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 X013647.67+412416.0 chandra ccd7 819.139 77.3298 776.128 28.4193 0.0513928 0.00188184 218.519 1 0.4074 0.4074 0 0.24135 F F 6.79e+20 2.30275e-13 1 dsxf
Report srcpi bgdpi arf 4 X013642.91+412413.7 chandra ccd7 927.885 72.7341 48.7223 7.30609 0.00322624 0.000483787 13.7178 1 0.519085 0.519085 0 0.669708 F F 6.8e+20 2.44422e-14 1 dsx
Report srcpi bgdpi arf 3 X013712.87+412441.6 chandra ccd7 242.974 129.772 21.7589 5.78138 0.00144081 0.000382824 6.12623 1 0.957951 0.957951 0 4.97528 F F 6.74e+20 1.13224e-14 1 dsx
Report srcpi bgdpi arf 2 X013701.32+412431.2 chandra ccd7 506.975 108.375 14.0262 4.07858 0.00092877 0.00027007 3.94909 0.999712 0.621895 0.621895 0 2.80502 F F 6.76e+20 7.10228e-15 1 dsx
Report srcpi bgdpi arf 1 X013607.52+412352.6 chandra ccd6 693.955 52.2273 8.85907 3.31666 0.000586619 0.000219619 6.54162 0.999996 1.53815 0.752735 139.861 7.31171 A F 6.88e+20 6.67315e-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