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 arf rmf 1 X074232.81+494834.3 xmm pn 291.123 276.785 17186.4 145.411 7.17881 0.0607387 273.178 1 5.88502 5.74834 302.341 1.64953 13767 4082 -0.542607 0.00857989 F F 5.27e+20 2.09127e-11 1 dsx
Report srcpi bgdpi arf rmf 1 X074232.80+494834.6 xmm mos2 291.146 276.861 4089.77 73.4895 2.20354 0.0395957 112.956 1 6.61347 6.1426 353.557 1.64932 3318.5 1327.17 -0.428642 0.0162162 F F 5.27e+20 2.45522e-11 1 dsx
Report srcpi bgdpi arf rmf 3 X074232.79+494834.4 xmm mos1 291.161 276.797 4172.58 72.8071 2.22299 0.0387888 174.758 1 6.80396 6.47172 343.763 1.64819 3418.73 1339.61 -0.436942 0.016069 F F 5.27e+20 2.19857e-11 1 dsx

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