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 X032848.21-271735.8 chandra ccd7 902.667 870.833 5.90057 2.44949 0.00117775 0.000488919 2.15504 0.978502 0.492 0.492 116.565 1.52719 F F 8.57e+19 8.88624e-15 1 dx
Report srcpi bgdpi arf 2 X032910.82-271615.8 chandra ccd7 289.938 1033.12 14.9316 4.00002 0.00298034 0.000798404 5.45338 0.999996 1.21441 1.02886 164.801 5.86684 F F 8.08e+19 3.01905e-14 1 dx
Report srcpi bgdpi arf 3 X032849.03-271900.0 chandra ccd7 880.816 700.185 90.4813 9.89839 0.0180601 0.00197572 33.046 1 0.361704 0.361704 0 0.308293 F F 8.54e+19 1.35055e-13 1 dsx
Report srcpi bgdpi arf 5 X032903.76-271738.2 chandra ccd7 481.333 865.833 5.7038 2.4495 0.00113848 0.00048892 2.08317 0.978502 0.875393 0.492 116.93 3.85284 A F 8.08e+19 8.97081e-15 1 dx
Report srcpi bgdpi arf 6 X032852.71-272134.1 chandra ccd7 780.833 386.5 5.88537 2.44949 0.00117472 0.000488919 2.14948 0.978502 0.492 0.492 10.278 2.68358 F F 8.47e+19 9.09309e-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