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 1 X174357.69-294349.5 xmm pn 302.941 272.732 412.917 33.6693 0.0611328 0.00498477 0 10.875 10.875 0 1.89201 U U 1.27e+22 d
Report 2 X174355.65-294347.1 xmm pn 309.053 273.517 605.156 37.3858 0.0950503 0.00587209 0 10.875 10.875 0 1.96379 U U 1.27e+22 d
Report 3 X174357.09-294248.6 xmm pn 304.765 286.625 123.967 25.8618 0.0172723 0.00360331 0 10.875 10.875 0 0.971536 U U 1.27e+22 d
Report 4 X174401.51-294351.9 xmm pn 291.513 272.272 131.007 24.1875 0.0185642 0.00342746 0 10.875 10.875 0 1.96222 U U 1.27e+22 d
Report 1 X174359.86-294402.1 xmm mos2 296.462 270.969 132.434 17.9776 0.0151028 0.00205017 0 10.875 10.875 0 1.99653 U U 1.27e+22 d
Report 2 X174417.53-294947.5 xmm mos2 243.586 189.388 55.8996 11.2084 0.00842478 0.00168924 0 10.875 10.875 0 8.84983 U U 1.25e+22 d

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