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 X100120.84+555349.6 chandra ccd7 274.99 229.904 391.367 20.4077 0.130858 0.00682356 81.6609 1 0.394662 0.394662 0 0.292069 F F 9.29e+19 9.70913e-13 1 dsxf
Report srcpi bgdpi arf rmf 1 X100120.69+555355.7 chandra ccd7 277.58 242.246 288.594 17.5904 0.0964946 0.00588155 60.2167 1 0.394412 0.394412 0 0.390868 F F 9.29e+19 7.18956e-13 1 dsx
Report srcpi bgdpi arf 2 X100132.95+555906.7 chandra ccd7 67.8333 873.944 8.78409 3 0.00293706 0.00100308 1.83285 0.957021 0.662731 0.492 51.845 5.7456 F F 9.37e+19 2.34887e-14 1 dx
Report srcpi bgdpi arf 1 X100119.70+554556.8 chandra ccd6 319 321.5 7.41506 2.82844 0.00247934 0.000945733 16.5499 1 1.03698 0.83352 50.1524 7.63646 F F 9.24e+19 2.97699e-14 1 dx
Report srcpi bgdpi arf 2 X100113.93+554955.8 chandra ccd6 417.75 807.25 3.91697 2 0.0013097 0.000668732 8.74243 0.999998 0.600805 0.492 140.944 3.81545 F F 9.27e+19 1.44566e-14 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