activity
20172022
most citedA giant exoplanet orbiting a very low-mass star challenges planet formation models

130 citations · 481 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.IM202227 cited

MAROON-X: The first two years of EPRVs from Gemini North

Andreas Seifahrt, Jacob L. Bean, David Kasper +11

MAROON-X is a fiber-fed, optical EPRV spectrograph at the 8-m Gemini North Telescope on Mauna Kea, Hawai'i. MAROON-X was commissioned as a visiting instrument in December 2019 and…

astro-ph.IM20221 cited

The CUBES Science Case

Chris Evans, Stefano Cristiani, Cyrielle Opitom +51

We introduce the scientific motivations for the development of the Cassegrain U-Band Efficient Spectrograph (CUBES) that is now in construction for the Very Large Telescope. The as…

astro-ph.IM2022

CUBES and its software ecosystem: instrument simulation, control, and data processing

Giorgio Calderone, Roberto Cirami, Guido Cupani +11

CUBES (Cassegrain U-Band Efficient Spectrograph) is the recently approved high-efficiency VLT spectrograph aimed to observe the sky in the UV ground-based region (305-400 nm) with…

astro-ph.IM202151 cited

On-sky commissioning of MAROON-X: A new precision radial velocity spectrograph for Gemini North

A. Seifahrt, J. L. Bean, J. Stürmer +10

MAROON-X is a fiber-fed, red-optical, high precision radial velocity spectrograph recently commissioned at the Gemini North telescope on Mauna Kea, Hawai'i. With a resolving power…

astro-ph.EP202178 cited

A nearby transiting rocky exoplanet that is suitable for atmospheric investigation

T. Trifonov, J. A. Caballero, J. C. Morales +66

Spectroscopy of transiting exoplanets can be used to investigate their atmospheric properties and habitability. Combining radial velocity (RV) and transit data provides additional…

astro-ph.EP2019130 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…