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 X110421.39+382323.5 xmm mos1 313.096 425.628 58.6033 19.9031 0.00527238 0.00179063 3.18982 0.99913 22.1178 22.1178 0 9.26065 T F 4.96497 0 1 dsb
Report srcpi bgdpi 4 X110428.51+382254.3 xmm mos1 293.845 419.008 35.9832 8.24384 0.00323731 0.000741675 1.95859 0.973415 10.875 10.875 0 8.74778 F F 4.98026 0 1 dcb
Report srcpi bgdpi 5 X110426.39+382235.2 xmm mos1 299.561 414.403 36.7877 8.84 0.00330969 0.000795311 2.00238 0.97649 10.875 10.875 0 8.40797 F F 4.97542 0 1 dpc
Report srcpi bgdpi 7 X110427.83+382421.1 xmm mos1 295.688 438.795 32.6516 8.51538 0.00293758 0.000766105 1.77725 0.962091 10.875 10.875 0 10.1779 F F 4.97039 0 1 db

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