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 X081059.21+760242.6 xmm pn 283.38 280.174 4722.86 76.9402 7.5185 0.122484 136.512 1 6.42296 6.42296 0 1.71967 F T 1.03327 0 1 ds
Report srcpi bgdpi 1 X081059.19+760243.2 xmm mos2 283.393 280.302 11264.1 120.406 2.37195 0.0253546 271.253 1 5.67287 5.67287 0 1.71847 F T 1.03328 0 1 dsp
Report srcpi bgdpi 1 X081059.29+760243.1 xmm mos1 283.309 280.276 11246 119.495 2.29914 0.0244296 279.919 1 6.01375 5.76211 5.24983 1.71944 F T 1.03328 0 1 ds
Report srcpi bgdpi 6 X081241.75+760609.4 xmm mos2 198.51 328.12 258.777 21.7759 0.0544923 0.00458549 6.23165 1 5.58066 5.58066 0 7.56548 F F 1.12123 0 1 ds
Report srcpi bgdpi 3 X081242.09+760609.1 xmm mos1 198.231 328.059 316.808 22.6266 0.0647684 0.0046258 7.88553 1 7.64155 5.85734 294.91 7.57234 F T 1.12129 0 1 ds
Report srcpi bgdpi 3 X081107.49+760313.1 xmm mos2 276.5 286.979 81.3907 16.4356 0.0169741 0.00342767 1.95998 0.97389 10.875 10.875 0 1.79429 F T 1.0396 0 1 dc

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