A comparison of effective field theory models of redshift space galaxy
power spectra for DESI 2024 and future surveys
M. Maus,Y. Lai,H. E. Noriega,S. Ramirez-Solano,A. Aviles,S. Chen,S. Fromenteau,H. Gil-Marín,C. Howlett, M. Vargas-Magaña,M. White,P. Zarrouk,J. Aguilar,S. Ahlen,O. Alves,S. Brieden,D. Brooks,E. Burtin,T. Claybaugh,S. Cole,K. Dawson,M. Icaza-Lizaola,A. de la Macorra,A. de Mattia,P. Doel,S. Ferraro,N. Findlay,J. E. Forero-Romero,E. Gaztañaga,S. Gontcho A Gontcho,C. Hahn,K. Honscheid,M. Ishak,A. Kremin,M. Landriau,L. Le Guillou,M. Manera,R. Miquel,E. Mueller,S. Nadathur,G. Niz,N. Palanque-Delabrouille,W. J. Percival,C. Poppett,F. Prada,M. Rezaie,A. Rocher,G. Rossi,E. Sanchez,D. Schlegel,M. Schubnell,D. Sprayberry,G. Tarlé,S. Yuan,R. Zhao,R. Zhou,H. Zou arxiv（2024）
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