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 X042021.43-502114.2 xmm pn 254.585 296.366 156.706 42.9734 0.00958918 0.00262964 3.58552 0.999795 4.84776 4.84776 0 3.16727 F T 4.3402 0 1 ds
Report srcpi bgdpi 2 X042001.87-502248.1 xmm pn 297.622 274.802 324.224 49.5431 0.0198399 0.00303164 7.41842 1 5.21079 5.21079 0 1.71192 F T 4.38642 0 1 ds
Report srcpi bgdpi 1 X042002.02-502249.9 xmm mos2 297.294 274.396 64.3085 13.5398 0.0046984 0.000989223 5.8947 1 5.65415 3.54596 53.6932 1.75323 F T 4.38574 0 1 ds
Report srcpi bgdpi 1 X042018.44-503159.1 xmm mos1 261.312 147.4 52.376 12.6081 0.00554821 0.00133558 0 10.875 10.875 0 11.2761 F T 4.31515 0 1 d
Report srcpi bgdpi 2 X041915.30-502239.5 xmm mos2 400.027 276.577 48.0494 10.4141 0.00517529 0.00112168 4.40435 0.999987 10.875 10.875 0 7.53385 F T 4.50837 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 - 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