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 X124543.80+135350.5 chandra ccd5 1171.27 849.363 44.087 9.74722 0.00866162 0.001915 34.5554 1 6.95396 6.08228 177.931 13.2587 F F 1.9e+20 9.32186e-14 1 dx
Report srcpi bgdpi arf 1 X124529.19+134131.4 chandra ccd7 275.945 951.505 38.9274 6.42469 0.00764795 0.00126224 35.7909 1 0.622758 0.349995 330.885 2.11945 F F 1.87e+20 5.72857e-14 1 dsx
Report srcpi bgdpi arf 6 X124514.53+133806.6 chandra ccd7 710.066 535.253 20.4678 4.52414 0.00402126 0.000888845 18.8186 1 1.10222 0.582554 298.112 4.01093 F F 1.87e+20 3.03743e-14 1 dsx
Report srcpi bgdpi arf 5 X124534.49+134054.2 chandra ccd7 118.2 875.5 9.61804 3.16229 0.00188962 0.000621284 8.84308 1 0.721954 0.492 5.12961 3.51276 F F 1.87e+20 1.91197e-14 1 dx
Report srcpi bgdpi arf 4 X124501.27+133847.9 chandra ccd7 1102.4 618.7 9.59884 3.16229 0.00188585 0.000621284 8.82543 1 0.819198 0.492 5.25253 5.58781 A F 1.86e+20 1.47152e-14 1 dx
Report srcpi bgdpi arf 2 X124531.15+134228.8 chandra ccd6 843.167 246.611 8.87117 3 0.00174289 0.000589401 13.8267 1 0.860499 0.492 170.552 2.65096 A F 1.87e+20 1.86492e-14 1 dx
Report srcpi bgdpi arf 3 X124516.15+134312.7 chandra ccd7 661.611 1156.83 8.68336 3.00001 0.00170599 0.000589401 7.98372 0.999999 0.562874 0.492 120.668 1.73741 F F 1.87e+20 1.27399e-14 1 dx
Report srcpi bgdpi arf 1 X124525.03+134409.3 chandra ccd6 1024.62 451 7.86959 2.82843 0.00154611 0.000555692 12.2656 1 0.815525 0.492 4.5994 2.5545 A F 1.87e+20 1.6597e-14 1 dx
Report srcpi bgdpi arf 4 X124533.96+134152.7 chandra ccd6 760.167 173.333 5.87037 2.44949 0.00115333 0.000481244 9.14961 1 0.925418 0.492 20.682 3.25423 A F 1.87e+20 1.25849e-14 1 dx
Report srcpi bgdpi arf 2 X124517.05+134131.7 chandra ccd7 634.9 951.7 4.78343 2.23607 0.000939784 0.000439314 4.39801 0.998603 0.492 0.492 75.1276 0.908021 F F 1.87e+20 6.89298e-15 1 dx
Report srcpi bgdpi arf 3 X124512.97+134545.5 chandra ccd6 1381.75 646.5 3.89462 2 0.000765163 0.000392934 6.07019 0.99993 0.492 0.492 129.116 4.32754 F F 1.87e+20 1.34286e-14 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