activity
20122026
most citedThe Li-age correlation: the Sun is unusually Li deficient for its age

65 citations · 333 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.EP2026

HD 715 b, a Warm Jupiter Orbiting a Massive Subgiant Discovered from a Single TESS Transit

Alexander Venner, Robert A. Wittenmyer, Andrew Vanderburg +23

Transiting Warm Jupiters orbiting bright stars are scarcely known, but a substantial number of these planets have been uncovered by the TESS mission. In this work we report the dis…

astro-ph.EP2026

TOI-6692b: An eccentric 130 day period giant planet with a single transit from TESS

Allyson Bieryla, Karen A. Collins, George Zhou +46

We report the discovery and characterization of TOI-6692 b, an eccentric (e~0.54) Jupiter on a 130-day orbit. TOI-6692 b was first detected as a community TESS Object of Interest (…

astro-ph.EP2025

Giant Planets and Eccentric Orbits Are Common Around Galactic Thick Disc Stars

Thiago Ferreira, Jhon Yana Galarza, Henrique Reggiani +15

Planet formation in the Galactic thick disc is expected to be inefficient---low solid reservoirs, short disc lifetimes, and harsh irradiation environments should conspire to inhibi…

astro-ph.SR2025

Extreme Lithium Depletion in Solar Twins: Challenging Non-Standard Mixing Models

Isabelle Winnick, Jhon Yana Galarza, Henrique Reggiani +12

Lithium (Li) is a powerful tracer of stellar mixing, gradually depleted in solar twins by non-standard transport below the convective zone. Here, we identify six new solar twins wi…

astro-ph.SR2024

HIP 8522: A Puzzling Young Solar Twin with the Lowest Detected Lithium

Jhon Yana Galarza, Diego Lorenzo-Oliveira, Thiago Ferreira +8

We present HIP 8522, a young solar twin with the lowest detected lithium, potentially a field blue straggler or the result of episodic early accretion. Its stellar parameters ($T_{…

astro-ph.GA2024

Chemical Diversity on Small Scales -- Abundance Analysis of the Tucana V Ultra-Faint Dwarf Galaxy

Terese T. Hansen, Joshua D. Simon, Ting S. Li +5

The growing number of Milky Way satellites detected in recent years has introduced a new focus for stellar abundance analysis. Abundances of stars in satellites have been used to p…

astro-ph.EP2024

TOI-1173 A : The First Inflated Super-Neptune in a Wide Binary System

Jhon Yana Galarza, Thiago Ferreira, Diego Lorenzo-Oliveira +8

Among Neptunian mass exoplanets ( M), puffy hot Neptunes are extremely rare, and their unique combination of low mass and extended radii implies very low density ($…

astro-ph.SR2023

Insight into the Formation of Pic b through the Composition of Its Parent Protoplanetary Disk as Revealed by the Pic Moving Group Member HD 181327

Henrique Reggiani, Jhon Yana Galarza, Kevin C. Schlaufman +5

It has been suggested that Pic b has a supersolar metallicity and subsolar C/O ratio. Assuming solar carbon and oxygen abundances for the star Pic and therefore the planet'…

astro-ph.SR2022★ 11 cited

The Chemical Composition of Extreme-Velocity Stars

Henrique Reggiani, Alexander P. Ji, Kevin C. Schlaufman +5

Little is known about the origin of the fastest stars in the Galaxy. Our understanding of the Milky Way and surrounding dwarf galaxies chemical evolution history allows us to use t…

astro-ph.SR2021

Rocky planet engulfment in the binary system HIP 71726-37

J. Yana Galarza, R. López-Valdivia, J. Meléndez +1

Binary stars are supposed to be chemically homogeneous, as they are born from the same molecular cloud. However, high precision chemical abundances show that some binary systems di…

astro-ph.SR2020★ 15 cited

Rotation of solar analogs cross-matching Kepler and Gaia DR2

Jose-Dias do Nascimento, Leandro de Almeida, Eduardo Nunes Velloso +10

A major obstacle to interpreting the rotation period distribution for main-sequence stars from Kepler mission data has been the lack of precise evolutionary status for these object…

astro-ph.HE2020★ 44 cited

Constraints on the Physical Properties of GW190814 through Simulations based on DECam Follow-up Observations by the Dark Energy Survey

R. Morgan, M. Soares-Santos, J. Annis +99

On 14 August 2019, the LIGO and Virgo Collaborations detected gravitational waves from a black hole and a 2.6 solar mass compact object, possibly the first neutron star -- black ho…

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.SR2018★ 31 cited

Thorium in solar twins: implications for habitability in rocky planets

Rafael B. Botelho, Andre de C. Milone, Jorge Melendez +10

We have investigated the thorium (Th) abundance in a sample of 53 thin disc solar twins covering a wide range of ages. These data provide constrains on the mantle energy budget of…

astro-ph.EP2016★ 53 cited

The Solar Twin Planet Search. V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468

Jorge Melendez, Megan Bedell, Jacob L. Bean +14

[Methods]. We obtained high-precision radial velocities with HARPS on the ESO 3.6 m telescope and determined precise stellar elemental abundances (~0.01 dex) using MIKE spectra on…

astro-ph.SR2016★ 38 cited

High precision analysis of the solar twin HIP 100963

Jhon Yana Galarza, Jorge Meléndez, Ivan Ramírez +3

Methods. We used the HIRES spectrograph on the Keck I telescope to acquire high-resolution (R 70000) spectra with a high signal-to-noise ratio (S/N 400 - 650 pe…

astro-ph.SR2016★ 28 cited

Serendipitous discovery of the faint solar twin Inti 1

Jhon Yana Galarza, Jorge Meléndez, Judith G. Cohen

Methods. We determine the atmospheric parameters and differential abundances using high-resolution (), high signal-to-noise (S/N 110 - 240 per pixel) Ke…

astro-ph.CO2012★ 48 cited

Number Counts and Non-Gaussianity

Sarah Shandera, Adrienne L. Erickcek, Pat Scott +1

We describe a general procedure for using number counts of any object to constrain the probability distribution of the primordial fluctuations, allowing for generic weak non-Gaussi…