Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Star formation, and Halo.
The evolution of star formation histories of quiescent galaxies
On the Nature of Disks at High Redshift Seen by JWST/CEERS with Contrastive Learning and Cosmological Simulations
The role of dissipation in the scaling relations of cosmological merger remnants
The AGORA High-resolution Galaxy Simulations Comparison Project. V. Satellite Galaxy Populations in a Cosmological Zoom-in Simulation of a Milky Way–Mass Halo
The AGORA High-resolution Galaxy Simulations Comparison Project. VI. Similarities and Differences in the Circumgalactic Medium
Conditions for clump survival in High-<i>z</i>disc galaxies
UV-bright Star-forming Clumps and Their Host Galaxies in UVCANDELS at 0.5 ≤ z ≤ 1
Clustering and halo abundances in early dark energy cosmological models
Mock light-cones and theory friendly catalogues for the CANDELS survey
The AGORA High-resolution Galaxy Simulations Comparison Project. III. Cosmological Zoom-in Simulation of a Milky Way–mass Halo
Core formation in high-z massive haloes: heating by post-compaction satellites and response to AGN outflows
The building up of <i>observed</i> stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
Quenching as a Contest between Galaxy Halos and Their Central Black Holes
A mass threshold for galactic gas discs by spin flips
A deep learning approach to test the small-scale galaxy morphology and its relationship with star formation activity in hydrodynamical simulations
Stellar masses of giant clumps in CANDELS and simulated galaxies using machine learning
Origin of star-forming rings around massive centres in massive galaxies at <i>z</i> &lt; 4
O <scp>vi</scp> traces photoionized streams with collisionally ionized boundaries in cosmological simulations of <i>z</i> ∼ 1 massive galaxies
The nature of giant clumps in high- <i>z</i> discs: a deep-learning comparison of simulations and observations
The evolution of galaxy shapes in CANDELS: from prolate to discy
Multi-filament gas inflows fuelling young star-forming galaxies
CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: dependence on redshift, halo mass, and radius
The global star formation law by supernova feedback
Dark matter halo properties versus local density and cosmic web location
Semi-analytic modelling of the extragalactic background light and consequences for extragalactic gamma-ray spectra
idUS (Universidad de Sevilla) 2017cited by 415position: middle
Galaxy properties from the ultraviolet to the far-infrared: Λ cold dark matter models confront observations
idUS (Universidad de Sevilla) 2017cited by 143position: middle
z ∼ 2: An Epoch of Disk Assembly
Structural and Star-forming Relations since z similar to 3: Connecting Compact Star-forming and Quiescent Galaxies
eScholarship (California Digital Library) 2017cited by 100position: middle
CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z ∼ 2
Spatially Resolved Kinematics in the Central 1 kpc of a Compact Star-forming Galaxy at z ∼ 2.3 from ALMA CO Observations