INTEGRAL Galactic Bulge MonitoringRevolution 0288: Observation start 2005-02-21 = MJD 53422
Total Observation GTI = 12409 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 1700-377 255.987 -37.842 0.5 347.756 +2.175 53.8 0.59 90.5 14.4 0.46 31.4
1E 1740.7-2942 265.972 -29.746 0.9 359.113 -0.101 9.4 0.25 38.0 6.6 0.21 32.0
GRS 1758-258 270.303 -25.741 0.9 4.510 -1.361 11.9 0.32 37.3 8.7 0.26 33.7
Ginga 1826-24 277.367 -23.795 1.0 9.275 -6.087 14.9 0.49 30.2 5.0 0.39 12.9
GX 354-0 262.983 -33.836 1.1 354.298 -0.147 8.3 0.29 28.9 0.0 0.00 0.0
GX 349+2 256.429 -36.415 1.4 349.107 +2.758 10.4 0.48 21.6 0.0 0.00 0.0
OAO 1657-415 255.194 -41.647 1.3 344.372 +0.330 28.1 1.25 22.4 6.3 0.92 6.8
H 1820-303 275.920 -30.362 1.5 2.788 -7.915 7.6 0.40 19.0 0.0 0.00 0.0
GX 1+4 263.002 -24.744 1.6 1.935 +4.801 5.4 0.30 18.0 0.0 0.00 0.0
4U 1722-30 261.888 -30.830 2.0 356.296 +2.283 4.0 0.30 13.7 1.3 0.24 5.3
3A 1822-371 276.467 -37.099 2.3 356.863 -11.304 6.7 0.57 11.7 0.0 0.00 0.0
GX 17+2 274.003 -14.014 2.6 16.450 +1.290 17.7 1.75 10.1 0.0 0.00 0.0
GX 9+1 270.394 -20.525 2.9 9.085 +1.148 3.8 0.41 9.1 0.0 0.00 0.0
SLX 1735-269 264.577 -27.012 2.8 0.784 +2.386 2.6 0.28 9.5 0.0 0.00 0.0
GX 5-1 270.286 -25.050 3.5 5.103 -1.006 2.3 0.32 7.2 0.0 0.00 0.0
GX 3+1 266.961 -26.550 2.9 2.296 +0.818 2.6 0.28 9.1 0.0 0.00 0.0
GRO J1655-40 253.499 -39.864 3.7 344.967 +2.446 5.9 0.86 6.8 2.5 0.00 3.9
SLX 1744-299_300 266.839 -30.050 4.6 359.245 -0.901 1.4 0.25 5.4 0.0 0.00 0.0
IGR J17456-2901 266.397 -28.928 4.2 0.003 +0.010 1.4 0.24 5.9 0.0 0.00 0.0
GX 13+1 273.695 -17.121 4.6 13.577 +0.071 3.9 0.72 5.4 0.0 0.00 0.0
IGR J17200-3116 259.999 -31.294 4.5 355.001 +3.359 1.8 0.31 5.6 0.0 0.00 0.0
IGR J17544-2619 268.589 -26.296 5.2 3.259 -0.305 1.4 0.30 4.7 0.0 0.00 0.0
3A 1728-169 262.946 -16.980 4.7 8.503 +9.019 3.2 0.61 5.2 0.0 0.00 0.0
1A 1742-294 266.483 -29.498 4.8 359.556 -0.350 1.2 0.24 5.1 0.0 0.00 0.0
1H 1746-370 267.656 -37.075 6.5 353.553 -5.087 1.5 0.40 3.7 0.0 0.00 0.0
XB 1832-330 278.908 -32.984 5.5 1.529 -11.349 2.3 0.52 4.5 0.0 0.00 0.0
IGR J17475-2822 266.935 -28.390 6.4 0.708 -0.114 0.9 0.00 3.8 0.0 0.00 0.0
Oph Cluster 258.183 -23.434 0.0 0.556 +9.182 1.3 0.00 3.7 0.0 0.00 0.0
H 1702-429 256.548 -43.072 6.5 343.851 -1.331 6.1 1.63 3.7 0.0 0.00 0.0
NEW_0287 256.634 -38.203 7.1 347.777 +1.550 1.9 0.00 3.4 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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
GX 354-0 262.989 -33.835 354.302 -0.150 19.1 1.32 5.3 0.87
1A 1742-294 266.523 -29.515 359.559 -0.389 1.6 0.27 0.5 0.18
GX 3+1 266.983 -26.564 2.294 +0.794 23.3 0.53 3.4 0.27
GX 5-1 270.284 -25.079 5.077 -1.019 83.3 2.02 5.7 0.84
Go back to Bulge home page
Revolution 0288: Observation start 2005-02-21 = MJD 53422
Total Observation GTI = 12409 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 1700-377 255.987 -37.842 0.5 347.756 +2.175 53.8 0.59 90.5 14.4 0.46 31.4 1E 1740.7-2942 265.972 -29.746 0.9 359.113 -0.101 9.4 0.25 38.0 6.6 0.21 32.0 GRS 1758-258 270.303 -25.741 0.9 4.510 -1.361 11.9 0.32 37.3 8.7 0.26 33.7 Ginga 1826-24 277.367 -23.795 1.0 9.275 -6.087 14.9 0.49 30.2 5.0 0.39 12.9 GX 354-0 262.983 -33.836 1.1 354.298 -0.147 8.3 0.29 28.9 0.0 0.00 0.0 GX 349+2 256.429 -36.415 1.4 349.107 +2.758 10.4 0.48 21.6 0.0 0.00 0.0 OAO 1657-415 255.194 -41.647 1.3 344.372 +0.330 28.1 1.25 22.4 6.3 0.92 6.8 H 1820-303 275.920 -30.362 1.5 2.788 -7.915 7.6 0.40 19.0 0.0 0.00 0.0 GX 1+4 263.002 -24.744 1.6 1.935 +4.801 5.4 0.30 18.0 0.0 0.00 0.0 4U 1722-30 261.888 -30.830 2.0 356.296 +2.283 4.0 0.30 13.7 1.3 0.24 5.3 3A 1822-371 276.467 -37.099 2.3 356.863 -11.304 6.7 0.57 11.7 0.0 0.00 0.0 GX 17+2 274.003 -14.014 2.6 16.450 +1.290 17.7 1.75 10.1 0.0 0.00 0.0 GX 9+1 270.394 -20.525 2.9 9.085 +1.148 3.8 0.41 9.1 0.0 0.00 0.0 SLX 1735-269 264.577 -27.012 2.8 0.784 +2.386 2.6 0.28 9.5 0.0 0.00 0.0 GX 5-1 270.286 -25.050 3.5 5.103 -1.006 2.3 0.32 7.2 0.0 0.00 0.0 GX 3+1 266.961 -26.550 2.9 2.296 +0.818 2.6 0.28 9.1 0.0 0.00 0.0 GRO J1655-40 253.499 -39.864 3.7 344.967 +2.446 5.9 0.86 6.8 2.5 0.00 3.9 SLX 1744-299_300 266.839 -30.050 4.6 359.245 -0.901 1.4 0.25 5.4 0.0 0.00 0.0 IGR J17456-2901 266.397 -28.928 4.2 0.003 +0.010 1.4 0.24 5.9 0.0 0.00 0.0 GX 13+1 273.695 -17.121 4.6 13.577 +0.071 3.9 0.72 5.4 0.0 0.00 0.0 IGR J17200-3116 259.999 -31.294 4.5 355.001 +3.359 1.8 0.31 5.6 0.0 0.00 0.0 IGR J17544-2619 268.589 -26.296 5.2 3.259 -0.305 1.4 0.30 4.7 0.0 0.00 0.0 3A 1728-169 262.946 -16.980 4.7 8.503 +9.019 3.2 0.61 5.2 0.0 0.00 0.0 1A 1742-294 266.483 -29.498 4.8 359.556 -0.350 1.2 0.24 5.1 0.0 0.00 0.0 1H 1746-370 267.656 -37.075 6.5 353.553 -5.087 1.5 0.40 3.7 0.0 0.00 0.0 XB 1832-330 278.908 -32.984 5.5 1.529 -11.349 2.3 0.52 4.5 0.0 0.00 0.0 IGR J17475-2822 266.935 -28.390 6.4 0.708 -0.114 0.9 0.00 3.8 0.0 0.00 0.0 Oph Cluster 258.183 -23.434 0.0 0.556 +9.182 1.3 0.00 3.7 0.0 0.00 0.0 H 1702-429 256.548 -43.072 6.5 343.851 -1.331 6.1 1.63 3.7 0.0 0.00 0.0 NEW_0287 256.634 -38.203 7.1 347.777 +1.550 1.9 0.00 3.4 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 19.1 1.32 5.3 0.87 1A 1742-294 266.523 -29.515 359.559 -0.389 1.6 0.27 0.5 0.18 GX 3+1 266.983 -26.564 2.294 +0.794 23.3 0.53 3.4 0.27 GX 5-1 270.284 -25.079 5.077 -1.019 83.3 2.02 5.7 0.84
Go back to Bulge home page