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 arf 1 X123905.05+174457.7 chandra ccd3 503.012 594.489 43.4051 6.76649 0.0325094 0.00506794 28.1335 1 5.67846 5.67846 0 12.1756 F F 1.59e+20 3.85022e-13 1 dsx
Report 3 X123916.50+174520.1 chandra ccd3 170.3 639.7 4.70627 2.23608 0.00352478 0.00167472 3.05042 0.996821 0.492 0.492 45 14.4249 F F 1.58e+20 0 1 d
Report 1 X123814.98+174932.5 chandra ccd7 685.5 679.833 2.97543 1.73205 0.00222826 0.00129711 5.81319 0.999841 0.492 0.492 90 2.2292 F F 1.69e+20 0 1 d
Report 1 X123906.38+174925.1 chandra ccd2 701.5 153.5 2.93412 1.73205 0.00219739 0.00129715 10.005 0.999998 0.492 0.492 90 10.9106 F F 1.57e+20 0 1 d
Report arf 2 X123914.12+174011.8 chandra ccd3 238.5 13.1667 2.69565 1.73207 0.00201892 0.00129724 1.74722 0.9655 3.80293 1.75708 115.361 16.7452 A F 1.61e+20 2.64581e-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