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 | X081422.12+514839.3 | chandra | ccd7 | 718.235 | 408.562 | 1094.53 | 33.7291 | 0.159866 | 0.00492645 | 166.674 | 1 | 0.436075 | 0.408731 | 147.085 | 0.585501 | F | F | 4.24e+20 | 1.11702e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 2 | X081414.07+513606.7 | chandra | ccd5 | 204.088 | 867.5 | 22.1306 | 6.08295 | 0.00323236 | 0.000888465 | 19.6016 | 1 | 2.28971 | 1.44181 | 146.798 | 12.0717 | A | F | 4.33e+20 | 2.65286e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X081356.57+513914.0 | chandra | ccd6 | 866.948 | 247.396 | 22.0512 | 5.38525 | 0.00322075 | 0.000786559 | 37.2031 | 1 | 3.50509 | 2.90327 | 100.237 | 9.63758 | F | F | 4.31e+20 | 3.57238e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X081346.26+514441.4 | chandra | ccd6 | 1060.72 | 913.109 | 21.6046 | 4.79585 | 0.00315553 | 0.000700473 | 36.4497 | 1 | 1.91273 | 1.28149 | 173.718 | 6.29294 | F | F | 4.27e+20 | 3.59171e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X081235.29+514556.9 | chandra | ccd2 | 1156.38 | 484.042 | 14.4611 | 4.89914 | 0.00211216 | 0.000715559 | 23.7817 | 1 | 4.89381 | 3.44117 | 62.0963 | 16.3805 | F | F | 4.26e+20 | 3.05196e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X081413.06+513554.0 | chandra | ccd5 | 223.184 | 841.658 | 13.4614 | 4.35899 | 0.00196615 | 0.000636666 | 11.9231 | 1 | 3.59624 | 2.5311 | 29.3336 | 12.2962 | F | F | 4.33e+20 | 1.6223e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X081354.35+514128.1 | chandra | ccd6 | 908.583 | 520 | 11.3538 | 3.46411 | 0.00165832 | 0.000505962 | 19.1553 | 1 | 1.72319 | 1.0557 | 108.636 | 7.78909 | A | F | 4.29e+20 | 1.77589e-14 | 1 | dx | ||||
| Report | 6 | X081427.58+514516.4 | chandra | ccd6 | 280.667 | 983.667 | 5.89892 | 2.44949 | 0.000861584 | 0.000357768 | 9.95222 | 1 | 0.663216 | 0.492 | 165.779 | 3.08858 | F | F | 4.27e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X081344.56+515411.3 | chandra | ccd3 | 148.333 | 480.667 | 5.55628 | 2.4495 | 0.000811539 | 0.000357769 | 9.15731 | 0.999997 | 1.29508 | 0.598005 | 172.185 | 8.17882 | A | F | 4.2e+20 | 1.04338e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X081415.60+514145.9 | chandra | ccd6 | 506.833 | 555.833 | 5.54045 | 2.4495 | 0.000809228 | 0.000357769 | 9.34744 | 0.999998 | 1.47784 | 0.531056 | 10.7314 | 6.42149 | A | F | 4.29e+20 | 8.33511e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X081312.50+514803.7 | chandra | ccd2 | 453.333 | 738.167 | 4.91294 | 2.44952 | 0.000717575 | 0.000357772 | 8.07947 | 0.999997 | 2.86217 | 1.68547 | 85.1989 | 10.4743 | A | F | 4.25e+20 | 9.12991e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X081316.47+514305.5 | chandra | ccd2 | 380.75 | 131.75 | 6.48074 | 2.82846 | 0.000946564 | 0.00041312 | 10.6578 | 1 | 2.72678 | 1.88219 | 144.97 | 11.0889 | F | F | 4.28e+20 | 1.29485e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X081425.88+514447.6 | chandra | ccd6 | 312.833 | 925.167 | 2.96078 | 1.73205 | 0.000432446 | 0.00025298 | 4.99522 | 0.99952 | 0.492 | 0.492 | 45 | 3.46362 | F | F | 4.27e+20 | 4.22663e-15 | 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