INTEGRAL Galactic Bulge MonitoringRevolution 0347: Observation start 2005-08-16 = MJD 53598
Total Observation GTI = 12294 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
H 1820-303 275.934 -30.358 0.6 2.797 -7.924 22.0 0.40 55.2 5.2 0.30 17.0
IGR J17464-3213 266.568 -32.234 0.7 357.256 -1.836 14.3 0.31 46.3 6.6 0.25 25.9
4U 1700-377 255.985 -37.852 0.7 347.747 +2.170 27.1 0.58 46.8 8.4 0.44 19.2
GRS 1758-258 270.302 -25.747 0.8 4.505 -1.363 13.0 0.32 40.3 7.8 0.26 30.4
Ginga 1826-24 277.376 -23.809 1.0 9.265 -6.100 16.9 0.51 33.2 6.4 0.38 16.6
GX 349+2 256.430 -36.420 1.1 349.104 +2.754 14.4 0.51 28.1 0.0 0.00 0.0
GX 5-1 270.305 -25.080 1.2 5.086 -1.035 7.9 0.31 25.9 0.0 0.00 0.0
1E 1740.7-2942 265.974 -29.748 1.2 359.112 -0.104 7.5 0.29 25.5 4.7 0.24 19.4
GRO J1655-40 253.512 -39.870 1.4 344.968 +2.434 19.4 0.97 20.0 6.5 0.72 9.0
MXB 1730-335 263.356 -33.406 1.7 354.828 -0.172 4.7 0.28 16.7 0.0 0.00 0.0
GX 354-0 262.999 -33.825 1.6 354.314 -0.152 5.5 0.31 17.7 0.0 0.00 0.0
4U 1722-30 261.928 -30.813 2.1 356.330 +2.264 3.6 0.28 13.0 0.8 0.22 3.7
XTE J1818-245 274.602 -24.535 1.7 7.446 -4.190 6.6 0.41 16.1 1.6 0.31 5.0
GX 9+1 270.390 -20.494 2.2 9.110 +1.166 4.8 0.40 12.1 0.0 0.00 0.0
3A 1822-371 276.431 -37.095 2.7 356.854 -11.276 5.7 0.58 9.8 0.0 0.00 0.0
SLX 1735-269 264.597 -27.013 3.4 0.792 +2.370 2.0 0.26 7.6 1.5 0.21 6.9
KS 1741-293 266.212 -29.337 0.0 359.570 -0.065 2.0 0.00 7.9 0.9 0.00 4.0
IGR J17252-3616 261.284 -36.285 3.1 351.489 -0.346 3.3 0.38 8.5 0.0 0.00 0.0
SLX 1744-299_300 266.808 -29.941 3.9 359.324 -0.822 1.9 0.29 6.5 1.0 0.25 4.1
GX 17+2 274.036 -14.029 3.5 16.453 +1.255 12.2 1.69 7.2 0.0 0.00 0.0
1E 1743.1-2843 266.587 -28.688 3.7 0.295 -0.007 1.7 0.25 6.8 0.0 0.00 0.0
GX 3+1 267.011 -26.546 3.9 2.322 +0.781 1.8 0.28 6.5 0.0 0.00 0.0
GX 1+4 262.964 -24.725 4.5 1.932 +4.841 1.6 0.29 5.5 0.0 0.00 0.0
IGR J17456-2901 266.401 -29.008 0.0 359.937 -0.034 1.2 0.00 5.0 0.0 0.00 0.0
OAO 1657-415 255.219 -41.639 4.6 344.389 +0.321 6.7 1.23 5.5 0.0 0.00 0.0
XB 1832-330 278.874 -33.024 5.3 1.479 -11.341 2.5 0.53 4.7 0.0 0.00 0.0
GX 13+1 273.626 -17.200 6.2 13.476 +0.090 2.7 0.71 3.9 0.0 0.00 0.0
3A 1728-169 262.953 -16.975 0.0 8.511 +9.015 2.5 0.00 3.8 0.0 0.00 0.0
SLX 1737-282 265.158 -28.254 7.5 0.005 +1.290 0.9 0.29 3.2 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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
MXB 1730-335 263.350 -33.388 354.841 -0.158 13.8 1.41 2.6 0.75
GX 354-0 262.989 -33.835 354.302 -0.150 11.3 1.66 2.9 0.95
4U 1722-30 261.888 -30.802 356.320 +2.298 4.5 0.67 1.5 0.46
1A 1742-294 266.523 -29.515 359.559 -0.389 3.0 0.31 0.7 0.18
GX 3+1 266.983 -26.564 2.294 +0.794 20.8 0.54 3.1 0.27
GX 5-1 270.284 -25.079 5.077 -1.019 93.0 2.13 9.8 0.94
IGR J17464-3213 266.567 -32.229 357.260 -1.832 15.5 0.57 2.9 0.31
Go back to Bulge home page
Revolution 0347: Observation start 2005-08-16 = MJD 53598
Total Observation GTI = 12294 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== H 1820-303 275.934 -30.358 0.6 2.797 -7.924 22.0 0.40 55.2 5.2 0.30 17.0 IGR J17464-3213 266.568 -32.234 0.7 357.256 -1.836 14.3 0.31 46.3 6.6 0.25 25.9 4U 1700-377 255.985 -37.852 0.7 347.747 +2.170 27.1 0.58 46.8 8.4 0.44 19.2 GRS 1758-258 270.302 -25.747 0.8 4.505 -1.363 13.0 0.32 40.3 7.8 0.26 30.4 Ginga 1826-24 277.376 -23.809 1.0 9.265 -6.100 16.9 0.51 33.2 6.4 0.38 16.6 GX 349+2 256.430 -36.420 1.1 349.104 +2.754 14.4 0.51 28.1 0.0 0.00 0.0 GX 5-1 270.305 -25.080 1.2 5.086 -1.035 7.9 0.31 25.9 0.0 0.00 0.0 1E 1740.7-2942 265.974 -29.748 1.2 359.112 -0.104 7.5 0.29 25.5 4.7 0.24 19.4 GRO J1655-40 253.512 -39.870 1.4 344.968 +2.434 19.4 0.97 20.0 6.5 0.72 9.0 MXB 1730-335 263.356 -33.406 1.7 354.828 -0.172 4.7 0.28 16.7 0.0 0.00 0.0 GX 354-0 262.999 -33.825 1.6 354.314 -0.152 5.5 0.31 17.7 0.0 0.00 0.0 4U 1722-30 261.928 -30.813 2.1 356.330 +2.264 3.6 0.28 13.0 0.8 0.22 3.7 XTE J1818-245 274.602 -24.535 1.7 7.446 -4.190 6.6 0.41 16.1 1.6 0.31 5.0 GX 9+1 270.390 -20.494 2.2 9.110 +1.166 4.8 0.40 12.1 0.0 0.00 0.0 3A 1822-371 276.431 -37.095 2.7 356.854 -11.276 5.7 0.58 9.8 0.0 0.00 0.0 SLX 1735-269 264.597 -27.013 3.4 0.792 +2.370 2.0 0.26 7.6 1.5 0.21 6.9 KS 1741-293 266.212 -29.337 0.0 359.570 -0.065 2.0 0.00 7.9 0.9 0.00 4.0 IGR J17252-3616 261.284 -36.285 3.1 351.489 -0.346 3.3 0.38 8.5 0.0 0.00 0.0 SLX 1744-299_300 266.808 -29.941 3.9 359.324 -0.822 1.9 0.29 6.5 1.0 0.25 4.1 GX 17+2 274.036 -14.029 3.5 16.453 +1.255 12.2 1.69 7.2 0.0 0.00 0.0 1E 1743.1-2843 266.587 -28.688 3.7 0.295 -0.007 1.7 0.25 6.8 0.0 0.00 0.0 GX 3+1 267.011 -26.546 3.9 2.322 +0.781 1.8 0.28 6.5 0.0 0.00 0.0 GX 1+4 262.964 -24.725 4.5 1.932 +4.841 1.6 0.29 5.5 0.0 0.00 0.0 IGR J17456-2901 266.401 -29.008 0.0 359.937 -0.034 1.2 0.00 5.0 0.0 0.00 0.0 OAO 1657-415 255.219 -41.639 4.6 344.389 +0.321 6.7 1.23 5.5 0.0 0.00 0.0 XB 1832-330 278.874 -33.024 5.3 1.479 -11.341 2.5 0.53 4.7 0.0 0.00 0.0 GX 13+1 273.626 -17.200 6.2 13.476 +0.090 2.7 0.71 3.9 0.0 0.00 0.0 3A 1728-169 262.953 -16.975 0.0 8.511 +9.015 2.5 0.00 3.8 0.0 0.00 0.0 SLX 1737-282 265.158 -28.254 7.5 0.005 +1.290 0.9 0.29 3.2 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== MXB 1730-335 263.350 -33.388 354.841 -0.158 13.8 1.41 2.6 0.75 GX 354-0 262.989 -33.835 354.302 -0.150 11.3 1.66 2.9 0.95 4U 1722-30 261.888 -30.802 356.320 +2.298 4.5 0.67 1.5 0.46 1A 1742-294 266.523 -29.515 359.559 -0.389 3.0 0.31 0.7 0.18 GX 3+1 266.983 -26.564 2.294 +0.794 20.8 0.54 3.1 0.27 GX 5-1 270.284 -25.079 5.077 -1.019 93.0 2.13 9.8 0.94 IGR J17464-3213 266.567 -32.229 357.260 -1.832 15.5 0.57 2.9 0.31
Go back to Bulge home page