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 X171509.09+600718.4 xmm mos1 313.544 279.993 38.5966 13.5353 0.00500585 0.00175549 3.2096 0.999085 5.67919 5.67919 0 1.74297 F T 5.18466 0 1 ds
Report srcpi bgdpi 1 X171336.93+600221.4 xmm pn 472.282 211.49 88.5909 19.0151 0.00908717 0.00195047 0 10.875 10.875 0 14.0922 F T 5.38379 0 1 d
Report srcpi bgdpi 2 X171509.14+600718.9 xmm pn 313.446 280.143 202.387 22.7012 0.0281834 0.00316125 0 10.875 10.875 0 1.71556 F T 5.18424 0 1 dp
Report srcpi bgdpi 3 X171500.59+601027.1 xmm pn 328.081 322.983 80.0336 18.9493 0.0120738 0.00285867 0 10.875 10.875 0 2.79037 F T 5.19623 0 1 dpb
Report srcpi bgdpi 1 X171508.82+600717.6 xmm mos2 314.006 279.821 45.5672 13.4068 0.00489184 0.00143928 3.99337 0.999922 4.45932 4.45932 0 1.75579 F T 5.18493 0 1 ds
Report srcpi bgdpi 3 X171450.36+601407.5 xmm mos2 345.54 374.095 48.2566 13.2095 0.00518055 0.0014181 4.22906 0.999971 6.76591 6.76591 0 6.47063 F T 5.21094 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