activity
19962026
most citedEuclid Definition Study Report

924 citations · 8.7k across the 152 of their papers we have counts for

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16 papers · 1 filter

astro-ph.EP2022★ 14 cited

Search for planets around stars with wide brown dwarfs

J. Šubjak, N. Lodieu, P. Kabáth +6

Aims. The project aims to understand better the role of wide brown dwarf companions on planetary systems. Methods. We obtained high-resolution spectra of six bright stars with co-m…

astro-ph.SR2022★ 19 cited

The CARMENES search for exoplanets around M dwarfs. Variability on long timescales as seen in chromospheric indicators

B. Fuhrmeister, S. Czesla, V. Perdelwitz +19

It is clearly established that the Sun has an 11-year cycle that is caused by its internal magnetic field. This cycle is also observed in a sample of M dwarfs. In the framework of…

astro-ph.SR2022★ 16 cited

Espresso observations of HE 01075240 and other CEMP-no stars with

D. Aguado, P. Molaro, E. Caffau +22

HE 01075240 is a hyper metal-poor star with . We performed high-res observations with the ESPRESSO spectrograph at the VLT to constrain the kinematical propert…

astro-ph.EP2022★ 38 cited

Automatic model-based telluric correction for the ESPRESSO data reduction software. Model description and application to radial velocity computation

R. Allart, C. Lovis, J. Faria +21

Ground-based high-resolution spectrographs are key instruments for several astrophysical domains. Unfortunately, the observed spectra are contaminated by the Earth's atmosphere. Wh…

astro-ph.EP2022★ 18 cited

Precise mass determination for the keystone sub-Neptune planet transiting the mid-type M dwarf G 9-40

R. Luque, G. Nowak, T. Hirano +45

Context. Despite being a prominent subset of the exoplanet population discovered in the past three decades, the nature and provenance of sub-Neptune-sized planets are still one of…

astro-ph.SR2022★ 21 cited

Physical properties and trigonometric distance of the peculiar dwarf WISE J181005.5101002.3

N. Lodieu, M. R. Zapatero Osorio, E. L. Martin +2

Our goal is to characterise the physical properties of the metal-poor brown dwarf population. In particular, we focus on the recently discovered peculiar dwarf WISE J18100551010…

astro-ph.EP2022★ 8 cited

HORuS transmission spectroscopy and revised planetary parameters of KELT-7b

H. M. Tabernero, M. R. Zapatero Osorio, C. Allende Prieto +7

We report on the high-resolution spectroscopic observations of two planetary transits of the hot Jupiter KELT-7b ( 1.28 0.17 M, 20…

astro-ph.EP2022★ 14 cited

A hot sub-Neptune in the desert and a temperate super-Earth around faint M dwarfs: Color validation of TOI-4479b and TOI-2081b

E. Esparza-Borges, H. Parviainen, F. Murgas +45

We report the discovery and validation of two TESS exoplanets orbiting faint M dwarfs: TOI-4479b and TOI-2081b. We have jointly analyzed space (TESS mission) and ground based (MuSC…

astro-ph.EP2022★ 47 cited

A detailed analysis of the Gl 486 planetary system

J. A. Caballero, E. Gonzalez-Alvarez, M. Brady +64

The Gl 486 system consists of a very nearby, relatively bright, weakly active M3.5 V star at just 8 pc with a warm transiting rocky planet of about 1.3 R_Terra and 3.0 M_Terra that…

astro-ph.EP2022★ 27 cited

Transmission spectroscopy of MASCARA-1b with ESPRESSO: Challenges of overlapping orbital and Doppler tracks

N. Casasayas-Barris, F. Borsa, E. Pallé +32

Atmospheric studies at high spectral resolution have shown the presence of molecules, neutral and ionised metals, and hydrogen in the transmission spectrum of ultra-hot Jupiters, a…

astro-ph.CO2022★ 8 cited

Fundamental physics with ESPRESSO: Constraints on Bekenstein and dark energy models from astrophysical and local probes

C. J. A. P. Martins, S. Cristiani, G. Cupani +21

Dynamical scalar fields in an effective four-dimensional field theory are naturally expected to couple to the rest of the theory's degrees of freedom, unless some new symmetry is p…

astro-ph.EP2022★ 35 cited

A novel framework for semi-Bayesian radial velocities through template matching

A. M. Silva, J. P. Faria, N. C. Santos +28

The detection and characterization of an increasing variety of exoplanets has been in part possible thanks to the continuous development of high-resolution, stable spectrographs, a…

astro-ph.EP2022★ 19 cited

A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514. A super-Earth on an eccentric orbit moving in and out of the habitable zone

M. Damasso, M. Perger, J. M. Almenara +31

We investigated the presence of planetary companions around the nearby (7.6 pc) and bright ( mag) early-type M dwarf Gl 514, analysing 540 radial velocities collected over nea…

astro-ph.EP2022★ 35 cited

The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc

R. Luque, B. J. Fulton, M. Kunimoto +64

We report the discovery of a multi-planetary system transiting the M0 V dwarf HD 260655 (GJ 239, TOI-4599). The system consists of at least two transiting planets, namely HD 260655…

astro-ph.EP2022★ 30 cited

The CARMENES search for exoplanets around M dwarfs: Two Saturn-mass planets orbiting active stars

A. Quirrenbach, V. M. Passegger, T. Trifonov +26

The CARMENES radial-velocity survey is currently searching for planets in a sample of 387 M dwarfs. Here we report on two Saturn-mass planets orbiting TYC 2187-512-1 ($M_\star = 0.…

astro-ph.EP2022★ 41 cited

The polar orbit of the warm Neptune GJ436b seen with VLT/ESPRESSO

V. Bourrier, M. R. Zapatero Osorio, R. Allart +24

GJ436b might be the prototype of warm Neptunes that have undergone late migration induced by an outer companion. Precise determination of the orbital architecture of such systems i…