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 5 X100120.85+555349.5 chandra ccd7 284.286 273.016 369.676 19.9845 0.123657 0.00668485 86.3972 1 0.381261 0.381261 0 0.274467 F F 9.29e+19 9.24322e-13 1 dsxf
Report srcpi bgdpi arf rmf 1 X100120.70+555355.5 chandra ccd7 286.846 285.331 279.722 17.4626 0.0935676 0.00584128 65.374 1 0.41486 0.41486 0 0.366502 F F 9.29e+19 6.97748e-13 1 dsx
Report srcpi bgdpi arf 2 X100103.13+555554.3 chandra ccd7 586.912 526.918 16.3252 4.04045 0.00546083 0.00135154 3.81537 0.999665 0.72184 0.72184 0 3.51138 F F 9.32e+19 4.55888e-14 1 dsx
Report srcpi bgdpi arf 1 X100119.82+554558.4 chandra ccd6 551.5 307 1.79708 1.41422 0.000601124 0.000473059 3.84797 0.99853 0.665224 0.492 123.69 7.6578 F F 9.24e+19 8.59178e-15 1 dx
Report srcpi bgdpi arf 2 X100113.90+554955.8 chandra ccd6 652.75 789.5 3.95765 2 0.00132384 0.000669002 8.47426 0.999997 0.492 0.492 140.31 3.87265 F F 9.27e+19 1.46885e-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