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 3 X145345.40+511111.0 chandra ccd7 682.343 105.985 143.436 11.9923 0.0930762 0.00778184 145.756 1 1.83987 1.01023 73.3953 5.27896 80.8605 57.7211 -0.166974 0.0938784 F F 1.89e+20 1.0718e-12 1 dsxf
Report srcpi bgdpi arf 1 X145353.56+511152.8 chandra ccd7 526.297 190.804 17.5162 4.18528 0.0113664 0.00271585 17.7995 1 1.12077 0.536786 94.3729 3.90022 13 2.95945 -0.629129 0.379252 F F 1.89e+20 9.18279e-14 1 dsx
Report srcpi bgdpi arf 2 X145408.99+511444.0 chandra ccd7 231.477 538.652 9.57431 3.47858 0.00621281 0.00225726 9.72916 1 0.271284 0.271284 0 0.168291 7 1.83008 -0.58549 0.546225 F F 1.91e+20 4.64918e-14 1 dsx
Report srcpi bgdpi arf 1 X145428.44+511824.4 chandra ccd6 908.333 924.167 6.88372 3.78388 0.00446699 0.00245544 20.1867 1 0.717482 0.492 18.0868 4.60743 5.94186 0.941858 -0.726352 0.687385 F F 1.93e+20 5.35318e-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