INTEGRAL Galactic bulge Monitoring

Revolution 1654: Observation start 2016-03-09T20:42 = MJD 57456.863
Total Observation GTI = 12538 seconds

IBIS/ISGRI

1654_isgri_mosa1.jpg 1654_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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
IGR J17464-3213       266.574  -32.238 0.7  357.256   -1.842   31.4  0.60  52.6   19.4  0.33  58.7
GX 1+4                263.001  -24.751 0.8    1.929   +4.798   26.9  0.59  45.3    0.0  0.00   0.0
GX 5-1                270.295  -25.079 1.1    5.082   -1.026   17.2  0.61  28.2    1.3  0.00   3.8
GRS 1758-258          270.309  -25.748 1.4    4.507   -1.369   13.1  0.62  21.1    7.8  0.34  22.8
IGR J17091-3624       257.268  -36.388 1.4  349.534   +2.233   18.2  0.90  20.2   11.4  0.48  23.8
OAO 1657-415          255.206  -41.645 1.9  344.379   +0.325   36.9  2.59  14.2   14.9  1.33  11.2
SLX 1735-269          264.574  -26.978 2.5    0.810   +2.407    5.8  0.53  10.8    2.0  0.30   6.6
GX 349+2              256.422  -36.397 2.6  349.118   +2.772    9.9  0.98  10.0    0.0  0.00   0.0
3A 1822-371           276.477  -37.097 3.6  356.869  -11.310    8.3  1.16   7.1    2.5  0.00   4.2
H 1820-303            275.908  -30.380 3.0    2.766   -7.914    6.8  0.79   8.7    0.0  0.00   0.0
SAX J1750.8-2900      267.582  -29.035 3.2    0.447   -0.932    3.7  0.47   8.0    1.0  0.27   3.7
SLX 1744-299_300      266.789  -30.016 4.2  359.251   -0.847    2.9  0.49   5.9    1.0  0.28   3.7
Swift J1753.7-2544    268.317  -25.710 4.4    3.641   +0.203    3.4  0.00   5.7    0.0  0.00   0.0
GX 3+1                266.901  -26.619 4.2    2.208   +0.828    3.2  0.53   6.0    0.0  0.00   0.0
GX 13+1               273.617  -17.089 5.3   13.570   +0.151    6.7  1.43   4.7    0.0  0.00   0.0
IGR J17541-2252       268.632  -22.862 5.6    6.242   +1.398    2.5  0.56   4.4    0.0  0.00   0.0
4U 1722-30            261.872  -30.722 3.9  356.379   +2.354    3.6  0.56   6.5    1.7  0.31   5.6
GX 354-0              263.036  -33.827 3.9  354.330   -0.178    3.4  0.53   6.4    1.0  0.00   3.5

JEM-X

1654_jemx_mosa1.jpg 1654_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           266.533  -29.521  359.558   -0.400    4.3  0.25  16.9    0.6  0.17   3.5
1E 1740.7-2942        265.978  -29.745  359.116   -0.106    1.1  0.25   4.4    0.3  0.17   1.8
GX 1+4                263.009  -24.746    1.937   +4.795    3.4  0.99   3.4    2.2  0.61   3.6
GX 3+1                266.983  -26.564    2.294   +0.794   11.5  0.36  32.3    1.4  0.21   6.8
GX 354-0              262.989  -33.835  354.302   -0.150   10.7  1.12   9.5    1.1  1.00   1.1
GX 5-1                270.284  -25.079    5.077   -1.019   93.1  1.39  66.7   18.8  0.71  26.3
IGR J17464-3213       266.550  -32.232  357.249   -1.822    6.2  0.39  15.8    3.2  0.29  10.9
SLX 1735-269          264.571  -26.994    0.796   +2.400    1.7  0.34   5.1    0.6  0.21   2.8
SLX 1744-299_300      266.858  -29.999  359.297   -0.889    1.6  0.26   6.2    0.2  0.17   1.3
Swift J174535.5-2901  266.398  -29.026  359.920   -0.042    0.9  0.25   3.6    0.3  0.17   1.9
CONFUSED ID           270.280  -25.077    5.077   -1.014   93.4  1.39  67.0   19.0  0.71  26.6
SAX J1750.8-2900      267.592  -29.040    0.448   -0.943    2.0  0.28   7.3    0.5  0.18   2.8
CONFUSED ID           270.276  -25.004    5.139   -0.975   33.5  1.31  25.6    5.3  0.68   7.7
NEW SOURCE            272.818  -27.142    4.381   -4.010    8.0  1.84   4.4    2.1  1.46   1.4
NEW SOURCE            272.413  -27.290    4.078   -3.765    4.7  1.18   4.0    0.0  0.00   0.0


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