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20042023
most citedCARMENES input catalogue of M dwarfs. I. Low-resolution spectroscopy with CAFOS

196 citations · 3.9k across the 120 of their papers we have counts for

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Showing 2019Show all

8 papers · 1 filter

astro-ph.EP2019★ 44 cited

Exomoons in the habitable zones of M dwarfs

Héctor Martínez-Rodríguez, José Antonio Caballero, Carlos Cifuentes +2

M dwarfs host most of the exoplanets in the local Milky Way. Some of these planets, ranging from sub-Earths to super-Jupiters, orbit in their stars' habitable zones (HZs), although…

astro-ph.EP2019★ 74 cited

Water vapor detection in the transmission spectra of HD 209458 b with the CARMENES NIR channel

A. Sánchez-López, F. J. Alonso-Floriano, M. López-Puertas +31

Aims: We aim at detecting HO in the atmosphere of the hot Jupiter HD 209458 b and perform a multi-band study in the near infrared with CARMENES. Methods: The HO absorption…

physics.app-ph2019★ 54 cited

Correlating Photovoltaic Soiling Losses to Waveband and Single-Value Transmittance Measurements

Leonardo Micheli, Jose A. Caballero, Eduardo F. Fernandez +4

This paper presents the results of an investigation on the spectral losses of photovoltaic (PV) soiling. The transmittance of a glass coupon exposed to natural soiling outdoors in…

astro-ph.IM2019★ 8 cited

Voyage 2050 White Paper: All-Sky Visible and Near Infrared Space Astrometry

David Hobbs, Anthony Brown, Erik Høg +27

A new all-sky visible and Near-InfraRed (NIR) space astrometry mission with a wavelength cutoff in the K-band is not just focused on a single or small number of key science cases.…

astro-ph.SR2019★ 6 cited

J-PLUS: Discovery and characterisation of ultracool dwarfs using Virtual Observatory tools

E. Solano, E. L. Martín, J. A. Caballero +20

Ultracool dwarfs (UCDs) are objects with spectral types equal or later than M7. Most of them have been discovered using wide-field imaging surveys. The Virtual Observatory (VO) has…

astro-ph.EP2019★ 1 cited

Ultraviolet Spectropolarimetry as a Tool for Understanding the Diversity of Exoplanetary Atmospheres

L. Fossati, L. Rossi, D. Stam +19

The polarization state of starlight reflected by a planetary atmosphere uniquely reveals coverage, particle size, and composition of aerosols as well as changing cloud patterns. It…