Cool and dense ejections, typically Hα surges, often appear alongside EUV or X-ray coronal jets as a result of the emergence of magnetized plasma from the solar...
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PublicaciónThe Cool Surge Following Flux Emergence in a Radiation-MHD Experiment
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PublicaciónThe correlation structure of dark matter halo properties
We investigate the correlation between nine different dark matter halo properties using a rank correlation analysis and a Principal Component Analysis for a...
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PublicaciónThe cosmic waltz of Coma Berenices and Latyshev 2 (Group X). Membership, phase-space structure, mass, and energy distributions
Context. Open clusters (OCs) are fundamental benchmarks where theories of star formation and stellar evolution can be tested and validated. Coma Berenices (Coma...
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PublicaciónThe cosmic web connection to the dark matter halo distribution through gravity
This work investigates the connection between the cosmic web and the halo distribution through the gravitational potential at the field level. We combine three...
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PublicaciónThe cosmic web from perturbation theory
Context. Analysing the large-scale structure (LSS) in the Universe with galaxy surveys demands accurate structure formation models. Such models should ideally...
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PublicaciónThe dark energy survey 5-yr photometrically identified type Ia supernovae
As part of the cosmology analysis using Type Ia Supernovae (SN Ia) in the Dark Energy Survey (DES), we present photometrically identified SN Ia samples using...
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PublicaciónThe Data Reduction Pipeline for the Apache Point Observatory Galactic Evolution Experiment
The Apache Point Observatory Galactic Evolution Experiment (APOGEE), part of the Sloan Digital Sky Survey III, explores the stellar populations of the Milky Way...
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PublicaciónThe Dawes Review 10: The impact of deep learning for the analysis of galaxy surveys
The amount and complexity of data delivered by modern galaxy surveys has been steadily increasing over the past years. New facilities will soon provide imaging...
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PublicaciónThe distribution of atomic hydrogen in EAGLE galaxies: morphologies, profiles, and H I holes
We compare the mass and internal distribution of atomic hydrogen (H I) in 2200 present-day central galaxies with Mstar > 1010 M⊙ from the 100 Mpc EAGLE...