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20002026
most citedObservations of the core of the Pleiades with the Chandra X-ray Observatory

18 citations · 42 across the 8 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2026

Halo stars harbour few wide ultracool companions

Jerry Jun-Yan Zhang, Nicolas Lodieu, Eduardo L. Martín

We conducted the first search for wide ultracool companions to metal-poor halo stars. A sample of nearby halo stars with spectroscopically determined metallicities and high proper…

astro-ph.SR2025

Euclid: Quick Data Release (Q1) -- Ultracool dwarfs in the Euclid Deep Fields

A. Mohandasan, R. L. Smart, C. Reylé +180

Ultracool dwarfs (UCDs) encompass the lowest-mass stars and brown dwarfs at the substellar boundary. These intrinsically faint objects are challenging to detect, but the wide cover…

astro-ph.SR2025

Detection of Methane in the Closest Extreme Metal-poor T Dwarf WISEA J181006.18-101000.5

Jerry Jun-Yan Zhang, Nicolas Lodieu, Eduardo L. Martín +7

WISEA J181006.18-101000.5 (WISE1810) is the nearest metal-poor ultracool dwarf to the Sun. It has a low effective temperature and has been classified as extreme early-T subdwarf. H…

astro-ph.SR2025★ 1 cited

Euclid: Quick Data Release (Q1) -- A photometric search for ultracool dwarfs in the Euclid Deep Fields

M. Žerjal, C. Dominguez-Tagle, N. Vitas +178

We present a catalogue of 5306 new ultracool dwarf (UCD) candidates in the three Euclid Deep Fields in the Q1 data release. They range from late M to late T dwarfs, and include 120…

astro-ph.SR2025★ 9 cited

Euclid Quick Data Release (Q1) -- Spectroscopic search, classification and analysis of ultracool dwarfs in the Deep Fields

C. Dominguez-Tagle, M. Žerjal, N. Sedighi +14

The Near-Infrared Spectrometer and Photometer onboard the Euclid space mission has obtained near-infrared (NIR) slitless spectra of millions of objects, including hundreds of ultra…

astro-ph.SR2023★ 13 cited

Young nearby open clusters and their luminosity functions

M. Žerjal, N. Lodieu, A. Pérez-Garrido +3

Context. Open clusters are groups of coeval stars sharing properties such as distance and metallicity, and they are key to understanding stellar evolution. Aims. Our main goal is t…