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 X003552.33+595002.2 xmm pn 321.78 305.074 7938.6 107.305 2.32669 0.0314496 132.756 1 5.78483 5.78483 0 1.77262 F T 2.97854 0 1 ds
Report srcpi bgdpi 2 X003552.50+595002.6 xmm mos2 321.487 305.157 1023.76 37.449 1.07548 0.0393409 52.6101 1 5.04289 5.04289 0 1.75106 F T 2.97859 0 1 ds
Report srcpi bgdpi 1 X003552.48+595002.2 xmm mos1 321.512 305.065 987.972 39.0491 1.10254 0.0435774 42.6397 1 5.37897 5.37897 0 1.75021 F T 2.97872 0 1 ds
Report srcpi bgdpi 2 X003545.24+595004.0 xmm pn 334.059 303.656 168.543 22.7894 0.0280337 0.00379055 2.81852 0.997454 10.875 10.875 0 2.61022 F T 2.97726 0 1 dpb
Report srcpi bgdpi 3 X003558.99+595106.9 xmm pn 310.227 320.044 140.444 27.5718 0.0377641 0.00741378 2.34862 0.990345 10.875 10.875 0 1.78455 F T 2.96155 0 1 dbp

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