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 9 X060426.86-352753.9 chandra ccd3 899.919 378.255 73.7701 8.92588 0.0156711 0.00189614 48.2543 1 2.17529 2.17529 0 8.09094 F F 3.95e+20 2.28947e-13 1 dsx
Report srcpi bgdpi arf 1 X060428.52-352454.9 chandra ccd3 858.994 742.124 20.8683 4.56818 0.00443307 0.000970424 13.6503 1 0.683634 0.683634 0 5.1605 F F 3.91e+20 5.69702e-14 1 dsx
Report srcpi bgdpi arf 1 X060512.12-351703.7 chandra ccd1 588.274 1090.17 23.8458 5.41339 0.0050623 0.00114923 11.7792 1 3.31865 2.365 20.316 7.58465 F F 3.88e+20 6.72297e-14 1 dsx
Report srcpi bgdpi arf 2 X060415.45-352611.1 chandra ccd3 1183.42 586.911 18.0361 4.37565 0.00383145 0.000929528 11.7977 1 2.07842 0.844688 13.4723 7.60716 F F 3.89e+20 5.46245e-14 1 dsx
Report srcpi bgdpi arf 7 X060506.41-352217.8 chandra ccd1 730.559 451.559 16.4248 4.12311 0.00348688 0.00087531 8.11345 1 1.00995 0.569777 3.93329 6.15945 A F 3.97e+20 4.49709e-14 1 dx
Report srcpi bgdpi arf 2 X060447.35-352005.7 chandra ccd1 1204.72 720.875 14.0251 3.74501 0.00297744 0.000795042 6.92805 1 0.907876 0.907876 0 1.88625 T F 3.88e+20 3.46665e-14 1 dsx
Report srcpi bgdpi arf 6 X060520.11-351709.1 chandra ccd1 389.266 1078.91 9.79394 4.07792 0.00207919 0.000865716 4.83796 0.999902 1.41183 1.41183 0 9.06412 F F 3.91e+20 3.08893e-14 1 dsx
Report srcpi bgdpi arf 4 X060521.31-352247.9 chandra ccd1 360.318 389.773 9.8202 3.31664 0.00208476 0.000704102 4.85093 0.999902 2.47628 1.26089 7.18682 9.19924 A F 4.02e+20 3.0436e-14 1 dx
Report srcpi bgdpi arf 3 X060448.88-352456.1 chandra ccd3 352.5 739.056 8.8265 3 0.00187501 0.00063729 5.77357 0.999993 0.852488 0.552628 2.05909 5.2743 A F 3.97e+20 2.3391e-14 1 dx
Report 1 X060430.52-352030.4 chandra ccd2 176.875 485.125 7.96215 2.82843 0.0016903 0.000600452 16.4102 1 0.492 0.492 72.3444 1.59189 F F 3.84e+20 0 1 d
Report srcpi bgdpi arf 2 X060419.57-352214.5 chandra ccd2 449.071 273.5 6.95101 2.64575 0.00147564 0.000561671 14.3263 1 0.492 0.492 55.4272 4.32645 F F 3.84e+20 1.86388e-14 1 dx
Report srcpi bgdpi arf 1 X060440.93-351312.0 chandra ccd0 791.928 740.357 6.71312 2.64576 0.00142516 0.000561682 13.4409 1 1.35674 0.622768 129.152 6.96387 A F 3.74e+20 1.93425e-14 1 dx
Report 6 X060425.28-352256.3 chandra ccd3 939.1 982.5 4.94441 2.23607 0.00105034 0.000475007 3.23423 0.99715 0.562527 0.492 132.145 3.83254 F F 3.87e+20 0 1 d
Report srcpi bgdpi arf 5 X060521.89-352054.2 chandra ccd1 345.3 620.9 4.64678 2.23608 0.000986481 0.000474705 2.29539 0.975568 1.5641 0.575556 75.8596 8.96062 A F 3.99e+20 1.42274e-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