Cosmology 2023 in Miramare

Session

Opening and Plenary Session - Chair Fabrizio Nesti

28 Aug 2023, 09:20

Main Auditorium (SISSA Building, Miramare, Trieste, Italy)

10. Lambda CDM cosmology model: current status, future prospects

Uros Seljak

28/08/2023, 09:30

TBA

11. Euclid mission: status and scientific goals

Alfonso Veropalumbo

28/08/2023, 10:00

Euclid is an ESA space mission that aims to investigate the dark Universe. Over the six years of nominal survey operations, Euclid will observe billions of galaxies, probing the Universe's large-scale structure out to 10 billion light-years, covering a third of the celestial sphere. Employing Weak Gravitational Lensing and Galaxy Clustering probes, Euclid aims to detect the signatures of dark...

12. Mining the Universe

Nicoletta Krachmalnikoff

28/08/2023, 10:30

In the upcoming decade, scientists will face significant new challenges in the field of Cosmology: experiments will observe our Universe collecting an unprecedented amount of data, which must be analyzed with an extraordinary level of precision in order to interpret them and efficiently extract valuable information for data-driven discoveries . Cosmology therefore represents the perfect...

13. The Search for Inflationary B-modes: Latest Results from BICEP/Keck

Clement Pryke (University of Minnesota)

28/08/2023, 11:30

The BICEP/Keck experiments are compact refracting telescopes mapping the polarization of the Cosmic Microwave Background (CMB) from the South Pole in Antarctica. The primary goal is to detect or set limits on primordial gravitational waves by observing B-modes of the polarization pattern. Recently the BK18 results have been released which include all data taken up to and including the 2018...

14. The Simons Observatory: next-generation CMB telescopes and science goals

Serena Giardiello

28/08/2023, 12:00

The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in 2024. SO will measure the temperature and polarization anisotropy of the cosmic microwave background in six frequency bands, from 27 to 280 GHz. The initial configuration of SO will have three small-aperture 0.5-m telescopes (SATs) and one large-aperture...

15. Extragalactic Background Light, Hubble constant and Intergalactic Magnetic Fields with Imaging Atmospheric Cherenkov Telescopes: status and perspectives

Daniel Mazin

28/08/2023, 12:30

Imaging Atmospheric Cherenkov Telescopes measure cosmic gamma radiation at very-high-energies (VHE) between 20 GeV and about 100 TeV. While most of the observations are devoted to study astrophysical processes in the sources of the gamma-ray emission (Supernova remnants, pulsar wind nebulae, gamma-ray binaries, active galactic nuclei, gamma ray bursts etc), distant gamma rays can also be used...