collaborators

6 papers

astro-ph.GA2026

FASTAR -- II. Semi-resolved evolutionary stellar population models

Ignacio Martín-Navarro, Alexandre Vazdekis, Luis Peralta de Arriba +12

Standard evolutionary synthesis models rely on the assumption of a fully sampled stellar initial mass function (IMF). Under this assumption, the age, chemical composition, and IMF…

astro-ph.GA2026

FASTAR -- I. Continuous and differentiable evolutionary stellar population models

Ignacio Martín-Navarro, Alexandre Vazdekis, Luis Peralta de Arriba +11

The development of evolutionary stellar population models is central to interpreting observations of galaxies in terms of astrophysical quantities. Stellar population models must t…

astro-ph.GA2026

Tracing the dynamical and structural complexity of spiral galaxy centres

Iris Breda, Glenn van de Ven, Sabine Thater +7

The formation of late-type galaxies has traditionally been described via two pathways: one producing pressure-supported classical bulges, the other rotationally supported pseudo-bu…

astro-ph.GA2026

Glance: A Comprehensive Framework for Galactic Archaeology

Iris Breda, Glenn van de Ven, Sabine Thater +8

A central topic in extragalactic astronomy is understanding the formation and evolutionary histories of galaxies. These systems often comprise multiple structural components with d…

astro-ph.GA2026

Orbital decomposition of the nuclear regions in the early-type galaxy FCC 47: Unveiling the nuclear cluster origin

Julia Lamprecht, Anja Feldmeier-Krause, Mariya Lyubenova +8

Nuclear star clusters (NSCs) are among the densest stellar systems in the Universe and often coexist with supermassive black holes (SMBHs) at galaxy centres. While SMBH formation h…

astro-ph.GA2025

3D Full Spectrum Fitting: Algorithm Comparison

Prashin Jethwa, Simon Hubmer, Ronny Ramlau +1

Full spectrum fitting is the prevailing method for extracting stellar kinematic and population measurements from 1D galaxy spectra. 3D methods refer to analysis of Integral Field S…