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91探花
Black Hole

Lensing of space time around a black hole. At 91探花 we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Dr Deaglan Bartlett

Eric and Wendy Schmidt AI in Science Postdoctoral Fellow

Research theme

  • Astronomy and astrophysics
  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
  • Cosmology
  • Galaxy formation and evolution
deaglan.bartlett@physics.ox.ac.uk
Denys Wilkinson Building, room 532G
  • About
  • Publications

Marginalised Normal Regression: Unbiased curve fitting in the presence of x-errors

The Open Journal of Astrophysics Maynooth University 6 (2023)

Authors:

Deaglan J Bartlett, Harry Desmond

Optimal Inflationary Potentials

(2023)

Authors:

Tom谩s Sousa, Deaglan J Bartlett, Harry Desmond, Pedro G Ferreira

Marginalised Normal Regression: Unbiased curve fitting in the presence of x-errors

ArXiv 2309.00948 (2023)

Authors:

Deaglan Bartlett, Harry Desmond

Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations

(2023)

Authors:

Anya Paopiamsap, David Alonso, Deaglan J Bartlett, Maciej Bilicki

Priors for symbolic regression

GECCO '23 Companion: Proceedings of the Companion Conference on Genetic and Evolutionary Computation Association for Computing Machinery (2023) 2402-2411

Authors:

Deaglan Bartlett, Harry Desmond, Pedro Ferreira

Abstract:

When choosing between competing symbolic models for a data set, a human will naturally prefer the 鈥渟impler鈥 expression or the one which more closely resembles equations previously seen in a similar context. This suggests a non-uniform prior on functions, which is, however, rarely considered within a symbolic regression (SR) framework. In this paper we develop methods to incorporate detailed prior information on both functions and their parameters into SR. Our prior on the structure of a function is based on a ngram language model, which is sensitive to the arrangement of operators relative to one another in addition to the frequency of occurrence of each operator. We also develop a formalism based on the Fractional Bayes Factor to treat numerical parameter priors in such a way that models may be fairly compared though the Bayesian evidence, and explicitly compare Bayesian, Minimum Description Length and heuristic methods for model selection. We demonstrate the performance of our priors relative to literature standards on benchmarks and a real-world dataset from the field of cosmology.

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