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 X120124.29+615458.5 chandra ccd7 161.353 384.292 16.7905 4.33015 0.00122358 0.000315553 3.13095 0.998156 0.477971 0.477971 0 1.36184 F F 1.89e+20 8.84873e-15 1 dsx
Report srcpi bgdpi arf 2 X120120.25+615527.5 chandra ccd7 219.325 443.123 13.5569 4.21513 0.000987936 0.000307171 2.52798 0.992233 0.488644 0.488644 0 1.95428 F F 1.89e+20 7.21288e-15 1 dsx
Report srcpi bgdpi arf 3 X120106.91+615859.4 chandra ccd7 410.183 873.97 24.2325 4.92265 0.0017659 0.00035873 4.51867 0.999967 2.61666 2.61666 0 5.79553 T F 1.88e+20 1.3927e-14 1 dsx
Report srcpi bgdpi arf rmf 4 X120126.74+615344.6 chandra ccd7 126.187 234.048 156.558 16.2918 0.0114089 0.00118724 29.1936 1 0.678371 0.678371 0 0.125025 F F 1.89e+20 7.29212e-14 1 dsxf
Report srcpi bgdpi arf 9 X120128.93+615339.0 chandra ccd7 94.2334 222.1 13.4941 3.87301 0.00098336 0.000282239 2.51627 0.992233 0.587439 0.492 150.66 0.310165 F F 1.89e+20 7.0615e-15 1 dpx

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