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Cavendish Astrophysics |
https://www.astro.phy.cam.ac.uk/5 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/reach5 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. -
Planck reveals first stars were born late | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/Planck5 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 -
M. Alsari | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/m-alsari5 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 -
ukri_logo.png | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/ukrilogopng5 Jul 2024: Search site. Cavendish Astrophysics. ukri_logo.png. Upcoming Talks. 05. 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 -
Graduate Research Opportunities for October 2024 Entry | Cavendish…
https://www.astro.phy.cam.ac.uk/gradresearch5 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 -
E. Sandford | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/e-sandford5 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/amilacropjpg5 Jul 2024: Search site. Cavendish Astrophysics. ami_la_crop.jpg. Upcoming Talks. 05. 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_adverts5 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 -
Overview | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/about5 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, -
group_2021.jpeg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/group2021jpeg5 Jul 2024: Search site. Cavendish Astrophysics. group_2021.jpeg. Upcoming Talks. 05. 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 -
Edward Gillen | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/edward-gillen5 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 -
Work has started on the HERA prototype antennas at the MRAO |…
https://www.astro.phy.cam.ac.uk/news/HERAatMRAO5 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 -
Current job vacancies | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/jobs5 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. -
Outreach | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/outreach5 Jul 2024: See here an extract from a news TV special about the MRAO. -
Research | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/research5 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 -
groupphoto2_.jpg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/groupphoto2jpg5 Jul 2024: Search site. Cavendish Astrophysics. groupphoto2_.jpg. Upcoming Talks. 05. 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/jobs/placements5 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-looser5 Jul 2024: Search site. Cavendish Astrophysics. Tobias Looser. Tobias Looser. Upcoming Talks. 05. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback driven quenching from cosmic -
Launch of new AP website | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/Website5 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 -
Blog | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/blog5 Jul 2024: Search site. Cavendish Astrophysics. Blog. Earliest galaxies in the Universe’s history spun like the Milky Way. Artist impression of rotation in a galaxy in the early Universe, credit: Institute of Astronomy, Amanda Smith. Astronomers have looked -
group_small.jpeg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/groupsmalljpeg5 Jul 2024: Search site. Cavendish Astrophysics. group_small.jpeg. Title Text:. Galaxy_Group_2022. Upcoming Talks. 05. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback driven quenching -
Nobel Prize in Physics for Didier Queloz | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/NobelPrize5 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 -
cheops_autoe.jpeg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/cheopsautoejpeg5 Jul 2024: Search site. Cavendish Astrophysics. cheops_autoe.jpeg. Upcoming Talks. 05. 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 -
Administrator | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/administrator5 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 -
Dr Xihan Ji | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/dr-xihan-ji5 Jul 2024: Kavli Building. Postdoctoral Research Associate. -
conference | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/subject/conference5 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 -
Annelies Mortier | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/annelies-mortier5 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? -
Amanda Stoffers | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/amanda-stoffers5 Jul 2024: Search site. Cavendish Astrophysics. Amanda Stoffers. Amanda Stoffers. Room K35. Kavli Building. Upcoming Talks. 05. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback -
Prof. D.P. Queloz | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/users/prof-dp-queloz5 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 2 months. Upcoming Talks. 05. 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-thompson5 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 2 months. Upcoming Talks. 05. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies -
HERA joins the SKA as a precursor | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/HERA_SKA5 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 -
http://www.astro.phy.cam.ac.uk/blog-support/blog-collection/RSS |…
https://www.astro.phy.cam.ac.uk/aggregator/sources/55 Jul 2024: Search site. Cavendish Astrophysics. http://www.astro.phy.cam.ac.uk/blog-support/blog-collection/RSS. URL:. Updated: 31 min 37 sec ago. Upcoming Talks. 12. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease -
Ignas Juodžbalis | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/ignas-juodzbalis5 Jul 2024: Search site. Cavendish Astrophysics. Ignas Juodžbalis. Ignas Juodžbalis. Room K35. Kavli Building. Upcoming Talks. 05. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN -
e-elt-1_2008.jpg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/e-elt-12008jpg5 Jul 2024: Search site. Cavendish Astrophysics. e-elt-1_2008.jpg. Upcoming Talks. 05. 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 -
Sources | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/aggregator/sources5 Jul 2024: Research Associate in Theoretical Many-Body Physics and Quantum Chaos 2 days 11 hours old. ... Research Associate in the study of spintronics and magnetism from dc to THz frequencies 2 weeks 2 days old. -
The RAPID portable interferometer deploys its first units | Cavendish …
https://www.astro.phy.cam.ac.uk/news/RAPID_update5 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, -
Galactic ‘hailstorm’ in the early Universe | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/hailstorm5 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 -
News | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/aggregator/RSS5 Jul 2024: 1 March 2021. Prof Roberto Maiolino awarded a prestigious Royal Society Research Professorship! ... Research Associate position (fixed term) to work on SKA1-LOW simulations and calibration. -
Cavendish Laboratory researchers detect hints of an Earth-size planet …
https://www.astro.phy.cam.ac.uk/news/ExoPlanet_Brice5 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 -
REACH, the Radio Experiment for the Analysis of Cosmic Hydrogen…
https://www.astro.phy.cam.ac.uk/news/REACH5 Jul 2024: Search site. Cavendish Astrophysics. REACH, the Radio Experiment for the Analysis of Cosmic Hydrogen begins its path to unveil the mysteries of the early Universe. Submitted by Dr. Eloy de Ler. on Sun, 20/01/2019 - 18:58. How did the first luminous -
SKA's 400 AAVS1 antennas on their way from Cambridge to Western…
https://www.astro.phy.cam.ac.uk/news/AAVS1_aerials5 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 -
William McClymont | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/william-mcclymont5 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 -
Launch of new AP website | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/WebSiteLaunch5 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 -
Dr Seunghwan Lim | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/dr-seunghwan-lim5 Jul 2024: Search site. Cavendish Astrophysics. Dr Seunghwan Lim. Dr Seunghwan Lim. Room K23. Kavli Building. Upcoming Talks. 05. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN feedback -
Dr Boris Bolliet | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/staff/dr-boris-bolliet5 Jul 2024: Search site. Cavendish Astrophysics. Dr Boris Bolliet. Dr Boris Bolliet. Assistant Teaching Professor. Upcoming Talks. 05. Jul. Type Ia supernova siblings and the Zwicky Transient Facility. Why do galaxies cease forming stars? Evidence for AGN -
3rd Global 21-cm Workshop | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/news/21cmGlobalWorkshop5 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 -
World’s Largest Radio Telescope Has A Permanent Home For Its…
https://www.astro.phy.cam.ac.uk/news/SKAHQ5 Jul 2024: Search site. Cavendish Astrophysics. World’s Largest Radio Telescope Has A Permanent Home For Its Headquarters. Submitted by Dr. Eloy de Ler. on Wed, 06/05/2015 - 09:58. SKA Organisation headquarters, Jodrell Bank, UK - At their meeting on -
Research Facilities | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/research/ResearchFacilities5 Jul 2024: Search site. Cavendish Astrophysics. Research Facilities. Research Facilities. Research Facilities for the Astronomical Community. -
9egejjzqp2gwzv7pe7etf5.jpg | Cavendish Astrophysics
https://www.astro.phy.cam.ac.uk/file/9egejjzqp2gwzv7pe7etf5jpg5 Jul 2024: Search site. Cavendish Astrophysics. 9egejjzqp2gwzv7pe7etf5.jpg. Upcoming Talks. 05. 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
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