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 | X011925.86+142616.7 | chandra | ccd3 | 231.074 | 1074.99 | 118.219 | 11.943 | 0.0085563 | 0.000864395 | 133.797 | 1 | 1.96958 | 1.51331 | 177.432 | 9.9767 | 49.7398 | 67.4795 | 0.151338 | 0.10275 | F | F | 3.38e+20 | 2.0495e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X012002.62+142142.4 | chandra | ccd7 | 504.365 | 317.749 | 67.9238 | 10.328 | 0.00491499 | 0.000747335 | 16.8549 | 1 | 0.57391 | 0.57391 | 0 | 0.212881 | 53.3096 | 27.2313 | -0.323789 | 0.133372 | F | F | 3.36e+20 | 3.70062e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X012004.79+141308.3 | chandra | ccd6 | 717.532 | 280.258 | 56.0482 | 8.92149 | 0.00405566 | 0.000645561 | 22.974 | 1 | 3.38731 | 2.73688 | 137.476 | 8.41994 | 33.4949 | 23.1005 | -0.183661 | 0.160556 | F | F | 3.35e+20 | 5.3661e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 9 | X012010.98+141821.6 | chandra | ccd6 | 535.384 | 917.578 | 40.9676 | 6.40059 | 0.00296443 | 0.000463149 | 27.3947 | 1 | 1.25665 | 0.637032 | 95.1152 | 3.83294 | 32.7854 | 8.69953 | -0.580593 | 0.210651 | F | F | 3.35e+20 | 3.57988e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X011919.83+141323.8 | chandra | ccd2 | 679.305 | 510.134 | 29.5095 | 7.61438 | 0.00213532 | 0.000550978 | 8.0343 | 1 | 5.36688 | 4.4768 | 98.3468 | 13.0804 | 20.0335 | 9.6061 | -0.351806 | 0.270297 | F | F | 3.37e+20 | 3.23979e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 15 | X012005.36+142105.4 | chandra | ccd7 | 423.405 | 242.452 | 25.3955 | 5.48106 | 0.00183762 | 0.000396611 | 6.30173 | 1 | 0.614915 | 0.265427 | 115.252 | 0.903742 | 18.9269 | 5.89035 | -0.525302 | 0.277602 | F | F | 3.36e+20 | 1.39856e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X012002.33+142144.9 | chandra | ccd7 | 512.413 | 322.283 | 22.517 | 6.07445 | 0.00162934 | 0.000439548 | 14.2898 | 1 | 0.769768 | 0.492 | 70.0791 | 0.222183 | 18.3071 | 4.20997 | -0.626064 | 0.319567 | A | F | 3.36e+20 | 1.22674e-14 | 1 | dpx |
| Report | srcpi bgdpi arf | 10 | X012014.02+142516.4 | chandra | ccd7 | 167.808 | 752.747 | 15.4141 | 4.55469 | 0.00111537 | 0.000329578 | 3.82491 | 0.999645 | 1.55416 | 0.395339 | 120.759 | 4.7249 | 11.8492 | 1.43999 | -0.783284 | 0.465784 | A | F | 3.35e+20 | 1.20209e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 6 | X012020.64+141943.7 | chandra | ccd6 | 249.934 | 1084.55 | 25.8886 | 5.45869 | 0.00187331 | 0.000394993 | 17.3115 | 1 | 1.87684 | 0.711195 | 98.9727 | 4.83524 | 19.8396 | 9.64706 | -0.345666 | 0.235668 | F | F | 3.34e+20 | 2.40598e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X012008.24+141918.8 | chandra | ccd6 | 616.104 | 1033.86 | 9.54529 | 3.51364 | 0.0006907 | 0.000254248 | 6.38287 | 0.999996 | 0.434499 | 0.434499 | 0 | 2.6717 | 3 | 7.83025 | 0.445996 | 0.451325 | F | F | 3.35e+20 | 7.47353e-15 | 1 | dsx |
| Report | srcpi bgdpi arf | 14 | X011938.58+142608.3 | chandra | ccd7 | 1213.5 | 857.833 | 15.8118 | 5.21307 | 0.00114415 | 0.000377219 | 14.5056 | 1 | 1.4189 | 0.94818 | 51.0745 | 7.32507 | 10.7171 | 4.20787 | -0.43613 | 0.374483 | F | F | 3.38e+20 | 1.82036e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 6 | X011959.59+142419.4 | chandra | ccd7 | 593.1 | 636.2 | 9.91531 | 4.27872 | 0.000717474 | 0.000309609 | 34.0707 | 1 | 0.492 | 0.492 | 25.1715 | 2.85505 | 8 | 1.91531 | -0.613667 | 0.510787 | F | F | 3.36e+20 | 5.50996e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 11 | X012003.39+142712.9 | chandra | ccd7 | 480.9 | 988.8 | 11.5334 | 4.57071 | 0.000834561 | 0.000330738 | 16.8849 | 1 | 0.714426 | 0.492 | 132.618 | 5.68954 | 5.76671 | 3.82503 | -0.202432 | 0.459164 | F | F | 3.36e+20 | 6.71675e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X012006.30+141626.4 | chandra | ccd6 | 672.944 | 682.944 | 11.5712 | 4.57071 | 0.000837292 | 0.000330738 | 17.6698 | 1 | 1.07768 | 0.54564 | 167.815 | 5.19326 | 6.82847 | 4.7427 | -0.180256 | 0.404434 | A | F | 3.35e+20 | 1.07336e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X012010.24+142334.1 | chandra | ccd7 | 278.875 | 544.125 | 7.57653 | 3.95804 | 0.00054824 | 0.000286405 | 11.6429 | 1 | 0.492 | 0.492 | 7.85432 | 2.83139 | 4 | 3.57653 | -0.0558919 | 0.52877 | F | F | 3.35e+20 | 4.32426e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X011924.54+141142.7 | chandra | ccd2 | 540.879 | 305.199 | 13.1224 | 6.51283 | 0.00094954 | 0.00047127 | 2.42449 | 0.989644 | 3.77309 | 3.77309 | 0 | 13.365 | 13.4759 | 6.69773 | -0.335991 | 0.318935 | F | F | 3.37e+20 | 1.61831e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 5 | X012016.11+141908.7 | chandra | ccd6 | 383.333 | 1012.83 | 7.74592 | 3.95804 | 0.000560497 | 0.000286405 | 15.367 | 1 | 0.492 | 0.492 | 72.1618 | 4.14808 | 4.83061 | 2.91531 | -0.247267 | 0.531953 | F | F | 3.35e+20 | 6.35208e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X012008.62+141741.0 | chandra | ccd6 | 604.5 | 834.5 | 4.78578 | 3.39792 | 0.0003463 | 0.000245874 | 10.3401 | 1 | 0.777873 | 0.492 | 110.301 | 4.16094 | 3 | 1.78578 | -0.253714 | 0.743616 | A | F | 3.35e+20 | 3.93068e-15 | 1 | dx |
| Report | 7 | X012000.96+141421.4 | chandra | ccd6 | 830.833 | 428.833 | 2.7803 | 1.73206 | 0.000201183 | 0.000125332 | 1.85917 | 0.973318 | 0.678773 | 0.492 | 155.994 | 7.18173 | F | F | 3.35e+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