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 193.885 313.628 543.677 36.8396 0.112309 0.00761007 17.9539 1 1.48 1.48 0 0.749296 T F 1.94e+20 0 1 dpsc
Report 2 X123048.88+122330.7 chandra ccd7 197.385 315.42 125.778 14.3878 0.0259822 0.00297213 4.15357 0.999976 0.492 0.492 36.4379 0.749333 F F 1.94e+20 0 1 dcb
Report 3 X123048.63+122332.4 chandra ccd7 205.355 319.29 1178.99 45.9919 0.243548 0.0095007 38.9339 1 0.503136 0.503136 0 0.76064 F F 1.93e+20 0 1 ds
Report 4 X123049.25+122334.7 chandra ccd7 187.005 323.94 54.5886 28.1027 0.0112765 0.00580526 1.80268 0.963122 0.609347 0.609347 0 0.843551 F F 1.94e+20 0 1 ds
Report 5 X123048.23+122335.2 chandra ccd7 217.252 325.045 106.24 28.3567 0.0219463 0.00585772 3.50837 0.999728 0.692678 0.692678 0 0.791433 F F 1.93e+20 0 1 ds
Report 10 X123049.38+122328.4 chandra ccd7 183.018 311.113 5662.47 84.0514 1.16971 0.0173628 186.992 1 0.638629 0.402912 334.885 0.757705 A 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