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 1 X122232.97+153754.7 chandra ccd6 1292.59 607.143 69.6175 8.34371 0.0359458 0.00430813 175.27 1 1.5573 0.818109 37.4325 4.11331 T F 2e+20 0 1 ds
Report 1 X122222.14+153301.0 chandra ccd7 952.718 825.38 10.3323 3.21439 0.00533488 0.00165969 17.6801 1 0.769853 0.769853 0 3.81369 F F 2.01e+20 0 1 ds
Report 2 X122245.59+153232.6 chandra ccd7 263.375 767 7.91588 2.82843 0.00408718 0.00146039 13.5452 1 0.558454 0.492 35.9979 2.40061 F F 2.02e+20 0 1 d
Report 2 X122236.36+153653.0 chandra ccd6 1192.5 481.357 6.953 2.64575 0.00359001 0.00136607 17.5049 1 0.492 0.492 123.401 2.95134 F F 2.01e+20 0 1 d
Report 3 X122241.68+153106.3 chandra ccd7 378.214 591.643 6.90013 2.64575 0.00356272 0.00136607 11.8071 1 0.492 0.492 22.5 3.01331 F F 2.02e+20 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