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 X180950.99-194352.6 xmm pn 284.986 278.01 1248.3 40.196 0.33156 0.0106764 81.7936 1 5.61746 5.61746 0 1.77122 F T 0.158481 6.13688e-13 1 dsxf
Report srcpi bgdpi arf rmf 3 X180950.99-194352.2 xmm mos2 284.998 278.089 1026.86 37.4312 0.107516 0.00391919 53.0812 1 5.63721 4.80574 10.8541 1.77098 F T 0.158435 7.06622e-13 1 dsxf
Report srcpi bgdpi arf rmf 1 X180950.99-194351.9 xmm mos1 285.015 278.158 1000.93 37.5203 0.105571 0.00395737 49.624 1 6.03379 4.81168 34.4989 1.76893 F T 0.15839 6.62734e-13 1 dsxf
Report srcpi bgdpi arf rmf 2 X180939.99-194103.9 xmm pn 320.725 316.769 109.306 14.4125 0.0290326 0.00382808 7.16216 1 5.92518 5.92518 0 2.10721 F F 0.097918 1.03274e-13 1 dbsx
Report srcpi bgdpi arf 4 X181009.66-194828.3 xmm pn 224.42 214.486 94.0247 15.409 0.0183297 0.00300392 6.16087 1 10.875 10.875 0 8.11428 F F 0.259612 6.9605e-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