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 1 X011012.81+600434.6 xmm pn 281.618 282.468 1471 42.8455 0.690742 0.0201191 104.841 1 5.76965 5.76965 0 1.69187 F T 2.71007 0 1 ds
Report srcpi bgdpi 1 X011012.75+600434.6 xmm mos2 281.713 282.463 1052.45 37.533 0.303795 0.0108341 55.7579 1 5.19865 5.19865 0 1.6875 F T 2.70991 0 1 ds
Report srcpi bgdpi 1 X011012.78+600435.1 xmm mos1 281.663 282.297 1523.95 46.4208 0.384619 0.0117158 0 10.875 10.875 0 1.68762 F T 2.70994 0 1 db
Report srcpi bgdpi 2 X011027.51+600039.8 xmm pn 256.242 228.524 26.7364 7.46532 0.0125547 0.00350551 1.90555 0.969219 4.42766 4.42766 0 5.92027 F F 2.77297 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