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 | 1 | X170144.32-405130.3 | chandra | ccd7 | 185.237 | 235.666 | 25608.8 | 181.408 | 0.913581 | 0.00647163 | 792.992 | 1 | 0.837788 | 0.773895 | 312.172 | 0.174288 | 2646.25 | 27171.2 | 0.822503 | 0.00762068 | T | F | 1.28e+22 | 2.62653e-11 | 1 | dsxf |
Report | srcpi bgdpi arf rmf | 2 | X170145.23-405131.6 | chandra | ccd7 | 164.265 | 233.016 | 413.994 | 39.4309 | 0.0147691 | 0.00140668 | 12.8196 | 1 | 1.82292 | 0.320032 | 352.914 | 0.0882992 | 121.758 | 842.462 | 0.747448 | 0.045394 | A | F | 1.28e+22 | 1.90631e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 3 | X170146.11-405132.8 | chandra | ccd7 | 143.943 | 230.607 | 414.915 | 27.771 | 0.0148019 | 0.00099072 | 12.8481 | 1 | 1.78984 | 0.293013 | 352.561 | 0.183176 | 61.876 | 421.457 | 0.743961 | 0.0687774 | A | F | 1.28e+22 | 1.91259e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 4 | X170146.76-405133.6 | chandra | ccd7 | 129.065 | 228.815 | 344.582 | 25.0258 | 0.0122928 | 0.000892786 | 10.6702 | 1 | 1.5 | 0.32732 | 351.928 | 0.327259 | 62.389 | 392.944 | 0.725963 | 0.0661866 | A | F | 1.28e+22 | 1.58936e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 5 | X170146.62-405133.5 | chandra | ccd7 | 132.256 | 229.182 | 420.285 | 26.8157 | 0.0149935 | 0.00095664 | 13.0144 | 1 | 1.81575 | 0.411711 | -0 | 0.280499 | 103.11 | 608.037 | 0.710018 | 0.0532314 | A | F | 1.28e+22 | 1.95084e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 6 | X170145.86-405132.4 | chandra | ccd7 | 149.665 | 231.302 | 397.579 | 29.5752 | 0.0141834 | 0.00105508 | 12.3113 | 1 | 1.78401 | 0.294051 | 352.916 | 0.134983 | 58.8197 | 456.259 | 0.771609 | 0.0675631 | A | F | 1.28e+22 | 1.83315e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 7 | X170145.61-405132.1 | chandra | ccd7 | 155.469 | 232.014 | 363.555 | 31.2025 | 0.0129697 | 0.00111314 | 11.2577 | 1 | 1.79104 | 0.300203 | 353.746 | 0.104279 | 71.194 | 525.023 | 0.761181 | 0.0613908 | A | F | 1.28e+22 | 1.67487e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 8 | X170143.48-405129.2 | chandra | ccd7 | 204.742 | 237.92 | 305.783 | 34.3329 | 0.0109087 | 0.00122481 | 9.46875 | 1 | 1.5 | 0.333177 | 354.467 | 0.355464 | 95.1281 | 719.803 | 0.766537 | 0.0511671 | A | F | 1.28e+22 | 1.40729e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 9 | X170143.35-405129.0 | chandra | ccd7 | 207.667 | 238.303 | 363.492 | 33.883 | 0.0129674 | 0.00120876 | 11.2557 | 1 | 1.83165 | 0.326037 | 352.42 | 0.380737 | 110.26 | 745.644 | 0.742355 | 0.0484484 | A | F | 1.28e+22 | 1.67393e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 10 | X170143.22-405128.8 | chandra | ccd7 | 210.726 | 238.687 | 384.337 | 31.068 | 0.0137111 | 0.00110834 | 11.9012 | 1 | 1.85566 | 0.336087 | 352.455 | 0.413388 | 99.2735 | 653.347 | 0.736192 | 0.052343 | A | F | 1.28e+22 | 1.77119e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 11 | X170142.87-405128.3 | chandra | ccd7 | 218.612 | 239.653 | 334.362 | 27.2245 | 0.0119282 | 0.000971223 | 10.3537 | 1 | 1.5 | 0.333035 | 352.836 | 0.460779 | 54.0815 | 368.51 | 0.744048 | 0.075976 | A | F | 1.28e+22 | 1.54016e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 12 | X170142.67-405128.0 | chandra | ccd7 | 223.215 | 240.201 | 309.864 | 24.346 | 0.0110543 | 0.000868532 | 9.59512 | 1 | 1.85548 | 0.364233 | 353.428 | 0.51674 | 51.4307 | 400.166 | 0.772227 | 0.0742915 | A | F | 1.28e+22 | 1.66263e-13 | 1 | dscx |
Report | srcpi bgdpi arf rmf | 13 | X170147.27-405134.4 | chandra | ccd7 | 117.314 | 227.379 | 324.239 | 22.1146 | 0.0115671 | 0.000788928 | 10.0403 | 1 | 1.84751 | 0.359538 | 353.922 | 0.408456 | 59.9416 | 356.683 | 0.712251 | 0.0689058 | A | F | 1.28e+22 | 2.1883e-13 | 1 | dscx |
Report | srcpi bgdpi arf | 14 | X170147.54-405134.7 | chandra | ccd7 | 110.566 | 226.205 | 127.767 | 13.3187 | 0.00455804 | 0.000475138 | 26.5076 | 1 | 0.492 | 0.492 | 23.8697 | 0.472222 | 20.0232 | 105.953 | 0.682112 | 0.127292 | F | F | 1.28e+22 | 1.18871e-13 | 1 | dpcbx |
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