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 X142129.89+474722.3 xmm pn 287.734 317.52 27245.6 187.616 2.33686 0.0160918 305.492 1 5.86612 5.7684 89.3638 1.59833 F F 2.88641 6.84414e-12 1 dsxf
Report srcpi bgdpi arf rmf 2 X142129.84+474722.4 xmm mos2 287.844 317.543 9598.1 113.13 0.918723 0.0108287 236.42 1 5.58576 4.9503 304.802 1.59147 F T 2.8866 1.01064e-11 1 dsxf
Report srcpi bgdpi arf rmf 2 X142129.86+474722.9 xmm mos1 287.794 317.648 9459.32 111.13 0.885587 0.010404 175.944 1 5.41629 5.41629 0 1.60057 F T 2.88634 8.83712e-12 1 dsxf
Report srcpi bgdpi arf 1 X142229.72+473915.3 xmm mos1 148.733 205.916 521.034 27.8933 0.0406458 0.00217596 9.69124 1 10.875 10.875 0 12.759 F F 2.84979 1.24528e-12 1 dx
Report srcpi bgdpi arf rmf 1 X142229.61+473913.9 xmm mos2 148.998 205.495 305.675 20.0424 0.029259 0.00191844 7.52938 1 5.37882 5.37882 0 12.782 F F 2.84967 1.52237e-12 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