INTEGRAL Galactic bulge Monitoring

Revolution 1343: Observation start 2013-10-12T18:18 = MJD 56577.763
Total Observation GTI = 12157 seconds

IBIS/ISGRI

1343_isgri_mosa1.jpg 1343_isgri_mosa2.jpg

IBIS/ISGRI significance mosaic images. Left: IBIS/ISGRI 18-40 keV. Right: 40-100 keV
Sources detected > 10σ 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 OSA10.1, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 208 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 100 cps ) where available.
NOTES: 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 < 6σ towards the border of the image may be spurious.

IBIS/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 1700-377           255.983  -37.853 0.7  347.746   +2.171   44.3  0.98  45.4   13.6  0.63  21.7
GX 1+4                263.006  -24.747 0.8    1.934   +4.796   17.9  0.41  44.1    0.0  0.00   0.0
Ginga 1826-24         277.364  -23.791 1.0    9.276   -6.082   18.7  0.59  32.0    6.9  0.39  17.6
GRS 1758-258          270.310  -25.751 1.0    4.505   -1.372   10.6  0.36  29.6    7.7  0.25  30.2
GX 5-1                270.279  -25.078 1.0    5.076   -1.014   11.7  0.39  30.1    0.0  0.00   0.0
OAO 1657-415          255.186  -41.645 1.4  344.369   +0.336   45.2  2.18  20.8   12.3  1.31   9.4
H 1820-303            275.933  -30.388 1.7    2.770   -7.936    8.4  0.51  16.5    0.0  0.00   0.0
3A 1822-371           276.467  -37.123 2.5  356.842  -11.314    6.7  0.62  10.7    0.0  0.00   0.0
SAX J1806.5-2215      271.693  -22.257 2.8    8.169   -0.756    4.1  0.44   9.2    2.0  0.31   6.4
GX 9+1                270.397  -20.485 3.1    9.120   +1.166    4.3  0.52   8.3    0.0  0.00   0.0
GX 354-0              262.995  -33.810 3.0  354.325   -0.141    3.9  0.45   8.8    0.0  0.00   0.0
1E 1740.7-2942        266.029  -29.781 3.9  359.108   -0.162    2.4  0.37   6.4    2.0  0.25   7.9
Swift J1734.5-3027    263.637  -30.380 4.0  357.498   +1.271    2.3  0.35   6.4    1.6  0.25   6.3
GX 349+2              256.409  -36.406 3.8  349.104   +2.776    5.6  0.84   6.6    0.0  0.00   0.0
GX 3+1                266.987  -26.576 3.5    2.285   +0.784    2.8  0.39   7.3    0.0  0.00   0.0
SLX 1735-269          264.532  -27.033 4.6    0.744   +2.409    2.0  0.36   5.4    1.0  0.26   3.9
1A 1742-294           266.497  -29.540 4.8  359.526   -0.383    1.9  0.37   5.2    0.0  0.00   0.0
4U 1722-30            261.850  -30.755 0.0  356.340   +2.352    2.0  0.00   4.7    0.0  0.00   0.0
SLX 1737-282          265.248  -28.317 0.0  359.994   +1.190    1.9  0.00   4.7    0.0  0.00   0.0
V1223 Sgr             283.829  -31.104 0.0    5.039  -14.386    6.9  0.00   4.5    0.0  0.00   0.0
AX J1749.2-2725       267.188  -27.411 4.8    1.662   +0.200    1.7  0.34   5.1    0.0  0.00   0.0
SAX J1712.6-3739      258.179  -37.607 6.0  348.982   +0.925    2.9  0.72   4.1    0.0  0.00   0.0
SLX 1746-331          267.460  -33.214 6.2  356.803   -2.984    1.5  0.38   3.9    0.0  0.00   0.0
1E 1742.9-2849        266.643  -28.829 0.0    0.200   -0.122    1.5  0.00   4.1    0.0  0.00   0.0
IGR J17354-3255       263.961  -32.884 0.0  355.542   -0.315    1.4  0.00   4.0    0.0  0.00   0.0

JEM-X

1343_jemx_mosa1.jpg 1343_jemx_mosa2.jpg

JEM-X1+2 combined significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.

Sources labelled were detected in the 3-10 keV image > 6σ. The sources detected above 3σ in the 3-10 keV and/or 10-25 keV band are listed in the table below. Fluxes are extracted at the known catalogue 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 ~ 97 cps [J1], 103 cps [J2]); B = 10-25 keV (1 Crab ~ 29 cps [J1], 27 cps [J2]).
NOTES: The object marked as SLX 1744-299_300 is used to indicate two low-mass x-ray binaries separated by 2.7 arcminutes, SLX 1744-299 and SLX 1744-300; the position for SLX 1744-299 is used, although it can not be ruled out that SLX 1744-300 may dominate the emission some of the time. The systematic noise increases towards the edge of the field of view and in the vicinity of very bright sources, such as GX 5-1; NEW SOURCEs < 6σ towards the border of the image and/or near GX 5-1 may, therefore, be spurious.

JEM-X1+2 Detected Sources in 3-10 keV (A) and 10-25 keV (B).

Source Name             RA       dec      l        b     A(cps)  +/-   sig  B(cps)  +/-   sig  
==================== ========  ======= ======== ======== ====== ===== ===== ====== ===== =====
1A 1742-294           266.515  -29.514  359.557   -0.383   10.7  0.26  40.4    2.1  0.14  15.0
4U 1722-30            261.888  -30.802  356.320   +2.298    5.9  0.94   6.3    0.8  0.60   1.3
GRS 1758-258          270.303  -25.741    4.511   -1.361    0.9  0.65   1.3    1.4  0.32   4.4
GX 3+1                266.981  -26.567    2.290   +0.794   51.9  0.45 116.3    6.0  0.21  28.9
GX 354-0              263.000  -33.831  354.311   -0.155   20.8  2.15   9.7    4.8  1.48   3.3
GX 5-1                270.296  -25.066    5.094   -1.021  120.5  1.05 114.9   15.0  0.46  32.6
SLX 1735-269          264.571  -26.994    0.796   +2.400    2.2  0.46   4.7    0.6  0.24   2.5
SLX 1744-299_300      266.858  -29.999  359.297   -0.889    2.5  0.25  10.3    0.4  0.14   2.9
Swift J174535.5-2901  266.398  -29.026  359.920   -0.042    1.7  0.26   6.6    0.5  0.14   3.6
XTE J1739-285         264.975  -28.496  359.714   +1.298    1.1  0.34   3.1    0.0  0.00   0.0
NEW SOURCE            271.644  -23.858    6.749   -1.497   14.2  2.50   5.7    2.5  1.41   1.8
NEW SOURCE            268.542  -25.507    3.918   +0.130    2.8  0.56   5.1    0.4  0.27   1.4


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