activity
20092022
most cited4MOST: Project overview and information for the First Call for Proposals

311 citations · 1.5k across the 21 of their papers we have counts for

collaborators

22 papers

astro-ph.IM2022★ 1 cited

CUBES: a UV spectrograph for the future

S. Covino, S. Cristiani, J. M. Alcala' +86

In spite of the advent of extremely large telescopes in the UV/optical/NIR range, the current generation of 8-10m facilities is likely to remain competitive at ground-UV wavelength…

astro-ph.IM2022

CUBES, the Cassegrain U-Band Efficient Spectrograph

S. Cristiani, J. M. Alcalá, S. H. P. Alencar +74

In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at ground-UV wavelengths for the foreseeable future. The Casse…

astro-ph.IM2022★ 7 cited

CUBES Phase A design overview -- The Cassegrain U-Band Efficient Spectrograph for the Very Large Telescope

Alessio Zanutta, Stefano Cristiani, David Atkinson +51

We present the baseline conceptual design of the Cassegrain U-Band Efficient Spectrograph (CUBES) for the Very Large Telescope. CUBES will provide unprecedented sensitivity for spe…

astro-ph.IM2020

MOSAIC: the high-multiplex and multi-IFU spectrograph for the ELT

Rubén Sánchez-Janssen, Francois Hammer, Simon Morris +40

MOSAIC is the planned multi-object spectrograph for the 39m Extremely Large Telescope (ELT). Conceived as a multi-purpose instrument, it offers both high multiplex and multi-IFU ca…

astro-ph.EP2019★ 130 cited

A giant exoplanet orbiting a very low-mass star challenges planet formation models

J. C. Morales, A. J. Mustill, I. Ribas +179

Statistical analyses from exoplanet surveys around low-mass stars indicate that super-Earth and Neptune-mass planets are more frequent than gas giants around such stars, in agreeme…

astro-ph.GA2019★ 1 cited

3C 294 revisited: Deep Large Binocular Telescope AO NIR images and optical spectroscopy

J. Heidt, A. Quirrenbach, N. Hoyer +11

Context. High redshift radio galaxies are among the most massive galaxies at their redshift, are often found at the center of protoclusters of galaxies, and are expected to evolve…