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 2 X191055.43+004234.3 xmm mos2 384.842 418.97 154.785 21.9003 0.00884185 0.00125102 8.58808 1 18.0117 4.44225 28.0866 10.7574 A F 4.01076 1.97378e-13 1 dscxf
Report srcpi bgdpi arf 1 X191053.58+004220.8 xmm mos1 391.228 415.654 61.7931 12.2637 0.00608997 0.00120864 3.3184 0.999387 10.875 10.875 0 10.8387 F F 4.00495 9.87445e-14 1 dbx
Report srcpi bgdpi arf 2 X191141.97+003840.5 xmm mos1 224.385 365.216 79.1652 16.6221 0.00450239 0.000945355 4.25132 0.999979 11.4125 5.81013 342.457 7.24923 F F 4.2127 8.04358e-14 1 dsx
Report srcpi bgdpi arf 3 X191055.75+004238.0 xmm mos1 383.726 419.811 91.8446 24.2533 0.00522351 0.00137937 4.93223 0.999999 4.41763 4.41763 0 10.7709 F F 4.01044 1.08699e-13 1 dsx
Report srcpi bgdpi arf 1 X191053.60+004221.5 xmm mos2 391.155 415.957 56.4923 11.8907 0.00307799 0.000647867 3.13441 0.998921 10.875 10.875 0 10.8527 F F 4.00494 5.91909e-14 1 dbcx

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