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 rmf 1 X042600.70-571202.3 xmm mos1 313.563 279.566 2356.61 55.0694 1.81093 0.042318 90.6368 1 5.71847 5.71847 0 1.74158 F T 1.99637 1.51134e-11 1 dsxf
Report srcpi bgdpi arf rmf 1 X042600.76-571201.9 xmm mos2 313.449 279.646 2464.57 58.1792 1.75392 0.0414033 81.2434 1 5.25604 5.25604 0 1.73719 F T 1.99629 1.62114e-11 1 dsxf
Report srcpi bgdpi arf 1 X042538.60-571436.3 xmm pn 354.781 244.104 1689.68 49.7472 1.86183 0.0548156 54.5833 1 10.875 10.875 0 5.6748 F T 2.03309 5.4452e-12 1 dx
Report srcpi bgdpi arf 2 X042612.79-571506.7 xmm pn 290.999 237.023 105.939 13.7334 0.107183 0.0138946 3.42223 0.999632 10.875 10.875 0 4.48507 F F 1.95654 3.23046e-13 1 dpx
Report srcpi bgdpi arf rmf 3 X042600.71-571202.0 xmm pn 313.555 279.638 3346.67 65.6121 6.5351 0.128122 108.11 1 5.90089 5.90089 0 1.74653 F T 1.99657 1.26362e-11 1 dsxf

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