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 X174724.13-314051.8 chandra ccd3 509.247 337.949 21.6012 5.91713 0.0110902 0.0030379 5.89853 1 0.918222 0.247509 113.382 4.82628 9 12.9543 0.180116 0.268243 F F 6.89e+21 1.60061e-13 1 dsx
Report srcpi bgdpi arf 1 X174628.54-314858.6 chandra ccd0 753.786 233.643 6.63523 3.78388 0.00340679 0.0019428 10.9862 1 3.47368 1.24707 29.7311 9.71628 5.90881 0.787219 -0.76487 0.719816 A F 7.14e+21 5.51128e-14 1 dx
Report srcpi bgdpi arf 2 X174634.64-314851.0 chandra ccd0 595.75 249.25 3.88745 3.17945 0.00199597 0.00163246 11.5876 1 1.36519 0.604884 89.6745 8.69082 1.92497 1.96248 0.0096507 0.832479 A F 7.07e+21 3.3869e-14 1 dx
Report 1 X174722.63-314404.3 chandra ccd2 394.833 967.167 2.97643 1.73205 0.00152815 0.000889267 8.41162 0.999991 0.492 0.492 16.845 4.45162 F F 6.8e+21 0 1 d
Report 1 X174649.46-314010.5 chandra ccd1 375.167 273.5 2.96319 1.73205 0.00152139 0.000889286 8.60296 0.999992 0.529672 0.492 100.278 3.73504 F F 7.22e+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