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 X123049.02+122329.8 chandra ccd7 457.883 297.948 325.332 37.1606 0.067938 0.00776014 11.3737 1 1.21449 1.21449 0 0.74116 T F 1.94e+20 0 1 dsp
Report 2 X123048.63+122332.4 chandra ccd7 469.358 303.234 1188.36 45.8766 0.248161 0.00958024 41.5452 1 0.498776 0.498776 0 0.723359 F F 1.93e+20 0 1 ds
Report 3 X123048.25+122335.1 chandra ccd7 480.782 308.765 83.6504 26.493 0.0174685 0.00553245 2.92443 0.997953 0.653259 0.653259 0 0.712484 F F 1.93e+20 0 1 ds
Report 6 X123049.86+122337.1 chandra ccd7 432.934 312.71 62.868 24.4488 0.0131285 0.00510557 2.19787 0.98579 0.875781 0.875781 0 0.978617 T F 1.94e+20 0 1 ds
Report 11 X123049.80+122402.2 chandra ccd7 434.667 363.675 66.7349 18.3194 0.013936 0.00382558 2.33306 0.989096 1.5 1.5 0 1.29484 T F 1.93e+20 0 1 ds
Report 12 X123049.39+122328.4 chandra ccd7 446.852 294.98 5063.71 81.111 1.05744 0.0169382 177.028 1 0.514313 0.514313 0 0.795472 F F 1.94e+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