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 rmf 1 X144557.63-445203.2 chandra ccd7 223.712 306.08 1731.27 42.411 0.274926 0.00673488 316.13 1 0.416521 0.381747 15.9926 0.592088 F F 9.53e+20 8.13042e-13 1 dsxf
Report srcpi bgdpi arf rmf 4 X144556.19-445234.7 chandra ccd7 254.761 241.938 365.339 19.693 0.0580158 0.00312725 66.7109 1 0.428808 0.372833 164.952 0.383111 F F 9.53e+20 3.56091e-13 1 dsx
Report srcpi bgdpi arf 2 X144554.67-445121.8 chandra ccd7 287.654 390.223 13.3712 3.66666 0.00212336 0.000582269 2.44158 0.990308 0.468851 0.468851 0 1.42501 F F 9.53e+20 1.31893e-14 1 dsx
Report srcpi bgdpi arf 1 X144614.90-445721.6 chandra ccd6 237.5 621.167 2.58347 1.73207 0.000410313 0.000275091 2.9517 0.992162 1.31251 0.492 67.8626 5.56479 A F 9.52e+20 3.82574e-15 1 dx
Report srcpi bgdpi arf 2 X144606.63-445528.2 chandra ccd6 415.9 851.7 4.85311 2.23607 0.000770782 0.000355138 5.54484 0.999854 0.632037 0.492 49.9329 3.19695 F F 9.53e+20 6.9087e-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