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 X173439.54-291112.7 chandra ccd3 441.167 390.389 8.64251 3.00001 0.00400115 0.00138889 18.0993 1 1.0689 0.751904 74.7757 6.02304 F F 5.89e+21 5.60963e-14 1 dx
Report srcpi bgdpi arf 1 X173517.89-291104.1 chandra ccd1 467.389 365.722 8.49653 3.00001 0.00393357 0.00138889 18.4584 1 1.43152 1.10694 44.2986 7.68761 F F 6.31e+21 5.78875e-14 1 dx
Report 1 X173443.90-290950.3 chandra ccd3 325.1 558.1 4.96111 2.23607 0.00229681 0.00103521 10.3896 1 0.781026 0.492 45 4.37148 A F 5.89e+21 0 1 d
Report 3 X173429.82-291309.7 chandra ccd3 699.5 152.5 4.62075 2.23608 0.00213923 0.00103522 9.67685 0.999996 0.492 0.492 31.7175 8.77986 F T 5.86e+21 0 1 d
Report 1 X173503.03-285917.2 chandra ccd0 823.25 780.75 3.94763 2 0.0018276 0.000925925 8.499 0.999997 0.771819 0.639127 90 6.98351 F F 5.72e+21 0 1 d
Report srcpi bgdpi arf 1 X173422.84-290335.2 chandra ccd2 857.5 302 1.94848 1.41422 0.000902073 0.000654728 4.00719 0.998153 0.5535 0.492 90 6.77028 F F 5.55e+21 1.32165e-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