INTEGRAL Galactic bulge Monitoring

Revolution 0658: Observation start 2008-03-03T12:56 = MJD 54528.539
Total Observation GTI = 10773 seconds

IBIS/ISGRI

0658_isgri_mosa1.jpg 0658_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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
GRO J1750-27          267.293  -26.642 0.4    2.370   +0.516   40.3  0.38 106.3    2.1  0.30   7.1
4U 1700-377           255.989  -37.845 0.5  347.755   +2.172   57.3  0.80  71.8   16.9  0.59  28.7
H 1820-303            275.917  -30.365 1.0    2.784   -7.914   17.5  0.59  29.5    0.0  0.00   0.0
Ginga 1826-24         277.363  -23.784 1.1    9.282   -6.079   19.4  0.74  26.3    6.3  0.55  11.4
4U 1722-30            261.874  -30.791 1.5  356.323   +2.314    7.9  0.40  19.4    3.9  0.31  12.5
GRS 1758-258          270.296  -25.766 2.3    4.486   -1.368    4.5  0.39  11.6    2.5  0.30   8.2
GX 349+2              256.418  -36.428 2.0  349.091   +2.757    9.8  0.73  13.5    0.0  0.00   0.0
GX 3+1                266.951  -26.546 0.0    2.293   +0.827    4.2  0.00  10.9    0.0  0.00   0.0
OAO 1657-415          255.155  -41.631 3.0  344.366   +0.363   13.4  1.53   8.8    0.0  0.00   0.0
3A 1822-371           276.521  -37.032 3.3  356.944  -11.314    5.5  0.70   7.9    0.0  0.00   0.0
GX 9+1                270.288  -20.504 4.2    9.054   +1.244    3.6  0.60   5.9    0.0  0.00   0.0
1E 1740.7-2942        265.933  -29.726 3.9  359.111   -0.062    2.4  0.37   6.4    1.2  0.00   4.1
GX 17+2               274.017  -13.962 3.9   16.502   +1.303   27.5  4.25   6.5    0.0  0.00   0.0
GX 5-1                270.233  -24.988 3.9    5.134   -0.933    2.6  0.40   6.5    0.0  0.00   0.0
3A 1728-169           262.983  -16.958 4.5    8.541   +9.000    6.2  1.12   5.5    0.0  0.00   0.0
SLX 1735-269          264.510  -26.946 4.8    0.808   +2.472    2.0  0.38   5.1    0.0  0.00   0.0
GX 354-0              262.995  -33.845 4.4  354.297   -0.160    2.4  0.43   5.6    0.0  0.00   0.0
IGR J17488-3253       267.300  -32.975 7.3  356.939   -2.746    1.3  0.38   3.3    0.0  0.00   0.0

JEM-X

0658_jemx_mosa1.jpg 0658_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    2.8  0.36   7.8    0.5  0.22   2.3
4U 1722-30            261.888  -30.802  356.320   +2.298    2.6  0.62   4.1    1.7  0.40   4.4
GRO J1750-27          267.304  -26.635    2.381   +0.512   17.5  0.71  24.8   10.6  0.40  26.8
GX 3+1                266.988  -26.565    2.295   +0.789   40.6  0.71  57.1    4.7  0.36  13.0
GX 354-0              262.989  -33.835  354.302   -0.150   10.6  1.01  10.4    2.0  0.69   3.0
GX 5-1                270.278  -25.082    5.072   -1.015   88.6  2.65  33.4    5.9  1.34   4.4
MXB 1730-335          263.350  -33.388  354.841   -0.158    8.3  0.78  10.6    1.6  0.52   3.0
SLX 1744-299_300      266.858  -29.999  359.297   -0.889    2.2  0.35   6.3    0.3  0.21   1.6
SLX 1746-331          267.469  -33.201  356.817   -2.983    3.5  0.54   6.4    0.0  0.00   0.0
NEW SOURCE            268.796  -27.590    2.235   -1.118    2.5  0.57   4.4    0.5  0.34   1.4
NEW SOURCE            272.443  -26.571    4.723   -3.442   12.4  3.23   3.8    0.0  0.00   0.0
NEW SOURCE            271.030  -24.972    5.504   -1.554   14.5  4.07   3.6    0.0  0.00   0.0
NEW SOURCE            265.314  -24.216    3.510   +3.305    5.5  1.65   3.4    0.0  0.00   0.0


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