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 | X163227.00+052029.5 | chandra | ccd0 | 991.087 | 395.158 | 122.837 | 11.1457 | 0.0246381 | 0.00223556 | 193.485 | 1 | 0.940622 | 0.573957 | 351.086 | 4.18599 | F | F | 5.55e+20 | 3.04104e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 3 | X163223.45+052546.0 | chandra | ccd2 | 233.924 | 509.566 | 114.659 | 10.7079 | 0.0229974 | 0.00214771 | 74.9816 | 1 | 1.29243 | 1.29243 | 0 | 4.99266 | F | F | 5.59e+20 | 4.50896e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X163155.85+052803.3 | chandra | ccd2 | 1071.6 | 788.558 | 25.3571 | 5.68965 | 0.00508593 | 0.00114119 | 16.5823 | 1 | 1.59844 | 1.59844 | 0 | 7.28074 | F | F | 5.51e+20 | 7.30573e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X163202.53+052751.1 | chandra | ccd2 | 868.188 | 763.188 | 15.3136 | 4.00001 | 0.0030715 | 0.000802293 | 10.0144 | 1 | 1.51411 | 0.91083 | 26.3859 | 6.37674 | A | F | 5.54e+20 | 4.21225e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X163213.28+051927.1 | chandra | ccd1 | 844.383 | 1137.31 | 13.4431 | 3.66648 | 0.00269636 | 0.000735408 | 23.588 | 1 | 0.422117 | 0.422117 | 0 | 2.44887 | F | F | 5.48e+20 | 3.14539e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X163206.32+052411.5 | chandra | ccd2 | 753.744 | 317.421 | 11.8786 | 3.44653 | 0.00238252 | 0.00069128 | 7.76805 | 1 | 0.659234 | 0.659234 | 0 | 2.63419 | F | F | 5.51e+20 | 2.81483e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X163222.04+052231.6 | chandra | ccd0 | 1141.49 | 643.313 | 11.3735 | 3.3777 | 0.00228126 | 0.000677486 | 17.9148 | 1 | 0.653133 | 0.653133 | 0 | 2.81604 | F | F | 5.55e+20 | 2.65212e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X163225.19+051440.0 | chandra | ccd1 | 482.409 | 553.318 | 10.5568 | 3.31663 | 0.00211742 | 0.000665232 | 18.5235 | 1 | 1.0253 | 0.492799 | 73.4647 | 7.98715 | A | F | 5.48e+20 | 2.83791e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X163144.09+052110.9 | chandra | ccd3 | 879.056 | 834.833 | 8.65745 | 3.00001 | 0.0017386 | 0.000602464 | 15.1156 | 1 | 1.25027 | 0.943978 | 128.642 | 6.74835 | F | F | 5.39e+20 | 2.32267e-14 | 1 | dx | ||||
| Report | 2 | X163150.96+052323.1 | chandra | ccd3 | 670.625 | 1103.62 | 7.89773 | 2.82843 | 0.00158603 | 0.000568007 | 13.7891 | 1 | 0.644581 | 0.492 | 65.8168 | 5.24058 | F | F | 5.44e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 6 | X163140.36+052247.5 | chandra | ccd3 | 992.125 | 1031.25 | 7.77193 | 2.82843 | 0.00156077 | 0.000568008 | 13.5695 | 1 | 1.12864 | 0.492 | 106.752 | 7.70264 | A | F | 5.4e+20 | 2.1911e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X163148.29+051930.1 | chandra | ccd3 | 751.5 | 629.928 | 6.77525 | 2.64576 | 0.00136061 | 0.000531323 | 11.8293 | 1 | 0.954703 | 0.572612 | 44.7272 | 6.13324 | A | F | 5.39e+20 | 1.82698e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X163237.77+051715.3 | chandra | ccd1 | 100.5 | 869 | 5.61128 | 2.4495 | 0.00112548 | 0.000491307 | 9.84586 | 0.999999 | 1.08516 | 0.595184 | 138.563 | 8.07353 | A | F | 5.55e+20 | 1.50108e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X163143.80+052046.4 | chandra | ccd3 | 887.833 | 785.167 | 5.59796 | 2.4495 | 0.00112419 | 0.000491911 | 9.77382 | 0.999999 | 1.34657 | 0.492 | 95.1284 | 6.87121 | A | F | 5.39e+20 | 1.50278e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X163156.59+051806.6 | chandra | ccd3 | 499.75 | 460.25 | 3.94479 | 2 | 0.000792195 | 0.000401642 | 6.88745 | 0.999976 | 0.740365 | 0.492 | 72.3444 | 5.18729 | A | F | 5.4e+20 | 9.69839e-15 | 1 | dx | ||||
| Report | 2 | X163222.26+051713.5 | chandra | ccd1 | 571.5 | 865.25 | 3.90945 | 2 | 0.000784135 | 0.000401149 | 6.85973 | 0.999977 | 0.705181 | 0.492 | 65.078 | 5.38926 | F | F | 5.49e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X163218.06+052207.6 | chandra | ccd0 | 1262 | 594 | 1.97153 | 1.41421 | 0.000395442 | 0.000283657 | 3.10543 | 0.991909 | 0.492 | 0.492 | 45 | 1.76193 | F | F | 5.53e+20 | 4.77923e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X163224.23+052217.2 | chandra | ccd0 | 1074.5 | 613.667 | 5.88066 | 2.44949 | 0.00117952 | 0.000491309 | 9.26283 | 1 | 0.640291 | 0.492 | 3.75607 | 3.30643 | F | F | 5.56e+20 | 1.38408e-14 | 1 | dx | ||||
| Report | 5 | X163219.42+052254.8 | chandra | ccd0 | 1220.5 | 690 | 7.85263 | 2.82843 | 0.00157505 | 0.000567315 | 12.3689 | 1 | 0.655164 | 0.492 | 114.699 | 2.33985 | F | F | 5.55e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 6 | X163230.09+052407.2 | chandra | ccd0 | 896.75 | 837.25 | 3.90941 | 2 | 0.000784133 | 0.000401153 | 6.15784 | 0.999937 | 0.609238 | 0.492 | 7.01812 | 5.25466 | F | F | 5.6e+20 | 1.05787e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X163238.46+052214.0 | chandra | ccd0 | 642.833 | 607.167 | 5.32483 | 2.44951 | 0.00106803 | 0.000491312 | 8.38733 | 0.999996 | 1.19299 | 0.975721 | 66.1987 | 6.827 | F | F | 5.6e+20 | 1.38059e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X163230.02+051946.7 | chandra | ccd0 | 899.218 | 308.212 | 23.5292 | 4.85069 | 0.00471939 | 0.000972931 | 37.0617 | 1 | 0.943651 | 0.943651 | 0 | 5.14559 | F | F | 5.55e+20 | 6.22284e-14 | 1 | dsx |
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