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Institute of Astronomy

 
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This is a List of Talks Lists that is a List of all IoA Seminars, Colloquia, Extra talks, IoA Stellar Pops and Extragalactic Gathering, etc. It is used as a feed for the IOA website and Digital Display screens. Individual Talks should NOT be added to this Talk lists. They should be added to one of the series that feed this list.
Updated: 1 hour 35 min ago

Fri 30 Jan 11:30: Title to be confirmed

Wed, 17/09/2025 - 16:41
Title to be confirmed

Abstract not available

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Fri 21 Nov 11:30: Early Massive Galaxies and Scaled-Up LRDs: Clues from Euclid and JWST

Tue, 16/09/2025 - 12:43
Early Massive Galaxies and Scaled-Up LRDs: Clues from Euclid and JWST

The formation of massive galaxies in the first billion years of cosmic time is one of the most remarkable findings of Extragalactic Astronomy and challenges the predictions of galaxy formation models. Finding the right candidates is the first step towards understanding how such efficient galaxy formation could have happened at early cosmic time. Another, a priori completely different, high-z galaxy population whose formation is also very puzzling are the so-called ‘Little Red Dots (LRDs)’. Discovered almost by chance in JWST galaxy surveys, most of these objects appear to host overgrown super-massive black holes. An intriguing issue is how bright and extreme these objects could be. In the first part of this talk, I will present the results of our search of massive galaxy candidates at the end of the Epoch of Reionization using the first set of Euclid images over several tens of square degrees of the sky. I will also discuss the presence of massive galaxies in JWST surveys at similar redshifts and the coherence of all results in a common context. In the second part of my talk, I will present our results on the study of Euclid sources with double-power-law spectral energy distributions at z>4 in the COSMOS field, where the Euclid data has already a depth very similar to the final expected depth of the Euclid Deep Surveys. I will discuss the presence of scaled-up LRD candidates, identified based on their compactness, and their derived properties in comparison to those of classical JWST -selected LRDs. Finally, I will conclude by discussing whether LRDs could also eventually give rise to massive galaxy formation.

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Fri 12 Dec 11:30: Title to be confirmed

Wed, 10/09/2025 - 14:45
Title to be confirmed

Abstract not available

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Fri 14 Nov 11:30: From Primordial Magnetic Fields to AGN-Driven Magnetized Outflows

Wed, 10/09/2025 - 08:11
From Primordial Magnetic Fields to AGN-Driven Magnetized Outflows

Magnetic fields are ubiquitous across cosmic scales, yet their role in galaxy formation remains elusive. In this talk, I show that primordial magnetic fields, originating before the end of recombination, can amplify small perturbations, accelerating the collapse of the first dark matter halos. This results in an early onset and efficient star formation, consistent with JWST observations. However, primordial fields are not the only source of magnetization at high redshifts. Using RAMSES -RTMHD cosmological simulations, I compare the role of primordial fields and AGN -driven outflows in shaping the magnetic landscape of the high-redshift universe.

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Fri 31 Oct 11:30: Title to be confirmed

Tue, 09/09/2025 - 14:01
Title to be confirmed

Abstract not available

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Mon 08 Dec 16:00: Title to be confirmed

Mon, 08/09/2025 - 21:54
Title to be confirmed

Abstract not available

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Fri 26 Sep 11:30: The curious case of metal-poor DLAs at cosmic noon

Mon, 01/09/2025 - 21:26
The curious case of metal-poor DLAs at cosmic noon

Abstract not available

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Fri 14 Nov 11:30: Physics of Ultra-Faint Dwarfs

Thu, 28/08/2025 - 09:05
Physics of Ultra-Faint Dwarfs

Abstract not available

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Fri 28 Nov 11:30: Dwarf Galaxies in the Local Universe

Thu, 28/08/2025 - 09:03
Dwarf Galaxies in the Local Universe

Abstract not available

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Fri 28 Nov 11:30: Local satellite galaxies

Wed, 27/08/2025 - 12:38
Local satellite galaxies

Abstract not available

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Tue 23 Sep 13:00: Planetary Evolution Across Stellar Lifetimes

Mon, 25/08/2025 - 10:48
Planetary Evolution Across Stellar Lifetimes

Over the past thirty years, nearly 6,000 planets have been confirmed. These systems provide key insights into how planet populations evolve over time, sculpted by planetary dynamics and stellar processes. Such mechanisms can drive dramatic changes on the planet and, in extreme cases, lead to its destruction. However, there are many gaps in our understanding of the evolution of planetary systems. In particular, the ultimate fate of these systems as their host stars evolve off the main sequence remains largely unknown. In this talk, I will present my work probing the mechanisms that shape planets over their lifetime. First, I will examine the impact of migration and photoevaporation on main-sequence systems. The recently confirmed planet, TOI -5800 b, provides a unique case study of an eccentric sub-Neptune on a close-in orbit, and may provide insight into how evolutionary processes contribute to population-level features such as the Neptunian desert. Second, I will describe how stellar evolution transforms planetary systems. In addition to destroying inner planets and dramatically altering the dynamics of outer planets, this process may also fundamentally alter the atmospheric composition of giant planets through a phase called common envelope evolution. Finally, I will discuss the ultimate fate of planet populations as their host stars evolve to their final state as white dwarfs. Even in these mature systems, planets can be destroyed through scattering into their host’s Roche radius, leaving an observational signature called “pollution.” I will also highlight ongoing efforts to probe the surviving planet population around white dwarf stars with JWST .

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