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 X004328.54+644535.1 xmm pn 321.45 305.433 341.308 25.6436 0.12403 0.0093188 19.1914 1 6.16727 5.07377 51.7104 1.76284 F F 1.90128 0 1 ds
Report srcpi bgdpi 1 X004328.40+644535.1 xmm mos1 321.657 305.435 442.841 28.7569 0.0464388 0.00301561 22.5952 1 5.32969 5.32969 0 1.7593 F F 1.9011 0 1 ds
Report srcpi bgdpi 2 X004328.49+644534.2 xmm mos2 321.518 305.223 490.112 28.9201 0.0484304 0.00285774 26.3388 1 5.69043 5.05104 51.9078 1.749 F T 1.90083 0 1 ds
Report srcpi bgdpi 2 X004425.13+644235.8 xmm pn 238.13 264.184 96.9588 17.3252 0.0135684 0.00242448 5.45189 1 10.875 10.875 0 5.02823 F T 1.8484 0 1 d
Report srcpi bgdpi 1 X004425.21+644237.4 xmm mos2 238.009 264.578 54.2626 11.7459 0.00638329 0.00138176 2.91609 0.997829 10.875 10.875 0 5.02186 F F 1.84885 0 1 dp

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