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 X123049.17+122329.0 chandra ccd7 83.7117 812.587 666.876 43.055 0.143122 0.00924029 22.3323 1 1.49 1.49 0 0.300656 T F 1.94e+20 1.00359e-12 1 dscxf
Report srcpi bgdpi arf rmf 2 X123049.00+122329.5 chandra ccd7 88.694 813.431 468.55 37.9156 0.100558 0.00813729 15.6908 1 1.5 1.5 0 0.270142 T F 1.94e+20 7.3743e-13 1 dscx
Report srcpi bgdpi arf rmf 3 X123048.63+122332.5 chandra ccd7 99.7533 819.586 998.856 42.8465 0.21437 0.00919554 33.4496 1 0.488329 0.488329 0 0.224328 F F 1.93e+20 1.57174e-12 1 dsx
Report srcpi bgdpi arf 4 X123048.23+122335.2 chandra ccd7 111.508 825.118 78.3598 26.9057 0.0168173 0.0057744 2.6241 0.995426 0.852899 0.852899 0 0.181964 F F 1.93e+20 1.23245e-13 1 dsx
Report srcpi bgdpi arf rmf 10 X123049.39+122328.3 chandra ccd7 76.8922 811.142 7276.71 89.9824 1.5617 0.0193116 243.682 1 0.708169 0.413397 334.54 0.371838 A F 1.94e+20 1.14524e-11 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