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Peter M. Tamblyn

Southwest Research Institute

71

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The triaxial ellipsoid size, density, and rotational pole of asteroid (16) Psyche from Keck and Gemini AO observations 2004–2015

2018 Icarus
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Physical, spectral, and dynamical properties of asteroid (107) Camilla and its satellites

2018 Icarus
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Dwarf planet Ceres: Ellipsoid dimensions and rotational pole from Keck and VLT adaptive optics images☆

2014 Icarus
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The Resolved Asteroid Program - Size, shape, and pole of (52) Europa

2013 Icarus
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Shape modeling technique KOALA validated by ESA Rosetta at (21) Lutetia

2012 Planetary and Space Science
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The Irregular Shape of (21) Lutetia as Determined from Ground-based Observations

2010
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Physical properties of the ESA Rosetta target asteroid (21) Lutetia I. The triaxial ellipsoid dimensions, rotational pole, and bulk density

2010 Astronomy and Astrophysics
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Pre-flyby Determination Of The Size, Shape, Pole, Density, And Satellites Of (21) Lutetia From Ground-based Observations

2010
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High-Resolution AO Imaging of Asteroids/Satellites

2009
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Recent Results from Imaging Asteroids with Adaptive Optics

2009
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