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 X184323.19-731044.0 xmm pn 352.665 357.057 70.8198 17.6356 0.0221818 0.00552372 0 10.875 10.875 0 5.78959 U U 6.8e+20 d
Report 2 X184321.73-731118.9 xmm pn 354.089 349.359 77.3988 17.6768 0.0242424 0.00553664 0 10.875 10.875 0 5.46895 U U 6.81e+20 d
Report 3 X184334.48-731228.3 xmm pn 341.33 332.957 78.7792 17.8094 0.043468 0.00982671 0 10.875 10.875 0 3.99174 U U 6.81e+20 d
Report 4 X184321.59-731021.8 xmm pn 354.279 362.121 86.4584 17.7434 0.02708 0.0055575 0 10.875 10.875 0 6.14074 U U 6.79e+20 d
Report 1 X184438.84-731812.9 xmm mos1 277.332 253.705 72.073 15.5885 0.0142101 0.00307346 0 10.875 10.875 0 3.58586 U U 6.79e+20 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