activity
20092026
most citedTOI-5005 b: A super-Neptune in the savanna near the ridge

33 citations · 49 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.EP2026

Two extremely irradiated volatile-rich sub-Neptunes with companions in the TOI-426 and TOI-1839 systems: Insights into arrival and survival near the lower edge of the Neptunian desert

A. Castro-González, O. Barragán, D. J. Armstrong +26

Using TESS photometry and 147 HARPS radial velocities, we confirm two extremely irradiated, volatile-rich sub-Neptunes near the lower edge of the Neptunian desert: TOI-426 b and TO…

astro-ph.EP2026★ 2 cited

Assessment of PLATO Science Performance

Juan Cabrera, Heike Rauer, Reza Samadi +121

The PLATO mission is scheduled for launch early 2027. In this paper we present an overview of the performance drivers for the mission at the time where all flight models of the cam…

astro-ph.GA2025

Mapping the Ages of Stars with Chemistry

Carlos Viscasillas Vázquez, Giada Casali, Laura Magrini +11

Chemical clocks, based on age-sensitive stellar abundance ratios, offer a powerful and scalable approach to reconstruct the formation history of the Milky Way. This white paper out…

astro-ph.EP2024★ 33 cited

TOI-5005 b: A super-Neptune in the savanna near the ridge

A. Castro-González, J. Lillo-Box, D. J. Armstrong +38

The Neptunian desert and savanna have recently been found to be separated by a ridge, an overdensity of planets in the period range of 3-5 days. These features are thought…

astro-ph.IM2024★ 12 cited

The Wide-field Spectroscopic Telescope (WST) Science White Paper

Vincenzo Mainieri, Richard I. Anderson, Jarle Brinchmann +214

The Wide-field Spectroscopic Telescope (WST) is proposed as a new facility dedicated to the efficient delivery of spectroscopic surveys. This white paper summarises the initial con…

astro-ph.SR2023

The PL diagram for Sct stars: back in business as distance estimators

A. García Hernández, J. Pascual-Granado, M. Lares-Martiz +4

In this work, we focus on the period-luminosity relation (PLR) of Sct stars, in which mode excitation and selection mechanisms are still poorly constrained, and whose structure…

astro-ph.SR2010

Towards a detection of individual g modes in the Sun

R. A. Garcia, J. Ballot, A. Eff-Darwich +10

Since the detection of the asymptotic properties of the dipole gravity modes in the Sun, the quest to find the individual gravity modes has continued. A deeper analysis of the GOLF…

astro-ph.SR2010

New Generation Stellar Physics: Asteroseismology & Virtual Observatory

J. C. Suárez, E. Solano, C. Rodrigo +2

In the last years we have witnessed a dramatic change in the research infrastructures: Advances in communication networks, computational resources and data storage devices are fost…

astro-ph.SR2010

Modelling delta Scuti stars using asteroseismic space data

A. Moya, A. García Hernández, J. -C. Suárez +2

In the last years, space missions such as COROT, Kepler or MOST have provided very accurate photometric observational data. In the particular case of Scuti stars, the observed…

astro-ph.SR2010

Sensitivity of the g-mode frequencies to pulsation codes and their parameters

A. Moya, S. Mathur, R. A. Garcia

From the recent work of the Evolution and Seismic Tools Activity (ESTA, Lebreton et al. 2006; Monteiro et al. 2008), whose Task 2 is devoted to compare pulsational frequencies comp…

astro-ph.SR2009★ 2 cited

Detecting individual gravity modes in the Sun: Chimera or reality?

Rafael A. Garcia, J. Ballot, A. Eff-Darwich +11

Over the past 15 years, our knowledge of the interior of the Sun has tremendously progressed by the use of helioseismic measurements. However, to go further in our understanding of…