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 X134735.50+121811.9 chandra ccd7 21.9341 846.855 14.5209 5.25612 0.0005782 0.000209291 2.30198 0.987181 0.333361 0.333361 0 0.430625 F F 1.88e+20 5.4825e-15 1 dsx
Report srcpi bgdpi arf 3 X134734.58+121237.7 chandra ccd7 49.4853 167.714 29.9734 6.29854 0.0011935 0.000250799 4.75164 0.999991 1.34502 1.34502 0 5.3666 F F 1.9e+20 1.22756e-14 1 dsx
Report srcpi bgdpi arf 4 X134733.70+121246.0 chandra ccd7 75.4919 184.603 33.1231 7.59455 0.00131891 0.000302404 5.25095 0.999998 1.88199 1.88199 0 5.23069 F F 1.9e+20 7.37877e-15 1 dsx
Report srcpi bgdpi arf rmf 5 X134733.36+121724.2 chandra ccd7 85.6685 750.014 1328.35 37.9494 0.0528928 0.00151109 210.581 1 0.408432 0.408432 0 0.610763 F T 1.88e+20 9.61617e-13 1 dsxf

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