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 X002903.05+593419.1 chandra ccd7 374.156 220.75 140.964 12.2805 0.00571363 0.000497761 51.4155 1 0.410364 0.410364 0 0.1208 F F 4.53e+21 4.44612e-14 1 dsxf
Report srcpi bgdpi arf 2 X002908.92+593657.7 chandra ccd7 283.645 543.117 10.5268 4.93045 0.000426678 0.000199843 3.83957 0.999689 0.316908 0.316908 0 2.80167 F F 4.54e+21 4.12855e-15 1 dsx
Report srcpi bgdpi arf 3 X002912.38+593829.8 chandra ccd7 230.427 730.444 18.878 4.34488 0.000765173 0.000176109 6.88561 1 1.26013 1.26013 0 4.41377 F F 4.55e+21 7.54215e-15 1 dsx
Report srcpi bgdpi arf 4 X002903.06+593334.2 chandra ccd7 373.872 129.516 29.0733 6.16347 0.00117842 0.000249822 10.6043 1 0.44409 0.44409 0 0.731985 F F 4.52e+21 1.10188e-14 1 dsx
Report srcpi bgdpi arf 6 X002854.01+593255.2 chandra ccd7 513.25 49.875 6.74408 2.82848 0.000273355 0.000114646 2.45985 0.989549 0.593184 0.492 30.5946 1.71257 F F 4.53e+21 2.58518e-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