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 1 X144707.09+114744.7 chandra ccd7 676.5 664.5 4.98239 2.23607 0.00487575 0.00218821 11.1186 1 0.492 0.492 45 1.67835 F F 1.65e+20 0 1 d
Report 2 X144657.82+114637.7 chandra ccd7 953.167 528.5 2.97869 1.73205 0.00291493 0.00169498 6.6472 0.999942 0.492 0.492 161.565 3.97723 F F 1.66e+20 0 1 d
Report 3 X144711.99+115039.3 chandra ccd7 530.167 1019.5 2.97489 1.73205 0.00291122 0.00169498 6.63873 0.999942 0.492 0.492 2.7791e-08 1.47395 F F 1.65e+20 0 1 d
Report 4 X144709.59+114715.6 chandra ccd7 602.51 605.873 14.8082 3.84814 0.0144912 0.00376577 33.0458 1 0.493545 0.493545 0 2.00842 F F 1.65e+20 0 1 ds

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