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 2 X174615.58-310858.4 chandra ccd3 526.7 597.9 4.95471 2.23607 0.0022971 0.00103668 12.1338 1 0.492 0.492 48.5625 5.16547 F F 8.53e+21 3.43561e-14 1 dx
Report 1 X174615.66-310053.7 chandra ccd2 731.1 549.1 4.79095 2.23607 0.00222117 0.00103669 11.8427 0.999999 0.599645 0.492 1.14531 6.08117 F F 8.82e+21 0 1 d
Report 3 X174630.55-310401.6 chandra ccd2 342 167.25 3.95058 2 0.00183156 0.000927238 9.76537 0.999999 0.492 0.492 97.4657 1.69785 F F 8.57e+21 0 1 d
Report 1 X174649.88-310651.0 chandra ccd1 672.5 1017.83 2.98976 1.73205 0.00138611 0.000803011 7.33102 0.999972 0.492 0.492 180 3.67537 F F 8.31e+21 0 1 d
Report 1 X174623.51-310550.0 chandra ccd3 319.833 980.833 2.98786 1.73205 0.00138523 0.000803011 7.31707 0.999972 0.492 0.492 45 2.21105 F F 8.57e+21 0 1 d
Report 2 X174650.05-310704.4 chandra ccd1 668.167 990.5 2.95915 1.73205 0.00137192 0.000803012 7.25595 0.999972 0.492 0.492 161.565 3.79147 F F 8.3e+21 0 1 d
Report srcpi bgdpi arf 2 X174604.35-310258.3 chandra ccd2 1026.5 295.5 0.881667 1.00001 0.000408757 0.000463622 2.17938 0.987983 0.492 0.492 90 6.81833 F F 8.86e+21 6.79798e-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