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 X040917.91+110820.5 chandra ccd7 300.443 468.82 124.011 11.4586 0.0578233 0.00534288 45.9333 1 0.504444 0.403367 351.274 1.23883 F F 1.25e+21 4.5291e-13 1 dsxf
Report srcpi bgdpi arf 3 X040909.44+111022.7 chandra ccd7 553.167 716.833 8.88743 3 0.00414389 0.00139879 3.29188 0.998537 0.610434 0.492 20.593 2.02446 F F 1.25e+21 3.21468e-14 1 dx
Report srcpi bgdpi arf 2 X040916.59+110841.6 chandra ccd7 339.375 511.25 7.87788 2.82843 0.00367317 0.0013188 2.91795 0.996465 0.492 0.492 109.33 0.911296 F F 1.25e+21 2.85703e-14 1 dx
Report srcpi bgdpi arf 1 X040918.83+110837.6 chandra ccd7 272.5 503.214 6.89039 2.64575 0.00321274 0.00123362 2.55218 0.991916 0.492 0.492 90 1.44972 F F 1.26e+21 2.51894e-14 1 dx
Report 1 X040919.69+110653.6 chandra ccd6 984.5 1006.83 2.96991 1.73205 0.00138476 0.000807594 7.92929 0.999986 0.492 0.492 151.845 2.34058 F F 1.25e+21 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