activity
20192026
most citedA Guide to Realistic Uncertainties on Fundamental Properties of Solar-Type Exoplanet Host Stars

207 citations · 639 across the 31 of their papers we have counts for

collaborators

32 papers

astro-ph.SR2026

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet

Diego Godoy-Rivera, Savita Mathur, Tyler Richey-Yowell +5

For low-mass stars (M < 1.4 Msun), the connection between stellar rotation and magnetic activity governs stellar spin-down, shapes the environments of their exoplanets, and provide…

astro-ph.SR2026

Quantifying isochrone-based age uncertainties for rapidly rotating A-type stars

Simon J. Murphy, Anuj Gautam, Zachary R. Claytor

Accurate stellar ages and masses are essential for interpreting the demographics and physical properties of exoplanets, particularly for intermediate-mass, early-type stars where c…

cs.CV2026

ArtHOI: Taming Foundation Models for Monocular 4D Reconstruction of Hand-Articulated-Object Interactions

Zikai Wang, Zhilu Zhang, Yiqing Wang +2

Existing hand-object interactions (HOI) methods are largely limited to rigid objects, while 4D reconstruction methods of articulated objects generally require pre-scanning the obje…

astro-ph.IM2025

The Impact of the MAST Data Archive

Richard A. Shaw, Jenny L. Novacescu, Sarah Weissman +31

The Barbara A. Mikulski Archive for Space Telescopes (MAST) hosts science-ready data products from over twenty NASA missions, plus community-contributed data collections, and other…

astro-ph.SR2025★ 1 cited

200,000+ Deep Learning-inferred Periods of Stellar Variability from the All-Sky Automated Survey for Supernovae

Meir E. Schochet, Penelope Planet, Zachary R. Claytor +2

Stars exhibit a range of variability periods that depend on their mass, age, and evolutionary stage. For space-based photometric data, convolutional neural networks (CNNs) have dem…

astro-ph.SR2025

New Rotation Periods from the Kepler Bonus Background Light Curves

Zachary R. Claytor, Jamie Tayar

The Kepler field hosts the best studied sample of field star rotation periods. However, due to Kepler's large 4" pixels, many of its light curves are at high risk of contamination…

astro-ph.SR2025

Model Choice Matters for Age Inference on the Red Giant Branch

Leslie M. Morales, Jamie Tayar, Zachary R. Claytor

Galactic archaeology relies on accurate stellar parameters to reconstruct the galaxy's history, including information on stellar ages. While the precision of data has improved sign…

astro-ph.GA2025

Trials and Tribulations of Chemodynamical Tagging: Investigating the Recovery of Open Clusters in the Gaia DR3-GALAH DR4 Catalog

Nicholas A. Barth, David Mendez, Rana Ezzeddine +5

Chemodynamical tagging has been suggested as a powerful tool to trace stars back to their birth clusters. However, the efficacy of chemodynamical tagging as a means to recover indi…

astro-ph.SR2025★ 1 cited

Magnetic activity evolution of solar-like stars: II. -Ro evolution of Kepler main-sequence targets

Savita Mathur, Angela R. G. Santos, Zachary R. Claytor +16

There is now a large sample of stars observed by the Kepler satellite with measured rotation periods and photometric activity index . We use this data, in conjunction w…

astro-ph.SR2024

Evidence of Truly Young high- Dwarf Stars

Yuxi Lu, Isabel L. Colman, Maryum Sayeed +14

The existence of high- stars with inferred ages < 6 Gyr has been confirmed recently with large spectroscopic and photometric surveys. However, stellar mergers or binary interact…

astro-ph.SR2024★ 8 cited

TESS asteroseismology of Hydri: a subgiant with a born-again dynamo

Travis S. Metcalfe, Jennifer L. van Saders, Daniel Huber +12

The solar-type subgiant Hyi has long been studied as an old analog of the Sun. Although the rotation period has never been measured directly, it was estimated to be near 27 day…

astro-ph.EP2024

A Testbed for Tidal Migration: the 3D Architecture of an Eccentric Hot Jupiter HD 118203 b Accompanied by a Possibly Aligned Outer Giant Planet

Jingwen Zhang, Daniel Huber, Lauren M. Weiss +31

Characterizing outer companions to hot Jupiters plays a crucial role in deciphering their origins. We present the discovery of a long-period giant planet, HD 118203 c ($m_{c}=11.79…

astro-ph.SR2023

TESS Stellar Rotation up to 80 days in the Southern Continuous Viewing Zone

Zachary R. Claytor, Jennifer L. van Saders, Lyra Cao +3

The TESS mission delivers time-series photometry for millions of stars across the sky, offering a probe into stellar astrophysics, including rotation, on a population scale. Howeve…

astro-ph.SR2023★ 23 cited

A close-in giant planet escapes engulfment by its star

Marc Hon, Daniel Huber, Nicholas Z. Rui +39

When main-sequence stars expand into red giants, they are expected to engulf close-in planets. Until now, the absence of planets with short orbital periods around post-expansion, c…

astro-ph.SR2023★ 26 cited

Magnetic activity evolution of solar-like stars: I. S_ph-Age relation derived from Kepler observations

Savita Mathur, Zachary R. Claytor, Angela R. G. Santos +9

The ages of solar-like stars have been at the center of many studies such as exoplanet characterization or Galactic-archaeology. While ages are usually computed from stellar evolut…

astro-ph.IM2023★ 1 cited

Roman CCS White Paper: Adding Fields Hosting Globular Clusters To The Galactic Bulge Time Domain Survey

Samuel K. Grunblatt, Robert F. Wilson, Andrew Winter +9

Despite multiple previous searches, no transiting planets have yet been identified within a globular cluster. This is believed to be due to a combination of factors: the low metall…

astro-ph.SR2023★ 21 cited

Temporal variation of the photometric magnetic activity for the Sun and Kepler solar-like stars

A. R. G. Santos, S. Mathur, R. A. García +9

The photometric time series of solar-like stars can exhibit rotational modulation due to active regions co-rotating with the stellar surface, allowing us to constrain stellar rotat…

astro-ph.EP2023

Nuggets of Wisdom: Determining an Upper Limit on the Number Density of Chickens in the Universe

Rachel Losacco, Zachary Claytor

The lower limit on the chicken density function (CDF) of the observable Universe was recently determined to be approximately 10 chickens pc. For over a year, however…

astro-ph.EP2023★ 34 cited

The TIME Table: Rotation and Ages of Cool Exoplanet Host Stars

Eric Gaidos, Zachary Claytor, Ryan Dungee +2

Age is a stellar parameter that is both fundamental and difficult to determine. Among middle-aged M dwarfs, the most prolific hosts of close-in and detectable exoplanets, gyrochron…

astro-ph.EP2022★ 5 cited

Kepler-102: Masses and Compositions for a Super-Earth and Sub-Neptune Orbiting an Active Star

Casey Brinkman, James Cadman, Lauren Weiss +24

Radial velocity (RV) measurements of transiting multiplanet systems allow us to understand the densities and compositions of planets unlike those in the Solar System. Kepler-102, w…

astro-ph.SR2022★ 12 cited

Is [Y/Mg] a Reliable Age Diagnostic for FGK Stars?

Travis A. Berger, Jennifer L. van Saders, Daniel Huber +3

Current spectroscopic surveys are producing large catalogs of chemical abundances for stars of all types. The yttrium to magnesium ratio, [Y/Mg], has emerged as a candidate age ind…

astro-ph.EP2022

The TESS-Keck Survey. XI. Mass Measurements for Four Transiting sub-Neptunes orbiting K dwarf TOI-1246

Emma V. Turtelboom, Lauren M. Weiss, Courtney D. Dressing +78

Multi-planet systems are valuable arenas for investigating exoplanet architectures and comparing planetary siblings. TOI-1246 is one such system, with a moderately bright K dwarf (…

astro-ph.CO2022★ 2 cited

Worry No More, The Hubble Tension is Relieved: A Truly Direct Measurement of the Hubble Constant from Mooniversal Expansion

Gagandeep S. Anand, Zachary R. Claytor, Ryan Dungee

Using sedimentary and eclipse-based measurements of the lunar recession velocity, we derive a new local-Universe measurement of the Hubble constant () from the recession rate…

astro-ph.SR2022★ 37 cited

Rotation Distributions around the Kraft Break with TESS and Kepler: The Influences of Age, Metallicity, and Binarity

Ellis A. Avallone, Jamie N. Tayar, Jennifer L. van Saders +6

Stellar rotation is a complex function of mass, metallicity, and age and can be altered by binarity. To understand the importance of these parameters in main sequence stars, we hav…