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Black Hole

Lensing of space time around a black hole. At Oxford 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
arxiv.org/a/bartlett_d_1
orcid.org/0000-0001-9426-7723
www.aquila-consortium.org
  • About
  • Publications

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

(2023)

Authors:

Anya Paopiamsap, David Alonso, Deaglan J Bartlett, Maciej Bilicki
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Details from ArXiV

Modeling and Testing Screening Mechanisms in the Laboratory and in Space

Universe MDPI 9:7 (2023) 340

Authors:

Valeri Vardanyan, Deaglan J Bartlett
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Priors for symbolic regression

Association for Computing Machinery (ACM) (2023) 2402-2411

Authors:

Deaglan Bartlett, Harry Desmond, Pedro Ferreira
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Modeling and testing screening mechanisms in the laboratory and in space

ArXiv 2305.18899 (2023)

Authors:

Valeri Vardanyan, Deaglan J Bartlett
Details from ArXiV

Exhaustive symbolic regression

IEEE Transactions on Evolutionary Computation IEEE (2023)

Authors:

Deaglan Bartlett, Harry Desmond, Pedro Ferreira

Abstract:

Symbolic Regression (SR) algorithms attempt to learn analytic expressions which fit data accurately and in a highly interpretable manner. Conventional SR suffers from two fundamental issues which we address here. First, these methods search the space stochastically (typically using genetic programming) and hence do not necessarily find the best function. Second, the criteria used to select the equation optimally balancing accuracy with simplicity have been variable and subjective. To address these issues we introduce Exhaustive Symbolic Regression (ESR), which systematically and efficiently considers all possible equations—made with a given basis set of operators and up to a specified maximum complexity— and is therefore guaranteed to find the true optimum (if parameters are perfectly optimised) and a complete function ranking subject to these constraints. We implement the minimum description length principle as a rigorous method for combining these preferences into a single objective. To illustrate the power of ESR we apply it to a catalogue of cosmic chronometers and the Pantheon+ sample of supernovae to learn the Hubble rate as a function of redshift, finding 40 functions (out of 5.2 million trial functions) that fit the data more economically than the Friedmann equation. These low-redshift data therefore do not uniquely prefer the expansion history of the standard model of cosmology. We make our code and full equation sets publicly available.
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