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 X120959.04+104320.7 chandra ccd7 633.1 574.3 4.96747 2.23607 0.00422646 0.00190251 15.6463 1 0.492 0.492 24.8818 2.35452 F F 1.8e+20 0 1 d
Report srcpi bgdpi arf 2 X121010.18+104604.1 chandra ccd7 299.5 906.3 4.96047 2.23607 0.00422051 0.00190251 15.6242 1 0.56786 0.492 117.504 5.84836 F F 1.82e+20 2.5822e-14 1 dx
Report srcpi bgdpi arf 1 X121005.22+104501.0 chandra ccd7 447.833 778.167 2.96861 1.73205 0.00252578 0.00147368 9.35038 0.999996 0.492 0.492 63.4349 4.36361 F F 1.81e+20 1.4924e-14 1 dx
Report 1 X120938.34+103405.8 chandra ccd6 1014.5 427.5 2 1.41421 0.00170165 0.00120325 12.1481 0.999997 0.492 0.492 90 8.46757 F F 1.74e+20 0 1 d
Report 3 X120956.49+104648.0 chandra ccd7 709.5 995.5 1.96341 1.41422 0.00167052 0.00120325 6.18425 0.999842 0.492 0.492 180 5.81869 F F 1.81e+20 0 1 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