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 3 X111110.70+243602.1 chandra ccd7 829.1 654.5 4.95764 2.23607 0.0033829 0.00152581 11.3205 1 0.492 0.492 101.31 2.71621 F F 9.76e+19 0 1 d
Report 1 X111103.89+244228.5 chandra ccd6 907.7 396.9 4.80185 2.23607 0.0032766 0.00152581 16.0569 1 1.57571 0.492 70.1312 5.93692 A F 1.01e+20 0 1 d
Report 2 X111119.55+243128.3 chandra ccd7 583.9 98.1001 4.79707 2.23607 0.00327334 0.00152581 10.9539 0.999998 0.886092 0.492 126.805 6.3054 A F 9.52e+19 0 1 d
Report 1 X111120.56+243740.6 chandra ccd7 555.75 854.75 3.99236 2 0.00272424 0.00136472 9.11637 0.999998 0.492 0.492 45 0.187101 F F 9.85e+19 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