INTEGRAL Galactic Bulge MonitoringRevolution 0408: Observation start 2006-02-14 = MJD 53780
Total Observation GTI = 12503 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
4U 1700-377 255.976 -37.848 0.7 347.746 +2.178 29.5 0.62 47.4 7.6 0.48 15.7
XTE J1817-330 274.422 -33.025 0.8 359.808 -7.991 17.1 0.38 45.0 6.8 0.30 22.4
GRS 1758-258 270.297 -25.746 0.9 4.503 -1.359 11.8 0.31 38.4 7.4 0.25 29.7
GX 349+2 256.442 -36.425 0.9 349.105 +2.743 20.2 0.54 37.8 0.0 0.00 0.0
GX 5-1 270.280 -25.083 0.9 5.072 -1.018 12.3 0.34 36.5 0.0 0.00 0.0
Ginga 1826-24 277.371 -23.797 0.9 9.274 -6.090 18.4 0.52 35.3 7.7 0.40 19.2
GX 1+4 263.008 -24.744 0.9 1.938 +4.796 11.4 0.33 35.0 0.0 0.00 0.0
1A 1742-294 266.513 -29.512 1.3 359.558 -0.381 6.2 0.27 23.3 2.7 0.22 12.1
GX 354-0 262.997 -33.823 1.8 354.316 -0.149 4.8 0.31 15.5 0.0 0.00 0.0
GX 17+2 274.009 -14.040 2.3 16.431 +1.273 21.7 1.88 11.5 0.0 0.00 0.0
H 1820-303 275.902 -30.385 2.4 2.760 -7.912 4.3 0.40 10.9 0.0 0.00 0.0
4U 1722-30 261.871 -30.814 3.0 356.301 +2.303 2.6 0.31 8.6 1.5 0.25 5.9
3A 1822-371 276.433 -37.172 3.1 356.784 -11.311 4.4 0.53 8.3 1.6 0.00 3.8
IGR J17456-2901 266.436 -29.004 4.4 359.956 -0.058 1.4 0.25 5.7 0.0 0.00 0.0
SLX 1735-269 264.549 -26.965 3.7 0.810 +2.433 2.0 0.28 6.9 1.5 0.24 6.1
SLX 1744-299_300 266.881 -30.029 3.3 359.281 -0.921 2.3 0.30 7.8 0.0 0.00 0.0
GX 9+1 270.401 -20.532 4.5 9.082 +1.139 2.3 0.42 5.6 0.0 0.00 0.0
GX 13+1 273.701 -17.126 4.3 13.576 +0.063 4.3 0.74 5.9 0.0 0.00 0.0
GX 3+1 266.996 -26.588 4.4 2.279 +0.771 1.5 0.27 5.7 0.0 0.00 0.0
Oph Cluster 258.150 -23.296 5.0 0.652 +9.286 2.2 0.44 5.0 0.0 0.00 0.0
SLX 1737-282 265.125 -28.361 5.0 359.899 +1.258 1.4 0.28 5.0 0.0 0.00 0.0
AX J1749.1-2733 267.349 -27.573 5.5 1.597 -0.006 1.4 0.31 4.4 0.0 0.00 0.0
XB 1832-330 278.891 -32.894 6.5 1.605 -11.299 2.1 0.00 3.7 1.8 0.00 4.1
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 > 10σ 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).
NOTES: Fluxes for light curves are extracted from the images using mosaic_spec; 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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
XTE J1739-285 264.975 -28.496 359.714 +1.298 4.9 0.39 0.8 0.22
GRS 1747-312 267.690 -31.292 358.555 -2.168 2.7 0.54 1.0 0.61
GX 354-0 262.989 -33.835 354.302 -0.150 19.9 1.57 4.8 0.98
GX 3+1 266.983 -26.564 2.294 +0.794 20.9 0.56 2.8 0.29
GX 5-1 270.284 -25.079 5.077 -1.019 107.8 2.29 13.3 0.96
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Revolution 0408: Observation start 2006-02-14 = MJD 53780
Total Observation GTI = 12503 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 4U 1700-377 255.976 -37.848 0.7 347.746 +2.178 29.5 0.62 47.4 7.6 0.48 15.7 XTE J1817-330 274.422 -33.025 0.8 359.808 -7.991 17.1 0.38 45.0 6.8 0.30 22.4 GRS 1758-258 270.297 -25.746 0.9 4.503 -1.359 11.8 0.31 38.4 7.4 0.25 29.7 GX 349+2 256.442 -36.425 0.9 349.105 +2.743 20.2 0.54 37.8 0.0 0.00 0.0 GX 5-1 270.280 -25.083 0.9 5.072 -1.018 12.3 0.34 36.5 0.0 0.00 0.0 Ginga 1826-24 277.371 -23.797 0.9 9.274 -6.090 18.4 0.52 35.3 7.7 0.40 19.2 GX 1+4 263.008 -24.744 0.9 1.938 +4.796 11.4 0.33 35.0 0.0 0.00 0.0 1A 1742-294 266.513 -29.512 1.3 359.558 -0.381 6.2 0.27 23.3 2.7 0.22 12.1 GX 354-0 262.997 -33.823 1.8 354.316 -0.149 4.8 0.31 15.5 0.0 0.00 0.0 GX 17+2 274.009 -14.040 2.3 16.431 +1.273 21.7 1.88 11.5 0.0 0.00 0.0 H 1820-303 275.902 -30.385 2.4 2.760 -7.912 4.3 0.40 10.9 0.0 0.00 0.0 4U 1722-30 261.871 -30.814 3.0 356.301 +2.303 2.6 0.31 8.6 1.5 0.25 5.9 3A 1822-371 276.433 -37.172 3.1 356.784 -11.311 4.4 0.53 8.3 1.6 0.00 3.8 IGR J17456-2901 266.436 -29.004 4.4 359.956 -0.058 1.4 0.25 5.7 0.0 0.00 0.0 SLX 1735-269 264.549 -26.965 3.7 0.810 +2.433 2.0 0.28 6.9 1.5 0.24 6.1 SLX 1744-299_300 266.881 -30.029 3.3 359.281 -0.921 2.3 0.30 7.8 0.0 0.00 0.0 GX 9+1 270.401 -20.532 4.5 9.082 +1.139 2.3 0.42 5.6 0.0 0.00 0.0 GX 13+1 273.701 -17.126 4.3 13.576 +0.063 4.3 0.74 5.9 0.0 0.00 0.0 GX 3+1 266.996 -26.588 4.4 2.279 +0.771 1.5 0.27 5.7 0.0 0.00 0.0 Oph Cluster 258.150 -23.296 5.0 0.652 +9.286 2.2 0.44 5.0 0.0 0.00 0.0 SLX 1737-282 265.125 -28.361 5.0 359.899 +1.258 1.4 0.28 5.0 0.0 0.00 0.0 AX J1749.1-2733 267.349 -27.573 5.5 1.597 -0.006 1.4 0.31 4.4 0.0 0.00 0.0 XB 1832-330 278.891 -32.894 6.5 1.605 -11.299 2.1 0.00 3.7 1.8 0.00 4.1
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 > 10σ 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).
NOTES: Fluxes for light curves are extracted from the images using mosaic_spec; 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== XTE J1739-285 264.975 -28.496 359.714 +1.298 4.9 0.39 0.8 0.22 GRS 1747-312 267.690 -31.292 358.555 -2.168 2.7 0.54 1.0 0.61 GX 354-0 262.989 -33.835 354.302 -0.150 19.9 1.57 4.8 0.98 GX 3+1 266.983 -26.564 2.294 +0.794 20.9 0.56 2.8 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 107.8 2.29 13.3 0.96
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