DiRAC-3 Operations 2023-26 - UCL - Additional Grant
Lead Research Organisation:
UNIVERSITY COLLEGE LONDON
Department Name: Physics and Astronomy
Abstract
This JeS form is a resubmission of part of the UCL DiRAC Operations grant request containing only the DI posts which have been approved for funding at 100% by STFC.
Organisations
People |
ORCID iD |
| Clare Jenner (Principal Investigator) |
Publications
Armijo J
(2024)
A new test of gravity - I. Introduction to the method
in Monthly Notices of the Royal Astronomical Society
Dhandha J
(2025)
Narrowing the discovery space of the cosmological 21-cm signal using multi-wavelength constraints
in Monthly Notices of the Royal Astronomical Society
Mak M
(2025)
The impact of different haze types on the atmospheres and observations of hot Jupiters: 3D simulations of HD 189733b, HD 209458b, and WASP-39b
in Monthly Notices of the Royal Astronomical Society
Yurchenko S
(2024)
ExoMol line lists - LIV. Empirical line lists for AlH and AlD and experimental emission spectroscopy of AlD in A1? ( v = 0, 1, 2)
in Monthly Notices of the Royal Astronomical Society
He Q
(2023)
Testing strong lensing subhalo detection with a cosmological simulation
in Monthly Notices of the Royal Astronomical Society
Ji X
(2025)
BlackTHUNDER - A non-stellar Balmer break in a black hole-dominated little red dot at z = 7.04
in Monthly Notices of the Royal Astronomical Society
CamposĀ Estrada B
(2024)
On the likely magnesium-iron silicate dusty tails of catastrophically evaporating rocky planets
in Monthly Notices of the Royal Astronomical Society
Sanati M
(2025)
The emergence and ionizing feedback of Pop III.1 stars as progenitors for supermassive black holes
in Monthly Notices of the Royal Astronomical Society
Lange S
(2025)
Galaxy mass modelling from multiwavelength JWST strong lens analysis: dark matter substructure, angular mass complexity, or both?
in Monthly Notices of the Royal Astronomical Society
Roth A
(2024)
Hot Jupiter diversity and the onset of TiO/VO revealed by a large grid of non-grey global circulation models
in Monthly Notices of the Royal Astronomical Society