activity
20202025
most citedThe EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities

61 citations · 121 across the 13 of their papers we have counts for

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11 papers · 1 filter

astro-ph.EP2025★ 4 cited

A New Brown Dwarf Orbiting an M star and An Investigation on the Eccentricity Distribution of Transiting Long-Period Brown Dwarfs

Tianjun Gan, Charles Cadieux, Shigeru Ida +32

The orbital eccentricities of brown dwarfs encode valuable information of their formation and evolution history, providing insights into whether they resemble giant planets or stel…

astro-ph.EP2024

A long spin period for a sub-Neptune-mass exoplanet

Ellen M. Price, Juliette Becker, Zoë L. de Beurs +2

HIP 41378 f is a sub-Neptune exoplanet with an anomalously low density. Its long orbital period and deep transit make it an ideal candidate for detecting oblateness photometrically…

astro-ph.EP2024★ 16 cited

Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3

Michaël Gillon, Peter P. Pedersen, Benjamin V. Rackham +81

Located at the bottom of the main sequence, ultracool dwarf stars are widespread in the solar neighbourhood. Nevertheless, their extremely low luminosity has left their planetary p…

astro-ph.EP2024★ 4 cited

The coevolution of migrating planets and their pulsating stars through episodic resonance locking

Jared Bryan, Julien de Wit, Meng Sun +2

Hot Jupiters are expected to form far from their host star and move toward close-in, circular orbits via a smooth, monotonic decay due to mild and constant tidal dissipation. Yet,…

astro-ph.EP2024

Characterization of K2-167 b and CALM, a new stellar activity mitigation method

Zoë L. de Beurs, Andrew Vanderburg, Erica Thygesen +13

We report precise radial velocity (RV) observations of HD 212657 (= K2-167), a star shown by K2 to host a transiting sub-Neptune-sized planet in a 10 day orbit. Using Transiting Ex…

astro-ph.EP2024

TESS Hunt for Young and Maturing Exoplanets (THYME) XI: An Earth-sized Planet Orbiting a Nearby, Solar-like Host in the 400Myr Ursa Major Moving Group

Benjamin K. Capistrant, Melinda Soares-Furtado, Andrew Vanderburg +32

Young terrestrial worlds are critical test beds to constrain prevailing theories of planetary formation and evolution. We present the discovery of HD 63433d - a nearby (22pc), Eart…

astro-ph.EP2023

DEATHSTAR: A system for confirming planets and identifying false positive signals in TESS data using ground-based time domain surveys

Gabrielle Ross, Andrew Vanderburg, Zoë L. de Beurs +3

We present a technique for verifying or refuting exoplanet candidates from the Transiting Exoplanet Survey Satellite (TESS) mission by searching for nearby eclipsing binary stars u…

astro-ph.EP2023★ 12 cited

Revisiting Orbital Evolution in HAT-P-2 b and Confirmation of HAT-P-2 c

Zoë L. de Beurs, Julien de Wit, Alexander Venner +5

One possible formation mechanism for Hot Jupiters is that high-eccentricity gas giants experience tidal interactions with their host star that cause them to lose orbital energy and…

astro-ph.EP2023★ 6 cited

TTV Constraints on Additional Planets in the WD 1856+534 system

Sarah Kubiak, Andrew Vanderburg, Juliette Becker +4

WD 1856+534 b (or WD 1856 b for short) is the first known transiting planet candidate around a white dwarf star. WD 1856 b is about the size of Jupiter, has a mass less than about…

astro-ph.EP2022★ 61 cited

The EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities

Lily L. Zhao, Debra A. Fischer, Eric B. Ford +40

Measured spectral shifts due to intrinsic stellar variability (e.g., pulsations, granulation) and activity (e.g., spots, plages) are the largest source of error for extreme precisi…

astro-ph.EP2020★ 8 cited

Identifying Exoplanets with Deep Learning. IV. Removing Stellar Activity Signals from Radial Velocity Measurements Using Neural Networks

Zoe L. de Beurs, Andrew Vanderburg, Christopher J. Shallue +24

Exoplanet detection with precise radial velocity (RV) observations is currently limited by spurious RV signals introduced by stellar activity. We show that machine learning techniq…