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 X182615.07-145053.0 xmm pn 283.493 278.376 5970.03 95.9432 0.571446 0.00918359 104.963 1 5.52523 5.48797 28.8034 1.82249 F F 1.28947 3.65773e-12 1 dsxf
Report srcpi bgdpi arf rmf 2 X182615.06-145052.8 xmm mos2 283.551 278.423 2138.42 54.4664 0.28316 0.00721219 101.962 1 5.18181 4.89701 4.24234 1.81945 F T 1.28935 5.26206e-12 1 dbsxf
Report srcpi bgdpi arf rmf 2 X182615.08-145052.5 xmm mos1 283.47 278.479 2059.15 52.3163 0.28223 0.00717055 79.09 1 5.38296 5.38296 0 1.81979 F T 1.28936 4.72189e-12 1 dsxf
Report srcpi bgdpi arf 1 X182539.06-144504.8 xmm mos2 403.562 358.374 43.0444 9.72529 0.00569973 0.00128778 2.0524 0.977764 7.47271 7.47271 0 8.79653 F F 1.11568 1.34343e-13 1 dsx
Report srcpi bgdpi arf 1 X182538.76-144505.8 xmm mos1 404.577 357.768 52.9883 10.8637 0.00497018 0.00101899 2.03523 0.977424 10.875 10.875 0 8.81578 F F 1.11509 1.11084e-13 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