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 X010715.98-083429.6 chandra ccd7 301.549 256.387 96.1778 10.1304 0.0311178 0.00327762 37.8809 1 0.430407 0.430407 0 0.289183 F F 4.69e+20 2.29211e-13 1 dsx
Report srcpi bgdpi arf 1 X010642.90-084149.2 chandra ccd2 321.419 294.683 29.8126 5.46009 0.0096457 0.00176658 56.5866 1 7.14234 7.14234 0 11.0204 F F 4.55e+20 1.31368e-13 1 dsx
Report srcpi bgdpi arf 1 X010640.57-083300.8 chandra ccd3 189.625 362 7.10088 2.82845 0.00229744 0.000915122 13.1639 1 1.86468 1.47938 161.764 9.11586 F F 4.85e+20 3.10275e-14 1 dx
Report srcpi bgdpi arf 1 X010713.56-083708.2 chandra ccd6 569.071 958.5 6.88746 2.64575 0.00222838 0.000856014 12.2695 1 0.695362 0.492 134.628 2.56863 F F 4.66e+20 2.28675e-14 1 dx
Report srcpi bgdpi arf 2 X010716.72-083654.5 chandra ccd6 473.75 986.25 3.94249 2 0.00127556 0.000647085 7.02326 0.99998 0.492 0.492 45 2.21206 F F 4.65e+20 1.29789e-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