H2020Индивидуална стипендия2018–2020

HALOS2020 · Accurate halo masses in the precision cosmology era

„Хоризонт 2020“ — Действия „Мария Склодовска-Кюри“

Период: 2018-09-01 → 2020-08-31
Финансиране от ЕС: 165 599 €
Участници: 1
Схема: MSCA-IF-EF-ST

Линиите свързват координатора с партньорите.

Накратко на български

Разпределението на тъмната материя в масивните галактики се анализира чрез гравитационни лещи и компютърни симулации. Това помага да се разберат свойствата на тъмната материя, която съставлява 90% от масата на Вселената, но все още не е открита в лаборатория.

Този кратък обзор е генериран от изкуствен интелект

Кратко обяснение, генерирано от езиков модел по текста на CORDIS. Оригиналът е по-долу.

Резултати накратко

Accurate halo masses in the precision cosmology era

The overall goal is to develop techniques for obtaining accurate measurements of the distribution of dark matter in galaxies and apply these to observational data. Dark matter constitutes 90% of the mass of the Universe, but so far has never been detected by a laboratory experiment. Consequently, our understanding of the properties of dark matter, such as its ability to interact with ordinary matter, is very limited. One of the ways to gain knowledge on dark matter is by measuring its distribution in galaxies. This project is aimed at obtaining improved measurements of the distribution of dark matter in massive galaxies and comparing these measurements with predictions from numerical simulations. The main tool used for these measurements are strong gravitational lensing and weak gravitational lensing.

Текст от CORDIS, на английски · Данни: CORDIS, © Европейски съюз

Цел на проекта

Weak gravitational lensing is a very powerful tool for investigating the relation between galaxies and their host dark matter halos.Thanks to current photometric surveys such as KiDS, DES and HSC, the quality of the data available for weak lensing studies is rapidly improving.However, there has not yet been a corresponding improvement in the methods used for the analysis of this data: most weak lensing studies are still carried out by stacking the signal in bins, resulting in a net loss of information.As an alternative to stacking, I have recently developed a new method to infer the distribution of halo masses of a population of galaxies with weak lensing data. The method, based on a Bayesian hierarchical inference formalism, allows for an easy exploration of correlations in many dimensions, and to directly constrain the intrinsic scatter in halo mass.In this project, I will use my method to look for correlations between halo mass and secondary galaxy properties at fixed stellar mass, such as the age of the stellar population, in KiDS data.I will first test the robustness of my method on hydrodynamical simulations.Then, after receiving a training on the most technical aspects of KiDS weak lensing measurements, I will apply it on real data.Finally, I will compare the results of my analysis with predictions from theoretical models. By detecting or ruling out correlations between halo mass and galaxy properties, I will be able to put powerful constraints on galaxy evolution models.This project will produce an immediate return in terms of science, and will pave the way for the use of more efficient analysis methods in future surveys such as Euclid.

Оригинален текст от CORDIS (на английски).

Участници

UNIVERSITEIT LEIDEN · LeidenКоординаторНидерландия