activity
20112021
most citedThe APOKASC Catalog: An Asteroseismic and Spectroscopic Joint Survey of Targets in the Kepler Fields

344 citations · 1.8k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2021★ 48 cited

The K2 Galactic Archaeology Program Data Release 3: Age-abundance patterns in C1-C8 and C10-C18

Joel C. Zinn, Dennis Stello, Yvonne Elsworth +28

We present the third and final data release of the K2 Galactic Archaeology Program (K2 GAP) for Campaigns C1-C8 and C10-C18. We provide asteroseismic radius and mass coefficients,…

astro-ph.SR2020★ 5 cited

Weighing stars from birth to death: mass determination methods across the HRD

Aldo Serenelli, Achim Weiss, Conny Aerts +31

The mass of a star is the most fundamental parameter for its structure, evolution, and final fate. It is particularly important for any kind of stellar archaeology and characteriza…

astro-ph.GA2020★ 84 cited

Age dating of an early Milky Way merger via asteroseismology of the naked-eye star Indi

William J. Chaplin, Aldo M. Serenelli, Andrea Miglio +81

Over the course of its history, the Milky Way has ingested multiple smaller satellite galaxies. While these accreted stellar populations can be forensically identified as kinematic…

astro-ph.SR2019★ 36 cited

Coupling 1D stellar evolution with 3D-hydrodynamical simulations on-the-fly II: Stellar Evolution and Asteroseismic Applications

Jakob Rørsted Mosumgaard, Andreas Christ Sølvsten Jørgensen, Achim Weiss +2

Models of stellar structure and evolution are an indispensable tool in astrophysics, yet they are known to incorrectly reproduce the outer convective layers of stars. In the first…

astro-ph.EP2019★ 118 cited

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

Aldo S. Bonomo, Li Zeng, Mario Damasso +49

Measures of exoplanet bulk densities indicate that small exoplanets with radius less than 3 Earth radii () range from low-density sub-Neptunes containing volatile element…

astro-ph.EP2017★ 13 cited

Time-Series Analysis of Broadband Photometry of Neptune from K2

Jason F. Rowe, Patrick Gaulme, Jack J. Lissauer +19

We report here on our search for excess power in photometry of Neptune collected by the K2 mission that may be due to intrinsic global oscillations of the planet Neptune. To conduc…

astro-ph.SR2014★ 344 cited

The APOKASC Catalog: An Asteroseismic and Spectroscopic Joint Survey of Targets in the Kepler Fields

Marc H. Pinsonneault, Yvonne Elsworth, Courtney Epstein +42

We present the first APOKASC catalog of spectroscopic and asteroseismic properties of 1916 red giants observed in the Kepler fields. The spectroscopic parameters provided from the…

astro-ph.GA2014★ 235 cited

The APOGEE red-clump catalog: Precise distances, velocities, and high-resolution elemental abundances over a large area of the Milky Way's disk

Jo Bovy, David L. Nidever, Hans-Walter Rix +48

The Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution near-infrared spectroscopic survey covering all of the major…

astro-ph.SR2014★ 111 cited

Testing the Asteroseismic Mass Scale Using Metal-Poor Stars Characterized with APOGEE and Kepler

Courtney R. Epstein, Yvonne P. Elsworth, Jennifer A. Johnson +29

Fundamental stellar properties, such as mass, radius, and age, can be inferred using asteroseismology. Cool stars with convective envelopes have turbulent motions that can stochast…

astro-ph.EP2013★ 62 cited

Accurate parameters of the oldest known rocky-exoplanet hosting system: Kepler-10 revisited

Alexandra Fogtmann-Schulz, Brian Hinrup, Vincent Van Eylen +4

Since the discovery of Kepler-10, the system has received considerable interest because it contains a small, rocky planet which orbits the star in less than a day. The system's par…

astro-ph.EP2013★ 318 cited

Stellar Spin-Orbit Misalignment in a Multiplanet System

Daniel Huber, Joshua A. Carter, Mauro Barbieri +32

Stars hosting hot Jupiters are often observed to have high obliquities, whereas stars with multiple co-planar planets have been seen to have low obliquities. This has been interpre…

astro-ph.SR2013★ 334 cited

Fundamental Properties of Kepler Planet-Candidate Host Stars using Asteroseismology

Daniel Huber, William J. Chaplin, Jørgen Christensen-Dalsgaard +31

We have used asteroseismology to determine fundamental properties for 66 Kepler planet-candidate host stars, with typical uncertainties of 3% and 7% in radius and mass, respectivel…

astro-ph.SR2011★ 65 cited

Asteroseismic diagrams from a survey of solar-like oscillations with Kepler

Timothy R. White, Timothy R. Bedding, Dennis Stello +30

Photometric observations made by the NASA Kepler Mission have led to a dramatic increase in the number of main-sequence and subgiant stars with detected solar-like oscillations. We…