8   7.6    0.0   0.0   0.0
OAO 1657-415          255.214  -41.674 2.4  344.360   +0.302    6.0   0.5  11.0    1.9   0.4   4.9
XTE J1543-568         235.970  -56.814 6.2  324.907   -1.488    2.3   0.0   3.9    0.0   0.0   0.0

JEM-X

1265np_jemx_mosa1.png1265np_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            248.509  -47.395  336.911   +0.247    0.3   0.0 107.5   0.0   0.0    9.4 
GX 340+0              251.452  -45.615  339.587   -0.083    0.4   0.0  47.6   0.1   0.0   17.3 
H 1624-490            247.007  -49.207  334.906   -0.267    0.1   0.0  28.8   0.0   0.0    6.2 
H 1636-536            250.240  -53.749  332.920   -4.821    0.1   0.0  12.3   0.0   0.0    1.8 

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