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 X095639.85+084447.8 chandra ccd7 74.1667 931.5 2.90206 1.73205 0.000603716 0.000360319 3.21526 0.990346 0.492 0.492 180 1.60591 F F 3.08e+20 0 1 d
Report 2 X095628.07+084139.8 chandra ccd7 429.1 549.3 4.88148 2.23607 0.00101549 0.00046517 5.4083 0.999797 0.492 0.492 43.4101 2.67231 F F 3.08e+20 0 1 d
Report 3 X095632.77+084336.6 chandra ccd7 287.5 786.75 3.88208 2 0.000807589 0.000416061 4.30104 0.998473 0.492 0.492 28.9973 0.693267 F F 3.08e+20 0 1 d
Report 4 X095628.37+084132.4 chandra ccd7 420.481 534.915 9.59053 3.09686 0.00199514 0.000644245 10.6256 1 0.717762 0.281681 106.236 2.7126 F F 3.08e+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