INTEGRAL Galactic bulge Monitoring

Revolution 1407: Observation start 2014-04-24T12:36 = MJD 56771.526
Total Observation GTI = 14125 seconds

IBIS/ISGRI

1407_isgri_mosa1.jpg 1407_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 J1744-28          266.134  -28.741 0.4    0.042   +0.304   47.0  0.35 134.8    6.2  0.22  28.7
4U 1700-377           255.992  -37.843 0.4  347.758   +2.171   69.8  0.70  99.8   29.0  0.40  71.9
GRS 1739-278          265.665  -27.750 0.5    0.670   +1.176   30.6  0.37  82.7    8.6  0.23  36.5
GX 1+4                263.005  -24.745 0.7    1.935   +4.798   21.8  0.41  53.0    0.0  0.00   0.0
GRS 1758-258          270.295  -25.724 1.2    4.522   -1.347   10.5  0.44  24.1    8.0  0.26  30.3
Ginga 1826-24         277.374  -23.801 1.3    9.271   -6.095   19.5  0.84  23.1    9.0  0.48  18.6
GX 349+2              256.433  -36.464 2.0  349.070   +2.725    8.6  0.62  13.9    0.0  0.00   0.0
H 1820-303            275.913  -30.365 2.5    2.782   -7.911    6.2  0.57  10.9    0.0  0.00   0.0
4U 1722-30            261.851  -30.831 3.0  356.278   +2.309    3.5  0.41   8.6    1.2  0.25   5.0
GX 354-0              262.995  -33.793 2.8  354.339   -0.131    3.6  0.39   9.3    0.0  0.00   0.0
1E 1740.7-2942        265.983  -29.752 3.2  359.112   -0.113    3.0  0.37   8.1    1.8  0.23   7.9
GX 9+1                270.401  -20.516 4.3    9.096   +1.147    3.5  0.60   5.8    0.0  0.00   0.0
SLX 1735-269          264.584  -27.020 3.8    0.780   +2.376    2.5  0.38   6.7    1.3  0.23   5.8
3A 1822-371           276.516  -37.115 4.9  356.866  -11.346    4.3  0.85   5.1    0.0  0.00   0.0
IGR J17445-2747       266.063  -27.764 0.0    0.843   +0.869    2.1  0.00   5.8    0.0  0.00   0.0
GX 13+1               273.723  -17.121 4.3   13.591   +0.047    8.2  1.39   5.9    0.0  0.00   0.0
IGR J18027-2016       270.602  -20.213 4.4    9.452   +1.132    3.4  0.00   5.6    0.0  0.00   0.0
Swift J175759.9-2246  269.403  -22.817 4.6    6.638   +0.806    2.7  0.00   5.5    0.0  0.00   0.0

JEM-X

1407_jemx_mosa1.jpg 1407_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 ~ 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+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           266.514  -29.518  359.553   -0.384    9.6  0.28  34.6    1.8  0.15  11.6
4U 1722-30            261.888  -30.802  356.320   +2.298    2.2  0.35   6.4    0.6  0.22   3.0
GRO J1744-28          266.138  -28.741    0.045   +0.301   24.9  0.31  80.7   12.8  0.17  73.5
GRS 1739-278          265.664  -27.748    0.671   +1.178   35.5  0.38  94.1    8.7  0.20  43.4
GX 1+4                263.009  -24.746    1.937   +4.795    8.2  1.33   6.1    4.5  0.84   5.3
GX 3+1                266.980  -26.570    2.287   +0.793   52.2  0.61  86.0    4.6  0.29  16.0
GX 354-0              262.989  -33.835  354.302   -0.150   15.7  0.50  31.2    2.8  0.33   8.6
GX 5-1                270.286  -25.078    5.079   -1.020  152.2  4.07  37.4    8.2  2.00   4.1
SLX 1735-269          264.571  -26.994    0.796   +2.400    2.0  0.43   4.7    0.4  0.23   1.8
SLX 1744-299_300      266.858  -29.999  359.297   -0.889    0.9  0.27   3.1    0.0  0.00   0.0
Swift J174535.5-2901  266.398  -29.026  359.920   -0.042    0.9  0.27   3.4    0.2  0.15   1.3
NEW SOURCE            269.021  -24.735    4.804   +0.146    9.7  2.03   4.8    0.0  0.00   0.0
NEW SOURCE            262.871  -29.721  357.691   +2.185    1.2  0.30   4.0    0.3  0.18   1.6


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