activity
20022024
most citedThe UKIRT Infrared Deep Sky Survey (UKIDSS)

2.5k citations · 6.5k across the 114 of their papers we have counts for

collaborators

111 papers

astro-ph.SR2024★ 7 cited

Primeval very low-mass stars and brown dwarfs -- VIII. The first age benchmark L subdwarf, a wide companion to a halo white dwarf

Z. H. Zhang, R. Raddi, A. J. Burgasser +12

We report the discovery of five white dwarf + ultracool dwarf systems identified as common proper motion wide binaries in the Gaia Catalogue of Nearby Stars. The discoveries includ…

astro-ph.SR2023★ 1 cited

Substellar science in the wake of the ESA Euclid space mission

Eduardo L. Martín, Hervé Bouy, Diego Martín +16

The ESA space mission Euclid was launched on July 1st, 2023 and is undergoing its science verification phase. In this invited review we show that Euclid means a before and an after…

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…

astro-ph.SR2023★ 6 cited

Optical Properties of Metal-poor T Dwarf Candidates

Jerry Jun-Yan Zhang, Nicolas Lodieu, Eduardo Martín

Context. Metal-poor brown dwarfs are poorly understood because they are extremely faint and rare. Only a few candidates have been identified as T-type subdwarfs in infrared surveys…

astro-ph.SR2023★ 10 cited

The CARMENES search for exoplanets around M dwarfs. Behaviour of the Paschen lines during flares and quiescence

B. Fuhrmeister, S. Czesla, J. H. M. M. Schmitt +17

The hydrogen Paschen lines are known activity indicators, but studies of them in M~dwarfs during quiescence are as rare as their reports in flare studies. This situation is mostly…

astro-ph.SR2023★ 9 cited

The cosmic waltz of Coma Berenices and Latyshev 2 (Group X). Membership, phase-space structure, mass, and energy distributions

J. Olivares, N. Lodieu, V. J. S. Béjar +3

Context. Open clusters (OCs) are fundamental benchmarks where theories of star formation and stellar evolution can be tested and validated. Coma Ber and Latyshev 2 (Group X) are th…