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          • IPPL: A Massively Parallel, Performance Portable C++ Library for Particle-Mesh Methods
          • Cosmological neutrino mass bounds with DESI from a Bayesian & frequentist perspective
          • Recent Results from the Atacama Cosmology Telescope: Implications for our Understanding of Cosmology and Fundamental Physics
          • Cosmic Clocks and Cosmic Chronometers: Constraining the Hubble Parameter Now and Then
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          • How to make trustworthy simulation-based inference for large-scale structure cosmology?
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          • Cosmology in Teleparallel Gravity
          • Constraining baryonic feedback with kinematic Sunyaev Zel'dovich signal
          • Using the combination of CMB and LSS datasets to understand our Universe
          • Our Universe in Simulation
          • Investigating the Epoch of Reionisation with Closure Phases
          • The Unique Challenges Facing Studies of the 21-cm Signal at 55 > z
          • Explainable Deep Learning Models for Cosmological Structure Formation
          • DES+KiDS: Cosmic Shear Cosmology with 127 Million Galaxies
          • Cosmology in the Era of Multi-Messenger Astrophysics with Gravitational Waves
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          • Steps towards accurate simulations of structure formation and Reionization
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CosmoClub HS24

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  • Cosmology in Teleparallel Gravitychevron_right
  • Constraining baryonic feedback with kinematic Sunyaev Zel'dovich signalchevron_right
  • Using the combination of CMB and LSS datasets to understand our Universechevron_right
  • Our Universe in Simulationchevron_right
  • Investigating the Epoch of Reionisation with Closure Phaseschevron_right
  • The Unique Challenges Facing Studies of the 21-cm Signal at 55 > zchevron_right
  • Explainable Deep Learning Models for Cosmological Structure Formationchevron_right
  • DES+KiDS: Cosmic Shear Cosmology with 127 Million Galaxieschevron_right
  • Cosmology in the Era of Multi-Messenger Astrophysics with Gravitational Waveschevron_right
  • Cosmology from eROSITA’s X-ray Observationschevron_right
  • Steps towards accurate simulations of structure formation and Reionizationchevron_right

CosmoClub is a periodic seminar organized by the Cosmology Research Group, offering a platform for both internal and external researchers to present their work. Each session features a 45-minute presentation followed by a 15-minute Q&A session. The talks provide insights into the latest developments in cosmology, they are delivered in English and can be followed in person or online.

Subscribe to the CosmoClub mailing list here.

Room: HIT J 43.1 (meeting room)

external page Zoom link

Program Autumn Semester 2024

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Ana Milena Ramirez Barrero
  • Location location_onHIT J 13.2
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