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 arf 2 X112802.97+785953.4 chandra ccd7 393.885 792.221 295.385 17.5317 0.0288209 0.00171058 144.532 1 0.385361 0.332078 76.6547 0.0802596 F F 3.43e+20 1.55754e-13 1 dsx
Report arf 1 X112649.07+790557.1 chandra ccd6 437.542 575.083 22.3047 4.899 0.0021763 0.000478002 4.35975 0.999957 1.94496 1.15224 137.461 6.97817 A F 3.49e+20 2.07276e-14 1 dx
Report arf 2 X112627.24+790825.5 chandra ccd6 561.845 877.976 56.4055 9.08732 0.00550357 0.000886663 11.0252 1 4.6209 1.82729 76.4185 9.65206 F F 3.52e+20 5.58682e-14 1 dsx
Report arf 1 X112729.12+790058.7 chandra ccd7 590.542 925.171 16.9081 4.11195 0.00164973 0.000401205 8.27315 1 0.45115 0.45115 0 1.88777 F F 3.43e+20 1.1e-14 1 dsx
Report arf 3 X112807.15+785926.0 chandra ccd7 369.514 736.538 11.3611 3.452 0.0011085 0.000336812 5.559 0.999992 0.13081 0.13081 0 0.520219 F F 3.42e+20 6.01586e-15 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 - 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