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 7 X182508.73-125331.6 chandra ccd7 560.163 830.556 89.5294 9.55797 0.0108487 0.00115819 29.576 1 0.443618 0.443618 0 0.467989 F F 1.53e+22 1.48883e-13 1 dsx
Report srcpi bgdpi arf 2 X182511.59-125157.6 chandra ccd7 475.381 1021.62 44.1217 7.22261 0.00534646 0.000875202 14.5756 1 0.471246 0.471246 0 1.25267 F F 1.53e+22 7.43564e-14 1 dsx
Report srcpi bgdpi arf 4 X182457.35-125115.0 chandra ccd7 898.646 1108.28 16.7052 5.85878 0.00202426 0.000709939 5.51855 0.999996 0.727452 0.727452 0 3.43051 F F 1.53e+22 2.9046e-14 1 dsx
Report srcpi bgdpi arf 1 X182548.90-125215.3 chandra ccd2 801.714 266.929 10.8329 3.74171 0.00131267 0.0004534 11.4841 1 2.11959 1.42862 92.5686 9.69663 F F 1.53e+22 2.56151e-14 1 dx
Report srcpi bgdpi arf 1 X182503.16-125211.3 chandra ccd7 725.4 993.3 9.6339 3.16228 0.00116738 0.000383188 3.18255 0.997061 0.492 0.492 139.399 1.73241 F F 1.53e+22 1.62433e-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