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 X174401.03+275312.3 chandra ccd7 516.648 246.032 26.2102 5.11959 0.00294653 0.000575539 4.82738 0.999991 0.413023 0.413023 0 1.33865 F F 4.61e+20 1.85505e-14 1 dsx
Report srcpi bgdpi arf 2 X174402.70+275432.0 chandra ccd7 471.591 408.009 11.9607 3.7662 0.00134461 0.000423391 2.20291 0.982719 0.317322 0.317322 0 2.41086 F F 4.62e+20 8.68347e-15 1 dsx
Report srcpi bgdpi arf rmf 3 X174356.44+275250.3 chandra ccd7 640.211 201.38 2352.65 49.6662 0.264482 0.00558342 433.309 1 0.396703 0.396703 0 0.261293 F F 4.6e+20 1.58566e-12 1 dsxf
Report srcpi bgdpi arf 5 X174351.49+275230.4 chandra ccd7 773.64 160.908 10.9504 3.54434 0.00123103 0.00039845 2.01684 0.974342 0.378682 0.378682 0 0.882134 F F 4.6e+20 7.72014e-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