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 X010833.57+214942.3 chandra ccd3 922.5 217.5 2.96823 1.73205 0.000831868 0.00048542 5.64445 0.999804 0.492 0.492 90 1.7197 F F 4.69e+20 8.51339e-15 1 dx
Report 2 X010842.30+215029.0 chandra ccd3 675.7 312.5 4.97512 2.23607 0.00139431 0.000626674 9.4608 1 0.492 0.492 60.4819 2.95451 F F 4.7e+20 0 1 d
Report 3 X010859.16+215240.6 chandra ccd3 198.5 580.167 2.92681 1.73206 0.000820259 0.000485421 5.56568 0.999804 0.492 0.492 90 7.24522 F F 4.7e+20 0 1 d
Report srcpi bgdpi arf 4 X010835.15+214818.7 chandra ccd3 877.9 47.6001 9.89358 3.16228 0.00277274 0.000886251 18.8138 1 0.542569 0.492 153.291 0.284148 F F 4.69e+20 2.81005e-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