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+122329.6 chandra ccd7 255.887 636.842 435.479 35.4591 0.0935552 0.00761778 17.8606 1 1.5 1.5 0 0.736746 T F 1.94e+20 0 1 dbsc
Report 2 X123048.89+122330.7 chandra ccd7 259.336 638.629 181.738 16.9415 0.039043 0.00363956 7.45374 1 0.492 0.492 42.5508 0.758228 F F 1.94e+20 0 1 dc
Report 3 X123048.63+122332.3 chandra ccd7 267.633 642.355 974.605 43.2247 0.209377 0.00928608 39.9721 1 0.458731 0.458731 0 0.790315 F F 1.93e+20 0 1 ds
Report 4 X123048.22+122335.1 chandra ccd7 279.805 648.032 118.998 27.0574 0.0255648 0.00581283 4.88054 0.999999 0.856609 0.856609 0 0.839378 T F 1.93e+20 0 1 ds
Report 7 X123049.37+122328.3 chandra ccd7 245.356 634.135 9070.7 95.4982 1.94868 0.0205161 372.022 1 0.544214 0.517862 351.106 0.708723 F 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