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 X081717.60+103907.3 chandra ccd7 774.496 784.703 16.242 4.03014 0.00462301 0.00114711 15.6433 1 0.601091 0.601091 0 3.28563 F F 2.92e+20 3.25935e-14 1 dsx
Report srcpi bgdpi arf 5 X081714.52+103903.1 chandra ccd7 866.882 776.19 14.7549 3.84121 0.00419971 0.00109333 14.211 1 0.665073 0.665073 0 3.2664 F F 2.93e+20 3.02695e-14 1 dsx
Report srcpi bgdpi arf 4 X081709.80+104141.4 chandra ccd7 1007.79 1097.36 13.4005 3.74167 0.00381419 0.00106499 12.9066 1 1.29448 0.524431 37.527 6.10656 A F 2.96e+20 3.80057e-14 1 dx
Report srcpi bgdpi arf 1 X081704.68+102724.8 chandra ccd6 706.429 269.357 11.4346 3.7417 0.00325463 0.001065 24.8594 1 3.98389 1.70458 6.84948 8.9491 A F 2.91e+20 3.80913e-14 1 dx
Report srcpi bgdpi arf 3 X081722.07+104050.3 chandra ccd7 640.462 993.991 12.8361 4.05008 0.00365357 0.00115278 12.3629 1 2.49939 0.363096 115.115 5.1706 A F 2.92e+20 2.63746e-14 1 dsx
Report srcpi bgdpi arf 1 X081642.57+104141.9 chandra ccd3 595.862 331.136 11.6302 4.79057 0.00331033 0.00136355 3.45681 0.998504 3.67349 3.67349 0 10.2677 F F 3.04e+20 4.29239e-14 1 dsx
Report srcpi bgdpi arf 2 X081713.33+103654.2 chandra ccd7 902 513.6 9.62589 3.16228 0.00273981 0.000900079 9.27106 1 0.561557 0.492 99.8269 1.38335 F F 2.93e+20 1.88082e-14 1 dx
Report srcpi bgdpi arf 2 X081658.60+103218.6 chandra ccd6 888.389 866.611 8.82349 3 0.00251142 0.000853889 19.1827 1 0.854879 0.514135 142.519 5.72277 A F 2.94e+20 2.76578e-14 1 dx
Report 4 X081706.69+102914.8 chandra ccd6 646.1 492.9 4.89124 2.23607 0.00139219 0.000636451 10.6338 1 0.492 0.492 95.655 7.05814 F F 2.91e+20 0 1 d
Report srcpi bgdpi arf 7 X081704.47+103801.7 chandra ccd7 1167.5 650.9 4.83312 2.23607 0.00137565 0.000636452 4.65496 0.999127 0.492 0.492 49.2654 3.76431 F F 2.95e+20 1.06586e-14 1 dx
Report srcpi bgdpi arf 1 X081645.84+103819.8 chandra ccd2 120.5 860.75 3.83171 2.00001 0.00109062 0.00056926 12.5397 0.999997 0.751905 0.492 114.922 8.03414 A F 3e+20 1.41818e-14 1 dx
Report 3 X081652.24+103033.9 chandra ccd6 1079.17 653.833 2.94901 1.73205 0.000839375 0.000492993 6.41129 0.999929 0.492 0.492 105.941 8.04064 F F 2.95e+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