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 X200751.31-110834.2 xmm mos2 281.901 281.289 1279 42.9495 0.198783 0.00667524 53.7766 1 4.9201 3.90478 77.9302 1.71783 F T 1.95729 2.32305e-12 1 dsxf
Report srcpi bgdpi arf rmf 1 X200751.30-110834.0 xmm mos1 281.921 281.335 1472.89 42.9394 0.224182 0.00653563 76.4783 1 5.72643 5.72643 0 1.73015 F T 1.95741 2.17335e-12 1 dsxf
Report srcpi bgdpi arf 1 X200744.15-111445.8 xmm pn 306.11 195.942 99.333 12.7051 0.0269998 0.00345337 3.01516 0.998515 10.875 10.875 0 7.4517 F T 1.97448 1.15029e-13 1 dbx
Report srcpi bgdpi arf rmf 2 X200751.30-110834.4 xmm pn 281.919 281.248 3884.77 70.499 0.70919 0.01287 117.919 1 5.83347 5.83347 0 1.73352 F T 1.9575 1.92705e-12 1 dsxf
Report srcpi bgdpi arf 4 X200803.29-105552.4 xmm pn 241.312 455.986 61.928 10.3774 0.00879033 0.00147301 1.87977 0.969551 10.875 10.875 0 12.15 F F 1.91258 5.94635e-14 1 dpx

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