INTEGRAL Galactic Bulge MonitoringRevolution 0844: Observation start 2009-09-12T03:21 = MJD 55086.14
Total Observation GTI = 13816 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
1E 1740.7-2942 265.972 -29.749 0.8 359.110 -0.103 12.2 0.29 42.0 7.4 0.25 29.9
GX 5-1 270.280 -25.089 0.9 5.067 -1.020 11.9 0.35 34.3 0.0 0.00 0.0
GRS 1758-258 270.301 -25.732 1.1 4.517 -1.355 9.2 0.35 26.5 6.1 0.29 21.3
Ginga 1826-24 277.364 -23.793 1.1 9.275 -6.083 14.8 0.56 26.4 5.6 0.44 12.7
GX 1+4 263.008 -24.747 1.3 1.935 +4.794 8.2 0.35 23.5 0.0 0.00 0.0
IGR J17511-3057 267.810 -30.961 1.7 358.893 -2.088 5.5 0.33 16.5 2.3 0.28 8.1
H 1820-303 275.965 -30.380 1.8 2.789 -7.958 6.3 0.42 15.2 0.0 0.00 0.0
4U 1722-30 261.899 -30.818 2.5 356.312 +2.281 3.6 0.34 10.6 1.3 0.00 4.8
GX 349+2 256.460 -36.428 2.6 349.112 +2.730 5.9 0.57 10.3 0.0 0.00 0.0
3A 1822-371 276.483 -37.065 2.8 356.900 -11.300 6.3 0.66 9.5 0.0 0.00 0.0
GX 9+1 270.381 -20.552 2.7 9.055 +1.145 4.2 0.42 9.9 0.0 0.00 0.0
IGR J17586-2129 269.678 -21.388 3.2 8.003 +1.300 3.1 0.38 8.0 0.0 0.00 0.0
4U 1700-377 255.984 -37.826 3.2 347.768 +2.186 5.4 0.67 8.1 3.4 0.53 6.3
MXB 1730-335 263.432 -33.367 5.5 354.896 -0.204 1.5 0.34 4.5 0.0 0.00 0.0
GX 13+1 273.667 -17.144 3.7 13.544 +0.083 5.2 0.76 6.9 0.0 0.00 0.0
1A 1742-294 266.519 -29.530 4.5 359.545 -0.394 1.6 0.29 5.5 0.0 0.00 0.0
GX 17+2 273.925 -14.023 3.9 16.407 +1.353 11.5 1.80 6.4 0.0 0.00 0.0
XTE J1710-281 257.611 -28.167 4.3 356.360 +6.858 2.5 0.43 5.8 0.0 0.00 0.0
3A 1728-169 262.947 -17.006 5.2 8.481 +9.004 3.1 0.65 4.8 0.0 0.00 0.0
GX 354-0 263.074 -33.871 6.2 354.311 -0.229 1.3 0.33 4.0 0.0 0.00 0.0
1RXS J175113.3-20121 267.879 -20.234 5.9 8.154 +3.334 1.8 0.00 4.2 0.0 0.00 0.0
GX 3+1 267.047 -26.521 0.0 2.360 +0.767 1.2 0.00 4.0 0.0 0.00 0.0
NEW_1 282.367 -37.428 2.9 358.517 -15.727 12.1 1.33 9.1 0.0 0.00 0.0
NEW_2 282.679 -33.294 4.2 2.566 -14.357 7.2 1.14 6.1 0.0 0.00 0.0
NEW_3 284.201 -36.154 3.2 0.322 -16.609 17.8 2.03 8.2 0.0 0.00 0.0
NEW_4 285.160 -36.033 3.7 0.738 -17.285 21.0 3.00 6.9 0.0 0.00 0.0
NEW_5 280.935 -27.289 3.4 7.537 -10.515 6.4 0.88 7.5 0.0 0.00 0.0
NEW_6 269.890 -34.465 4.6 356.732 -5.357 2.0 0.36 5.4 0.0 0.00 0.0
NEW_7 266.572 -22.215 4.0 5.824 +3.364 2.2 0.35 6.3 0.0 0.00 0.0
NEW_8 261.882 -25.166 3.9 1.023 +5.421 2.2 0.34 6.4 0.0 0.00 0.0
NEW_9 270.000 -21.496 0.0 8.059 +0.986 2.3 0.00 6.0 0.0 0.00 0.0
NEW_10 262.029 -43.355 4.7 345.927 -4.756 9.5 1.79 5.3 0.0 0.00 0.0
NEW_11 275.876 -39.550 3.7 354.401 -11.941 5.4 0.77 7.0 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 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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
MXB 1730-335 263.350 -33.388 354.841 -0.158 8.8 1.22 2.1 0.74
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.3 0.40 1.3 0.22
1A 1742-294 266.523 -29.515 359.559 -0.389 5.3 0.35 1.0 0.23
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.2 0.40 0.9 0.30
GX 3+1 266.983 -26.564 2.294 +0.794 30.0 0.56 3.7 0.31
GX 5-1 270.284 -25.079 5.077 -1.019 125.7 2.04 15.7 0.93
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Revolution 0844: Observation start 2009-09-12T03:21 = MJD 55086.14
Total Observation GTI = 13816 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 1E 1740.7-2942 265.972 -29.749 0.8 359.110 -0.103 12.2 0.29 42.0 7.4 0.25 29.9 GX 5-1 270.280 -25.089 0.9 5.067 -1.020 11.9 0.35 34.3 0.0 0.00 0.0 GRS 1758-258 270.301 -25.732 1.1 4.517 -1.355 9.2 0.35 26.5 6.1 0.29 21.3 Ginga 1826-24 277.364 -23.793 1.1 9.275 -6.083 14.8 0.56 26.4 5.6 0.44 12.7 GX 1+4 263.008 -24.747 1.3 1.935 +4.794 8.2 0.35 23.5 0.0 0.00 0.0 IGR J17511-3057 267.810 -30.961 1.7 358.893 -2.088 5.5 0.33 16.5 2.3 0.28 8.1 H 1820-303 275.965 -30.380 1.8 2.789 -7.958 6.3 0.42 15.2 0.0 0.00 0.0 4U 1722-30 261.899 -30.818 2.5 356.312 +2.281 3.6 0.34 10.6 1.3 0.00 4.8 GX 349+2 256.460 -36.428 2.6 349.112 +2.730 5.9 0.57 10.3 0.0 0.00 0.0 3A 1822-371 276.483 -37.065 2.8 356.900 -11.300 6.3 0.66 9.5 0.0 0.00 0.0 GX 9+1 270.381 -20.552 2.7 9.055 +1.145 4.2 0.42 9.9 0.0 0.00 0.0 IGR J17586-2129 269.678 -21.388 3.2 8.003 +1.300 3.1 0.38 8.0 0.0 0.00 0.0 4U 1700-377 255.984 -37.826 3.2 347.768 +2.186 5.4 0.67 8.1 3.4 0.53 6.3 MXB 1730-335 263.432 -33.367 5.5 354.896 -0.204 1.5 0.34 4.5 0.0 0.00 0.0 GX 13+1 273.667 -17.144 3.7 13.544 +0.083 5.2 0.76 6.9 0.0 0.00 0.0 1A 1742-294 266.519 -29.530 4.5 359.545 -0.394 1.6 0.29 5.5 0.0 0.00 0.0 GX 17+2 273.925 -14.023 3.9 16.407 +1.353 11.5 1.80 6.4 0.0 0.00 0.0 XTE J1710-281 257.611 -28.167 4.3 356.360 +6.858 2.5 0.43 5.8 0.0 0.00 0.0 3A 1728-169 262.947 -17.006 5.2 8.481 +9.004 3.1 0.65 4.8 0.0 0.00 0.0 GX 354-0 263.074 -33.871 6.2 354.311 -0.229 1.3 0.33 4.0 0.0 0.00 0.0 1RXS J175113.3-20121 267.879 -20.234 5.9 8.154 +3.334 1.8 0.00 4.2 0.0 0.00 0.0 GX 3+1 267.047 -26.521 0.0 2.360 +0.767 1.2 0.00 4.0 0.0 0.00 0.0 NEW_1 282.367 -37.428 2.9 358.517 -15.727 12.1 1.33 9.1 0.0 0.00 0.0 NEW_2 282.679 -33.294 4.2 2.566 -14.357 7.2 1.14 6.1 0.0 0.00 0.0 NEW_3 284.201 -36.154 3.2 0.322 -16.609 17.8 2.03 8.2 0.0 0.00 0.0 NEW_4 285.160 -36.033 3.7 0.738 -17.285 21.0 3.00 6.9 0.0 0.00 0.0 NEW_5 280.935 -27.289 3.4 7.537 -10.515 6.4 0.88 7.5 0.0 0.00 0.0 NEW_6 269.890 -34.465 4.6 356.732 -5.357 2.0 0.36 5.4 0.0 0.00 0.0 NEW_7 266.572 -22.215 4.0 5.824 +3.364 2.2 0.35 6.3 0.0 0.00 0.0 NEW_8 261.882 -25.166 3.9 1.023 +5.421 2.2 0.34 6.4 0.0 0.00 0.0 NEW_9 270.000 -21.496 0.0 8.059 +0.986 2.3 0.00 6.0 0.0 0.00 0.0 NEW_10 262.029 -43.355 4.7 345.927 -4.756 9.5 1.79 5.3 0.0 0.00 0.0 NEW_11 275.876 -39.550 3.7 354.401 -11.941 5.4 0.77 7.0 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 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== MXB 1730-335 263.350 -33.388 354.841 -0.158 8.8 1.22 2.1 0.74 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.3 0.40 1.3 0.22 1A 1742-294 266.523 -29.515 359.559 -0.389 5.3 0.35 1.0 0.23 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.2 0.40 0.9 0.30 GX 3+1 266.983 -26.564 2.294 +0.794 30.0 0.56 3.7 0.31 GX 5-1 270.284 -25.079 5.077 -1.019 125.7 2.04 15.7 0.93
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