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 1 X122903.51+294646.1 chandra ccd7 541.129 663.206 38.0761 6.56816 0.00957285 0.00165132 23.9274 1 0.350315 0.350315 0 0.589313 F F 1.76e+20 6.50816e-14 1 dsx
Report srcpi bgdpi arf 2 X122907.65+294556.7 chandra ccd7 431.125 562.25 7.87654 2.82843 0.00198025 0.000711098 4.94969 0.999931 0.492 0.492 3.2599 1.78284 F F 1.76e+20 1.36397e-14 1 dx
Report srcpi bgdpi arf 3 X122855.63+294809.7 chandra ccd7 748.929 832.643 6.939 2.64575 0.00174454 0.000665171 4.36054 0.999694 0.492 0.492 124.099 1.68273 F F 1.76e+20 1.20383e-14 1 dx
Report 4 X122859.42+294852.6 chandra ccd7 648.786 919.929 6.93081 2.64575 0.00174248 0.000665171 4.35538 0.999694 0.492 0.492 132.801 1.6997 F F 1.76e+20 0 1 d
Report srcpi bgdpi arf 5 X122910.92+294502.8 chandra ccd7 344.873 453.203 13.8187 3.71735 0.00347421 0.000934594 8.6838 1 0.947236 0.367883 357.886 2.92848 F F 1.76e+20 2.45101e-14 1 dsx

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