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 X175709.53-272533.1 chandra ccd2 477.666 724.35 14.3869 4.38035 0.00667977 0.00203377 6.56633 1 1.09518 1.09518 0 6.52295 F F 7.4e+21 9.89519e-14 1 dsx
Report srcpi bgdpi arf 1 X175709.79-273250.0 chandra ccd3 313.929 842.928 6.9531 2.64575 0.00322359 0.00122662 14.9491 1 0.56679 0.492 49.9631 2.33678 F F 7.15e+21 4.40284e-14 1 dx
Report srcpi bgdpi arf 1 X175734.94-273654.2 chandra ccd1 664.214 526.357 6.85281 2.64576 0.00317709 0.00122662 14.8472 1 0.700089 0.492 150.715 6.26015 F F 6.71e+21 4.58308e-14 1 dx
Report 3 X175712.27-273315.3 chandra ccd3 246.75 791.5 3.97485 2 0.00184281 0.000927238 8.54589 0.999997 0.492 0.492 180 2.14687 F T 7.11e+21 0 1 d
Report srcpi bgdpi arf 2 X175701.24-273443.6 chandra ccd3 544.75 611.75 3.90718 2 0.00181144 0.000927239 8.40042 0.999997 0.500222 0.492 115.67 4.96234 F F 7.17e+21 2.62732e-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