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 X135037.37-063215.3 chandra ccd7 534.685 830.886 223.898 15.1 0.14492 0.0097736 110.428 1 0.440141 0.440141 0 0.573632 F F 1.97e+20 0 1 ds
Report 1 X135104.87-062000.0 chandra ccd5 277.722 317.784 50.7198 9.00028 0.0328286 0.00582548 88.9298 1 7.9485 5.03224 3.74281 13.4581 A F 1.96e+20 0 1 d
Report 1 X135049.03-063140.5 chandra ccd7 180.8 901.1 9.94134 3.16228 0.00643458 0.0020468 4.90313 0.999973 0.492 0.492 16.7083 2.64287 F F 1.98e+20 0 1 d
Report 1 X135112.52-063021.0 chandra ccd2 998.278 595.611 8.45639 3.00001 0.00547344 0.00194177 28.4348 1 2.15121 0.988299 155.241 8.58987 A F 1.98e+20 0 1 d
Report 2 X135111.19-063750.5 chandra ccd3 808.7 700.9 4.64736 2.23608 0.00300803 0.00144731 15.9816 1 2.17488 1.12294 29.5027 10.177 A F 2e+20 0 1 d
Report 1 X135105.64-063526.8 chandra ccd3 976.833 993.167 2.88637 1.73205 0.00186822 0.00112108 9.92584 0.999905 1.19172 0.492 50.5351 7.71434 A F 1.99e+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