papers

Publications (13)

astro-ph.SR2021

Chronostar. II. Kinematic age and substructure of the Scorpius-Centaurus OB2 association

Maruša Žerjal, Michael J. Ireland, Timothy D. Crundall +2

The nearest region of massive star formation - the Scorpius-Centaurus OB2 association (Sco-Cen) - is a local laboratory ideally suited to the study of a wide range of astrophysical…

astro-ph.EP2025

TSD: An inverse problem approach for recovering the exoplanetary atmosphere transmission spectrum from high-resolution spectroscopy

Nikolai Piskunov, Adam D. Rains, Linn Boldt-Christmas

Our ability to observe, detect, and characterize exoplanetary atmospheres has grown by leaps and bounds over the last 20 years, aided largely by developments in astronomical instru…

astro-ph.SR2020

Very regular high-frequency pulsation modes in young intermediate-mass stars

Timothy R. Bedding, Simon J. Murphy, Daniel R. Hey +33

Asteroseismology is a powerful tool for probing the internal structures of stars by using their natural pulsation frequencies. It relies on identifying sequences of pulsation modes…

astro-ph.SR2020

Precision angular diameters for 16 southern stars with VLTI/PIONIER

Adam D. Rains, Michael J. Ireland, Timothy R. White +2

In the current era of Gaia and large, high signal to noise stellar spectroscopic surveys, there is an unmet need for a reliable library of fundamentally calibrated stellar effectiv…

astro-ph.SR2024

Cool and Data-Driven: An Exploration of Optical Cool Dwarf Chemistry with Both Data-Driven and Physical Models

Adam D. Rains, Thomas Nordlander, Stephanie Monty +6

Detailed chemical studies of F/G/K -- or Solar-type -- stars have long been routine in stellar astrophysics, enabling studies in both Galactic chemodynamics, and exoplanet demograp…

astro-ph.EP2026

VLT/CRIRES+ observations of warm Neptune WASP-107 b: Challenges in detecting molecules with ground-based transmission spectroscopy of cooler and cloudy exoplanets

Linn Boldt-Christmas, Adam D. Rains, Nikolai Piskunov +15

Atmospheres of transiting exoplanets can be studied spectroscopically using space-based or ground-based observations. Each has its own strengths and weaknesses, so there are benefi…