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 X122736.03+442327.5 chandra ccd3 230.608 368.442 36.0116 6.00097 0.00646336 0.00107705 42.2869 1 0.506192 0.506192 0 2.49855 F F 1.61e+20 6.72149e-14 1 dsx
Report srcpi bgdpi arf 5 X122754.35+442149.6 chandra ccd2 865.426 97.4933 23.4272 4.84017 0.00426123 0.000880389 27.511 1 0.406509 0.406509 0 1.75345 F F 1.63e+20 4.28484e-14 1 dsx
Report 6 X122738.90+442132.3 chandra ccd3 168.059 134.315 20.5667 4.53792 0.00369132 0.000814468 24.1506 1 0.327042 0.327042 0 1.03845 F T 1.62e+20 0 1 ds
Report srcpi bgdpi arf 3 X122807.08+442622.4 chandra ccd2 588.033 651.567 13.9465 3.873 0.00253551 0.000704123 16.3776 1 1.28581 0.606564 176.946 6.30199 A F 1.61e+20 2.89483e-14 1 dx
Report srcpi bgdpi arf 1 X122705.62+441551.5 chandra ccd1 963.5 487.885 9.78162 3.60561 0.00175083 0.000645374 11.4587 1 2.49667 2.05182 140.208 8.98486 F F 1.61e+20 2.10677e-14 1 dx
Report srcpi bgdpi arf 1 X122822.27+441915.1 chandra ccd0 324.8 795.6 9.02101 3.1623 0.00161561 0.000566349 10.5658 1 1.28493 1.01555 42.9841 7.08167 F F 1.64e+20 1.9576e-14 1 dx
Report srcpi bgdpi arf 3 X122728.19+441427.9 chandra ccd1 470.786 317.214 6.57754 2.64576 0.00117732 0.000473569 7.7053 0.999999 0.566374 0.492 107.219 7.63068 F F 1.64e+20 1.4785e-14 1 dx
Report srcpi bgdpi arf 2 X122703.78+441932.9 chandra ccd1 1002.79 938.072 6.26381 2.64577 0.00112117 0.00047357 7.33777 0.999989 1.27363 1.0033 109.936 7.57425 F F 1.59e+20 1.37656e-14 1 dx
Report srcpi bgdpi arf 2 X122757.41+441708.4 chandra ccd0 866.833 537.5 5.79014 2.4495 0.00103698 0.00043869 6.78165 0.999988 0.492 0.492 110.994 4.91531 F F 1.65e+20 1.1187e-14 1 dx
Report srcpi bgdpi arf 2 X122738.95+442401.7 chandra ccd3 166.5 437.5 4.83286 2.23607 0.000867028 0.000401157 5.67503 0.999891 0.492 0.492 45 2.73101 F F 1.61e+20 9.7224e-15 1 dx
Report srcpi bgdpi arf 4 X122726.08+442518.7 chandra ccd3 446.7 594.1 4.81723 2.23607 0.000864223 0.000401157 5.65667 0.999891 0.651847 0.492 134.132 5.06087 F F 1.59e+20 9.78912e-15 1 dx
Report srcpi bgdpi arf 4 X122739.27+441657.3 chandra ccd1 228.7 620.9 4.81381 2.23607 0.000861631 0.000400238 5.63916 0.999888 0.492 0.492 130.935 4.64671 F F 1.64e+20 9.12092e-15 1 dx
Report srcpi bgdpi arf 4 X122814.51+442710.5 chandra ccd2 426.5 749.7 4.40324 2.23608 0.000800522 0.000406527 5.1708 0.999891 1.16688 0.492 2.35031e-08 7.78087 A F 1.6e+20 9.81519e-15 1 dx
Report 2 X122755.43+442438.6 chandra ccd2 841.5 440.5 3.89318 2 0.000707792 0.000363606 4.57183 0.999082 0.492 0.492 2.35031e-08 3.68174 F F 1.62e+20 0 1 d
Report srcpi bgdpi arf 1 X122806.41+442312.8 chandra ccd2 602.25 266.25 3.87942 2 0.00070529 0.000363606 4.55567 0.999082 0.492 0.492 90 4.23931 F F 1.63e+20 7.66531e-15 1 dx
Report srcpi bgdpi arf 6 X122742.42+441643.0 chandra ccd1 160 591.75 3.86717 2 0.000692191 0.000357984 4.53022 0.999062 0.492 0.492 70.6701 4.80019 F T 1.64e+20 7.77098e-15 1 dx
Report 3 X122705.92+442449.7 chandra ccd3 885.833 535.833 2.84486 1.73206 0.000510374 0.000310735 3.3406 0.9935 0.492 0.492 45 7.68903 F F 1.57e+20 0 1 d
Report srcpi bgdpi arf 5 X122712.71+442657.3 chandra ccd3 737.5 794.833 2.69809 1.73206 0.000484043 0.000310736 3.16825 0.9935 0.492 0.492 180 7.90119 F F 1.57e+20 6.1193e-15 1 dx
Report 5 X122740.15+441838.5 chandra ccd1 209.5 826.5 1.90846 1.41422 0.000341598 0.000253133 2.23568 0.962274 0.492 0.492 90 2.97189 F F 1.63e+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