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 X132031.74+293130.5 chandra ccd7 797 251.625 7.51203 2.82844 0.00163971 0.000617384 9.50456 1 1.45999 0.492 23.857 5.16086 A T 1.14e+20 0 1 d
Report 2 X132041.50+293013.8 chandra ccd7 537.928 95.9285 5.87587 2.64578 0.00128257 0.000577513 7.43441 0.999996 1.09391 0.762748 110.301 7.10864 F F 1.15e+20 0 1 d
Report 3 X132029.11+293921.2 chandra ccd7 867.303 1208.8 25.8313 5.08245 0.00563845 0.0011094 32.6829 1 0.99027 0.356503 68.4036 2.87383 A F 1.13e+20 0 1 ds
Report 4 X132032.28+293255.4 chandra ccd7 782.833 424.167 2.93357 1.73205 0.000640332 0.000378068 3.71169 0.99613 0.492 0.492 4.73116 3.83222 F F 1.13e+20 0 1 d
Report 5 X132036.99+293517.7 chandra ccd7 657.833 713.5 2.93417 1.73205 0.000640464 0.000378068 3.71245 0.99613 0.529672 0.492 79.722 2.61174 F F 1.13e+20 0 1 d
Report 6 X132053.41+293433.0 chandra ccd7 222.5 623 3.7007 2.00001 0.000807778 0.000436557 4.68229 0.999527 0.492 0.492 90 6.1936 F F 1.16e+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