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 X123049.01+122330.1 chandra ccd7 545.707 236.083 290.244 35.1018 0.0616805 0.00745957 9.68374 1 1.5 0.360368 341.095 0.285095 A F 1.94e+20 3.65517e-13 1 dscxf
Report srcpi bgdpi arf rmf 2 X123048.93+122330.7 chandra ccd7 548.297 237.305 464.79 37.7054 0.0987738 0.00801287 15.5073 1 1.5 1.5 0 0.291697 T F 1.94e+20 7.25e-13 1 dscx
Report srcpi bgdpi arf rmf 3 X123048.63+122332.4 chandra ccd7 557.218 240.744 969.525 41.6181 0.206036 0.00884438 32.3474 1 0.50541 0.50541 0 0.329751 F F 1.93e+20 1.5123e-12 1 dsx
Report srcpi bgdpi arf rmf 4 X123048.22+122334.8 chandra ccd7 569.291 245.65 117.069 23.468 0.0248787 0.00498727 3.9059 0.999937 0.997771 0.997771 0 0.396985 T F 1.93e+20 1.82436e-13 1 dsx
Report srcpi bgdpi arf rmf 11 X123049.39+122328.3 chandra ccd7 534.647 232.418 6208.24 87.2062 1.31933 0.0185324 207.132 1 0.538599 0.538599 0 0.281232 F F 1.94e+20 9.68769e-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