activity
20032020
most citedA planet within the debris disk around the pre-main-sequence star AU Microscopii

242 citations · 1.4k across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.EP2020★ 242 cited

A planet within the debris disk around the pre-main-sequence star AU Microscopii

Peter Plavchan, Thomas Barclay, Jonathan Gagné +84

AU Microscopii (AU Mic) is the second closest pre main sequence star, at a distance of 9.79 parsecs and with an age of 22 million years. AU Mic possesses a relatively rare and spat…

astro-ph.IM2016★ 2 cited

Building an Inclusive AAS - The Critical Role of Diversity and Inclusion Training for AAS Council and Astronomy Leadership

Carolyn Brinkworth, Allison Byrd Skaer, Chanda Prescod-Weinstein +2

Diversity, equity and inclusion are the science leadership issues of our time. As our nation and the field of astronomy grow more diverse, we find ourselves in a position of enormo…

astro-ph.EP2016★ 30 cited

The Detection of Dust around NN Ser

Adam Hardy, Matthias R. Schreiber, Steven G. Parsons +6

Eclipse timing variations observed from the post common-envelope binary (PCEB) NN Ser offer strong evidence in favour of circumbinary planets existing around PCEBs. If real, these…

astro-ph.SR2016

Precise Near-Infrared Radial Velocities

Peter Plavchan, Peter Gao, Jonathan Gagne +31

We present the results of two 2.3 micron near-infrared radial velocity surveys to detect exoplanets around 36 nearby and young M dwarfs. We use the CSHELL spectrograph (R ~46,000)…

astro-ph.SR2016★ 211 cited

A High-Precision NIR Survey for RV Variable Low-Mass Stars

Jonathan Gagné, Peter Plavchan, Peter Gao +26

We present the results of a precise near-infrared (NIR) radial velocity (RV) survey of 32 low-mass stars with spectral types K2-M4 using CSHELL at the NASA IRTF in the -band wit…

astro-ph.IM2016★ 15 cited

Retrieval of Precise Radial Velocities from Near-Infrared High Resolution Spectra of Low Mass Stars

Peter Gao, Peter Plavchan, Jonathan Gagné +21

Given that low-mass stars have intrinsically low luminosities at optical wavelengths and a propensity for stellar activity, it is advantageous for radial velocity (RV) surveys of t…