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 X182948.45-110601.3 xmm pn 306.415 293.91 109.921 19.8406 0.0311626 0.00562482 6.52571 1 13.5099 8.19465 88.0975 0.652788 T F 0.315118 3.30257e-13 1 dsxf
Report srcpi bgdpi arf 2 X182943.84-105757.0 xmm pn 322.038 405.288 78.2134 15.0432 0.0156443 0.00300897 4.64332 0.999995 10.875 10.875 0 7.93345 F F 0.235603 8.14341e-14 1 dx
Report srcpi bgdpi arf 1 X182948.77-110605.2 xmm mos1 305.335 293.02 40.648 15.4813 0.00550988 0.00209851 3.2222 0.998998 6.30578 6.30578 0 0.655833 F F 0.315865 6.5553e-14 1 dsx
Report srcpi bgdpi arf 2 X182943.96-105759.5 xmm mos1 321.622 404.673 35.2761 12.4309 0.00478171 0.00168502 2.79636 0.996743 5.21418 5.21418 0 7.87354 F F 0.23701 1.14274e-13 1 dbsx
Report srcpi bgdpi arf 2 X182948.67-110601.7 xmm mos2 305.669 293.805 26.3864 15.4313 0.00357526 0.00209089 1.81334 0.965121 5.22689 5.22689 0 0.583178 F F 0.31613 4.78852e-14 1 dsx

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