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BIBTEX RIS

A comparison of effective field theory models of redshift space galaxy power spectra for DESI 2024 and future surveys

2025; Institute of Physics; Volume: 2025; Issue: 01 Linguagem: Inglês

10.1088/1475-7516/2025/01/134

ISSN

1475-7516

Autores

M. Maus, Yan Lai, H. E. Noriega, S. Ramirez-Solano, Alejandro Avilés, Shi-Fan Chen, S. Fromenteau, Héctor Gil-Marín, Cullan Howlett, M. Vargas-Magaña, Martin White, Pauline Zarrouk, José Edgar Madriz Aguilar, S. P. Ahlen, O. Alves, S. Brieden, D. Brooks, E. Burtin, T. Claybaugh, Shaun Cole, K. Dawson, Miguel Icaza-Lizaola, Axel de la Macorra, A. de Mattia, Peter Doel, Simone Ferraro, N. Findlay, J. E. Forero-Romero, E. Gaztañaga, Satya Gontcho A Gontcho, ChangHoon Hahn, K. Honscheid, Mustapha Ishak, A. Kremin, Martin Landriau, L. Le Guillou, Marc Manera, R. Miquel, Eva-Maria Mueller, S. Nadathur, Gustavo Niz, N. Palanque‐Delabrouille, Will J. Percival, Claire Poppett, Francisco Prada, Mehdi Rezaie, A. Rocher, Graziano Rossi, E. Sánchez, D. Schlegel, M. Schubnell, D. Sprayberry, G. Tarlé, Sihan Yuan, Ruiyang Zhao, Rongpu Zhou, Hu Zou,

Tópico(s)

Stellar, planetary, and galactic studies

Referência(s)