PIRSA:17010076

Video URL

https://pirsa.org/17010076

CHIME: The Canadian Hydrogen Intensity Mapping Experiment

Smith, K. (2017). CHIME: The Canadian Hydrogen Intensity Mapping Experiment. Perimeter Institute for Theoretical Physics. https://pirsa.org/17010076

Smith, Kendrick. CHIME: The Canadian Hydrogen Intensity Mapping Experiment. Perimeter Institute for Theoretical Physics, Jan. 17, 2017, https://pirsa.org/17010076 

          @misc{ scivideos_PIRSA:17010076,
            doi = {10.48660/17010076},
            url = {https://pirsa.org/17010076},
            author = {Smith, Kendrick},
            keywords = {Cosmology},
            language = {en},
            title = {CHIME: The Canadian Hydrogen Intensity Mapping Experiment},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2017},
            month = {jan},
            note = {PIRSA:17010076 see, \url{https://scivideos.org/index.php/pirsa/17010076}}
          }

Kendrick Smith Perimeter Institute for Theoretical Physics

Talk numberPIRSA:17010076
DOI10.48660/17010076
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

CHIME is a new interferometric telescope at radio frequencies 400-800 MHz.  The mapping speed (or total statistical power) of CHIME is among the largest of any radio telescope in the world, and the technology powering CHIME could be used to build telescopes which are orders of magnitude more powerful.  This breakthrough sensitivity has the power to revolutionize radio astronomy, but meeting the computational challenges will require breakthroughs on the algorithmic side.  I'll give a status update on CHIME, with an emphasis on new algorithms being developed to search for fast radio bursts and pulsars.