Revolution 1204

Observation start: 2012-08-22T19:26 = MJD 56161.81
Total Observation GTI = 9140 seconds

ISGRI

1204np_isgri_mosa1.png1204np_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 OSA9, 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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
1A 1744-361           267.140  -36.111 6.2  354.174   -4.240    9.6   2.4   3.9    0.0   0.0   0.0
3EG J1704-4732        256.079  -47.525 6.4  340.099   -3.757    1.9   0.5   3.8    0.0   0.0   0.0
4U 1700-377           255.984  -37.844 0.4  347.753   +2.175   73.8   0.6 115.8   22.7   0.4  53.4
4U 1735-444           264.649  -44.415 3.3  346.049   -6.919    6.2   0.8   7.7    0.0   0.0   0.0
GRS 1730-312          263.373  -31.185 0.0  356.699   +1.024   19.7   0.0   5.2    9.5   0.0   4.2
GX 349+2              256.417  -36.417 1.7  349.099   +2.764   12.6   0.8  16.5    0.0   0.0   0.0
H 1702-429            256.642  -43.037 3.4  343.920   -1.365    3.4   0.5   7.5    0.0   0.0   0.0
H 1705-440            257.223  -44.122 3.0  343.304   -2.351    4.0   0.5   8.8    0.0   0.0   0.0
IGR J15415-5029       235.483  -50.475 5.5  328.519   +3.730    3.1   0.7   4.5    0.0   0.0   0.0
IGR J16207-5129       245.147  -51.467 5.2  332.463   -1.005    2.2   0.5   4.8    0.0   0.0   0.0
IGR J16318-4848       247.980  -48.806 1.2  335.637   -0.454   10.7   0.4  25.0    3.4   0.3  11.3
IGR J16320-4751       247.991  -47.840 5.5  336.347   +0.200    1.8   0.4   4.5    0.0   0.0   0.0
IGR J17091-3624       257.273  -36.421 5.1  349.509   +2.210    3.6   0.8   4.8    2.0   0.5   4.0
NEW_1                 274.415  -53.306 3.2  341.038  -16.710   35.6   4.4   8.1    0.0   0.0   0.0
NEW_2                 264.129  -48.260 3.8  342.553   -8.626    4.3   0.7   6.6    0.0   0.0   0.0
NEW_3                 263.654  -31.694 0.0  356.402   +0.547   20.9   0.0   6.3    0.0   0.0   0.0
NEW_4                 261.861  -29.795 5.4  357.145   +2.877   38.3   7.0   4.5    0.0   0.0   0.0
OAO 1657-415          255.208  -41.657 0.8  344.370   +0.316   20.4   0.5  40.6    5.3   0.3  15.6

JEM-X

1204np_jemx_mosa1.png1204np_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            248.512  -47.391  336.915   +0.249   75.5   0.7 105.6   3.2   0.3   10.9 
GX 340+0              251.451  -45.602  339.596   -0.074   91.7   0.7 129.1   7.9   0.3   26.8 
H 1624-490            247.003  -49.174  334.929   -0.242   14.0   1.1  13.1   1.9   0.5    4.0 
H 1705-440            257.230  -44.099  343.325   -2.342  107.0   3.1  34.7  20.6   1.8   11.4 

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