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 X182615.04-145053.2 xmm pn 279.445 283.027 6589.06 93.2629 0.626941 0.00887386 143.481 1 5.93912 5.69491 32.1026 1.77501 F T 1.2894 3.7649e-12 1 dsxf
Report srcpi bgdpi arf rmf 3 X182615.00-145052.9 xmm mos2 279.562 283.1 3233.76 66.3757 0.303321 0.00622593 94.4603 1 5.63707 4.94703 14.5998 1.76637 F T 1.28914 5.62806e-12 1 dsxf
Report srcpi bgdpi arf 1 X182615.00-145052.2 xmm mos1 279.576 281.043 3292.97 78.417 0.410239 0.0097692 338.394 1 10.875 10.875 0 1.86012 F T 1.28909 4.09179e-12 1 dpx
Report srcpi bgdpi arf 2 X182538.73-144504.4 xmm mos1 400.526 363.181 35.2089 11.3976 0.00330263 0.0010691 3.61816 0.999665 5.92911 5.92911 0 8.77055 F F 1.11454 9.40925e-14 1 dsx
Report srcpi bgdpi arf 3 X182626.57-143842.2 xmm mos1 240.956 450.88 34.8827 8.37916 0.00327201 0.000785968 3.58464 0.999665 10.875 10.875 0 11.8117 F T 1.23589 7.82188e-14 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