INTEGRAL Galactic bulge Monitoring

Revolution 1806: Observation start 2017-04-18T00:45 = MJD 57861.032
Total Observation GTI = 12472 seconds

IBIS/ISGRI

1806_isgri_mosa1.jpg 1806_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  
==================== ========  ======= === ======== ======== ====== ===== ===== ====== ===== =====
GRS 1716-249          259.911  -25.020 0.4    0.144   +6.984  108.7  0.89 121.8   52.0  0.41 128.4
4U 1700-377           255.984  -37.843 0.5  347.755   +2.176  133.1  1.57  84.8   34.2  0.71  48.5
GX 1+4                263.008  -24.741 0.8    1.940   +4.798   29.6  0.72  41.0    0.0  0.00   0.0
1E 1740.7-2942        265.991  -29.707 1.6  359.154   -0.095   12.1  0.70  17.3    7.7  0.34  22.8
KS 1741-293           266.166  -29.341 0.0  359.546   -0.033    9.7  0.00  16.5    3.8  0.00  13.3
GRS 1758-258          270.313  -25.804 2.0    4.460   -1.400    9.5  0.70  13.5    4.8  0.33  14.6
OAO 1657-415          255.196  -41.722 2.9  344.313   +0.283   39.1  4.38   8.9    9.3  1.83   5.1
H 1820-303            275.864  -30.393 2.6    2.738   -7.886    8.8  0.87  10.1    0.0  0.00   0.0
GX 5-1                270.288  -25.096 3.3    5.064   -1.029    4.8  0.63   7.7    0.0  0.00   0.0
GX 9+1                270.369  -20.615 3.3    8.995   +1.124    7.6  0.97   7.8    0.0  0.00   0.0
GX 354-0              262.952  -33.835 3.2  354.285   -0.124    6.3  0.77   8.1    0.0  0.00   0.0
SLX 1735-269          264.634  -27.013 0.0    0.810   +2.343    5.3  0.00   7.3    0.0  0.00   0.0
GX 349+2              256.449  -36.396 3.1  349.132   +2.756   11.3  1.34   8.4    0.0  0.00   0.0
3A 1822-371           276.425  -37.200 3.7  356.756  -11.317    8.0  0.00   6.8    0.0  0.00   0.0
H 1702-429            256.500  -43.070 3.7  343.831   -1.301   42.8  6.18   6.9    0.0  0.00   0.0
GRS 1739-278          265.705  -27.745 4.7    0.693   +1.149    3.3  0.64   5.3    1.8  0.33   5.5

JEM-X

1806_jemx_mosa1.jpg 1806_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           266.523  -29.515  359.559   -0.389    2.4  0.23  10.2    0.4  0.18   2.4
1E 1740.7-2942        265.978  -29.745  359.116   -0.106    1.3  0.24   5.4    1.1  0.19   5.8
4U 1722-30            261.888  -30.802  356.320   +2.298    3.3  0.80   4.1    0.0  0.00   0.0
GRS 1758-258          270.303  -25.741    4.511   -1.361    2.3  0.55   4.1    1.2  0.33   3.8
GX 3+1                266.979  -26.564    2.291   +0.796   18.1  0.35  51.0    3.0  0.24  12.9
GX 354-0              262.989  -33.835  354.302   -0.150    8.5  1.57   5.4    0.0  0.00   0.0
GX 5-1                270.273  -25.084    5.068   -1.013   65.4  0.83  78.8    8.8  0.44  20.1
KS 1741-293           266.223  -29.337  359.575   -0.074    1.8  0.23   7.9    0.8  0.18   4.6
CONFUSED ID           270.282  -25.079    5.077   -1.016   67.3  0.84  80.4    8.9  0.45  20.0
CONFUSED ID           270.270  -25.164    4.997   -1.049   16.2  0.71  22.8    2.1  0.40   5.3
NEW SOURCE            274.166  -28.404    3.831   -5.657    4.1  1.04   3.9    0.0  0.00   0.0
CONFUSED ID           270.270  -25.005    5.135   -0.971   24.6  0.80  30.6    2.7  0.46   6.0
NEW SOURCE            272.200  -24.907    6.078   -2.449    5.7  1.25   4.5    0.0  0.00   0.0


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