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 X202027.77+435117.0 xmm pn 280.198 284.608 77882 312.616 3.76812 0.0151251 552.83 1 5.90726 5.90726 0 1.65192 58979.8 41830.5 -0.170115 0.00321485 F T 8.4e+21 2.06825e-11 1 dsx
Report srcpi bgdpi arf rmf 2 X202027.73+435117.3 xmm mos2 280.275 284.667 31929.1 206.316 1.41182 0.00912276 309.58 1 5.61005 5.0196 26.8033 1.64827 23998.8 18560.5 -0.12778 0.00491976 F T 8.4e+21 2.43238e-11 1 dsx
Report srcpi bgdpi arf rmf 1 X202027.77+435117.4 xmm mos1 280.183 284.683 32112 203.58 1.42029 0.00900419 332.4 1 5.49501 5.30659 23.267 1.65314 23938.5 18531.8 -0.127306 0.00492536 F T 8.4e+21 2.32167e-11 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