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 X123049.02+122330.3 chandra ccd7 530.893 258.886 299.218 37.6659 0.0636762 0.00801563 8.72489 1 1.5 0.429885 349.577 0.759952 A F 1.94e+20 0 1 dbsc
Report 2 X123048.88+122330.9 chandra ccd7 534.491 259.628 121.62 14.1425 0.0258816 0.00300963 3.5463 0.999754 0.492 0.492 8.029 0.732469 F F 1.94e+20 0 1 dc
Report 3 X123048.62+122332.5 chandra ccd7 542.764 263.445 1085.62 44.4845 0.231028 0.00946665 31.6555 1 0.615509 0.467972 338.045 0.701818 T F 1.93e+20 0 1 ds
Report 4 X123048.23+122335.2 chandra ccd7 554.516 268.968 106.618 26.5999 0.0226892 0.00566067 3.10887 0.998898 0.697798 0.697798 0 0.679477 F F 1.93e+20 0 1 ds
Report 12 X123049.38+122328.5 chandra ccd7 520.354 255.243 6808.43 94.3359 1.44889 0.0200755 198.527 1 0.787502 0.787502 0 0.802234 T F 1.94e+20 0 1 ds

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