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Cavendish Astrophysics |
https://www.astro.phy.cam.ac.uk/9 Jul 2024: Search site. Cavendish Astrophysics. Astronomy in Cambridge. Several groups do research in astronomy at Cambridge. ... Research. Follow this link to find more about our research projects and research activities at the Astrophysics Group. . -
REACH | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/research/research-projects/reach9 Jul 2024: Search site. Cavendish Astrophysics. REACH. REACH. RADIO EXPERIMENT FOR THE ANALYSIS OF COSMIC HYDROGEN. Artist impression of first stars. Adolf Schaller for STScI. Index. Upcoming Talks. Type Ia supernova siblings and the Zwicky Transient Facility. -
M. Alsari | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/m-alsari9 Jul 2024: Search site. Cavendish Astrophysics. M. Alsari. Real name:. Name:. M. Alsari. History. Member for. 3 years 11 months. Upcoming Talks. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN -
Planck reveals first stars were born late | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/Planck9 Jul 2024: Search site. Cavendish Astrophysics. Planck reveals first stars were born late. Submitted by Dr. Eloy de Ler. on Tue, 21/04/2015 - 16:15. New maps from the Planck satellite have uncovered the ‘polarised’ light from the early Universe. New maps -
ukri_logo.png | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/ukrilogopng9 Jul 2024: Search site. Cavendish Astrophysics. ukri_logo.png. 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 the -
Current job vacancies | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/jobs9 Jul 2024: Research Associate in Theoretical Many-Body Physics and Quantum Chaos. ... Research Associate in the study of spintronics and magnetism from dc to THz frequencies. -
E. Sandford | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/e-sandford9 Jul 2024: Search site. Cavendish Astrophysics. E. Sandford. You can see the full profile for Dr Emily Sandford here.. Name:. E. Sandford. History. Member for. 3 years 8 months. Upcoming Talks. Type Ia supernova siblings and the Zwicky Transient Facility. Why -
ami_la_crop.jpg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/amilacropjpg9 Jul 2024: Search site. Cavendish Astrophysics. ami_la_crop.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 the -
2 postdoc positions in the Novel Sensors group! | Cavendish…
https://www.astro.phy.cam.ac.uk/news/job_adverts9 Jul 2024: Search site. Cavendish Astrophysics. 2 postdoc positions in the Novel Sensors group! Submitted by Dr. Eloy de Ler. on Mon, 18/03/2019 - 18:23. See here for more information:. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky -
Graduate Research Opportunities for October 2024 Entry | Cavendish…
https://www.astro.phy.cam.ac.uk/gradresearch9 Jul 2024: PhD Positions. Graduate Research Opportunities for October 2024 Entry. There are wide-ranging opportunities for postgraduate research in the Cavendish Astrophysics Group. ... Information on the current research programmes being carried out in the group -
group_2021.jpeg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/group2021jpeg9 Jul 2024: Search site. Cavendish Astrophysics. group_2021.jpeg. 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 the -
Overview | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/about9 Jul 2024: These techniques are widely applicable outside astronomy. Radio astronomy is thus important both as pure research and as a training for scientists. ... In 1957, through the generosity of Mullard Ltd. and with support from the Science Research Council, -
groupphoto2_.jpg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/groupphoto2jpg9 Jul 2024: Search site. Cavendish Astrophysics. groupphoto2_.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 the -
Outreach | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/outreach9 Jul 2024: See here an extract from a news TV special about the MRAO. -
Current job vacancies | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/jobs/placements9 Jul 2024: Search site. Cavendish Astrophysics. Current job vacanciesPOST-DOCTORAL FELLOWSHIP AVAILABLE. RADIO TELESCOPE HARDWARE SYSTEM DESIGN: ANTENNAS AND RF FRONT-ENDS. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. -
Tobias Looser | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/tobias-looser9 Jul 2024: Search site. Cavendish Astrophysics. Tobias Looser. Tobias Looser. 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 -
Edward Gillen | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/edward-gillen9 Jul 2024: Search site. Cavendish Astrophysics. Edward Gillen. Real name:. Name:. Edward Gillen. History. Member for. 8 years 9 months. Upcoming Talks. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence -
group_small.jpeg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/groupsmalljpeg9 Jul 2024: Search site. Cavendish Astrophysics. group_small.jpeg. Title Text:. Galaxy_Group_2022. Upcoming Talks. 12. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback driven quenching -
Administrator | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/administrator9 Jul 2024: Search site. Cavendish Astrophysics. Administrator. Real name:. Name:. Administrator. History. Member for. 8 years 11 months. Upcoming Talks. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence -
cheops_autoe.jpeg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/cheopsautoejpeg9 Jul 2024: Search site. Cavendish Astrophysics. cheops_autoe.jpeg. 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 the -
Work has started on the HERA prototype antennas at the MRAO |…
https://www.astro.phy.cam.ac.uk/news/HERAatMRAO9 Jul 2024: Search site. Cavendish Astrophysics. Work has started on the HERA prototype antennas at the MRAO. Submitted by Dr. Eloy de Ler. on Sat, 20/02/2016 - 09:19. The Hydrogen Epoch of Re-ionization Array, HERA (www.reionization.org) is major international -
Dr Xihan Ji | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/dr-xihan-ji9 Jul 2024: Kavli Building. Postdoctoral Research Associate. -
Amanda Stoffers | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/amanda-stoffers9 Jul 2024: Search site. Cavendish Astrophysics. Amanda Stoffers. Amanda Stoffers. Room K35. Kavli Building. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback -
Annelies Mortier | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/annelies-mortier9 Jul 2024: Search site. Cavendish Astrophysics. Annelies Mortier. Real name:. Name:. Annelies Mortier. History. Member for. 5 years 8 months. Upcoming Talks. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? -
e-elt-1_2008.jpg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/e-elt-12008jpg9 Jul 2024: Search site. Cavendish Astrophysics. e-elt-1_2008.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 the -
Research | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/research9 Jul 2024: Research. The Astrophysics Group carries out a wide range of research activities and projects, with particular emphasis on the fields of optical interferometry, the cosmic microwave background (CMB) radiation,and exoplanets. ... If you are -
Ignas Juodžbalis | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/ignas-juodzbalis9 Jul 2024: Search site. Cavendish Astrophysics. Ignas Juodžbalis. Ignas Juodžbalis. Room K35. Kavli Building. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN -
http://www.astro.phy.cam.ac.uk/blog-support/blog-collection/RSS |…
https://www.astro.phy.cam.ac.uk/aggregator/sources/59 Jul 2024: Search site. Cavendish Astrophysics. http://www.astro.phy.cam.ac.uk/blog-support/blog-collection/RSS. URL:. Updated: 1 hour 14 min ago. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease -
conference | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/subject/conference9 Jul 2024: Search site. Cavendish Astrophysics. conferenceOur experiment is the Universe'' Dr Rosie Bolton said. The International Conference for High Performance Computing, Networking, Storage and Analysis , held in Denver (Colorado) in November 2017, was the -
Prof. D.P. Queloz | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/prof-dp-queloz9 Jul 2024: Search site. Cavendish Astrophysics. Prof. D.P. Queloz. You can see theReal name:. Name:. Prof. D.P. Queloz. History. Member for. 10 years 3 months. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do -
Dr S.J. Thompson | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/dr-sj-thompson9 Jul 2024: Search site. Cavendish Astrophysics. Dr S.J. Thompson. You can see theReal name:. Name:. Dr S.J. Thompson. History. Member for. 10 years 3 months. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies -
Nobel Prize in Physics for Didier Queloz | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/NobelPrize9 Jul 2024: Search site. Cavendish Astrophysics. Nobel Prize in Physics for Didier Queloz. Submitted by Dr. Eloy de Ler. on Tue, 08/10/2019 - 11:30. Nobel Prize in Physics awarded to Prof Didier Queloz from Cavendish Astrophysics. Congratulations Didier Queloz -
Launch of new AP website | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/Website9 Jul 2024: on Tue, 21/04/2015 - 16:24. 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 talks are now news feeds -
Cavendish Laboratory researchers detect hints of an Earth-size planet …
https://www.astro.phy.cam.ac.uk/news/ExoPlanet_Brice9 Jul 2024: Search site. Cavendish Astrophysics. Cavendish Laboratory researchers detect hints of an Earth-size planet in the Alpha Centauri star system. Submitted by Dr. Eloy de Ler. on Tue, 21/04/2015 - 16:32. Brice-Oliver Demory (Cavendish Laboratory) leads -
Dr Boris Bolliet | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/dr-boris-bolliet9 Jul 2024: Search site. Cavendish Astrophysics. Dr Boris Bolliet. Dr Boris Bolliet. Assistant Teaching Professor. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN -
Dr Seunghwan Lim | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/dr-seunghwan-lim9 Jul 2024: Search site. Cavendish Astrophysics. Dr Seunghwan Lim. Dr Seunghwan Lim. Room K23. Kavli Building. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback -
William McClymont | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/william-mcclymont9 Jul 2024: Search site. Cavendish Astrophysics. William McClymont. 2022 - present: PhD in Physics (Cavendish Astrophysics, Kavli Institute for Cosmology). 2018 - 2022: Physics MPhys (University of Surrey). Contact Details. Email address:. K31. Not available -
The RAPID portable interferometer deploys its first units | Cavendish …
https://www.astro.phy.cam.ac.uk/news/RAPID_update9 Jul 2024: Search site. Cavendish Astrophysics. The RAPID portable interferometer deploys its first units. Submitted by Dr. Eloy de Ler. on Mon, 22/05/2017 - 12:43. The Radio Array of Portable Interferometric Detectors (RAPID) is a collaboration between MIT, -
3rd Global 21-cm Workshop | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/21cmGlobalWorkshop9 Jul 2024: Search site. Cavendish Astrophysics. 3rd Global 21-cm Workshop. Submitted by Dr. Eloy de Ler. on Tue, 16/06/2020 - 12:33. Registration is open! The 3rd Global 21-cm Workshop will take place in Cambridge (and online!) from the 19th to the 22nd of -
Sources | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/aggregator/sources9 Jul 2024: Research Associate in Theoretical Many-Body Physics and Quantum Chaos 6 days 11 hours old. ... Research Associate in the study of spintronics and magnetism from dc to THz frequencies 2 weeks 6 days old. -
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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