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Photo of Diana Valencia
Assistant Professor, UTSC Composition and Structure of Super-Earths and Mini-Neptunes, Formation processes and chemistry of Rocky Planets, Thermal evolution and Interior Dynamics of Rocky and Icy PlanetsPh.D. 2008, Harvard
Work Phone: 416-208-2986 Website: http://www.astro.utoronto.ca/~valencia/

Biographical Info

The characterisation of the low-mass planets: super-Earths and mini-Neptunes. The former are planets that are mostly solid, either rocky or icy in composition, while the latter posses also a volatile
envelope. My goal is to determine if planets with masses between 1-15 Earth-masses are scaled up versions of Earth, or scaled-down versions of Neptune in terms of their composition, evolution and physical properties.

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Photo of Marten van Kerkwijk
Professor Compact objects, stars and binaries, their structure, formation and evolution, and their use to infer fundamental physical properties.Ph.D. 1993, Amsterdam
Work Phone: 416-946-7288 Website: http://www.astro.utoronto.ca/~mhvk/

Biographical Info

I am interested in compact objects, stars and binaries, their structure, formation and evolution, and their use to infer fundamental physical properties. My research is based on observations, but includes interpretation, theory and numerical modelling as required. Currently, I am trying to use neutron stars to study physics in conditions out of reach of terrestrial experiment, and to solve associated astronomical puzzles. I’ve become particularly intrigued by the possibilities of extremely high resolution astrometry offered by pulsar scintillation.

Categories: Faculty
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Photo of Keith Vanderlinde
Associate Professor, DAA & Dunlap Long wavelength (radio, microwave) instrumentation and cosmology, particularly large scale structure and the expansion history of the universe.Ph.D. 2008, Chicago
Work Phone: 416-946-5436 Website: http://dunlap.utoronto.ca/~vanderlinde

Biographical Info

My primary research interests involve the Large Scale Structure (LSS) in the Universe. By studying its properties and evolution, we can make firm statements about the physical processes which must have been active. Despite — or perhaps because of — its size, the LSS is difficult to observe, and specialized instruments and surveys are required to study it. I work on two such instruments, the South Pole Telescope (SPT), and the Canadian Hydrogen Intensity Mapping Experiment (CHIME).

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Website: https://www.astro.utoronto.ca/~vanderwoude/
Categories: Graduate Students
Updated 6 days ago. Return to top.