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 1 X151321.96+571356.4 xmm mos2 143.608 358.034 34.0363 8.49845 0.0124501 0.00310864 5.50785 1 9.70397 5.41413 90 12.0438 F F 0.86473 3.14526e-13 1 dsx
Report srcpi bgdpi arf 1 X151321.75+571401.1 xmm mos1 144.006 359.097 38.4544 11.597 0.0118569 0.00357578 3.92401 0.999898 9.48291 5.63098 118.985 12.0414 F F 0.864761 2.59771e-13 1 dsx
Report srcpi bgdpi arf 1 X151320.27+570038.8 xmm pn 145.84 174.599 55.6329 10.1385 0.00940937 0.00171476 13.5904 1 10.875 10.875 0 14.248 F F 0.995217 6.96036e-14 1 dx
Report srcpi bgdpi arf 5 X151209.83+570748.6 xmm pn 278.171 273.077 8.6071 5.37935 0.0110712 0.00691936 2.10261 0.978288 6.06821 6.06821 0 2.31774 F F 1.05738 3.04964e-14 1 dsx
Report srcpi bgdpi arf 6 X151253.56+565839.3 xmm pn 195.899 146.982 13.5151 5.1671 0.0173843 0.00664635 3.30157 0.998835 4.3951 4.3951 0 13.2258 F F 1.06385 1.35099e-13 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