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 X170205.91-295619.3 chandra ccd7 265.955 358.253 30.7803 5.84468 0.00113849 0.000216181 11.9883 1 0.415712 0.415712 0 0.963231 F F 1.82e+21 8.52589e-15 1 dsx
Report srcpi bgdpi arf 2 X170206.97-295534.6 chandra ccd7 237.4 448.5 8.64688 3.1623 0.000319826 0.000116965 3.36779 0.998664 0.504006 0.492 143.086 1.73376 F F 1.81e+21 2.42027e-15 1 dx
Report srcpi bgdpi arf 3 X170207.00-295352.5 chandra ccd7 237.122 656.545 14.0985 3.7548 0.000521469 0.000138881 5.4911 0.999994 1.53446 0.615596 135.299 3.42091 T F 1.8e+21 4.04914e-15 1 dsx
Report srcpi bgdpi arf rmf 4 X170206.53-295644.3 chandra ccd7 249.488 307.417 256.623 16.55 0.00949188 0.000612144 99.9498 1 0.436785 0.361881 82.0802 0.59007 F F 1.82e+21 3.61119e-14 1 dsxf
Report srcpi bgdpi arf 6 X170202.86-295742.8 chandra ccd7 345.929 187.928 6.15092 2.64577 0.000227507 9.78603e-05 2.39567 0.982263 0.492 0.492 37.4658 0.706862 F F 1.83e+21 1.70098e-15 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