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Building unbiased estimators from non-Gaussian likelihoods with application to shear estimation

  • Mathew S. Madhavacheril
  • , Patrick McDonald
  • , Neelima Sehgal
  • , Anže Slosar
  • Stony Brook University
  • Lawrence Berkeley National Laboratory
  • Brookhaven National Laboratory

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

Abstract

We develop a general framework for generating estimators of a given quantity which are unbiased to a given order in the difference between the true value of the underlying quantity and the fiducial position in theory space around which we expand the likelihood. We apply this formalism to rederive the optimal quadratic estimator and show how the replacement of the second derivative matrix with the Fisher matrix is a generic way of creating an unbiased estimator (assuming choice of the fiducial model is independent of data). Next we apply the approach to estimation of shear lensing, closely following the work of Bernstein and Armstrong (2014). Our first order estimator reduces to their estimator in the limit of zero shear, but it also naturally allows for the case of non-constant shear and the easy calculation of correlation functions or power spectra using standard methods. Both our first-order estimator and Bernstein and Armstrong's estimator exhibit a bias which is quadratic in true shear. Our third-order estimator is, at least in the realm of the toy problem of Bernstein and Armstrong, unbiased to 0.1% in relative shear errors Δg/g for shears up to |g|=0.2.

Original languageEnglish
Article number022
JournalJournal of Cosmology and Astroparticle Physics
Volume2015
Issue number1
DOIs
StatePublished - Jan 1 2015

Keywords

  • gravitational lensing
  • weak gravitational lensing

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