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 X222313.35-295955.7 chandra ccd1 768.411 969.178 15.1567 3.89316 0.00573383 0.0014728 32.4141 1 1.48017 1.48017 0 7.07022 F F 1.08e+20 7.5966e-14 1 dsx
Report srcpi bgdpi arf 5 X222326.80-295817.0 chandra ccd3 1068.48 364.096 7.94248 2.81826 0.00300467 0.00106616 16.5698 1 0.39983 0.39983 0 4.84369 F F 1.08e+20 5.4703e-14 1 dsx
Report srcpi bgdpi arf 4 X222328.91-300422.8 chandra ccd1 356.667 426.167 9.88582 3.16228 0.00373981 0.00119629 21.1418 1 0.492 0.492 50.3098 5.06543 F F 1.09e+20 4.99773e-14 1 dx
Report srcpi bgdpi arf 4 X222322.48-295404.0 chandra ccd3 1182.41 877.773 9.82944 3.31665 0.00371848 0.00125469 20.5064 1 2.78168 1.00737 172.123 8.45319 A F 1.09e+20 5.32168e-14 1 dx
Report 3 X222325.51-295855.4 chandra ccd1 446.929 1091.5 8.96154 3 0.00339015 0.0011349 19.1651 1 0.492 0.492 110.593 4.78518 F F 1.08e+20 0 1 d
Report srcpi bgdpi arf 1 X222402.54-300653.2 chandra ccd0 287.5 752.5 5.61682 2.4495 0.00212484 0.000926646 11.5511 1 1.12815 0.492 137.382 7.04271 A F 1.09e+20 2.91436e-14 1 dx
Report srcpi bgdpi arf 3 X222331.34-295457.6 chandra ccd3 948.1 768.9 4.91656 2.23607 0.00185994 0.000845905 10.2571 1 0.502686 0.492 5.65497 6.66823 F F 1.09e+20 2.50677e-14 1 dx
Report 2 X222334.36-300605.6 chandra ccd0 1030.75 849.25 3.97831 2 0.00150499 0.0007566 8.18145 0.999995 0.492 0.492 64.3299 5.78581 F F 1.09e+20 0 1 d
Report 2 X222323.68-295938.9 chandra ccd1 495.25 1003 3.9711 2 0.00150227 0.0007566 8.49259 0.999997 0.492 0.492 72.3912 4.92426 F F 1.08e+20 0 1 d
Report 2 X222334.92-295648.3 chandra ccd3 853.5 544 3.94729 2 0.00149326 0.000756601 8.23495 0.999996 0.546444 0.492 34.722 4.67865 F F 1.09e+20 0 1 d
Report 3 X222331.06-300608.1 chandra ccd0 1117.75 844.25 3.86551 2 0.00146232 0.000756602 7.94947 0.999995 0.492 0.492 159.407 6.15814 F F 1.09e+20 0 1 d
Report srcpi bgdpi arf 1 X222347.64-295603.5 chandra ccd3 517.5 635.167 2.97962 1.73205 0.00112719 0.000655235 6.21616 0.999903 0.492 0.492 90 4.8162 F F 1.09e+20 1.4887e-14 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