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 1 X191019.27+163912.5 chandra ccd7 837.333 262.879 40.1993 6.34029 0.0276601 0.0043626 91.9675 1 0.854191 0.575355 31.4664 3.15954 F F 5.42e+21 2.74435e-13 1 dsx
Report srcpi bgdpi arf 1 X191056.25+163655.0 chandra ccd6 483.5 677 3.93603 2 0.00270823 0.00137612 15.4246 1 0.714565 0.492 123.69 7.15264 F F 5.76e+21 3.61474e-14 1 dx
Report 1 X190947.93+162715.5 chandra ccd0 512.5 1066.5 1.93524 1.41422 0.00133156 0.000973067 9.06559 0.998993 2.60922 0.492 171.87 16.9315 A F 5.3e+21 0 1 d
Report 1 X190943.24+163809.3 chandra ccd3 700.5 949.5 0.999803 1 0.000687925 0.00068806 4.02013 0.998164 0.492 0.492 90 11.6971 F F 5.13e+21 0 1 d

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