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 X174937.74-305853.6 chandra ccd2 404 637 3.97152 2 0.00203888 0.00102675 10.7895 1 0.683104 0.492 103.283 6.01889 F F 6.84e+21 0 1 d
Report 3 X174921.21-305403.3 chandra ccd3 993 191.25 3.97157 2 0.00203886 0.00102673 10.2937 0.999999 0.492 0.492 104.872 0.864432 F F 7.18e+21 0 1 d
Report 2 X174928.57-305015.3 chandra ccd3 800.25 654.5 3.96128 2 0.00203358 0.00102673 10.267 0.999999 0.514845 0.492 120.779 4.89161 F F 7.2e+21 0 1 d
Report srcpi bgdpi arf 1 X174840.90-305549.7 chandra ccd0 854.25 853.25 4.9591 3.39792 0.00254598 0.00174448 24.5214 1 1.5181 0.733301 107.993 8.06772 0.959101 4 0.613196 0.815948 A F 7.6e+21 4.02793e-14 1 dx
Report 1 X174923.47-305415.1 chandra ccd3 933.833 167.167 2.96928 1.73205 0.00152432 0.000889173 7.69591 0.999982 0.563657 0.492 45 1.2081 F F 7.15e+21 0 1 d
Report srcpi bgdpi arf 1 X174858.99-304716.8 chandra ccd1 544.833 862.167 3.83316 3.17945 0.00196789 0.00163228 9.3843 0.999999 0.749069 0.492 34.722 8.38566 0.944385 2.88877 0.507254 0.946633 A F 7.62e+21 3.23168e-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