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 X220245.49+185716.1 xmm mos2 360.206 345.317 16.0856 4.01069 0.00297727 0.000742335 4.48734 0.999926 7.5267 7.5267 0 5.57138 F F 8.40882 0 1 ds
Report srcpi bgdpi 2 X220312.21+185635.2 xmm mos2 273.064 335.902 34.8567 6.97001 0.00645159 0.00129007 9.72385 1 5.60272 5.60272 0 3.28764 F F 8.48775 0 1 ds
Report srcpi bgdpi 3 X220302.07+185238.1 xmm mos2 306.153 281.403 11.8594 6.05117 0.00219504 0.00112 3.30837 0.998284 3.57005 3.57005 0 1.35606 F F 8.50903 0 1 ds
Report srcpi bgdpi 4 X220320.54+184929.7 xmm mos2 245.85 237.771 27.195 6.26181 0.00731584 0.00168452 7.58648 1 10.875 10.875 0 5.82066 F F 8.59688 0 1 dp
Report srcpi bgdpi 5 X220340.16+184751.1 xmm mos2 181.804 215.479 14.7844 5.26326 0.00273642 0.000974167 4.12435 0.99983 3.47452 3.47452 156.655 10.4089 F F 8.66974 0 1 ds
Report srcpi bgdpi 6 X220357.63+190156.9 xmm mos2 125.017 409.722 37.7045 7.33416 0.0069786 0.00135745 10.5183 1 10.875 10.875 0 14.939 F F 8.54321 0 1 dp

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