activity
20192026
most citedDESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

1.1k citations · 3.1k across the 50 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2024★ 9 cited

Validating the clustering predictions of empirical models with the FLAMINGO simulations

Sergio Contreras, Raul E. Angulo, Jonás Chaves-Montero +3

Context. Mock galaxy catalogues are essential for correctly interpreting current and future generations of galaxy surveys. Despite their significance in galaxy formation and cosmol…

astro-ph.GA2023

Active galactic nuclei and gravitational redshifts

N. D. Padilla, S. Carneiro, J. Chaves-Montero +4

Context: Gravitational redshift is a classical effect of Einstein's General Relativity, already measured in stars, quasars and clusters of galaxies. Aims: We here aim to identify t…

astro-ph.GA2023★ 12 cited

The miniJPAS survey quasar selection II: Machine learning classification with photometric measurements and uncertainties

Natália V. N. Rodrigues, L. Raul Abramo, Carolina Queiroz +23

Astrophysical surveys rely heavily on the classification of sources as stars, galaxies or quasars from multi-band photometry. Surveys in narrow-band filters allow for greater discr…

astro-ph.GA2023★ 20 cited

The miniJPAS survey: AGN & host galaxy co-evolution of X-ray selected sources

I. E. López, M. Brusa, S. Bonoli +35

Studies indicate strong evidence of a scaling relation in the local Universe between the supermassive black hole mass ($M_\rm{BH}$) and the stellar mass of their host galaxies ($M_…

astro-ph.GA2022★ 4 cited

Tracking the evolution of satellite galaxies: mass stripping and dark-matter deficient galaxies

Antonio D. Montero-Dorta, Facundo Rodriguez, M. Celeste Artale +2

Satellite galaxies undergo a variety of physical processes when they are accreted by groups and clusters, often resulting in the loss of baryonic and dark matter (DM) mass. In this…

astro-ph.GA2022★ 26 cited

Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History

Alex Alarcon, Andrew P. Hearin, Matthew R. Becker +1

We present Diffstar, a smooth parametric model for the in-situ star formation history (SFH) of galaxies. Diffstar is distinct from conventional SFH models that are used to interpre…

astro-ph.GA2022

The miniJPAS survey quasar selection I: Mock catalogues for classification

Carolina Queiroz, L. Raul Abramo, Natália V. N. Rodrigues +27

In this series of papers, we employ several machine learning (ML) methods to classify the point-like sources from the miniJPAS catalogue, and identify quasar candidates. Since no r…

astro-ph.GA2021★ 20 cited

DSPS: Differentiable Stellar Population Synthesis

Andrew P. Hearin, Jonás Chaves-Montero, Alex Alarcon +2

Models of stellar population synthesis (SPS) are the fundamental tool that relates the physical properties of a galaxy to its spectral energy distribution (SED). In this paper, we…

astro-ph.GA2021★ 9 cited

Black hole virial masses from single-epoch photometry: the miniJPAS test case

Jonás Chaves-Montero, Silvia Bonoli, Benny Trakhtenbrot +25

Precise measurements of black hole masses are essential to understanding the coevolution of these sources and their host galaxies. We develop a novel approach for computing black h…

astro-ph.GA2021★ 48 cited

On the influence of halo mass accretion history on galaxy properties and assembly bias

Antonio D. Montero-Dorta, Jonás Chaves-Montero, M. Celeste Artale +1

Halo assembly bias is the secondary dependence of the clustering of dark-matter haloes on their assembly histories at fixed halo mass. This established dependence is expected to ma…

astro-ph.GA2021★ 20 cited

Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies

Jonas Chaves-Montero, Andrew Hearin

Among the properties shaping the light of a galaxy, the star formation history (SFH) is one of the most challenging to model due to the variety of correlated physical processes reg…