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 2 X181210.57-184208.4 xmm mos2 183.767 303.885 115.605 14.6555 0.0133322 0.00169016 0 10.875 10.875 0 8.32291 F T 0.143732 2.85088e-13 1 dx
Report srcpi bgdpi arf 3 X181113.20-182757.3 xmm mos1 371.238 499.763 86.4927 12.9085 0.00998376 0.00149002 13.6586 1 10.875 10.875 0 15.5211 F T 0.168638 2.93468e-13 1 dpx
Report srcpi bgdpi arf 2 X181210.51-184213.9 xmm mos1 183.943 302.794 20.8176 8.67867 0.00556929 0.00232179 3.28745 0.99873 5.96282 5.96282 0 8.31927 F T 0.14384 1.36708e-13 1 dsx
Report srcpi bgdpi arf 1 X181113.24-182755.8 xmm mos2 371.113 499.234 78.9429 11.9762 0.00910413 0.00138116 0 10.875 10.875 0 15.482 F T 0.168709 3.26977e-13 1 dpx
Report srcpi bgdpi arf 1 X181102.41-183251.6 xmm mos1 406.499 432.085 19.9321 6.75501 0.00533238 0.00180715 3.14761 0.99873 5.64365 5.64365 0 12.4378 F T 0.166472 1.22158e-13 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