Observational Cosmology Using Large Imaging Surveys

OCULIS aims to enhance the understanding of dark matter and energy by leveraging Euclid satellite data to accurately measure galaxy properties and their relation to cosmic structure formation.

Subsidie
€ 2.457.977
2023

Projectdetails

Introduction

The current standard model of cosmology successfully describes a variety of measurements, but its main ingredients, dark matter and dark energy, are a great mystery. ESA’s Euclid satellite is the biggest step forward towards solving this fundamental problem in physics.

Objectives of Euclid

It is designed to reveal the nature of the dark constituents and gravity by measuring the growth of structure over most of cosmic time with unprecedented precision. However, the interpretation of the data is complex:

  • Incorrect modelling of the galaxy populations
  • Astrophysical processes
  • Instrumental effects

These factors can easily be mistaken as evidence for new physics. To fully exploit the statistical power of Euclid, the intricacies of the data need to be understood. Additionally, we need an accurate model of structure formation that can describe the interplay between galaxy formation, astrophysics, dark matter, and cosmology.

Approach of OCULIS

OCULIS tackles both aspects by providing the best measurements of the lensing signal and using the Euclid data in novel ways to relate observed galaxy properties directly to the matter distribution. To do so, we will:

  1. Use in-flight data to correct for instrumental biases.
  2. Measure the intrinsic alignments of galaxies that contaminate the lensing signal.
  3. Exploit Euclid’s unique ability to determine the lensing signal on small scales to directly determine the stellar masses of galaxies for the first time and to study the tidal stripping of dark matter halos.
  4. Use the results to inform models that describe the small-scale astrophysics in hydrodynamic simulations, yielding robust predictions of the cosmological signals.

Unique Position of the PI

As the cosmology coordinator of the Euclid mission, the PI is uniquely positioned to achieve these objectives. The synergetic approach of OCULIS exploits that Euclid is much more than a cosmology mission; it is also a prime dataset for the study of the formation and evolution of galaxies.

Maximizing Scientific Return

By linking both science cases, OCULIS maximizes the scientific return of Euclid.

Financiële details & Tijdlijn

Financiële details

Subsidiebedrag€ 2.457.977
Totale projectbegroting€ 2.457.977

Tijdlijn

Startdatum1-9-2023
Einddatum31-8-2028
Subsidiejaar2023

Partners & Locaties

Projectpartners

  • UNIVERSITEIT LEIDENpenvoerder

Land(en)

Netherlands

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