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 X183054.56+011547.4 xmm mos2 123.109 355.917 52.8741 12.1406 0.0160631 0.00368828 2.27697 0.988242 10.875 10.875 0 13.3769 F F 5.14284 0 1 d
Report srcpi bgdpi 3 X183055.60+011410.0 xmm mos2 119.507 333.393 56.6915 11.8409 0.0172228 0.00359726 2.44136 0.991576 10.875 10.875 0 13.2176 F F 5.12663 0 1 d
Report srcpi bgdpi 4 X183055.45+011101.3 xmm mos2 120.024 290.736 63.3836 12.2427 0.0192558 0.00371932 2.72955 0.99633 10.875 10.875 0 12.9469 F F 5.10329 0 1 d
Report srcpi bgdpi 6 X183003.17+011000.6 xmm mos2 300.259 276.322 47.2579 24.2174 0.014357 0.00735726 2.03512 0.978004 14.5417 5.65106 63.7429 1.68454 F F 5.28925 0 1 ds
Report srcpi bgdpi 7 X182953.33+010941.6 xmm mos2 334.2 271.821 58.707 12.9573 0.0194925 0.00430222 2.52816 0.993306 10.875 10.875 0 3.23208 F F 5.3235 0 1 db
Report srcpi bgdpi 8 X183051.42+011732.3 xmm mos2 133.931 376.921 81.7667 17.1986 0.0248406 0.00522491 3.5212 0.999692 10.875 10.875 0 13.2145 F F 5.16776 0 1 db

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