INTEGRAL Galactic bulge Monitoring

Revolution 1934: Observation start 2018-03-24T09:05 = MJD 58201.379
Total Observation GTI = 10859 seconds

IBIS/ISGRI

1934_isgri_mosa1.jpg 1934_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           255.992  -37.850 0.5  347.753   +2.167  149.8  1.89  79.1   31.3  0.65  47.9
1E 1740.7-2942        265.988  -29.751 1.0  359.115   -0.116   25.0  0.84  29.8    8.9  0.33  27.3
GX 354-0              262.988  -33.842 1.1  354.296   -0.153   24.4  0.90  27.1    3.9  0.34  11.5
GRS 1758-258          270.295  -25.746 1.7    4.502   -1.358   17.7  1.04  17.0    7.2  0.38  19.2
GX 1+4                262.985  -24.723 2.8    1.944   +4.826    8.8  0.94   9.4    0.0  0.00   0.0
H 1820-303            275.953  -30.344 3.0    2.817   -7.932   11.0  1.25   8.8    0.0  0.00   0.0
3A 1822-371           276.442  -37.127 3.8  356.829  -11.298   10.1  1.50   6.8    0.0  0.00   0.0
IGR J17559-2612       269.050  -26.205 3.9    3.546   -0.616    5.9  0.00   6.5    0.0  0.00   0.0
GX 3+1                266.983  -26.527 3.9    2.325   +0.812    5.2  0.80   6.5    0.0  0.00   0.0
GX 349+2              256.447  -36.450 4.2  349.087   +2.725    9.5  1.59   6.0    0.0  0.00   0.0
NEW SOURCE            258.437  -40.516 3.3  346.744   -0.945   12.8  1.65   7.7    3.1  0.44   7.0
NEW SOURCE            273.612  -19.246 3.0   11.673   -0.876   15.8  1.83   8.7    0.0  0.00   0.0
NEW SOURCE            267.116  -23.087 3.4    5.335   +2.484    8.2  1.07   7.6    0.0  0.00   0.0
NEW SOURCE            273.640  -37.019 4.1  355.919   -9.247    8.5  1.34   6.1    0.0  0.00   0.0
NEW SOURCE            267.943  -26.904 3.8    2.442   -0.117    6.0  0.90   6.7    0.0  0.00   0.0
NEW SOURCE            264.129  -20.809 4.3    5.830   +6.037    7.4  1.29   5.8    0.0  0.00   0.0
NEW SOURCE            262.040  -31.275 4.0  355.998   +1.928    6.3  1.00   6.3    0.0  0.00   0.0
NEW SOURCE            259.880  -36.519 0.0  350.655   +0.452    7.0  0.00   6.4    0.0  0.00   0.0
NEW SOURCE            260.193  -37.406 4.8  350.071   -0.261    6.2  1.23   5.2    0.0  0.00   0.0
NEW SOURCE            263.840  -27.978 4.1  359.617   +2.420    5.4  0.88   6.2    0.0  0.00   0.0
NEW SOURCE            273.080  -39.085 3.9  353.851   -9.796    9.6  1.49   6.5    0.0  0.00   0.0
NEW SOURCE            261.102  -26.091 0.0  359.858   +5.494    5.8  0.00   6.2    0.0  0.00   0.0
NEW SOURCE            270.276  -20.462 3.7    9.085   +1.276    9.9  1.40   6.9    0.0  0.00   0.0
NEW SOURCE            268.547  -40.893 4.3  350.575   -7.596    9.7  1.69   5.8    0.0  0.00   0.0
NEW SOURCE            264.443  -36.734 0.0  352.505   -2.716    6.1  0.00   6.0    0.0  0.00   0.0

JEM-X

1934_jemx_mosa1.jpg 1934_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    2.1  0.20  10.5    0.2  0.16   1.4
1E 1740.7-2942        265.978  -29.745  359.116   -0.106    1.6  0.19   8.6    0.5  0.16   3.4
4U 1722-30            261.888  -30.802  356.320   +2.298    1.2  0.32   3.8    0.0  0.00   0.0
GX 3+1                266.983  -26.564    2.294   +0.794   10.6  0.38  28.2    0.7  0.27   2.5
GX 354-0              262.989  -33.835  354.302   -0.150    6.3  0.43  14.6    1.3  0.41   3.2
GX 5-1                270.294  -25.080    5.081   -1.026   38.1  2.27  16.8    2.8  1.83   1.5
SLX 1744-299_300      266.858  -29.999  359.297   -0.889    1.2  0.20   6.1    0.0  0.00   0.0


Go back to the INTEGRAL Galactic bulge home page