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 | X013809.13+661356.1 | chandra | ccd2 | 695.365 | 1118.85 | 29.6253 | 6.08286 | 0.00595342 | 0.0012224 | 47.6107 | 1 | 4.86725 | 4.29351 | 144.859 | 11.9465 | F | F | 5.07e+21 | 9.61367e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X013741.73+661243.1 | chandra | ccd2 | 1031.12 | 968.017 | 25.2895 | 5.38521 | 0.00508212 | 0.0010822 | 40.6427 | 1 | 3.19964 | 2.80488 | 99.9972 | 9.01769 | F | F | 5.12e+21 | 7.40529e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X013758.31+660133.4 | chandra | ccd3 | 361.714 | 549.286 | 9.98174 | 3.74174 | 0.0020059 | 0.00075193 | 15.9913 | 1 | 4.11966 | 1.81765 | 75.9646 | 14.5529 | A | F | 5.28e+21 | 3.21792e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X013632.82+660924.5 | chandra | ccd7 | 322 | 717.4 | 9.64519 | 3.16228 | 0.00193827 | 0.000635484 | 9.79592 | 1 | 0.772785 | 0.492 | 32.9884 | 2.86849 | A | F | 5.24e+21 | 1.92371e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X013710.70+661649.7 | chandra | ccd6 | 301.611 | 684.389 | 7.97502 | 3.00002 | 0.00160264 | 0.000602876 | 12.5399 | 1 | 1.35734 | 0.758223 | 55.4915 | 7.88433 | A | F | 5.08e+21 | 2.17653e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X013644.59+661301.6 | chandra | ccd6 | 620.833 | 219.833 | 5.90232 | 2.44949 | 0.00118611 | 0.000492243 | 9.28081 | 1 | 0.538108 | 0.492 | 158.745 | 3.52488 | F | F | 5.17e+21 | 1.44801e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X013621.25+660928.6 | chandra | ccd7 | 464.667 | 725.667 | 5.86012 | 2.44949 | 0.00117763 | 0.000492244 | 5.9517 | 0.999931 | 0.492 | 0.492 | 31.2236 | 2.16278 | F | F | 5.25e+21 | 1.15075e-14 | 1 | dx | ||||
| Report | 2 | X013646.62+660138.6 | chandra | ccd3 | 1249.83 | 555.833 | 5.32963 | 2.44951 | 0.00107103 | 0.000492247 | 8.53835 | 0.999997 | 0.492 | 0.492 | 45 | 10.4031 | F | F | 5.35e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X013609.99+661157.5 | chandra | ccd7 | 603.3 | 1028.3 | 4.8695 | 2.23607 | 0.000978562 | 0.000449355 | 4.9456 | 0.999494 | 0.492 | 0.492 | 95.655 | 0.576533 | F | F | 5.22e+21 | 9.60386e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X013711.68+661538.7 | chandra | ccd6 | 289.1 | 540.3 | 4.62747 | 2.23608 | 0.000929925 | 0.000449356 | 7.27624 | 0.999996 | 0.692098 | 0.492 | 170.783 | 7.21771 | F | F | 5.1e+21 | 1.25864e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X013607.13+661605.7 | chandra | ccd6 | 1081.25 | 593.75 | 3.95941 | 2 | 0.000795672 | 0.000401915 | 6.22578 | 0.999936 | 0.492 | 0.492 | 45 | 4.65454 | F | T | 5.15e+21 | 1.04166e-14 | 1 | dx | ||||
| Report | 4 | X013622.83+661722.7 | chandra | ccd6 | 888.75 | 750.25 | 3.87967 | 2 | 0.000779648 | 0.000401915 | 6.10039 | 0.999936 | 1.05433 | 0.492 | 105.767 | 5.97703 | A | F | 5.12e+21 | 0 | 1 | d | |||||
| Report | 6 | X013605.11+661519.8 | chandra | ccd6 | 1106.17 | 500.5 | 2.96198 | 1.73205 | 0.000595231 | 0.000348069 | 4.65742 | 0.999191 | 0.492 | 0.492 | 180 | 3.93484 | F | F | 5.17e+21 | 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