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.

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.

Publications

10 25 50

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

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

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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

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Gerardi F (2023) Direct cosmological inference from three-dimensional correlations of the Lyman a forest in Monthly Notices of the Royal Astronomical Society

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Hasebe T (2022) Sensitivity Modeling for LiteBIRD in Journal of Low Temperature Physics

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Hubmayr J (2022) Optical Characterization of OMT-Coupled TES Bolometers for LiteBIRD in Journal of Low Temperature Physics

 
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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
Start Year 2017