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 | 1 | X142652.26+380248.3 | chandra | ccd0 | 530.745 | 625.339 | 43.789 | 6.61921 | 0.00877713 | 0.00132676 | 73.0894 | 1 | 2.72013 | 2.72013 | 0 | 7.77421 | 29.3226 | 9.88323 | -0.495829 | 0.215157 | F | F | 1.12e+20 | 1.23274e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X142530.00+380826.4 | chandra | ccd3 | 1106.93 | 837.433 | 28.5191 | 6.54527 | 0.00571265 | 0.00131108 | 23.435 | 1 | 3.03007 | 1.65618 | 106.396 | 9.38314 | 19.676 | 8.88929 | -0.377617 | 0.245767 | A | F | 1.1e+20 | 9.13426e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X142609.02+375935.6 | chandra | ccd1 | 619.189 | 697.947 | 28.3029 | 5.32005 | 0.00567651 | 0.001067 | 45.0705 | 1 | 2.2004 | 0.860524 | 106.283 | 6.26465 | 17.9338 | 7.27152 | -0.423016 | 0.266917 | A | F | 1.1e+20 | 7.91659e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X142615.74+375734.6 | chandra | ccd1 | 457.222 | 451.556 | 17.3593 | 5.33013 | 0.00348163 | 0.00106902 | 21.6881 | 1 | 1.72719 | 0.816765 | 58.9567 | 8.14626 | 10.7998 | 6.59959 | -0.2414 | 0.31684 | A | F | 1.09e+20 | 4.84497e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X142546.01+380923.4 | chandra | ccd3 | 722.875 | 952.625 | 8.62627 | 4.1225 | 0.00172793 | 0.000825778 | 14.1105 | 1 | 1.50136 | 0.828339 | 154.913 | 6.88854 | 5.81313 | 2.81313 | -0.347775 | 0.510859 | A | F | 1.11e+20 | 2.44965e-14 | 1 | dx |
| Report | 2 | X142626.90+380833.1 | chandra | ccd2 | 662.643 | 404.071 | 6.91874 | 2.64575 | 0.0013859 | 0.000529975 | 11.6028 | 1 | 0.547008 | 0.492 | 24.9495 | 3.58957 | F | F | 1.13e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X142616.92+380025.3 | chandra | ccd1 | 428.9 | 798.5 | 4.91531 | 3.39792 | 0.000985825 | 0.000681494 | 16.8899 | 1 | 0.492 | 0.492 | 129.345 | 5.30704 | 2.91531 | 2 | -0.186216 | 0.713849 | F | F | 1.1e+20 | 1.39889e-14 | 1 | dx |
| Report | 3 | X142613.75+380500.7 | chandra | ccd3 | 58 | 418.25 | 3.94348 | 2 | 0.000789918 | 0.00040062 | 6.29871 | 0.999944 | 0.492 | 0.492 | 37.9819 | 0.80517 | F | F | 1.11e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X142618.82+380039.0 | chandra | ccd1 | 383.25 | 826.25 | 3.92605 | 3.17945 | 0.000787418 | 0.000637678 | 14.4376 | 1 | 0.56384 | 0.492 | 165.321 | 5.11163 | 3 | 0.926053 | -0.528253 | 0.932192 | F | F | 1.1e+20 | 9.90549e-15 | 1 | dx |
| Report | 1 | X142617.52+381121.3 | chandra | ccd2 | 887.5 | 745.833 | 2.96325 | 1.73205 | 0.000593574 | 0.00034695 | 4.96941 | 0.999498 | 0.621484 | 0.492 | 165.695 | 5.64384 | F | F | 1.13e+20 | 0 | 1 | d | |||||
| Report | 2 | X142620.02+380148.3 | chandra | ccd1 | 354.5 | 967.167 | 2.95178 | 1.73205 | 0.000592016 | 0.000347384 | 4.70051 | 0.999263 | 0.627179 | 0.492 | 33.6901 | 4.01084 | F | F | 1.11e+20 | 0 | 1 | d | |||||
| Report | 2 | X142646.86+380545.2 | chandra | ccd0 | 660.5 | 984.167 | 2.75551 | 1.73206 | 0.000552312 | 0.000347173 | 4.59929 | 0.99948 | 0.492 | 0.492 | 108.435 | 6.1378 | F | F | 1.13e+20 | 0 | 1 | d |
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