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 2 X233246.07-561548.3 xmm mos2 276.539 179.922 27.269 7.34162 0.00923201 0.00248553 5.76291 1 6.88694 3.64653 15.4878 8.73785 F F 7.63374 2.04877e-13 1 dsx
Report srcpi bgdpi arf 2 X233246.61-561545.7 xmm mos1 275.517 180.529 32.2956 6.187 0.0106372 0.00203781 9.47207 1 9.80756 5.41511 166.37 8.72097 F F 7.63457 2.0118e-13 1 dsx
Report srcpi bgdpi arf 1 X233413.72-560620.4 xmm mos1 107.918 309.914 23.7302 6.40289 0.00781603 0.00210892 6.9599 1 6.70991 1.97579 99.3352 13.8422 A F 7.87842 2.79279e-13 1 dsx
Report srcpi bgdpi arf 1 X233413.68-560621.2 xmm mos2 107.994 309.727 24.3375 6.51821 0.00823956 0.00220677 5.14338 0.999996 7.96337 2.37352 95.9222 13.8451 F F 7.87787 3.26533e-13 1 dsx
Report srcpi bgdpi arf 1 X233246.26-561550.7 xmm pn 276.187 179.399 61.3671 11.8154 0.0039574 0.000761946 0 10.875 10.875 0 8.77971 F F 7.63311 1.76756e-14 1 dpx

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