INTEGRAL Galactic bulge Monitoring

Revolution 1458: Observation start 2014-09-21T19:02 = MJD 56921.794
Total Observation GTI = 12190 seconds

IBIS/ISGRI

1458_isgri_mosa1.jpg 1458_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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
4U 1700-377           255.989  -37.851 0.5  347.750   +2.167   64.7  0.78  83.3   22.9  0.48  47.4
IGR J17464-3213       266.567  -32.233 0.5  357.256   -1.834   27.1  0.36  75.3   19.8  0.25  79.1
GX 354-0              263.004  -33.844 1.1  354.301   -0.166   12.6  0.47  27.0    5.1  0.31  16.6
GRS 1758-258          270.305  -25.749 1.2    4.505   -1.366   11.0  0.42  26.0    8.8  0.28  31.6
Ginga 1826-24         277.371  -23.793 1.3    9.277   -6.089   16.4  0.74  22.3    5.4  0.47  11.6
GX 5-1                270.262  -25.080 1.7    5.067   -1.002    7.5  0.45  16.8    1.1  0.30   3.8
GX 349+2              256.429  -36.426 1.5  349.098   +2.750   14.3  0.75  19.0    0.0  0.00   0.0
1E 1740.7-2942        265.992  -29.756 2.1  359.113   -0.121    4.6  0.35  13.1    2.3  0.24   9.6
GX 1+4                263.031  -24.750 2.6    1.944   +4.775    4.7  0.46  10.3    0.0  0.00   0.0
IGR J17252-3616       261.389  -36.240 2.9  351.574   -0.391    4.6  0.51   9.0    1.7  0.33   5.1
3A 1822-371           276.479  -37.026 3.9  356.935  -11.281    4.5  0.69   6.5    0.0  0.00   0.0
H 1820-303            275.935  -30.327 4.6    2.825   -7.911    3.2  0.60   5.4    0.0  0.00   0.0
IGR J17454-2919       266.380  -29.345 0.0  359.640   -0.194    1.8  0.00   5.2    0.0  0.00   0.0
SLX 1735-269          264.580  -27.002 4.6    0.794   +2.389    2.0  0.37   5.4    1.6  0.25   6.6
AX J1820.5-1434       275.046  -14.630 5.0   16.387   +0.109   13.2  2.66   5.0    0.0  0.00   0.0
4U 1722-30            261.902  -30.775 5.8  356.349   +2.303    1.9  0.46   4.2    0.0  0.00   0.0
IGR J17507-2856       267.745  -28.932 5.2    0.609   -1.002    1.7  0.37   4.7    1.1  0.25   4.5

JEM-X

1458_jemx_mosa1.jpg 1458_jemx_mosa2.jpg

JEM-X1+2 combined 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 ~ 109 cps [J1], 116 cps [J2]); B = 10-25 keV (1 Crab ~ 34 cps [J1], 32 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+2 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    6.8  0.25  26.8    1.1  0.13   8.8
1E 1740.7-2942        265.978  -29.745  359.116   -0.106    1.5  0.24   6.2    0.8  0.13   6.3
1E 1743.1-2843        266.587  -28.729    0.260   -0.029    0.9  0.26   3.3    0.2  0.14   1.5
4U 1722-30            261.888  -30.802  356.320   +2.298    6.0  0.46  13.2    1.4  0.27   5.2
CONFUSED ID           266.518  -29.557  359.521   -0.407    4.1  0.25  16.6    0.6  0.13   4.9
GRS 1739-278          265.659  -27.748    0.669   +1.181   17.1  0.33  51.7    0.0  0.00   0.0
GX 3+1                266.995  -26.558    2.304   +0.788   30.8  0.46  66.5    3.2  0.21  15.3
GX 354-0              262.989  -33.835  354.302   -0.150    7.2  0.73   9.8    2.5  0.47   5.4
GX 5-1                270.283  -25.080    5.076   -1.018  108.2  1.89  57.3   11.0  0.84  13.1
IGR J17464-3213       266.567  -32.229  357.260   -1.832    6.8  0.29  23.2    3.8  0.17  21.8
SLX 1744-299_300      266.858  -29.999  359.297   -0.889    3.0  0.24  12.4    0.7  0.13   5.2
NEW SOURCE            268.805  -25.262    4.249   +0.050    4.0  0.95   4.2    0.0  0.00   0.0
NEW SOURCE            268.520  -23.764    5.411   +1.030   10.8  2.69   4.0    1.9  1.41   1.3
Swift J1753.7-2544    268.478  -25.706    3.718   +0.080    2.8  0.69   4.0    0.0  0.00   0.0
NEW SOURCE            269.190  -33.319  357.443   -4.286    2.0  0.47   4.2    0.0  0.00   0.0
NEW SOURCE            266.313  -24.345    3.877   +2.462    3.8  1.05   3.6    0.7  0.55   1.2


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