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 4 X152005.48+201605.5 chandra ccd7 550.253 734.632 265.31 16.5598 0.0271262 0.00169313 88.8457 1 0.418515 0.418515 0 0.284829 F F 4.16e+20 1.93528e-13 1 dsxf
Report srcpi bgdpi arf 1 X151956.78+202010.1 chandra ccd6 208.583 359.25 11.5384 3.46411 0.00117972 0.000354182 11.1712 1 0.912286 0.49756 75.8057 4.34992 A F 4.15e+20 1.29368e-14 1 dx
Report srcpi bgdpi arf 2 X151954.18+201922.1 chandra ccd6 283.562 262.163 31.4009 5.60365 0.00321053 0.000572936 30.4016 1 1.47103 0.920051 77.1472 3.95666 F F 4.14e+20 3.80088e-14 1 dsx
Report srcpi bgdpi arf 3 X151957.68+201903.0 chandra ccd6 183 222.875 7.68382 2.82843 0.000785618 0.000289188 7.43928 0.999998 0.623298 0.492 23.4973 3.25425 F F 4.15e+20 8.24411e-15 1 dx
Report srcpi bgdpi arf 6 X151955.28+201833.8 chandra ccd6 251.389 163.611 8.69048 3.00001 0.000888542 0.00030673 8.41391 1 0.711949 0.492 98.9781 3.18197 F F 4.14e+20 9.31866e-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