activity
20152021
most citedA planet within the debris disk around the pre-main-sequence star AU Microscopii

242 citations · 788 across the 14 of their papers we have counts for

collaborators

19 papers

astro-ph.EP202178 cited

A nearby transiting rocky exoplanet that is suitable for atmospheric investigation

T. Trifonov, J. A. Caballero, J. C. Morales +66

Spectroscopy of transiting exoplanets can be used to investigate their atmospheric properties and habitability. Combining radial velocity (RV) and transit data provides additional…

astro-ph.IM20201 cited

A small actively-controlled high-resolution spectrograph based on off-the-shelf components

H. R. A. Jones, W. E. Martin, G. Anglada-Escudé +5

We present the design and testing of a prototype in-plane echelle spectrograph based on an actively controlled fibre-fed double-pass design. This system aims to be small and effici…

astro-ph.IM20201 cited

Identification and Mitigation of a Vibrational Telescope Systematic with Application to Spitzer

Ryan C. Challener, Joseph Harrington, James Jenkins +17

We observed Proxima Centauri with the Spitzer Space Telescope InfraRed Array Camera (IRAC) five times in 2016 and 2017 to search for transits of Proxima Centauri b. Following stand…

astro-ph.EP2020242 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.EP2020

Transmission spectroscopy and Rossiter-McLaughlin measurements of the young Neptune orbiting AU Mic

E. Palle, M Oshagh, N. Casasayas-Barris +8

AU Mic~b is a Neptune size planet on a 8.47-day orbit around the nearest pre-main sequence (20 Myr) star to the Sun, the bright (V=8.81) M dwarf AU Mic. The planet was prelim…

astro-ph.EP201919 cited

PEXO: a global modeling framework for nanosecond timing, microsecond astrometry, and m/s radial velocities

Fabo Feng, Maksym Lisogorskyi, Hugh R. A. Jones +4

The ability to make independent detections of the signatures of exoplanets with complementary telescopes and instruments brings a new potential for robust identification of exoplan…