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 2 X090423.35+130921.0 chandra ccd7 526.013 892.95 25.9555 5.09465 0.0168664 0.0033106 58.714 1 0.716125 0.408512 103.559 0.165729 22 1.85503 -0.844475 0.329206 F F 2.83e+20 1.26225e-13 1 dsx
Report 1 X090421.31+130545.1 chandra ccd7 586.357 453.643 6.91219 2.64575 0.00449157 0.00171922 15.6361 1 0.540161 0.492 45 3.7558 F F 2.78e+20 0 1 d
Report srcpi bgdpi arf 1 X090414.67+131238.3 chandra ccd6 1092.25 337.5 3.91531 3.17945 0.00254418 0.00206602 13.4537 1 0.492 0.492 90 3.74408 2 1.91531 -0.0216313 0.82671 F F 2.92e+20 2.88064e-14 1 dx
Report srcpi bgdpi arf 2 X090445.34+131626.5 chandra ccd6 182.563 801.964 26.5559 5.15769 0.0172565 0.00335156 92.7244 1 3.36165 3.36165 0 8.84088 18.746 8.15326 -0.393792 0.255115 F F 3e+20 2.19352e-13 1 dsx
Report srcpi bgdpi arf 3 X090415.56+131253.1 chandra ccd6 1066.32 368.101 25.6076 5.0604 0.0166403 0.00328834 89.4133 1 1.35572 0.66331 67.0075 3.84881 26 -0.041896 -1 0.337026 F F 2.92e+20 1.87619e-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 - 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