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 X173339.49-303543.7 chandra ccd3 705.9 996.3 9.90527 4.27872 0.00509048 0.00219891 32.182 1 1.58438 0.590876 41.5987 7.49419 2.90527 7 0.41339 0.471559 A F 8.3e+21 7.95888e-14 1 dx
Report srcpi bgdpi arf 1 X173351.53-305030.4 chandra ccd2 218.667 193.667 5.88896 3.59808 0.00302644 0.00184911 17.6725 1 1.4122 0.926013 171.687 9.73729 3.94448 0.94448 -0.613628 0.827814 A F 9.3e+21 5.42685e-14 1 dx
Report 2 X173326.15-304024.3 chandra ccd3 1056.1 426.1 4.98457 2.23607 0.00256166 0.00114915 12.2731 1 0.583846 0.492 51.6962 2.17375 F F 8.44e+21 0 1 d
Report 1 X173310.26-304827.9 chandra ccd0 255.1 288.9 4.40878 2.23608 0.00226575 0.00114916 11.454 0.999999 1.07632 0.614357 109.954 6.72016 A F 8.74e+21 0 1 d
Report srcpi bgdpi arf 1 X173311.67-303836.6 chandra ccd1 394 476.75 3.91531 3.17945 0.00201535 0.00163658 13.4537 1 0.492 0.492 142.018 4.92339 3 0.915307 -0.532447 0.936375 F F 8.29e+21 2.97308e-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