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 1 X120629.36+281436.2 chandra ccd2 206.625 914.75 7.84344 2.82843 0.00364678 0.00131507 19.2803 1 0.717151 0.492 110.547 3.36365 F F 1.72e+20 4.10862e-14 1 dx
Report srcpi bgdpi arf 1 X120702.17+280604.5 chandra ccd3 12.5 637 5.6466 2.4495 0.00262537 0.00113889 10.6928 0.999999 1.39757 0.789 1.95579 8.06128 A F 1.73e+20 3.58515e-14 1 dx
Report srcpi bgdpi arf 1 X120706.93+280726.4 chandra ccd1 641.5 133.5 3.77943 2.00001 0.0017547 0.000928558 8.76113 0.999957 1.60521 0.592255 33.2857 8.10873 A F 1.72e+20 2.39057e-14 1 dx
Report 1 X120636.08+281659.8 chandra ccd0 845 513.5 1.97415 1.41421 0.000916554 0.000656588 4.94843 0.999403 0.492 0.492 180 5.51928 F F 1.72e+20 0 1 d
Report 2 X120628.21+281620.3 chandra ccd0 1056.5 433.167 2.98419 1.73205 0.00138549 0.000804152 7.4802 0.999976 0.492 0.492 90 5.08356 F F 1.72e+20 0 1 d
Report 2 X120558.11+281036.7 chandra ccd2 1046.5 428.5 1.94392 1.41422 0.000903817 0.000657535 4.77842 0.999332 0.492 0.492 180 8.18435 F F 1.73e+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