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 1 X122038.46+334725.8 chandra ccd7 829.224 530.543 248.897 16.3012 0.0806325 0.00528091 120.062 1 0.441286 0.385317 90 0.592593 F F 1.21e+20 0 1 ds
Report 10 X122033.85+334312.0 chandra ccd7 945.867 14.6626 194.235 13.9497 0.0629241 0.00451913 93.6945 1 1.14732 1.14732 0 4.24583 F F 1.24e+20 0 1 ds
Report 2 X122032.72+334356.0 chandra ccd7 974.631 103.987 102.389 10.1187 0.0331698 0.00327805 49.3901 1 1.08976 0.60372 17.0932 3.54736 A F 1.24e+20 0 1 ds
Report 3 X122037.04+334359.2 chandra ccd7 865.079 110.492 44.3552 6.65997 0.0143693 0.00215756 21.3959 1 1.20555 0.605662 17.6322 3.45732 F F 1.24e+20 0 1 ds
Report 1 X121913.90+334744.7 chandra ccd5 914.167 1007.75 9.09042 3.46417 0.00294492 0.00112225 11.2889 1 3.51806 2.64838 35.3369 16.9788 F F 1.19e+20 0 1 d
Report 1 X122000.57+335548.9 chandra ccd2 680.25 406.125 7.06388 2.82845 0.00228841 0.000916301 17.7503 1 2.00464 1.07001 87.8771 11.0995 A F 1.21e+20 0 1 d
Report 2 X122015.03+335508.6 chandra ccd2 314.4 323.9 9.59781 3.16229 0.00310929 0.00102445 24.1176 1 1.94984 0.492 174.612 8.81684 A F 1.21e+20 0 1 d
Report 4 X122032.65+334540.0 chandra ccd7 975.929 314.928 6.90089 2.64575 0.00223561 0.000857115 3.32883 0.998341 0.616294 0.492 144.952 1.86755 F F 1.21e+20 0 1 d
Report 1 X121956.51+334159.2 chandra ccd6 855.5 34.9285 5.73966 2.64579 0.00185941 0.000857126 13.9911 1 2.19918 1.27122 162.702 9.78084 A F 1.2e+20 0 1 d
Report 2 X122004.08+334912.1 chandra ccd6 662.333 914.5 5.71646 2.4495 0.0018519 0.000793536 13.9345 1 0.818204 0.787584 146.31 6.78279 F F 1.21e+20 0 1 d
Report 3 X122013.33+334426.5 chandra ccd6 428.7 333.7 4.91135 2.23607 0.00159107 0.000724395 11.972 1 0.549654 0.492 58.8793 5.5105 F F 1.21e+20 0 1 d
Report 8 X122016.18+334952.5 chandra ccd6 356 996.25 3.97231 2 0.00128687 0.000647918 9.68296 0.999999 0.492 0.492 37.9819 4.71779 F T 1.21e+20 0 1 d
Report 4 X122026.73+334312.8 chandra ccd6 89 183.75 3.96806 2 0.00128549 0.000647918 9.67259 0.999999 0.492 0.492 142.018 4.60281 F F 1.23e+20 0 1 d
Report 5 X122025.02+334716.0 chandra ccd6 132.167 678.167 2.98141 1.73205 0.000965854 0.000561113 7.26752 0.999971 0.492 0.492 19.9028 2.20497 F F 1.21e+20 0 1 d
Report 7 X122017.68+334834.9 chandra ccd6 318 838.5 1.97989 1.41421 0.000641403 0.000458147 4.82621 0.999299 0.492 0.492 180 3.897 F F 1.21e+20 0 1 d
Report 6 X122013.62+334743.9 chandra ccd6 421 735 1.97827 1.41421 0.000640877 0.000458147 4.82225 0.999299 0.492 0.492 45 4.57747 F F 1.21e+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