PC
P. Corcho-Caballero
astro-ph.GAastro-ph.COastro-ph.IMastro-ph.HEastro-ph.SRgr-qc
On Valency
published · living versionsW_3ukvwsjm·v1 · currentpublished
Euclid Quick Data Release (Q1). A systematic study of the intracluster light fraction at 0.2 < z < 1.5
with Euclid Collaboration, H. Gully, N. A. Hatch, H. Gao +311
1 version
Preprints & journals
30 papers in the corpus · 2020–2026Euclid Quick Data Release (Q1). A systematic study of the intracluster light fraction at 0.2 < z < 1.52610.29684v1 · H. Gully, N. A. Hatch, H. Gao et al.2026 · 0 citationsarXivon Valency
Euclid Bypass end-to-end simulations for spectroscopic galaxy clustering performance assessment2610.26990v1 · B. R. Granett, S. de la Torre, M. Moresco et al.2026 · 0 citationsarXiv
Euclid Quick Data Release (Q1). Exploring the complexity of quenching processes across time, environment, and mass through recently quenched galaxies2610.08999v1 · Z. Mao, L. Pozzetti, A. Enia et al.2026 · 0 citationsarXiv
Euclid Quick Data Release (Q1) Euclid spectroscopy of quasars. 2. Physical properties from spectral fitting2609.20947v1 · J. Calhau, G. Calderone, A. Feltre et al.2026 · 0 citationsarXiv
Euclid. A two-point correlation approach to diagnosing star-related systematics in the Euclid spectroscopic survey2609.05155v1 · I. Risso, B. R. Granett, E. Branchini et al.2026 · 0 citationsarXiv
Euclid preparation. The shape of halo profiles in CDM and non-standard cosmologies2609.04192v1 · L. Pizzuti, G. Y. Ferron, A. Ragagnin et al.2026 · 0 citationsarXiv
The MAGPI Survey: Evidence for Non-Universal Resolved Dust Attenuation Relations Beyond the Local Universe2607.07122v1 · A. Mailvaganam, T. Zafar, P. Corcho-Caballero et al.2026 · 0 citationsarXiv
Predicting Resolved Dust Attenuation from Local Galaxy Properties Using MaNGA2602.23767v1 · Anilkumar Mailvaganam, Tayyaba Zafar, Pablo Corcho-Caballero et al.2026 · 0 citationsPubl. Astron. Soc. Aust. 43 (2026) e056
Euclid preparation: LXXXI. The impact of nonparametric star formation histories on spatially resolved galaxy property estimation using synthetic Euclid images2511.22399v1 · A. Nersesian, Abdurro'uf, M. Baes et al.2025 · 0 citationsarXiv
Euclid Quick Data Release (Q1). Quenching precedes bulge formation in dense environments but follows it in the field2511.02964v2 · F. Gentile, E. Daddi, D. Elbaz et al.2025 · 0 citationsarXiv
The role of black hole feedback on galaxy star formation and the degeneracy with halo quenching2510.26305v2 · Hao Fu, Francesco Shankar, Feng Yuan et al.2025 · 2 citationsarXiv
Hector Galaxy Survey: Data Processing, Quality Control and Early Science2509.25784v1 · S. Oh, M. L. P. Gunawardhana, S. M. Croom et al.2025 · 4 citationsarXiv
The PyKOALA python library: a multi-instrument package for IFS data reduction2507.18347v1 · Pablo Corcho-Caballero, Yago Ascasibar, 'Angel R. L'opez-S'anchez et al.2025 · 2 citationsarXiv
The Population Synthesis Toolkit (PST) Python library2503.22802v2 · Pablo Corcho-Caballero, Yago Ascasibar, Daniel Jim'enez-L'opez et al.2025 · 0 citationsJournal of Open Source Software, 2025, 10(111), 8203
Euclid Quick Data Release (Q1) -- Data release overview2503.15302v1 · H. Aussel, I. Tereno, M. Schirmer et al.2025 · 3 citationsarXiv
Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between and 2503.15313v2 · C. Cleland, S. Mei, G. De Lucia et al.2025 · 4 citationsarXiv
Euclid Quick Data Release (Q1). A first view of the star-forming main sequence in the Euclid Deep Fields2503.15314v3 · A. Enia, L. Pozzetti, M. Bolzonella et al.2025 · 0 citationsarXiv
Euclid Quick Data Release (Q1). A probabilistic classification of quenched galaxies2503.15315v3 · P. Corcho-Caballero, Y. Ascasibar, G. Verdoes Kleijn et al.2025 · 4 citationsarXiv
Euclid: Finding strong gravitational lenses in the Early Release Observations using convolutional neural networks2502.09802v1 · B. C. Nagam, J. A. Acevedo Barroso, J. Wilde et al.2025 · 8 citationsarXiv
Euclid. I. Overview of the Euclid mission2405.13491v2 · Y. Mellier, Abdurro'uf, J. A. Acevedo Barroso et al.2024 · 622 citationsA&A 697, A1 (2025)
Ageing and Quenching through the ageing diagram II: physical characterization of galaxies2307.02024v2 · Pablo Corcho-Caballero, Yago Ascasibar, Luca Cortese et al.2023 · 8 citationsarXiv
Characterizing the ELG luminosity functions in the nearby Universe2303.11031v2 · G. Favole, V. Gonzalez-Perez, Y. Ascasibar et al.2023 · 8 citationsarXiv
The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation2212.03981v2 · Shoko Jin, Scott C. Trager, Gavin B. Dalton et al.2022 · 221 citationsarXiv
GRB 180325A: dust grain-size distribution and interstellar iron nanoparticles contribution2210.10423v1 · Elizabeth Cappellazzo, Tayyaba Zafar, Pablo Corcho-Caballero et al.2022 · 1 citationarXiv
Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints2208.14084v2 · Pablo Corcho-Caballero, Yago Ascasibar, Sebasti'an F. S'anchez et al.2022 · 13 citationsarXiv
Predicting interstellar radiation fields from chemical evolution models2203.04782v3 · Mario Romero, Pablo Corcho-Caballero, Iker Mill'an-Irigoyen et al.2022 · 2 citationsarXiv
Galaxy evolution on resolved scales: ageing and quenching in CALIFA2107.13478v1 · Pablo Corcho-Caballero (UAM, MQU), Javier Casado (UAM) et al.2021 · 12 citationsarXiv
Polynomial expansion of the star formation history in galaxies2105.08591v3 · D. Jim'enez-L'opez, P. Corcho-Caballero, S. Zamora et al.2021 · 5 citationsA&A 662, A1 (2022)
Do galaxies die? Different views from simulations and observations in the Local Universe2105.05298v2 · Pablo Corcho-Caballero (UAM, AAO-MQ), Yago Ascasibar (UAM) et al.2021 · 17 citationsarXiv
A single galaxy population? statistical evidence that the Star-Forming Main Sequence might be the tip of the iceberg2009.06931v1 · P. Corcho-Caballero, Y. Ascasibar, 'A. R. L'opez-S'anchez2020 · 15 citationsarXiv
Career total: at least 56 works. 30 are in this corpus.
Profile built from the corpus for this byline.
Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.