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 X191116.08+003506.8 xmm mos1 314.549 314.94 697.268 30.6312 0.106878 0.0046952 77.7732 1 5.41296 5.41296 0 1.68232 F F 4.14326 0 1 ds
Report srcpi bgdpi 2 X191055.63+004236.9 xmm mos2 385.037 418.426 62.933 12.1248 0.0100607 0.00193831 7.67609 1 13.5287 4.73376 20.2216 10.7232 F F 4.01044 0 1 ds
Report srcpi bgdpi 2 X191052.03+004213.6 xmm mos1 397.477 413.052 104.829 10.2386 0.0160683 0.00156938 11.6926 1 23.691 23.691 0 10.839 T F 4.00521 0 1 dbcs
Report srcpi bgdpi 3 X191055.81+004235.9 xmm mos1 384.414 418.185 134.416 11.5995 0.0206035 0.00177798 14.9927 1 23.6961 23.6961 0 10.7019 T F 4.01071 0 1 dsc
Report srcpi bgdpi 1 X191137.92+002518.7 xmm mos2 239.225 179.752 22.8938 8.55858 0.00365987 0.0013682 2.79241 0.996689 7.70705 2.80755 23.251 9.60324 F F 4.29905 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