Hannah Uebler

Name:	Hannah Uebler
Affiliation:	Cavendish
E-mail:	(only provided to users who are logged into talks.cam)
Last login:	11 Jul 2024, 9:57 a.m.

Public lists managed by Hannah Uebler

• Institute of Astronomy Seminars

Talks given by Hannah Uebler

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.

• TBC

Talks organised by Hannah Uebler

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

• Modelling the impact of host galaxy dust on type Ia supernova distance measurements
• Low luminosity AGN across cosmic time - a preliminary census
• Diving chaotic orbits in axisymmetric potentials
• New frontiers in strongly lensed supernova studies with JWST and the Vera C. Rubin Observatory
• Type Ia supernovae: Constraining thermonuclear explosion physics with machine learning
• The cometary delivery of prebiotic feedstock molecules to the early-Earth and rocky exoplanets
• Constraining physics and astrophysics with multifrequency CMB data
• A new convection scheme for exoplanet atmospheres
• Stellar Mass Assembly of Galaxy Populations up to z = 4 with pop-cosmos
• Gaussian Processes for Systematic Mitigation for Global 21-cm Cosmology Experiments
• EDI Seminar: Dignity at Work Policy and Code of Behaviour
• Supermassive black hole binaries and their spin evolution in gas-rich circumbinary discs
• Photometric redshifts for high-z quasars in the era of LSST
• EDI Matters at the IoA
• GausSN: Bayesian Time Delay Estimation for Strongly Lensed Supernovae
• New Detector Technology for Astronomy
• Features of Gaia DR3 Spectroscopic Binaries: Tidal circularization of main-sequence stars
• Post-main sequence thermal evolution of planetesimals: Implications on white dwarf pollutants
• Evolution of the Stellar Initial Mass Function over the Past 10 Gyr
• The Complexity of Extinction at High-Galactic Latitudes
• Inside-out growth in the early Universe: a core in a vigorously star-forming disc
• Peculiar velocity surveys for cosmology: recent results and future plans
• Exploding Wolf-Rayet Stars
• Cosmos and Canvas: Using Data Visualization to Explore and Communicate Your Science
• The ultradense, interacting environment of a dual AGN at z ∼ 3.3 revealed by JWST/NIRSpec IFS
• Orbital Torus Imaging: Using elemental abundances to map orbital structure and mass in the Galactic disc
• Deciphering the Enigma of the Cosmic Ray Anisotropy
• Flat-sky angular power spectrum revisited
• The Advanced X-ray Imaging Satellite : High-resolution X-ray astronomy in the 2030s
• Probing reionization with radiative transfer simulations
• Carbonaceous dust grains within galaxies seen in the first billion years of cosmic time
• 3D models for the multiphase wind of M82
• JWST reveals galaxy mergers driving Lyman-alpha emission at z >7
• Murdin Prize Ceremony -- Constraining Beyond the Standard Model Physics with X-ray telescopes: Tightest constraints on low-mass Axion Like Particles with Chandra observations of H1821+643
• Murdin Prize Ceremony -- Proposed energy-metabolisms cannot explain the atmospheric chemistry of Venus
• Murdin Prize Ceremony -- Inward and outward migration of massive planets: moving towards a stalling radius
• Uncovering the ancient central Milky Way with the Pristine Inner Galaxy Survey (PIGS)
• The impact of a massive Sagittarius dSph on GD-1-like stellar streams
• Quantifying the tumor vasculature environment using deep learning
• The Nature of the Star Forming Main Sequence
• A new method for age-dating the formation of bars in disc galaxies
• Dynamics of dust and gas in protoplanetary disks with massive embedded planets
• Putting brakes on star formation in central galaxies
• Stellar Fireworks: A journey through the spirally dust plumes of Wolf-Rayet binaries
• Preparing for JWST with HST/COS spectroscopy of Pox 186: a local analogue of z > 6 galaxies
• Robustness of Molecular Detections Using High-Resolution Transmission Spectroscopy
• The Awakening Beast in the Seyfert 1 Galaxy KUG 1141+371
• The High-z Cosmic Web in Fuzzy Dark Matter Cosmologies
• Orbital alignment and mass segregation in galactic nuclei via Vector Resonant Relaxation
• Detection of massive molecular and dust reservoirs around z~2 extremely red quasars: CGM enrichment by quasar-driven outflows
• A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
• High-resolution Spectroscopy of Thermal Emission from Exoplanets
• Tightest constraints on very-light Axion-Like Particles (ALPs) using the X-ray spectrum of the H1821+643 cluster-hosted quasar
• Do Supermassive Black Holes need Iron Supplements?
• What dust sizes tell us about planet-forming disc evolution
• Evidence for Gaseous Halos Around AGN at Cosmic Noon from ALMA CO(3-2) Observations
• A BayeSN Analysis of the SN Ia Trio of Siblings in NGC 3147
• Rethinking about Data Processing in the SKA Era
• The bispectrum of reconstructed CMB lensing convergence
• The role of AGN feedback in dwarf galaxies
• Investigating the composition of planets formed by Gravitational Instability
• Studying the magnetic evolution of black hole accretion disks
• Life after death: evidence of dry minor-merger driven growth of massive quiescent galaxies
• Spectroscopic studies of star-forming galaxies in the Epoch of Reionisation
• The unquiet neighbour: how the LMC bugs the Milky Way
• Connecting X-ray nuclear winds with galaxy-scale ionised outflows in nearby and z~1.5 quasars
• Through the Amber Spyglass: searching for Axion-like signals in X-ray spectra of cluster-hosted AGN
• The changing astrometry of Gaia's unresolved binaries