activity
20182021
most citedTime Inference with MUSE in Extragalactic Rings (TIMER): Properties of the Survey and High-Level Data Products

126 citations · 531 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2021★ 31 cited

NGC 5746: formation history of a massive disc-dominated galaxy

Marie Martig, Francesca Pinna, Jesús Falcón-Barroso +6

The existence of massive galaxies lacking a classical bulge has often been proposed as a challenge to CDM. However, recent simulations propose that a fraction of massive disc ga…

astro-ph.GA2021★ 20 cited

Mapping Accreted Stars in Early-Type Galaxies Across the Mass-Size Plane

Thomas A. Davison, Mark A. Norris, Ryan Leaman +3

Galaxy mergers are instrumental in dictating the final mass, structure, stellar populations, and kinematics of galaxies. Cosmological galaxy simulations indicate that the most mass…

astro-ph.GA2021★ 15 cited

Joint Gas and Stellar Dynamical Models of WLM: An isolated dwarf galaxy within a cored, prolate DM halo

Gigi Y. C. Leung, Ryan Leaman, Giuseppina Battaglia +4

We present multi-tracer dynamical models of the low mass (), isolated dwarf irregular galaxy WLM in order to simultaneously constrain the inner slope of the dark…

astro-ph.GA2021★ 8 cited

What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies

Meghan E. Hughes, Prashin Jethwa, Michael Hilker +8

Dynamical models allow us to connect the motion of a set of tracers to the underlying gravitational potential, and thus to the total (luminous and dark) matter distribution. They a…

astro-ph.GA2020★ 25 cited

Dynamical modelling of globular clusters: challenges for the robust determination of IMBH candidates

Francisco I. Aros, Anna C. Sippel, Alessandra Mastrobuono-Battisti +3

The presence or absence of intermediate-mass black holes (IMBHs) at the centre of Milky Way globular clusters (GCs) is still an open question. This is either due to observational r…

astro-ph.GA2020★ 21 cited

On the accretion of a new group of galaxies onto Virgo: I. Internal kinematics of nine in-falling dEs

Bahar Bidaran, Anna Pasquali, Thorsten Lisker +12

Galaxy environment has been shown to play an important role in transforming late-type, star-forming galaxies to quiescent spheroids. This transformation is expected to be more seve…

astro-ph.GA2020★ 38 cited

The SAMI -- Fornax Dwarfs Survey I: Sample, observations and the specific stellar angular momentum of dwarf elliptical galaxies

Nicholas Scott, F. Sara Eftekhari, Reynier F. Peletier +13

Dwarf ellipticals are the most common galaxy type in cluster environments, however the challenges associated with their observation mean their formation mechanisms are still poorly…

astro-ph.GA2019★ 15 cited

Mapping the dark matter halo of early-type galaxy NGC 2974 through orbit-based models with combined stellar and cold gas kinematics

Meng Yang, Ling Zhu, Anne-Marie Weijmans +4

We present an orbit-based method of combining stellar and cold gas kinematics to constrain the dark matter profile of early-type galaxies. We apply this method to early-type galaxy…

astro-ph.GA2019★ 35 cited

A dwarf-dwarf merger and dark matter core as a solution to the Globular Cluster problems in the Fornax dSph

Gigi Y. C. Leung, Ryan Leaman, Glenn van de Ven +1

The five globular clusters (GCs) of the Fornax dSph are puzzling for two reasons; the mass in GCs is high with respect to the galaxy's old stellar mass, and their survival and larg…

astro-ph.GA2019★ 21 cited

Is There a Fundamental Upper Limit to the Mass of a Star Cluster?

Mark A. Norris, Glenn van de Ven, Sheila J. Kannappan +2

The discovery around the turn of the millenium of a population of very massive (M > 210 M) compact stellar systems (CSS) with physical properties (radiu…

astro-ph.GA2019★ 34 cited

A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations

Dandan Xu, Ling Zhu, Robert Grand +16

Motivated by the recently discovered kinematic "Hubble sequence" shown by the stellar orbit-circularity distribution of 260 CALIFA galaxies, we make use of a comparable galaxy samp…

astro-ph.GA2019★ 43 cited

Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation

Yunpeng Jin, Ling Zhu, R. J. Long +4

We evaluate the capabilities of Schwarzschild's orbit-superposition method by applying it to galaxies from the large scale, high resolution Illustris simulation. Nine early-type ga…

astro-ph.GA2019★ 67 cited

Combining Stellar Populations with Orbit-Superposition Dynamical Modelling - the Formation History of the Lenticular Galaxy NGC 3115

Adriano Poci, Richard M. McDermid, Ling Zhu +1

We present a combination of the Schwarzschild orbit-superposition dynamical modelling technique with the spatially-resolved mean stellar age and metallicity maps to uncover the for…

astro-ph.GA2018★ 32 cited

Inner bars also buckle. The MUSE TIMER view of the double-barred galaxy NGC 1291

J. Mendez-Abreu, A. de Lorenzo-Caceres, D. A. Gadotti +8

Double bars are thought to be important features for secular evolution in the central regions of galaxies. However, observational evidence about their origin and evolution is still…

astro-ph.GA2018★ 126 cited

Time Inference with MUSE in Extragalactic Rings (TIMER): Properties of the Survey and High-Level Data Products

Dimitri A. Gadotti, Patricia Sánchez-Blázquez, Jesús Falcón-Barroso +14

The Time Inference with MUSE in Extragalactic Rings (TIMER) project is a survey with the VLT-MUSE integral-field spectrograph of 24 nearby barred galaxies with prominent central st…