INTEGRAL Galactic bulge Monitoring

Revolution 0659: Observation start 2008-03-06T12:43 = MJD 54531.53
Total Observation GTI = 13079 seconds

IBIS/ISGRI

0659_isgri_mosa1.jpg 0659_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          267.295  -26.646 0.4    2.367   +0.513   38.5  0.33 117.1    1.4  0.26   5.4
4U 1700-377           255.987  -37.842 0.4  347.756   +2.175   71.4  0.74  96.0   18.7  0.55  34.0
Ginga 1826-24         277.360  -23.793 1.2    9.272   -6.080   17.2  0.66  26.0    6.5  0.49  13.2
H 1820-303            275.922  -30.355 1.1    2.795   -7.914   12.7  0.48  26.3    0.0  0.00   0.0
4U 1722-30            261.892  -30.801 1.3  356.323   +2.296    7.7  0.35  21.9    3.7  0.28  13.4
GRS 1758-258          270.314  -25.744 2.1    4.513   -1.371    5.2  0.41  12.7    2.7  0.32   8.6
GX 349+2              256.417  -36.409 2.0  349.106   +2.769    8.6  0.63  13.6    0.0  0.00   0.0
GX 3+1                266.952  -26.538 0.0    2.301   +0.831    4.0  0.00  12.3    0.0  0.00   0.0
3A 1822-371           276.441  -37.082 2.3  356.870  -11.278    7.6  0.64  11.8    0.0  0.00   0.0
1E 1740.7-2942        265.964  -29.775 2.8  359.084   -0.110    2.9  0.31   9.2    2.6  0.25  10.4
GX 17+2               274.006  -14.022 2.5   16.445   +1.284   33.3  3.13  10.6    0.0  0.00   0.0
GX 9+1                270.358  -20.551 3.6    9.045   +1.165    3.6  0.50   7.1    0.0  0.00   0.0
GX 354-0              262.994  -33.844 3.1  354.296   -0.159    3.4  0.40   8.5    0.0  0.00   0.0
SLX 1735-269          264.481  -27.000 3.9    0.748   +2.465    2.1  0.33   6.5    1.2  0.27   4.6
GX 1+4                263.042  -24.718 3.8    1.977   +4.784    2.9  0.43   6.7    0.0  0.00   0.0
GX 5-1                270.247  -25.035 5.5    5.098   -0.967    1.8  0.41   4.4    0.0  0.00   0.0
1A 1742-294           266.401  -29.500 0.0  359.516   -0.291    1.5  0.00   4.8    0.0  0.00   0.0
GRS 1741.9-2853       266.315  -28.864 5.5    0.020   +0.105    1.3  0.30   4.5    0.0  0.00   0.0
1RXS J165424.7-29541  253.633  -29.859 4.8  352.882   +8.618    3.2  0.61   5.1    0.0  0.00   0.0
XTE J1709-267         257.365  -26.627 6.0  357.490   +7.937    1.9  0.47   4.1    0.0  0.00   0.0
H 1745-203            267.151  -20.450 7.1    7.618   +3.811    1.7  0.49   3.4    0.0  0.00   0.0
1RXS J163759.7-26062  249.460  -26.009 8.4  353.552  +13.907    6.5  2.32   2.8    0.0  0.00   0.0
SLX 1744-299_300      266.781  -30.076 0.0  359.196   -0.872    1.2  0.00   3.7    0.0  0.00   0.0
PKS 1830-211          278.334  -21.135 0.0   12.065   -5.677    3.0  0.00   3.5    0.0  0.00   0.0
IGR J17254-3257       261.222  -32.929 7.1  354.238   +1.580    1.3  0.40   3.4    0.0  0.00   0.0

JEM-X

0659_jemx_mosa1.jpg 0659_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    4.9  0.36  13.7    0.7  0.21   3.6
1E 1740.7-2942        265.978  -29.745  359.116   -0.106    1.4  0.35   4.1    0.3  0.21   1.4
4U 1722-30            261.888  -30.802  356.320   +2.298    3.1  0.67   4.6    0.5  0.44   1.2
GRO J1750-27          267.298  -26.650    2.365   +0.508   14.1  0.58  24.5   10.3  0.32  32.2
GX 3+1                266.983  -26.562    2.295   +0.795   47.0  0.59  79.2    5.0  0.29  17.1
GX 354-0              262.989  -33.835  354.302   -0.150    5.5  1.30   4.2    1.8  0.97   1.9
GX 5-1                270.288  -25.072    5.085   -1.018   88.9  2.24  39.8    4.2  0.99   4.2
MXB 1730-335          263.350  -33.388  354.841   -0.158   10.0  1.00   9.9    2.0  0.70   2.8
SLX 1744-299_300      266.858  -29.999  359.297   -0.889    1.1  0.36   3.1    0.2  0.21   1.1
SLX 1746-331          267.465  -33.210  356.808   -2.985    3.9  0.70   5.5    0.0  0.00   0.0
NEW SOURCE            270.370  -31.109  359.864   -4.060    0.0  0.00   0.0    1.4  0.45   3.2


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