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 2 X142732.68+343040.5 chandra ccd1 566.491 769.757 49.1693 9.09947 0.0104291 0.00193005 8.47859 1 1.53402 0.887564 18.3019 7.40629 F F 1.16e+20 1.28915e-13 1 dsx
Report 3 X142645.11+342724.4 chandra ccd2 299.71 527.573 13.5083 3.67536 0.00286519 0.000779566 32.2515 1 0.731965 0.492845 341.602 2.979 F F 1.17e+20 0 1 ds
Report srcpi bgdpi arf 4 X142702.92+342654.6 chandra ccd3 661.884 1102.94 11.6345 3.41094 0.00246774 0.000723478 26.7866 1 0.391858 0.391858 0 2.12005 F F 1.16e+20 2.723e-14 1 dsx
Report 1 X142644.85+343021.1 chandra ccd2 306.067 886.677 10.2767 3.20573 0.00217975 0.000679954 24.5359 1 0.889231 0.485739 124.595 3.13146 F F 1.18e+20 0 1 ds
Report srcpi bgdpi arf 3 X142708.92+342123.6 chandra ccd3 510.167 429.611 8.67584 3.00001 0.00184017 0.000636311 19.9747 1 1.08643 0.561928 72.5679 7.71404 A F 1.13e+20 2.38404e-14 1 dx
Report 1 X142705.09+343353.2 chandra ccd0 426.167 498.333 5.96941 2.44949 0.00126613 0.000519545 13.7285 1 0.57389 0.492 111.187 5.32542 F F 1.18e+20 0 1 d
Report 2 X142652.06+343252.6 chandra ccd0 753.3 375.1 4.94789 2.23607 0.00104946 0.000474278 11.3792 1 0.543911 0.492 6.04738 4.28519 F F 1.18e+20 0 1 d
Report srcpi bgdpi arf 3 X142657.05+343143.7 chandra ccd0 628.1 235.1 4.94163 2.23607 0.00104814 0.000474278 11.3648 1 0.505304 0.492 8.34962 2.96707 F F 1.18e+20 1.1735e-14 1 dx
Report 1 X142652.67+342300.9 chandra ccd3 919.25 627.5 3.93792 2 0.000835246 0.000424207 9.06643 0.999998 0.755099 0.492 180 5.85516 A F 1.14e+20 0 1 d
Report 2 X142656.58+342443.0 chandra ccd3 820.833 834.833 2.98066 1.73205 0.000632209 0.000367374 6.8625 0.999955 0.492 0.492 19.9028 4.06222 F F 1.15e+20 0 1 d
Report 5 X142706.39+342519.3 chandra ccd3 574.167 908.833 2.97784 1.73205 0.00063161 0.000367374 6.856 0.999955 0.492 0.492 90 3.85848 F F 1.15e+20 0 1 d
Report 2 X142638.38+342948.7 chandra ccd2 468.167 820.5 2.94197 1.73205 0.000624002 0.000367374 7.02405 0.999966 0.602575 0.492 90 4.16899 F F 1.18e+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