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Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis

Author(s): Ferrero, I. ; Crocce, M. ; Tutusaus, I. ; Porredon, A. ; Blot, L. ; Fosalba, P. ; Carnero Rosell, A. ; Avila, S. ; Izard, A. ; Elvin-Poole, J. ; Chan, K. C. ; Camacho, H. [UNESP] ; Rosenfeld, R. ; Sanchez, E. ; Tallada-Crespí, P. ; Carretero, J. ; Sevilla-Noarbe, I. ; Gaztanaga, E. ; Andrade-Oliveira, F. [UNESP] ; De Vicente, J. ; Mena-Fernández, J. ; Ross, A. J. ; Sanchez Cid, D. ; Ferté, A. ; Brandao-Souza, A. ; Fang, X. ; Krause, E. ; Gomes, D. ; Aguena, M. ; Allam, S. ; Annis, J. ; Bertin, E. ; Brooks, D. ; Carrasco Kind, M. ; Castander, F. J. ; Cawthon, R. ; Choi, A. ; Conselice, C. ; Costanzi, M. ; Da Costa, L. N. ; Pereira, M. E.S. ; Diehl, H. T. ; Doel, P. ; Drlica-Wagner, A. ; Everett, S. ; Evrard, A. E. ; Flaugher, B. ; Frieman, J. ; García-Bellido, J. ; Gerdes, D. W. ; Gruen, D. ; Gruendl, R. A. ; Gschwend, J. ; Gutierrez, G. ; Hinton, S. R. ; Hollowood, D. L. ; Honscheid, K. ; Hoyle, B. ; Huterer, D. ; James, D. J. ; Kuehn, K. ; Lima, M. ; Maia, M. A.G. ; Marshall, J. L. ; Menanteau, F. ; Miquel, R. ; Morgan, R. ; Muir, J. ; Ogando, R. L.C. ; Palmese, A. ; Paz-Chinchón, F. ; Percival, W. J. ; Plazas Malagón, A. A. ; Rodriguez-Monroy, M. ; Scarpine, V. ; Schubnell, M. ; Serrano, S. ; Smith, M. ; Soares-Santos, M. ; Suchyta, E. ; Swanson, M. E.C. ; Tarle, G. ; Thomas, D. ; To, C. ; Tucker, D. L. ; Varga, T. N.

Date: 2022

Persistent ID: http://hdl.handle.net/11449/230060

Origin: Oasisbr

Subject(s): Catalogs; Galaxies: distances and redshifts; Galaxy: halo; Large-scale structure of Universe; Methods: numerical


Description

Made available in DSpace on 2022-04-29T08:37:23Z (GMT). No. of bitstreams: 0 Previous issue date: 2021-12-01

The calibration and validation of scientific analysis in simulations is a fundamental tool to ensure unbiased and robust results in observational cosmology. In particular, mock galaxy catalogs are a crucial resource to achieve these goals in the measurement of baryon acoustic oscillation (BAO) in the clustering of galaxies. Here we present a set of 1952 galaxy mock catalogs designed to mimic the Dark Energy Survey Year 3 BAO sample over its full photometric redshift range 0:6 < zphoto < 1:1. The mocks are based upon 488 ICE-COLA fast N-body simulations of full-sky light cones and were created by populating halos with galaxies, using a hybrid halo occupation distribution halo abundance matching model. This model has ten free parameters, which were determined, for the first time, using an automatic likelihood minimization procedure.We also introduced a novel technique to assign photometric redshift for simulated galaxies, following a two-dimensional probability distribution with VIMOS Public Extragalactic Redshift Survey data. The calibration was designed to match the observed abundance of galaxies as a function of photometric redshift, the distribution of photometric redshift errors, and the clustering amplitude on scales smaller than those used for BAO measurements. An exhaustive analysis was done to ensure that the mocks reproduce the input properties. Finally, mocks were tested by comparing the angular correlation function w(θ), angular power spectrum ζp(rΓ) and projected clustering p(r?) to theoretical predictions and data. The impact of volume replication in the estimate of the covariance is also investigated. The success in accurately reproducing the photometric redshift uncertainties and the galaxy clustering as a function of redshift render this mock creation pipeline as a benchmark for future analyses of photometric galaxy surveys.

Institute of Theoretical Astrophysics University of Oslo, PO Box 1029, Blindern

Institut d'Estudis Espacials de Catalunya (IEEC)

Institute of Space Sciences (ICE CSIC) Campus UAB, Carrer de Can Magrans, s/n

Center for Cosmology and Astro-Particle Physics The Ohio State University

Department of Physics The Ohio State University

Max-Planck-Institut für Astrophysik, Karl-Schwarzschild Str. 1

Instituto de Astrofisica de Canarias, Tenerife

Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, RJ

Universidad de La Laguna Dpto. Astrofísica, Tenerife

Instituto de Fisica Teorica UAM/CSIC Universidad Autonoma de Madrid

Institute of Cosmology and Gravitation University of Portsmouth, Dennis Sciama Building, Burnaby Road

School of Physics and Astronomy Sun Yat-sen University, 2 Daxue Road, Tangjia

Instituto de Física Teórica Universidade Estadual Paulista

ICTP South American Institute for Fundamental Research

Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)

Port d'Informació Científica (PIC) Campus UAB, C. Albareda s/n, Bellaterra

Institut de Física d'Altes Energies (IFAE) The Barcelona Institute of Science and Technology Campus UAB, Bellaterra

Jet Propulsion Laboratory California Institute of Technology, 4800 Oak Grove Dr.

Instituto de Física Gleb Wataghin Universidade Estadual de Campinas, SP

Department of Astronomy/Steward Observatory University of Arizona, 933 North Cherry Avenue

Departamento de Física Matemática Instituto de Física Universidade de São Paulo, CP 66318, SP

Laboratório Interinstitucional de e-Astronomia Rua General José Cristino, 77, São Cristóvão, RJ

Fermi National Accelerator Laboratory, PO Box 500

CNRS UMR 7095 Institut d'Astrophysique de Paris

Sorbonne Universités UPMC Univ. Paris 06 UMR 7095 Institut d'Astrophysique de Paris

Department of Physics and Astronomy University College London, Gower Street

Center for Astrophysical Surveys National Center for Supercomputing Applications, 1205 West Clark St.

Department of Astronomy University of Illinois at Urbana-Champaign, 1002 W. Green Street

Physics Department University of Wisconsin-Madison, 2320 Chamberlin Hall, 1150 University Avenue Madison

Jodrell Bank Center for Astrophysics School of Physics and Astronomy University of Manchester, Oxford Road

University of Nottingham School of Physics and Astronomy

Astronomy Unit Department of Physics University of Trieste, Via Tiepolo 11

INAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11

Institute for Fundamental Physics of the Universe, Via Beirut 2

Observatório Nacional, Rua Gal. José Cristino 77, RJ

Department of Physics University of Michigan

Department of Astronomy and Astrophysics University of Chicago

Kavli Institute for Cosmological Physics University of Chicago

Santa Cruz Institute for Particle Physics

Department of Astronomy University of Michigan

Department of Physics Stanford University, 382 Via Pueblo Mall

Kavli Institute for Particle Astrophysics and Cosmology Stanford University, PO Box 2450

SLAC National Accelerator Laboratory

School of Mathematics and Physics University of Queensland

Faculty of Physics Ludwig-Maximilians-Universität, Scheinerstr. 1

Center for Astrophysics | Harvard and Smithsonian, 60 Garden Street

Australian Astronomical Optics Macquarie University

Lowell Observatory, 1400 Mars Hill Rd

George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy Department of Physics and Astronomy Texas AandM University

Institució Catalana de Recerca i Estudis Avançats

Institute of Astronomy University of Cambridge, Madingley Road

Department of Physics and Astronomy University of Waterloo, 200 University Ave W

Perimeter Institute for Theoretical Physics, 31 Caroline St. North

Department of Astrophysical Sciences Princeton University, Peyton Hall

School of Physics and Astronomy University of Southampton

Computer Science and Mathematics Division Oak Ridge National Laboratory

Institute of Cosmology and Gravitation University of Portsmouth

Max Planck Institute for Extraterrestrial Physics Giessenbachstrasse

Universitäts-Sternwarte Fakultät für Physik Ludwig-Maximilians Universität München, Scheinerstr. 1

Instituto de Física Teórica Universidade Estadual Paulista

Document Type Journal article
Language English
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