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 | 1 | X140327.44+292556.6 | chandra | ccd7 | 1012.44 | 889.443 | 50.415 | 7.42129 | 0.0120388 | 0.00177216 | 31.1849 | 1 | 1.69934 | 1.69934 | 0 | 6.15617 | F | F | 1.25e+20 | 0 | 1 | ds | |||||
Report | 2 | X140345.04+292143.8 | chandra | ccd7 | 545.273 | 375.555 | 21.3218 | 5.26034 | 0.00509152 | 0.00125614 | 13.1889 | 1 | 0.445985 | 0.445985 | 0 | 0.568148 | F | F | 1.27e+20 | 0 | 1 | ds | |||||
Report | 4 | X140343.71+292320.4 | chandra | ccd7 | 580.527 | 571.905 | 12.4233 | 3.54031 | 0.0029666 | 0.000845404 | 7.6846 | 1 | 0.826071 | 0.826071 | 0 | 2.20223 | F | F | 1.27e+20 | 0 | 1 | ds | |||||
Report | 5 | X140355.43+292045.3 | chandra | ccd7 | 268.5 | 256.1 | 4.78474 | 2.23607 | 0.00114257 | 0.000533961 | 2.95966 | 0.994504 | 0.58188 | 0.492 | 12.222 | 2.25553 | F | F | 1.28e+20 | 0 | 1 | d | |||||
Report | 6 | X140357.20+292152.2 | chandra | ccd7 | 221.625 | 392.125 | 7.71936 | 2.82843 | 0.00184334 | 0.000675413 | 4.77491 | 0.999909 | 0.82103 | 0.492 | 61.7298 | 2.6966 | A | F | 1.28e+20 | 0 | 1 | d | |||||
Report | 7 | X140400.24+292414.6 | chandra | ccd7 | 141.525 | 682.047 | 17.1397 | 4.14001 | 0.00409285 | 0.000988609 | 10.602 | 1 | 0.984509 | 0.984509 | 0 | 4.4885 | F | F | 1.28e+20 | 0 | 1 | ds | |||||
Report | 8 | X140348.66+292046.9 | chandra | ccd7 | 448.903 | 259.909 | 20.8361 | 4.7732 | 0.00497555 | 0.00113981 | 12.8884 | 1 | 0.42569 | 0.42569 | 0 | 0.836677 | F | F | 1.28e+20 | 0 | 1 | ds |
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