activity
20102021
most citedPrecise Radial Velocities of Giant Stars VII. Occurrence Rate of Giant Extrasolar Planets as a Function of Mass and Metallicity

252 citations · 659 across the 12 of their papers we have counts for

collaborators

13 papers

astro-ph.EP2021★ 11 cited

HD 76920b pinned down: a detailed analysis of the most eccentric planetary system around an evolved star

C. Bergmann, M. I. Jones, J. Zhao +9

We present 63 new multi-site radial velocity measurements of the K1III giant HD 76920, which was recently reported to host the most eccentric planet known to orbit an evolved star.…

astro-ph.EP2020★ 60 cited

Cluster Difference Imaging Photometric Survey. II. TOI 837: A Young Validated Planet in IC 2602

L. G. Bouma, J. D. Hartman, R. Brahm +42

We report the discovery of TOI 837b and its validation as a transiting planet. We characterize the system using data from the NASA TESS mission, the ESA Gaia mission, ground-based…

astro-ph.SR2020★ 114 cited

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.EP2019★ 26 cited

Truly eccentric. II. When can two circular planets mimic a single eccentric orbit?

Robert A. Wittenmyer, Christoph Bergmann, Jonathan Horner +2

When, in the course of searching for exoplanets, sparse sampling and noisy data make it necessary to disentangle possible solutions to the observations, one must consider the possi…

astro-ph.EP2019★ 95 cited

A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS

Daniel Huber, William J. Chaplin, Ashley Chontos +139

We present the discovery of TOI-197.01, the first transiting planet identified by the Transiting Exoplanet Survey Satellite (TESS) for which asteroseismology of the host star is po…

astro-ph.IM2018

Veloce Rosso: Australia's new precision radial velocity spectrograph

James Gilbert, Christoph Bergmann, Gabe Bloxham +24

Veloce is an ultra-stable fibre-fed R4 echelle spectrograph for the 3.9 m Anglo-Australian Telescope. The first channel to be commissioned, Veloce 'Rosso', utilises multiple low-co…