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 X042257.83+602446.9 chandra ccd7 730 997.667 5.89912 2.44949 0.00501913 0.0020841 9.03611 1 0.540222 0.492 86.9422 1.86615 F F 3.49e+21 4.21532e-14 1 dx
Report srcpi bgdpi arf 1 X042350.15+603519.3 chandra ccd5 905.5 432.5 4.69628 2.23608 0.00399572 0.00190251 10.625 0.999998 1.79931 0.492 174.938 12.0682 A F 3.4e+21 4.22507e-14 1 dx
Report 2 X042331.45+602642.9 chandra ccd6 665.167 247.5 2.9971 1.73205 0.00255001 0.00147368 13.7261 1 0.492 0.492 180 3.46502 F F 3.45e+21 0 1 d
Report 1 X042322.89+603338.7 chandra ccd6 794.5 1092.5 2 1.41421 0.00170165 0.00120325 9.15958 0.999983 1.16688 0.492 161.565 9.5417 A F 3.42e+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