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Sam Walker

University of Hawai'i System

United States

Research Interests

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Articles (6)

Year:

2026

Year:

2026

Year:

2026

Year:

2026

Year:

2021

Year:

2020

Collaborators (1)

Hans Kjeldsen

Professor

Aarhus University

DENMARK

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Sam Walker

Research Interests

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Articles (6)

The Companions to B and A Stars Snapshot (C-BASS) Survey. I. Discovery of a Young Brown Dwarf Companion to HIP 17453

A Test of Substellar Evolutionary Models with High-precision Ages from Asteroseismology and Gyrochronology for the Benchmark System HR 7672AB

Keck Observations in the INfrared of Taurus and ρ Oph Exoplanets And Ultracool Dwarfs (KOINTREAU). II. Two Young Bound Companions to Ophiuchus Stars

Keck Observations in the INfrared of Taurus and ρ Oph Exoplanets And Ultracool Dwarfs (KOINTREAU) I: A Planetary-mass Companion and a Disk-obscured Stellar Companion Discovered in Taurus

An HST/STIS view of protoplanetary discs in Upper Scorpius: observations of three young M stars

Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5

Collaborators (1)

Hans Kjeldsen

Make your next move.

Sam Walker

Research Interests

Explore related searches

Articles (6)

The Companions to B and A Stars Snapshot (C-BASS) Survey. I. Discovery of a Young Brown Dwarf Companion to HIP 17453

A Test of Substellar Evolutionary Models with High-precision Ages from Asteroseismology and Gyrochronology for the Benchmark System HR 7672AB

Keck Observations in the INfrared of Taurus and ρ Oph Exoplanets And Ultracool Dwarfs (KOINTREAU). II. Two Young Bound Companions to Ophiuchus Stars

Keck Observations in the INfrared of Taurus and ρ Oph Exoplanets And Ultracool Dwarfs (KOINTREAU) I: A Planetary-mass Companion and a Disk-obscured Stellar Companion Discovered in Taurus

An HST/STIS view of protoplanetary discs in Upper Scorpius: observations of three young M stars

Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 &lt; z &lt; 5

Collaborators (1)

Hans Kjeldsen

Make your next move.

Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5