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 X123049.02+122329.9 chandra ccd7 113.615 837.171 303.569 36.01 0.0645724 0.00765972 9.55036 1 1.5 0.647653 -0 0.130604 A T 1.94e+20 4.58563e-13 1 dscxf
Report srcpi bgdpi arf rmf 2 X123048.88+122330.8 chandra ccd7 117.347 838.506 139.868 15.1991 0.0297512 0.00323298 4.40028 0.999992 0.492 0.492 32.7845 0.147461 F F 1.94e+20 2.16019e-13 1 dpcx
Report srcpi bgdpi arf rmf 3 X123048.63+122332.4 chandra ccd7 125.328 842.122 1029.34 43.1755 0.218952 0.00918389 32.3833 1 0.504196 0.504196 0 0.200444 F F 1.93e+20 1.58881e-12 1 dsx
Report srcpi bgdpi arf 5 X123048.23+122334.8 chandra ccd7 137.01 847.093 71.3924 25.088 0.0151859 0.00533648 2.24602 0.986716 0.87527 0.377912 -0 0.293001 T F 1.93e+20 1.10355e-13 1 dsx
Report srcpi bgdpi arf rmf 11 X123049.37+122328.3 chandra ccd7 103.051 833.946 8352.56 100.04 1.77668 0.0212796 262.774 1 0.60304 0.418337 337.038 0.103456 F F 1.94e+20 1.2882e-11 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