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 srcpi bgdpi arf 2 X013707.10+244049.5 chandra ccd7 865.811 858.104 11.3588 4.13569 0.00360598 0.00131292 4.73894 0.999967 0.464368 0.464368 0 5.11268 F F 8.01e+20 2.82421e-14 1 dsx
Report 1 X013730.90+243747.5 chandra ccd7 205.9 487.7 7.90196 2.82843 0.00250856 0.000897914 3.29673 0.997513 0.492 0.492 103.283 3.10221 F F 8.07e+20 0 1 d
Report srcpi bgdpi arf 3 X013720.37+243910.4 chandra ccd7 497.786 656.214 6.87441 2.64575 0.00218235 0.000839922 2.86803 0.993698 0.492 0.492 45 2.76893 F F 8.04e+20 1.78061e-14 1 dx
Report 1 X013727.14+243246.4 chandra ccd6 586.833 867.833 2.94959 1.73205 0.000936378 0.000549858 6.20001 0.999909 0.492 0.492 16.845 4.13949 F F 8.15e+20 0 1 d
Report 2 X013709.94+243308.2 chandra ccd6 1064 912 1.96917 1.41421 0.000625132 0.000448957 4.13917 0.998368 0.492 0.492 45 3.84339 F F 8.13e+20 0 1 d
Report srcpi bgdpi arf 3 X013719.62+243313.7 chandra ccd6 795.5 923.167 2.96987 1.73205 0.000942816 0.000549858 6.24264 0.999909 0.492 0.492 90 3.21276 F F 8.14e+20 9.95985e-15 1 dx
Report srcpi bgdpi arf 4 X013743.18+243043.3 chandra ccd6 142 617.75 6.60412 2.64576 0.00209654 0.000839924 13.8818 1 0.959238 0.492 29.8718 7.98616 A F 8.19e+20 2.91431e-14 1 dx
Report srcpi bgdpi arf 5 X013743.24+243050.9 chandra ccd6 140.3 633.3 4.71794 2.23608 0.00149776 0.000709865 9.91707 0.999996 1.16551 0.694617 10.5699 7.90538 A F 8.19e+20 2.03632e-14 1 dx
Report srcpi bgdpi arf 6 X013714.36+243348.3 chandra ccd6 941.775 994.1 14.0267 3.74522 0.00445296 0.00118897 29.484 1 0.536913 0.536913 0 2.80082 F F 8.13e+20 4.6503e-14 1 dsx

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