papers

Publications (18)

astro-ph.EP2026

TESS Hunt for Young and Maturing Exoplanets (THYME) XIV: A Comoving-Based Age Constraint for KELT-20

Adam Distler, Melinda Soares-Furtado, Andrew W. Mann +9

Young stellar moving groups offer unique opportunities to investigate the early evolution of stellar and planetary systems. In continuation of an ongoing effort to age-date compell…

astro-ph.SR2025

SPYGLASS. VII-A. The Demographics and Ages of Small Nearby Young Associations

Ronan Kerr, Facundo Peŕez Paolino, Jonathan C. Tan +5

Recent Gaia-based young stellar association surveys have revealed dozens of low-mass populations that have, until recently, been too small or sparse to detect. These populations re…

astro-ph.EP2025

THYME XIII: Two young Neptunes orbiting a 75-Myr star in the Alpha Persei Cluster

Anne Dattilo, Andrew M. Vanderburg, Madyson G. Barber +28

Young planets with mass measurements are particularly valuable in studying atmospheric mass-loss processes, but these planets are rare and their masses difficult to measure due to…

astro-ph.SR2024

SPYGLASS. V. Spatially and Temporally Structured Star-Forming Environments in the Cepheus-Hercules Complex

Ronan Kerr, Adam L. Kraus, Daniel Krolikowski +2

Young associations record complete histories of star forming events through their demographics and dynamics, and Gaia has greatly expanded our knowledge of these associations. We p…

astro-ph.GA2019

The Green Bank Ammonia Survey: A Virial Analysis of Gould Belt Clouds in Data Release 1

Ronan Kerr, Helen Kirk, James Di Francesco +14

We perform a virial analysis of starless dense cores in three nearby star-forming regions : L1688 in Ophiuchus, NGC 1333 in Perseus, and B18 in Taurus. Our analysis takes advantage…

astro-ph.EP2022

TESS Hunt for Young and Maturing Exoplanets (THYME) VI: an 11 Myr giant planet transiting a very low-mass star in Lower Centaurus Crux

Andrew W. Mann, Mackenna L. Wood, Stephen P. Schmidt +48

Mature super-Earths and sub-Neptunes are predicted to be Jovian radius when younger than 10 Myr. Thus, we expect to find 5-15 planets around young stars even if t…

astro-ph.SR2020

Intermediate-Mass Stars Become Magnetic White Dwarfs

Ilaria Caiazzo, Jeremy Heyl, Harvey Richer +8

When a star exhausts its nuclear fuel, it either explodes as a supernova or more quiescently becomes a white dwarf, an object about half the mass of our Sun with a radius of about…

astro-ph.SR2021

Massive White Dwarfs in Young Star Clusters

Harvey B. Richer, Ilaria Caiazzo, Helen Du +6

We have carried out a search for massive white dwarfs (WDs) in the direction of young open star clusters using the Gaia DR2 database. The aim of this survey was to provide robust d…

astro-ph.GA2025

Stellar populations in STARFORGE II: Comparison with observations

Juan P. Farias, Stella S. R. Offner, Ronan Kerr +1

Recent studies suggest that most star-forming regions in our Galaxy form stellar associations rather than bound clusters. We analyse models from the STARFORGE simulation suite, a s…

astro-ph.SR2022

TESS Hunt for Young and Maturing Exoplanets (THYME) VII : Membership, rotation, and lithium in the young cluster Group-X and a new young exoplanet

Elisabeth R. Newton, Rayna Rampalli, Adam L. Kraus +36

The public, all-sky surveys Gaia and TESS provide the ability to identify new young associations and determine their ages. These associations enable study of planetary evolution by…

astro-ph.GA2022

SPYGLASS. III. The Fornax-Horologium Association and its Traceback History within the Austral Complex

Ronan Kerr, Adam L. Kraus, Simon J. Murphy +3

The study of young associations is essential for building a complete record of local star formation processes. The Fornax-Horologium association (FH), including the Fornacis…

astro-ph.GA2023

SPYGLASS. IV. New Stellar Survey of Recent Star Formation within 1 kpc

Ronan Kerr, Adam Kraus, Aaron Rizzuto

Young stellar populations provide a powerful record that traces millions of years of star formation history in the solar neighborhood. Using a revised form of the SPYGLASS young st…

astro-ph.GA2021

Stars with Photometrically Young Gaia Luminosities Around the Solar System (SPYGLASS) I: Mapping Young Stellar Structures and their Star Formation Histories

Ronan Kerr, Aaron C. Rizzuto, Adam L. Kraus +1

Young stellar associations hold a star formation record that can persist for millions of years, revealing the progression of star formation long after the dispersal of the natal cl…

astro-ph.SR2022

SPYGLASS. II. The Multi-Generational and Multi-Origin Star Formation History of Cepheus Far North

Ronan Kerr, Adam L. Kraus, Simon J. Murphy +4

Young stellar populations provide a record of past star formation, and by establishing their members' dynamics and ages, it is possible to reconstruct the full history of star form…

astro-ph.GA2026

SPYGLASS. VII-B. Tracing the Fragments of Massive Star Formation Using Low-Mass Associations

Ronan Kerr, Adam L. Kraus, Jonathan C. Tan +6

New observations from the Gaia spacecraft have traced an emerging demographic of low-mass associations disconnected from larger associations or GMCs. The first of these association…

astro-ph.GA2025

SPYGLASS. VI. Feedback-Driven Star Formation in the Circinus Complex

Ronan Kerr, Juan P. Farias, Lisa Prato +3

Young associations provide a record that traces the star formation process, and the youngest populations connect progenitor gas dynamics to the resulting stellar populations. We th…

astro-ph.EP2023

TOI-4562 b: A highly eccentric temperate Jupiter analog orbiting a young field star

Alexis Heitzmann, George Zhou, Samuel N. Quinn +47

We report the discovery of TOI-4562 b (TIC-349576261), a Jovian planet orbiting a young F7V-type star, younger than the Praesepe/Hyades clusters (< Myr). This planet stands o…

astro-ph.GA2025

The JCMT Gould Belt Survey Complete Core Catalogue: Core mass function variations between nearby molecular clouds

Kate Pattle, James Di Francesco, Jenny Hatchell +14

We present a catalogue of dense cores identified in James Clerk Maxwell Telescope (JCMT) Gould Belt Survey SCUBA-2 observations of nearby star-forming clouds. We identified 2257 de…