Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Cosmology and Gravitation Theories, Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, and Dark Matter and Cosmic Phenomena.
Comparing Compressed and Full-Modeling analyses with FOLPS: implications for DESI 2024 and beyond
Validating the galaxy and quasar catalog-level blinding scheme for the DESI 2024 analysis
Taming assembly bias for primordial non-Gaussianity
Quijote-PNG: Simulations of Primordial Non-Gaussianity and the Information Content of the Matter Field Power Spectrum and Bispectrum
Unveiling the Universe with emerging cosmological probes
Quijote PNG: The information content of the halo power spectrum and bispectrum
The effect of outflows on CMB bounds from Primordial Black Hole accretion
Quijote-PNG: Quasi-maximum Likelihood Estimation of Primordial Non-Gaussianity in the Nonlinear Dark Matter Density Field
Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension
Cosmology intertwined III: <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si4.svg"><mml:mrow><mml:mi>f</mml:mi><mml:msub><mml:mi>σ</mml:mi><mml:mn>8</mml:mn></mml:msub></mml:mrow></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si3.svg"><mml:msub><mml:mi>S</mml:mi><mml:mn>8</mml:mn></mml:msub></mml:math>
Snowmass2021 - Letter of interest cosmology intertwined IV: The age of the universe and its curvature
Snowmass2021 - Letter of interest cosmology intertwined I: Perspectives for the next decade
Cosmology and fundamental physics with the Euclid satellite
Constraining primordial non-Gaussianity with bispectrum and power spectrum from upcoming optical and radio surveys
GW×LSS: chasing the progenitors of merging binary black holes
Relativistic wide-angle galaxy bispectrum on the light cone
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12
Cosmic Explosions, Life in the Universe, and the Cosmological Constant
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring DA and H at z = 0.57 from the baryon acoustic peak in the Data Release 9 spectroscopic Galaxy sample
General relativistic corrections and non-Gaussianity in large-scale structure
The Baryon Oscillation Spectroscopic Survey of SDSS-III
Dipòsit Digital de la Universitat de Barcelona (Universitat de Barcelona) 2012cited by 1,026position: first
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Release 9 spectroscopic galaxy sample
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at<i>z</i>= 0.57 from anisotropic clustering
ACOUSTIC SCALE FROM THE ANGULAR POWER SPECTRA OF SDSS-III DR8 PHOTOMETRIC LUMINOUS GALAXIES
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring structure growth using passive galaxies