INTEGRAL Galactic Bulge Monitoring

Revolution 0530: Observation start 2007-02-15 = MJD 54146

Total Observation GTI = 13960 seconds


ISGRI



ISGRI significance mosaic images. Left: 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 OSA7, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 206 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 103 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.


ISGRI Detected Sources 18-40 keV (A) and 40-100 keV (B)

Source Name             RA       dec   +/-    l        b     A(cps)  +/-   sig  B(cps)  +/-   sig  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
GX 354-0              262.988  -33.829 0.5  354.306   -0.146   25.8  0.32  80.1    7.7  0.26  29.7
4U 1700-377           255.986  -37.838 0.6  347.759   +2.178   38.5  0.58  66.6   10.5  0.45  23.4
GX 1+4                263.012  -24.748 0.7    1.937   +4.791   15.4  0.32  48.2    0.0  0.00   0.0
GRS 1758-258          270.307  -25.754 0.8    4.501   -1.370   12.3  0.32  38.6    8.5  0.26  32.7
1E 1740.7-2942        265.979  -29.746 0.9  359.116   -0.107   10.0  0.28  36.3    6.9  0.24  29.4
Ginga 1826-24         277.366  -23.795 1.0    9.273   -6.086   16.1  0.53  30.5    7.1  0.42  17.2
GX 349+2              256.435  -36.433 1.4  349.096   +2.742    9.7  0.47  20.6    0.0  0.00   0.0
H 1820-303            275.915  -30.376 1.6    2.773   -7.917    7.3  0.41  17.6    0.0  0.00   0.0
GX 5-1                270.290  -25.069 1.9    5.089   -1.018    4.4  0.31  14.2    0.0  0.00   0.0
3A 1822-371           276.452  -37.107 2.0  356.851  -11.297    6.9  0.51  13.6    0.0  0.00   0.0
GX 3+1                266.977  -26.565 2.3    2.290   +0.798    3.3  0.29  11.5    0.0  0.00   0.0
GX 17+2               273.991  -14.053 2.3   16.410   +1.282   23.3  2.00  11.6    0.0  0.00   0.0
4U 1722-30            261.885  -30.821 2.3  356.302   +2.290    3.4  0.30  11.5    1.6  0.25   6.3
GRS 1741.9-2853       266.342  -28.930 3.0  359.977   +0.051    2.4  0.28   8.6    0.8  0.24   3.4
GX 9+1                270.384  -20.545 2.9    9.063   +1.147    3.8  0.42   9.0    0.0  0.00   0.0
IGR J17252-3616       261.303  -36.271 3.2  351.510   -0.351    3.1  0.38   8.1    0.0  0.00   0.0
SLX 1735-269          264.545  -26.995 4.1    0.783   +2.420    1.8  0.29   6.1    1.7  0.24   6.9
SLX 1744-299_300      266.822  -29.985 4.6  359.292   -0.855    1.5  0.28   5.5    1.0  0.23   4.3
H 1702-429            256.524  -43.083 4.8  343.832   -1.324    7.8  1.49   5.2    0.0  0.00   0.0
SAX J1712.6-3739      258.214  -37.552 5.5  349.042   +0.935    2.2  0.49   4.5    0.0  0.00   0.0
V2400 Oph             258.254  -24.232 5.1  359.933   +8.671    1.9  0.39   4.8    0.0  0.00   0.0
SLX 1737-282          265.128  -28.262 5.3  359.984   +1.308    1.3  0.29   4.7    0.0  0.00   0.0
IGR J17200-3116       259.933  -31.242 5.8  355.011   +3.435    1.3  0.31   4.2    0.0  0.00   0.0
XTE J1710-281         257.536  -28.173 6.4  356.315   +6.909    1.4  0.37   3.8    0.0  0.00   0.0
Oph Cluster           258.063  -23.286 0.0    0.614   +9.357    1.6  0.00   3.7    0.0  0.00   0.0
1H 1746-370           267.525  -37.060 6.0  353.513   -4.990    1.6  0.40   4.1    0.0  0.00   0.0
GRS 1734-292          264.317  -29.187 8.2  358.823   +1.417    0.8  0.27   2.9    0.0  0.00   0.0
3A 1728-169           262.936  -16.941 6.7    8.531   +9.047    2.6  0.74   3.6    0.0  0.00   0.0

JEM-X



JEM-X significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.

Note: Sources labelled were detected with in the 3-10 keV image > 5σ and 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 ~ 88 cps); B = 10-25 keV (1 Crab ~ 32 cps).

NOTE: 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.


JEM-X Detected Sources in 3-10 keV (A) and 10-25 keV (B).

Source Name             RA      dec       l        b     A(cps)  +/-  B(cps)  +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
GX 354-0              262.989  -33.835  354.302   -0.150   11.5  1.18    4.1  0.89
4U 1722-30            261.888  -30.802  356.320   +2.298    4.1  0.62    0.9  0.41
1A 1742-294           266.523  -29.515  359.559   -0.389    2.4  0.28    0.6  0.18
GX 3+1                266.983  -26.564    2.294   +0.794   35.8  0.55    4.5  0.29
GX 5-1                270.284  -25.079    5.077   -1.019   78.8  2.09    6.3  0.90


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