Events

Hanyu Zhang is a postdoctoral fellow at the Waterloo Centre for Astrophysics. He completed his Ph.D in physics at Kansas State University under the supervision of Dr. Lado Samushia. Hanyu is actively involved in the DESI collaboration, contributing to various projects, working groups, and co-leading the Galaxy-Halo Connection topical group.

Renee Hlozek is an Associate Professor at the Dunlap Institute of Astronomy and Astrophysics and the Department of Astronomy and Astrophysics at UofT. She was born in Pretoria, South Africa where she completed her undergraduate degree. She completed her DPhil at Oxford University in 2011 as a South African Rhodes Scholar.

The WCA-KPL Astronomy Talk series takes place on the last Wednesday of each month, and is jointly organized by the Waterloo Centre for Astrophysics and KPL.

Ryan Cloutier is an Assistant Professor in the Department of Physics and Astronomy at McMaster University. Ryan completed his PhD at the University of Toronto before taking up a postdoctoral fellowship and a Banting Fellowship at the Center for Astrophysics, Harvard and Smithsonian.

Astroseminar Series - Lara Phillips - HYBRID

Astronomy on Tap at the Crazy Canuck Kitchener

Bobby Bickley is an astronomy Ph.D. candidate at the University of Victoria (Victoria, BC). He also holds a B.Sc. in mechanical engineering from the University of Connecticut.

The WCA-KPL Astronomy Talk series takes place on the last Wednesday of each month, and is jointly organized by the Waterloo Centre for Astrophysics and KPL.

Gerrit Farren is a final year PhD student at the University of Cambridge working primarily on CMB lensing and CMB lensing cross-correlations. Originally from Mönchengladbach in Germany, Gerrit studied at Haverford College in Philadelphia working with Bruce Partridge and Daniel Grin, before moving to Cambridge to pursue his PhD under the supervision of Blake Sherwin.

Sean Ressler is a postdoctoral fellow at CITA working on general relativistic and Newtonian simulations of black hole accretion. The motivation of his work is to make these simulations more realistic by incorporating more physics, more observational input, or connecting smaller scales to larger scales (or vice versa).