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 X123049.00+122330.0 chandra ccd7 199.887 705.906 145.688 36.5435 0.0304007 0.00762553 4.798 0.999999 0.549128 0.549128 0 0.753228 F F 1.94e+20 0 1 dsc
Report 2 X123048.93+122330.7 chandra ccd7 202.114 707.213 542.762 39.7044 0.113258 0.0082851 17.875 1 1.48014 1.48014 0 0.757993 T F 1.94e+20 0 1 dsc
Report 3 X123048.61+122332.4 chandra ccd7 211.399 710.785 1276.54 46.6651 0.266374 0.00973756 42.0408 1 0.511055 0.511055 0 0.770776 F F 1.93e+20 0 1 ds
Report 4 X123048.21+122335.1 chandra ccd7 223.362 716.129 94.7506 28.0241 0.0197716 0.00584777 3.12046 0.998918 0.664471 0.664471 0 0.797367 F F 1.93e+20 0 1 ds
Report 8 X123049.39+122318.5 chandra ccd7 188.375 682.415 69.0161 28.5646 0.0144016 0.00596056 2.27294 0.988295 1.17034 1.17034 0 0.882009 F F 1.94e+20 0 1 ds
Report 13 X123049.37+122328.4 chandra ccd7 188.842 702.474 5087.33 78.8888 1.06157 0.0164617 167.543 1 0.837921 0.399848 336.235 0.736406 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