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 2 X124238.39+032134.7 chandra ccd7 744.833 372 5.90268 2.44949 0.00327762 0.00136015 10.9148 1 0.513212 0.492 54.9276 4.81604 F F 1.96e+20 2.69912e-14 1 dx
Report 1 X124255.27+032953.2 chandra ccd6 476 372.25 3.93439 2 0.00218468 0.00111055 11.0058 1 0.692332 0.492 17.1651 4.57797 F F 1.95e+20 0 1 d
Report 2 X124243.82+033204.9 chandra ccd6 824.5 640 5.89367 2.44949 0.00327262 0.00136015 16.4865 1 0.781147 0.492 130.48 5.97555 A F 1.95e+20 0 1 d
Report srcpi bgdpi arf 1 X124254.18+032015.7 chandra ccd7 264.25 211.5 3.79021 2.00001 0.00210461 0.00111056 7.00859 0.999986 1.01055 0.492 90 6.29336 A F 1.95e+20 1.87769e-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