activity
20042026
most citedProperties of RR Lyrae stars in the Inner Regions of the Large Magellanic Cloud

63 citations · 89 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2026

ESO User Support and Observation Preparation for VLTI Science Operations

M. Wittkowski, G. Beccari, A. Corporaal +15

We present recent enhancements to VLTI observing capabilities from a user-oriented perspective, together with new developments in ESO's Observation Handling Tools and end-to-end op…

astro-ph.IM2026

ESOFinder: an LLM-powered tool to help users navigate ESO documentation

P. Sánchez-Sáez, C. Reinero, M. Vioque +6

The large amount and diversity of documentation available for users of the European Southern Observatory (ESO), spanning the full observing lifecycle from proposal preparation and…

astro-ph.GA2025

Absolute Calibration of Cluster Mira Variables to Provide a New Anchor for the Hubble Constant Determination

Anupam Bhardwaj, Noriyuki Matsunaga, Caroline D. Huang +2

Mira variables in globular clusters can provide an accurate and precise absolute calibration of their period-luminosity relations (PLRs) to independently anchor the cosmic distance…

astro-ph.SR2025★ 3 cited

The VMC Survey -- LIV. Anomalous Cepheids in the Magellanic Clouds Period-Luminosity relations in the near-infrared bands

Teresa Sicignano, Vincenzo Ripepi, Marina Rejkuba +12

Anomalous Cepheids (ACs) are less studied metal-poor pulsating stars ([Fe/H]<-1.5) compared to Classical Cepheids (CCs) and RR Lyrae stars. They follow distinct Period-Luminosity (…

astro-ph.SR2025

Euclid Quick Data Release (Q1) Ultracool dwarfs in the Euclid Deep Field North

A. Mohandasan, R. L. Smart, C. Reylé +176

Ultracool dwarfs (UCDs) encompass the lowest mass stars and brown dwarfs, defining the stellar substellar boundary. They have significant potential for advancing the understanding…

astro-ph.SR2021★ 23 cited

Towards a more complete sample of binary central stars of planetary nebulae with Gaia

N. Chornay, N. A. Walton, D. Jones +3

Context: Many if not most planetary nebulae (PNe) are now thought to be the outcome of binary evolutionary scenarios. However only a few percent of PNe in the Milky Way are known t…