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 X183452.12-084555.9 chandra ccd7 132.033 223.512 44.2184 8.1961 0.0011767 0.000218106 14.9772 1 0.645577 0.394802 324.674 0.176931 1.74102 45.5138 0.926314 0.234846 F F 1.63e+22 1.65827e-14 1 dsx
Report srcpi bgdpi arf 2 X183450.57-084304.0 chandra ccd7 178.894 572.891 16.3504 4.04356 0.000435101 0.000107603 5.53803 0.999998 1.35415 1.35415 0 2.96365 1.54453 9.68176 0.724837 0.589562 T F 1.65e+22 6.70929e-15 1 dsx
Report srcpi bgdpi arf 3 X183453.54-084707.4 chandra ccd7 89.2216 78.1862 23.0688 5.64953 0.000613883 0.000150339 7.81361 1 0.426597 0.426597 0 1.15578 11.0698 12.408 0.057001 0.260199 F F 1.62e+22 8.8105e-15 1 dsx

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