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 1 X025222.40+700252.6 xmm pn 218.392 334.956 879.993 41.3597 0.0350484 0.00164727 0 10.875 10.875 0 6.37871 U U 3.2e+21 d
Report 1 X025222.74+700252.3 xmm mos2 217.997 334.861 71.8526 10.7408 0.034204 0.00511294 0 10.875 10.875 0 6.40195 U U 3.2e+21 d
Report 2 X025305.03+700559.6 xmm pn 168.563 378.116 137.698 22.9973 0.00548425 0.000915936 0 10.875 10.875 0 11.0467 U U 3.2e+21 d
Report 3 X025202.24+700158.3 xmm pn 242.082 322.207 249.29 26.9416 0.018787 0.00203037 0 10.875 10.875 0 4.43432 U U 3.21e+21 d
Report 4 X025114.99+700945.6 xmm pn 297.721 430.228 70.5356 15.4292 0.00280929 0.000614513 0 21.75 21.75 0 9.55497 U U 3.23e+21 d
Report 5 X024901.78+700853.6 xmm pn 453.706 418.402 122.893 20.6287 0.00489457 0.0008216 0 10.875 10.875 0 14.2255 U U 3.24e+21 d

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