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 X130247.74-635009.6 xmm pn 307.159 320.175 44286.2 223.708 3.25409 0.0164377 583.579 1 7.20264 6.79506 335.52 1.69494 F T 0.991756 1.57806e-11 1 dsxf
Report srcpi bgdpi arf rmf 3 X130247.92-635009.6 xmm mos2 306.885 320.178 18359.6 154.51 1.33544 0.0112387 247.25 1 5.62237 4.95606 346.726 1.69111 F T 0.991903 2.00667e-11 1 dsxf
Report srcpi bgdpi arf rmf 1 X130247.87-635010.5 xmm mos1 306.96 319.97 17743.8 149.323 1.29089 0.0108635 262.946 1 5.21983 5.21983 0 1.67207 F T 0.992143 1.78816e-11 1 dscxf
Report srcpi bgdpi arf 2 X130158.85-635810.1 xmm mos2 381.108 209.786 5794.76 89.9314 0.710584 0.0110279 78.0385 1 10.875 10.875 0 8.78824 F T 1.12157 1.04995e-11 1 dbx
Report srcpi bgdpi arf 2 X130250.55-635055.9 xmm mos1 302.889 315.227 1036.38 195.662 0.0932645 0.0176077 15.3582 1 10.875 10.875 0 1.25935 T T 1.0051 8.59323e-13 1 dbcx

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