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 1 X154115.79-552128.7 chandra ccd7 624.831 543.076 82.4934 9.08259 0.0426633 0.00469726 128.221 1 0.408054 0.408054 0 1.33283 F F 1.81e+22 6.23798e-13 1 dsx
Report 3 X154110.74-552251.5 chandra ccd7 711.667 374.167 5.93298 2.44949 0.00306836 0.0012668 9.22176 1 0.492 0.492 63.4349 2.03585 F F 1.81e+22 0 1 d
Report 1 X154145.33-552243.2 chandra ccd6 746.5 1148 3.94448 2 0.00203997 0.00103434 9.33223 0.999999 0.492 0.492 90 3.08365 F F 1.8e+22 0 1 d
Report 2 X154113.77-552648.8 chandra ccd6 1292.83 648.833 2.96893 1.73205 0.00153544 0.000895765 7.02417 0.999963 0.492 0.492 45 4.92882 F F 1.81e+22 0 1 d
Report 2 X154133.11-552112.8 chandra ccd7 324.167 574.833 2.94382 1.73205 0.00152245 0.000895765 4.57564 0.99912 0.492 0.492 45 1.56535 F F 1.8e+22 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