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 X130635.67-460202.0 chandra ccd7 305.084 825.485 1403.53 38.3352 0.0375792 0.00102642 267.412 1 0.430539 0.430539 0 0.281924 F F 7.76e+20 1.47484e-13 1 dsxf
Report srcpi bgdpi arf 3 X130634.78-460414.0 chandra ccd7 323.958 557.051 28.7891 6.13296 0.000770824 0.000164209 5.48513 0.999999 0.481745 0.481745 0 2.41258 F F 7.81e+20 5.92376e-15 1 dsx
Report srcpi bgdpi arf 2 X130637.74-460317.5 chandra ccd7 261.356 671.896 27.3023 5.92118 0.000731014 0.000158538 5.20185 0.999997 0.413399 0.413399 0 1.5678 F F 7.8e+20 5.54826e-15 1 dsx
Report srcpi bgdpi arf 1 X130632.39-455608.4 chandra ccd6 153.629 517.117 31.05 5.74285 0.000831358 0.000153764 20.704 1 3.38229 1.42923 54.1768 5.67934 A F 7.63e+20 9.13733e-15 1 dsx
Report srcpi bgdpi arf 2 X130632.20-455932.8 chandra ccd6 157.125 101.125 7.31129 2.82844 0.000195759 7.5731e-05 4.87514 0.99988 0.525674 0.492 58.6498 2.31077 F F 7.7e+20 2.01158e-15 1 dx

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