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 2 X174522.62-254202.6 chandra ccd3 792.25 232.5 3.77062 2.00001 0.0017531 0.000929879 7.77539 0.999995 0.492 0.492 180 8.77063 F F 5.72e+21 0 1 d
Report srcpi bgdpi arf 1 X174625.77-253415.8 chandra ccd0 95.25 132 3.56974 2.00001 0.00165971 0.000929881 7.71261 0.999926 1.22169 0.492 149.046 8.51332 A F 6.42e+21 2.53125e-14 1 dx
Report srcpi bgdpi arf 1 X174601.81-253922.5 chandra ccd1 772.5 553.167 2.9732 1.73205 0.00138235 0.000805296 6.25101 0.999909 0.550073 0.492 18.4349 4.93508 F F 6.16e+21 1.9331e-14 1 dx
Report 1 X174541.37-253127.4 chandra ccd2 277.5 474.833 2.96322 1.73205 0.00137771 0.000805296 6.39764 0.999926 0.550073 0.492 161.565 4.31868 F F 5.74e+21 0 1 d
Report 2 X174613.49-253426.6 chandra ccd0 432.833 110.5 2.95771 1.73205 0.00137515 0.000805296 6.3903 0.999926 0.529672 0.492 79.722 5.75217 F F 6.21e+21 0 1 d
Report 1 X174543.21-254234.4 chandra ccd3 226.5 168.167 2.90423 1.73205 0.00135028 0.000805297 5.9888 0.999894 0.492 0.492 90 7.19535 F F 5.99e+21 0 1 d
Report 2 X174623.93-253922.8 chandra ccd1 164.5 552.167 2.7966 1.73206 0.00130025 0.000805298 5.87971 0.999909 1.09781 0.492 61.845 8.91096 A F 6.46e+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