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HERA joins the SKA as a precursor | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/HERA_SKA9 Jul 2024: Search site. Cavendish Astrophysics. HERA joins the SKA as a precursor. Submitted by Dr. Eloy de Ler. on Mon, 04/07/2016 - 12:49. The Hydrogen Epoch of Re-ionization array (HERA) has just joined the family of SKA precursors. HERA, which is being -
SKA's 400 AAVS1 antennas on their way from Cambridge to Western…
https://www.astro.phy.cam.ac.uk/news/AAVS1_aerials9 Jul 2024: Search site. Cavendish Astrophysics. SKA's 400 AAVS1 antennas on their way from Cambridge to Western Australia. Submitted by Dr. Eloy de Ler. on Fri, 04/11/2016 - 15:54. 444 units of the latest version of the SKALA antenna elements designed at -
9egejjzqp2gwzv7pe7etf5.jpg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/9egejjzqp2gwzv7pe7etf5jpg9 Jul 2024: Search site. Cavendish Astrophysics. 9egejjzqp2gwzv7pe7etf5.jpg. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback driven quenching from cosmic dawn -
ywmwrukktgprtkejwlypym.jpg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/ywmwrukktgprtkejwlypymjpg9 Jul 2024: Search site. Cavendish Astrophysics. ywmwrukktgprtkejwlypym.jpg. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback driven quenching from cosmic dawn -
Julia Riley | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/directory/julia-riley9 Jul 2024: Search site. Cavendish Astrophysics. Julia Riley. Julia Riley. Room F23,. Battcock Centre for Experimental Astrophysics. 44 (0)1223 337308. Contact us. Battcock Centre for Experimental Astrophysics. Cavendish Laboratory. JJ Thomson Avenue. Cambridge -
img-20230422-wa0025.jpg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/img-20230422-wa0025jpg9 Jul 2024: Search site. Cavendish Astrophysics. img-20230422-wa0025.jpg. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback driven quenching from cosmic dawn to -
Dr Charlotte Simmonds | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/dr-charlotte-simmonds9 Jul 2024: Search site. Cavendish Astrophysics. Dr Charlotte Simmonds. Dr Charlotte Simmonds. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback driven quenching -
Research Facilities | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/research/ResearchFacilities9 Jul 2024: Search site. Cavendish Astrophysics. Research Facilities. Research Facilities. Research Facilities for the Astronomical Community. -
Galactic ‘hailstorm’ in the early Universe | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/hailstorm9 Jul 2024: Search site. Cavendish Astrophysics. Galactic ‘hailstorm’ in the early Universe. Submitted by Dr. Eloy de Ler. on Wed, 15/04/2015 - 11:58. A group of scientists led by Claudia Cicone (PhD student at Cavendish) and Prof. Roberto Maiolino -
Launch of new AP website | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/WebSiteLaunch9 Jul 2024: Cavendish Astrophysics has developed a new website. Cavendish Astrophysics has developed a new website, more dynamic, with social network content and updated information of our research groups and projects. ... Furthermore our Latest news and Upcoming
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