papers

Publications (11)

astro-ph.SR2017

Clarifying the Status of HD 100546 as Observed by the Gemini Planet Imager

Thayne Currie, Sean Brittain, Carol Grady +2

HD 100546 is a young, early-type star and key laboratory for studying gas giant planet formation. GPI data taken in 2015 and reported by Currie et al. (2015) recover the previously…

astro-ph2002

A Spectroscopic Survey of Subarcsecond Binaries in the Taurus-Auriga Dark Cloud with the Hubble Space Telescope

Patrick Hartigan, Scott Kenyon

We report the results of a spectroscopic survey of 20 close T Tauri binaries in the Taurus-Auriga dark cloud where the separations between primaries and their secondaries are less…

astro-ph.SR2026

The MIRI Excess around Degenerates (MEAD) Survey II: A Probable Planet detected via IR Excess around WD 0644+025

Sabrina Poulsen, John Debes, Ashley Messier +14

The MIRI Excess Around Degenerates (MEAD) Survey is a cycle 2 JWST program designed to image nearby white dwarfs with MIRI at 10 and 15 microns. This survey targeted 56 white dwarf…

astro-ph2007

Discovery of Gas Accretion Onto Stars in 13 Myr old h and chi Persei

Thayne Currie, Scott Kenyon, Zoltan Balog +2

We report the discovery of accretion disks associated with ~ 13 Myr-old intermediate/low-mass stars in h and chi Persei. Optical spectroscopy of ~ 5000 stars in these clusters and…

astro-ph.EP2013

A Deep Keck/NIRC2 Search for Thermal Emission from Planetary Companions Orbiting Fomalhaut

Thayne Currie, Ryan Cloutier, John Debes +2

We present deep Keck/NIRC2 1.6 and 3.8 imaging of Fomalhaut to constrain the near-infrared (IR) brightness of Fomalhaut b, recently confirmed as a likely planet (Currie et al…

astro-ph2007

The Rise and Fall of Debris Disks: MIPS Observations of h and chi Persei and the Evolution of Mid-IR Emission from Planet Formation

Thayne Currie, Scott Kenyon, Zoltan Balog +3

We describe Spitzer/MIPS observations of the double cluster, h and Persei, covering a 0.6 square-degree area surrounding the cores of both clusters. The data are combin…