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 2 X170004.36-415804.4 chandra ccd3 769.588 5.84575 53.1494 7.40319 0.0475218 0.00661932 41.2795 1 0.976711 0.976711 0 0.600689 T F 1.57e+22 0 1 ds
Report srcpi bgdpi arf 1 X170024.81-415125.6 chandra ccd3 304.75 815.625 7.76358 2.82843 0.00694134 0.00252887 6.02974 0.99999 1.17388 0.492 43.9185 7.31071 A F 1.55e+22 1.32491e-13 1 dx
Report 1 X170039.37-420226.6 chandra ccd2 591.167 259.833 2.97936 1.73205 0.00266382 0.00154861 9.31991 0.999996 0.492 0.492 73.155 7.40107 F F 1.58e+22 0 1 d
Report 2 X170048.78-415703.3 chandra ccd2 376.833 916.5 2.9784 1.73205 0.00266296 0.00154861 9.31691 0.999996 0.492 0.492 180 7.72464 F F 1.57e+22 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