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 rmf 1 X123049.04+122330.0 chandra ccd7 436.883 289.683 475.318 37.5261 0.101113 0.00798282 15.7384 1 1.46 1.46 0 0.747695 T F 1.94e+20 1.19483e-12 1 dscxf
Report srcpi bgdpi arf rmf 2 X123048.89+122331.1 chandra ccd7 440.729 291.289 173.641 16.6437 0.0369379 0.00354054 5.74949 1 0.492 0.492 13.0941 0.739683 F F 1.94e+20 2.59724e-13 1 dpcx
Report srcpi bgdpi arf rmf 3 X123048.63+122332.6 chandra ccd7 449.066 294.91 1004.84 44.5283 0.213756 0.00947235 33.2717 1 0.483917 0.483917 0 0.723941 F F 1.93e+20 1.50302e-12 1 dsx
Report srcpi bgdpi arf 4 X123048.24+122335.0 chandra ccd7 460.735 299.83 79.3153 28.4831 0.0168725 0.00605912 2.62624 0.995305 0.641828 0.641828 0 0.71446 F F 1.93e+20 1.18525e-13 1 dsx
Report srcpi bgdpi arf rmf 10 X123049.37+122328.6 chandra ccd7 426.892 286.75 7064.66 95.5756 1.50284 0.0203315 233.921 1 0.862401 0.59991 333.138 0.78788 T F 1.94e+20 1.05676e-11 1 dspx

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