activity
20122025
most citedemcee: The MCMC Hammer

12.4k citations · 25.7k across the 104 of their papers we have counts for

collaborators

110 papers

astro-ph.GA2025

Gaussian Process Methods for Very Large Astrometric Data Sets

Timothy Hapitas, Lawrence M. Widrow, Thavisha E. Dharmawardena +1

We present a novel non-parametric method for inferring smooth models of the mean velocity field and velocity dispersion tensor of the Milky Way from astrometric data. Our approach…

astro-ph.EP2025

SiO and a super-stellar C/O ratio in the atmosphere of the giant exoplanet WASP-121b

Thomas M. Evans-Soma, David K. Sing, Joanna K. Barstow +15

Refractory elements such as iron, magnesium, and silicon can be detected in the atmospheres of ultrahot giant planets. This provides an opportunity to quantify the amount of refrac…

astro-ph.SR2025★ 6 cited

Measuring Long Stellar Rotation Periods (>10 days) from TESS FFI Light Curves is Possible: An Investigation Using TESS and ZTF

Soichiro Hattori, Ruth Angus, Daniel Foreman-Mackey +3

The rotation period of a star is an important quantity that provides insight into its structure and state. For stars with surface features like starspots, their periods can be infe…

astro-ph.EP2025★ 4 cited

Exoplanet Occurrence Rate with Age for FGK Stars in Kepler

Maryum Sayeed, Ruth Angus, Travis Berger +5

We measure exoplanet occurrence rate as a function of isochrone and gyrochronology ages using confirmed and candidate planets identified in Q1-17 DR25 Kepler data. We employ Kepler…

astro-ph.GA2024

All-sky three-dimensional dust density and extinction Maps of the Milky Way out to 2.8 kpc

T. E. Dharmawardena, C. A. L. Bailer-Jones, M. Fouesneau +5

Three-dimensional dust density maps are crucial for understanding the structure of the interstellar medium of the Milky Way and the processes that shape it. However, constructing t…

astro-ph.SR2024★ 2 cited

Precise Time-Domain Asteroseismology and a Revised Target List for TESS Solar-Like Oscillators

Daniel Hey, Daniel Huber, Joel Ong +2

The TESS mission has provided a wealth of asteroseismic data for solar-like oscillators. However, these data are subject to varying cadences, large gaps, and unequal sampling, whic…