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 1 X193840.10+303028.0 chandra ccd7 178.403 673.83 3826.58 63.5482 0.16918 0.00280957 497.834 1 1.5 0.851157 105.706 4.74375 A T 3.87e+21 0 1 ds
Report 2 X193832.77+302830.1 chandra ccd7 371.056 434.177 64.9569 8.32594 0.00287186 0.000368104 8.45083 1 0.548165 0.548165 0 2.22197 F F 3.87e+21 0 1 ds
Report 3 X193831.13+302713.6 chandra ccd7 413.963 278.589 21.0544 5.54275 0.000930853 0.000245055 2.73916 0.996093 0.32986 0.32986 0 1.11507 F F 3.89e+21 0 1 ds
Report 5 X193826.68+302657.4 chandra ccd7 531.004 245.679 38.8826 7.02764 0.00171907 0.000310704 5.05859 0.999998 0.332019 0.332019 0 0.219331 F F 3.87e+21 0 1 ds

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