Sara Ellison

Sara Ellison (birth date unknown) is an Astronomy Professor at University of Victoria. Her work involves observational extragalactic astronomy, galaxy mergers and evolution, galactic chemistry and AGN.[1]

Background and education

Dr. Ellison enrolled in Physics and Space Science in University of Kent in 1993 and received her Master of Physics from University of Kent in 1997. She went on to earn her PhD degree in Astronomy from University of Cambridge in 2000. Afterwards she was an ESO fellow working at Chile for three years, and in 2003 joined the faculty of University of Victoria as an Assistant Professor. The same year, she was selected as Canada Research Chair (Tier II), an grant given to extraordinary emerging researchers by the Canadian government. In 2008, she became an Associate Professor and in 2014 a full Professor at the University of Victoria.[2]

Research

The main themes of Ellison's research are studying absorption lines in quasar spectra and studying the effects of environment on galaxy evolution.[3] Her quasar work has focused on studying the chemistry of gas along the line-of-sight to quasars such as Damped Lyman-alpha systems[4] and the Lyman-alpha forest.[5] Much of Ellison's most recent work has focused on using close pairs of galaxies in the Sloan Digital Sky Survey to investigate how galaxy interactions affect galaxy evolution.[6][7]

Personal

Besides her work in astronomy, Professor Ellison is also very involved in science outreach since 1992.[8] She has appeared in CBC Radio's Quarks and Quirks to answer questions about lunar landing sites.[9] In a 2015 interview with Vancouver Sun, she spoke about how she got interested in Astronomy.[10] Her hobbies include painting on stretched canvas in acrylics.[11] An accomplished amateur athlete, Ellison has a Boston Qualifying marathon time and age group wins in both running and triathlon.[12]

Honours and awards

References

  1. ↑ "Astronomy Research". astro.uvic.ca. Retrieved 15 June 2016.
  2. ↑ "A Brief CV". astro.uvic.ca. Retrieved 15 June 2016.
  3. ↑ "Astronomy Research". astro.uvic.ca. Retrieved 15 June 2016.
  4. ↑ Ellison, S. L.; Yan, L.; Hook, I. M.; Pettini, M.; Wall, J. V.; Shaver, P. (2001). "The CORALS survey I: New estimates of the number density and gas content of damped Lyman alpha systems free from dust bias". Astronomy and Astrophysics. 379: 393–406. arXiv:astro-ph/0109205. Bibcode:2001A&A...379..393E. doi:10.1051/0004-6361:20011281.
  5. ↑ Ellison, Sara L.; Songaila, Antoinette; Schaye, Joop; Pettini, M. (2000). "The Enrichment History of the Intergalactic Medium-Measuring the C IV/H I Ratio in the Lyα Forest". The Astronomical Journal. 120: 1175–1191. arXiv:astro-ph/0005448. Bibcode:2000AJ....120.1175E. doi:10.1086/301511.
  6. ↑ Ellison, Sara L.; Patton, David R.; Simard, Luc; McConnachie, Alan W. (2008). "Galaxy Pairs in the Sloan Digital Sky Survey. I. Star Formation, Active Galactic Nucleus Fraction, and the Mass-Metallicity Relation". The Astronomical Journal. 135: 1877–1899. arXiv:0803.0161. Bibcode:2008AJ....135.1877E. doi:10.1088/0004-6256/135/5/1877.
  7. ↑ Ellison, Sara L.; Patton, David R.; Mendel, J. Trevor; Scudder, Jillian M. (2008). "Galaxy pairs in the Sloan Digital Sky Survey – IV. Interactions trigger active galactic nuclei". Monthly Notices of the Royal Astronomical Society. 418: 2043–2053. arXiv:1108.2711. Bibcode:2011MNRAS.418.2043E. doi:10.1088/0004-6256/135/5/1877.
  8. ↑ "Astronomy Outreach". astro.uvic.ca. Retrieved 15 June 2016.
  9. ↑ "Quirks Question Period – Lunar Landing Sites". Canadian Broadcasting Corporation. Retrieved 15 June 2016.
  10. ↑ Robinson, ,Matthew. "Q&A: Gazing into space to see the future". The Vancouver Sun. Retrieved 15 June 2016.
  11. ↑ "Sara's Art Page". astro.uvic.ca. Retrieved 15 June 2016.
  12. ↑ "Sara's Race Page". astro.uvic.ca. Retrieved 15 June 2016.
  13. ↑ "A Brief CV". astro.uvic.ca. Retrieved 15 June 2016.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.