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 2 X174147.73-264647.0 chandra ccd1 661.7 1006.4 9.89793 3.16228 0.00459538 0.00146817 24.1448 1 0.810428 0.492 160.088 3.85981 A F 5.15e+21 5.87043e-14 1 dx
Report srcpi bgdpi arf 1 X174206.16-264117.2 chandra ccd0 148.2 632.3 9.05808 3.1623 0.00420546 0.00146818 21.5829 1 2.7969 1.25234 143.513 9.59516 A F 5.19e+21 6.59102e-14 1 dx
Report srcpi bgdpi arf 1 X174205.38-265046.2 chandra ccd1 181.833 519.833 8.53054 3.00001 0.00396054 0.00139284 20.8092 1 3.46681 0.622073 27.9069 8.82795 A F 5.46e+21 5.72903e-14 1 dx
Report 2 X174109.41-264918.0 chandra ccd3 670.5 710.5 2.97831 1.73205 0.00138276 0.000804152 7.02819 0.999962 0.492 0.492 180 5.40428 F F 4.81e+21 0 1 d
Report 1 X174127.41-264646.2 chandra ccd3 180.833 1019.17 2.97454 1.73205 0.00138101 0.000804152 7.0193 0.999962 0.492 0.492 45 0.694798 F F 4.91e+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