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 1 X170356.82-375036.5 xmm mos2 285.263 279.735 262038 539.261 12.9588 0.0266687 1545.02 1 9.13769 9.001 0 1.68872 F T 2.17333 5.0366e-10 1 dsxf
Report srcpi bgdpi arf 2 X170400.43-375030.5 xmm mos2 275.435 281.412 2297.79 71.3197 0.144752 0.00449288 13.5481 1 10.875 10.875 0 2.0747 F T 2.16504 1.91036e-12 1 dbx
Report srcpi bgdpi arf 1 X170437.84-380022.5 xmm mos1 173.828 144.913 47.7807 18.2001 0.00243468 0.00092739 3.79213 0.999859 4.70852 4.70852 0 14.397 F T 1.96662 8.26189e-14 1 dsx
Report srcpi bgdpi arf 2 X170450.25-375438.7 xmm mos1 139.903 223.859 42.8762 12.6826 0.00218477 0.000646247 3.40288 0.999458 5.32439 2.82501 82.5883 12.714 F T 1.99289 7.36636e-14 1 dsx
Report srcpi bgdpi arf 3 X170428.85-374137.3 xmm mos1 197.831 403.609 50.3667 11.1897 0.00256645 0.000570174 3.99737 0.999941 6.83747 3.46634 112.947 10.5406 F F 2.1813 8.06785e-14 1 dsx

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