activity
20122026
most cited4MOST: Project overview and information for the First Call for Proposals

311 citations · 1.9k across the 55 of their papers we have counts for

collaborators

56 papers

astro-ph.GA2026

Euclid: Data Release 1 (DR1) -- Fornax-7, an ultra-faint companion to the Fornax dwarf spheroidal galaxy? A remote star cluster or dwarf satellite of the Fornax dSph

T. Saifollahi, A. Lançon, A. M. N. Ferguson +165

We report the discovery of an ultra-faint stellar system in the vicinity of the Fornax dwarf spheroidal (dSph) galaxy in Euclid DR1. This system, which we designate Fornax-7, is lo…

astro-ph.SR2026

Euclid: The convective-transition gap of 47 Tuc

M. Libralato, M. Griggio, R. Gerasimov +140

We report the first detection of the `convective-transition gap' (also known as `M-dwarf gap') in the globular cluster 47 Tuc (NGC 104) thanks to Euclid data. This feature, linked…

astro-ph.GA2026

The VMC survey -- LV. The coherent expansion of the SMC

S. Vijayasree, F. Niederhofer, M. -R. L. Cioni +8

The Small Magellanic Cloud (SMC) exhibits significant kinematic disequilibrium due to interactions with the Large Magellanic Cloud (LMC). Here, we investigate the two-dimensional s…

astro-ph.GA2025

Hubble Space Telescope proper motions of Large Magellanic Cloud star clusters -- II. Kinematic structure of young and intermediate-age clusters

F. Niederhofer, L. Cullinane, D. Massari +14

In this paper, we explore the kinematic properties of a sample of 19 young (<1 Gyr) and intermediate-age (1-2.5 Gyr) massive star clusters within the Large Magellanic Cloud (LMC).…

astro-ph.SR2025

Serendipitous Discovery of a Faint Planetary Nebula in the Massive Young LMC Cluster NGC 1866

Howard E. Bond, Nate Bastian, Andrea Bellini +5

During an integral-field spectroscopic study of stars in the massive young open cluster NGC 1866 in the Large Magellanic Cloud, we serendipitously discovered a faint planetary nebu…

astro-ph.GA2025

Cluster Ages to Reconstruct the Milky Way Assembly (CARMA) IV. Chrono-dynamics of seven old star clusters in the Large Magellanic Cloud and the peculiar origin of NGC 1841

F. Niederhofer, D. Massari, F. Aguado-Agelet +15

In this study, we report conclusive evidence for an ancient star cluster that has been accreted by the Large Magellanic Cloud (LMC). By leveraging observations from the Hubble Spac…

astro-ph.SR2025

Testing the Role of Merging Binaries in the Formation of the Split Main Sequence in Young Clusters

Nate Bastian, Sebastian Kamann, Florian Niederhofer +1

A number of theories have been put forward to explain the bi-modal stellar rotational distribution observed in young massive clusters. These include stellar mergers and interaction…

astro-ph.SR2025

Tracing stellar rotation in young massive LMC clusters

Sebastian Kamann, Nate Bastian, Florian Niederhofer +8

We present a detailed analysis of stellar rotation along the main sequences of NGC 1866 and NGC 1856, two young (~200-300 Myr) massive clusters in the Large Magellanic Cloud, using…

astro-ph.GA2025★ 7 cited

The VMC survey -- LIV. The internal kinematics of the LMC with new VISTA observations

S. Vijayasree, F. Niederhofer, M. -R. L. Cioni +10

Context: Studying the internal kinematics of galaxies provides insights into their past evolution, current dynamics, and future trajectory. The Large Magellanic Cloud (LMC), as the…

astro-ph.GA2024

Hubble Space Telescope proper motions of Large Magellanic Cloud star clusters -- I. Catalogues and results for NGC 1850

F. Niederhofer, A. Bellini, V. Kozhurina-Platais +11

We present proper motion (PM) measurements for a sample of 23 massive star clusters within the Large Magellanic Cloud using multi-epoch data from the Hubble Space Telescope (HST).…

astro-ph.SR2022★ 40 cited

The effects of stellar rotation along the main sequence of the 100 Myr old massive cluster NGC 1850

Sebastian Kamann, Sara Saracino, Nate Bastian +13

Young star clusters enable us to study the effects of stellar rotation on an ensemble of stars of the same age and across a wide range in stellar mass and are therefore ideal targe…

astro-ph.GA2022

The VMC survey -- XLVI. Stellar proper motions in the centre of the Large Magellanic Cloud

F. Niederhofer, M. -R. L. Cioni, T. Schmidt +7

We present proper motion (PM) measurements within the central region of the Large Magellanic Cloud (LMC) using near-infrared data from the VISTA survey of the Magellanic Cloud syst…

astro-ph.GA2022★ 8 cited

The VMC survey -- XLV. Proper motion of the outer LMC and the impact of the SMC

Thomas Schmidt, Maria-Rosa L. Cioni, Florian Niederhofer +8

The Large Magellanic Cloud (LMC) is the most luminous satellite galaxy of the Milky Way and owing to its companion, the Small Magellanic Cloud (SMC), represents an excellent labora…

astro-ph.GA2021★ 17 cited

Presence of red giant population in the foreground stellar sub-structure of the Small Magellanic Cloud

Dizna James, Smitha Subramanian, Abinaya O. Omkumar +8

The eastern region of the Small Magellanic Cloud (SMC) is found to have a foreground stellar sub-structure, which is identified as a distance bimodality (12 kpc apart) in the previ…

astro-ph.GA2021★ 41 cited

The VMC survey -- XLIV: Mapping metallicity trends in the Large Magellanic Cloud using near-infrared passbands

Samyaday Choudhury, Richard de Grijs, Kenji Bekki +9

We have derived high-spatial-resolution metallicity maps covering 105~deg across the Large Magellanic Cloud (LMC) using near-infrared passbands from the VISTA Survey of t…

astro-ph.GA2021★ 3 cited

Role of host galaxy in the formation of multiple stellar populations: Analysis of NGC 1786 and NGC 1898

Viswajith Vanaraj, Florian Niederhofer, Paul Goudfrooij

Even after decades of research, the origin of multiple stellar populations in globular clusters remains enigmatic. The question as to whether the galaxy environment plays a role in…

astro-ph.GA2021★ 35 cited

Stellar substructures in the periphery of the Magellanic Clouds with the VISTA Hemisphere Survey from the red clump and other tracers

Dalal El Youssoufi, Maria-Rosa L. Cioni, Cameron P. M. Bell +11

We study the morphology of the stellar periphery of the Magellanic Clouds in search of substructure using near-infrared imaging data from the VISTA Hemisphere Survey (VHS). Based o…

astro-ph.GA2021★ 36 cited

The VMC survey -- XLI. Stellar proper motions within the Small Magellanic Cloud

F. Niederhofer, M. -R. L. Cioni, S. Rubele +13

We used data from the near-infrared VISTA survey of the Magellanic Cloud system (VMC) to measure proper motions (PMs) of stars within the Small Magellanic Cloud (SMC). The data ana…

astro-ph.GA2020★ 33 cited

Gaia view of a stellar sub-structure in front of the Small Magellanic Cloud

Abinaya O. Omkumar, Smitha Subramanian, Florian Niederhofer +6

Recent observational studies identified a foreground stellar sub-structure traced by red clump (RC) stars (~ 12 kpc in front of the main body) in the eastern regions of the Small M…

astro-ph.GA2020★ 15 cited

The intrinsic reddening of the Magellanic Clouds as traced by background galaxies -- II. The Small Magellanic Cloud

Cameron P. M. Bell, Maria-Rosa L. Cioni, A. H. Wright +23

We present a map of the total intrinsic reddening across ~34 deg of the Small Magellanic Cloud (SMC) derived using optical () and near-infrared (IR; …

astro-ph.GA2020★ 26 cited

The VMC survey -- XXXIX: Mapping metallicity trends in the Small Magellanic Cloud using near-infrared passbands

Samyaday Choudhury, Richard de Grijs, Stefano Rubele +7

We have derived high spatial resolution metallicity maps covering 42 deg across the Small Magellanic Cloud (SMC) in an attempt to understand its metallicity distribution…

astro-ph.GA2020★ 33 cited

The VMC survey -- XXXVIII. Proper motion of the Magellanic Bridge

Thomas Schmidt, Maria-Rosa L. Cioni, Florian Niederhofer +14

The Magellanic Clouds are a nearby pair of interacting dwarf galaxies and satellites of the Milky Way. Studying their kinematic properties is essential to understanding their origi…

astro-ph.GA2020★ 11 cited

Searching for globular cluster chemical anomalies on the main sequence of a young massive cluster

I. Cabrera-Ziri, J. S. Speagle, E. Dalessandro +9

The spectroscopic and photometric signals of the star-to-star abundance variations found in globular clusters seem to be correlated with global parameters like the cluster's metall…

astro-ph.SR2020★ 6 cited

The VMC survey -- XXXVI. Young stellar variability in the Large Magellanic Cloud

Viktor Zivkov, Joana M. Oliveira, Monika G. Petr-Gotzens +11

Studies of young stellar objects (YSOs) in the Galaxy have found that a significant fraction exhibit photometric variability. However, no systematic investigation has been conducte…