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 X081929.22+704219.3 xmm pn 306.72 319.638 6948.76 93.4119 1.99217 0.0267807 269.04 1 5.81279 5.81279 0 1.66462 F T 2.72387 4.12019e-12 1 dsxf
Report srcpi bgdpi arf rmf 2 X081929.16+704219.1 xmm mos2 306.791 319.587 3682.8 70.0393 0.559499 0.0106405 105.321 1 5.17323 4.8258 55.1474 1.6685 F T 2.72391 5.21873e-12 1 dscxf
Report srcpi bgdpi arf rmf 1 X081929.27+704219.1 xmm mos1 306.659 319.593 3795.86 70.2833 0.57235 0.0105975 112.233 1 5.62188 5.62188 0 1.66294 F T 2.72385 4.54684e-12 1 dsxf
Report srcpi bgdpi arf 1 X081930.29+704216.9 xmm mos2 305.5 318.065 1106.47 135.004 0.0988234 0.0120578 31.6429 1 10.875 10.875 0 1.5124 T T 2.72565 9.49681e-13 1 dcbx
Report srcpi bgdpi arf 2 X081857.62+703709.1 xmm pn 342.92 248.371 78.0552 13.8415 0.022378 0.00396827 3.02212 0.998585 5.8012 5.8012 0 4.86172 F T 2.69793 8.6262e-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