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20032026
most citedCALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation

1.3k citations · 13.5k across the 186 of their papers we have counts for

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23 papers · 1 filter

astro-ph.GA2023★ 1 cited

The universal variability of the stellar initial mass function probed by the TIMER survey

Ignacio Martín-Navarro, Adriana de Lorenzo-Cáceres, Dimitri A. Gadotti +7

The debate about the universality of the stellar initial mass function (IMF) revolves around two competing lines of evidence. While measurements in the Milky Way, an archetypal spi…

astro-ph.GA2023

The SAMI -- Fornax Dwarfs Survey IV. Star Formation Histories of Dwarf and Early-Type Galaxies: Insights from Full Spectral Fitting

J. Romero-Gómez, J. A. L. Aguerri, Reynier F. Peletier +3

We present a study on the star formation histories (SFHs) of galaxies covering the range < M/M < , leveraging full spectral fitting algorithms…

astro-ph.GA2023★ 4 cited

Total mass slopes and enclosed mass constrained by globular cluster system dynamics

Tadeja Veršič, Sabine Thater, Glenn van de Ven +4

The goal of this work is to probe the total mass distribution of early-type galaxies with globular clusters (GCs) as kinematic tracers, by constraining the parameters of the profil…

astro-ph.GA2023

The distribution of stellar orbits in Eagle galaxies -- the effect of mergers, gas accretion, and secular evolution

Giulia Santucci, Claudia Del P. Lagos, Katherine E. Harborne +9

The merger history of a galaxy is thought to be one of the major factors determining its internal dynamics, with galaxies having undergone different types or mergers (e.g. dry, min…

astro-ph.GA2023★ 16 cited

Quantifying the stellar ages of dynamically separated bulges and disks of CALIFA spiral galaxies

Yunpeng Jin, Ling Zhu, Stefano Zibetti +3

We employ a recently developed population-orbit superposition technique to simultaneously fit the stellar kinematic and age maps of 82 CALIFA spiral galaxies and obtain the ages of…

astro-ph.GA2023★ 1 cited

Schwarzschild Modeling of Barred S0 Galaxy NGC 4371

Behzad Tahmasebzadeh, Ling Zhu, Juntai Shen +15

We apply the barred Schwarzschild method developed by Tahmasebzadeh et al. (2022) to a barred S0 galaxy, NGC 4371, observed by IFU instruments from the TIMER and ATLAS3D projects.…

astro-ph.GA2023★ 8 cited

Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSE

Teodora-Elena Bulichi, Katja Fahrion, François Mernier +10

The mass-metallicity relation (MZR) represents one of the most important scaling relations in the context of galaxy evolution, comprising a positive correlation between stellar mas…

astro-ph.GA2023★ 6 cited

Dark Matter Fraction in Disk-Like Galaxies Over the Past 10 Gyr

G. Sharma, G. van de Ven, P. Salucci +1

We present an observational study of the dark matter fraction in star-forming disk-like galaxies up to redshift , selected from publicly available integral field spectr…

astro-ph.GA2023★ 28 cited

oMEGACat I: MUSE spectroscopy of 300,000 stars within the half-light radius of Centauri

M. S. Nitschai, N. Neumayer, C. Clontz +17

Omega Centauri ( Cen) is the most massive globular cluster of the Milky Way and has been the focus of many studies that reveal the complexity of its stellar populations and kine…

astro-ph.GA2023

On the accretion of a new group of galaxies onto Virgo: III. The stellar population radial gradients of dEs

Bahar Bidaran, Francesco La Barbera, Anna Pasquali +6

Using MUSE data, we investigate the radial gradients of stellar population properties (namely age, [M/H], and the abundance ratio of elements [/Fe]) for a sample of nine dwa…

astro-ph.GA2023★ 14 cited

Disc galaxies are still settling: The discovery of the smallest nuclear discs and their young stellar bars

Camila de Sá-Freitas, Dimitri A. Gadotti, Francesca Fragkoudi +11

When galactic discs settle and become massive enough, they are able to form stellar bars. These non-axisymmetric structures induce shocks in the gas, causing it to flow to the cent…

astro-ph.GA2023★ 2 cited

Stellar Half-Mass Radii of Galaxies: Comparison with JWST/NIRCam Half-Light Radii

Arjen van der Wel, Marco Martorano, Boris Haussler +12

We use CEERS JWST/NIRCam imaging to measure rest-frame near-IR light profiles of 500 galaxies in the redshift range . We compare the resulti…

astro-ph.GA2023

ReveaLLAGN 0: First Look at JWST MIRI data of Sombrero and NGC 1052

K. Goold, A. Seth, M. Molina +28

We present the first results from the Revealing Low-Luminosity Active Galactic Nuclei (ReveaLLAGN) survey, a JWST survey of seven nearby LLAGN. We focus on two observations with th…

astro-ph.GA2023★ 13 cited

Composite Bulges -- IV. Detecting Signatures of Gas Inflows in the IFU data: The MUSE View of Ionized Gas Kinematics in NGC 1097

Tutku Kolcu, Witold Maciejewski, Dimitri A. Gadotti +8

Using VLT/MUSE integral-field spectroscopic data for the barred spiral galaxy NGC 1097, we explore techniques that can be used to search for extended coherent shocks that can drive…

astro-ph.GA2023

The flattening of dark matter halo of Centaurus A galaxy (NGC 5128) out to 40 kpc

Tadeja Veršič, Marina Rejkuba, Magda Arnaboldi +4

Cosmological simulations predict dark matter shapes that deviate from spherical symmetry. The exact shape depends on the prescription of the simulation and the interplay between da…

astro-ph.GA2023★ 3 cited

Dynamical modelling of ATLAS galaxies

Sabine Thater, Prashin Jethwa, Edward J. Lilley +3

Triaxial dynamical models of massive galaxies observed in the ATLAS3D project can provide new insights into the complex evolutionary processes that shape galaxies. The ATLAS3D surv…

astro-ph.GA2023★ 12 cited

NGC 1436: the making of a lenticular galaxy in the Fornax cluster

Alessandro Loni, Paolo Serra, Marc Sarzi +25

We study the evolutionary path of the Fornax cluster galaxy NGC1436, which is known to be currently transitioning from a spiral into a lenticular morphology. This galaxy hosts a…

astro-ph.GA2023★ 18 cited

Effect of the initial mass function on the dynamical SMBH mass estimate in the nucleated early-type galaxy FCC 47

Sabine Thater, Mariya Lyubenova, Katja Fahrion +4

Supermassive black holes (SMBHs) and nuclear star clusters (NSCs) co-exist in many galaxies. While the formation history of the black hole is essentially lost, NSCs preserve their…

astro-ph.GA2023★ 21 cited

The SAMI-Fornax Dwarfs Survey III: Evolution of [/Fe] in dwarfs, from Galaxy Clusters to the Local Group

J. Romero-Gómez, Reynier F. Peletier, J. A. L. Aguerri +10

Using very deep, high spectral resolution data from the SAMI Integral Field Spectrograph we study the stellar population properties of a sample of dwarf galaxies in the Fornax Clus…

astro-ph.GA2023★ 21 cited

The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies

Giulia Santucci, Sarah Brough, Jesse van de Sande +11

Most dynamical models of galaxies to date assume axisymmetry, which is not representative of a significant fraction of massive galaxies. We have built triaxial orbit-superposition…

astro-ph.GA2023★ 19 cited

The Fornax3D project: Environmental effects on the assembly of dynamically cold disks in Fornax cluster galaxies

Y. Ding, L. Zhu, G. van de Ven +12

We apply a population-orbit superposition method to 16 galaxies in the Fornax cluster observed with MUSE/VLT in the context of the Fornax3D project. By fitting the luminosity distr…

astro-ph.GA2023★ 5 cited

A general basis set algorithm for galactic haloes and discs

E. J. Lilley, G. van de Ven

We present a unified approach to (bi-)orthogonal basis sets for gravitating systems. Central to our discussion is the notion of mutual gravitational energy, which gives rise to the…

astro-ph.GA2023★ 9 cited

The vertical structure of the spiral galaxy NGC 3501: first stages of the formation of a thin metal-rich disc

Natascha Sattler, Francesca Pinna, Nadine Neumayer +5

We trace the evolution of the edge-on spiral galaxy NGC 3501, making use of its stellar populations extracted from deep integral-field spectroscopy MUSE observations. We present st…