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 1 X142439.27+054920.1 chandra ccd3 446.779 550.307 28.1484 5.30551 0.00936829 0.00176577 64.4925 1 1.39821 1.39821 0 7.18245 F F 2.21e+20 1.25616e-13 1 dsx
Report 7 X142411.13+054911.1 chandra ccd3 1300.23 531.997 21.2476 4.63148 0.00707157 0.00154144 48.6816 1 0.402624 0.402624 0 0.221417 F F 2.21e+20 0 1 ds
Report 3 X142412.26+055014.5 chandra ccd3 1266.15 660.76 15.4585 3.93173 0.00514485 0.00130855 35.4179 1 0.336406 0.336406 0 1.27432 F F 2.21e+20 0 1 ds
Report srcpi bgdpi arf 5 X142401.65+055130.5 chandra ccd1 702.858 269.384 10.2487 3.20136 0.00341095 0.00106547 24.8508 1 0.598551 0.598551 0 3.28913 F F 2.21e+20 3.88071e-14 1 dsx
Report srcpi bgdpi arf 1 X142328.44+054650.8 chandra ccd0 1177.68 571.591 10.2365 3.31664 0.00340688 0.00110383 24.4376 1 2.49296 1.27081 142.066 10.6736 A F 2.19e+20 4.94175e-14 1 dx
Report srcpi bgdpi arf 5 X142428.66+054741.2 chandra ccd3 767.928 348.786 6.93201 2.64575 0.00230708 0.000880548 15.8823 1 0.680013 0.492 42.072 4.73556 F F 2.21e+20 2.82734e-14 1 dx
Report srcpi bgdpi arf 2 X142340.90+054515.6 chandra ccd0 799.667 378 5.82791 2.44949 0.00193962 0.00081523 13.9129 1 1.17551 0.87116 147.193 8.26397 F F 2.19e+20 2.5541e-14 1 dx
Report 3 X142354.02+055008.7 chandra ccd0 401.643 973.643 6.95249 2.64575 0.0023139 0.000880548 16.5976 1 0.554173 0.492 156.513 4.22526 F F 2.2e+20 0 1 d
Report srcpi bgdpi arf 1 X142412.01+054031.7 chandra ccd2 712 282.833 5.28236 2.44951 0.00175805 0.000815234 12.4361 1 2.72784 1.28654 161.981 8.53025 A F 2.2e+20 2.37589e-14 1 dx
Report 2 X142422.19+054932.3 chandra ccd3 964.3 574.5 4.97678 2.23607 0.00165635 0.000744199 11.4026 1 0.492 0.492 3.28463e-08 2.96535 F F 2.21e+20 0 1 d
Report 6 X142434.33+055301.8 chandra ccd3 596.25 1000.5 3.98893 2 0.00132758 0.000665632 9.13927 0.999998 0.795693 0.492 66.5762 7.15317 A F 2.21e+20 0 1 d
Report 1 X142418.79+055422.0 chandra ccd1 182.5 617.5 3.98005 2 0.00132462 0.000665632 9.65073 0.999999 0.492 0.492 45 5.70955 F F 2.21e+20 0 1 d
Report 2 X142404.06+055517.9 chandra ccd1 629.25 731 3.88902 2 0.00129433 0.000665633 9.43 0.999999 0.492 0.492 127.982 6.44621 F F 2.21e+20 0 1 d
Report srcpi bgdpi arf 2 X142433.30+054431.7 chandra ccd2 66.25 770.75 3.87138 2 0.00128846 0.000665633 9.11427 0.999999 0.492 0.492 45 7.26599 F F 2.21e+20 1.71431e-14 1 dx
Report 4 X142421.24+055113.6 chandra ccd3 993.167 780.5 2.98514 1.73205 0.000993502 0.000576454 6.83943 0.999953 0.492 0.492 3.11242e-08 3.45924 F F 2.21e+20 0 1 d
Report srcpi bgdpi arf 3 X142400.07+055219.4 chandra ccd1 750.167 368.167 2.97636 1.73205 0.000990579 0.000576454 7.217 0.99997 0.492 0.492 16.845 4.16536 F F 2.21e+20 1.15202e-14 1 dx
Report 4 X142410.32+055358.3 chandra ccd1 439.5 569.167 2.97185 1.73205 0.000989077 0.000576454 7.20606 0.99997 0.492 0.492 28.155 4.92145 F F 2.21e+20 0 1 d
Report 3 X142403.13+054318.8 chandra ccd2 981.5 622.5 2.92646 1.73205 0.000973974 0.000576455 6.88968 0.999962 0.492 0.492 90 6.0166 F F 2.2e+20 0 1 d
Report 4 X142351.46+054906.7 chandra ccd0 479.5 847.5 1.96034 1.41422 0.000652431 0.000470673 4.6799 0.99921 0.492 0.492 90 4.7195 F F 2.2e+20 0 1 d
Report 5 X142330.83+054938.1 chandra ccd0 1105.25 911.5 3.95992 2 0.00131792 0.000665632 9.4535 0.999999 0.492 0.492 180 9.86768 F F 2.19e+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