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 X124132.54+093151.3 chandra ccd6 465.933 461.698 35.0354 5.91907 0.00679475 0.00114794 65.2178 1 2.23721 2.23721 0 7.15907 F F 1.35e+20 0 1 ds
Report 6 X124139.78+093840.4 chandra ccd7 563.18 319.163 24.7116 4.97108 0.00479256 0.000964089 29.0403 1 0.387933 0.387933 0 1.26637 F F 1.34e+20 0 1 ds
Report 1 X124109.90+092915.9 chandra ccd5 876.048 1150.44 22.8108 5.56787 0.00442389 0.00107982 21.9234 1 3.47374 2.19234 11.1303 11.5064 A F 1.35e+20 0 1 d
Report 3 X124139.70+094144.1 chandra ccd7 565.686 692.673 18.815 4.33763 0.00364898 0.000841239 22.1108 1 0.753117 0.753117 0 2.99296 F F 1.33e+20 0 1 ds
Report 1 X124135.90+093931.4 chandra ccd7 679.934 422.775 17.0949 4.1346 0.00331539 0.000801865 20.0894 1 0.42034 0.42034 0 0.590743 F F 1.33e+20 0 1 ds
Report 4 X124150.23+093750.3 chandra ccd7 249.074 217.351 18.5909 4.31172 0.00360551 0.000836212 21.8475 1 1.45864 0.692295 97.799 3.97069 F F 1.34e+20 0 1 ds
Report 2 X124141.58+093941.2 chandra ccd7 508.75 442.375 7.81279 2.82843 0.0015152 0.000548542 9.18136 1 0.492 0.492 71.7356 1.80455 F F 1.33e+20 0 1 d
Report 1 X124105.74+094028.7 chandra ccd2 50.7856 963.929 6.55111 2.64576 0.00127051 0.000513115 12.0817 1 1.28916 0.649733 179.229 7.31703 A F 1.32e+20 0 1 d
Report 4 X124122.18+093606.4 chandra ccd6 776.667 979.833 5.91199 2.44949 0.00114656 0.000475051 11.0051 1 0.607961 0.492 70.3153 4.24637 F F 1.34e+20 0 1 d
Report 2 X124055.66+093612.0 chandra ccd2 354.1 442.3 4.44588 2.23608 0.000862228 0.000433663 8.19918 0.999986 1.37567 0.492 51.5347 10.0484 A F 1.33e+20 0 1 d
Report 5 X124130.84+094120.4 chandra ccd7 831.5 644 3.88688 2 0.000753817 0.000387878 4.56775 0.999088 0.492 0.492 90 2.54169 F F 1.33e+20 0 1 d
Report 2 X124133.62+093353.1 chandra ccd6 432.833 708.833 2.89632 1.73205 0.000561709 0.000335912 5.39145 0.99977 0.771213 0.492 169.375 5.11841 A F 1.35e+20 0 1 d
Report 3 X124124.29+093246.5 chandra ccd6 713.5 573.5 0.898451 1.00001 0.000174244 0.00019394 1.67245 0.965565 0.492 0.492 90 6.73945 F F 1.35e+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