activity
20122026
most citedESPRESSO@VLT -- On-sky performance and first results

537 citations · 4.4k across the 88 of their papers we have counts for

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Showing 2022Show all

14 papers · 1 filter

astro-ph.EP2022★ 55 cited

Detection of barium in the atmospheres of the ultra-hot gas giants WASP-76b and WASP-121b

T. Azevedo Silva, O. D. S. Demangeon, N. C. Santos +33

High-resolution spectroscopy studies of ultra-hot Jupiters have been key in our understanding of exoplanet atmospheres. Observing into the atmospheres of these giant planets allows…

astro-ph.EP2022★ 56 cited

The GAPS Programme at TNG. XLI. The climate of KELT-9b revealed with a new approach to high spectral resolution phase curves

L. Pino, M. Brogi, J. M. Désert +25

[Abridged] We present a novel method to study the thermal emission of exoplanets as a function of orbital phase at very high spectral resolution, and apply it to investigate the cl…

astro-ph.EP2022★ 19 cited

Planetary parameters, XUV environments and mass-loss rates for nearby gaseous planets with X-ray detected host-stars

R. Spinelli, E. Gallo, F. Haardt +4

We leverage Gaia DR2 parallactic distances to deliver new or revised estimates of planetary parameters and X-ray irradiation for a distance-limited ( pc) sample of 27…

astro-ph.EP2022★ 50 cited

The GAPS Programme at TNG XXXVIII. Five molecules in the atmosphere of the warm giant planet WASP-69b detected at high spectral resolution

G. Guilluy, P. Giacobbe, I. Carleo +32

The field of exo-atmospheric characterisation is progressing at an extraordinary pace. Atmospheric observations are now available for tens of exoplanets, mainly hot and warm inflat…

astro-ph.EP2022★ 39 cited

The GAPS Programme at TNG XXXIX -- Multiple molecular species in the atmosphere of the warm giant planet WASP-80 b unveiled at high resolution with GIANO-B

Ilaria Carleo, Paolo Giacobbe, Gloria Guilluy +28

Detections of molecules in the atmosphere of gas giant exoplanets allow us to investigate the physico-chemical properties of the atmospheres. Their inferred chemical composition is…

astro-ph.EP2022★ 16 cited

The GAPS Programme at TNG XL: A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422

L. Naponiello, L. Mancini, M. Damasso +55

We investigate the exoplanet candidate TOI-1422b, which was discovered by the TESS space telescope around the high proper-motion G2V star TOI-1422 ( mag), 155pc away, with…

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.EP2022★ 46 cited

The GAPS Programme with HARPS-N at TNG. XXXVII. A precise density measurement of the young ultra-short period planet TOI-1807 b

D. Nardiello, L. Malavolta, S. Desidera +38

Great strides have been made in recent years in the understanding of the mechanisms involved in the formation and evolution of planetary systems; despite this, many observational f…

astro-ph.SR2022★ 58 cited

The GAPS Programme with HARPS-N at TNG. XXXV. Fundamental properties of transiting exoplanet host stars

K. Biazzo, V. D'Orazi, S. Desidera +38

Exoplanetary properties depend on stellar properties: to know the planet with accuracy and precision it is necessary to know the star as accurately and precisely as possible. Our i…

astro-ph.EP2022★ 13 cited

A giant planet shaping the disk around the very low-mass star CIDA 1

P. Curone, A. F. Izquierdo, L. Testi +13

(Abridged) Exoplanetary research has provided us with exciting discoveries of planets around very low-mass (VLM) stars (e.g., TRAPPIST-1 and Proxima Centauri). However, current the…

astro-ph.EP2022★ 28 cited

The GAPS Programme at TNG XXXIII. HARPS-N detects multiple atomic species in emission from the dayside of KELT-20b

F. Borsa, P. Giacobbe, A. S. Bonomo +31

The detection of lines in emission in planetary atmospheres provides direct evidence of temperature inversion. We confirm the trend of ultra-hot Jupiters orbiting A-type stars show…

astro-ph.EP2022★ 34 cited

The PEPSI Exoplanet Transit Survey (PETS) I: Investigating the presence of a silicate atmosphere on the super-Earth 55 Cnc e

Engin Keles, Matthias Mallonn, Daniel Kitzmann +26

The study of exoplanets and especially their atmospheres can reveal key insights on their evolution by identifying specific atmospheric species. For such atmospheric investigations…

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…

astro-ph.EP2022★ 10 cited

CaRM: Exploring the chromatic Rossiter-McLaughlin effect. The cases of HD 189733b and WASP-127b

E. Cristo, N. C. Santos, O. Demangeon +34

In this paper we introduce CaRM, a semi-automatic code for the retrieval of broadband transmission spectra of transiting planets through the chromatic Rossiter-McLaughlin method. W…