activity
20182025
most citedThe Li-age correlation: the Sun is unusually Li deficient for its age

65 citations · 334 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2025

A High-Resolution NUV Transmission Spectrum of KELT-9b: Mg II and Fe II Escaping from the Hottest Known Giant Planet

Austin Baldwin, Joshua D. Lothringer, Leonardo A. Dos Santos +5

We present high-resolution NUV observations from Hubble Space Telescope's (HST) Space Telescope Imaging Spectrograph (STIS) data for the hottest known gas planet, KELT-9b. Observat…

astro-ph.EP2025★ 1 cited

Tracing the Winds: A Uniform Interpretation of Helium Escape in Exoplanets from Archival Spectroscopic Observations

Patrick McCreery, Leonardo A. Dos Santos, Néstor Espinoza +2

Over the past decade, observations of evaporating exoplanets have become increasingly common, driven by the discovery of the near-infrared helium-triplet line as a powerful probe o…

astro-ph.EP2025

Stellar X-ray variability and planetary evolution in the DS Tucanae system

George W. King, Lía R. Corrales, Vincent Bourrier +5

We present an analysis of four Chandra observations of the 45 Myr old DS Tuc binary system. We observed X-ray variability of both stars on timescales from hours to months, includin…

astro-ph.EP2022★ 5 cited

Observations of planetary winds and outflows

Leonardo A. Dos Santos

We have recently hit the milestone of 5,000 exoplanets discovered. In stark contrast with the Solar System, most of the exoplanets we know to date orbit extremely close to their ho…

astro-ph.EP2022★ 59 cited

Water and an escaping helium tail detected in the hazy and methane-depleted atmosphere of HAT-P-18b from JWST NIRISS/SOSS

Guangwei Fu, Néstor Espinoza, David K. Sing +11

JWST is here. The early release observation program (ERO) provides us with the first look at the scientific data and the spectral capabilities. One of the targets from ERO is HAT-P…

astro-ph.EP2022★ 5 cited

The Hubble PanCET program: Emission spectrum of hot Jupiter HAT-P-41b

Guangwei Fu, David K. Sing, Drake Deming +6

We present the most complete emission spectrum for inflated hot Jupiter HAT-P-41b combining new HST WFC/G141 spectrum from the Hubble Panchromatic Comparative Exoplanet Treasury (P…

astro-ph.EP2022★ 16 cited

The Maximum Mass-Loss Efficiency for a Photoionization-Driven Isothermal Parker Wind

Shreyas Vissapragada, Heather A. Knutson, Leonardo A. dos Santos +2

Observations of present-day mass-loss rates for close-in transiting exoplanets provide a crucial check on models of planetary evolution. One common approach is to model the planeta…

astro-ph.SR2021★ 3 cited

Radial velocity precision of ESPRESSO through the analysis of the solar twin HIP 11915

Yuri Netto, Diego Lorenzo-Oliveira, Jorge Meléndez +4

Different stellar phenomena affect radial velocities (RVs), causing variations large enough to make it difficult to identify planet signals from the stellar variability. RV variati…

astro-ph.IM2021★ 51 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.EP2021★ 9 cited

HST PanCET program: Non-detection of atmospheric escape in the warm Saturn-sized planet WASP-29 b

L. A. dos Santos, V. Bourrier, D. Ehrenreich +10

(Abridged) Short-period gas giant exoplanets are susceptible to intense atmospheric escape due to their large scale heights and strong high-energy irradiation. This process is thou…

astro-ph.EP2021★ 9 cited

The Hubble PanCET program: Long-term chromospheric evolution and flaring activity of the M dwarf host GJ 3470

V. Bourrier, L. A. dos Santos, J. Sanz-Forcada +9

Neptune-size exoplanets seem particularly sensitive to atmospheric evaporation, making it essential to characterize the stellar high-energy radiation that drives this mechanism. Th…

astro-ph.EP2020★ 24 cited

The Hubble PanCET Program: A Metal-rich Atmosphere for the Inflated Hot Jupiter HAT-P-41b

Kyle B. Sheppard, Luis Welbanks, Avi Mandell +14

We present a comprehensive analysis of the 0.3--5\,m transit spectrum for the inflated hot Jupiter HAT-P-41b. The planet was observed in transit with Hubble STIS and WFC3 as par…

astro-ph.EP2020★ 32 cited

Search for helium in the upper atmosphere of the hot Jupiter WASP-127 b using Gemini/Phoenix

Leonardo A. dos Santos, David Ehrenreich, Vincent Bourrier +8

Large-scale exoplanet search surveys have shown evidence that atmospheric escape is a ubiquitous process that shapes the evolution and demographics of planets. However, we lack a d…

astro-ph.EP2020★ 43 cited

The high-energy environment and atmospheric escape of the mini-Neptune K2-18 b

Leonardo A. dos Santos, David Ehrenreich, Vincent Bourrier +6

K2-18 b is a transiting mini-Neptune that orbits a nearby (38 pc) cool M3 dwarf and is located inside its region of temperate irradiation. We report on the search for hydrogen esca…

astro-ph.SR2019★ 65 cited

The Li-age correlation: the Sun is unusually Li deficient for its age

M. Carlos, J. Melendez, L. Spina +8

The present work aims to examine in detail the depletion of lithium in solar twins to better constrain stellar evolution models and investigate its possible connection with exoplan…

astro-ph.EP2018★ 12 cited

Observability of hydrogen-rich exospheres in Earth-like exoplanets

Leonardo A. dos Santos, Vincent Bourrier, David Ehrenreich +1

(Abridged) The existence of an extended neutral hydrogen exosphere around small planets can be used as an evidence for the presence of water in their lower atmosphere but, to date,…