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 4 X223728.68+344004.2 chandra ccd5 505.5 795.3 4.66446 2.23608 0.000471386 0.000225976 2.28438 0.492 0.492 163.997 16.0013 U U 6.33e+20 d
Report 2 X223711.83+344045.1 chandra ccd5 927.9 878.3 4.63677 2.23608 0.000468588 0.000225976 2.25623 0.492 0.492 42.6182 15.9818 U U 6.39e+20 d
Report 1 X223730.20+343551.3 chandra ccd5 466.9 281.3 4.55144 2.23608 0.000459965 0.000225976 2.17275 0.559481 0.492 169.573 12.188 U U 6.25e+20 d
Report 3 X223729.97+343446.7 chandra ccd5 472.5 150 1.79647 1.41422 0.000181549 0.00014292 0.908917 0.492 0.492 90 11.2025 U U 6.24e+20 d
Report 6 X223719.50+343636.5 chandra ccd5 735.5 373 1.6832 1.41423 0.000170102 0.00014292 0.827994 0.5535 0.492 90 12.1506 U U 6.29e+20 d
Report 1 X223729.24+341516.9 chandra ccd3 1200.5 323.5 0.954744 1 9.65158e-05 0.000101091 0.504683 0.492 0.492 90 10.7892 U U 6.05e+20 d
Report 2 X223738.44+342224.3 chandra ccd3 969.8 1192.4 17.5475 4.24265 0.00177389 0.000428892 8.3695 0.492 0.492 71.565 7.32681 U U 6.09e+20 d
Report 5 X223733.31+343455.7 chandra ccd5 388.5 168.5 0.825607 1.00001 8.34352e-05 0.00010106 0.420916 0.492 0.492 90 11.6666 U U 6.24e+20 d

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