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 3 X170441.37+604430.7 chandra ccd7 743.708 143.842 2546.33 51.4971 0.278359 0.00562955 324.407 1 0.410135 0.384702 53.399 0.612542 F F 2.02e+20 2.39741e-12 1 dsxf
Report srcpi bgdpi arf rmf 1 X170355.78+604511.7 chandra ccd6 372.835 121.996 234.525 15.9092 0.0256393 0.00173927 54.4117 1 1.78197 1.05111 323.329 5.00865 F F 2e+20 2.19234e-13 1 dsxf
Report srcpi bgdpi arf 1 X170443.80+604448.5 chandra ccd7 707.6 180.066 80.6094 9.90979 0.00881206 0.00108332 10.2698 1 0.428626 0.428626 0 0.893996 F F 2.02e+20 4.86258e-14 1 dspx
Report srcpi bgdpi arf 2 X170443.49+604452.8 chandra ccd7 711.707 188.328 55.5446 7.6158 0.006072 0.000832541 7.07648 1 0.580741 0.539826 34.1181 0.870179 T F 2.02e+20 3.34318e-14 1 dpx

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