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 X182817.85-033445.2 xmm mos2 249.381 253.269 37.9645 11.4666 0.00172059 0.000519679 3.73528 0.999823 4.50095 4.50095 0 4.83709 F F 3.50074 3.22709e-14 1 dsx
Report srcpi bgdpi arf 2 X182808.19-033338.6 xmm mos2 282.631 268.573 35.8287 12.1912 0.0016238 0.000552519 3.52514 0.999656 3.78197 3.78197 0 2.43803 F F 3.54493 2.2327e-14 1 dsx
Report srcpi bgdpi arf 3 X182739.41-032728.9 xmm mos2 381.7 353.549 21.9575 11.2834 0.000995136 0.000511376 2.16037 0.983329 8.76687 5.79855 307.938 7.33196 A F 3.69983 1.56226e-14 1 dsx
Report srcpi bgdpi arf 4 X182803.00-033438.5 xmm mos2 300.507 254.804 26.699 11.3241 0.00121003 0.000513219 2.62688 0.995139 3.51828 3.51828 0 3.16439 F F 3.55652 2.13162e-14 1 dsx
Report srcpi bgdpi arf 5 X182746.76-032210.9 xmm mos2 356.39 426.621 36.5745 8.16133 0.0031667 0.000706627 3.59851 0.999656 10.875 10.875 0 10.199 F F 3.71212 5.96299e-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 - 10.00 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), A = 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