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 srcpi bgdpi arf rmf 1 X213126.19+471724.5 chandra ccd7 135.638 781.959 370.264 19.6758 0.0177752 0.000944572 93.3038 1 0.367691 0.3157 115.946 0.178333 356.199 9.78161 -0.946546 0.075936 F F 3.3e+21 7.28811e-14 1 dsxf
Report srcpi bgdpi arf 3 X213124.57+471712.4 chandra ccd7 169.114 757.48 64.5185 8.89607 0.00309732 0.000427071 16.2582 1 0.334786 0.334786 0 0.383962 46.9152 18.9152 -0.425336 0.151628 F F 3.3e+21 2.73557e-14 1 dsx
Report srcpi bgdpi arf 1 X213136.28+472206.0 chandra ccd6 323.75 397.75 3.66123 3.17945 0.000175769 0.00015264 6.29031 0.999972 0.492 0.492 123.019 4.89739 -0.169387 1.83061 1 2.11061 F F 3.32e+21 2.02618e-15 1 dx
Report srcpi bgdpi arf 2 X213133.65+472054.6 chandra ccd6 378.167 252.5 5.86119 3.59808 0.000281386 0.000172738 15.7318 1 0.600572 0.492 142.762 3.62588 3.9306 1.9306 -0.341228 0.657231 F F 3.32e+21 3.15299e-15 1 dx

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