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 rmf 1 X004050.54+100326.8 chandra ccd7 743.318 932.025 1638.94 42.6153 0.206353 0.00536554 202.039 1 0.483994 0.483994 0 0.315375 F F 5.33e+20 2.80492e-12 1 dsxf
Report srcpi bgdpi arf rmf 6 X004058.75+095802.2 chandra ccd7 496.827 272.316 494.243 22.6236 0.0622283 0.00284845 60.9273 1 2.35997 1.30069 160.567 5.99805 A F 5.33e+20 5.09125e-13 1 dsx
Report srcpi bgdpi arf 1 X004137.78+100642.7 chandra ccd3 638.397 1032.65 34.6819 8.86892 0.00436666 0.00111665 5.22993 0.999999 6.18116 5.29118 0 12.272 F F 5.31e+20 5.96314e-14 1 dsx
Report srcpi bgdpi arf 2 X004051.58+100300.0 chandra ccd7 712.157 877.634 17.9952 4.54956 0.0022657 0.000572817 2.21834 0.982696 0.47397 0.47397 0 0.79005 F F 5.33e+20 1.68318e-14 1 dsx
Report srcpi bgdpi arf 1 X004135.89+101449.7 chandra ccd2 352.167 1061 8.86643 3.46417 0.00111677 0.00043633 11.6136 1 4.1718 2.31875 162.565 16.055 A F 5.25e+20 1.68067e-14 1 dx
Report srcpi bgdpi arf 2 X004027.19+100704.5 chandra ccd6 1074.67 392.167 5.58046 2.4495 0.000702887 0.000308527 7.01057 0.999995 1.13721 0.989887 33.2645 6.48569 F F 5.32e+20 8.43527e-15 1 dx
Report srcpi bgdpi arf 1 X004052.60+100759.6 chandra ccd6 312 504 3.85057 2 0.000484998 0.00025191 4.83736 0.999496 0.558468 0.492 9.21747 4.4908 F F 5.33e+20 5.25107e-15 1 dx
Report 7 X004033.99+101054.0 chandra ccd6 870.5 858.5 2.74828 1.73206 0.00034616 0.000218161 3.45258 0.995932 0.492 0.492 90 8.2463 F F 5.32e+20 0 1 d
Report 3 X004028.02+100913.1 chandra ccd6 1049.5 653.5 2.73283 1.73206 0.000344214 0.000218161 3.43318 0.995932 0.492 0.492 45 7.71093 F F 5.32e+20 0 1 d
Report 4 X004040.40+101035.6 chandra ccd6 678.167 821.167 2.69725 1.73206 0.000339732 0.000218161 3.38847 0.995932 0.639127 0.492 78.6901 7.35934 F F 5.28e+20 0 1 d
Report srcpi bgdpi arf 5 X004055.86+100736.2 chandra ccd6 214 456.5 1.93202 1.41422 0.000243347 0.000178127 2.42714 0.973433 0.492 0.492 116.565 4.33591 F F 5.33e+20 2.67736e-15 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