Alejandro Avilés Cervantes

Artículos en revistas con arbitraje indizadas (Web of Science, JCR, SCOPUS)

1.- Unveiling neutrino masses: Insights from a robust BOSS and eBOSS data analysis and prospects for DESI and beyond Liga a la publicación

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2.- Modified gravity constraints from the full shape modeling of clustering measurements from DESI 2024 Liga a la publicación

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3.- DESI 2024 V: Full-Shape galaxy clustering from galaxies and quasars Liga a la publicación

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4.- DESI 2024 VII: cosmological constraints from the full-shape modeling of clustering measurements Liga a la publicación

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5.- Constraints on neutrino physics from DESI DR2 BAO and DR1 full shape Liga a la publicación

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6.- Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data Liga a la publicación

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7.- DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints Liga a la publicación

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8.- Positive Neutrino Masses with DESI DR2 via Matter Conversion to Dark Energy Liga a la publicación

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9.- Non-Gaussian statistics in galaxy weak lensing: compressed three-point correlations and cosmological forecasts Liga a la publicación

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10.- Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid Liga a la publicación

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11.- Galaxy bias in the era of LSST: perturbative bias expansions Liga a la publicación

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12.- Full shape cosmology analysis from BOSS in configuration space using neural network acceleration Liga a la publicación

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13.- fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum Liga a la publicación

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14.- DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics

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15.- DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars

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16.- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

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17.- DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest

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18.- A comparison between Shapefit compression and Full-Modelling method with PyBird for DESI 2024 and beyond

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19.- An analysis of parameter compression and full-modeling techniques with Velocileptors for DESI 2024 and beyond

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

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

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

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23.- Unveiling Neutrino Masses: Insights from Robust (e)BOSS Data Analysis and Prospects for DESI and Beyond

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24.- Modeling the 3-point correlation function of projected scalar fields on the sphere Liga a la publicación

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25.- Testing gravity with the full-shape galaxy power spectrum: first constraints on scale-dependent modified gravity Liga a la publicación

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26.- Modified Gravity Constraints from the Full Shape Modeling of Clustering Measurements from DESI 2024

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27.- DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars

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28.- DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements

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29.- fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum

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

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• Hernán Enrique Noriega Barros          (Doctorado)
• José Abraham Arvizu Valenzuela          (Doctorado)
• Christian Fary Mayorga Reyes          (Licenciatura)
• Isaac Mateo Garzón Muñoz          (Maestría)
• Jair Ferrara Andrade          (Maestría)
• Diego González Sandoval          (Maestría)

• Sofía del Pilar Samario Nava          (Doctorado)