activity
19992023
most citedThe GALAH Survey: Scientific Motivation

839 citations · 3.1k across the 59 of their papers we have counts for

collaborators

59 papers

astro-ph.GA2023

SimSpin v2.6.0 -- Constructing synthetic spectral IFU cubes for comparison with observational surveys

K. E. Harborne, A. Serene, E. J. A. Davies +10

In this work, we present a methodology and a corresponding code-base for constructing mock integral field spectrograph (IFS) observations of simulated galaxies in a consistent and…

astro-ph.IM2022★ 4 cited

FAIR standards for astronomical data

Simon O'Toole, James Tocknell

We present an overview of the "FAIR Guiding Principles for scientific data management and stewardship", first published in 2016, and how they relate to astronomical data management…

astro-ph.EP2021★ 11 cited

The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at 2 AU

Yunlin Zeng, Timothy D. Brandt, Gongjie Li +12

Gliese 86 is a nearby K dwarf hosting a giant planet on a 16-day orbit and an outer white dwarf companion on a century-long orbit. In this study we combine radial…

astro-ph.SR2021★ 2 cited

The Detectability of Binary Star Planetary and Brown Dwarf Companions From Eclipse Timing Variations

A. K. Getley, B. Carter, R. King +1

In this paper, we determine the detectability of eclipsing binary star companions from eclipse timing variations using the Kepler mission dataset. Extensive and precise stellar tim…

astro-ph.SR2020★ 6 cited

Stability of planetary, single M dwarf, and binary star companions to Kepler detached eclipsing binaries and a possible five body system

A. K. Getley, B. Carter, R. King +1

In this study we identify 11 Kepler systems (KIC 5255552, 5653126, 5731312, 7670617, 7821010, 8023317, 10268809, 10296163, 11519226, 11558882 and 12356914) with a "flip-flop" effec…

astro-ph.EP2020★ 33 cited

Transits of Known Planets Orbiting a Naked-Eye Star

Stephen R. Kane, Selçuk Yalçınkaya, Hugh P. Osborn +45

Some of the most scientifically valuable transiting planets are those that were already known from radial velocity (RV) surveys. This is primarily because their orbits are well cha…