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 X123049.20+122329.0 chandra ccd7 449.703 232.213 819.147 43.842 0.174173 0.00932202 29.6593 1 1.36683 1.36683 0 0.28472 T F 1.94e+20 1.10899e-12 1 dscbxf
Report srcpi bgdpi arf rmf 2 X123049.03+122329.9 chandra ccd7 454.713 234.077 252.85 32.0182 0.053763 0.00680796 9.15509 1 1.16491 1.16491 0 0.303592 T F 1.94e+20 3.98227e-13 1 dscx
Report srcpi bgdpi arf rmf 3 X123048.64+122332.6 chandra ccd7 466.537 239.392 917.004 40.6011 0.194981 0.00863293 33.2025 1 0.517208 0.517208 0 0.346197 F F 1.93e+20 1.44282e-12 1 dsx
Report srcpi bgdpi arf 4 X123048.23+122335.1 chandra ccd7 478.484 244.553 55.7253 25.1121 0.0118488 0.00533953 2.01768 0.977223 0.556589 0.556589 0 0.420889 F F 1.93e+20 8.76437e-14 1 dsx
Report srcpi bgdpi arf rmf 8 X123049.41+122328.3 chandra ccd7 443.466 230.76 3191.63 61.8379 0.67863 0.0131485 115.561 1 0.645505 0.418348 332.124 0.269442 T F 1.94e+20 5.02374e-12 1 dscx

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