activity
20162026
most citedScant evidence for thawing quintessence

123 citations · 952 across the 39 of their papers we have counts for

collaborators

41 papers

astro-ph.CO2026

An LSST-DESC Precursor Project: Hyper Suprime-Cam Year 1 pt in Harmonic Space

D. Sanchez-Cid, J. Sanchez, I. Sevilla-Noarbe +19

We present the first fully photometric joint analysis of weak gravitational lensing and galaxy clustering (32pt) in harmonic space with LSST-DESC analysis pipelines applied…

astro-ph.CO2026

Blast.jl: Differentiable Non-Limber Power Spectra for Joint Clustering, Shear, and CMB lensing Analyses

Sofia Chiarenza, Marco Bonici, Stefano Camera +4

Upcoming large-scale structure surveys require accurate theoretical predictions for angular power spectra on the largest angular scales, where the commonly used Limber approximatio…

astro-ph.CO2026

Fisher Forecasting for the DESC with

Paul Rogozenski, Sankarshana Srinivasan, Javier Sánchez +15

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) has begun its ten-year survey of the entire visible southern hemisphere. To ensure robust cosmological measurem…

astro-ph.CO2026

The Status of Single Scalar Field Dark Energy

Carlos García-García, Pedro G. Ferreira, William J. Wolf

We present an assessment of the current observational status of single scalar field models of dark energy. Motivated by recent cosmological measurements -- including baryon acousti…

astro-ph.CO2026

\textit{Euclid} preparation. Baryon acoustic oscillations extraction techniques: comparison and optimisation

Euclid Collaboration, E. Sarpa, A. Veropalumbo +296

We present the first end-to-end validation of the Euclid baryon acoustic oscillation (BAO) analysis pipeline, encompassing density-field reconstruction, two-point correlation funct…

astro-ph.CO2026

Propagating data-driven galaxy redshift distribution uncertainties in 32-pt analyses

Jaime Ruiz-Zapatero, Qianjun Hang, Yun-Hao Zhang +7

Uncertainties in the radial distribution of galaxies, , are one of the major contributions to the error budget of early Stage-IV galaxy survey analy…

astro-ph.CO2026

Joint tomographic measurement of thermal Sunyaev Zeldovich and the cosmic infrared background

Adrien La Posta, David Alonso, Carlos García-García +1

We present a novel method for the tomographic reconstruction of the bias-weighted mean electron pressure and star formation rate density $\langle bρ_{\mathrm…

astro-ph.CO2025

Low-redshift constraints on structure growth from CMB lensing tomography

Andrea Rubiola, Matteo Zennaro, Carlos García-García +2

We present constraints on the amplitude of matter fluctuations from the clustering of galaxies and their cross-correlation with the gravitational lensing convergence of the cosmic…

astro-ph.CO2025★ 28 cited

Cosmological constraints on Galileon dark energy with broken shift symmetry

William J. Wolf, Pedro G. Ferreira, Carlos García-García

Current cosmological data seem to show that dark energy is evolving in time and that it possibly crossed the phantom divide in the past. So far the only theories that lead to such…

astro-ph.CO2025★ 72 cited

Assessing cosmological evidence for non-minimal coupling

William J. Wolf, Carlos García-García, Theodore Anton +1

The recent observational evidence of deviations from the -Cold Dark Matter (CDM) model points towards the presence of evolving dark energy. The simplest possibility consists…

astro-ph.CO2025

Robust cosmic shear with small-scale nulling

Giulia Piccirilli, Matteo Zennaro, Carlos García-García +1

Standard cosmological weak lensing analyses using cosmic shear are inevitably sensitive to small-scale, non-linear clustering from low-redshift structures. The need to adequately m…

astro-ph.CO2025★ 75 cited

Robustness of dark energy phenomenology across different parameterizations

William J. Wolf, Carlos García-García, Pedro G. Ferreira

The recent evidence for dynamical dark energy from DESI, in combination with other cosmological data, has generated significant interest in understanding the nature of dark energy…

astro-ph.CO2024★ 4 cited

A 1% accurate method to include baryonic effects in galaxy-galaxy lensing models

Matteo Zennaro, Giovanni Aricò, Carlos García-García +6

Galaxy clustering and galaxy-galaxy lensing are two of the main observational probes in Stage-IV large-scale structure surveys. Unfortunately, the complicated relationship between…

astro-ph.CO2024★ 2 cited

: insights on gas thermodynamics from the combination of X-ray and thermal Sunyaev-Zel'dovich data cross-correlated with cosmic shear

Adrien La Posta, David Alonso, Nora Elisa Chisari +2

We measure the cross-correlation between cosmic shear from the third-year release of the Dark Energy Survey, thermal Sunyaev-Zel'dovich (tSZ) maps from Planck, and X-ray maps from…

astro-ph.CO2024★ 1 cited

: Normalising Flows for Joint Cosmological Analysis

Arrykrishna Mootoovaloo, Carlos García-García, David Alonso +1

Given the growth in the variety and precision of astronomical datasets of interest for cosmology, the best cosmological constraints are invariably obtained by combining data from d…

astro-ph.CO2024★ 92 cited

Matching current observational constraints with nonminimally coupled dark energy

William J. Wolf, Pedro G. Ferreira, Carlos García-García

We show that a Universe with a nonminimally coupled scalar field can fit current measurements of the expansion rate of the Universe better than the standard -Cold Dark Matter ($…

astro-ph.CO2024★ 123 cited

Scant evidence for thawing quintessence

William J. Wolf, Carlos García-García, Deaglan J. Bartlett +1

New constraints on the expansion rate of the Universe seem to favor evolving dark energy in the form of thawing quintessence models, i.e., models for which a canonical, minimally c…

astro-ph.IM2024★ 1 cited

Assessment of Gradient-Based Samplers in Standard Cosmological Likelihoods

Arrykrishna Mootoovaloo, Jaime Ruiz-Zapatero, Carlos García-García +1

We assess the usefulness of gradient-based samplers, such as the No-U-Turn Sampler (NUTS), by comparison with traditional Metropolis-Hastings algorithms, in tomographic $3 \times 2…

astro-ph.CO2024★ 44 cited

Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1

Carlos García-García, Matteo Zennaro, Giovanni Aricò +2

We present a cosmological analysis of the combination of the DES-Y3, KiDS-1000 and HSC-DR1 weak lensing samples under a joint harmonic-space pipeline making use of angular scales d…

astro-ph.CO2024

Growth history and quasar bias evolution at z < 3 from Quaia

G. Piccirilli, G. Fabbian, D. Alonso +4

We make use of the Gaia-Unwise quasar catalogue, Quaia, to constrain the growth history out to high redshifts from the clustering of quasars and their cross-correlation with maps o…

astro-ph.CO2023★ 11 cited

LimberJack.jl: auto-differentiable methods for angular power spectra analyses

J. Ruiz-Zapatero, D. Alonso, C. García-García +5

We present LimberJack.jl, a fully auto-differentiable code for cosmological analyses of 2 point auto- and cross-correlation measurements from galaxy clustering, CMB lensing and wea…

astro-ph.CO2023★ 2 cited

X-Ray-Cosmic-Shear Cross-Correlations: First Detection and Constraints on Baryonic Effects

Tassia Ferreira, David Alonso, Carlos Garcia-Garcia +1

We report a first detection, at very high significance (), of the cross-correlation between cosmic shear and the diffuse X-ray background, using data from the Dark Energy Surv…

astro-ph.CO2023★ 3 cited

Galaxy bias in the era of LSST: perturbative bias expansions

Andrina Nicola, Boryana Hadzhiyska, Nathan Findlay +14

Upcoming imaging surveys will allow for high signal-to-noise measurements of galaxy clustering at small scales. In this work, we present the results of the LSST bias challenge, the…

astro-ph.CO2023★ 5 cited

Constraining cosmology with the Gaia-unWISE Quasar Catalog and CMB lensing: structure growth

David Alonso, Giulio Fabbian, Kate Storey-Fisher +4

We study the angular clustering of Quaia, a Gaia- and unWISE-based catalog of over a million quasars with an exceptionally well-defined selection function. With it, we derive cosmo…