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 X173458.55-301004.8 chandra ccd3 345.694 551.34 15.8776 3.98467 0.00737173 0.00185002 35.8295 1 0.672698 0.672698 0 4.38008 F F 7.99e+21 1.05758e-13 1 dsx
Report srcpi bgdpi arf 1 X173539.28-301017.4 chandra ccd1 332.16 696.466 10.9497 3.30903 0.00509111 0.00153855 25.2833 1 1.6245 1.6245 0 7.36887 F F 8.5e+21 7.80368e-14 1 dsx
Report srcpi bgdpi arf 1 X173534.80-295942.8 chandra ccd0 605.5 950 4.30895 2.23608 0.00200055 0.00103816 10.167 0.999999 0.760713 0.492 14.0362 8.62514 A F 7.85e+21 3.26327e-14 1 dx
Report srcpi bgdpi arf 2 X173535.27-295940.2 chandra ccd0 593.214 955.214 13.1923 3.873 0.00612486 0.00179815 31.1273 1 0.96139 0.613356 176.798 8.72133 A F 7.85e+21 1.00202e-13 1 dx
Report 2 X173517.56-300741.5 chandra ccd1 904.167 1013.17 2.97393 1.73205 0.00138272 0.000805311 6.86692 0.999956 0.492 0.492 90 2.01857 F F 8.09e+21 0 1 d
Report 3 X173515.64-301055.9 chandra ccd1 954.833 618.167 2.96734 1.73205 0.00137965 0.000805311 6.8517 0.999956 0.492 0.492 163.155 4.60978 F F 8.24e+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