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 X174430.63-255158.9 chandra ccd1 679 433 5.67289 2.4495 0.00262633 0.00113402 13.7313 1 1.11532 1.00135 110.593 6.08604 F F 5.31e+21 3.51208e-14 1 dx
Report 1 X174400.56-254402.3 chandra ccd2 469.3 362.7 4.92416 2.23607 0.0022797 0.00103522 12.2737 1 0.592813 0.492 97.4657 4.37782 F F 4.81e+21 0 1 d
Report srcpi bgdpi arf 2 X174442.97-254932.4 chandra ccd1 340.1 730.5 4.88195 2.23607 0.00226016 0.00103522 11.8169 1 1.112 0.492 3.95358 6.87242 A F 5.42e+21 3.16823e-14 1 dx
Report srcpi bgdpi arf 3 X174427.11-255308.4 chandra ccd1 775.5 291.786 6.77665 2.64576 0.00313733 0.00122488 16.403 1 1.5134 0.586443 11.1589 6.67176 A F 5.28e+21 4.44912e-14 1 dx
Report srcpi bgdpi arf 3 X174353.32-254457.5 chandra ccd2 668.167 250.5 2.97014 1.73205 0.00137506 0.000801874 7.40322 0.999975 0.492 0.492 180 5.21419 F F 4.77e+21 1.97245e-14 1 dx
Report 2 X174344.23-254641.7 chandra ccd2 917.5 38.5 0.969644 1 0.000448908 0.000462963 2.41689 0.988356 0.492 0.492 90 6.80631 F F 4.73e+21 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