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 2 X104023.64+204859.1 chandra ccd7 443.116 724.076 57.0521 7.55328 0.0113033 0.00149648 16.7708 1 0.85721 0.85721 0 3.72453 F F 1.56e+20 8.28652e-14 1 dsx
Report srcpi bgdpi arf 3 X104023.91+204945.9 chandra ccd7 435.464 819.161 11.7165 3.42294 0.00232131 0.000678162 3.44414 0.999081 0.731932 0.731932 0 4.50764 F F 1.56e+20 1.72362e-14 1 dsx
Report srcpi bgdpi arf rmf 4 X104034.36+205112.4 chandra ccd7 137.591 994.956 101.618 10.5534 0.0201328 0.00209086 29.8713 1 2.58346 2.58346 0 6.56938 F F 1.56e+20 1.56404e-13 1 dsxf
Report srcpi bgdpi arf rmf 5 X104026.85+204544.2 chandra ccd7 351.48 327.91 787.859 28.7123 0.156093 0.00568856 231.596 1 0.449512 0.449512 0 1.16204 F F 1.56e+20 1.1042e-12 1 dsx

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