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 X173624.25-284532.6 chandra ccd1 535.281 610.836 23.5398 4.85178 0.0108982 0.00224624 48.0208 1 2.45905 0.45235 356.091 6.04753 A F 6.07e+21 1.60489e-13 1 dsx
Report 1 X173610.60-283752.1 chandra ccd0 856.167 505.5 5.94034 2.44949 0.00275015 0.00113402 12.18 1 0.492 0.492 90 4.88869 F F 5.68e+21 0 1 d
Report srcpi bgdpi arf 1 X173548.67-284710.0 chandra ccd3 458.7 445.5 4.91043 2.23607 0.00227334 0.00103522 9.90246 1 0.668613 0.492 101.749 5.58554 F F 5.79e+21 3.14461e-14 1 dx
Report srcpi bgdpi arf 1 X173540.12-283710.1 chandra ccd2 622.1 647.7 4.74561 2.23608 0.00219704 0.00103522 9.51311 0.999994 1.39577 0.492 119.49 6.8739 A F 5.42e+21 3.33628e-14 1 dx
Report 2 X173609.02-284548.9 chandra ccd1 941.75 577.25 3.98476 2 0.00184479 0.000925924 8.12886 0.999995 0.492 0.492 7.01812 3.9413 F F 5.92e+21 0 1 d
Report 2 X173617.15-284042.3 chandra ccd0 681.25 159.5 3.94926 2 0.00182836 0.000925925 8.09749 0.999995 0.492 0.492 147.312 3.86882 F F 5.83e+21 0 1 d
Report srcpi bgdpi arf 4 X173600.36-284754.1 chandra ccd3 146.167 355.833 2.9724 1.73205 0.00137611 0.000801874 5.9942 0.999875 0.492 0.492 90 5.62034 F F 5.91e+21 1.87975e-14 1 dx
Report 2 X173551.13-284244.5 chandra ccd3 393.167 985.167 2.96707 1.73205 0.00137364 0.000801874 5.98344 0.999875 0.492 0.492 16.845 2.22204 F F 5.68e+21 0 1 d
Report srcpi bgdpi arf 3 X173555.22-284752.3 chandra ccd3 283.5 359.5 2.93485 1.73205 0.00135872 0.000801875 5.91846 0.999875 0.492 0.492 45 5.73193 F F 5.87e+21 1.94363e-14 1 dx
Report 3 X173608.80-283626.1 chandra ccd0 904.5 680.167 2.90737 1.73205 0.001346 0.000801875 5.96121 0.99989 0.492 0.492 28.155 6.09047 F F 5.62e+21 0 1 d
Report 4 X173606.33-283342.1 chandra ccd0 970.5 1013.5 2.86909 1.73206 0.00132828 0.000801876 5.88272 0.99989 1.08631 0.492 180 8.65939 A F 5.5e+21 0 1 d
Report 5 X173618.01-284020.2 chandra ccd0 658.25 204.25 3.95737 2 0.00183211 0.000925925 8.11412 0.999995 0.492 0.492 90 4.19866 F F 5.83e+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