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 X215852.02-301332.3 xmm pn 317.6 311.211 458766 695.964 17.2365 0.0261484 3876.92 1 6.96284 6.96284 0 1.67422 F T 2.24583 3.646e-11 1 dsxf
Report srcpi bgdpi arf rmf 2 X215851.96-301333.0 xmm mos2 317.784 311.062 150173 416.296 5.60161 0.0155283 987.442 1 6.46937 6.39816 359.175 1.67157 F T 2.24587 5.67247e-11 1 dsxf
Report srcpi bgdpi arf rmf 1 X215852.01-301332.7 xmm mos1 317.61 311.128 142030 409.426 5.29904 0.0152754 887.688 1 6.13396 5.9043 25.1493 1.66919 F T 2.24593 4.74341e-11 1 dsxf
Report srcpi bgdpi arf rmf 2 X215854.84-301528.3 xmm pn 309.196 284.558 852.475 57.0761 0.0320288 0.00214444 7.20406 1 14.3961 14.3961 0 1.53892 T T 2.26315 1.03768e-13 1 dsx
Report srcpi bgdpi arf 3 X215856.68-301633.0 xmm pn 303.705 269.963 642.794 34.8879 0.038685 0.00209964 5.4321 1 10.875 10.875 0 2.0994 F T 2.26817 1.52269e-13 1 dpx
Report srcpi bgdpi arf 1 X215848.86-301355.6 xmm mos2 327.019 306.969 345.182 34.6755 0.017512 0.00175919 2.26969 0.988273 10.875 10.875 0 2.16255 F T 2.23542 2.5294e-13 1 dbx

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