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 3 X103638.12+124745.9 chandra ccd6 280.733 511.455 46.6687 6.83145 0.00922037 0.00134969 73.4583 1 2.82814 1.92264 1.63967 6.24766 F F 2.34e+20 1.0701e-13 1 dsx
Report srcpi bgdpi arf 1 X103617.07+124252.9 chandra ccd7 765.854 944.79 33.9575 5.82731 0.006709 0.0011513 35.6352 1 0.650947 0.479428 118.1 1.78848 F F 2.33e+20 4.96861e-14 1 dsx
Report 5 X103627.42+124126.2 chandra ccd7 457.883 768.724 25.4802 5.04779 0.00503414 0.000997296 26.7391 1 0.41019 0.41019 0 1.32328 F F 2.33e+20 0 1 ds
Report 3 X103622.10+124221.4 chandra ccd7 615.8 880.3 9.80339 3.16228 0.00193686 0.000624773 10.2877 1 0.492 0.492 42.2538 0.545168 F F 2.33e+20 0 1 d
Report srcpi bgdpi arf 1 X103642.99+124847.2 chandra ccd6 135.625 635.5 7.35229 2.82844 0.00145259 0.000558817 11.5728 1 1.17486 0.662374 144.975 7.76474 A F 2.34e+20 1.83165e-14 1 dx
Report srcpi bgdpi arf 1 X103711.55+123737.6 chandra ccd3 462.5 664.125 6.58268 2.82846 0.00130054 0.00055882 10.6761 1 2.61554 1.23723 135.011 12.53 A F 2.36e+20 1.82295e-14 1 dx
Report srcpi bgdpi arf 2 X103626.28+124959.9 chandra ccd6 632.3 783.3 4.80556 2.23607 0.000949436 0.000441782 7.56414 0.999996 0.598016 0.492 105.482 7.50558 F F 2.35e+20 1.117e-14 1 dx
Report srcpi bgdpi arf 4 X103611.03+124253.4 chandra ccd7 944.9 945.5 4.75355 2.23608 0.000939161 0.000441782 4.9884 0.99964 0.649616 0.492 8.4292 3.24426 F F 2.33e+20 7.63471e-15 1 dx
Report srcpi bgdpi arf 1 X103655.84+124430.5 chandra ccd2 1070.3 471.9 4.7325 2.23608 0.000935003 0.000441782 7.70081 0.999997 0.945265 0.492 178.913 7.96086 A F 2.37e+20 1.26009e-14 1 dx
Report 2 X103719.57+124733.5 chandra ccd2 365.1 844.5 4.41961 2.23608 0.000873184 0.000441784 7.19166 0.999953 1.37789 0.492 52.5806 14.4044 A F 2.4e+20 0 1 d
Report srcpi bgdpi arf 3 X103720.66+124624.9 chandra ccd2 332.389 704.944 6.85485 3.00006 0.00135431 0.000592722 11.1543 1 1.3714 0.492 19.2494 14.3015 A F 2.4e+20 1.99303e-14 1 dx
Report srcpi bgdpi arf 2 X103632.62+124135.7 chandra ccd7 302.75 787.5 3.86098 2 0.000762816 0.000395142 4.05173 0.997565 0.492 0.492 2.35031e-08 2.23903 F F 2.33e+20 5.94041e-15 1 dx
Report 6 X103630.32+124708.3 chandra ccd6 512.167 434.5 2.92573 1.73205 0.000578038 0.000342203 4.60521 0.999198 0.492 0.492 18.4349 4.86061 F F 2.33e+20 0 1 d
Report 4 X103624.83+124907.1 chandra ccd6 675.5 676 1.91981 1.41422 0.000379297 0.000279407 3.02185 0.991878 0.492 0.492 26.5651 6.61076 F F 2.34e+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