INTEGRAL Galactic Bulge Monitoring

Revolution 0543: Observation start 2007-03-25 = MJD 54184

Total Observation GTI = 12136 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 1+4                263.009  -24.742 0.6    1.940   +4.797   22.8  0.33  68.7    0.0  0.00   0.0
GX 5-1                270.277  -25.077 0.6    5.076   -1.012   17.9  0.31  58.0    1.3  0.25   5.3
GRS 1758-258          270.305  -25.746 0.9    4.506   -1.365   12.1  0.32  38.1    8.9  0.26  34.5
Ginga 1826-24         277.361  -23.796 0.9    9.270   -6.082   18.6  0.56  33.4    7.0  0.43  16.4
1E 1740.7-2942        265.975  -29.737 1.0  359.121   -0.099   10.3  0.33  31.1    6.7  0.28  23.9
GX 354-0              262.990  -33.818 1.5  354.316   -0.142    7.1  0.38  18.6    0.0  0.00   0.0
1A 1742-294           266.504  -29.503 1.6  359.561   -0.369    5.7  0.32  18.0    1.8  0.00   6.7
H 1820-303            275.889  -30.366 1.8    2.772   -7.893    7.0  0.44  15.8    0.0  0.00   0.0
GX 3+1                266.978  -26.568 2.0    2.288   +0.795    4.5  0.33  13.8    0.0  0.00   0.0
GX 9+1                270.448  -20.483 2.2    9.146   +1.125    5.3  0.43  12.3    0.0  0.00   0.0
4U 1700-377           255.981  -37.830 2.1  347.763   +2.185    9.8  0.77  12.7    3.9  0.60   6.5
GRS 1741.9-2853       266.331  -28.898 2.8  359.999   +0.075    2.9  0.30   9.4    1.2  0.26   4.9
OAO 1657-415          255.180  -41.656 2.5  344.358   +0.333   24.0  2.26  10.6    6.4  1.70   3.8
3A 1822-371           276.447  -37.067 2.8  356.886  -11.276    5.7  0.61   9.4    0.0  0.00   0.0
4U 1722-30            261.894  -30.804 2.4  356.321   +2.292    4.0  0.37  11.0    2.0  0.29   6.9
GX 349+2              256.429  -36.388 2.8  349.128   +2.774    5.9  0.63   9.4    0.0  0.00   0.0
GX 13+1               273.628  -17.133 3.6   13.536   +0.120    4.7  0.66   7.1    0.0  0.00   0.0
IGR J18027-2016       270.681  -20.183 0.0    9.515   +1.083    2.8  0.00   6.4    0.0  0.00   0.0
GX 17+2               273.988  -14.026 3.6   16.432   +1.298   10.4  1.47   7.1    0.0  0.00   0.0
SLX 1735-269          264.529  -27.031 4.1    0.744   +2.412    2.0  0.33   6.2    2.1  0.28   7.5
SLX 1744-299_300      266.850  -29.987 4.1  359.304   -0.877    1.9  0.30   6.2    0.0  0.00   0.0
XB 1832-330           278.919  -33.000 4.5    1.518  -11.365    3.3  0.60   5.5    2.0  0.46   4.4
3A 1728-169           262.952  -16.951 4.7    8.532   +9.029    3.3  0.63   5.2    0.0  0.00   0.0
IGR J16500-3307       252.443  -33.178 0.0  349.628   +7.330    3.6  0.00   4.1    0.0  0.00   0.0
GRS 1734-292          264.330  -29.118 7.5  358.886   +1.444    1.1  0.33   3.2    0.0  0.00   0.0
AX J1749.1-2733       267.216  -27.578 0.0    1.532   +0.093    1.1  0.00   3.8    0.9  0.00   3.8
NEW_1                 257.264  -31.092 3.9  353.802   +5.381    2.9  0.45   6.4    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 3+1                266.983  -26.564    2.294   +0.794   29.7  0.52    3.8  0.26
GX 5-1                270.284  -25.079    5.077   -1.019   77.0  1.34   15.4  0.66


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