Revolution 1276

Observation start: 2013-03-28T18:04 = MJD 56379.753
Total Observation GTI = 8608 seconds

ISGRI

1276ss_isgri_mosa1.png1276ss_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 1812-12            273.782  -12.144 2.5   17.994   +2.370    5.2   0.5  10.6    3.5   0.4   9.5
AX J1818.8-1527       274.812  -15.438 0.0   15.568   -0.073    3.2   0.0   5.1    0.0   0.0   0.0
AX J1908.3+0745       287.077   +7.756 5.7   41.752   -0.190    4.6   1.1   4.3    0.0   0.0   0.0
GRS 1915+105          288.801  +10.941 1.8   45.363   -0.224   77.7   4.9  15.9    0.0   0.0   0.0
GX 13+1               273.589  -17.123 4.2   13.527   +0.159    6.0   1.0   6.1    0.0   0.0   0.0
GX 17+2               274.006  -14.028 1.2   16.440   +1.281   13.2   0.6  23.8    0.0   0.0   0.0
IGR J18246-1425       276.153  -14.425 0.0   17.071   -0.741    2.6   0.0   4.5    0.0   0.0   0.0
IGR J18538-0102       283.393   -1.089 5.6   32.206   -0.971    1.5   0.3   4.4    0.0   0.0   0.0
NEW_1                 288.253   -4.940 3.6   30.972   -7.043    3.9   0.5   7.2    0.0   0.0   0.0
NEW_2                 269.342  -18.193 3.9   10.617   +3.168   10.7   1.6   6.5    0.0   0.0   0.0
NEW_3                 271.830   +9.241 3.9   36.288  +13.962   10.6   1.6   6.5    0.0   0.0   0.0
NEW_4                 295.273  -12.914 4.5   26.735  -16.762   39.1   7.1   5.5    0.0   0.0   0.0
NEW_5                 283.685  +10.506 3.6   42.671   +4.045   14.5   2.0   7.2    0.0   0.0   0.0
NEW_6                 271.268  -15.905 4.1   13.519   +2.695    5.5   0.9   6.2    0.0   0.0   0.0
SWIFT J1753.5-0127    268.374   -1.490 2.4   24.866  +12.163    7.7   0.7  10.9    4.2   0.5   8.8
Ser X-1               280.052   +5.051 6.1   36.159   +4.794    2.5   0.6   4.0    0.0   0.0   0.0
XTE J1810-189         272.615  -19.032 3.5   11.408   +0.054   14.9   2.0   7.3    0.0   0.0   0.0
XTE J1829-098         277.425   -9.945 5.4   21.615   +0.244    1.6   0.3   4.5    0.0   0.0   0.0

JEM-X

1276ss_jemx_mosa1.png1276ss_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  
==================== ========  ======= ======== ======== ====== ===== ===== ====== ===== =====

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