Document details

Dark Energy Survey Year 3 results: Marginalization over redshift distribution uncertainties using ranking of discrete realizations

Author(s): Cordero, Juan P. ; Harrison, Ian ; Rollins, Richard P. ; Bernstein, G. M. ; Bridle, S. L. ; Alarcon, A. ; Alves, O. [UNESP] ; Amon, A. ; Andrade-Oliveira, F. [UNESP] ; Camacho, H. [UNESP] ; Campos, A. ; Choi, A. ; Derose, J. ; Dodelson, S. ; Eckert, K. ; Eifler, T. F. ; Everett, S. ; Fang, X. ; Friedrich, O. ; Gruen, D. ; Gruendl, R. A. ; Hartley, W. G. ; Huff, E. M. ; Krause, E. ; Kuropatkin, N. ; MacCrann, N. ; McCullough, J. ; Myles, J. ; Pandey, S. ; Raveri, M. ; Rosenfeld, R. [UNESP] ; Rykoff, E. S. ; Sánchez, C. ; Sánchez, J. ; Sevilla-Noarbe, I. ; Sheldon, E. ; Troxel, M. ; Wechsler, R. ; Yanny, B. ; Yin, B. ; Zhang, Y. ; Aguena, M. ; Allam, S. ; Bertin, E. ; Brooks, D. ; Burke, D. L. ; Carnero Rosell, A. ; Carrasco Kind, M. ; Carretero, J. ; Castander, F. J. ; Cawthon, R. ; Costanzi, M. ; Da Costa, L. ; Da Silva Pereira, M. E. ; De Vicente, J. ; Diehl, H. T. ; Dietrich, J. ; Doel, P. ; Elvin-Poole, J. ; Ferrero, I. ; Flaugher, B. ; Fosalba, P. ; Frieman, J. ; Garcia-Bellido, J. ; Gerdes, D. ; Gschwend, J. ; Gutierrez, G. ; Hinton, S. ; Hollowood, D. L. ; Honscheid, K. ; Hoyle, B. ; James, D. ; Kuehn, K. ; Lahav, O. ; Maia, M. A.G. ; March, M. ; Menanteau, F. ; Miquel, R. ; Morgan, R. ; Muir, J. ; Palmese, A. ; Paz-Chinchon, F. ; Pieres, A. ; Plazas Malagón, A. ; Sánchez, E. ; Scarpine, V. ; Serrano, S. ; Smith, M. ; Soares-Santos, M. ; Suchyta, E. ; Swanson, M. ; Tarle, G. ; Thomas, D. ; To, C. ; Varga, T. N.

Date: 2022

Persistent ID: http://hdl.handle.net/11449/230478

Origin: Oasisbr

Subject(s): Galaxies: distances and redshifts; Gravitational lensing: weak; Large-scale structure of Universe; Methods: numerical


Description

Made available in DSpace on 2022-04-29T08:40:12Z (GMT). No. of bitstreams: 0 Previous issue date: 2022-04-01

Cosmological information from weak lensing surveys is maximized by sorting source galaxies into tomographic redshift subsamples. Any uncertainties on these redshift distributions must be correctly propagated into the cosmological results. We present hyperrank, a new method for marginalizing over redshift distribution uncertainties, using discrete samples from the space of all possible redshift distributions, improving over simple parametrized models. In hyperrank, the set of proposed redshift distributions is ranked according to a small (between one and four) number of summary values, which are then sampled, along with other nuisance parameters and cosmological parameters in the Monte Carlo chain used for inference. This approach can be regarded as a general method for marginalizing over discrete realizations of data vector variation with nuisance parameters, which can consequently be sampled separately from the main parameters of interest, allowing for increased computational efficiency. We focus on the case of weak lensing cosmic shear analyses and demonstrate our method using simulations made for the Dark Energy Survey (DES). We show that the method can correctly and efficiently marginalize over a wide range of models for the redshift distribution uncertainty. Finally, we compare hyperrank to the common mean-shifting method of marginalizing over redshift uncertainty, validating that this simpler model is sufficient for use in the DES Year 3 cosmology results presented in companion papers.

Jodrell Bank Centre for Astrophysics Department of Physics and Astronomy The University of Manchester

Department of Physics University of Oxford Denys Wilkinson Building, Keble Road

Institute for Astronomy University of Edinburgh

Department of Physics and Astronomy University of Pennsylvania

Argonne National Laboratory, 9700 South Cass Avenue

Institute of Space Sciences (ICE CSIC) Campus Uab Carrer de Can Magrans S/n

Institut d'Estudis Espacials de Catalunya (IEEC)

Department of Physics University of Michigan

Instituto de Física Teorica Universidade Estadual Paulista

Department of Physics Stanford University 382 Via Pueblo Mall

Kavli Institute for Particle Astrophysics &cosmology Stanford University, PO Box 2450

Slac National Accelerator Laboratory

Laboratorio Interinstitucional de E-Astronomia-LIneA, Rua Gal. Jose Cristino 77

Department of Physics Carnegie Mellon University

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

Santa Cruz Institute for Particle Physics

Department of Astronomy University of California Berkeley 501 Campbell Hall

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

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

Kavli Institute for Cosmology University of Cambridge, Madingley Road

Churchill College University of Cambridge

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

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

Departement de Physique Theorique Center for Astroparticle Physics Université de Geneve, 24 quai Ernest Ansermet

Fermi National Accelerator Laboratory, PO Box 500

Department of Applied Mathematics and Theoretical Physics University of Cambridge

Kavli Institute for Cosmological Physics University of Chicago

Ictp South American Institute for Fundamental Research Instituto de Física Teorica Universidade Estadual Paulista

Centro de Investigaciones Energeticas Medioambientales y Tecnologicas (CIEMAT)

Brookhaven National Laboratory Bldg 510

Department of Physics Duke University

Departamento de Física Matematica Instituto de Física Universidade de Sao Paulo, CP 66318, SP

Cnrs Umr 7095 Institut d'Astrophysique de Paris

Sorbonne Universites Upmc Univ Paris 06 Umr 7095 Institut d'Astrophysique de Paris

Department of Physics &astronomy University College London, Gower Street

Instituto de Astrofisica de Canarias, Tenerife

Universidad de la Laguna Dpto. Astrofísica, Tenerife

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

Physics Department 2320 Chamberlin Hall University of WisconsinMadison, 1150 University Avenue

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

Institute for Fundamental Physics of the Universe, Via Beirut 2

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

Department of Physics The Ohio State University

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

Instituto de Fisica Teorica UAM/CSIC Universidad Autonoma de Madrid

Department of Astronomy University of Michigan

School of Mathematics and Physics University of Queensland

Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse

Universitats-Sternwarte Fakultat fur Physik Ludwig-Maximilians Universitat Munchen, Scheinerstr. 1

Center for Astrophysics | Harvard &smithsonian, 60 Garden Street

Australian Astronomical Optics Macquarie University

Lowell Observatory, 1400 Mars Hill Rd

Institucio Catalana de Recerca i Estudis Avancats

Perimeter Institute for Theoretical Physics, 31 Caroline St. North

Institute of Astronomy University of Cambridge, Madingley Road

Observatorio Nacional, Rua Gal. José Cristino 77

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

Instituto de Física Teorica Universidade Estadual Paulista

Ictp South American Institute for Fundamental Research Instituto de Física Teorica Universidade Estadual Paulista

Document Type Journal article
Language English
facebook logo  linkedin logo  twitter logo 
mendeley logo

Related documents

No related documents