Source List

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 2 X174423.57-311636.7 chandra ccd3 863.914 1100.26 28.1187 5.38517 0.0130549 0.00250021 63.0143 1 1.81658 1.0059 97.14 6.69014 A F 9.36e+21 2.15787e-13 1 dx
Report srcpi bgdpi arf 1 X174506.66-312542.3 chandra ccd1 794.5 140.875 7.48987 2.82844 0.00347738 0.00131318 16.4596 1 1.68096 0.823655 159.127 8.80671 A F 8.53e+21 5.68839e-14 1 dx
Report 2 X174442.33-311634.0 chandra ccd2 543.1 73.2998 4.97145 2.23607 0.00231146 0.00103965 11.1535 1 0.492 0.492 148.283 2.7423 F F 9.18e+21 0 1 d
Report 1 X174536.81-311651.0 chandra ccd0 152.5 223.9 4.66427 2.23608 0.00216551 0.00103816 10.662 0.999998 0.780549 0.492 122.886 9.00098 A F 8.57e+21 0 1 d
Report 1 X174453.31-312124.8 chandra ccd3 88.75 515.25 3.95897 2 0.00183806 0.000928555 8.87209 0.999998 0.5535 0.492 11.3099 4.14991 F F 8.87e+21 0 1 d
Report 3 X174454.62-311959.2 chandra ccd3 54.75 689.25 3.95663 2 0.00183698 0.000928555 8.86687 0.999998 0.492 0.492 3.56251 2.71224 F F 8.91e+21 0 1 d
Report 1 X174425.30-311518.3 chandra ccd2 986.833 226.833 2.92238 1.73205 0.00135875 0.000805312 6.5564 0.999945 0.492 0.492 16.845 6.5884 F F 9.39e+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