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 X142438.10+225600.4 chandra ccd7 379.101 529.482 5786.27 77.2089 0.121232 0.00161765 861.439 1 0.58282 0.58282 0 1.24396 F T 3.25e+20 0 1 ds
Report 2 X142434.38+225618.8 chandra ccd7 483.552 566.766 18.9443 5.8575 0.000396914 0.000122724 2.82036 0.996856 0.568171 0.568171 0 1.94065 F F 3.24e+20 0 1 ds
Report 3 X142427.03+225332.2 chandra ccd7 690.101 228.186 18.707 6.18758 0.000391942 0.00012964 2.78503 0.995341 1.16216 1.16216 0 4.77603 F F 3.24e+20 0 1 ds
Report 4 X142440.65+225542.0 chandra ccd7 307.583 492.006 22.6859 5.69056 0.000475306 0.000119226 3.37739 0.99911 0.328444 0.328444 0 1.08209 F F 3.25e+20 0 1 ds
Report 7 X142431.05+225447.9 chandra ccd7 577.091 382.043 17.1263 4.8101 0.000358824 0.00010078 2.5497 0.993191 0.843719 0.843719 0 3.2637 F F 3.24e+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