INTEGRAL Galactic bulge Monitoring

Revolution 0292: Observation start 2005-03-05T16:57 = MJD 53434.707
Total Observation GTI = 11932 seconds

IBIS/ISGRI

0292_isgri_mosa1.jpg 0292_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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
GRS 1758-258          270.305  -25.742 0.9    4.511   -1.363   13.1  0.35  36.9    8.5  0.28  30.2
1E 1740.7-2942        265.975  -29.754 0.9  359.107   -0.108    9.7  0.27  35.9    6.9  0.23  30.4
GX 349+2              256.421  -36.428 1.1  349.093   +2.754   14.8  0.55  27.1    0.0  0.00   0.0
Ginga 1826-24         277.360  -23.790 1.2    9.276   -6.078   15.1  0.58  26.0    6.9  0.45  15.4
GX 5-1                270.278  -25.079 1.3    5.074   -1.013    8.5  0.37  22.9    0.0  0.00   0.0
GRO J1655-40          253.497  -39.851 1.5  344.976   +2.455   21.1  1.08  19.6   13.8  0.80  17.3
GX 1+4                262.991  -24.774 1.6    1.905   +4.793    6.9  0.38  18.1    0.0  0.00   0.0
GX 354-0              262.973  -33.831 1.6  354.298   -0.137    6.5  0.36  18.0    0.0  0.00   0.0
1A 1742-294           266.500  -29.518 1.6  359.546   -0.374    4.8  0.28  17.6    1.6  0.00   7.0
4U 1700-377           255.974  -37.855 1.7  347.740   +2.174   10.0  0.59  17.0    0.0  0.00   0.0
H 1820-303            275.901  -30.346 1.7    2.795   -7.893    7.3  0.44  16.4    0.0  0.00   0.0
OAO 1657-415          255.212  -41.668 1.9  344.364   +0.307   24.5  1.70  14.4    8.6  1.21   7.1
4U 1722-30            261.896  -30.802 2.0  356.324   +2.292    4.3  0.31  13.7    1.8  0.25   7.3
GX 9+1                270.355  -20.502 2.5    9.086   +1.191    4.6  0.43  10.7    0.0  0.00   0.0
SLX 1735-269          264.573  -26.976 2.7    0.813   +2.408    2.9  0.29   9.9    0.0  0.00   0.0
3A 1822-371           276.399  -37.099 2.7  356.840  -11.255    5.9  0.60   9.8    0.0  0.00   0.0
GX 3+1                267.003  -26.527 3.4    2.334   +0.798    2.4  0.31   7.5    0.0  0.00   0.0
GX 17+2               273.960  -14.101 4.2   16.353   +1.286   15.0  2.53   6.0    0.0  0.00   0.0
3A 1728-169           262.920  -16.957 3.6    8.510   +9.052    4.9  0.70   7.0    0.0  0.00   0.0
SLX 1744-299_300      266.901  -29.991 5.8  359.322   -0.917    1.2  0.28   4.2    0.0  0.00   0.0
Oph Cluster           258.197  -23.431 5.0    0.566   +9.173    2.1  0.43   5.0    0.0  0.00   0.0
1E 1742.8-2853        266.479  -28.921 5.4    0.047   -0.048    1.2  0.27   4.5    0.0  0.00   0.0
SLX 1737-282          265.254  -28.300 6.1    0.011   +1.193    1.1  0.00   4.0    0.0  0.00   0.0

JEM-X

0292_jemx_mosa1.jpg 0292_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    1.8  0.23   7.7    0.7  0.13   5.3
1E 1740.7-2942        265.994  -29.733  359.133   -0.110    2.6  0.23  11.5    1.3  0.13   9.6
4U 1722-30            261.888  -30.802  356.320   +2.298    2.2  0.40   5.4    0.5  0.26   2.0
GX 3+1                266.987  -26.563    2.296   +0.791   27.8  0.38  73.0    3.2  0.18  17.7
GX 354-0              262.987  -33.833  354.303   -0.148   23.4  0.98  23.9    4.2  0.67   6.3
GX 5-1                270.286  -25.077    5.080   -1.019  101.7  1.72  59.3    7.2  0.74   9.6
SLX 1744-299_300      266.858  -29.999  359.297   -0.889    2.8  0.25  11.0    0.5  0.14   3.6
NEW SOURCE            268.688  -24.261    5.060   +0.647    5.8  1.11   5.2    0.0  0.00   0.0
NEW SOURCE            266.222  -22.857    5.106   +3.307    7.9  1.65   4.8    0.0  0.00   0.0
NEW SOURCE            267.060  -22.765    5.585   +2.694    8.9  1.91   4.6    0.0  0.00   0.0
NEW SOURCE            271.673  -25.013    5.753   -2.083   13.7  3.11   4.4    0.0  0.00   0.0
NEW SOURCE            266.696  -28.796    0.252   -0.145    1.1  0.23   4.6    0.0  0.00   0.0


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