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 X114916.82-291341.7 xmm mos1 295.103 351.229 280.094 23.7677 0.0191975 0.00162902 23.2069 1 10.875 10.875 0 3.83509 F F 1.71086 2.00136e-13 1 dx
Report srcpi bgdpi arf 1 X114924.60-292236.6 xmm mos2 271.734 228.535 62.0264 11.4346 0.0111247 0.00205084 6.15015 1 13.0004 13.0004 0 5.46572 F F 1.57638 1.71435e-13 1 dsx
Report srcpi bgdpi arf 2 X114832.53-292558.1 xmm mos2 428.122 182.115 17.9099 10.9843 0.00321221 0.00197009 1.77583 0.95833 7.68615 7.68615 0 12.6917 F F 1.46909 9.57724e-14 1 dsx
Report srcpi bgdpi arf 1 X114856.74-290716.4 xmm pn 355.571 440.061 34.7193 15.4678 0.0168039 0.00748635 2.5857 0.994688 23.9963 4.25269 61.3641 11.1392 A F 1.79551 9.50059e-14 1 dsx
Report srcpi bgdpi arf 2 X114905.89-290140.1 xmm pn 328.045 516.671 60.7448 11.1786 0.00436304 0.000802913 4.52394 0.999993 10.875 10.875 0 15.9669 F F 1.89205 4.6708e-14 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