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 3 X095337.44-050825.6 chandra ccd1 707.242 1259.57 11.9809 3.46134 0.00491347 0.00141953 29.3581 1 0.516993 0.219934 359.953 1.82733 F F 3.15e+20 5.90438e-14 1 dsx
Report srcpi bgdpi arf 1 X095406.64-050452.7 chandra ccd0 593.9 996.9 9.60845 3.16229 0.00394044 0.00129686 24.3728 1 1.47773 0.795064 13.2376 7.71036 A F 3.05e+20 5.48074e-14 1 dx
Report srcpi bgdpi arf 1 X095341.03-051712.0 chandra ccd1 597.5 189.167 8.3073 3.00002 0.00340684 0.00123031 20.3563 1 1.90551 1.45536 26.5651 10.6456 F F 3.25e+20 5.06778e-14 1 dx
Report srcpi bgdpi arf 2 X095336.25-051300.4 chandra ccd1 742.786 700.643 6.80002 2.64576 0.0027887 0.00108503 16.6628 1 1.11575 0.628163 165.964 6.39097 A F 3.21e+20 3.51799e-14 1 dx
Report 2 X095354.78-050501.1 chandra ccd0 954.167 979.833 2.96563 1.73205 0.00121621 0.000710318 7.52262 0.999979 0.492 0.492 16.845 4.82973 F F 3.07e+20 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