Bayesian optimisation for likelihood-free cosmological inference
Leclercq
The phase-space structure of nearby dark matter as constrained by the SDSS
Leclercq, Jasche, Lavaux, Wandelt, Percival
Comparing cosmic web classifiers using information theory
Leclercq, Lavaux, Jasche, Wandelt
Cosmic web-type classification using decision theory
Leclercq, Jasche, Wandelt
Bayesian analysis of the dynamic cosmic web in the SDSS galaxy survey
Leclercq, Jasche, Wandelt
Dark matter voids in the SDSS galaxy survey
Leclercq, Jasche, Sutter, Hamaus, Wandelt
Past and present cosmic structure in the SDSS DR7 main sample
Jasche, Leclercq, Wandelt
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Bayesian large-scale structure inference and cosmic web analysis
Inférence bayésienne et analyse des grandes structures de l'Univers
My PhDWelcome!
My name is Florent Leclercq. I am a Research Fellow at the Imperial Centre for Inference and Cosmology. I work in the fields of theoretical and observational cosmology, focusing in particular on the analysis of galaxy survey data.
My current research interests are related to the study of the cosmological large-scale structure using statistical data analysis tools. I am particularly interested in the initial conditions from which the large-scale structure originates, its formation history and the description of the cosmic web.
Please check the full version of my CV, my list of publications and my list of communications.
News
- 14-11-2017
New page: media and outreach, and update of research pages. - 27-10-2016
Update of the BORG SDSS data, here and on GitHub.
The BORG SDSS data release
This website hosts the BORG SDSS data release, a set of data products that follow a chrono-cosmographic analysis of the three-dimensional large-scale structure of the nearby Universe.
Public data and software
Charting the unseen sky
November 2017Cosmologists from the U.K., France and Germany have come up with new maps of how dark matter moves throughout the universe.
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A light in the dark
September 2017Dr Florent Leclercq of the University of Portsmouth, UK, discusses the creation of new maps of dark matter dynamics in the Universe.
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