activity
20192026
most citedGlobular cluster numbers in dark matter haloes in a dual formation scenario: an empirical model within EMERGE

29 citations · 232 across the 53 of their papers we have counts for

collaborators
Showing 2025Show all

15 papers · 1 filter

astro-ph.GA2025

The MAGPI Survey: forward modelled gas-phase metallicity gradients in galaxies at

Yifan Mai, Scott M. Croom, Emily Wisnioski +19

We measure the seeing-deconvolved gas-phase metallicity gradients of 70 star-forming galaxies at from the MAGPI survey and investigate their relationship with galaxy pr…

astro-ph.GA2025★ 2 cited

The GECKOS Survey: Resolved, multiphase observations of mass-loading and gas density in the galactic wind of NGC 4666

Barbara Mazzilli Ciraulo, D. B. Fisher, R. Elliott +24

We present a multiphase, resolved study of the galactic wind extending from the nearby starburst galaxy NGC 4666. For this we use VLT/MUSE observations from the GECKOS program and…

astro-ph.GA2025★ 1 cited

Analysis of Galaxies at the Extremes: Failed Galaxy Progenitors in the MAGNETICUM Simulations

Jonah S. Gannon, Lucas C. Kimmig, Duncan A. Forbes +5

There is increasing observational evidence for a failed galaxy formation pathway for some ultradiffuse galaxies (UDGs) at low redshift however they currently lack simulated counter…

astro-ph.GA2025

A Census of Double-Peaked Lyman-alpha Emitters in MAGPI: Classification, Global Characteristics, and Spatially Resolved Properties

Tamal Mukherjee, Tayyaba Zafar, Themiya Nanayakkara +17

Double-peaked Ly profiles provide critical insights into gas kinematics and the distribution of neutral hydrogen (HI) from the interstellar to the intergalactic medium (ISM to I…

astro-ph.GA2025★ 1 cited

Living the stream: Properties and progenitors of tidal shells and streams around galaxies from Magneticum

Johannes Stoiber, Lucas M. Valenzuela, Rhea-Silvia Remus +4

Stellar shells and streams are remnants of satellite galaxies visible around galaxies. Advances in low-surface-brightness observations and increasing resolution of cosmological sim…

astro-ph.GA2025

Tidal features around simulated groups and cluster galaxies: Enhancement and suppression of merger events through environment in LSST-like mock observations

Aman Khalid, Sarah Brough, Garreth Martin +5

Generally, merger likelihood increases in denser environments; however, the large relative velocities at the centres of dense clusters are expected to reduce the likelihood of merg…

astro-ph.GA2025★ 1 cited

Towards Precision Cosmology With Improved PNLF Distances Using VLT-MUSE. III. Impact of Stellar Populations in Early-Type Galaxy

Azlizan A. Soemitro, Lucas M. Valenzuela, Martin M. Roth +5

Distance measurements using the planetary nebula luminosity function (PNLF) rely on the bright-end power-law cut-off magnitude (), which is defined by a number of the [OIII]$\…

astro-ph.GA2025★ 2 cited

The GECKOS survey: Jeans anisotropic models of edge-on discs uncover the impact of dust and kinematic structures

T. H. Rutherford, A. Fraser-McKelvie, E. Emsellem +17

The central regions of disc galaxies host a rich variety of stellar structures: nuclear discs, bars, bulges, and boxy-peanut (BP) bulges. These components are often difficult to di…

astro-ph.GA2025

The PICS Project: II. Circumnebular extinction variations and their effect on the planetary nebula luminosity function

Lucas M. Valenzuela, George H. Jacoby, Rhea-Silvia Remus +2

For decades, the theoretical understanding of planetary nebulae (PNe) has remained in tension with the observed universal bright-end cutoff of the PN luminosity function (PNLF). Th…

astro-ph.CO2025★ 5 cited

Encyclopedia Magneticum: Scaling Relations from Cosmic Dawn to Present Day

Klaus Dolag, Rhea-Silvia Remus, Lucas M. Valenzuela +10

Galaxy and halo scaling relations, connecting a broad range of parameters, are well established from observations. The origin of many of these relations and their scatter is still…

astro-ph.CO2025★ 1 cited

Go with the Flow: The Self-Similar and Non-Linear Behaviour of Large-Scale In- and Outflows and the Impact of Accretion Shocks from Galaxies to Galaxy Clusters

Benjamin A. Seidel, Rhea-Silvia Remus, Lucas M. Valenzuela +2

From the scale-free nature of gravity, the structure in the universe is expected to be self-similar on large scales. However, this self-similarity will eventually break down due to…

astro-ph.GA2025

The MAGPI Survey: the kinematic morphology-density relation (or lack thereof) and the Hubble sequence at

Caroline Foster, Mark W. Donoghoe, Andrew Battisti +26

This work presents visual morphological and dynamical classifications for 637 spatially resolved galaxies, most of which are at intermediate redshift (), in the Middle-Ag…

astro-ph.GA2025★ 17 cited

A new class of dark matter-free dwarf galaxies? I. Clues from FCC 224, NGC 1052-DF2 and NGC 1052-DF4

Maria Luisa Buzzo, Duncan A. Forbes, Aaron J. Romanowsky +8

The discovery of quiescent, dark matter (DM)-deficient ultra-diffuse galaxies (UDGs) with overluminous globular clusters (GCs) has challenged galaxy formation models within the Lam…

astro-ph.GA2025★ 1 cited

The MAGPI Survey: the subtle role of environment and not-so-subtle impact of generations of stars on galaxy dynamics

Caroline Foster, Sabine Bellstedt, Francesco DEugenio +23

The stellar age and mass of galaxies have been suggested as the primary determinants for the dynamical state of galaxies, with environment seemingly playing no or only a very minor…

astro-ph.GA2025★ 4 cited

The PICS Project. I. The impact of metallicity and helium abundance on the bright end of the planetary nebula luminosity function

Lucas M. Valenzuela, Marcelo M. Miller Bertolami, Rhea-Silvia Remus +1

Planetary nebulae (PNe) and their luminosity function (PNLF) in galaxies have been used as a cosmic distance indicator for decades, yet a fundamental understanding is still lacking…