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are invited for a UKRI funded postdoctoral position at the Institute of Astronomy, University of Cambridge, to work within the research group of Prof. Nikku Madhusudhan. The group has extensive expertise and
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postdoctoral researchers, early-career academics, and established professors. Project aims and objectives Aim: The project aims to design context-aware multimodal learning frameworks to effectively understand
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University of Sussex; | The City of Brighton and Hove, England | United Kingdom | about 21 hours ago
. Taking a case study approach oriented around UK copyright libraries between 1836 and 1914, the project asks questions including: which textual forms and genres do deposit libraries reject? How and why does
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use ultrafast spectroscopic techniques, including gas-phase methods such as tandem ion mobility mass spectrometry and time-resolved photoelectron spectroscopy, together with solution-phase transient
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understanding of the underlying mechanisms, (2) optimise the process with online monitoring to ensure high consistency of quality, (3) use the knowledge gained to understand the opportunities and limitations
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participation in the only set of telescopes currently able to identify new habitable rocky planets whose atmosphere can then be probed for evidence of biological processes. We use the SPECULOOS network
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are possible related to the detection or mass characterisation of small planets, star-planet connections, stellar variability mitigation techniques, or Sun-as-a-star studies. The project will make use of data
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its first two years of science operations. However, new modelling efforts are needed to fully interpret these datasets. In this PhD project, the researcher will use atmospheric modelling techniques
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-physics-and-astronomy/astronomy-and-experimental-gravity/sun-stars-and-exoplanets . Our group has 5 permanent academics, 12 postdoctoral researchers, and 10 PhD students and is gender-balanced. In 2024, a
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predictive checking, model comparison) • Computational modelling with Python and Dynesty, JAX, NumPyro, and PyTorch • Use of asteroseismic and spectroscopic survey data (e.g. PLATO, Gaia, APOGEE, TESS) • High