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 | 10 | X161932.20-494430.7 | chandra | ccd2 | 835.068 | 48.4245 | 130.514 | 11.6684 | 0.0274659 | 0.00245555 | 54.9682 | 1 | 0.484382 | 0.484382 | 0 | 0.41627 | F | T | 1.65e+22 | 0 | 1 | ds | |||||
| Report | 1 | X161826.53-494436.8 | chandra | ccd3 | 1328.46 | 788.202 | 38.9891 | 6.85573 | 0.00820502 | 0.00144275 | 55.6152 | 1 | 4.80339 | 2.85805 | 91.2209 | 10.5035 | A | F | 1.62e+22 | 0 | 1 | d | |||||
| Report | 1 | X162019.21-494538.5 | chandra | ccd0 | 586.674 | 676.848 | 21.8843 | 4.79585 | 0.00460542 | 0.00100926 | 31.7207 | 1 | 1.72829 | 1.14115 | 58.1299 | 7.73787 | A | F | 1.68e+22 | 0 | 1 | d | |||||
| Report | 4 | X161950.20-493831.5 | chandra | ccd2 | 479.167 | 777.833 | 19.9473 | 4.58259 | 0.00419778 | 0.000964379 | 8.40113 | 1 | 2.04668 | 0.970554 | 139.944 | 7.06638 | A | F | 1.62e+22 | 0 | 1 | d | |||||
| Report | 1 | X161918.72-495231.5 | chandra | ccd1 | 1019.4 | 581.452 | 19.7542 | 4.58259 | 0.00415716 | 0.000964379 | 28.515 | 1 | 1.66359 | 0.9593 | 104.508 | 7.88823 | A | F | 1.69e+22 | 0 | 1 | d | |||||
| Report | 9 | X161946.19-493705.4 | chandra | ccd2 | 558.269 | 952.808 | 11.9026 | 3.60557 | 0.00250484 | 0.00075877 | 5.01299 | 0.999974 | 2.26746 | 0.710538 | 148.251 | 8.1741 | A | F | 1.61e+22 | 0 | 1 | d | |||||
| Report | 7 | X161952.86-493924.1 | chandra | ccd2 | 426.8 | 670.9 | 9.62644 | 3.16228 | 0.00202583 | 0.000665484 | 4.05434 | 0.999738 | 1.31938 | 0.530317 | 128.449 | 6.50265 | A | F | 1.63e+22 | 0 | 1 | d | |||||
| Report | 2 | X162009.61-494336.3 | chandra | ccd0 | 775.278 | 925.722 | 8.64879 | 3.00001 | 0.00182009 | 0.000631334 | 12.5362 | 1 | 0.492 | 0.492 | 90 | 6.29201 | F | F | 1.66e+22 | 0 | 1 | d | |||||
| Report | 3 | X161940.02-493848.6 | chandra | ccd2 | 680.214 | 743.214 | 6.44983 | 2.64576 | 0.00135733 | 0.000556785 | 2.71645 | 0.994574 | 1.11079 | 0.582182 | 0.53375 | 6.25573 | A | F | 1.62e+22 | 0 | 1 | d | |||||
| Report | 8 | X161952.26-493756.3 | chandra | ccd2 | 438.5 | 849.214 | 6.33888 | 2.64577 | 0.00133398 | 0.000556786 | 2.66972 | 0.986911 | 1.57274 | 0.687029 | 160.769 | 7.73828 | A | F | 1.62e+22 | 0 | 1 | d | |||||
| Report | 3 | X161946.85-494422.5 | chandra | ccd0 | 1224 | 832.5 | 3.94227 | 2 | 0.000829627 | 0.000420888 | 5.71422 | 0.999863 | 0.492 | 0.492 | 180 | 2.53398 | F | F | 1.65e+22 | 0 | 1 | d | |||||
| Report | 3 | X161911.36-494338.4 | chandra | ccd3 | 445.25 | 909 | 3.93978 | 2 | 0.000829102 | 0.000420888 | 5.61982 | 0.999841 | 0.492 | 0.492 | 52.0181 | 3.49663 | F | F | 1.63e+22 | 0 | 1 | d | |||||
| Report | 2 | X161929.59-494902.6 | chandra | ccd1 | 806 | 1006.25 | 3.93019 | 2 | 0.000827086 | 0.000420889 | 5.67319 | 0.999857 | 0.492 | 0.492 | 37.9819 | 4.14249 | F | F | 1.68e+22 | 0 | 1 | d | |||||
| Report | 2 | X161905.63-494719.0 | chandra | ccd3 | 557.5 | 460.5 | 2.92322 | 1.73205 | 0.000615174 | 0.0003645 | 4.16977 | 0.998354 | 0.602575 | 0.492 | 180 | 4.82152 | F | F | 1.65e+22 | 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