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 X123049.03+122330.3 chandra ccd7 477.461 287.046 176.668 16.6136 0.0336456 0.00316398 5.34748 1 0.492 0.492 9.96232 0.75151 F F 1.94e+20 0 1 dbcp
Report 2 X123048.82+122331.7 chandra ccd7 484.118 290.376 190.608 37.5581 0.0363003 0.00715273 5.76941 1 1.5 1.5 0 0.736526 T F 1.94e+20 0 1 dsc
Report 3 X123048.63+122332.6 chandra ccd7 489.771 292.092 1197.64 46.2982 0.228084 0.00881726 36.2507 1 0.487425 0.487425 0 0.717319 F F 1.93e+20 0 1 dsc
Report 4 X123048.25+122335.2 chandra ccd7 501.211 297.533 129.217 28.8414 0.0246088 0.00549271 3.9112 0.999938 1.5 0.372582 336.68 0.705415 A F 1.93e+20 0 1 ds
Report 8 X123047.55+122347.9 chandra ccd7 522.1 323.206 73.54 20.9909 0.0140053 0.0039976 2.22594 0.98681 1.42605 1.42605 0 0.83921 T F 1.93e+20 0 1 ds
Report 9 X123049.38+122328.6 chandra ccd7 467.539 283.969 9565.07 108.568 1.82162 0.0206762 289.52 1 0.525514 0.525514 0 0.793247 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