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 X054334.26-682221.3 xmm pn 296.602 321.956 464.43 74.8126 0.053581 0.00863108 6.4827 1 5.61333 5.61333 0 1.7114 F F 1.30595 8.1506e-14 1 dsxf
Report srcpi bgdpi arf rmf 1 X054134.34-682548.4 xmm mos2 448.632 273.751 384.754 29.8769 0.0536173 0.00416349 17.0728 1 5.95027 5.95027 0 11.0541 F F 1.48414 2.62083e-12 1 dsxf
Report srcpi bgdpi arf rmf 1 X054134.16-682545.8 xmm mos1 448.861 274.331 291.889 37.3735 0.0389455 0.00498659 8.78129 1 9.05854 3.89114 296.503 11.0512 A F 1.48415 2.39036e-12 1 dsxf
Report srcpi bgdpi arf 2 X054334.13-682221.5 xmm mos2 296.774 321.868 149.406 19.1774 0.0175387 0.00225122 6.62962 1 10.875 10.875 0 1.70306 F F 1.306 1.86983e-13 1 dbx
Report srcpi bgdpi arf 3 X054237.69-683206.0 xmm mos2 367.998 187.225 71.552 14.6973 0.0079786 0.00163886 3.17499 0.999079 10.875 10.875 0 9.5102 F F 1.37762 1.59539e-13 1 dx

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