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 4 X173546.28-320709.8 chandra ccd7 674.173 285.778 43.5449 6.79362 0.0216703 0.00338087 26.9619 1 0.490418 0.361803 142.313 0.558973 F F 1.32e+22 2.82136e-13 1 dsx
Report srcpi bgdpi arf 2 X173557.59-320154.0 chandra ccd7 381.5 927.269 12.6547 3.60556 0.00629765 0.00179432 7.83547 1 0.952942 0.691146 95.6129 5.88483 F F 1.32e+22 8.83795e-14 1 dpx
Report srcpi bgdpi arf 1 X173525.76-321931.0 chandra ccd5 877.734 860.023 12.4579 6.62701 0.00619974 0.00329796 2.22111 0.980111 5.91444 3.37702 239.265 12.9702 F F 1.33e+22 1.19438e-13 1 dsx
Report srcpi bgdpi arf 3 X173540.81-320101.0 chandra ccd7 815.333 1035 5.54786 2.4495 0.00276092 0.001219 3.4351 0.99848 1.30084 0.598164 26.5326 6.64923 A F 1.33e+22 4.01904e-14 1 dx
Report 1 X173549.72-320256.2 chandra ccd7 585 800.75 3.89796 2 0.00193984 0.000995309 2.41352 0.982561 0.762661 0.492 32.1616 4.53149 A F 1.32e+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