INTEGRAL Galactic bulge Monitoring

Revolution 0791: Observation start 2009-04-05T23:30 = MJD 54926.98
Total Observation GTI = 11947 seconds

IBIS/ISGRI

0791_isgri_mosa1.jpg 0791_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           255.992  -37.842 0.8  347.759   +2.172   36.3  0.88  41.3    8.8  0.68  12.8
1E 1740.7-2942        265.981  -29.744 1.1  359.118   -0.107   10.6  0.37  28.7    7.4  0.32  23.3
Ginga 1826-24         277.373  -23.801 1.1    9.271   -6.094   16.1  0.59  27.3    5.5  0.48  11.7
GX 1+4                263.016  -24.749 1.2    1.938   +4.788   10.7  0.42  25.2    0.0  0.00   0.0
GRS 1758-258          270.320  -25.757 1.3    4.504   -1.382    8.2  0.36  22.5    5.2  0.30  17.0
GX 349+2              256.448  -36.418 1.7  349.114   +2.743   12.5  0.75  16.6    0.0  0.00   0.0
H 1820-303            275.913  -30.360 1.8    2.787   -7.908    7.4  0.49  15.1    2.1  0.39   5.2
GX 5-1                270.287  -25.075 1.9    5.082   -1.019    5.3  0.36  14.6    0.0  0.00   0.0
GX 9+1                270.384  -20.540 2.2    9.067   +1.149    5.9  0.48  12.3    0.0  0.00   0.0
GX 17+2               274.015  -14.034 2.5   16.438   +1.271   30.4  2.81  10.8    0.0  0.00   0.0
OAO 1657-415          255.211  -41.665 2.6  344.365   +0.309   23.3  2.29  10.2    0.0  0.00   0.0
3A 1822-371           276.473  -37.019 3.1  356.939  -11.273    5.1  0.61   8.3    0.0  0.00   0.0
GX 3+1                266.986  -26.567 2.6    2.292   +0.790    3.7  0.36  10.2    0.0  0.00   0.0
GX 354-0              263.053  -33.834 3.3  354.332   -0.194    3.1  0.39   7.9    0.0  0.00   0.0
IGR J17252-3616       261.376  -36.344 3.9  351.482   -0.441    3.4  0.53   6.4    0.0  0.00   0.0
4U 1722-30            261.847  -30.823 4.0  356.283   +2.316    2.6  0.42   6.3    0.0  0.00   0.0
SLX 1735-269          264.607  -26.959 4.3    0.843   +2.392    2.3  0.39   5.9    0.0  0.00   0.0
3A 1728-169           262.954  -16.918 4.3    8.560   +9.044    4.9  0.84   5.8    0.0  0.00   0.0
XTE J1709-267         257.405  -26.692 4.0  357.458   +7.870    3.6  0.57   6.2    0.0  0.00   0.0
GX 13+1               273.636  -17.196 4.1   13.485   +0.084    5.2  0.85   6.1    0.0  0.00   0.0
1E 1742.8-2853        266.473  -28.959 5.3    0.011   -0.063    1.6  0.35   4.6    0.0  0.00   0.0
SLX 1744-299_300      266.801  -29.921 5.7  359.338   -0.806    1.7  0.39   4.3    0.0  0.00   0.0
Swift J1734.5-3027    263.680  -30.499 6.1  357.418   +1.175    1.4  0.00   4.0    0.0  0.00   0.0
4U 1735-444           264.677  -44.528 5.2  345.962   -6.995   17.7  3.70   4.8    0.0  0.00   0.0

JEM-X

0791_jemx_mosa1.jpg 0791_jemx_mosa2.jpg

JEM-X1 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 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           266.523  -29.517  359.558   -0.390    3.9  0.29  13.4    0.7  0.18   3.5
1E 1740.7-2942        265.978  -29.745  359.116   -0.106    1.9  0.29   6.4    1.4  0.20   6.9
GRS 1734-292          264.367  -29.142  358.883   +1.404    1.1  0.37   3.1    0.4  0.24   1.5
GX 3+1                266.981  -26.556    2.299   +0.799   36.1  0.47  76.4    4.2  0.24  17.3
GX 5-1                270.281  -25.073    5.081   -1.013   92.9  1.15  81.0    5.8  0.50  11.6
SLX 1744-299_300      266.858  -29.999  359.297   -0.889    1.4  0.28   5.2    0.0  0.00   0.0
NEW SOURCE            269.481  -22.926    6.579   +0.690   19.7  3.17   6.2    0.0  0.00   0.0
NEW SOURCE            273.682  -26.234    5.550   -4.258   10.3  2.18   4.7    0.0  0.00   0.0
NEW SOURCE            270.387  -25.783    4.512   -1.447    3.3  0.69   4.8    0.0  0.00   0.0
NEW SOURCE            269.112  -22.578    6.710   +1.158   15.1  3.18   4.7    0.0  0.00   0.0


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