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 X192804.24+735313.5 chandra ccd7 167.102 186.741 56.006 7.7241 0.00667335 0.000920359 6.60285 1 1.5955 1.5955 0 5.19414 F F 7.24e+20 0 1 ds
Report 2 X192748.52+735801.5 chandra ccd7 300.115 771.974 6972.73 85.44 0.83083 0.0101805 822.053 1 0.406067 0.406067 0 0.284122 F F 7.15e+20 0 1 ds
Report 3 X192744.54+735756.7 chandra ccd7 333.684 762.095 17.0799 5.81649 0.00203514 0.000693059 2.01364 0.977884 0.717668 0.717668 0 0.463846 F F 7.15e+20 0 1 ds
Report 4 X192744.58+735921.5 chandra ccd7 333.298 934.467 15.5662 4.55643 0.00185478 0.000542918 1.83518 0.963436 0.434802 0.434802 0 1.08977 F F 7.13e+20 0 1 ds
Report 6 X192800.20+735535.0 chandra ccd7 201.572 474.274 37.2964 6.64513 0.00444402 0.000791793 4.39708 0.999982 0.82234 0.295489 337.923 2.83625 A F 7.2e+20 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