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 1 X173854.89-274028.5 chandra ccd0 806.218 651.475 22.3936 4.73219 0.010397 0.00219707 53.0211 1 1.64365 1.64365 0 6.03069 F F 5.26e+21 1.42901e-13 1 dsx
Report srcpi bgdpi arf 3 X173849.33-274843.9 chandra ccd1 995.125 669 7.96008 2.82843 0.00369568 0.00131317 17.7428 1 0.492 0.492 45.716 3.08827 F F 5.49e+21 4.8724e-14 1 dx
Report 1 X173856.43-274833.3 chandra ccd1 803.5 690.5 3.97625 2 0.00184608 0.000928555 8.86297 0.999998 0.492 0.492 180 3.89506 F F 5.55e+21 0 1 d
Report srcpi bgdpi arf 2 X173924.15-274658.1 chandra ccd1 55.75 883.25 3.65551 2.00001 0.00169717 0.000928558 8.14806 0.999942 1.46442 1.05181 95.1944 9.07357 F F 5.74e+21 3.02769e-14 1 dx
Report 2 X173833.36-274440.1 chandra ccd2 346.833 164.5 2.95046 1.73205 0.00136983 0.000804153 6.78656 0.999954 0.602575 0.492 90 2.55678 F F 5.22e+21 0 1 d
Report srcpi bgdpi arf 1 X173822.10-274231.3 chandra ccd2 650.833 426.167 2.89367 1.73205 0.00134346 0.000804154 6.65592 0.999954 0.678773 0.492 65.9936 5.81927 F F 5.05e+21 1.91165e-14 1 dx

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