Revolution 1166

Observation start: 2012-05-03T11:27 = MJD 56050.478
Total Observation GTI = 27402 seconds

ISGRI

1166ss_isgri_mosa1.png1166ss_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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
3A 1850-087           283.288   -8.695 3.5   25.372   -4.331    1.7   0.2   7.2    0.0   0.0   0.0
3EG J1800-0146        270.181   -1.854 0.0   25.406  +10.397    1.8   0.0   5.0    0.0   0.0   0.0
4U 1812-12            273.764  -12.100 1.7   18.024   +2.406    5.6   0.4  16.0    2.6   0.3   9.9
4U 1916-053           289.708   -5.176 3.7   31.418   -8.443    2.1   0.3   6.9    0.8   0.2   3.6
GRS 1915+105          288.797  +10.947 0.6   45.366   -0.217   79.5   1.2  68.4    0.0   0.0   0.0
GX 17+2               274.016  -14.044 1.7   16.430   +1.266    6.9   0.4  16.3    0.0   0.0   0.0
NEW_1                 265.900   -5.941 4.7   19.659  +12.182    5.9   1.0   5.3   31.7   5.2   6.1
NEW_10                273.390  -21.586 5.0    9.517   -1.811   13.5   2.8   4.9    0.0   0.0   0.0
NEW_11                277.734  -17.717 0.0   14.857   -3.613    3.6   0.0   6.2    0.0   0.0   0.0
NEW_12                275.783   -5.889 3.8   24.451   +3.571    1.5   0.2   6.7    0.0   0.0   0.0
NEW_13                292.715   -4.584 0.0   33.321  -10.853    2.6   0.0   6.1    0.0   0.0   0.0
NEW_14                290.489   -8.809 4.7   28.468  -10.754    1.6   0.3   5.3    0.0   0.0   0.0
NEW_2                 285.660   +0.449 4.1   34.609   -2.288    1.4   0.2   6.1    0.0   0.0   0.0
NEW_3                 277.956  -14.467 4.6   17.844   -2.307    1.9   0.3   5.5    0.0   0.0   0.0
NEW_4                 268.399   -5.619 5.2   21.181  +10.168    2.7   0.5   4.8    0.0   0.0   0.0
NEW_5                 273.327  -20.871 4.4   10.117   -1.417    9.0   1.6   5.7    0.0   0.0   0.0
NEW_6                 286.920   +2.060 3.9   36.620   -2.671    1.7   0.3   6.5    0.0   0.0   0.0
NEW_7                 290.132   -9.517 4.8   27.663  -10.749    1.8   0.3   5.2    0.0   0.0   0.0
NEW_8                 289.957   -7.990 4.2   28.979   -9.920    1.8   0.3   6.0    0.0   0.0   0.0
NEW_9                 286.742  -13.731 0.0   22.339   -9.600    2.4   0.0   6.5    0.0   0.0   0.0
SS 433                287.978   +4.995 4.9   39.715   -2.258    2.0   0.0   5.1    0.0   0.0   0.0
SWIFT J1753.5-0127    268.381   -1.447 1.5   24.908  +12.177    9.8   0.5  19.7    4.7   0.4  12.6
Ser X-1               279.938   +5.114 4.5   36.164   +4.923    1.7   0.0   5.6    0.0   0.0   0.0

JEM-X

1166ss_jemx_mosa1.png1166ss_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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