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 X100120.67+555355.5 chandra ccd7 817.894 346.654 294.017 17.6647 0.0963173 0.0057868 73.861 1 0.381714 0.381714 0 0.381892 F F 9.29e+19 6.86386e-13 1 dsxf
Report srcpi bgdpi arf rmf 3 X100120.81+555349.5 chandra ccd7 815.431 334.377 292.311 17.4922 0.0957582 0.00573028 73.4325 1 0.410234 0.410234 0 0.29626 F F 9.29e+19 7.12109e-13 1 dsx
Report srcpi bgdpi arf 2 X100156.40+555440.3 chandra ccd7 206.808 437.808 12.6668 3.60556 0.00414949 0.00118114 3.18206 0.99809 1.1065 0.584742 92.1994 5.24614 A F 9.13e+19 3.27054e-14 1 dx
Report srcpi bgdpi arf 1 X100037.37+555054.7 chandra ccd6 621.5 488.5 1.93444 1.41422 0.000633701 0.000463282 4.13372 0.998513 0.825109 0.492 116.565 6.51788 A F 9.28e+19 7.94039e-15 1 dx
Report srcpi bgdpi arf 2 X100059.41+555140.1 chandra ccd6 244.1 580.1 4.95654 2.23607 0.00162371 0.000732511 10.5917 1 0.492 0.492 2.8553 3.43213 F F 9.28e+19 1.78239e-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