activity
20192025
most citedThe wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

211 citations · 419 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2025★ 1 cited

Open clusters in the outer disc studied with MEGARA@GTC Auner 1 and Berkeley 102

J. Carbajo-Hijarrubia, R. Carrera, F. Anders +4

Open clusters offer crucial insights into stellar nucleosynthesis and the chemical evolution of the Galactic disc, as their ages and distances can be determined with higher accurac…

astro-ph.GA2024★ 13 cited

The Kinematics of 30 Milky Way Globular Clusters and the Multiple Stellar Populations within

Ellen Leitinger, Holger Baumgardt, Ivan Cabrera-Ziri +5

The spectroscopic and photometric classification of multiple stellar populations (MPs) in Galactic globular clusters (GCs) has enabled comparisons between contemporary observations…

astro-ph.GA2024★ 31 cited

OCCASO V. Chemical-abundance trends with Galactocentric distance and age

J. Carbajo-Hijarrubia, L. Casamiquela, R. Carrera +12

Context. Open clusters provide valuable information on stellar nucleosynthesis and the chemical evolution of the Galactic disc, as their age and distances can be measured more prec…

astro-ph.HE2024

The extreme coronal line emitter AT 2022fpx: Varying optical polarization properties and late-time X-ray flare

Karri I. I. Koljonen, Ioannis Liodakis, Elina Lindfors +8

Supermassive black holes disrupt passing stars, producing outbursts called tidal disruption events (TDEs). TDEs have recently gained attention due to their unique dynamics and emis…

astro-ph.IM2022★ 211 cited

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Shoko Jin, Scott C. Trager, Gavin B. Dalton +212

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree…

astro-ph.SR2022★ 16 cited

One Star to Tag Them All (OSTTA): I. Radial velocities and chemical abundances for 20 poorly studied open clusters

R. Carrera, L. Casamiquela, A. Bragaglia +9

Context: Open clusters are ideal laboratories to investigate a variety of astrophysical topics, from the properties of the Galactic disc to stellar evolution models. For this purpo…

astro-ph.SR2021★ 17 cited

OCCASO IV. Radial Velocities and Open Cluster Kinematics

R. Carrera, L. Casamiquela, J. Carbajo-Hijarrubia +8

Context: Open clusters (OCs) are widely used as test particles to investigate a variety of astrophysical phenomena, from stellar evolution to Galactic evolution. Gaia and the compl…

astro-ph.GA2021★ 58 cited

Abundance-age relations with red clump stars in open clusters

L. Casamiquela, C. Soubiran, P. Jofré +8

Context: Precise chemical abundances coupled with reliable ages are key ingredients to understand the chemical history of our Galaxy. Open Clusters (OCs) are useful for this purpos…

astro-ph.IM2019★ 21 cited

Clusterix 2.0. A Virtual Observatory tool to estimate cluster membership probability

L. Balaguer-Núñez, M. Lopez, E. Solano +6

Clusterix 2.0 is a web-based, Virtual Observatory-compliant, interactive tool for the determination of membership probabilities in stellar clusters based on proper motion data usin…

astro-ph.GA2019★ 51 cited

OCCASO III. Iron peak and elements of 18 open clusters. Comparison with chemical evolution models and field stars

L. Casamiquela, S. Blanco-Cuaresma, R. Carrera +10

The study of open-cluster chemical abundances provides insights on stellar nucleosynthesis processes and on Galactic chemo-dynamical evolution. In this paper we present an extended…