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 X004429.53+412136.3 chandra ccd1 725.214 466.643 6.92435 2.64575 0.0228527 0.00873186 30.0811 1 0.519021 0.492 166.224 5.70145 F F 1.36e+21 2.68912e-13 1 dx
Report srcpi bgdpi arf 1 X004344.61+412410.4 chandra ccd3 721.5 744.167 5.91592 2.44949 0.0195245 0.00808413 25.7094 1 0.957027 0.582929 78.4007 5.77795 A F 1.36e+21 2.39436e-13 1 dx
Report 3 X004412.87+412556.0 chandra ccd3 75.2998 958.3 4.9802 2.23607 0.0164363 0.00737976 21.6429 1 0.492 0.492 45 0.466275 F F 1.38e+21 0 1 d
Report 2 X004356.37+412203.3 chandra ccd3 452.833 485.5 2.99514 1.73205 0.00988494 0.00571634 13.0163 1 0.529672 0.492 100.278 5.35308 F F 1.36e+21 0 1 d
Report 1 X004424.80+413201.9 chandra ccd0 852.167 677.167 2.99159 1.73205 0.00987342 0.00571645 14.5537 1 1.11381 0.492 128.66 6.04765 A F 1.43e+21 0 1 d
Report srcpi bgdpi arf 1 X004415.91+413058.4 chandra ccd2 17 514 1.98248 1.41421 0.00654283 0.00466737 8.65141 0.999977 0.492 0.492 45 4.60654 F F 1.42e+21 7.68925e-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