Sandro Tacchella

Name:	Sandro Tacchella
Affiliation:	University of Cambridge, UK
E-mail:	(only provided to users who are logged into talks.cam)
Last login:	24 Feb 2026, 9:06 a.m.

Public lists managed by Sandro Tacchella

• Galaxies Discussion Group

Talks given by Sandro Tacchella

Obviously this only lists talks that are listed through talks.cam. Furthermore, this facility only works if the speaker's e-mail was specified in a talk. Most talks have not done this.

• Modeling H-alpha emission in galaxies: insights into star formation and time variability

Talks organised by Sandro Tacchella

This list is based on what was entered into the 'organiser' field in a talk. It may not mean that Sandro Tacchella actually organised the talk, they may have been responsible only for entering the talk into the talks.cam system.

• Dwarf Galaxies in the Local Universe
• Disentangling preventative & ejective AGN feedback on a population basis with simulations, observations & machine learning
• Title to be confirmed
• Feedback and the circumgalactic medium
• Shining a light on the origin of supermassive black holes with cosmological simulations
• Zooming in on the assembly of galaxies in the early Universe
• Mergers all the way down: simulating the origin of globular clusters in a galactic context
• Reproducibility In Astrophysical Simulations: The AGORA Initiative and a 14-Year Human Experiment (In Memory of Joel Primack)
• The search for a new population of strong gravitational lenses with JWST
• The LMC-SMC System: A New Laboratory for Galaxy Evolution, Dynamics and Dark Matter
• Beyond Hubble: Studying the Earliest Galaxies with the James Webb Space Telescope
• Unveiling the turbulent assembly of the first galaxies with JWST slitless spectroscopy
• SMBH growth and formation at z~1-10 revealed by space telescopes
• Merger-driven growth of galaxies at z~3–9 with JWST
• The Origin of Supermassive Black Holes from Pop III.1 Seeds and Implications for Particle Physics and Cosmology
• The Quasi-star Channel of Supermassive Black Hole Formation
• Chemical abundance patterns at high redshift: insights from deep spectroscopy and multi-component photoionisation models
• Can dwarf galaxies reionise the Universe?
• Ly-alpha emission in local dwarfs
• Cooling Flows and Feedback in Clusters and Groups
• Simulations of radio galaxy flickering jets: travelling shocks, hotspot brightening and stability
• Primeval galaxies and infant black holes at cosmic dawn
• The average far-infrared properties of Euclid-selected star-forming galaxies
• Dust in shocks: the missing link in AGN feedback
• Tracing the Evolution of the Mass–Metallicity and Fundamental Relations at z=2-10 with Direct Te-Based Metallicities
• A view of the cosmic web through the lens of HI galaxies
• Exploring the Cosmos with Hydrogen Observation
• Early Massive Galaxies and Scaled-Up LRDs: Clues from Euclid and JWST
• From Primordial Magnetic Fields to AGN-Driven Magnetized Outflows
• JWST Spectroscopic Insights Into the Evolution and Diversity of Galaxies within the First Billion Years
• Mapping the Cosmic Web in Lyα emission around quasars and non-AGN galaxies
• Disrupting the Baryon Cycle: Galaxy Evolution in Cluster Environments
• Learning galaxy properties with machine learning and simulation based inference
• Novel approaches to simulating the observable Universe
• Where You Live Matters: Host Galaxy Insights into Transient Progenitors
• Probing early star formation and ionized bubble growth with JWST
• The curious case of metal-poor DLAs at cosmic noon
• Mid-Infrared diversity in nearby AGN: New insights from JWST/MIRI
• The Reionization of our Local Universe
• Dust grains across the universe: JWST and ALMA insights from cosmic noon to the early universe
• Unveiling the shape of the ionizing spectrum of galaxies
• Nucleosynthesis at the isotopic level: how chemical abundances enhance our understanding of globular clusters and dwarf galaxies
• The Dynamics of Debris Disk Creation in Neutron Star Mergers
• Exploring the End of Reionization
• Chasing the Light: Shadowing, Collimation, and the Rapid Growth of Infant Black Holes
• Towards understanding the epoch of reionization out to the cosmic dawn
• How do the most luminous black holes accrete and expel gas?
• Exploring high-redshift quenched galaxies: from low-mass to massive
• The Thesan-Zoom simulations: Studying high-redshift galaxy formation with cosmological radiation-hydrodynamics simulations
• Unveiling AGN Outflows: A High Resolution Morphological Study with LOFAR-VLBI
• The first stars: window to cosmic dawn
• Modelling black hole accretion through an 𝛼-disc with a resolved interstellar medium in dwarf galaxies
• Unveiling the Intrinsic Mass Step of Type Ia Supernovae
• Baryonic feedback: How extreme is too extreme?
• Simulating supermassive black holes: from event horizon to cosmic web and back again
• A cosmic ballet of dwarf galaxies as challenge for cosmology
• Galactic Archaeology in the Gaia era: a surprising population of very metal-poor stars in the Milky Way disc
• The history of the Milky Way's bar
• Galaxy-halo connection in current CMB cross-correlation science
• Determining Galaxy Kinematics and ISM conditions with the JWST/NIRSpec IFU
• Reanalysis of KiDS-1000 cosmic shear using MetaCalibration
• Two-Dimensional Kinematics and Dynamical Modelling of SLACS Lenses: Insights from Deep MUSE Observations
• The Environments of Type Ia Supernovae
• How hypervelocity stars constrain the Galactic Centre
• Bridging the Gap with MAGPI: Exploring Star Formation Radial Trends in Galaxies through Simulations and Observations
• Search for AGN in the era of JWST
• Unveiling the Low Surface Brightness Universe: a CFHT and Euclid perspective
• Unveiling the ionising properties of galaxies at the Epoch of Reionisation with NIRCam
• Testing the Robustness of NANOGrav’s Gravitational Wave Background Signal
• Probing the Post to Early Stage of Cosmic Reionization using JWST and Subaru
• Connecting Star Formation, Feedback, and the ISM in Galaxy Disks
• Cosmic rays in star-forming galaxies
• Widespread rapid quenching at cosmic noon
• Revealing the physical drivers of galaxy kinematic structure with SAMI
• Seeking (and Finding!) the Photons for Reionization with JWST
• Why do galaxies cease forming stars? Evidence for AGN feedback driven quenching from cosmic dawn to the present epoch
• Type Ia supernova siblings and the Zwicky Transient Facility
• Challenges to galaxy formation models at the cosmic frontier
• Impact of primordial magnetic fields on matter power spectrum
• Modelling supermassive black holes: accretion, spin evolution, jets and winds
• Title to be confirmed
• Introducing Azahar: the blooming of non-thermal physics in galaxy formation
• Evolution of Galaxy Structure in the rest-NIR as revealed by JWST/NIRCam: What changes and what doesn't?
• A Look Into Galaxy Morphologies with Machine Learning
• The Extremes of Resolved Stellar Spectroscopy
• Early r-process enrichment in globular clusters
• Machine Learning enhanced Bayesian Workflows for Galaxies
• Halpha filaments in Massive Ellipticals: the roles played by Turbulence and type Ia Supernovae
• TBD
• The Via Project: Mapping the invisible Galactic halo
• Probing the epoch of galaxy assembly with MUSE
• Chemo-dynamical evolution of disks over cosmic time
• Effects of primordial black holes on early star formation
• Obscured AGN across cosmic time
• The chemical abundance pattern of a nitrogen-loud AGN in the early Universe
• Light from the Cosmic Dawn: origin and observational signatures of the first black holes
• The quest for the earliest black holes: a theoretical perspective
• Problems with (our) galaxy formation simulations and some new angles
• IoA/KICC Open Day
• From Little Things Big Things Grow: Tracing the Milky Way’s Assembly History
• Galactic Archaeology with Globular Clusters
• Warps, bending waves and corrugations in the Milky Way
• The extreme masses of the dark matter haloes hosting z > 6 quasars: two new pieces of evidence
• Challenging our understanding of high-redshift galaxy formation with JWST observations
• AGN in Clumpy DisCs (ACDC): How does ISM structure shape multiphase outflows?
• Blown away: relative velocities and the first galaxies
• The structure of the interstellar medium as probe of the baryonic physics of galaxy evolution
• Towards homogeneous studies of high-z protoclusters
• Observations of kinetic feedback in radio-loud Active Galactic Nuclei (AGN) hosts
• LINCC Frameworks - developing software for large-scale analysis of data
• Constraints on DM and the cusp/core problem with MUSE
• Reionizing the Universe: A Brief History of Baryons and the Cosmic Web
• Super-massive black holes across cosmic time
• Not so Slow: Do Galactic Bars Slow Down?
• What we think we know about reionization
• Kinematics of galaxy bulges, disks, and ionised gas from 3D spectroscopy
• Probing the early Universe with the oldest stars in the Milky Way
• Mapping the Circumgalactic Medium and Intergalactic Medium through Lya and MgII Emission
• Galaxy kinematics within the cosmic web
• Unveiling the Interstellar Medium in High-Redshift Galaxies
• Internal kinematics of Gaia DR3 wide binaries
• The effect of cosmic rays in the evolution of a Milky Way-like galaxy and its circum-galactic medium
• Mapping dark and luminous matter with cosmological simulations
• The Lyman-alpha cosmic web in IllustrisTNG
• Science with Very Large Cosmological Simulations
• A new theory of the universe
• TBC
• AGN revisited: from dwarf galaxies to new black hole accretion models
• Using galaxies to study supernovae and supernovae to study galaxies
• JWST view of star formation in local galaxies
• TBD
• The Nature of Dark Matter from high-redshift Cosmic Web
• Current constraints on escape fractions
• Exploring early galaxy evolution in the JWST-era with novel statistical and machine learning techniques
• Pandora: exploring galaxy formation with radiation, magnetic fields and cosmic rays
• An updated view on the properties of the first galaxies from the first JWST observations
• Constraining Cosmic Baryons and Dark Matter with the Lyman-alpha Forest
• The Fornax3D survey with MUSE - final results and future spin-off directions
• A resolved view of z>6 quasar host galaxies
• TBC
• Uncovering Extremely Metal-Poor Galaxies in the Era of JWST Studies
• Decoding the Origin of the Elements