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 X171518.87+214621.0 chandra ccd7 880.771 391.345 736.881 27.7333 0.0772178 0.00290617 203.751 1 0.415932 0.415932 0 0.773986 F F 4.71e+20 5.84577e-13 1 dsxf
Report srcpi bgdpi arf 2 X171535.71+214343.3 chandra ccd7 404.049 70.8058 15.7457 3.96809 0.00164999 0.000415816 4.35377 0.999901 0.79613 0.79613 0 4.06954 F F 4.76e+20 1.20661e-14 1 dsx
Report srcpi bgdpi arf 3 X171521.26+214531.8 chandra ccd7 813.152 291.28 84.027 9.54001 0.0088052 0.000999699 23.2339 1 0.414301 0.414301 0 0.260259 F F 4.73e+20 6.10423e-14 1 dsx
Report srcpi bgdpi arf 4 X171527.06+214716.7 chandra ccd7 648.625 504.125 7.77308 2.82843 0.00081454 0.000296391 2.1493 0.973553 0.492 0.492 71.565 2.27036 F F 4.68e+20 5.72695e-15 1 dx
Report srcpi bgdpi arf 8 X171516.13+214528.7 chandra ccd7 958.056 284.5 8.56802 3.00001 0.000897842 0.000314371 2.3691 0.985027 0.585484 0.492 69.2083 0.974465 T F 4.73e+20 6.24215e-15 1 dx

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 - 7.99 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), T = 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