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In each 5 week collection period about 100 GPs each records information for approximately 30 consecutive patients for each topic, a completed sample of about 3000 patients per substudy.
We calculated that we needed a completed sample of 1300 participants to have 80% power at a significance level of 5% to detect differences of at most five points in these subscales between groups, provided that the mean correlation coefficient between operators was less than 0.02 (very likely according to our feasibility study).
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For the case of a complete sample of univariate predictors and responses, the modern nonparametric regression matches results known for parametric and semiparametric regressions.
What is needed, says Bahcall, is a complete sample of distant clusters for which masses are known exactly, for instance through gravitational-lens observations.
As previously explained, we restricted the sample to 124 observations (from a complete sample of 670 observations), although we will use the complete dataset to test the robustness of the results.
We have performed a spectral principal component analysis for a complete sample of 22 low redshift QSOs with spectra from Lyα to Hα, and found three significant principal components, which account for ∼78% of the spectrum-to-spectrum variance.
For this reason, we have selected a complete sample of 42 low redshift BL Lacs (independently of their gamma-ray properties) to study with a multi-wavelength (radio, optical, X-ray, gamma-ray) approach.
We are using this unique facility to observe a complete sample of Pearson-Readhead Survey sources (Pearson and Readhead 1988) at 4.8 GHz, to determine core brightness temperatures and pc-scale jet properties.
Let the order statistics for a complete sample of n observations be defined as X j : n where j = 1,2,3,… n, where X 1 : n ≤ X 2 : n ≤ … X n : n.
We show that, adopting our cross section database, we are able to provide a good fit of a complete sample of CR observables, including: leptonic and hadronic spectra measured at Earth, the local interstellar spectra measured by Voyager, and the gamma-ray emissivities from Fermi-LAT collaboration.
With a 1y/5σ survey sensitivity Fx (40 80 keV) ∼ 5 × 10−13 erg cm−2 s−1, comparable to the ROSAT soft X-ray (0.3 2.5 keV) sky survey, a large sample (≳2 4 × 104) of obscured AGN will be identified and a complete sample of accreting stellar mass BHs in the Galaxy will be found.
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