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 X123049.03+122330.1 chandra ccd7 175.694 742.175 240.563 30.6287 0.0514164 0.00654638 9.45411 1 1.5 0.513811 340.331 0.287446 A F 1.94e+20 3.04865e-13 1 dscxf
Report srcpi bgdpi arf rmf 2 X123048.89+122331.2 chandra ccd7 179.486 744.007 121.998 14.7991 0.0260749 0.00316303 4.79452 0.999998 0.492 0.492 34.9939 0.270818 F F 1.94e+20 1.93671e-13 1 dbcx
Report srcpi bgdpi arf rmf 3 X123048.62+122332.5 chandra ccd7 187.836 747.213 916.61 40.8059 0.19591 0.0087216 36.0227 1 0.49997 0.49997 0 0.259715 F F 1.93e+20 1.45594e-12 1 dsx
Report srcpi bgdpi arf 5 X123048.22+122335.3 chandra ccd7 199.842 752.724 84.0688 23.9849 0.0179683 0.00512638 3.3039 0.999405 0.758181 0.758181 0 0.26323 F F 1.93e+20 1.33531e-13 1 dsx
Report srcpi bgdpi arf 8 X123049.73+122318.9 chandra ccd7 154.714 719.443 50.011 20.8014 0.0106891 0.00444597 1.96543 0.974309 0.959668 0.959668 0 0.515374 F F 1.94e+20 7.9281e-14 1 dbsx
Report srcpi bgdpi arf rmf 11 X123049.39+122328.3 chandra ccd7 165.025 738.653 3726.89 68.1488 0.796563 0.0145657 146.466 1 0.864505 0.399226 337.834 0.336121 A F 1.94e+20 5.90984e-12 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