activity
20132026
most citedThe Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment

681 citations · 6.5k across the 116 of their papers we have counts for

collaborators
Showing 2021Show all

8 papers · 1 filter

astro-ph.EP2021★ 19 cited

The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets

Robert F. Wilson, Caleb I. Cañas, Steven R. Majewski +15

The chemical abundances of planet-hosting stars offer a glimpse into the composition of planet-forming environments. To further understand this connection, we make the first ever m…

astro-ph.SR2021

Stellar multiplicity and stellar rotation: Insights from APOGEE

Christine Mazzola Daher, Carles Badenes, Jamie Tayar +18

We measure rotational broadening in spectra taken by the Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey to characterise the relationship between stellar mul…

astro-ph.GA2021★ 99 cited

Final Targeting Strategy for the SDSS-IV APOGEE-2N Survey

Rachael L. Beaton, Ryan J. Oelkers, Christian R. Hayes +57

APOGEE-2 is a dual-hemisphere, near-infrared (NIR), spectroscopic survey with the goal of producing a chemo-dynamical mapping of the Milky Way Galaxy. The targeting for APOGEE-2 is…

astro-ph.SR2021

A 'Quick Look' at All-Sky Galactic Archeology with TESS: 158,000 Oscillating Red Giants from the MIT Quick-Look Pipeline

Marc Hon, Daniel Huber, James S. Kuszlewicz +6

We present the first near all-sky yield of oscillating red giants from the prime mission data of NASA's Transiting Exoplanet Survey Satellite (TESS). We apply machine learning towa…

astro-ph.SR2021★ 33 cited

Age-Dating Red Giant Stars Associated with Galactic Disk and Halo Substructures

Samuel K. Grunblatt, Joel C. Zinn, Adrian M. Price-Whelan +12

The vast majority of Milky Way stellar halo stars were likely accreted from a small number (3) of relatively large dwarf galaxy accretion events. However, the timing of t…

astro-ph.SR2021★ 94 cited

Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs

Oliver J. Hall, Guy R. Davies, Jennifer van Saders +9

Studies using asteroseismic ages and rotation rates from star-spot rotation have indicated that standard age-rotation relations may break down roughly half-way through the main seq…

astro-ph.SR2021★ 20 cited

Testing the Limits of Precise Subgiant Characterization with APOGEE and Gaia: Opening a Window to Unprecedented Astrophysical Studies

Diego Godoy-Rivera, Jamie Tayar, Marc H. Pinsonneault +6

Given their location on the Hertzsprung-Russell (HR) diagram, thoroughly characterized subgiant stars can place stringent constraints on a wide range of astrophysical problems. Acc…

astro-ph.SR2021★ 13 cited

Projected Rotational Velocities and Fundamental Properties of Low-Mass Pre-Main Sequence Stars in the Taurus-Auriga Star Forming Region

Larissa A. Nofi, Christopher M. Johns-Krull, Ricardo López-Valdivia +11

The projected stellar rotational velocity () is critical for our understanding of processes related to the evolution of angular momentum in pre-main sequence stars. We pr…