TBC
Lead Research Organisation:
University of Cambridge
Department Name: Physics
Abstract
TBC
Organisations
- University of Cambridge, United Kingdom (Lead Research Organisation)
- Washington University in St. Louis (Collaboration)
- University of California, Berkeley (Collaboration)
- University of Pennsylvania, United States (Collaboration)
- Massachusetts Institute of Technology (Collaboration)
- National Radio Astronomy Observatory (NRAO) (Collaboration)
- Scuola Normale Superiore di Pisa (Collaboration)
- Square Kilometre Array (SKA) Africa (Collaboration)
- Arizona State University (Collaboration)
- University of California Los Angeles, United States (Collaboration)
- Brown University, United States (Collaboration)
- ESO - European Southern Observatory, Germany (Student Project Partner)
Studentship Projects
| Project Reference | Relationship | Related To | Start | End | Student Name |
|---|---|---|---|---|---|
| ST/P006787/1 | 30/09/2017 | 29/09/2024 | |||
| 2025421 | Studentship | ST/P006787/1 | 30/09/2017 | 29/03/2022 | Matyas David Molnar |
| Description | Stachulski Dudding Fund - Fitzwilliam College Travel and Research Funding |
| Amount | £400 (GBP) |
| Organisation | University of Cambridge |
| Department | Fitzwilliam College |
| Sector | Academic/University |
| Country | United Kingdom |
| Start | 03/2018 |
| End | 05/2018 |
| Description | HERA |
| Organisation | Arizona State University |
| Country | United States |
| Sector | Academic/University |
| PI Contribution | The Hydrogen Epoch of Reionization Array (HERA) collaboration aims to observe large scale structure during and prior to the epoch of reionization, through radio interferometry. My contribution to the collaboration is to perform independent analysis of the interferometric dataset, and to develop novel calibration methods to better extract the important features of the data. |
| Collaborator Contribution | Ultimately, HERA aims to make a robust statistical detection of the light from the first stars in the Universe (this is when reionization occurs). Currently, upper bounds have been set on this signal, enabled by advances in instrumentation, calibration methods, and power spectrum estimation techniques. |
| Impact | A list of papers from the collaboration can be found here: http://reionization.org/science/papers/. |
| Start Year | 2012 |
| Description | HERA |
| Organisation | Brown University |
| Country | United States |
| Sector | Academic/University |
| PI Contribution | The Hydrogen Epoch of Reionization Array (HERA) collaboration aims to observe large scale structure during and prior to the epoch of reionization, through radio interferometry. My contribution to the collaboration is to perform independent analysis of the interferometric dataset, and to develop novel calibration methods to better extract the important features of the data. |
| Collaborator Contribution | Ultimately, HERA aims to make a robust statistical detection of the light from the first stars in the Universe (this is when reionization occurs). Currently, upper bounds have been set on this signal, enabled by advances in instrumentation, calibration methods, and power spectrum estimation techniques. |
| Impact | A list of papers from the collaboration can be found here: http://reionization.org/science/papers/. |
| Start Year | 2012 |
| Description | HERA |
| Organisation | Massachusetts Institute of Technology |
| Country | United States |
| Sector | Academic/University |
| PI Contribution | The Hydrogen Epoch of Reionization Array (HERA) collaboration aims to observe large scale structure during and prior to the epoch of reionization, through radio interferometry. My contribution to the collaboration is to perform independent analysis of the interferometric dataset, and to develop novel calibration methods to better extract the important features of the data. |
| Collaborator Contribution | Ultimately, HERA aims to make a robust statistical detection of the light from the first stars in the Universe (this is when reionization occurs). Currently, upper bounds have been set on this signal, enabled by advances in instrumentation, calibration methods, and power spectrum estimation techniques. |
| Impact | A list of papers from the collaboration can be found here: http://reionization.org/science/papers/. |
| Start Year | 2012 |
| Description | HERA |
| Organisation | National Radio Astronomy Observatory (NRAO) |
| Country | United States |
| Sector | Public |
| PI Contribution | The Hydrogen Epoch of Reionization Array (HERA) collaboration aims to observe large scale structure during and prior to the epoch of reionization, through radio interferometry. My contribution to the collaboration is to perform independent analysis of the interferometric dataset, and to develop novel calibration methods to better extract the important features of the data. |
| Collaborator Contribution | Ultimately, HERA aims to make a robust statistical detection of the light from the first stars in the Universe (this is when reionization occurs). Currently, upper bounds have been set on this signal, enabled by advances in instrumentation, calibration methods, and power spectrum estimation techniques. |
| Impact | A list of papers from the collaboration can be found here: http://reionization.org/science/papers/. |
| Start Year | 2012 |
| Description | HERA |
| Organisation | Scuola Normale Superiore di Pisa |
| Country | Italy |
| Sector | Academic/University |
| PI Contribution | The Hydrogen Epoch of Reionization Array (HERA) collaboration aims to observe large scale structure during and prior to the epoch of reionization, through radio interferometry. My contribution to the collaboration is to perform independent analysis of the interferometric dataset, and to develop novel calibration methods to better extract the important features of the data. |
| Collaborator Contribution | Ultimately, HERA aims to make a robust statistical detection of the light from the first stars in the Universe (this is when reionization occurs). Currently, upper bounds have been set on this signal, enabled by advances in instrumentation, calibration methods, and power spectrum estimation techniques. |
| Impact | A list of papers from the collaboration can be found here: http://reionization.org/science/papers/. |
| Start Year | 2012 |
| Description | HERA |
| Organisation | Square Kilometre Array (SKA) Africa |
| Country | South Africa |
| Sector | Academic/University |
| PI Contribution | The Hydrogen Epoch of Reionization Array (HERA) collaboration aims to observe large scale structure during and prior to the epoch of reionization, through radio interferometry. My contribution to the collaboration is to perform independent analysis of the interferometric dataset, and to develop novel calibration methods to better extract the important features of the data. |
| Collaborator Contribution | Ultimately, HERA aims to make a robust statistical detection of the light from the first stars in the Universe (this is when reionization occurs). Currently, upper bounds have been set on this signal, enabled by advances in instrumentation, calibration methods, and power spectrum estimation techniques. |
| Impact | A list of papers from the collaboration can be found here: http://reionization.org/science/papers/. |
| Start Year | 2012 |
| Description | HERA |
| Organisation | University of California, Berkeley |
| Country | United States |
| Sector | Academic/University |
| PI Contribution | The Hydrogen Epoch of Reionization Array (HERA) collaboration aims to observe large scale structure during and prior to the epoch of reionization, through radio interferometry. My contribution to the collaboration is to perform independent analysis of the interferometric dataset, and to develop novel calibration methods to better extract the important features of the data. |
| Collaborator Contribution | Ultimately, HERA aims to make a robust statistical detection of the light from the first stars in the Universe (this is when reionization occurs). Currently, upper bounds have been set on this signal, enabled by advances in instrumentation, calibration methods, and power spectrum estimation techniques. |
| Impact | A list of papers from the collaboration can be found here: http://reionization.org/science/papers/. |
| Start Year | 2012 |
| Description | HERA |
| Organisation | University of California, Los Angeles (UCLA) |
| Country | United States |
| Sector | Academic/University |
| PI Contribution | The Hydrogen Epoch of Reionization Array (HERA) collaboration aims to observe large scale structure during and prior to the epoch of reionization, through radio interferometry. My contribution to the collaboration is to perform independent analysis of the interferometric dataset, and to develop novel calibration methods to better extract the important features of the data. |
| Collaborator Contribution | Ultimately, HERA aims to make a robust statistical detection of the light from the first stars in the Universe (this is when reionization occurs). Currently, upper bounds have been set on this signal, enabled by advances in instrumentation, calibration methods, and power spectrum estimation techniques. |
| Impact | A list of papers from the collaboration can be found here: http://reionization.org/science/papers/. |
| Start Year | 2012 |
| Description | HERA |
| Organisation | University of Pennsylvania |
| Country | United States |
| Sector | Academic/University |
| PI Contribution | The Hydrogen Epoch of Reionization Array (HERA) collaboration aims to observe large scale structure during and prior to the epoch of reionization, through radio interferometry. My contribution to the collaboration is to perform independent analysis of the interferometric dataset, and to develop novel calibration methods to better extract the important features of the data. |
| Collaborator Contribution | Ultimately, HERA aims to make a robust statistical detection of the light from the first stars in the Universe (this is when reionization occurs). Currently, upper bounds have been set on this signal, enabled by advances in instrumentation, calibration methods, and power spectrum estimation techniques. |
| Impact | A list of papers from the collaboration can be found here: http://reionization.org/science/papers/. |
| Start Year | 2012 |
| Description | HERA |
| Organisation | University of Washington |
| Country | United States |
| Sector | Academic/University |
| PI Contribution | The Hydrogen Epoch of Reionization Array (HERA) collaboration aims to observe large scale structure during and prior to the epoch of reionization, through radio interferometry. My contribution to the collaboration is to perform independent analysis of the interferometric dataset, and to develop novel calibration methods to better extract the important features of the data. |
| Collaborator Contribution | Ultimately, HERA aims to make a robust statistical detection of the light from the first stars in the Universe (this is when reionization occurs). Currently, upper bounds have been set on this signal, enabled by advances in instrumentation, calibration methods, and power spectrum estimation techniques. |
| Impact | A list of papers from the collaboration can be found here: http://reionization.org/science/papers/. |
| Start Year | 2012 |