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 X153923.02-521747.1 chandra ccd7 310.056 347.056 8.06183 3.00002 0.00150572 0.000560319 8.36354 0.999999 1.32927 0.734425 94.8086 5.65074 A F 6.37e+21 0 1 d
Report 2 X153927.90-521851.4 chandra ccd7 218.833 216.5 7.9457 3.00002 0.00148403 0.000560319 8.24306 0.999999 1.10858 0.876399 168.401 5.86412 F F 6.45e+21 0 1 d
Report 3 X153929.97-521324.9 chandra ccd7 181.1 880.3 9.82155 3.16228 0.00183439 0.000590624 10.1891 1 0.652086 0.505557 47.7638 3.52194 F F 6.22e+21 0 1 d
Report 4 X153924.13-521722.5 chandra ccd7 289.5 397.1 4.57923 2.23608 0.00085527 0.000417636 4.7506 0.999594 0.686153 0.492 95.0623 5.27042 F F 6.36e+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