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 2 X093844.46+005715.6 chandra ccd7 574.335 870.538 123.902 11.7065 0.0889254 0.00840187 48.1716 1 0.474175 0.474175 0 0.597663 F F 4.36e+20 0 1 ds
Report 1 X093845.60+005926.6 chandra ccd7 539.508 1136.9 17.0025 4.13436 0.0122028 0.00296727 6.61037 1 0.364104 0.364104 0 1.72855 F F 4.37e+20 0 1 ds
Report 1 X093901.40+010533.0 chandra ccd6 591.611 992.056 8.45272 3.00001 0.00606656 0.00215312 29.0212 1 2.00445 1.38909 160.965 8.72619 F F 4.44e+20 0 1 d
Report 1 X093924.61+005118.8 chandra ccd3 358 1018 1.91373 1.41422 0.00137349 0.00101499 7.09457 0.997478 2.03787 0.492 95.1944 11.5829 A F 4.61e+20 0 1 d
Report 2 X093905.51+005147.0 chandra ccd3 940.3 1075.3 4.91313 2.23607 0.00352618 0.00160484 18.2139 1 0.885112 0.492 49.8099 7.68095 A F 4.49e+20 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