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 X191011.03+092517.8 chandra ccd5 595.283 341.117 17.0686 5.18792 0.0104495 0.00317609 5.43963 0.999995 5.94076 5.94076 0 11.7576 F T 1.55e+22 1.92296e-13 1 dsx
Report 1 X191049.31+092828.0 chandra ccd2 1244.3 780.1 4.79091 2.23607 0.002933 0.00136893 13.0147 1 0.492 0.492 108.435 11.3116 F T 1.55e+22 0 1 d
Report 2 X191043.17+092201.5 chandra ccd6 309 691.5 3.93014 2 0.00240604 0.0012244 10.7006 1 0.703059 0.492 20.8168 4.87287 F F 1.55e+22 0 1 d
Report srcpi bgdpi arf 1 X191031.52+092239.0 chandra ccd6 659.5 767.75 3.8805 2 0.00237565 0.0012244 10.5654 1 0.60809 0.492 96.4375 6.4789 F T 1.55e+22 4.12101e-14 1 dx

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