Observation details report
Detailed source parameters (including errors) in a comma-separated values file
Click on source number for detailed analysis, including spectral fits if applicable
| data | idnum | idradec | telescope | instrument | x | y | cnts | cntserr | rate | rateerr | SNR | poisprob | sigmaj | sigmin | incang | offax | cnts_soft | cnts_hard | hr | hr_err | ext | var | N_H | flux | vign | flags | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Report | srcpi bgdpi arf rmf | 3 | X175359.88-292907.0 | chandra | ccd1 | 143.978 | 493.218 | 145.858 | 12.0772 | 0.0750137 | 0.0062112 | 325.552 | 1 | 0.977566 | 0.52528 | 334.213 | 4.34326 | 75 | 69.818 | -0.0357828 | 0.0903991 | F | F | 5.43e+21 | 1.18117e-12 | 1 | dsxf |
| Report | srcpi bgdpi arf | 1 | X175432.16-292824.3 | chandra | ccd3 | 342.105 | 676.651 | 64.2972 | 8.01855 | 0.0330134 | 0.00411713 | 138.859 | 1 | 2.53856 | 1.24141 | 127.834 | 7.48809 | 50.793 | 11.7102 | -0.625294 | 0.169826 | A | F | 5.06e+21 | 4.77751e-13 | 1 | dsx |
| Report | 4 | X175413.20-292859.2 | chandra | ccd3 | 845.445 | 606.042 | 17.5543 | 4.18979 | 0.00901328 | 0.00215125 | 37.9111 | 1 | 0.560855 | 0.560855 | 0 | 4.55297 | F | F | 5.28e+21 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 5 | X175418.30-293641.3 | chandra | ccd2 | 601.317 | 676.752 | 9.2867 | 4.01012 | 0.00476835 | 0.00205904 | 3.56277 | 0.999303 | 0.427759 | 0.427759 | 0 | 4.36179 | 1 | 12.8305 | 0.855392 | 0.463653 | F | F | 5.09e+21 | 6.54934e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X175419.97-293816.5 | chandra | ccd2 | 556.682 | 482.773 | 10.939 | 4.42783 | 0.00561664 | 0.00227347 | 44.3026 | 1 | 0.683319 | 0.492 | 115.131 | 5.87571 | 9 | 1.93903 | -0.645484 | 0.48572 | F | F | 5.04e+21 | 8.57783e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X175351.49-293901.1 | chandra | ccd0 | 253.5 | 323.25 | 8.86022 | 4.1225 | 0.00454946 | 0.00211678 | 23.6981 | 1 | 1.78815 | 0.492 | 145.735 | 6.56084 | 1.93011 | 6.93011 | 0.56432 | 0.539411 | A | F | 5.35e+21 | 6.42251e-14 | 1 | dx |
| Report | 3 | X175417.20-292536.5 | chandra | ccd3 | 738.667 | 1017.5 | 5.82899 | 2.44949 | 0.00299283 | 0.00125767 | 12.5886 | 1 | 0.783396 | 0.492 | 174.005 | 8.0308 | A | F | 5.31e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X175344.87-292940.5 | chandra | ccd1 | 541.7 | 424.5 | 4.93791 | 3.39792 | 0.00253946 | 0.00174748 | 19.8169 | 1 | 0.689245 | 0.504742 | 49.2654 | 5.81378 | 4 | 0.937911 | -0.620118 | 0.821988 | F | F | 5.6e+21 | 3.62631e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X175410.07-292548.8 | chandra | ccd3 | 927.9 | 992.7 | 4.88807 | 3.39792 | 0.00250973 | 0.00174462 | 14.6104 | 1 | 0.778599 | 0.51499 | 58.2825 | 7.4977 | 4.88807 | 0 | -1 | 0.998005 | A | F | 5.4e+21 | 3.57112e-14 | 1 | dx |
| Report | 6 | X175411.51-293221.2 | chandra | ccd3 | 889.75 | 195 | 3.95869 | 2 | 0.00203255 | 0.00102688 | 8.54936 | 0.999997 | 0.492 | 0.492 | 127.982 | 1.51374 | F | F | 5.24e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X175356.38-292830.6 | chandra | ccd1 | 236.25 | 566.75 | 3.83061 | 3.17945 | 0.00197 | 0.00163512 | 9.30741 | 0.999999 | 0.492 | 0.492 | 45 | 5.18021 | 2 | 1.83061 | -0.0442192 | 0.845617 | F | F | 5.5e+21 | 2.60909e-14 | 1 | dx |
| Report | 5 | X175409.48-292935.0 | chandra | ccd3 | 943.5 | 532.833 | 2.97654 | 1.73205 | 0.00152827 | 0.000889303 | 6.42827 | 0.999926 | 0.492 | 0.492 | 90 | 3.7531 | F | F | 5.31e+21 | 0 | 1 | d | |||||
| Report | 2 | X175357.83-293615.0 | chandra | ccd0 | 85.5 | 660.833 | 2.96034 | 1.73205 | 0.00152005 | 0.000889359 | 6.49969 | 0.999935 | 0.632468 | 0.492 | 81.6504 | 3.47275 | F | F | 5.33e+21 | 0 | 1 | d |
counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 7.99 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), T = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters,
b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters,
i = psf spatial fitting parameters, f = spectral fitting parameters,
c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest