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 X053528.77-691559.0 chandra ccd7 784.261 350.86 25.217 8.01915 0.00293789 0.000934265 2.84063 0.997224 0.967415 0.967415 0 0.449391 F F 2.65e+21 2.46648e-14 1 dsx
Report srcpi bgdpi arf rmf 2 X053527.98-691610.9 chandra ccd7 792.739 326.645 11866.1 110.337 1.38245 0.0128547 1336.68 1 0.712141 0.617716 13.9471 0.292709 T F 2.65e+21 5.75351e-12 1 dsxf
Report srcpi bgdpi arf 5 X053526.96-691628.3 chandra ccd7 803.774 291.28 46.2124 6.79797 0.00538395 0.000791993 5.2057 0.999999 1.49683 1.49683 0 0.314483 T F 2.65e+21 4.53128e-14 1 dsx
Report srcpi bgdpi arf 6 X053528.97-691554.7 chandra ccd7 782.126 359.618 16.3364 6.56904 0.00190327 0.000765323 1.84025 0.966939 0.685553 0.685553 0 0.505689 F F 2.65e+21 1.59842e-14 1 dsx
Report srcpi bgdpi arf 7 X053526.48-691635.9 chandra ccd7 808.947 275.859 36.9673 7.55122 0.00430685 0.000879749 4.16427 0.999948 1.5 0.446742 68.301 0.398894 A F 2.65e+21 4.48329e-14 1 dbsx

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