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 X141730.55-440257.6 chandra ccd2 701.332 515.984 51.1508 7.15198 0.025257 0.00353148 124.129 1 1.52289 0.779266 54.6482 5.01841 F F 6.72e+20 3.98815e-13 1 dsx
Report srcpi bgdpi arf 1 X141717.71-440650.7 chandra ccd3 585.5 1007.5 4.97583 2.23607 0.00245693 0.00110411 12.333 1 0.492 0.492 80.7825 4.5715 F F 6.74e+20 3.07479e-14 1 dx
Report 3 X141737.58-440845.2 chandra ccd3 150.5 775.167 2.96579 1.73205 0.00146442 0.000855239 7.35093 0.999974 0.492 0.492 180 1.6135 F F 6.81e+20 0 1 d
Report 2 X141741.26-440831.2 chandra ccd3 70 803.5 1.97965 1.41421 0.000977497 0.000698299 4.90672 0.999363 0.492 0.492 180 1.10439 F F 6.81e+20 0 1 d
Report 1 X141832.24-440759.8 chandra ccd0 260.5 334 1.82678 1.41422 0.000902012 0.000698302 4.88722 0.991103 1.23766 0.492 26.5651 8.86075 A F 6.93e+20 0 1 d
Report 2 X141751.61-440629.2 chandra ccd0 1149.5 519.5 0.999999 1 0.000493771 0.000493772 2.67532 0.991103 0.492 0.492 90 1.8327 F F 6.81e+20 0 1 d
Report 3 X141758.98-440713.9 chandra ccd0 988.3 428.5 4.96112 2.23607 0.00244966 0.00110411 13.2726 1 0.504455 0.492 164.767 2.88457 F F 6.84e+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