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 3 X085312.87+162615.7 chandra ccd7 539.646 894.645 16.1165 4.2265 0.00757401 0.00198626 12.1941 1 0.385563 0.385563 0 0.402164 F F 2.43e+20 5.60978e-14 1 dsx
Report 1 X085319.63+162643.9 chandra ccd7 341.5 951.5 5.9421 2.44949 0.00279248 0.00115114 4.49593 0.999537 0.492 0.492 163.155 1.82019 F F 2.43e+20 0 1 d
Report srcpi bgdpi arf 2 X085256.14+162551.0 chandra ccd7 1028.5 844 3.86772 2 0.00181763 0.0009399 2.92641 0.990943 0.492 0.492 90 3.89253 F F 2.42e+20 1.59518e-14 1 dx
Report 1 X085319.97+162756.2 chandra ccd6 578.833 88.5 2.97699 1.73205 0.00139904 0.000813976 7.00249 0.999962 0.529672 0.492 100.278 2.31235 F F 2.42e+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