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 rmf 4 X232019.03+554828.2 chandra ccd7 412.009 964.245 801.881 29.1125 0.104017 0.00377637 170.948 1 0.445068 0.445068 0 1.13043 F T 3.52e+21 1.20253e-12 1 dsxf
Report srcpi bgdpi arf 2 X232004.94+554222.3 chandra ccd7 653.082 220.127 34.2413 8.18559 0.00289931 0.000693099 7.29969 1 2.30884 1.48075 31.7162 6.07798 A F 3.41e+21 2.72573e-14 1 dx
Report srcpi bgdpi arf 3 X231956.28+554157.8 chandra ccd7 802.035 170.43 18.1294 6.55768 0.00153507 0.000555258 3.8649 0.999812 2.0404 1.46602 115.97 6.75198 F F 3.39e+21 1.48734e-14 1 dbx
Report srcpi bgdpi arf 1 X231955.01+554221.5 chandra ccd7 823.682 218.652 15.993 5.74474 0.00135417 0.000486424 3.40945 0.998782 1.80477 0.775452 33.926 6.4368 A F 3.39e+21 1.28352e-14 1 dx
Report srcpi bgdpi arf 5 X231958.43+555159.9 chandra ccd7 764.563 1394.6 12.8454 4.34213 0.00166626 0.000563245 2.73843 0.993624 0.911673 0.911673 0 4.01923 F F 3.55e+21 1.52687e-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