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 X045513.26+301745.2 chandra ccd7 128.064 292.659 34.9703 5.91357 0.00256542 0.000433819 8.38251 1 1.10159 1.10159 0 4.51366 F F 2.51e+21 2.24283e-14 1 dsx
Report srcpi bgdpi arf 2 X045517.59+301559.9 chandra ccd7 13.7 78.2 7.96226 3.16234 0.000584111 0.000231989 1.90858 0.967918 0.778292 0.630689 42.182 6.42112 F F 2.52e+21 9.37629e-15 1 dx
Report srcpi bgdpi arf 3 X045513.73+301634.5 chandra ccd7 115.829 148.876 29.7857 6.84628 0.00218508 0.000502244 7.13974 1 1.83042 1.83042 0 5.69332 F F 2.52e+21 1.95859e-14 1 dsx
Report srcpi bgdpi arf rmf 4 X045510.99+302159.4 chandra ccd7 187.815 809.276 611.668 25.4322 0.044872 0.0018657 146.619 1 0.385181 0.385181 0 0.295655 F F 2.5e+21 2.10283e-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