INTEGRAL Galactic Bulge MonitoringRevolution 0292: Observation start 2005-03-05 = MJD 53434
Total Observation GTI = 12329 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GRS 1758-258 270.306 -25.740 0.8 4.512 -1.363 13.1 0.32 41.4 8.7 0.26 33.7
1E 1740.7-2942 265.977 -29.750 0.8 359.111 -0.107 10.0 0.25 40.6 6.9 0.21 33.3
Ginga 1826-24 277.357 -23.791 1.0 9.274 -6.076 16.2 0.52 31.2 5.8 0.41 14.3
GX 349+2 256.418 -36.421 1.1 349.096 +2.761 13.6 0.49 27.8 0.0 0.00 0.0
GX 5-1 270.275 -25.085 1.2 5.068 -1.014 7.9 0.33 23.8 0.0 0.00 0.0
GRO J1655-40 253.501 -39.850 1.3 344.979 +2.453 21.5 0.95 22.6 15.8 0.72 21.8
GX 1+4 262.998 -24.773 1.5 1.909 +4.789 6.6 0.34 19.6 0.0 0.00 0.0
GX 354-0 262.983 -33.836 1.4 354.298 -0.147 6.7 0.32 20.6 0.0 0.00 0.0
1A 1742-294 266.511 -29.518 1.5 359.551 -0.382 4.8 0.25 19.2 1.6 0.00 7.4
H 1820-303 275.908 -30.340 1.5 2.803 -7.895 7.3 0.40 18.5 0.0 0.00 0.0
4U 1700-377 255.971 -37.857 1.7 347.737 +2.176 8.9 0.54 16.5 0.0 0.00 0.0
4U 1722-30 261.893 -30.793 1.8 356.330 +2.300 4.5 0.28 15.7 1.7 0.23 7.2
OAO 1657-415 255.203 -41.657 1.9 344.368 +0.319 21.5 1.48 14.6 8.2 1.07 7.7
GX 9+1 270.369 -20.516 2.3 9.081 +1.173 4.5 0.39 11.5 0.0 0.00 0.0
SLX 1735-269 264.571 -26.981 2.2 0.807 +2.407 3.2 0.26 12.3 0.0 0.00 0.0
3A 1822-371 276.433 -37.109 2.4 356.843 -11.284 6.0 0.53 11.4 0.0 0.00 0.0
GX 3+1 267.033 -26.539 3.1 2.338 +0.768 2.3 0.28 8.3 0.0 0.00 0.0
GX 17+2 273.967 -14.092 3.7 16.366 +1.284 14.0 2.04 6.9 0.0 0.00 0.0
3A 1728-169 262.907 -16.966 3.4 8.496 +9.057 4.8 0.64 7.5 0.0 0.00 0.0
Oph Cluster 258.151 -23.380 5.4 0.584 +9.237 1.8 0.39 4.6 0.0 0.00 0.0
SLX 1744-299_300 266.941 -29.954 6.2 359.372 -0.927 1.0 0.26 3.9 0.0 0.00 0.0
1E 1743.1-2843 266.532 -28.748 6.5 0.219 +0.003 0.9 0.25 3.7 0.0 0.00 0.0
GX 13+1 273.590 -17.083 6.4 13.563 +0.176 2.7 0.71 3.8 0.0 0.00 0.0
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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.34 1.4 0.21
GX 354-0 262.989 -33.835 354.302 -0.150 24.6 1.48 5.3 0.94
GX 3+1 266.983 -26.564 2.294 +0.794 26.6 0.54 4.0 0.28
GX 5-1 270.284 -25.079 5.077 -1.019 86.4 2.15 7.6 0.91
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.6 0.36 0.7 0.23
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Revolution 0292: Observation start 2005-03-05 = MJD 53434
Total Observation GTI = 12329 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRS 1758-258 270.306 -25.740 0.8 4.512 -1.363 13.1 0.32 41.4 8.7 0.26 33.7 1E 1740.7-2942 265.977 -29.750 0.8 359.111 -0.107 10.0 0.25 40.6 6.9 0.21 33.3 Ginga 1826-24 277.357 -23.791 1.0 9.274 -6.076 16.2 0.52 31.2 5.8 0.41 14.3 GX 349+2 256.418 -36.421 1.1 349.096 +2.761 13.6 0.49 27.8 0.0 0.00 0.0 GX 5-1 270.275 -25.085 1.2 5.068 -1.014 7.9 0.33 23.8 0.0 0.00 0.0 GRO J1655-40 253.501 -39.850 1.3 344.979 +2.453 21.5 0.95 22.6 15.8 0.72 21.8 GX 1+4 262.998 -24.773 1.5 1.909 +4.789 6.6 0.34 19.6 0.0 0.00 0.0 GX 354-0 262.983 -33.836 1.4 354.298 -0.147 6.7 0.32 20.6 0.0 0.00 0.0 1A 1742-294 266.511 -29.518 1.5 359.551 -0.382 4.8 0.25 19.2 1.6 0.00 7.4 H 1820-303 275.908 -30.340 1.5 2.803 -7.895 7.3 0.40 18.5 0.0 0.00 0.0 4U 1700-377 255.971 -37.857 1.7 347.737 +2.176 8.9 0.54 16.5 0.0 0.00 0.0 4U 1722-30 261.893 -30.793 1.8 356.330 +2.300 4.5 0.28 15.7 1.7 0.23 7.2 OAO 1657-415 255.203 -41.657 1.9 344.368 +0.319 21.5 1.48 14.6 8.2 1.07 7.7 GX 9+1 270.369 -20.516 2.3 9.081 +1.173 4.5 0.39 11.5 0.0 0.00 0.0 SLX 1735-269 264.571 -26.981 2.2 0.807 +2.407 3.2 0.26 12.3 0.0 0.00 0.0 3A 1822-371 276.433 -37.109 2.4 356.843 -11.284 6.0 0.53 11.4 0.0 0.00 0.0 GX 3+1 267.033 -26.539 3.1 2.338 +0.768 2.3 0.28 8.3 0.0 0.00 0.0 GX 17+2 273.967 -14.092 3.7 16.366 +1.284 14.0 2.04 6.9 0.0 0.00 0.0 3A 1728-169 262.907 -16.966 3.4 8.496 +9.057 4.8 0.64 7.5 0.0 0.00 0.0 Oph Cluster 258.151 -23.380 5.4 0.584 +9.237 1.8 0.39 4.6 0.0 0.00 0.0 SLX 1744-299_300 266.941 -29.954 6.2 359.372 -0.927 1.0 0.26 3.9 0.0 0.00 0.0 1E 1743.1-2843 266.532 -28.748 6.5 0.219 +0.003 0.9 0.25 3.7 0.0 0.00 0.0 GX 13+1 273.590 -17.083 6.4 13.563 +0.176 2.7 0.71 3.8 0.0 0.00 0.0
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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.34 1.4 0.21 GX 354-0 262.989 -33.835 354.302 -0.150 24.6 1.48 5.3 0.94 GX 3+1 266.983 -26.564 2.294 +0.794 26.6 0.54 4.0 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 86.4 2.15 7.6 0.91 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.6 0.36 0.7 0.23
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