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Post Docs

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Photo of Daniel Gilman
Postdoctoral Fellow with Prof. Bovy Strong gravitational lensing, dark matter substructure, galactic dynamicsPhD in Physics, UCLA
Website: https://www.astro.utoronto.ca/~gilman/
Categories: Post Docs
Updated 6 days ago. Return to top.
Photo of Nina Gusinskaia
Postdoctoral Fellow with Prof. van Kerkwijk & Pen Multi-wavelength observations of accreting neutron stars and radio pulsars, pulsar scintillometry, radio interferometry, theories of gravity (tests of GR and alternatives)
Work Phone: 416-978-2870 Website: https://www.astro.utoronto.ca/~gusinskaia
Categories: Post Docs
Updated 7 months ago. Return to top.

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Photo of David Hendel
Postdoctoral Fellow with Prof. Bovy
Website: http://www.astro.utoronto.ca/~hendel/
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Photo of Jing Luo
Postdoctoral Fellow with Prof. van Kerkwijk
Website: http://www.astro.utoronto.ca/~luo/
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Updated 4 months ago. Return to top.

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Photo of Irene Pintos-Castro
Postdoctoral Fellow with Prof. Yee Galaxy clusters and their galaxy population, galaxy evolution, emission-line galaxies, star formation quenching
Website: http://www.astro.utoronto.ca/~pintos/
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S

Photo of Josh Speagle
Postdoctoral Fellow with Prof. Eadie Astrostatistics and data science with multi-wavelength, large-area surveys; Galactic structure and dynamics; stars and stellar populations; dust and the interstellar medium; galaxy formation and evolution; scalable inference; Monte Carlo samplingPh.D. 2020, Harvard University
Website: https://www.astro.utoronto.ca/~speagle

Biographical Info

I am a Banting-Dunlap Postdoctoral Fellow jointly hosted between the
Department of Statistical Sciences, the Department of Astronomy &
Astrophysics, and the Dunlap Institute. My research focuses on using a
combination of astronomy, statistics, and computer science to combine and
analyze billions of stars and galaxies from wide-field imaging and
spectroscopic surveys to better understand the how galaxies like the Milky
Way form, behave, and evolve over time.

Categories: Post Docs
Updated 6 days ago. Return to top.