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 4 X100120.85+555349.7 chandra ccd7 841.403 553.427 371.333 19.9297 0.119373 0.00640683 88.9123 1 0.423331 0.423331 0 0.299122 F F 9.29e+19 9.11327e-13 1 dsxf
Report srcpi bgdpi arf rmf 1 X100120.70+555355.8 chandra ccd7 843.927 565.764 268.632 16.6631 0.0863576 0.00535671 64.3215 1 0.409231 0.409231 0 0.309622 F F 9.29e+19 6.41799e-13 1 dsx
Report srcpi bgdpi arf 3 X100142.23+555218.6 chandra ccd7 475.125 368 7.80281 2.82843 0.00250837 0.000909258 1.86831 0.967205 0.554582 0.492 147.16 3.61083 F F 9.28e+19 1.92093e-14 1 dx
Report srcpi bgdpi arf 2 X100147.10+555040.0 chandra ccd7 391.5 167.625 7.74015 2.82843 0.00248823 0.000909258 1.85331 0.967205 0.715957 0.492 145.798 5.05745 F F 9.27e+19 1.95001e-14 1 dx
Report srcpi bgdpi arf 1 X100103.50+555320.8 chandra ccd6 142.5 87.1667 2.97695 1.73205 0.000957001 0.000556804 5.53371 0.999768 0.492 0.492 90 2.18124 F F 9.29e+19 1.81438e-14 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