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 X063518.36-533905.8 xmm pn 341.906 331.654 45.2199 9.91864 0.0452015 0.00991459 14.9333 1 10.875 10.875 0 3.96633 F F 3.85105 1.86285e-13 1 dx
Report srcpi bgdpi arf 2 X063604.20-534838.0 xmm pn 248.416 198.404 10.9938 3.95601 0.0109909 0.00395498 3.63057 0.999445 4.96916 4.96916 0 8.11481 F F 3.77937 7.40768e-14 1 dsx
Report srcpi bgdpi arf 3 X063553.79-534515.0 xmm pn 269.574 245.083 15.3275 5.47856 0.0153234 0.00547711 5.06172 0.999988 4.60691 4.60691 0 4.40823 F F 3.79076 7.09054e-14 1 dsx
Report srcpi bgdpi arf 4 X063509.68-534710.4 xmm pn 359.45 218.518 7.99562 4.21876 0.00799353 0.00421766 2.64045 0.993623 2.51768 2.51768 0 7.28426 F T 3.90409 0 1 ds
Report srcpi bgdpi arf 5 X063636.67-533153.3 xmm pn 181.53 429.201 12.9539 4.52619 0.0129505 0.00452499 4.27786 0.999912 5.55863 5.55863 0 12.7314 F F 3.63367 1.07147e-13 1 dsx

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