INTEGRAL Galactic bulge Monitoring

Revolution 0474: Observation start 2006-08-31T03:22 = MJD 53978.141
Total Observation GTI = 12085 seconds

IBIS/ISGRI

0474_isgri_mosa1.jpg 0474_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           255.984  -37.848 0.4  347.751   +2.173   74.1  0.73 102.1   17.5  0.53  33.2
GX 354-0              262.992  -33.833 0.7  354.305   -0.151   21.4  0.41  52.0    5.6  0.33  17.2
GX 1+4                263.011  -24.741 0.8    1.942   +4.796   17.1  0.40  42.4    0.0  0.00   0.0
Ginga 1826-24         277.371  -23.795 1.0    9.276   -6.090   18.8  0.62  30.4    6.5  0.46  14.1
GX 349+2              256.427  -36.430 1.3  349.094   +2.749   14.6  0.67  21.8    0.0  0.00   0.0
1A 1742-294           266.509  -29.505 1.4  359.562   -0.373    5.9  0.29  20.0    2.6  0.24  10.9
GRS 1758-258          270.311  -25.753 1.5    4.504   -1.373    7.3  0.39  19.0    4.2  0.31  13.7
1E 1740.7-2942        265.987  -29.748 2.0  359.118   -0.113    4.5  0.32  14.0    2.3  0.26   9.1
H 1820-303            275.921  -30.340 2.1    2.808   -7.905    6.5  0.49  13.2    0.0  0.00   0.0
GX 5-1                270.287  -25.103 2.8    5.058   -1.032    3.8  0.41   9.3    0.0  0.00   0.0
3A 1822-371           276.443  -37.129 2.7  356.828  -11.299    6.3  0.65   9.7    0.0  0.00   0.0
GX 9+1                270.366  -20.507 3.2    9.088   +1.180    3.7  0.46   8.0    0.0  0.00   0.0
4U 1722-30            261.844  -30.768 3.0  356.327   +2.348    3.3  0.37   8.7    0.0  0.00   0.0
GX 3+1                266.981  -26.569 3.6    2.288   +0.793    2.3  0.32   7.1    0.0  0.00   0.0
1E 1742.9-2849        266.596  -28.900 4.1    0.118   -0.124    1.8  0.29   6.2    0.0  0.00   0.0
SLX 1735-269          264.570  -27.025 3.9    0.770   +2.385    2.1  0.33   6.4    1.2  0.00   4.4
SLX 1744-299_300      266.874  -30.039 5.2  359.269   -0.921    1.4  0.30   4.7    1.4  0.25   5.8
IGR J17252-3616       261.277  -36.168 5.3  351.583   -0.276    2.2  0.47   4.6    0.0  0.00   0.0
IGR J17586-2129       269.635  -21.280 5.3    8.077   +1.388    2.0  0.44   4.6    0.0  0.00   0.0
GRS 1734-292          264.424  -29.188 5.4  358.871   +1.337    1.4  0.32   4.6    1.0  0.26   3.9
1H 1746-370           267.493  -37.004 5.5  353.548   -4.940    2.0  0.45   4.4    0.0  0.00   0.0
Oph Cluster           258.105  -23.369 5.9    0.568   +9.278    2.1  0.50   4.1    0.0  0.00   0.0
V2400 Oph             258.057  -24.269 5.9  359.797   +8.796    2.0  0.49   4.1    0.0  0.00   0.0
XTE J1817-330         274.436  -33.103 6.7  359.743   -8.037    1.6  0.44   3.6    0.0  0.00   0.0
3A 1728-169           262.939  -16.897 6.3    8.571   +9.068    3.1  0.81   3.8    0.0  0.00   0.0

JEM-X

0474_jemx_mosa1.jpg 0474_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  -29.515  359.559   -0.389    1.9  0.29   6.7    0.7  0.17   4.1
1E 1740.7-2942        265.978  -29.745  359.116   -0.106    1.4  0.29   4.8    0.6  0.18   3.2
1E 1743.1-2843        266.587  -28.729    0.260   -0.029    1.0  0.30   3.4    0.3  0.18   1.9
GX 3+1                266.986  -26.567    2.292   +0.790   28.6  0.46  62.3    3.1  0.23  13.6
GX 354-0              262.993  -33.828  354.309   -0.149   10.7  1.26   8.5    3.0  1.02   2.9
GX 5-1                270.294  -25.079    5.081   -1.026   84.6  1.59  53.3    5.2  0.65   8.0
SLX 1744-299_300      266.858  -29.999  359.297   -0.889    1.0  0.29   3.4    0.3  0.18   1.9
NEW SOURCE            273.372  -27.640    4.177   -4.679   11.7  3.25   3.6    0.0  0.00   0.0
NEW SOURCE            266.856  -24.559    3.951   +1.928    3.1  0.76   4.0    0.0  0.00   0.0
NEW SOURCE            270.091  -24.877    5.166   -0.766    5.4  1.39   3.9    0.0  0.00   0.0


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