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 X223839.82-203418.1 xmm pn 297.076 328.955 449.513 48.0957 0.0109843 0.00117527 0 10.875 10.875 0 2.21474 U U 2.08e+20 d
Report 2 X223840.57-203440.4 xmm pn 294.643 322.924 394.816 49.1342 0.00911289 0.00113408 0 10.875 10.875 0 1.79648 U U 2.08e+20 d
Report 3 X223841.19-203501.5 xmm pn 292.658 318.903 465.387 52.3821 0.0105465 0.00118708 0 10.875 10.875 0 1.5418 U U 2.07e+20 d
Report 4 X223837.17-203603.8 xmm pn 305.63 304.111 773.412 54.2452 0.0178739 0.00125363 0 10.875 10.875 0 0.664255 U U 2.07e+20 d
Report 5 X223845.23-203652.7 xmm pn 279.6 292.726 113471 436.585 2.42511 0.0093307 0 10.875 10.875 0 1.42701 U U 2.06e+20 d
Report 6 X223855.66-203644.1 xmm pn 245.963 294.508 101.487 25.8521 0.0027216 0.000693281 0 10.875 10.875 0 3.81502 U U 2.06e+20 d
Report 7 X223845.55-203717.2 xmm pn 278.596 287.264 489455 829.858 10.4937 0.0177918 0 10.875 10.875 0 1.65084 U U 2.06e+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