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 3 X014737.23+272042.4 chandra ccd7 432.056 687.611 8.70577 3.00001 0.00505586 0.00174225 8.19459 1 0.492 0.492 74.1203 2.55201 F F 6.96e+20 0 1 d
Report 2 X014726.58+272046.9 chandra ccd7 720.5 696.833 5.68653 2.4495 0.00330244 0.00142254 5.35263 0.999826 0.625354 0.492 123.019 2.83762 F F 6.98e+20 0 1 d
Report 1 X014634.66+271018.9 chandra ccd2 1242.1 755.9 4.83046 2.23607 0.00280528 0.00129859 15.9781 1 1.61191 0.494747 135.663 15.2506 A F 7.22e+20 0 1 d
Report 1 X014715.46+272003.2 chandra ccd7 1021.83 608.167 2.8814 1.73205 0.00167337 0.00100589 2.71221 0.993961 0.492 0.492 16.845 4.26548 F F 7.01e+20 0 1 d
Report 1 X014743.85+271149.9 chandra ccd6 717.5 519.5 1.89068 1.41422 0.00109801 0.000821305 5.70129 0.999796 1.04369 0.492 45 6.92984 A F 7.06e+20 0 1 d

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