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 X095417.07-040827.3 chandra ccd3 652.75 284.5 3.85645 2 0.00157956 0.000819178 9.89666 0.999999 1.3816 0.492 87.8521 6.59217 A F 2.75e+20 2.05909e-14 1 dx
Report 2 X095422.96-040539.7 chandra ccd3 473.5 625.167 2.98176 1.73205 0.00122129 0.000709427 7.65198 0.99998 0.627179 0.492 33.6901 3.99433 F F 2.74e+20 0 1 d
Report 1 X095435.56-040023.7 chandra ccd2 829.5 493.5 2.96815 1.73205 0.00121572 0.000709428 7.50644 0.999978 0.587531 0.492 151.845 4.20261 F F 2.72e+20 0 1 d
Report srcpi bgdpi arf 1 X095425.92-041122.5 chandra ccd1 1111.5 631.5 2.86547 1.73206 0.00117366 0.000709429 7.31588 0.99998 0.830895 0.492 16.845 7.50302 A F 2.73e+20 1.5554e-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