Nuisance parameter

Results: 21



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1Properties of Doubly Robust Estimators when Nuisance Functions are Estimated Nonparametrically Christoph Rothe and Sergio Firpo Abstract An estimator of a finite-dimensional parameter is said to be doubly robust (DR)

Properties of Doubly Robust Estimators when Nuisance Functions are Estimated Nonparametrically Christoph Rothe and Sergio Firpo Abstract An estimator of a finite-dimensional parameter is said to be doubly robust (DR)

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Source URL: www.christophrothe.net

Language: English - Date: 2018-01-18 06:11:41
    2Testing Spatial Dependence When a Nuisance Parameter is not Identified Under the Null Hypothesis Sheena Kao and Anil K. Bera  Department of Economics, University of Illinois at Urbana-Champaign

    Testing Spatial Dependence When a Nuisance Parameter is not Identified Under the Null Hypothesis Sheena Kao and Anil K. Bera Department of Economics, University of Illinois at Urbana-Champaign

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    Source URL: www.real.illinois.edu

    Language: English - Date: 2014-12-11 08:33:04
      3Introduction to Confidence Intervals and Limit Setting via APEX Center for Cosmology and

      Introduction to Confidence Intervals and Limit Setting via APEX Center for Cosmology and

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      Source URL: hallaweb.jlab.org

      Language: English - Date: 2010-12-08 12:58:19
      4Some Problems Connected with Statistical Inference D. R. Cox The Annals of Mathematical Statistics, Vol. 29, No. 2. (Jun., 1958), ppStable URL: http://links.jstor.org/sici?sici=%%2929%3A2%3C35

      Some Problems Connected with Statistical Inference D. R. Cox The Annals of Mathematical Statistics, Vol. 29, No. 2. (Jun., 1958), ppStable URL: http://links.jstor.org/sici?sici=%%2929%3A2%3C35

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      Source URL: www.phil.vt.edu

      Language: English - Date: 2011-03-10 20:01:08
      5The Return of the Prodigal: Bayesian Inference For Astrophysics Thomas J. Loredo Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, New York 14853

      The Return of the Prodigal: Bayesian Inference For Astrophysics Thomas J. Loredo Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, New York 14853

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      Source URL: www.astro.cornell.edu

      Language: English - Date: 2010-05-17 14:20:55
      6Draft version March 26, 2015 Preprint typeset using LATEX style emulateapj vESTIMATING THE GALACTIC MASS PROFILE IN THE PRESENCE OF INCOMPLETE DATA Gwendolyn M. Eadie1 , William E. Harris1 , and Lawrence M. Widr

      Draft version March 26, 2015 Preprint typeset using LATEX style emulateapj vESTIMATING THE GALACTIC MASS PROFILE IN THE PRESENCE OF INCOMPLETE DATA Gwendolyn M. Eadie1 , William E. Harris1 , and Lawrence M. Widr

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      Source URL: lanl.arxiv.org

      Language: English - Date: 2015-03-26 00:39:45
      7Why Try Bayesian Methods? (Lecture 5) Tom Loredo Dept. of Astronomy, Cornell University  http://www.astro.cornell.edu/staff/loredo/bayes/

      Why Try Bayesian Methods? (Lecture 5) Tom Loredo Dept. of Astronomy, Cornell University http://www.astro.cornell.edu/staff/loredo/bayes/

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      Source URL: www.astro.cornell.edu

      Language: English - Date: 2002-10-18 06:37:39
      8

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      Source URL: www.spatial-statistics.com

      Language: English - Date: 2000-10-13 17:24:39
      9

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      Source URL: www.astro.cornell.edu

      Language: English - Date: 2010-05-17 14:22:44
      10Hypothesis testing when a nuisance parameter is present only under the alternative - linear model case

      Hypothesis testing when a nuisance parameter is present only under the alternative - linear model case

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      Source URL: www.robertnz.net

      Language: English - Date: 2010-02-24 03:24:45