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 X112416.77+212019.6 chandra ccd1 587.371 387.185 17.5821 5.22793 0.00351268 0.00104447 5.63102 0.999999 2.93923 2.93923 0 9.24859 F F 1.65e+20 5.01075e-14 1 dsx
Report srcpi bgdpi arf 1 X112433.83+212723.1 chandra ccd0 685.497 400.273 15.9261 3.99075 0.00318183 0.000797302 10.0453 1 3.69211 0.766655 336.098 6.76294 A F 1.65e+20 4.20987e-14 1 dsx
Report srcpi bgdpi arf 2 X112422.59+213132.2 chandra ccd0 1004.71 906.273 45.1821 7.08585 0.00902681 0.00141566 28.4984 1 1.48354 0.50472 6.44164 4.54225 A F 1.58e+20 1.13102e-13 1 dsx
Report srcpi bgdpi arf 2 X112348.75+212831.3 chandra ccd3 528.538 744.663 15.8847 3.9856 0.00317552 0.000796763 15.8603 1 0.940421 0.940421 0 4.03256 F F 1.55e+20 3.97162e-14 1 dsx
Report srcpi bgdpi arf 4 X112418.69+212442.2 chandra ccd1 532.5 920.5 9.83178 3.16228 0.00196426 0.000631782 3.14883 0.997382 0.492 0.492 163.155 5.41846 F F 1.62e+20 2.57983e-14 1 dx
Report srcpi bgdpi arf 1 X112356.65+213716.1 chandra ccd2 930.682 1009.77 8.99692 3.31666 0.00179747 0.000662625 12.5458 1 3.0583 2.13489 71.8904 8.32739 F F 1.49e+20 2.67306e-14 1 dx
Report srcpi bgdpi arf 2 X112406.26+212752.2 chandra ccd1 885.389 1306.5 8.8321 3 0.00176454 0.000599361 2.82866 0.994422 0.492 0.492 58.7038 1.35286 F F 1.58e+20 3.74746e-14 1 dx
Report srcpi bgdpi arf 1 X112346.30+212832.9 chandra ccd3 597.5 747.5 8.72297 3.00001 0.00174381 0.000599733 8.70955 1 0.660442 0.509657 105.482 4.58764 F F 1.55e+20 2.27387e-14 1 dx
Report srcpi bgdpi arf 7 X112400.80+212809.6 chandra ccd3 186.214 699.928 6.45953 2.64576 0.00129133 0.000528916 6.44958 0.99999 0.492 0.492 142.628 1.57484 F T 1.57e+20 1.50917e-14 1 dx
Report srcpi bgdpi arf 7 X112404.32+213147.2 chandra ccd2 713.5 341.3 5.88401 2.44949 0.00117555 0.000489376 8.20496 0.999999 0.492 0.492 90 2.59259 F T 1.55e+20 1.41698e-14 1 dx
Report srcpi bgdpi arf 3 X112403.63+212639.9 chandra ccd1 960 1159.67 5.83684 2.44949 0.00116612 0.000489377 1.86937 0.959432 0.55708 0.492 6.66227 2.60306 F F 1.59e+20 1.36187e-14 1 dx
Report 4 X112409.37+213329.3 chandra ccd2 570.1 548.7 4.92945 2.23607 0.00098484 0.000446737 6.87388 0.999983 0.492 0.492 16.2356 4.34917 F F 1.54e+20 0 1 d
Report srcpi bgdpi arf 6 X112350.13+213315.7 chandra ccd2 1115.7 521.3 4.88186 2.23607 0.00097533 0.000446737 6.8075 0.999983 0.603188 0.492 63.7843 5.44608 F F 1.52e+20 1.29812e-14 1 dx
Report srcpi bgdpi arf 5 X112345.08+213303.0 chandra ccd2 1258.9 495.5 4.6185 2.23608 0.000922714 0.00044674 6.44026 0.999983 0.797182 0.65727 172.238 6.15919 F F 1.51e+20 1.30342e-14 1 dx
Report srcpi bgdpi arf 6 X112338.44+212831.0 chandra ccd3 820.5 743.7 4.57479 2.23608 0.000914549 0.000447016 4.56775 0.999396 1.10184 0.492 154.822 6.4056 A F 1.53e+20 1.24019e-14 1 dx
Report srcpi bgdpi arf 3 X112410.95+213231.2 chandra ccd2 525.25 430.75 3.93638 2 0.000786436 0.000399574 5.48908 0.999804 0.492 0.492 45 3.51215 F F 1.55e+20 9.82754e-15 1 dx
Report srcpi bgdpi arf 3 X112345.76+213150.5 chandra ccd3 612.75 1149 3.83301 2.00001 0.00076626 0.000399822 3.82712 0.996293 0.492 0.492 7.46571 5.35126 F F 1.52e+20 1.02549e-14 1 dx
Report 2 X112408.19+213210.1 chandra ccd2 603.5 387.833 2.93061 1.73205 0.000585496 0.000346041 4.08659 0.998062 0.492 0.492 90 3.0021 F F 1.55e+20 0 1 d

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