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 1 X080335.24-400013.3 xmm pn 297.088 321.319 122175 384.415 5.5918 0.0175942 1427.52 1 5.93833 5.93833 0 1.65063 F T 4.70534 0 1 ds
Report srcpi bgdpi 1 X080335.20-400012.7 xmm mos1 297.207 321.45 31652 200.225 1.49747 0.00947273 344.569 1 5.84165 5.57225 325.847 1.65517 F T 4.70556 0 1 ds
Report srcpi bgdpi 2 X080326.85-400159.7 xmm pn 319.24 296.844 455.653 46.8367 0.0208547 0.00214366 5.32395 1 14.0629 14.0629 0 1.50294 T T 4.74367 0 1 dsc
Report srcpi bgdpi 4 X080325.60-400221.4 xmm pn 322.542 291.868 447.154 39.4507 0.0204657 0.00180561 5.22464 1 14.3503 14.3503 0 1.86587 T F 4.75137 0 1 dsc
Report srcpi bgdpi 5 X080323.78-400244.1 xmm pn 327.345 286.645 452.346 36.1203 0.0207034 0.00165319 5.28531 1 14.723 14.723 0 2.31059 T F 4.75958 0 1 dsc

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