activity
20052026
most citedBaryon Acoustic Oscillations in the Ly-α forest of BOSS quasars

630 citations · 3.7k across the 46 of their papers we have counts for

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Showing 2023Show all

8 papers · 1 filter

astro-ph.GA2023

Stream Members Only: Data-Driven Characterization of Stellar Streams with Mixture Density Networks

Nathaniel Starkman, Jacob Nibauer, Jo Bovy +4

Stellar streams are sensitive probes of the Milky Way's gravitational potential. The mean track of a stream constrains global properties of the potential, while its fine-grained su…

astro-ph.IM202344 cited

Towards an astronomical foundation model for stars with a Transformer-based model

Henry W. Leung, Jo Bovy

Rapid strides are currently being made in the field of artificial intelligence using Transformer-based models like Large Language Models (LLMs). The potential of these methods for…

astro-ph.GA2023

Decoding the age-chemical structure of the Milky Way disk: An application of Copulas and Elicitable Maps

Aarya A. Patil, Jo Bovy, Sebastian Jaimungal +2

In the Milky Way, the distribution of stars in the vs. and vs. age planes holds essential information about the history of sta…

astro-ph.GA20231 cited

The stellar mass of the Gaia-Sausage/Enceladus accretion remnant

James Lane, Jo Bovy, Ted Mackereth

The \textit{Gaia}-Sausage/Enceladus (GS/E) structure is an accretion remnant which comprises a large fraction of the Milky Way's stellar halo. We study GS/E using high-purity sampl…

astro-ph.GA2023

Disentangling Stellar Age Estimates from Galactic Chemodynamical Evolution

Jeff Shen, Joshua S. Speagle, J. Ted Mackereth +2

Stellar ages are key for determining the formation history of the Milky Way, but are difficult to measure precisely. Furthermore, methods that use chemical abundances to infer ages…

astro-ph.GA202317 cited

Constraints on the Galactic Centre environment from \textit{Gaia} hypervelocity stars III: Insights on a possible companion to Sgr A*

Fraser A. Evans, Alexander Rasskazov, Amber Remmelzwaal +4

We consider a scenario in which Sgr A* is in a massive black hole binary (MBHB) with an as-of-yet undetected supermassive or intermediate-mass black hole companion. Dynamical encou…