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 X174517.00-321356.5 chandra ccd2 101.389 522.203 66.3392 8.14489 0.0341563 0.00419358 165.764 1 1.06378 0.663257 70.6998 3.72949 3.8944 61.9472 0.881704 0.185989 F F 6.96e+21 4.72924e-13 1 dsx
Report srcpi bgdpi arf 2 X174454.75-321145.4 chandra ccd2 675 788 3.93582 3.17945 0.00202642 0.00163699 15.5356 1 0.649303 0.492 145.901 7.76904 4 -0.0641822 -1 1.14412 F F 7.21e+21 3.20069e-14 1 dx
Report 3 X174459.32-321625.8 chandra ccd2 556.75 218.25 3.95815 2 0.00203792 0.00102973 9.89035 0.999999 0.492 0.492 161.565 4.26894 F F 7.03e+21 0 1 d
Report srcpi bgdpi arf 4 X174502.69-321721.9 chandra ccd2 470.313 104.627 21.1652 4.60057 0.0108974 0.0023687 52.8862 1 0.573681 0.573681 0 3.38949 5.83053 15.7458 0.459544 0.295626 F F 6.97e+21 1.54624e-13 1 dsx

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