Lecture
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10 Jan 2024 (2h 00m)
Simona Gallerani - Course (teaching activity) - Both face to face and online
Prima lezione: Pillars of the Standard Cosmological model; Expansion of the Universe (Cepheids, SN Ia, quasars)
17 Jan 2024 (2h 00m)
Simona Gallerani - Course (teaching activity) - Both face to face and online
Seconda lezione: The Cosmic Microwave background (origin and statistics); Polarization constrains on Cosmic Reionization
24 Jan 2024 (2h 00m)
Simona Gallerani - Course (teaching activity) - Both face to face and online
Terza lezione: Big Bang Nucleosynthesis
31 Jan 2024 (2h 00m)
Simona Gallerani - Course (teaching activity) - Both face to face and online
Quarta lezione: Absorption spectra as tools for studying the intergalactic medium; The Gunn and Peterson test
07 Feb 2024 (2h 00m)
Simona Gallerani - Course (teaching activity) - Both face to face and online
Quinta lezione: Absorption spectra as tools for studying the cosmic reionization process; redshift evolution of the GP optical depth
14 Feb 2024 (2h 00m)
Simona Gallerani - Course (teaching activity) - Face to face
Sesta lezione: Absorption spectra as tools for studying the cosmic reionization process; proximity effect and damping wings
21 Feb 2024 (2h 00m)
Simona Gallerani - Course (teaching activity) - Face to face
Settima lezione: The Lyman Break technique; constraints on the reionization from the UV luminosity function.
28 Feb 2024 (2h 00m)
Simona Gallerani - Course (teaching activity) - Face to face
Ottava lezione: Lyman alpha emitting galaxies; far infrared emission lines from galaxies in the EOR
06 Mar 2024 (2h 00m)
Simona Gallerani - Course (teaching activity) - Face to face
Nona lezione: Detection and identification of high-z quasars; BH mass measurements (Reverberation mapping technique); properties of the ISM in the host galaxies (FIR emission lines)
07 Mar 2024 (2h 00m)
Stefano Carniani - Course (teaching activity) - Face to face
Introduzione all'astrofisica extragalattica, componenti principali di una galassia, equilibrio idrostatico, dinamica del gas, stelle, e materia oscura
13 Mar 2024 (2h 00m)
Simona Gallerani - Course (teaching activity) - Both face to face and online
Decima Lezione: Seeding models; contribution of AGN to reionization; constraints from the HeII Lya forest
14 Mar 2024 (2h 00m)
Stefano Carniani - Course (teaching activity) - Face to face
Gas and stellar dynamics; collisionless systems; application of Boltzmann and Jeans equations in astrophysics
20 Mar 2024 (2h 00m)
Stefano Carniani - Course (teaching activity) - Both face to face and online
Galaxy formation; shock heating; cooling processes.
21 Mar 2024 (2h 00m)
Stefano Carniani - Course (teaching activity) - Both face to face and online
Galaxy formation: heating processes; overcooling problem; stellar-to-halo mass ratio; introduction to interstellar medium and molecular cloud
27 Mar 2024 (2h 00m)
Stefano Carniani - Course (teaching activity) - Both face to face and online
properties of giant molecular clouds, isothermal sphere, instabilities, Toomre Q parameter, parameter star formation processes, star formation law
28 Mar 2024 (2h 00m)
Stefano Carniani - Course (teaching activity) - Both face to face and online
initial mass function; spectroscopic properties of stars; stellar populations in galaxies; definition of star-formation rate; bi-modality distribution in the SFR-Mstar diagram
03 Apr 2024 (2h 00m)
Stefano Carniani - Course (teaching activity) - Both face to face and online
Inter-stellar medium properties; HII regions; neutral and molecular gas; dust properties
11 Apr 2024 (2h 00m)
Stefano Carniani - Course (teaching activity) - Online
Super-massive black holes; active galactic nuclei; BPT digram, spectroscopic properties of AGN; reverberation mapping; unified model
18 Apr 2024 (2h 00m)
Stefano Carniani - Course (teaching activity) - Both face to face and online
Accretion disk; thin disk model; emission; accretion disk size
24 Apr 2024 (2h 00m)
Stefano Carniani - Course (teaching activity) - Face to face
Galaxy-SMBH co-evolution; AGN feedback; Eddington limit; radiation pressure; properties of galactic scale outflows
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