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 1 X165749.77+352032.1 xmm mos1 286.408 275.715 1099.58 39.1228 1.72139 0.0612464 0 10.875 10.875 0 1.86391 F F 7.52284 0 1 db
Report srcpi bgdpi 1 X165749.75+352031.8 xmm mos2 286.47 275.476 620.374 28.2238 1.93873 0.0882023 46.7344 1 5.81693 5.81693 0 1.89388 F F 7.52281 0 1 dbs
Report srcpi bgdpi 1 X165743.55+352129.6 xmm pn 303.907 288.755 192.484 41.7368 0.176371 0.0382431 3.96162 0.999956 14.0193 14.0193 0 1.16212 T F 7.53751 0 1 ds
Report srcpi bgdpi 2 X165749.75+352031.5 xmm pn 286.469 275.401 5560.21 93.446 5.09477 0.0856237 114.438 1 5.71424 5.20878 346.694 1.89286 F T 7.52289 0 1 ds

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