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 6 X110838.99-771604.0 chandra ccd3 59.7147 143.129 33.4781 6.36344 0.00803957 0.00152814 12.6398 1 0.369933 0.369933 0 0.479499 F F 7.52e+20 8.95674e-14 1 dsx
Report srcpi bgdpi arf 1 X110716.51-772305.8 chandra ccd1 696.912 324.265 14.8324 4.12314 0.00356189 0.000990141 25.1415 1 2.19209 1.72435 13.1441 8.75889 F F 7.55e+20 4.74579e-14 1 dx
Report srcpi bgdpi arf 2 X110759.98-771730.2 chandra ccd1 410.267 1008.43 23.4874 4.84963 0.00564037 0.00116461 39.8121 1 0.470926 0.470926 0 3.05187 F F 7.52e+20 6.48362e-14 1 dsx
Report srcpi bgdpi arf 5 X110631.39-770926.7 chandra ccd3 924.389 945.722 7.66559 3.00003 0.00184083 0.000720434 2.89417 0.994174 2.66556 1.34067 2.65307 9.89045 A F 7.47e+20 2.70789e-14 1 dx
Report srcpi bgdpi arf 3 X110702.56-771251.3 chandra ccd3 710.071 531.643 6.5935 2.64576 0.00158338 0.000635359 2.4894 0.986971 1.29105 0.667144 125.164 6.51656 A T 7.49e+20 2.18168e-14 1 dx
Report srcpi bgdpi arf 2 X110752.82-771623.4 chandra ccd3 369.333 102.5 5.86266 2.44949 0.00140787 0.000588227 2.21347 0.972596 0.663606 0.492 119.577 3.03117 F F 7.52e+20 1.60049e-14 1 dx
Report srcpi bgdpi arf 1 X111028.26-771658.4 chandra ccd0 452.833 967.5 2.91566 1.73205 0.000700174 0.00041594 5.14457 0.999657 0.492 0.492 61.845 5.67892 F F 7.54e+20 9.58967e-15 1 dx
Report 2 X110906.66-771704.0 chandra ccd0 1000.5 958.5 0.993236 1 0.000238518 0.000240143 1.75253 0.958237 0.492 0.492 90 1.6021 F F 7.53e+20 0 1 d
Report srcpi bgdpi arf 3 X111035.28-772205.6 chandra ccd0 410.5 342.833 5.04834 2.44952 0.00121232 0.000588233 8.9076 0.999999 1.96818 0.77747 119.7 8.59404 A T 7.57e+20 1.63674e-14 1 dx
Report 4 X111006.54-771955.2 chandra ccd0 600.643 609.214 6.93594 2.64575 0.00166561 0.000635358 12.2382 1 0.492 0.492 53.3496 5.94805 F T 7.55e+20 0 1 d
Report srcpi bgdpi arf 1 X110938.57-771040.0 chandra ccd2 700.5 704.5 0.957232 1 0.000229872 0.000240143 1.68988 0.958316 0.492 0.492 90 5.94323 F F 7.5e+20 3.00921e-15 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