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 2 X190813.20+074357.7 chandra ccd7 701.9 680.004 135.677 11.9119 0.0945902 0.00830465 76.9552 1 0.622388 0.417971 289.081 2.18335 F F 1.45e+22 9.62395e-13 1 dsxf
Report srcpi bgdpi arf 1 X190850.90+074207.7 chandra ccd3 813.461 969 22.9222 5.09906 0.0159803 0.00355483 64.8447 1 3.23993 2.46794 44.0989 8.82445 F F 1.4e+22 2.98208e-13 1 dx
Report srcpi bgdpi arf 1 X190825.47+074428.2 chandra ccd7 331.175 741.987 11.9584 3.45809 0.00833702 0.00241087 6.78274 1 0.66586 0.29645 339.906 2.16177 F F 1.44e+22 1.12988e-13 1 dsx
Report 1 X190822.74+074748.8 chandra ccd6 676.167 161.167 2.98528 1.73205 0.0020812 0.00120751 8.58867 0.999992 0.492 0.492 45 2.34785 F F 1.45e+22 0 1 d
Report 1 X190847.99+074453.9 chandra ccd2 1158.5 315.833 2.93307 1.73205 0.0020448 0.00120751 8.47135 0.999992 1.01316 0.85351 123.019 7.38166 F F 1.41e+22 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