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 X123048.99+122329.3 chandra ccd7 75.6966 813.215 430.233 38.7816 0.0915502 0.00825242 16.2623 1 1.5 1.5 0 0.274502 T F 1.94e+20 5.96398e-13 1 dbsxf
Report srcpi bgdpi arf rmf 2 X123048.63+122332.5 chandra ccd7 86.5429 819.669 979.275 41.2713 0.208382 0.0087822 37.0154 1 0.672884 0.430058 161.377 0.220359 F F 1.93e+20 1.54039e-12 1 dsx
Report srcpi bgdpi arf 3 X123048.23+122335.1 chandra ccd7 98.3265 824.848 82.5173 25.9325 0.017559 0.00551824 3.11905 0.998927 0.770926 0.770926 0 0.17107 F F 1.93e+20 1.29967e-13 1 dsx
Report srcpi bgdpi arf rmf 8 X123049.38+122328.5 chandra ccd7 64.07 811.45 3684.14 67.6114 0.783955 0.0143872 139.256 1 0.913516 0.414203 338.765 0.373645 A F 1.94e+20 5.78403e-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