INTEGRAL Galactic Bulge MonitoringRevolution 0474: Observation start 2006-08-31 = MJD 53978
Total Observation GTI = 12305 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 1700-377 255.981 -37.847 0.4 347.750 +2.175 71.9 0.65 110.3 17.8 0.48 37.1
GX 354-0 262.990 -33.833 0.6 354.304 -0.150 21.3 0.37 57.8 5.9 0.30 19.9
GX 1+4 263.010 -24.744 0.8 1.939 +4.795 16.5 0.39 42.4 0.0 0.00 0.0
Ginga 1826-24 277.375 -23.804 1.0 9.269 -6.097 17.6 0.56 31.6 7.1 0.42 17.0
GX 349+2 256.430 -36.431 1.1 349.095 +2.748 15.2 0.58 26.4 0.0 0.00 0.0
1A 1742-294 266.494 -29.506 1.3 359.554 -0.363 5.9 0.27 21.7 2.2 0.22 10.1
1E 1740.7-2942 265.983 -29.755 1.4 359.110 -0.114 5.6 0.28 20.0 3.0 0.23 13.4
GRS 1758-258 270.314 -25.765 1.5 4.494 -1.381 6.7 0.35 19.1 4.2 0.28 14.9
H 1820-303 275.915 -30.342 2.0 2.804 -7.902 6.0 0.44 13.6 0.0 0.00 0.0
GX 5-1 270.294 -25.117 2.7 5.048 -1.046 3.6 0.37 9.9 0.0 0.00 0.0
3A 1822-371 276.441 -37.137 2.5 356.820 -11.301 6.2 0.57 10.7 0.0 0.00 0.0
4U 1722-30 261.854 -30.785 2.5 356.318 +2.332 3.5 0.34 10.4 0.0 0.00 0.0
GX 9+1 270.402 -20.496 3.3 9.113 +1.155 3.3 0.43 7.8 0.0 0.00 0.0
GX 3+1 266.997 -26.561 3.2 2.302 +0.784 2.4 0.30 8.1 0.0 0.00 0.0
SLX 1744-299_300 266.839 -30.025 3.7 359.265 -0.888 1.9 0.28 6.8 1.2 0.23 5.4
1E 1742.9-2849 266.581 -28.886 4.2 0.123 -0.106 1.6 0.27 5.9 0.0 0.00 0.0
SLX 1735-269 264.576 -27.050 3.7 0.751 +2.367 2.1 0.30 6.9 1.1 0.24 4.7
IGR J17252-3616 261.246 -36.257 4.3 351.495 -0.305 2.5 0.00 5.9 0.0 0.00 0.0
Oph Cluster 258.056 -23.366 0.0 0.544 +9.317 2.1 0.00 4.7 0.0 0.00 0.0
XTE J1817-330 274.429 -33.112 6.1 359.733 -8.036 1.6 0.40 4.0 0.0 0.00 0.0
NEW_0347 251.507 -28.284 4.8 352.949 +11.053 4.9 0.94 5.2 0.0 0.00 0.0
1H 1746-370 267.506 -37.019 5.1 353.541 -4.956 2.0 0.41 4.8 0.0 0.00 0.0
NEW_0365 250.461 -34.422 6.1 347.599 +7.793 4.6 0.00 4.0 0.0 0.00 0.0
H 1705-440 257.156 -44.079 5.2 343.309 -2.287 15.6 3.33 4.7 0.0 0.00 0.0
V1223 Sgr 283.697 -31.155 6.6 4.945 -14.302 6.7 1.83 3.7 0.0 0.00 0.0
IGR J17544-2619 268.692 -26.355 6.3 3.255 -0.415 1.2 0.00 3.8 0.0 0.00 0.0
4U 1735-444 264.726 -44.459 5.6 346.041 -6.988 15.0 3.41 4.4 0.0 0.00 0.0
NEW_0287 256.656 -38.194 7.0 347.795 +1.542 2.2 0.64 3.4 0.0 0.00 0.0
GRS 1734-292 264.390 -29.160 5.9 358.879 +1.378 1.2 0.29 4.1 0.0 0.00 0.0
NEW_1 269.423 -38.416 4.3 353.084 -6.967 2.8 0.48 5.9 0.0 0.00 0.0
NEW_2 247.692 -36.770 4.3 344.318 +7.913 17.4 2.84 5.9 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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
GX 354-0 262.989 -33.835 354.302 -0.150 8.5 1.31 3.0 1.09
GX 3+1 266.983 -26.564 2.294 +0.794 23.4 0.55 3.5 0.30
GX 5-1 270.284 -25.079 5.077 -1.019 85.8 2.10 7.7 1.00
Go back to Bulge home page
Revolution 0474: Observation start 2006-08-31 = MJD 53978
Total Observation GTI = 12305 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 1700-377 255.981 -37.847 0.4 347.750 +2.175 71.9 0.65 110.3 17.8 0.48 37.1 GX 354-0 262.990 -33.833 0.6 354.304 -0.150 21.3 0.37 57.8 5.9 0.30 19.9 GX 1+4 263.010 -24.744 0.8 1.939 +4.795 16.5 0.39 42.4 0.0 0.00 0.0 Ginga 1826-24 277.375 -23.804 1.0 9.269 -6.097 17.6 0.56 31.6 7.1 0.42 17.0 GX 349+2 256.430 -36.431 1.1 349.095 +2.748 15.2 0.58 26.4 0.0 0.00 0.0 1A 1742-294 266.494 -29.506 1.3 359.554 -0.363 5.9 0.27 21.7 2.2 0.22 10.1 1E 1740.7-2942 265.983 -29.755 1.4 359.110 -0.114 5.6 0.28 20.0 3.0 0.23 13.4 GRS 1758-258 270.314 -25.765 1.5 4.494 -1.381 6.7 0.35 19.1 4.2 0.28 14.9 H 1820-303 275.915 -30.342 2.0 2.804 -7.902 6.0 0.44 13.6 0.0 0.00 0.0 GX 5-1 270.294 -25.117 2.7 5.048 -1.046 3.6 0.37 9.9 0.0 0.00 0.0 3A 1822-371 276.441 -37.137 2.5 356.820 -11.301 6.2 0.57 10.7 0.0 0.00 0.0 4U 1722-30 261.854 -30.785 2.5 356.318 +2.332 3.5 0.34 10.4 0.0 0.00 0.0 GX 9+1 270.402 -20.496 3.3 9.113 +1.155 3.3 0.43 7.8 0.0 0.00 0.0 GX 3+1 266.997 -26.561 3.2 2.302 +0.784 2.4 0.30 8.1 0.0 0.00 0.0 SLX 1744-299_300 266.839 -30.025 3.7 359.265 -0.888 1.9 0.28 6.8 1.2 0.23 5.4 1E 1742.9-2849 266.581 -28.886 4.2 0.123 -0.106 1.6 0.27 5.9 0.0 0.00 0.0 SLX 1735-269 264.576 -27.050 3.7 0.751 +2.367 2.1 0.30 6.9 1.1 0.24 4.7 IGR J17252-3616 261.246 -36.257 4.3 351.495 -0.305 2.5 0.00 5.9 0.0 0.00 0.0 Oph Cluster 258.056 -23.366 0.0 0.544 +9.317 2.1 0.00 4.7 0.0 0.00 0.0 XTE J1817-330 274.429 -33.112 6.1 359.733 -8.036 1.6 0.40 4.0 0.0 0.00 0.0 NEW_0347 251.507 -28.284 4.8 352.949 +11.053 4.9 0.94 5.2 0.0 0.00 0.0 1H 1746-370 267.506 -37.019 5.1 353.541 -4.956 2.0 0.41 4.8 0.0 0.00 0.0 NEW_0365 250.461 -34.422 6.1 347.599 +7.793 4.6 0.00 4.0 0.0 0.00 0.0 H 1705-440 257.156 -44.079 5.2 343.309 -2.287 15.6 3.33 4.7 0.0 0.00 0.0 V1223 Sgr 283.697 -31.155 6.6 4.945 -14.302 6.7 1.83 3.7 0.0 0.00 0.0 IGR J17544-2619 268.692 -26.355 6.3 3.255 -0.415 1.2 0.00 3.8 0.0 0.00 0.0 4U 1735-444 264.726 -44.459 5.6 346.041 -6.988 15.0 3.41 4.4 0.0 0.00 0.0 NEW_0287 256.656 -38.194 7.0 347.795 +1.542 2.2 0.64 3.4 0.0 0.00 0.0 GRS 1734-292 264.390 -29.160 5.9 358.879 +1.378 1.2 0.29 4.1 0.0 0.00 0.0 NEW_1 269.423 -38.416 4.3 353.084 -6.967 2.8 0.48 5.9 0.0 0.00 0.0 NEW_2 247.692 -36.770 4.3 344.318 +7.913 17.4 2.84 5.9 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 8.5 1.31 3.0 1.09 GX 3+1 266.983 -26.564 2.294 +0.794 23.4 0.55 3.5 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 85.8 2.10 7.7 1.00
Go back to Bulge home page