INTEGRAL Galactic Bulge MonitoringRevolution 0662: Observation start 2008-03-15T13:04 = MJD 54540.545
Total Observation GTI = 8513 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GRO J1750-27 267.298 -26.638 0.5 2.376 +0.514 29.9 0.36 82.2 1.6 0.31 5.1
4U 1700-377 255.986 -37.849 0.5 347.750 +2.170 67.7 0.95 71.5 13.2 0.71 18.6
Ginga 1826-24 277.364 -23.797 1.2 9.271 -6.085 18.4 0.76 24.3 7.1 0.57 12.4
4U 1722-30 261.890 -30.805 1.3 356.318 +2.295 9.4 0.43 22.0 3.6 0.34 10.6
SAX J1750.8-2900 267.615 -29.046 1.2 0.453 -0.963 9.8 0.40 24.6 2.4 0.33 7.1
H 1820-303 275.919 -30.358 1.7 2.791 -7.913 9.7 0.58 16.9 0.0 0.00 0.0
GX 5-1 270.296 -25.083 1.8 5.079 -1.030 7.1 0.46 15.3 0.0 0.00 0.0
GRS 1758-258 270.317 -25.740 2.2 4.517 -1.372 5.6 0.47 12.1 3.9 0.36 10.6
GX 3+1 266.887 -26.528 0.0 2.279 +0.886 4.2 0.00 11.2 0.0 0.00 0.0
1E 1740.7-2942 266.001 -29.733 2.2 359.136 -0.116 4.5 0.37 12.2 2.9 0.31 9.6
XTE J1810-189 272.590 -19.078 3.1 11.356 +0.052 5.5 0.65 8.5 3.1 0.52 5.9
OAO 1657-415 255.174 -41.654 3.0 344.357 +0.338 20.6 2.34 8.8 6.8 1.71 4.0
GX 349+2 256.439 -36.360 3.8 349.156 +2.784 5.2 0.77 6.7 0.0 0.00 0.0
GX 1+4 263.018 -24.747 3.3 1.940 +4.787 3.6 0.45 7.9 0.0 0.00 0.0
Oph Cluster 258.104 -23.386 3.6 0.553 +9.269 3.8 0.54 7.2 0.0 0.00 0.0
3A 1822-371 276.505 -37.153 4.1 356.828 -11.354 5.2 0.85 6.1 0.0 0.00 0.0
SLX 1744-299_300 266.800 -30.032 3.8 359.242 -0.863 2.6 0.38 6.8 0.0 0.00 0.0
GX 354-0 263.013 -33.789 4.6 354.351 -0.142 2.4 0.44 5.5 0.0 0.00 0.0
GX 17+2 274.001 -14.017 3.5 16.447 +1.291 13.5 1.85 7.3 0.0 0.00 0.0
GRS 1747-312 267.667 -31.271 4.5 358.564 -2.140 2.5 0.45 5.6 0.0 0.00 0.0
3A 1728-169 262.991 -16.962 5.2 8.542 +8.992 3.5 0.73 4.8 0.0 0.00 0.0
IGR J17473-2721 266.800 -27.434 0.0 1.465 +0.483 1.6 0.00 4.2 0.0 0.00 0.0
XB 1832-330 278.999 -32.920 5.8 1.621 -11.391 3.6 0.00 4.2 0.0 0.00 0.0
GRS 1734-292 264.394 -29.045 5.6 358.979 +1.436 1.7 0.40 4.3 0.0 0.00 0.0
GRO J1655-40 253.542 -39.861 6.0 344.990 +2.422 7.6 1.86 4.1 0.0 0.00 0.0
SLX 1735-269 264.600 -27.002 5.7 0.803 +2.374 1.5 0.36 4.3 1.4 0.00 4.7
GX 9+1 270.399 -20.562 5.1 9.055 +1.126 2.5 0.52 4.8 0.0 0.00 0.0
Swift J174535.5-2901 266.339 -28.998 5.6 359.917 +0.017 1.8 0.41 4.4 0.0 0.00 0.0
4U 1812-12 273.797 -12.169 6.1 17.979 +2.345 22.6 5.72 4.0 0.0 0.00 0.0
NEW_1 255.584 -28.405 2.7 355.097 +8.154 6.2 0.64 9.8 0.0 0.00 0.0
NEW_2 267.764 -18.544 3.8 9.558 +4.285 4.6 0.68 6.7 0.0 0.00 0.0
NEW_3 256.790 -18.053 4.3 4.296 +13.330 4.9 0.86 5.8 0.0 0.00 0.0
** NOTE **: NEW sources are artefacts from the detection of SAX J1750.8-2900
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) +/-
==================== ======== ======== ======== ======== ====== ===== ====== =====
SAX J1750.8-2900 267.603 -29.037 0.455 -0.949 6.9 0.67 2.1 0.42
GX 3+1 266.983 -26.564 2.294 +0.794 37.6 0.86 6.6 0.47
GX 5-1 270.284 -25.079 5.077 -1.019 77.9 2.22 10.1 1.13
GRO J1750-27 267.303 -26.643 2.373 +0.508 7.6 0.69 6.9 0.41
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Revolution 0662: Observation start 2008-03-15T13:04 = MJD 54540.545
Total Observation GTI = 8513 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRO J1750-27 267.298 -26.638 0.5 2.376 +0.514 29.9 0.36 82.2 1.6 0.31 5.1 4U 1700-377 255.986 -37.849 0.5 347.750 +2.170 67.7 0.95 71.5 13.2 0.71 18.6 Ginga 1826-24 277.364 -23.797 1.2 9.271 -6.085 18.4 0.76 24.3 7.1 0.57 12.4 4U 1722-30 261.890 -30.805 1.3 356.318 +2.295 9.4 0.43 22.0 3.6 0.34 10.6 SAX J1750.8-2900 267.615 -29.046 1.2 0.453 -0.963 9.8 0.40 24.6 2.4 0.33 7.1 H 1820-303 275.919 -30.358 1.7 2.791 -7.913 9.7 0.58 16.9 0.0 0.00 0.0 GX 5-1 270.296 -25.083 1.8 5.079 -1.030 7.1 0.46 15.3 0.0 0.00 0.0 GRS 1758-258 270.317 -25.740 2.2 4.517 -1.372 5.6 0.47 12.1 3.9 0.36 10.6 GX 3+1 266.887 -26.528 0.0 2.279 +0.886 4.2 0.00 11.2 0.0 0.00 0.0 1E 1740.7-2942 266.001 -29.733 2.2 359.136 -0.116 4.5 0.37 12.2 2.9 0.31 9.6 XTE J1810-189 272.590 -19.078 3.1 11.356 +0.052 5.5 0.65 8.5 3.1 0.52 5.9 OAO 1657-415 255.174 -41.654 3.0 344.357 +0.338 20.6 2.34 8.8 6.8 1.71 4.0 GX 349+2 256.439 -36.360 3.8 349.156 +2.784 5.2 0.77 6.7 0.0 0.00 0.0 GX 1+4 263.018 -24.747 3.3 1.940 +4.787 3.6 0.45 7.9 0.0 0.00 0.0 Oph Cluster 258.104 -23.386 3.6 0.553 +9.269 3.8 0.54 7.2 0.0 0.00 0.0 3A 1822-371 276.505 -37.153 4.1 356.828 -11.354 5.2 0.85 6.1 0.0 0.00 0.0 SLX 1744-299_300 266.800 -30.032 3.8 359.242 -0.863 2.6 0.38 6.8 0.0 0.00 0.0 GX 354-0 263.013 -33.789 4.6 354.351 -0.142 2.4 0.44 5.5 0.0 0.00 0.0 GX 17+2 274.001 -14.017 3.5 16.447 +1.291 13.5 1.85 7.3 0.0 0.00 0.0 GRS 1747-312 267.667 -31.271 4.5 358.564 -2.140 2.5 0.45 5.6 0.0 0.00 0.0 3A 1728-169 262.991 -16.962 5.2 8.542 +8.992 3.5 0.73 4.8 0.0 0.00 0.0 IGR J17473-2721 266.800 -27.434 0.0 1.465 +0.483 1.6 0.00 4.2 0.0 0.00 0.0 XB 1832-330 278.999 -32.920 5.8 1.621 -11.391 3.6 0.00 4.2 0.0 0.00 0.0 GRS 1734-292 264.394 -29.045 5.6 358.979 +1.436 1.7 0.40 4.3 0.0 0.00 0.0 GRO J1655-40 253.542 -39.861 6.0 344.990 +2.422 7.6 1.86 4.1 0.0 0.00 0.0 SLX 1735-269 264.600 -27.002 5.7 0.803 +2.374 1.5 0.36 4.3 1.4 0.00 4.7 GX 9+1 270.399 -20.562 5.1 9.055 +1.126 2.5 0.52 4.8 0.0 0.00 0.0 Swift J174535.5-2901 266.339 -28.998 5.6 359.917 +0.017 1.8 0.41 4.4 0.0 0.00 0.0 4U 1812-12 273.797 -12.169 6.1 17.979 +2.345 22.6 5.72 4.0 0.0 0.00 0.0 NEW_1 255.584 -28.405 2.7 355.097 +8.154 6.2 0.64 9.8 0.0 0.00 0.0 NEW_2 267.764 -18.544 3.8 9.558 +4.285 4.6 0.68 6.7 0.0 0.00 0.0 NEW_3 256.790 -18.053 4.3 4.296 +13.330 4.9 0.86 5.8 0.0 0.00 0.0
** NOTE **: NEW sources are artefacts from the detection of SAX J1750.8-2900
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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== SAX J1750.8-2900 267.603 -29.037 0.455 -0.949 6.9 0.67 2.1 0.42 GX 3+1 266.983 -26.564 2.294 +0.794 37.6 0.86 6.6 0.47 GX 5-1 270.284 -25.079 5.077 -1.019 77.9 2.22 10.1 1.13 GRO J1750-27 267.303 -26.643 2.373 +0.508 7.6 0.69 6.9 0.41
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