activity
20092026
most citedThe Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

1.4k citations · 5.2k across the 30 of their papers we have counts for

collaborators

31 papers

physics.gen-ph2026

Constraints on unimodular diffusion models with latest observables

Jesús Chavarría, Sebastien Fromenteau, Daniel Sudarsky +1

Cosmological models incorporating a time-dependent equation of state have recently been explored \cite{DESI:2025fii}, showing a preference for a dynamical dark energy component. In…

astro-ph.CO2024★ 1 cited

Constraining the phase shift of relativistic species in DESI BAOs

Abbé M. Whitford, Hugo Rivera-Morales, Cullan Howlett +36

In the early Universe, neutrinos decouple quickly from the primordial plasma and propagate without further interactions. The impact of free-streaming neutrinos is to create a tempo…

astro-ph.CO2024

Full Modeling and Parameter Compression Methods in configuration space for DESI 2024 and beyond

S. Ramirez-Solano, M. Icaza-Lizaola, H. E. Noriega +49

In the contemporary era of high-precision spectroscopic surveys, led by projects like DESI, there is an increasing demand for optimizing the extraction of cosmological information…

astro-ph.CO2024★ 2 cited

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 +54

In preparation for the next generation of galaxy redshift surveys, and in particular the year-one data release from the Dark Energy Spectroscopic Instrument (DESI), we investigate…

astro-ph.CO2024★ 1 cited

Comparing Compressed and Full-modeling Analyses with FOLPS: Implications for DESI 2024 and beyond

H. E. Noriega, A. Aviles, H. Gil-Marín +51

The Dark Energy Spectroscopic Instrument (DESI) will provide unprecedented information about the large-scale structure of our Universe. In this work, we study the robustness of the…

astro-ph.CO2023

Full Shape Cosmology Analysis from BOSS in configuration space using Neural Network Acceleration

Sadi Ramirez, Miguel Icaza-Lizaola, Sebastien Fromenteau +2

Recently, a new wave of full modeling analyses have emerged within the Large-Scale Structure community, leading mostly to tighter constraints on the estimation of cosmological para…

astro-ph.EP2023★ 7 cited

Evolution of the eccentricity and inclination of low-mass planets subjected to thermal forces: a numerical study

S. Cornejo, F. S. Masset, R. O. Chametla +1

By means of three dimensional, high resolution hydrodynamical simulations we study the orbital evolution of weakly eccentric or inclined low-mass protoplanets embedded in gaseous d…

astro-ph.CO2022★ 42 cited

Fast computation of non-linear power spectrum in cosmologies with massive neutrinos

Hernán E. Noriega, Alejandro Aviles, Sebastien Fromenteau +1

We compute 1-loop corrections to the redshift space galaxy power spectrum in cosmologies containing additional scales, and hence kernels different from Einstein-de Sitter (EdS). Sp…

astro-ph.IM2022★ 465 cited

Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument

B. Abareshi, J. Aguilar, S. Ahlen +264

The Dark Energy Spectroscopic Instrument (DESI) has embarked on an ambitious five-year survey to explore the nature of dark energy with spectroscopy of 40 million galaxies and quas…

astro-ph.GA2022★ 5 cited

The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data

Abdurro'uf, Katherine Accetta, Conny Aerts +337

This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete…

astro-ph.CO2020★ 78 cited

Testing the theory of gravity with DESI: estimators, predictions and simulation requirements

Shadab Alam, Christian Arnold, Alejandro Aviles +33

Shortly after its discovery, General Relativity (GR) was applied to predict the behavior of our Universe on the largest scales, and later became the foundation of modern cosmology.…

astro-ph.CO2020★ 77 cited

The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample

Seshadri Nadathur, Alex Woodfinden, Will J. Percival +12

We present an analysis of the anisotropic redshift-space void-galaxy correlation in configuration space using the Sloan Digital Sky Survey extended Baryon Oscillation Spectroscopic…

astro-ph.CO2020★ 42 cited

The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Pairwise-Inverse-Probability and Angular Correction for Fibre Collisions in Clustering Measurements

Faizan G. Mohammad, Will J. Percival, Hee-Jong Seo +28

The completed eBOSS catalogues contain redshifts of 344080 QSOs over 0.8<z<2.2 covering 4808 deg, 174816 LRGs over 0.6<z<1.0 covering 4242 deg and 173736 ELGs over 0.6<z<1.…

astro-ph.CO2020★ 41 cited

The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements

Graziano Rossi, Peter D. Choi, Jeongin Moon +19

We develop a series of N-body data challenges, functional to the final analysis of the extended Baryon Oscillation Spectroscopic Survey (eBOSS) Data Release 16 (DR16) galaxy sample…

astro-ph.CO2020★ 194 cited

The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogs for Cosmological Analysis

Ashley J. Ross, Julian Bautista, Rita Tojeiro +53

We present large-scale structure catalogs from the completed extended Baryon Oscillation Spectroscopic Survey (eBOSS). Derived from Sloan Digital Sky Survey (SDSS) -IV Data Release…

astro-ph.CO2020★ 313 cited

The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0

Héctor Gil-Marín, Julián E. Bautista, Romain Paviot +37

We analyse the clustering of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey Data Release 16 luminous red galaxy sample (DR16 eBOSS LRG) in combina…

astro-ph.CO2020★ 335 cited

The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1

Julian E. Bautista, Romain Paviot, Mariana Vargas Magaña +30

We present the cosmological analysis of the configuration-space anisotropic clustering in the completed Sloan Digital Sky Survey IV (SDSS-IV) extended Baryon Oscillation Spectrosco…

astro-ph.CO2020★ 1.4k cited

The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

eBOSS Collaboration, Shadab Alam, Marie Aubert +97

We present the cosmological implications from final measurements of clustering using galaxies, quasars, and Ly forests from the completed Sloan Digital Sky Survey (SDSS) lineage…

astro-ph.CO2019★ 55 cited

The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 LRG sample: structure growth rate measurement from the anisotropic LRG correlation function in the redshift range 0.6 < z < 1.0

M. Icaza-Lizaola, M. Vargas-Magaña, S. Fromenteau +14

We analyze the anisotropic clustering of the Sloan Digital Sky Survey-IV Extended Baryon Oscillation Spectroscopic Survey (eBOSS) Luminous Red Galaxy Data Release 14 (DR14) sample…

astro-ph.EP2019★ 23 cited

Impact of thermal effects on the evolution of eccentricity and inclination of low-mass planets

Sebastien Fromenteau, Frederic Masset

Using linear perturbation theory, we evaluate the time-dependent force exerted on an eccentric and inclined low-mass planet embedded in a gaseous protoplanetary disc with finite th…

astro-ph.CO2015★ 21 cited

Prospects for high-z cluster detections with Planck, based on a follow-up of 28 candidates using MegaCam@CFHT

R. F. J. van der Burg, H. Aussel, G. W. Pratt +13

The Planck catalogue of SZ sources limits itself to a significance threshold of 4.5 to ensure a low contamination rate by false cluster candidates. This means that only the most ma…

astro-ph.CO2015★ 16 cited

The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Effect of smoothing of density field on reconstruction and anisotropic BAO analysis

M. Vargas-Magaña, S. Ho, S. Fromenteau +1

The reconstruction algorithm introduced by \cite{Eis07}, which is widely used in clustering analysis, is based on the inference of the first order Lagrangian displacement field fro…

astro-ph.CO2015★ 39 cited

Planck Intermediate Results. XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes in the Canary Islands Observatories

Planck Collaboration, P. A. R. Ade, N. Aghanim +187

We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with telescopes at the Canary Islands observatories as part of the gene…

astro-ph.CO2015★ 125 cited

Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources: Addendum

Planck Collaboration, P. A. R. Ade, N. Aghanim +276

We update the all-sky Planck catalogue of 1227 clusters and cluster candidates (PSZ1) published in March 2013, derived from Sunyaev-Zeldovich (SZ) effect detections using the first…