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 6 X104439.19+384534.2 chandra ccd7 833.474 945.95 620.775 25.5693 0.126765 0.00522135 184.102 1 0.369274 0.369274 0 0.335322 F F 1.29e+20 1.01506e-12 1 dsxf
Report srcpi bgdpi arf 1 X104452.02+384007.9 chandra ccd7 527.98 282.796 49.3265 7.10087 0.0100727 0.00145003 14.6286 1 2.00526 2.00526 0 6.31338 F F 1.26e+20 8.14752e-14 1 dsx
Report srcpi bgdpi arf 1 X104434.11+384952.0 chandra ccd6 447.284 520.919 20.1571 4.48967 0.00411619 0.000916815 32.4834 1 1.13875 0.718123 69.145 4.10373 F F 1.29e+20 4.63245e-14 1 dsx
Report srcpi bgdpi arf 2 X104522.32+384750.1 chandra ccd3 1079.8 720.096 12.6222 4.35828 0.00257755 0.000889994 5.00015 0.999961 2.71088 2.71088 0 8.84721 F F 1.24e+20 3.70586e-14 1 dsx
Report srcpi bgdpi arf 3 X104431.70+384146.4 chandra ccd7 1011.8 482.911 12.1483 3.48544 0.00248073 0.000711741 3.60279 0.999274 1.21674 1.21674 0 4.23918 F F 1.29e+20 2.08235e-14 1 dsx
Report srcpi bgdpi arf 2 X104411.56+384758.4 chandra ccd6 982.5 289.9 9.8189 3.16228 0.00200508 0.000645756 15.8233 1 0.968847 0.492 95.122 5.5984 A F 1.29e+20 2.57715e-14 1 dx
Report srcpi bgdpi arf 1 X104525.95+384701.1 chandra ccd3 992.8 620.2 8.64537 3.16231 0.00176545 0.000645767 3.42477 0.999051 2.09174 1.3551 120.219 9.40179 A F 1.24e+20 2.51893e-14 1 dx
Report srcpi bgdpi arf 7 X104430.63+384731.3 chandra ccd6 529.375 234.375 7.93386 2.82843 0.00162014 0.000577582 12.7855 1 0.492 0.492 68.4238 2.23143 F F 1.29e+20 1.76171e-14 1 dx
Report srcpi bgdpi arf 1 X104504.93+385220.5 chandra ccd2 1006.17 357.611 7.68158 3.00003 0.00156865 0.000612633 12.6047 1 2.50431 1.16915 36.0992 8.35018 A F 1.24e+20 2.27593e-14 1 dx
Report srcpi bgdpi arf 4 X104437.54+384153.1 chandra ccd7 872.357 496.072 6.72956 2.64576 0.0013742 0.000540275 1.99577 0.976287 0.760359 0.492 20.7276 3.94513 A F 1.26e+20 1.07505e-14 1 dx
Report srcpi bgdpi arf 5 X104444.91+384922.0 chandra ccd6 190.167 459.5 5.91084 2.44949 0.00120703 0.000500201 9.52537 1 0.672343 0.492 156.682 3.77897 F F 1.29e+20 1.37823e-14 1 dx
Report srcpi bgdpi arf 3 X104419.68+384637.3 chandra ccd6 789.7 124.9 4.92377 2.23607 0.00100546 0.000456619 7.9347 0.999997 0.828667 0.492 64.9682 3.67604 A F 1.29e+20 1.15047e-14 1 dx
Report srcpi bgdpi arf 6 X104433.63+385156.5 chandra ccd6 458 773.5 3.74223 2.00001 0.000764185 0.000408413 6.03063 0.999949 0.837885 0.492 40.2688 6.17459 A F 1.28e+20 9.58191e-15 1 dx
Report 4 X104423.12+384759.3 chandra ccd6 707.833 291.5 2.95975 1.73205 0.000604398 0.000353695 4.76966 0.999325 0.492 0.492 161.565 3.63076 F F 1.29e+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