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 X122906.71+020308.2 xmm pn 304.906 320.806 591093 785.298 23.3261 0.0309899 5771.57 1 7.07008 7.07008 0 1.69686 F F 4.36006 0 1 ds
Report srcpi bgdpi 2 X122906.71+020307.8 xmm mos1 304.911 320.711 209806 485.187 7.56178 0.017487 2259.47 1 6.36044 6.36044 0 1.69455 F F 4.35977 0 1 ds
Report srcpi bgdpi 2 X122903.52+020110.0 xmm pn 315.887 294.062 722.308 42.6295 0.0428154 0.0025269 7.05279 1 10.875 10.875 0 1.30432 T F 4.32506 0 1 dcb
Report srcpi bgdpi 3 X122902.60+020050.6 xmm pn 319.067 289.175 1502.74 78.1835 0.059302 0.00308532 14.6731 1 14.1615 14.1615 0 1.79418 T F 4.31396 0 1 dsc
Report srcpi bgdpi 4 X122901.76+020004.6 xmm pn 321.958 278.608 904.963 46.4893 0.0357122 0.00183459 8.83628 1 9.17688 9.17688 0 2.2463 F F 4.30564 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