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 1 X153253.98-601417.0 xmm pn 344.181 297.927 43.9755 14.5185 0.039451 0.0130248 3.74311 0.999852 10.875 10.875 0 3.31669 33.9323 4.77365 -0.753338 0.455333 F F 4.96e+21 3.03823e-13 1 dbpx
Report srcpi bgdpi arf 2 X153323.20-601017.9 xmm mos1 294.167 352.099 26.5946 14.3128 0.00336971 0.00181352 1.99189 0.973319 3.97902 3.97902 0 3.86478 26.2789 0.580251 -0.956793 0.385468 F F 5.01e+21 9.30362e-14 1 dbsx
Report srcpi bgdpi arf 2 X153323.28-601019.4 xmm pn 294.03 351.615 28.0404 14.4815 0.0251554 0.0129915 2.26723 0.987904 10.875 10.875 0 3.8686 22.7601 5.59781 -0.605203 0.586491 F F 5.01e+21 1.70643e-13 1 dbpx

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