UCL Astrophysics Consolidated Grant 2021-2024
Lead Research Organisation:
UNIVERSITY COLLEGE LONDON
Department Name: Physics and Astronomy
Abstract
The research we conduct in the UCL Astrophysics Group encompasses all the big questions of modern Astrophysics and on all scales, from exoplanets to the entire Universe. We have leading roles in large, international projects which are gathering data for millions of stars and galaxies. Our overall goals are to (1) analyse these data to answer fundamental questions about the Universe, (2) develop the theory and models that enable the interpretation for these data, and (3) produce the technologies making these state-of-the-art facilities a reality.
We propose a programme of ten science projects, divided in five themes covering the full range of topics studied within our group: Exoplanets, Galactic Astrophysics, Extragalactic Astrophysics, Cosmology and Instrumentation.
By the nature of our group, most of this work is observational; one of our keys to success is the close interaction between our instrumentation and science groups, allowing us direct access to large international projects. Our observational projects make use of facilities such as eMERLIN, the James Clerk Maxwell Telescope (JCMT), the Dark Energy Spectroscopic Instrument (DESI), and Euclid. With these facilities, we will study debris disks around white dwarf stars, the most massive stars in our Galaxy as well as some of the most massive galaxies in the early Universe, investigate the connection between galaxies and their dark matter halos, and answer fundamental questions in our cosmological model. We also propose two projects that are theoretical and numerical in nature, both concerned with the molecules that make up the atmospheres of exoplanets and the birth clouds of stars. In addition, we present an outreach case, designed to enable us to disseminate to the public the specific outputs of the research to be funded by this grant.
We propose a programme of ten science projects, divided in five themes covering the full range of topics studied within our group: Exoplanets, Galactic Astrophysics, Extragalactic Astrophysics, Cosmology and Instrumentation.
By the nature of our group, most of this work is observational; one of our keys to success is the close interaction between our instrumentation and science groups, allowing us direct access to large international projects. Our observational projects make use of facilities such as eMERLIN, the James Clerk Maxwell Telescope (JCMT), the Dark Energy Spectroscopic Instrument (DESI), and Euclid. With these facilities, we will study debris disks around white dwarf stars, the most massive stars in our Galaxy as well as some of the most massive galaxies in the early Universe, investigate the connection between galaxies and their dark matter halos, and answer fundamental questions in our cosmological model. We also propose two projects that are theoretical and numerical in nature, both concerned with the molecules that make up the atmospheres of exoplanets and the birth clouds of stars. In addition, we present an outreach case, designed to enable us to disseminate to the public the specific outputs of the research to be funded by this grant.
Planned Impact
Our Group will continue to develop its current Knowledge Exchange and Outreach programmes, to increase even further the impact of our STFC-funded research activities.
Our general outreach strategy has the support of our Ogden Science Officer and the UCL Widening Participation and Public Engagement teams. We also benefit from access to a unique facility, the UCL Observatory in Mill Hill (UCLO). We specifically target:
* our local community: We have strong ties with schools in the London boroughs of Islington, Hackney and Barnet (where UCLO is located) and offer them multiple opportunities to engage through trips to UCLO, large scale festival events such as Your Universe and Dark Matter Day, and targeted classroom visits.
* the next generation of scientists: We directly involve secondary school pupils in our research through our ORBYTS programme. The measured positive outcomes of this programme include an increase in the desire of young people to pursue scientific research as a career, and publications of the outcomes in scientific journals.
* the national scene: Group members routinely speak at large scale events across the country (e.g. New Scientist Scientist Live, Cheltenham Festival), feature on TV/Radio programmes (e.g. The Sky at Night), and write popular magazine articles and books, allowing us to disseminate our research outputs to large, diverse audiences
Our knowledge exchange activities have the professional support of UCL Business (for IP support) and UCL Enterprise (for entrepreneurship training, mentorship and access to venture capital). The transfer of the results of our innovation is being achieved as follows:
* by working with business to train the next generation of data scientists: we take advantage of our Astrophysical research to connect with businesses in need of Big-data infrastructure, as part of our STFC-funded doctoral training centre.
* by taking opportunities to commercialise our work: a start-up company Blue Skies Space Ltd (BSSL) has been formed by members of our group. BSSL employs an innovative commercial approach to create new opportunities for cutting-edge science, by enabling cost-effective, quickly-delivered scientific instruments for users worldwide through a service-based model.
* by contributing to the testing and design of new hardware and software solutions: Since January 2020 and for 4.5 years, our group is host the National Hub for the ExCALIBUR Hardware and Enabling Software Programme. This is both to support Exascale software design activities and to develop and test core technologies that will be used to design systems to solve both simulation and data Exascale-sized problems.
Our general outreach strategy has the support of our Ogden Science Officer and the UCL Widening Participation and Public Engagement teams. We also benefit from access to a unique facility, the UCL Observatory in Mill Hill (UCLO). We specifically target:
* our local community: We have strong ties with schools in the London boroughs of Islington, Hackney and Barnet (where UCLO is located) and offer them multiple opportunities to engage through trips to UCLO, large scale festival events such as Your Universe and Dark Matter Day, and targeted classroom visits.
* the next generation of scientists: We directly involve secondary school pupils in our research through our ORBYTS programme. The measured positive outcomes of this programme include an increase in the desire of young people to pursue scientific research as a career, and publications of the outcomes in scientific journals.
* the national scene: Group members routinely speak at large scale events across the country (e.g. New Scientist Scientist Live, Cheltenham Festival), feature on TV/Radio programmes (e.g. The Sky at Night), and write popular magazine articles and books, allowing us to disseminate our research outputs to large, diverse audiences
Our knowledge exchange activities have the professional support of UCL Business (for IP support) and UCL Enterprise (for entrepreneurship training, mentorship and access to venture capital). The transfer of the results of our innovation is being achieved as follows:
* by working with business to train the next generation of data scientists: we take advantage of our Astrophysical research to connect with businesses in need of Big-data infrastructure, as part of our STFC-funded doctoral training centre.
* by taking opportunities to commercialise our work: a start-up company Blue Skies Space Ltd (BSSL) has been formed by members of our group. BSSL employs an innovative commercial approach to create new opportunities for cutting-edge science, by enabling cost-effective, quickly-delivered scientific instruments for users worldwide through a service-based model.
* by contributing to the testing and design of new hardware and software solutions: Since January 2020 and for 4.5 years, our group is host the National Hub for the ExCALIBUR Hardware and Enabling Software Programme. This is both to support Exascale software design activities and to develop and test core technologies that will be used to design systems to solve both simulation and data Exascale-sized problems.
Organisations
- UNIVERSITY COLLEGE LONDON (Lead Research Organisation)
- European Southern Observatory (ESO) (Collaboration)
- University of Orsay (Collaboration)
- University of Paris-Saclay (Collaboration)
- University College London (Collaboration)
- Japanese Aerospace Exploration Agency (Collaboration)
- KEK (Collaboration)
- CARDIFF UNIVERSITY (Collaboration)
- UK Space Agency (Collaboration)
Publications

Amon A
(2023)
Consistent lensing and clustering in a low- S 8 Universe with BOSS, DES Year 3, HSC Year 1, and KiDS-1000
in Monthly Notices of the Royal Astronomical Society


Bernard J
(2023)
Performance of the polarization leakage correction in the PILOT data
in Experimental Astronomy

Bhambra P
(2021)
Explaining deep learning of galaxy morphology with saliency mapping

Bhambra P
(2022)
Explaining deep learning of galaxy morphology with saliency mapping
in Monthly Notices of the Royal Astronomical Society

Burger P
(2023)
KiDS-1000 cosmology: Constraints from density split statistics
in Astronomy & Astrophysics

Burger, Pierre A.
(2023)
KiDS-1000 cosmology: Constraints from density split statistics

Cuceu A
(2023)
The Alcock-Paczynski effect from Lyman- a forest correlations: analysis validation with synthetic data
in Monthly Notices of the Royal Astronomical Society

Cuceu A
(2023)
Constraints on the Cosmic Expansion Rate at Redshift 2.3 from the Lyman-a Forest.
in Physical review letters
Description | BISOU - Balloon Experiment for Cosmic Microwave spectral distortion |
Organisation | University of Orsay |
Department | Space Astrophysics Institute |
Country | France |
Sector | Academic/University |
PI Contribution | We have and continue to contribute to overall optical architecture, Fourier modulation analysis and mission operations concept. |
Collaborator Contribution | The partners are the lead organization for this activity. |
Impact | A few scientific papers on the mission concept and an ongoing Phase A study from CNRS. |
Start Year | 2021 |
Description | Euclid |
Organisation | UK Space Agency |
Department | Euclid Consortium |
Country | France |
Sector | Charity/Non Profit |
PI Contribution | Predictive pipeline for science performance of Euclid Justification of photometric redshift requirements Simulation tool for validation of Euclid data products |
Collaborator Contribution | full access to Euclid data |
Impact | ESA Space Mission to be launched in 2021 |
Start Year | 2009 |
Description | KiDS |
Organisation | European Southern Observatory (ESO) |
Department | VST |
Country | Chile |
Sector | Academic/University |
PI Contribution | infrastructure contributions to data analysis |
Collaborator Contribution | full data access to value-added weak lensing quality data analysis |
Impact | early data publications: public data release; refereed publications; press release |
Start Year | 2013 |
Description | Litebird Experiment |
Organisation | Cardiff University |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | In this collaboration there are at present 80 institutes involved (see link to general paper below) I have added the lead institutes, my main activity partner in France and the other UK institutes. We are tasked to design and model the ground based tests for spectral and polarimetric performance of the High Frequency Telescope for Litebird (which will be conducted in France). This is achieved through modelling and simulation efforts of the instrument performance as designed. While the experiment was conceived and the designed started prior to this grant, we have joined this consortium officially with this activity, thus adding this at the forefront of collaboration lists as a direct outcome of the activity. |
Collaborator Contribution | Litebird is the next generation Cosmic Microwave Background space satellite experiment for the measurement of the B-mode (considered to be the smoking gun of inflation in the first expansion phases of the Universe). It is led by the Japanese Space Agency (JAXA) and involves a 3-continent consortium with Japan leading the overall project and building the Low Frequency Telescope, institutes in the US (led by Berkeley University) working on the detectors for both focal planes and a European Consortium providing the High Frequency Telescope. In the UK, the institutes currently involved are Cardiff University (leading the UK consortium), UCL and MSSL with a plan to expand the consortium as the experiment evolves. |
Impact | So far, five publications on the design of the experiment (at this early stage of the project) in an Astronomical Telescopes conference journal have been published. Since the last report, more papers have been added, but also a new grant from the UKSA (led by Cardiff University) in which we also participate is continuing the support of this activity with our contribution adding an optical modelling aspect to the design and calibration support. The project itself has also past two of the main phases in the lead country (Japan). |
Start Year | 2017 |
Description | Litebird Experiment |
Organisation | Japanese Aerospace Exploration Agency |
Country | Japan |
Sector | Public |
PI Contribution | In this collaboration there are at present 80 institutes involved (see link to general paper below) I have added the lead institutes, my main activity partner in France and the other UK institutes. We are tasked to design and model the ground based tests for spectral and polarimetric performance of the High Frequency Telescope for Litebird (which will be conducted in France). This is achieved through modelling and simulation efforts of the instrument performance as designed. While the experiment was conceived and the designed started prior to this grant, we have joined this consortium officially with this activity, thus adding this at the forefront of collaboration lists as a direct outcome of the activity. |
Collaborator Contribution | Litebird is the next generation Cosmic Microwave Background space satellite experiment for the measurement of the B-mode (considered to be the smoking gun of inflation in the first expansion phases of the Universe). It is led by the Japanese Space Agency (JAXA) and involves a 3-continent consortium with Japan leading the overall project and building the Low Frequency Telescope, institutes in the US (led by Berkeley University) working on the detectors for both focal planes and a European Consortium providing the High Frequency Telescope. In the UK, the institutes currently involved are Cardiff University (leading the UK consortium), UCL and MSSL with a plan to expand the consortium as the experiment evolves. |
Impact | So far, five publications on the design of the experiment (at this early stage of the project) in an Astronomical Telescopes conference journal have been published. Since the last report, more papers have been added, but also a new grant from the UKSA (led by Cardiff University) in which we also participate is continuing the support of this activity with our contribution adding an optical modelling aspect to the design and calibration support. The project itself has also past two of the main phases in the lead country (Japan). |
Start Year | 2017 |
Description | Litebird Experiment |
Organisation | KEK |
Country | Japan |
Sector | Academic/University |
PI Contribution | In this collaboration there are at present 80 institutes involved (see link to general paper below) I have added the lead institutes, my main activity partner in France and the other UK institutes. We are tasked to design and model the ground based tests for spectral and polarimetric performance of the High Frequency Telescope for Litebird (which will be conducted in France). This is achieved through modelling and simulation efforts of the instrument performance as designed. While the experiment was conceived and the designed started prior to this grant, we have joined this consortium officially with this activity, thus adding this at the forefront of collaboration lists as a direct outcome of the activity. |
Collaborator Contribution | Litebird is the next generation Cosmic Microwave Background space satellite experiment for the measurement of the B-mode (considered to be the smoking gun of inflation in the first expansion phases of the Universe). It is led by the Japanese Space Agency (JAXA) and involves a 3-continent consortium with Japan leading the overall project and building the Low Frequency Telescope, institutes in the US (led by Berkeley University) working on the detectors for both focal planes and a European Consortium providing the High Frequency Telescope. In the UK, the institutes currently involved are Cardiff University (leading the UK consortium), UCL and MSSL with a plan to expand the consortium as the experiment evolves. |
Impact | So far, five publications on the design of the experiment (at this early stage of the project) in an Astronomical Telescopes conference journal have been published. Since the last report, more papers have been added, but also a new grant from the UKSA (led by Cardiff University) in which we also participate is continuing the support of this activity with our contribution adding an optical modelling aspect to the design and calibration support. The project itself has also past two of the main phases in the lead country (Japan). |
Start Year | 2017 |
Description | Litebird Experiment |
Organisation | University College London |
Department | Department of Space and Climate Physics (MSSL) |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | In this collaboration there are at present 80 institutes involved (see link to general paper below) I have added the lead institutes, my main activity partner in France and the other UK institutes. We are tasked to design and model the ground based tests for spectral and polarimetric performance of the High Frequency Telescope for Litebird (which will be conducted in France). This is achieved through modelling and simulation efforts of the instrument performance as designed. While the experiment was conceived and the designed started prior to this grant, we have joined this consortium officially with this activity, thus adding this at the forefront of collaboration lists as a direct outcome of the activity. |
Collaborator Contribution | Litebird is the next generation Cosmic Microwave Background space satellite experiment for the measurement of the B-mode (considered to be the smoking gun of inflation in the first expansion phases of the Universe). It is led by the Japanese Space Agency (JAXA) and involves a 3-continent consortium with Japan leading the overall project and building the Low Frequency Telescope, institutes in the US (led by Berkeley University) working on the detectors for both focal planes and a European Consortium providing the High Frequency Telescope. In the UK, the institutes currently involved are Cardiff University (leading the UK consortium), UCL and MSSL with a plan to expand the consortium as the experiment evolves. |
Impact | So far, five publications on the design of the experiment (at this early stage of the project) in an Astronomical Telescopes conference journal have been published. Since the last report, more papers have been added, but also a new grant from the UKSA (led by Cardiff University) in which we also participate is continuing the support of this activity with our contribution adding an optical modelling aspect to the design and calibration support. The project itself has also past two of the main phases in the lead country (Japan). |
Start Year | 2017 |
Description | Litebird Experiment |
Organisation | University of Paris-Saclay |
Country | France |
Sector | Academic/University |
PI Contribution | In this collaboration there are at present 80 institutes involved (see link to general paper below) I have added the lead institutes, my main activity partner in France and the other UK institutes. We are tasked to design and model the ground based tests for spectral and polarimetric performance of the High Frequency Telescope for Litebird (which will be conducted in France). This is achieved through modelling and simulation efforts of the instrument performance as designed. While the experiment was conceived and the designed started prior to this grant, we have joined this consortium officially with this activity, thus adding this at the forefront of collaboration lists as a direct outcome of the activity. |
Collaborator Contribution | Litebird is the next generation Cosmic Microwave Background space satellite experiment for the measurement of the B-mode (considered to be the smoking gun of inflation in the first expansion phases of the Universe). It is led by the Japanese Space Agency (JAXA) and involves a 3-continent consortium with Japan leading the overall project and building the Low Frequency Telescope, institutes in the US (led by Berkeley University) working on the detectors for both focal planes and a European Consortium providing the High Frequency Telescope. In the UK, the institutes currently involved are Cardiff University (leading the UK consortium), UCL and MSSL with a plan to expand the consortium as the experiment evolves. |
Impact | So far, five publications on the design of the experiment (at this early stage of the project) in an Astronomical Telescopes conference journal have been published. Since the last report, more papers have been added, but also a new grant from the UKSA (led by Cardiff University) in which we also participate is continuing the support of this activity with our contribution adding an optical modelling aspect to the design and calibration support. The project itself has also past two of the main phases in the lead country (Japan). |
Start Year | 2017 |