activity
20052025
most citedBaryon Acoustic Oscillations in the Ly-α forest of BOSS quasars

630 citations · 3.6k across the 34 of their papers we have counts for

collaborators
Showing 2018Show all

14 papers · 1 filter

astro-ph.IM2018

The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library

D. S. Aguado, Romina Ahumada, Andres Almeida +230

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years o…

astro-ph.GA2018

Searching for the GD-1 Stream Progenitor in Gaia DR2 with Direct N-body Simulations

Jeremy J. Webb, Jo Bovy

We perform a large suite of direct N-body simulations aimed at revealing the location of the progenitor, or its remnant, of the GD-1 stream. Data from \gaia\ DR2 reveals the GD-1 s…

astro-ph.GA2018

Effects of baryonic and dark matter substructure on the Pal 5 stream

Nilanjan Banik, Jo Bovy

Gravitational encounters between small-scale dark matter substructure and cold stellar streams in the Milky Way halo lead to density perturbations in the latter, making streams an…

astro-ph.GA2018

Vertical waves in the solar neighbourhood in Gaia DR2

Morgan Bennett, Jo Bovy

The vertical structure and dynamics of stars in our local Galactic neighbourhood contains much information about the local distribution of visible and dark matter and of perturbati…

astro-ph.GA2018

Deep learning of multi-element abundances from high-resolution spectroscopic data

Henry W. Leung, Jo Bovy

Deep learning with artificial neural networks is increasingly gaining attention, because of its potential for data-driven astronomy. However, this methodology usually does not prov…

astro-ph.GA2018

The origin of accreted stellar halo populations in the Milky Way using APOGEE, , and the EAGLE simulations

J. Ted Mackereth, Ricardo P. Schiavon, Joel Pfeffer +12

Recent work indicates that the nearby Galactic halo is dominated by the debris from a major accretion event. We confirm that result from an analysis of APOGEE-DR14 element abundanc…