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 2 X115017.46+251819.0 xmm mos2 304.796 320.627 113.043 15.1816 0.0156129 0.00209681 11.3548 1 4.40555 4.40555 0 1.68029 F F 6.17401 0 1 ds
Report srcpi bgdpi 1 X115017.33+251819.4 xmm mos1 305.193 320.717 12.4486 6.77977 0.0136534 0.00743595 2.15025 0.976667 3.52759 3.52759 0 1.66603 F F 6.1737 0 1 ds
Report srcpi bgdpi 1 X115027.77+252111.0 xmm mos2 272.66 360.109 124.099 14.7946 0.013081 0.00155947 12.4653 1 10.875 10.875 0 4.84607 F F 6.22147 0 1 d
Report srcpi bgdpi 5 X114930.87+251431.9 xmm mos2 450.1 268.843 78.8756 12.499 0.0129 0.00204419 7.92277 1 10.875 10.875 0 11.203 F F 5.99 0 1 d
Report srcpi bgdpi 4 X114934.86+252001.9 xmm mos2 437.565 344.396 64.008 11.7878 0.00975688 0.00179684 6.42938 1 10.875 10.875 0 10.6229 F F 6.02213 0 1 d
Report srcpi bgdpi 3 X115055.73+252703.3 xmm mos2 185.625 441.206 31.1418 10.5797 0.00430115 0.00146121 3.12808 0.99874 4.67691 4.67691 0 13.1888 F F 6.34307 0 1 ds

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