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 3 X205046.52+601505.2 chandra ccd1 597.386 188.326 31.7244 5.63554 0.00320087 0.000568604 41.4418 1 1.7617 0.889823 40.8332 6.50543 F F 2.92e+21 4.22527e-14 1 dsx
Report srcpi bgdpi arf 1 X205204.97+602536.8 chandra ccd3 303.191 928.51 31.0225 5.90428 0.00313003 0.000595715 14.5076 1 4.09646 2.04138 319.985 8.34185 F F 2.96e+21 4.39841e-14 1 dsx
Report srcpi bgdpi arf 1 X205048.25+601007.6 chandra ccd0 1106.8 447.302 35.2087 6.90344 0.00355125 0.000696301 9.97898 1 5.55653 1.911 40.315 9.81679 A F 2.92e+21 6.27602e-14 1 dsx
Report srcpi bgdpi arf 3 X205116.08+602351.5 chandra ccd3 1039.13 714.167 25.1754 5.52111 0.00254009 0.000557056 11.7732 1 2.26696 0.674532 343.02 5.86539 A F 2.94e+21 3.18286e-14 1 dsx
Report srcpi bgdpi arf 2 X205142.82+601148.1 chandra ccd0 278.808 650.115 12.1815 3.60557 0.00122866 0.000363668 3.45253 0.998871 1.14245 0.760589 127.35 6.67007 A F 2.98e+21 1.60227e-14 1 dx
Report srcpi bgdpi arf 1 X205033.40+601801.9 chandra ccd1 793.955 547.591 10.1838 3.31664 0.0010275 0.000334634 13.3032 1 1.79173 0.723487 133.92 7.27063 A F 2.9e+21 1.328e-14 1 dx
Report srcpi bgdpi arf 2 X205022.23+602049.3 chandra ccd1 961.167 888.5 9.62216 3.46415 0.000970833 0.000349517 12.5695 1 3.21242 0.994638 176.648 8.99196 A F 2.89e+21 1.30655e-14 1 dx
Report 6 X205111.54+601920.8 chandra ccd1 217.611 706.5 8.89375 3 0.000897339 0.000302687 11.618 1 0.492 0.492 90 2.73334 F F 2.94e+21 0 1 d
Report srcpi bgdpi arf 2 X205149.02+602623.9 chandra ccd3 542.833 1023.28 7.56024 3.00003 0.000762794 0.000302689 3.53552 0.999071 2.17353 1.5524 177.625 8.32995 F F 2.95e+21 1.05795e-14 1 dx
Report srcpi bgdpi arf 5 X205153.99+602106.2 chandra ccd3 467.167 377.667 5.88408 2.44949 0.000593677 0.000247143 2.75167 0.99254 0.730045 0.492 162.109 3.87635 F F 2.97e+21 7.54053e-15 1 dx
Report srcpi bgdpi arf 5 X205107.21+601811.8 chandra ccd1 283.3 566.3 4.78194 2.23607 0.000482476 0.00022561 6.24669 0.999966 0.72715 0.492 100.901 3.0805 F F 2.94e+21 5.59825e-15 1 dx
Report 4 X205121.99+602132.7 chandra ccd3 949.75 431.5 3.86707 2 0.00039017 0.000201791 1.80842 0.956283 0.535045 0.492 140.31 3.44303 F F 2.95e+21 0 1 d
Report srcpi bgdpi arf 4 X205047.81+602241.2 chandra ccd1 574.75 1114.5 3.65622 2.00001 0.000368896 0.000201792 4.77615 0.999645 0.867915 0.492 15.4189 6.9919 A F 2.92e+21 4.79001e-15 1 dx
Report srcpi bgdpi arf 1 X205230.70+601940.0 chandra ccd2 467.833 1071.83 2.69392 1.73206 0.000271717 0.000174701 3.50202 0.996802 0.7585 0.492 91.5899 7.38165 A F 3e+21 3.74915e-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