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 rmf 1 X234349.81-151659.5 chandra ccd7 272.619 500.285 485.11 24.413 0.0213538 0.00107462 60.1402 1 0.573764 0.573764 0 0.485036 F F 1.87e+20 8.95171e-14 1 dsxf
Report srcpi bgdpi arf rmf 2 X234348.65-151727.7 chandra ccd7 306.496 443.027 107.38 14.1447 0.00472669 0.000622625 13.3121 1 0.638526 0.638526 0 0.969431 F F 1.87e+20 2.68733e-14 1 dsx
Report srcpi bgdpi arf rmf 3 X234349.44-151704.7 chandra ccd7 283.339 489.828 107.365 11.7002 0.00472603 0.000515021 13.3103 1 0.736519 0.736519 0 0.598875 T F 1.87e+20 2.67492e-14 1 dsx
Report srcpi bgdpi arf rmf 8 X234335.94-151915.8 chandra ccd7 680.292 223.144 228.272 15.9821 0.0100481 0.000703503 28.2994 1 0.865835 0.865835 0 4.50543 F F 1.85e+20 6.01485e-14 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