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 2 X174031.25-284728.6 chandra ccd3 440.7 90.5 4.97348 2.23607 0.00431272 0.001939 13.3221 1 0.492 0.492 41.2027 4.22038 F F 9.07e+21 0 1 d
Report srcpi bgdpi arf 1 X173940.69-285114.6 chandra ccd0 794.9 764.7 4.75371 2.23607 0.00412215 0.001939 13.7835 1 1.0501 0.492 11.0832 7.54701 A F 8.58e+21 6.79532e-14 1 dx
Report 1 X174015.15-284101.1 chandra ccd3 870.75 878.25 3.92955 2 0.00340749 0.00173429 10.5258 1 0.929155 0.492 154.685 7.24508 A F 8.45e+21 0 1 d
Report 1 X174037.72-285452.8 chandra ccd2 319.5 223.5 3.84381 2.00001 0.00333314 0.00173429 10.7406 0.99999 1.30461 0.492 116.565 8.66749 A F 9.54e+21 0 1 d
Report 2 X173952.94-284915.0 chandra ccd0 468.167 1008.17 2.99608 1.73205 0.00259803 0.00150194 8.68718 0.999992 0.492 0.492 45 4.36064 F F 8.66e+21 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