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+303028.1 chandra ccd7 187.537 673.034 5639.82 76.4624 0.248489 0.00336891 755.859 1 1.30559 1.30559 0 4.74413 F T 3.87e+21 0 1 ds
Report 2 X193832.77+302830.1 chandra ccd7 380.106 433.009 63.5932 9.31322 0.0028019 0.000410338 8.52287 1 0.52848 0.52848 0 2.22023 F T 3.87e+21 0 1 ds
Report 3 X193831.13+302713.6 chandra ccd7 423.097 277.511 27.9164 6.00498 0.00122999 0.000264577 3.74141 0.999759 0.438666 0.364242 290.549 1.11333 F F 3.89e+21 0 1 ds
Report 4 X193838.77+302933.9 chandra ccd7 222.436 562.789 16.0509 6.57577 0.000707199 0.000289727 2.15117 0.979931 0.495014 0.495014 0 3.87478 F T 3.88e+21 0 1 ds
Report 6 X193826.70+302657.4 chandra ccd7 539.556 244.724 45.2032 7.64266 0.00199164 0.000336733 6.05821 1 0.478214 0.478214 0 0.220198 F T 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