activity
20072022
most citedAbundances, Stellar Parameters, and Spectra From the SDSS-III/APOGEE Survey

413 citations · 2.1k across the 19 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2022★ 15 cited

A Spectral Classification System for Hydrogen-deficient Carbon Stars

Courtney L. Crawford, Patrick Tisserand, Geoffrey C. Clayton +6

Stellar spectral classification has been highly useful in the study of stars. While there is a currently accepted spectral classification system for carbon stars, the subset of Hyd…

astro-ph.GA2022★ 54 cited

BACCHUS Analysis of Weak Lines in APOGEE Spectra (BAWLAS)

Christian R. Hayes, Thomas Masseron, Jennifer Sobeck +11

Elements with weak and blended spectral features in stellar spectra are challenging to measure and require specialized analysis methods to precisely measure their chemical abundanc…

astro-ph.GA2020★ 50 cited

Exploring the Galactic Warp Through Asymmetries in the Kinematics of the Galactic Disk

Xinlun Cheng, Borja Anguiano, Steven R. Majewski +10

Previous analyses of large databases of Milky Way stars have revealed the stellar disk of our Galaxy to be warped and that this imparts a strong signature on the kinematics of star…

astro-ph.GA2019★ 86 cited

Spatial variations in the Milky Way disc metallicity-age relation

Diane K. Feuillet, Neige Frankel, Karin Lind +5

Stellar ages are a crucial component to studying the evolution of the Milky Way. Using Gaia DR2 distance estimates, it is now possible to estimate stellar ages for a larger volume…

astro-ph.EP2019★ 15 cited

TOI-150: A transiting hot Jupiter in the TESS southern CVZ

Caleb I. Cañas, Gudmundur Stefansson, Andrew J. Monson +23

We report the detection of a hot Jupiter (, ) orbiting a middle-aged star () in the Tra…

astro-ph.SR2018★ 36 cited

Stellar and Planetary Characterization of the Ross 128 Exoplanetary System from APOGEE Spectra

Diogo Souto, Cayman T. Unterborn, Verne V. Smith +14

The first detailed chemical abundance analysis of the M dwarf (M4.0) exoplanet-hosting star Ross 128 is presented here, based upon near-infrared (1.5--1.7 \micron) high-resolution…