Revolution 1517

Observation start: 2015-03-13T11:09 = MJD 57094.465
Total Observation GTI = 15170 seconds

ISGRI

1517np_isgri_mosa1.png1517np_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  
==================== ========  ======= === ====== ===== ===== ====== ===== =====
1RXS J180408.9-34205  271.069  -34.416 6.5  21.1   5.7   3.7    0.0   0.0   0.0
4U 1630-47            248.499  -47.390 0.7  14.9   0.3  47.4    7.1   0.2  31.5
4U 1700-377           255.980  -37.841 0.4  61.8   0.5 126.9   20.0   0.3  63.0
4U 1735-444           264.684  -44.441 3.5   3.6   0.5   7.4    0.0   0.0   0.0
AX J1701.2-4212       255.361  -42.283 0.0   1.8   0.0   5.8    0.0   0.0   0.0
GX 339-4              255.695  -48.796 1.2   7.3   0.3  24.7    2.9   0.2  14.4
GX 340+0              251.409  -45.602 4.2   1.6   0.3   6.0    0.0   0.0   0.0
GX 349+2              256.426  -36.404 2.5   5.6   0.5  10.6    0.0   0.0   0.0
H 1538-522            235.594  -52.370 5.5   2.1   0.0   4.5    0.0   0.0   0.0
H 1553-542            239.562  -54.405 4.1   2.9   0.5   6.2    0.0   0.0   0.0
H 1608-522            243.226  -52.401 2.3   4.1   0.4  11.4    3.1   0.2  12.6
H 1636-536            250.248  -53.750 1.0  10.8   0.3  31.5    5.0   0.2  21.1
IGR J16207-5129       245.196  -51.412 4.2   1.9   0.3   6.0    0.0   0.0   0.0
IGR J16318-4848       247.928  -48.811 1.3   5.9   0.3  22.2    1.4   0.2   7.5
IGR J16320-4751       248.001  -47.882 1.4   6.3   0.3  20.9    1.0   0.2   5.1
IGR J16393-4643       249.732  -46.724 0.0   1.3   0.0   4.8    0.0   0.0   0.0
IGR J16418-4532       250.473  -45.552 3.0   2.2   0.3   8.8    0.0   0.0   0.0
IGR J16447-5138       251.080  -51.650 5.0   1.5   0.3   5.0    0.0   0.0   0.0
IGR J16479-4514       252.028  -45.187 4.2   1.6   0.3   5.9    0.0   0.0   0.0
IGR J16493-4348       252.280  -43.860 4.3   1.7   0.3   5.8    0.0   0.0   0.0
IGR J16500-3307       252.534  -33.036 5.1   4.9   0.0   4.8    0.0   0.0   0.0
IGR J17173-5855       259.457  -58.889 5.1   3.7   0.8   4.9    0.0   0.0   0.0
NEW_1                 256.237  -42.379 3.2   2.5   0.3   8.0    0.0   0.0   0.0
OAO 1657-415          255.153  -41.644 3.6   2.6   0.4   7.1    2.0   0.2   8.0

JEM-X

1517np_jemx_mosa1.png1517np_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  
==================== ========  ======= ====== ===== ===== ====== ===== =====
4U 1630-47            248.504  -47.398  30.2   0.3 118.8   3.2   0.1   27.2 
GX 339-4              255.708  -48.792  28.1   0.5  57.9   1.5   0.2    6.3 
GX 340+0              251.448  -45.616  50.0   0.2 205.3   3.3   0.1   31.5 
H 1624-490            247.010  -49.184   6.8   0.4  17.9   0.8   0.2    4.1 
H 1705-440            257.216  -44.102  22.2   0.7  32.1   2.3   0.3    6.5 

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