INTEGRAL Galactic Bulge MonitoringRevolution 0482: Observation start 1999-12-31 = MJD 51544
Total Observation GTI = 22765 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 1700-377 255.984 -37.849 0.3 347.750 +2.172 76.6 0.50 152.5 21.6 0.38 57.1
GX 354-0 262.986 -33.834 0.4 354.301 -0.148 25.5 0.25 103.5 6.8 0.20 34.5
IGR J17497-2821 267.408 -28.349 0.5 0.958 -0.450 15.8 0.22 70.4 10.7 0.18 58.1
GX 1+4 263.007 -24.741 0.6 1.940 +4.799 14.4 0.23 62.9 0.0 0.00 0.0
Ginga 1826-24 277.378 -23.797 0.8 9.277 -6.096 16.9 0.41 41.6 6.4 0.31 20.5
H 1820-303 275.922 -30.357 0.8 2.793 -7.914 12.0 0.31 38.8 0.0 0.00 0.0
GX 5-1 270.288 -25.095 0.9 5.065 -1.029 8.8 0.26 34.0 0.0 0.00 0.0
GX 349+2 256.438 -36.421 1.0 349.106 +2.748 13.4 0.41 32.6 0.0 0.00 0.0
1E 1740.7-2942 265.988 -29.749 1.0 359.117 -0.115 6.5 0.21 31.1 4.4 0.17 25.5
GRS 1758-258 270.295 -25.733 1.1 4.514 -1.351 6.7 0.24 28.1 4.6 0.19 24.1
1A 1742-294 266.513 -29.510 1.1 359.559 -0.379 5.8 0.20 28.6 1.9 0.17 11.4
4U 1722-30 261.885 -30.789 1.7 356.329 +2.307 3.9 0.24 16.4 1.8 0.19 9.8
3A 1822-371 276.438 -37.090 1.9 356.862 -11.279 6.4 0.43 14.7 0.0 0.00 0.0
OAO 1657-415 255.207 -41.663 2.2 344.365 +0.313 12.3 1.00 12.3 4.2 0.75 5.5
GX 17+2 274.013 -14.029 2.5 16.441 +1.275 20.7 1.91 10.9 0.0 0.00 0.0
GX 9+1 270.406 -20.511 2.8 9.102 +1.145 3.4 0.35 9.5 0.0 0.00 0.0
GX 3+1 266.966 -26.545 2.7 2.302 +0.817 2.2 0.23 9.9 0.0 0.00 0.0
GRS 1734-292 264.352 -29.145 3.1 358.874 +1.413 2.1 0.24 8.4 1.1 0.20 5.7
SLX 1744-299_300 266.896 -30.020 0.0 359.296 -0.928 1.6 0.00 7.4 0.0 0.00 0.0
SLX 1735-269 264.586 -26.999 3.7 0.799 +2.387 1.6 0.24 6.8 0.8 0.20 3.9
IGR J17252-3616 261.290 -36.395 0.0 351.401 -0.412 2.0 0.00 6.4 0.0 0.00 0.0
IGR J18027-2016 270.734 -20.319 0.0 9.421 +0.973 2.3 0.00 6.3 0.0 0.00 0.0
3A 1728-169 262.935 -16.966 4.4 8.510 +9.035 3.2 0.57 5.6 0.0 0.00 0.0
IGR J17475-2822 266.693 -28.473 4.8 0.527 +0.025 1.1 0.00 5.2 0.0 0.00 0.0
SLX 1737-282 265.198 -28.330 5.1 359.959 +1.220 1.0 0.21 4.8 0.9 0.17 5.1
IGR J17456-2901 266.392 -28.944 0.0 359.987 +0.006 0.9 0.00 4.5 0.0 0.00 0.0
1RXS J174607.8-21333 266.541 -21.654 5.2 6.290 +3.679 1.3 0.28 4.7 0.0 0.00 0.0
GX 13+1 273.639 -17.169 4.8 13.510 +0.095 3.3 0.62 5.2 0.0 0.00 0.0
NEW_0365 250.455 -34.454 4.8 347.571 +7.776 4.3 0.82 5.2 0.0 0.00 0.0
KS 1741-293 266.093 -29.334 0.0 359.519 +0.025 0.8 0.00 3.9 0.0 0.00 0.0
XB 1832-330 278.894 -33.035 5.1 1.476 -11.361 2.1 0.43 4.8 0.0 0.00 0.0
IGR J17204-3554 260.120 -35.898 6.4 351.275 +0.648 1.2 0.32 3.8 0.0 0.00 0.0
IGR J17254-3257 261.299 -32.981 7.8 354.231 +1.497 0.7 0.24 3.1 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 > 5σ 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).
NOTE: 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 1.8 0.35 0.9 0.17
GX 354-0 262.989 -33.835 354.302 -0.150 15.4 0.99 5.4 0.68
1A 1742-294 266.523 -29.515 359.559 -0.389 1.4 0.22 0.7 0.14
GX 3+1 266.983 -26.564 2.294 +0.794 27.1 0.47 3.5 0.25
GX 5-1 270.284 -25.079 5.077 -1.019 93.1 1.98 9.7 0.86
IGR J17497-2821 267.404 -28.358 0.949 -0.451 3.1 0.30 1.8 0.19
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.8 0.25 0.5 0.17
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Revolution 0482: Observation start 1999-12-31 = MJD 51544
Total Observation GTI = 22765 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 1700-377 255.984 -37.849 0.3 347.750 +2.172 76.6 0.50 152.5 21.6 0.38 57.1 GX 354-0 262.986 -33.834 0.4 354.301 -0.148 25.5 0.25 103.5 6.8 0.20 34.5 IGR J17497-2821 267.408 -28.349 0.5 0.958 -0.450 15.8 0.22 70.4 10.7 0.18 58.1 GX 1+4 263.007 -24.741 0.6 1.940 +4.799 14.4 0.23 62.9 0.0 0.00 0.0 Ginga 1826-24 277.378 -23.797 0.8 9.277 -6.096 16.9 0.41 41.6 6.4 0.31 20.5 H 1820-303 275.922 -30.357 0.8 2.793 -7.914 12.0 0.31 38.8 0.0 0.00 0.0 GX 5-1 270.288 -25.095 0.9 5.065 -1.029 8.8 0.26 34.0 0.0 0.00 0.0 GX 349+2 256.438 -36.421 1.0 349.106 +2.748 13.4 0.41 32.6 0.0 0.00 0.0 1E 1740.7-2942 265.988 -29.749 1.0 359.117 -0.115 6.5 0.21 31.1 4.4 0.17 25.5 GRS 1758-258 270.295 -25.733 1.1 4.514 -1.351 6.7 0.24 28.1 4.6 0.19 24.1 1A 1742-294 266.513 -29.510 1.1 359.559 -0.379 5.8 0.20 28.6 1.9 0.17 11.4 4U 1722-30 261.885 -30.789 1.7 356.329 +2.307 3.9 0.24 16.4 1.8 0.19 9.8 3A 1822-371 276.438 -37.090 1.9 356.862 -11.279 6.4 0.43 14.7 0.0 0.00 0.0 OAO 1657-415 255.207 -41.663 2.2 344.365 +0.313 12.3 1.00 12.3 4.2 0.75 5.5 GX 17+2 274.013 -14.029 2.5 16.441 +1.275 20.7 1.91 10.9 0.0 0.00 0.0 GX 9+1 270.406 -20.511 2.8 9.102 +1.145 3.4 0.35 9.5 0.0 0.00 0.0 GX 3+1 266.966 -26.545 2.7 2.302 +0.817 2.2 0.23 9.9 0.0 0.00 0.0 GRS 1734-292 264.352 -29.145 3.1 358.874 +1.413 2.1 0.24 8.4 1.1 0.20 5.7 SLX 1744-299_300 266.896 -30.020 0.0 359.296 -0.928 1.6 0.00 7.4 0.0 0.00 0.0 SLX 1735-269 264.586 -26.999 3.7 0.799 +2.387 1.6 0.24 6.8 0.8 0.20 3.9 IGR J17252-3616 261.290 -36.395 0.0 351.401 -0.412 2.0 0.00 6.4 0.0 0.00 0.0 IGR J18027-2016 270.734 -20.319 0.0 9.421 +0.973 2.3 0.00 6.3 0.0 0.00 0.0 3A 1728-169 262.935 -16.966 4.4 8.510 +9.035 3.2 0.57 5.6 0.0 0.00 0.0 IGR J17475-2822 266.693 -28.473 4.8 0.527 +0.025 1.1 0.00 5.2 0.0 0.00 0.0 SLX 1737-282 265.198 -28.330 5.1 359.959 +1.220 1.0 0.21 4.8 0.9 0.17 5.1 IGR J17456-2901 266.392 -28.944 0.0 359.987 +0.006 0.9 0.00 4.5 0.0 0.00 0.0 1RXS J174607.8-21333 266.541 -21.654 5.2 6.290 +3.679 1.3 0.28 4.7 0.0 0.00 0.0 GX 13+1 273.639 -17.169 4.8 13.510 +0.095 3.3 0.62 5.2 0.0 0.00 0.0 NEW_0365 250.455 -34.454 4.8 347.571 +7.776 4.3 0.82 5.2 0.0 0.00 0.0 KS 1741-293 266.093 -29.334 0.0 359.519 +0.025 0.8 0.00 3.9 0.0 0.00 0.0 XB 1832-330 278.894 -33.035 5.1 1.476 -11.361 2.1 0.43 4.8 0.0 0.00 0.0 IGR J17204-3554 260.120 -35.898 6.4 351.275 +0.648 1.2 0.32 3.8 0.0 0.00 0.0 IGR J17254-3257 261.299 -32.981 7.8 354.231 +1.497 0.7 0.24 3.1 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 > 5σ 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).
NOTE: 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 1.8 0.35 0.9 0.17 GX 354-0 262.989 -33.835 354.302 -0.150 15.4 0.99 5.4 0.68 1A 1742-294 266.523 -29.515 359.559 -0.389 1.4 0.22 0.7 0.14 GX 3+1 266.983 -26.564 2.294 +0.794 27.1 0.47 3.5 0.25 GX 5-1 270.284 -25.079 5.077 -1.019 93.1 1.98 9.7 0.86 IGR J17497-2821 267.404 -28.358 0.949 -0.451 3.1 0.30 1.8 0.19 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.8 0.25 0.5 0.17
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