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 1 X174549.45-262634.3 chandra ccd1 910.944 843.5 8.95096 3 0.00414991 0.00139088 18.8379 1 0.653178 0.492 95.7168 3.16614 F F 6.92e+21 0 1 d
Report srcpi bgdpi arf 1 X174503.62-263027.2 chandra ccd3 1134.5 196.5 6.42055 2.64577 0.00297247 0.00122489 14.3034 1 2.90015 1.27519 63.3035 11.017 A F 6.6e+21 4.98963e-14 1 dx
Report srcpi bgdpi arf 2 X174556.36-262727.5 chandra ccd1 722.5 735.3 4.92469 2.23607 0.00228322 0.0010367 10.3643 1 0.525389 0.492 7.76206 4.77154 F F 7.03e+21 3.13466e-14 1 dx
Report srcpi bgdpi arf 1 X174537.48-262222.2 chandra ccd2 388.833 133.833 2.99102 1.73205 0.00138672 0.000803026 6.66997 0.999942 0.492 0.492 73.155 1.84278 F F 6.71e+21 2.0375e-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