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 | 1 | X110950.83+564515.6 | chandra | ccd0 | 939.163 | 793.358 | 34.244 | 6.37539 | 0.00726332 | 0.00135225 | 13.5344 | 1 | 3.12736 | 2.9838 | 89.949 | 8.77646 | F | F | 7.35e+19 | 0 | 1 | ds | |||||
Report | 2 | X110954.45+564440.9 | chandra | ccd0 | 878.533 | 722.133 | 26.9863 | 5.47726 | 0.00572388 | 0.00116175 | 10.6659 | 1 | 2.35994 | 2.00629 | 13.3378 | 8.47101 | F | F | 7.34e+19 | 0 | 1 | d | |||||
Report | 2 | X111111.41+564048.8 | chandra | ccd2 | 648.333 | 322.833 | 11.2368 | 3.46411 | 0.00238493 | 0.000735233 | 19.2643 | 1 | 1.59864 | 0.715373 | 102.595 | 6.90781 | A | F | 7.34e+19 | 0 | 1 | d | |||||
Report | 1 | X111018.08+565439.3 | chandra | ccd1 | 556.326 | 909.713 | 12.0793 | 3.80151 | 0.00256208 | 0.000806321 | 7.84271 | 1 | 2.29359 | 2.29359 | 0 | 8.81473 | F | F | 7.51e+19 | 0 | 1 | ds | |||||
Report | 1 | X111059.43+565250.5 | chandra | ccd3 | 932.5 | 751.611 | 8.10525 | 3.00002 | 0.00171915 | 0.000636314 | 13.0816 | 1 | 0.825925 | 0.492 | 105.377 | 5.64273 | A | F | 7.49e+19 | 0 | 1 | d | |||||
Report | 3 | X111018.74+564633.3 | chandra | ccd0 | 471.875 | 949.5 | 7.8241 | 2.82843 | 0.00165952 | 0.000599919 | 3.09235 | 0.997429 | 0.71788 | 0.492 | 7.6691 | 4.79016 | F | F | 7.39e+19 | 0 | 1 | d | |||||
Report | 1 | X111143.79+564341.8 | chandra | ccd2 | 107 | 675.5 | 7.33383 | 2.82844 | 0.00155655 | 0.000600317 | 12.5731 | 1 | 1.2551 | 0.839892 | 150.29 | 7.78032 | F | F | 7.36e+19 | 0 | 1 | d | |||||
Report | 4 | X111040.19+564536.8 | chandra | ccd0 | 113.667 | 834.167 | 5.92159 | 2.44949 | 0.00125599 | 0.000519545 | 2.34041 | 0.985658 | 0.616392 | 0.492 | 157.754 | 2.44062 | F | F | 7.35e+19 | 0 | 1 | d | |||||
Report | 5 | X111107.97+564615.8 | chandra | ccd2 | 706.5 | 987.3 | 4.8975 | 2.23607 | 0.00103946 | 0.00047459 | 8.39623 | 0.999998 | 0.492 | 0.492 | 16.0027 | 2.23953 | F | F | 7.37e+19 | 0 | 1 | d | |||||
Report | 5 | X111029.46+564549.0 | chandra | ccd0 | 292.9 | 859.1 | 4.88305 | 2.23607 | 0.00103571 | 0.000474278 | 1.92995 | 0.969253 | 0.612253 | 0.492 | 165.595 | 3.57488 | F | F | 7.39e+19 | 0 | 1 | d | |||||
Report | 6 | X111015.46+564417.7 | chandra | ccd0 | 527.3 | 673.9 | 4.8996 | 2.23607 | 0.00103922 | 0.000474278 | 1.93649 | 0.969253 | 0.492 | 0.492 | 58.2825 | 5.97792 | F | F | 7.36e+19 | 0 | 1 | d | |||||
Report | 3 | X111109.74+564938.9 | chandra | ccd3 | 760.25 | 362.25 | 3.95444 | 2 | 0.00083875 | 0.000424207 | 6.38232 | 0.999949 | 0.492 | 0.492 | 18.4349 | 3.2776 | F | F | 7.39e+19 | 0 | 1 | d | |||||
Report | 3 | X111056.59+563920.2 | chandra | ccd2 | 896.5 | 142.5 | 3.87633 | 2 | 0.000822723 | 0.000424487 | 6.64554 | 0.999971 | 0.521845 | 0.492 | 45 | 7.93789 | F | F | 7.33e+19 | 0 | 1 | d | |||||
Report | 2 | X111116.95+565019.8 | chandra | ccd3 | 640.167 | 445.5 | 2.95411 | 1.73205 | 0.000626576 | 0.000367374 | 4.76783 | 0.999333 | 0.492 | 0.492 | 3.85109e-08 | 4.45642 | F | F | 7.39e+19 | 0 | 1 | d | |||||
Report | 4 | X111116.10+564536.9 | chandra | ccd2 | 570.5 | 908.5 | 2.94635 | 1.73205 | 0.000625342 | 0.000367616 | 5.0512 | 0.999574 | 0.624964 | 0.492 | 106.845 | 3.52677 | F | F | 7.37e+19 | 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