Catalog-level blinding on the bispectrum for DESI-like galaxy surveys

Abstract We evaluate the performance of the catalog-level blind analysis technique ( blinding ) presented in Brieden et al. (2020) in the context of a fixed template power spectrum and bispectrum analysis. This blinding scheme, which is tailored for galaxy redshift surveys similar to the Dark Energy Spectroscopic Instrument (DESI), has two components: the so-called “AP blinding” (concerning the dilation parameters α ∥ , α ⊥ ) and “RSD blinding” (redshift space distortions, affecting the growth rate parameter f ). Through extensive testing, including checks for the RSD part in cubic boxes, the impact of AP blinding on mocks with realistic survey sky coverage, and the implementation of a full AP+RSD blinding pipeline, our analysis demonstrates the effectiveness of the technique in preserving the integrity of cosmological parameter estimation when the analysis includes the bispectrum statistic. We emphasize the critical role of sophisticated — and difficult to accidentally unblind — blinding methods in precision cosmology.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2024-10-01
DOI
https://doi.org/10.1088/1475-7516/2024/10/089
Citations
3
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
0.99

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article

Catalog-level blinding on the bispectrum for DESI-like galaxy surveys

Andrew Lambert, D. Brooks, G. Niz, Graziano Rossi et al.
3 citations
Journal of Cosmology and Astroparticle Physics
Galaxies: Formation, Evolution, Phenomena
0.99
article

Catalog-level blinding on the bispectrum for DESI-like galaxy surveys

Andrew Lambert, D. Brooks, G. Niz, Graziano Rossi, Gregory Tarlé, José Edgar Madriz Aguilar, Benjamin Alan Weaver, David Sprayberry, Licia Verde, Axel de la Macorra, Héctor Gil-Marín, T. Kisner, M. E. Levi, S. Brieden, Marc Manera, Eusebio Sanchez, Satya Gontcho A Gontcho, Sergi Novell-Masot, ENRIQUE GAZTAÑAGA, G. Gutierrez, Cullan Howlett, J. E. Forero-Romero, Steven P. Ahlen, Aaron Meisner, R. Miquel, M. Schubnell, R. Kehoe, Hee‐Jong Seo, K. Honscheid, T. Claybaugh, F. Prada
article en
3 citations

Abstract

Abstract We evaluate the performance of the catalog-level blind analysis technique ( blinding ) presented in Brieden et al. (2020) in the context of a fixed template power spectrum and bispectrum analysis. This blinding scheme, which is tailored for galaxy redshift surveys similar to the Dark Energy Spectroscopic Instrument (DESI), has two components: the so-called “AP blinding” (concerning the dilation parameters α ∥ , α ⊥ ) and “RSD blinding” (redshift space distortions, affecting the growth rate parameter f ). Through extensive testing, including checks for the RSD part in cubic boxes, the impact of AP blinding on mocks with realistic survey sky coverage, and the implementation of a full AP+RSD blinding pipeline, our analysis demonstrates the effectiveness of the technique in preserving the integrity of cosmological parameter estimation when the analysis includes the bispectrum statistic. We emphasize the critical role of sophisticated — and difficult to accidentally unblind — blinding methods in precision cosmology.

Journal of Cosmology and Astroparticle PhysicsVol. 2024(10)
Boston University (US), Institució Catalana de Recerca i Estudis Avançats (ES), Universitat Autònoma de Barcelona (ES), Universidad de Guanajuato (MX), Fermi National Accelerator Laboratory (US), The University of Queensland (AU), Southern Methodist University (US), Institute for High Energy Physics (ES), University of Michigan (US), Sejong University (KR), National Solar Observatory (US), Institut d'Estudis Espacials de Catalunya (ES), Institut Català de Ciències del Clima (ES), Centre for Theoretical Physics and Astrophysics (UZ), Michigan United (US), Unidades Centrales Científico-Técnicas (ES), Institut Cartogràfic i Geològic de Catalunya (ES), Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (ES), State Library of Ohio (US), University College London (GB), University of Portsmouth (GB), Universidad Nacional Autónoma de México (MX), Netherlands Institute for Radio Astronomy (NL)
National Science Foundation, U.S. Department of Energy, Gordon and Betty Moore Foundation, European Commission, Ministerio de Ciencia e Innovación, Universitat de Barcelona, Office of Science, Science and Technology Facilities Council, Agencia Estatal de Investigación, Institut de Ciències del Cosmos, Division of Astronomical Sciences
Openalex Percentile: Top 23%
Galaxies: Formation, Evolution, Phenomena
0.99
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