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 2 X125851.46+235526.7 chandra ccd7 753.433 162.622 948.91 31.6586 0.0926792 0.00309206 204.964 1 0.398766 0.398766 0 0.62595 F F 1.39e+20 0 1 ds
Report 1 X125812.38+235626.3 chandra ccd6 796.409 220.269 85.0372 9.63999 0.00830465 0.000941432 30.2697 1 4.25973 2.45459 140.514 8.37814 F F 1.36e+20 0 1 ds
Report 1 X125857.00+235541.5 chandra ccd7 599.001 192.68 14.1412 4.51373 0.00138115 0.00044085 3.05449 0.997495 0.467824 0.467824 0 1.84663 F F 1.39e+20 0 1 ds
Report 4 X125854.61+235503.4 chandra ccd7 665.473 115.191 12.839 4.18961 0.00125397 0.000409196 2.77322 0.995652 0.294361 0.294361 0 1.44531 F F 1.39e+20 0 1 ds
Report 1 X125907.51+240314.7 chandra ccd3 216.564 126.021 11.0326 4.40005 0.00107754 0.000429748 3.82307 0.999583 2.09887 2.09887 0 8.66737 F F 1.33e+20 0 1 ds
Report 2 X125838.52+235539.5 chandra ccd6 67.5 124.125 7.79522 2.82843 0.00076127 0.00027622 2.77478 0.992697 0.648181 0.492 55.746 2.37395 F F 1.38e+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