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 X011218.04+381857.0 chandra ccd7 766.084 166.177 1907.41 44.345 0.138065 0.00320984 423.788 1 0.397572 0.397572 0 0.590193 F T 5.54e+20 9.87299e-13 1 dsxf
Report srcpi bgdpi arf 2 X011231.73+381853.0 chandra ccd7 438.624 158.255 21.2773 4.61273 0.00154012 0.000333885 4.72739 0.999984 0.760184 0.760184 0 3.25569 F F 5.53e+20 1.14545e-14 1 dsx
Report srcpi bgdpi arf 4 X011208.12+381940.6 chandra ccd7 1002.86 254.5 9.62127 3.31666 0.000696419 0.000240071 2.13765 0.974765 0.762069 0.492 110.718 1.48819 A F 5.55e+20 5.01156e-15 1 dx
Report srcpi bgdpi arf 5 X011246.18+381800.5 chandra ccd7 92.7361 51.9121 14.3178 5.62889 0.00103637 0.000407438 3.18113 0.998173 1.5 1.20116 50.9089 6.18934 F F 5.51e+20 8.26394e-15 1 dsx
Report srcpi bgdpi arf 6 X011222.52+381844.1 chandra ccd7 658.894 140.062 20.244 4.98397 0.00146533 0.000360757 4.49781 0.999966 0.451903 0.451903 0 1.49269 F F 5.54e+20 1.06377e-14 1 dsx

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