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 X013647.70+412416.0 chandra ccd7 820.219 84.1939 766.161 28.3384 0.0504878 0.00186742 195.595 1 0.416247 0.416247 0 0.243333 F F 6.79e+20 2.35574e-13 1 dsxf
Report srcpi bgdpi arf 4 X013642.93+412413.8 chandra ccd7 929.131 79.6889 40.3798 6.35451 0.00266091 0.000418744 10.3086 1 0.444907 0.444907 0 0.671869 F F 6.8e+20 2.01435e-14 1 dsx
Report srcpi bgdpi arf 2 X013701.35+412430.9 chandra ccd7 508.084 114.702 10.2331 4.39978 0.000674334 0.000289934 2.61243 0.991897 0.451335 0.451335 0 2.80881 F F 6.76e+20 5.1927e-15 1 dsx
Report srcpi bgdpi arf 3 X013712.82+412441.4 chandra ccd7 245.167 135.667 8.98617 3.1623 0.000592161 0.000208386 2.2941 0.985675 0.492 0.492 59.6789 4.96257 F F 6.74e+20 4.64546e-15 1 dx
Report srcpi bgdpi arf 1 X013635.81+412434.0 chandra ccd6 51.5 162.5 2.86947 1.73206 0.00018909 0.000114138 2.07531 0.954955 0.492 0.492 90 2.04396 F F 6.83e+20 2.12334e-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