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 2 X163630.95+661505.2 chandra ccd3 469.966 1061.33 32.7513 5.72288 0.0064101 0.00112008 27.2248 1 1.37746 0.724325 59.9944 5.87283 F F 2.61e+20 8.15617e-14 1 dsx
Report srcpi bgdpi arf 1 X163445.03+662049.0 chandra ccd0 545.7 941.3 8.86943 3.1623 0.00173592 0.000618923 2.99396 0.995853 2.70333 0.892359 7.93649 8.39472 A F 2.64e+20 2.3677e-14 1 dx
Report srcpi bgdpi arf 2 X163417.22+662125.7 chandra ccd0 885.5 1017.26 14.4657 4.12315 0.00283122 0.000806979 4.88305 0.999983 3.23987 2.35853 69.5095 10.6917 F F 2.65e+20 4.2503e-14 1 dx
Report srcpi bgdpi arf 3 X163412.43+661817.0 chandra ccd0 946.578 634.588 77.3673 9.28134 0.0151424 0.00181655 26.1161 1 3.4762 3.4762 0 9.22569 F F 2.64e+20 2.12979e-13 1 dsx
Report srcpi bgdpi arf 6 X163557.48+661436.8 chandra ccd3 880.25 1002 7.68108 2.82843 0.00150334 0.000553579 6.38497 0.999997 0.492 0.492 90 2.48012 F F 2.61e+20 1.72213e-14 1 dx
Report srcpi bgdpi arf 5 X163558.67+661250.8 chandra ccd3 865.3 786.7 7.56259 3.16232 0.00148014 0.000618927 6.28647 0.999997 0.770812 0.676027 93.4214 2.76966 F F 2.6e+20 1.71954e-14 1 dx
Report srcpi bgdpi arf 3 X163614.08+661409.5 chandra ccd3 676.214 946.929 6.66057 2.64576 0.0013036 0.000517826 5.53666 0.999979 0.581202 0.492 159.358 4.07726 F F 2.6e+20 1.56539e-14 1 dx
Report srcpi bgdpi arf 4 X163647.20+661448.5 chandra ccd3 269.786 1027.79 6.49216 2.64576 0.00127064 0.000517827 5.39667 0.999867 1.36683 0.492 133.715 7.45324 A F 2.6e+20 1.73348e-14 1 dx
Report srcpi bgdpi arf 7 X163606.48+661229.1 chandra ccd3 769.214 742.786 6.16899 2.64577 0.00120739 0.000517828 5.12803 0.999867 0.492 0.492 101.599 3.63594 F F 2.6e+20 1.44106e-14 1 dx
Report srcpi bgdpi arf 1 X163545.34+661713.9 chandra ccd1 813.7 310.1 4.95762 2.23607 0.000970301 0.000437642 7.6172 0.999994 0.492 0.492 58.2825 3.44633 F F 2.62e+20 1.12673e-14 1 dx
Report srcpi bgdpi arf 3 X163625.56+661638.6 chandra ccd1 320.25 239.5 3.93155 2 0.00076948 0.000391439 6.04069 0.99992 0.492 0.492 180 5.86028 F F 2.61e+20 9.6921e-15 1 dx
Report srcpi bgdpi arf 9 X163616.29+661104.3 chandra ccd3 648 570.75 3.90784 2 0.000764839 0.000391439 3.24843 0.996245 0.492 0.492 142.018 5.19797 F F 2.59e+20 9.74515e-15 1 dx
Report srcpi bgdpi arf 8 X163621.29+661143.0 chandra ccd3 586.75 649.5 3.84791 2 0.00075311 0.000391439 3.19861 0.996245 0.492 0.492 90 5.3151 F F 2.59e+20 9.57692e-15 1 dx
Report srcpi bgdpi arf 1 X163541.63+660809.8 chandra ccd2 48.5 420.25 3.84102 2.00001 0.000751762 0.00039144 5.40613 0.99982 0.687633 0.492 69.1832 5.88385 F F 2.59e+20 9.7627e-15 1 dx
Report srcpi bgdpi arf 2 X163521.69+662120.4 chandra ccd1 1103.25 811.25 3.72041 2.00001 0.000728156 0.00039144 5.71628 0.99992 0.917948 0.545637 52.2351 7.44645 A F 2.65e+20 9.59629e-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