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 X182929.41-092526.9 xmm pn 476.133 242.214 30.8515 7.73646 0.0521637 0.0130808 6.50194 1 15.8461 2.91027 90.1287 13.5656 A F 0.531566 5.49732e-13 1 dsx
Report srcpi bgdpi arf 2 X183041.53-092608.2 xmm pn 230.82 232.774 26.9096 6.55269 0.0454987 0.0110793 5.67119 1 9.2152 9.2152 0 6.84331 F F 0.263789 1.57511e-13 1 dsx
Report srcpi bgdpi arf 1 X182929.39-092531.6 xmm mos1 476.212 241.164 145.603 15.389 0.020144 0.00212906 20.4989 1 10.875 10.875 0 13.5411 F F 0.531262 8.61612e-13 1 dpx
Report srcpi bgdpi arf 1 X183041.39-092605.7 xmm mos2 231.295 233.349 31.2671 10.0717 0.0121322 0.003908 3.73255 0.999786 10.3259 4.62941 64.8366 6.81944 F F 0.264205 2.05997e-13 1 dsx
Report srcpi bgdpi arf 2 X183041.44-092606.3 xmm mos1 231.109 233.21 29.9472 8.96657 0.0122144 0.00365714 4.21616 0.999954 5.08546 5.08546 0 6.8388 F F 0.263669 1.85443e-13 1 dsx

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