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 X130247.68-635007.9 xmm pn 303.562 275.557 11362.7 121.551 2.28609 0.0244552 194.527 1 5.82754 5.82754 0 1.68739 F T 0.991582 1.13833e-11 1 dsxf
Report srcpi bgdpi arf rmf 1 X130247.63-635007.3 xmm mos2 303.633 275.693 4172.84 74.1734 1.0743 0.019096 114.471 1 5.19763 5.19763 0 1.68193 F T 0.991341 1.88488e-11 1 dsxf
Report srcpi bgdpi arf rmf 1 X130247.69-635007.2 xmm mos1 303.547 275.725 4047.2 72.8475 1.06067 0.0190915 114.037 1 5.32153 5.32153 0 1.67893 F T 0.991315 1.6645e-11 1 dsxf
Report srcpi bgdpi arf 5 X130158.66-635808.6 xmm mos1 377.721 165.041 3159.23 67.3486 1.21117 0.0258197 89.0166 1 10.875 10.875 0 11.2504 F T 1.12113 1.97058e-11 1 dx
Report srcpi bgdpi arf 4 X130158.49-635808.6 xmm mos2 377.97 165.037 3029.53 66.7754 0.586464 0.0129266 83.1069 1 10.875 10.875 0 11.26 F T 1.12111 1.1288e-11 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