activity
20162025
most citedA Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging

350 citations · 1.6k across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.GA2025★ 1 cited

J-PAS: A Neural Network Approach to Single Stellar Population Characterization

H. Domínguez Sánchez, P. Coelho, G. Bruzual +28

J-PAS (Javalambre Physics of the Accelerating Universe Astrophysical Survey) will present a groundbreaking photometric survey covering 8500 deg of the visible sky from Javalamb…

astro-ph.SR2025

J-PLUS: Understanding outlier white dwarfs in the third data release via dimensionality reduction

C. López-Sanjuan, P. -E. Tremblay, A. del Pino +20

We present the white dwarf catalog derived from the third data release of the Javalambre Photometric Local Universe Survey (J-PLUS DR3), which covers 3284 deg2 using 12 optical fil…

astro-ph.GA2025★ 1 cited

Euclid Quick Data Release (Q1) Exploring galaxy properties with a multi-modal foundation model

Euclid Collaboration, M. Siudek, M. Huertas-Company +321

Modern astronomical surveys, such as the Euclid mission, produce high-dimensional, multi-modal data sets that include imaging and spectroscopic information for millions of galaxies…

astro-ph.GA2025★ 2 cited

Euclid Quick Data Release (Q1), A first look at the fraction of bars in massive galaxies at

Euclid Collaboration, M. Huertas-Company, M. Walmsley +336

Stellar bars are key structures in disc galaxies, driving angular momentum redistribution and influencing processes such as bulge growth and star formation. Quantifying the bar fra…

astro-ph.GA2025★ 1 cited

The Cosmic Evolution Early Release Science Survey (CEERS)

Steven L. Finkelstein, Micaela B. Bagley, Pablo Arrabal Haro +96

We present the Cosmic Evolution Early Release Science (CEERS) Survey, a 77.2 hour Director's Discretionary Early Release Science Program. CEERS demonstrates, tests, and validates e…

astro-ph.GA2024★ 2 cited

Automated galaxy sizes in Euclid images using the Segment Anything Model

J. Vega-Ferrero, F. Buitrago, J. Fernández-Iglesias +3

Stellar disk truncations, also referred to as galaxy edges, are key indicators of galactic size, determined by the radial location of the gas density threshold for star formation.…

astro-ph.GA2024★ 6 cited

J-PLUS: Bayesian object classification with a strum of BANNJOS

A. del Pino, C. López-Sanjuan, A. Hernán-Caballero +22

With its 12 optical filters, the Javalambre-Photometric Local Universe Survey (J-PLUS) provides an unprecedented multicolor view of the local Universe. The third data release (DR3)…

astro-ph.GA2023★ 70 cited

A Milky Way-like barred spiral galaxy at a redshift of 3

Luca Costantin, Pablo G. Pérez-González, Yuchen Guo +30

The majority of massive disk galaxies in the local Universe show a stellar barred structure in their central regions, including our Milky Way. Bars are supposed to develop in dynam…

astro-ph.GA2023★ 7 cited

Galaxy Morphology from through the eyes of JWST

M. Huertas-Company, K. G. Iyer, E. Angeloudi +26

We analyze the Near Infrared (m) rest-frame morphologies of galaxies with in the redshift range , compare with previous HST-based results an…

astro-ph.IM2023★ 28 cited

Identification of tidal features in deep optical galaxy images with Convolutional Neural Networks

H. Domínguez Sánchez, G. Martin, I. Damjanov +14

Interactions between galaxies leave distinguishable imprints in the form of tidal features which hold important clues about their mass assembly. Unfortunately, these structures are…

astro-ph.CO2023★ 4 cited

On the nature of disks at high redshift seen by JWST/CEERS with contrastive learning and cosmological simulations

J. Vega-Ferrero, M. Huertas-Company, L. Costantin +26

Visual inspections of the first optical rest-frame images from JWST have indicated a surprisingly high fraction of disk galaxies at high redshifts. Here, we alternatively apply sel…

astro-ph.CO2022★ 35 cited

A Deep Learning Approach to Infer Galaxy Cluster Masses from Planck Compton parameter maps

Daniel de Andres, Weiguang Cui, Florian Ruppin +8

Galaxy clusters are useful laboratories to investigate the evolution of the Universe, and accurately measuring their total masses allows us to constrain important cosmological para…

astro-ph.GA2022★ 153 cited

CEERS Key Paper III: The Diversity of Galaxy Structure and Morphology at z=3-9 with JWST

Jeyhan S. Kartaltepe, Caitlin Rose, Brittany N. Vanderhoof +58

We present a comprehensive analysis of the evolution of the morphological and structural properties of a large sample of galaxies at z=3-9 using early JWST CEERS NIRCam observation…

astro-ph.GA2022★ 102 cited

First Look at z > 1 Bars in the Rest-Frame Near-Infrared with JWST Early CEERS Imaging

Yuchen Guo, Shardha Jogee, Steven L. Finkelstein +45

Stellar bars are key drivers of secular evolution in galaxies and can be effectively studied using rest-frame near-infrared (NIR) images, which trace the underlying stellar mass an…

astro-ph.GA2022★ 11 cited

Lessons Learned from the Two Largest Galaxy Morphological Classification Catalogues built by Convolutional Neural Networks

Ting-Yun Cheng, H. Domínguez Sánchez, J. Vega-Ferrero +54

We compare the two largest galaxy morphology catalogues, which separate early and late type galaxies at intermediate redshift. The two catalogues were built by applying supervised…

astro-ph.GA2022★ 139 cited

Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations

Jorge A. Zavala, Veronique Buat, Caitlin M. Casey +121

Lyman Break Galaxy (LBG) candidates at z>10 are rapidly being identified in JWST/NIRCam observations. Due to the (redshifted) break produced by neutral hydrogen absorption of rest-…

astro-ph.GA2022★ 57 cited

Expectations of the size evolution of massive galaxies at from the TNG50 simulation: the CEERS/JWST view

Luca Costantin, Pablo G. Pérez-González, Jesús Vega-Ferrero +16

We present a catalog of about 25,000 images of massive () galaxies at redshift from the TNG50 cosmological simulation, tailored for…

astro-ph.GA2022★ 350 cited

A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging

Steven L. Finkelstein, Micaela B. Bagley, Pablo Arrabal Haro +117

We report the discovery of a candidate galaxy with a photo-z of z~12 in the first epoch of the JWST Cosmic Evolution Early Release Science (CEERS) Survey. Following conservative se…

astro-ph.CO2021★ 37 cited

Shocks in the Stacked Sunyaev-Zel'dovich Profiles of Clusters I: Analysis with the Three Hundred Simulations

Eric J. Baxter, Susmita Adhikari, Jesús Vega-Ferrero +4

Gas infalling into the gravitational potential wells of massive galaxy clusters is expected to experience one or more shocks on its journey to becoming part of the intracluster med…

astro-ph.GA2020★ 44 cited

Pushing automated morphological classifications to their limits with the Dark Energy Survey

J. Vega-Ferrero, H. Domínguez Sánchez, M. Bernardi +60

We present morphological classifications of 27 million galaxies from the Dark Energy Survey (DES) Data Release 1 (DR1) using a supervised deep learning algorithm. The classif…

astro-ph.GA2018★ 231 cited

The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications

Weiguang Cui, Alexander Knebe, Gustavo Yepes +34

We introduce the THE THREE HUNDRED project, an endeavour to model 324 large galaxy clusters with full-physics hydrodynamical re-simulations. Here we present the data set and study…

astro-ph.CO2018★ 53 cited

CLUMP-3D. Testing CDM with galaxy cluster shapes

Mauro Sereno, Keiichi Umetsu, Stefano Ettori +5

The CDM model of structure formation makes strong predictions on concentration and shape of DM (dark matter) halos, which are determined by mass accretion processes. Comparison…

astro-ph.CO2017★ 125 cited

Dark matter under the microscope: Constraining compact dark matter with caustic crossing events

Jose M. Diego, Nick Kaiser, Tom Broadhurst +12

A galaxy cluster acts as a cosmic telescope over background galaxies but also as a cosmic microscope of the lens imperfections. The diverging magnification of lensing caustics enha…

astro-ph.GA2016★ 45 cited

A free-form lensing model of A370 revealing stellar mass dominated BCGs, in Hubble Frontier Fields images

Jose M. Diego, Kasper B. Schmidt, Tom Broadhurst +9

We derive a free-form mass distribution for the unrelaxed cluster A370 (z=0.375), using the latest Hubble Frontier Fields images and GLASS spectroscopy. Starting from a reliable se…