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pro vyhledávání: '"Large-Scale Structure of Universe [Cosmology]"'
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Autor:
Kyle, Dawson, Al., Yèche Christophe Et
Supplementary material to DESI's publication 'Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument'to comply with the data management plan.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f51b937da4435de44b428f0484108ab
Autor:
Tianyue Chen, Mathieu Remazeilles
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
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Residual foreground contamination by thermal Sunyaev–Zeldovich (tSZ) effect from galaxy clusters in cosmic microwave background (CMB) maps propagates into the reconstructed CMB lensing field, and thus biases the intrinsic cross-correlation between
Publikováno v:
Dakin, J, Hannestad, S & Tram, T 2022, ' The cosmological simulation code CONCEPT 1.0 ', Monthly Notices of the Royal Astronomical Society, vol. 513, no. 1, pp. 991-1014 . https://doi.org/10.1093/mnras/stac568
We present version 1.0 of the cosmological simulation code $\rm{{\small CO}{{\small N}}{\small CEPT}}$, designed for simulations of large-scale structure formation. $\rm{{\small CO}{\rm{\small N}}{\small CEPT}}$ 1.0 contains a P3M gravity solver, wit
Autor:
Steven Cunnington, Laura Wolz, Philip Bull, Isabella P Carucci, Keith Grainge, Melis O Irfan, Yichao Li, Alkistis Pourtsidou, Mario G Santos, Marta Spinelli, Jingying Wang
Publikováno v:
Cunnington, S, Wolz, L, Bull, P, Carucci, I P, Grainge, K, Irfan, M O, Spinelli, M & Wang, J 2023, ' The foreground transfer function for Hi intensity mapping signal reconstruction: MeerKLASS and precision cosmology applications ', MNRAS . https://doi.org/10.1093/mnras/stad1567
Blind cleaning methods are currently the preferred strategy for handling foreground contamination in single-dish HI intensity mapping surveys. Despite the increasing sophistication of blind techniques, some signal loss will be inevitable across all s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7bbc921551ceda91815e92473d4d9ed
http://arxiv.org/abs/2302.07034
http://arxiv.org/abs/2302.07034
Autor:
Mahony, Constance, Fortuna, Maria Cristina, Joachimi, Benjamin, Korn, Andreas, Hoekstra, Henk, Schmidt, Samuel J., Alonso, David, Singh, Sukhdeep, Ricci, Marina, Hildebrandt, Hendrik, Duncan, Christopher, Johnston, Harry, Sub String Theory Cosmology and ElemPart, Theoretical Physics
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 513(1), 1210-1228
Monthly Notices of the Royal Astronomical Society, 513(1), 1210. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 513(1), 1210. Oxford University Press
Recent works have shown that weak lensing magnification must be included in upcoming large-scale structure analyses, such as for the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), to avoid biasing the cosmological results. In this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cfed4e881431366bc83316571c8e1fe2
https://ora.ox.ac.uk/objects/uuid:648ca2f9-7ed2-47c1-99a2-633870240fc3
https://ora.ox.ac.uk/objects/uuid:648ca2f9-7ed2-47c1-99a2-633870240fc3
Autor:
Josh Frieman, R. L. C. Ogando, J. Calcino, David J. James, Pablo Fosalba, F. J. Castander, Ramon Miquel, O. Alves, Elisabeth Krause, J. Mena-Fernández, Will J. Percival, N. Weaverdyck, Karl Glazebrook, D Burke, A Roodman, C. Lidman, B. E. Tucker, A. Brandao-Souza, Erin Sheldon, A. Choi, T. M. C. Abbott, M. Carrasco Kind, F. Andrade-Oliveira, Jennifer L. Marshall, K. Honscheid, J. Carretero, Michael Schubnell, Jack Elvin-Poole, Tamara M. Davis, Anais Möller, E. Bertin, Chun-Hao To, Agnès Ferté, E. J. Sanchez, Ashley J. Ross, Martin Crocce, I. Sevilla-Noarbe, M. Soares-Santos, R. Cawthon, Daniel Thomas, A. G. Kim, E. Suchyta, J. Gschwend, August E. Evrard, Tommaso Giannantonio, A. A. Plazas Malagón, Geraint F. Lewis, G. Tarle, W. Riquelme, Rob Sharp, Santiago Avila, E. Buckley-Geer, S. A. Uddin, Ofer Lahav, Alex Drlica-Wagner, Dragan Huterer, A. Porredon, W. G. Hartley, M. Costanzi, Felipe Menanteau, A. Carnero Rosell, K. D. Eckert, T. N. Varga, Peter Doel, Douglas L. Tucker, V. Scarpine, Daniela Carollo, Robert Morgan, Juan Garcia-Bellido, S. Desai, Kyler Kuehn, D. L. Hollowood, J. Annis, H. T. Diehl, Christopher J. Conselice, S. Serrano, I. Ferrero, L. N. da Costa, Ben Hoyle, K. C. Chan, Rogerio Rosenfeld, Enrique Gaztanaga, B. Flaugher, David J. Brooks, Antonella Palmese, Marcos Lima, M. A. G. Maia, M. Rodriguez-Monroy, U. Malik, Adriano Pieres, F. Paz-Chinchón, Joseph J. Mohr, J. De Vicente, M.E. da Silva Pereira, M. Smith, S. Everett, Daniel Gruen, H. Camacho, J. Muir, Samuel Hinton, D. W. Gerdes, G. Gutierrez, M. E. C. Swanson, Jacobo Asorey, Michel Aguena, D. Sanchez Cid, S. Allam, Robert A. Gruendl
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 509 (1), pp.778-799. ⟨10.1093/mnras/stab2995⟩
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Digital.CSIC. Repositorio Institucional del CSIC
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Monthly Notices of the Royal Astronomical Society, 2021, 509 (1), pp.778-799. ⟨10.1093/mnras/stab2995⟩
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Digital.CSIC. Repositorio Institucional del CSIC
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Rosell, A., et al. (DES Collaboration)
In this paper, we present and validate the galaxy sample used for the analysis of the baryon acoustic oscillation (BAO) signal in the Dark Energy Survey (DES) Y3 data. The definition is based on a colour an
In this paper, we present and validate the galaxy sample used for the analysis of the baryon acoustic oscillation (BAO) signal in the Dark Energy Survey (DES) Y3 data. The definition is based on a colour an
Autor:
William Schoenell, Thom de Souza, Leonardo A. Almeida, Eduardo S. Pereira, D. R. Gonçalves, F. R. Herpich, L. Azanha, J. A. Hernandez-Jimenez, Martin Makler, Lilianne Mariko Izuti Nakazono, G. Damke, C. Lima-Dias, L. Sampedro, R. S. de Souza, R. Lopes de Oliveira, C. Queiroz, Antonio D. Montero-Dorta, S. Torres-Flores, E. Telles, P. A. A. Lopes, Vinicius M. Placco, L. Sodré, M. L. Buzzo, Luis Raul Weber Abramo, C. Mendes de Oliveira, S. V. Werner, L. Santana-Silva, Antonio Kanaan, Paula Coelho, Ana L. Chies-Santos, C. E. Barbosa, M. V. Costa-Duarte, Alberto Molino, Roderik Overzier, J. L. Nilo Castellón, Narciso Benítez, Alvaro Alvarez-Candal, N. Muñoz-Elgueta, Lima Ev, Y. Jimenez-Teja, Stavros Akras, Roberto K. Saito, T. Ribeiro, Arianna Cortesi, Thiago S. Gonçalves
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Digital.CSIC. Repositorio Institucional del CSIC
instname
Universidade de São Paulo (USP)
instacron:USP
Digital.CSIC. Repositorio Institucional del CSIC
instname
Authors: Molino, A.; Costa-Duarte, M. V.; Sampedro, L.; Herpich, F. R.; Sodré, L., Jr.; Mendes de Oliveira, C.; Schoenell, W.; Barbosa, C. E.; Queiroz, C.; Lima, E. V. R.; Azanha, L.; Muñoz-Elgueta, N.; Ribeiro, T.; Kanaan, A.; Hernandez-Jimenez, J
Publikováno v:
Journal of Physical Studies. 26
We calculated morphological parameters for 70821 galaxies from VIPERS (spectroscopic galaxy survey performed on VIMOS spectroscope at VLT). These parameters includes Gini, M20, Concentration, Asymmetry and Smoothness. Results correlate with the distr
Interferometric HI intensity mapping: perturbation theory predictions and foreground removal effects
Autor:
Alkistis Pourtsidou
Publikováno v:
Pourtsidou, A 2023, ' Interferometric H i intensity mapping: perturbation theory predictions and foreground removal effects ', Monthly Notices of the Royal Astronomical Society, vol. 519, no. 4, pp. 6246-6256 . https://doi.org/10.1093/mnras/stad127
We provide perturbation theory predictions for the HI intensity mapping power spectrum multipoles using the Effective Field Theory of Large Scale Structure (EFTofLSS), which should allow us to constrain cosmological parameters exploiting mildly nonli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fadc6e161203ff8bc935d4ca7b436c2d