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 1 X210501.15-484846.6 chandra ccd7 314.926 281.682 378.212 19.929 0.0739831 0.00389837 122.858 1 0.406633 0.360807 359.953 0.609508 F F 2.91e+20 0 1 ds
Report 2 X210432.08-484954.7 chandra ccd7 897.955 142.045 9.87673 3.31665 0.00193201 0.000648777 3.20836 0.998091 1.3983 0.561784 164.693 5.5264 A T 2.92e+20 0 1 d
Report 3 X210459.45-484942.7 chandra ccd7 349.079 167.643 16.0134 4.00167 0.00313242 0.000782778 5.20179 0.999993 0.375044 0.375044 0 1.41876 F F 2.91e+20 0 1 ds
Report 4 X210508.73-484958.9 chandra ccd7 162.3 134.1 9.8525 3.16228 0.00192727 0.000618582 3.20048 0.998091 0.492 0.492 50.1524 1.55328 F F 2.91e+20 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