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 X193015.74+493209.3 chandra ccd7 521.018 647.49 3537.86 60.8997 0.14934 0.0025707 277.707 1 0.366918 0.347246 75.8186 0.465046 3057.15 236.715 -0.856269 0.0233599 F T 6.58e+20 6.54751e-13 1 dsxf
Report srcpi bgdpi arf rmf 6 X193018.22+493133.5 chandra ccd7 471.763 574.821 2800.53 54.3526 0.118216 0.00229433 219.83 1 0.358759 0.358759 0 1.16284 2487.91 143.576 -0.890878 0.026649 F F 6.58e+20 8.94601e-13 1 dsx
Report srcpi bgdpi arf 1 X193117.36+493535.7 chandra ccd3 550.682 305.864 21.2861 5.97494 0.000898526 0.000252214 12.921 1 2.40145 1.32712 146.37 10.8594 12.6257 8.754 -0.181091 0.285205 A T 6.83e+20 1.21748e-14 1 dx
Report srcpi bgdpi arf 1 X193032.53+494042.6 chandra ccd2 808.322 95.4644 27.1872 6.63471 0.00114762 0.000280064 13.9233 1 3.9919 2.1921 22.4867 8.8639 12.3025 15.1171 0.102649 0.244052 A T 6.85e+20 1.58763e-14 1 dx

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