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 2 X174324.42-262452.3 chandra ccd3 472.7 832.3 4.95702 2.23607 0.00229491 0.00103522 10.4511 1 0.492 0.492 160.67 3.53282 F F 5.5e+21 0 1 d
Report srcpi bgdpi arf 1 X174339.02-262719.3 chandra ccd3 73.8999 533.5 4.93817 2.23607 0.00228619 0.00103522 10.4113 1 0.749315 0.492 43.2832 4.10678 A F 5.7e+21 2.9989e-14 1 dx
Report 1 X174407.92-262511.9 chandra ccd1 331.9 775.1 4.8971 2.23607 0.00226717 0.00103522 10.3601 1 0.492 0.492 30.4727 6.90908 F F 5.92e+21 0 1 d
Report srcpi bgdpi arf 1 X174336.99-261943.2 chandra ccd2 117.5 422.5 3.98077 2 0.00184295 0.000925924 8.24459 0.999995 0.508817 0.492 118.155 3.51079 F F 5.47e+21 2.4125e-14 1 dx
Report 2 X174329.63-262148.3 chandra ccd2 318.5 168.25 3.96507 2 0.00183568 0.000925925 8.21208 0.999995 0.492 0.492 90 2.41242 F F 5.46e+21 0 1 d
Report srcpi bgdpi arf 3 X174322.35-262837.6 chandra ccd3 529 374.25 3.89352 2 0.00180255 0.000925925 8.20886 0.999996 0.492 0.492 60.1282 6.48909 F T 5.58e+21 2.74268e-14 1 dx
Report 2 X174346.75-262600.3 chandra ccd1 909.833 677.167 2.96245 1.73205 0.0013715 0.000801874 6.26722 0.999913 0.492 0.492 90 3.36104 F F 5.73e+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