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Calendar overview of all LAIP-events

Kai Polsterer (Heidelberg Institute for Theoretical Studies)

Machine Learning in Astronomy - small lessons learned from learning machines

13 May, Tour over Telegrafenberg

Guided tour at the historical site at Potsdam-Telegrafenberg, including a visit to the Great Refractor (in German).

27 May: Tour over Telegrafenberg

Guided tour at the historical site at Potsdam-Telegrafenberg, including a visit to the Great Refractor (in German).

Christoffer Karoff (Aarhus University)

Using Sun-like stars and radio carbon to understand past solar activity

Nader Haghigipour (IfA - Hawaii)

Modern Simulations of Terrestrial Planet Formation and Origin of Earth's Water

JAMBOREE

Who does what

Wolf-Rainer Hamann

Massive stars, winds, feedback, gravitational wave progenitors

Shaun Cole (ICC, Durham, UK)

The DESI Bright Galaxy Survey

Florian Niederhofer (AIP)

The Magellanic Clouds - Discovering our Neighbours

Stephan Geier (Uni Potsdam)

Hot subdwarf stars in the Gaia era

Timur Doumler (AIP)

Life after astronomy

Gongbo Zhao (NAOC, China)

Understanding the cosmic acceleration using large scale structure surveys

Timothy Davis

The dark hearts of galaxies: Molecules as dynamical probes of galaxy evolution

Jan-Torge Schindler (University of Arizona)

The Extremely Luminous Quasar Survey (ELQS)

Alice Quillen (University of Rochester, USA)

Astro Visco-elastodynamics: Cracking moons and spin and obliquity evolution in tidally evolving and migrating satellite and planetary systems

Rolf Kuiper (University of Tuebingen)

Recycling of Embedded Planets??? First Atmospheres

Ines Juvan (Space Research Institute Graz, Austria)

Determining the spin-orbit alignment for an extra-solar super-Earth

Emma de Ona Wilhelmi (Institut de Ciencies de l'Espai)

An energy cutoff in the TeV gamma ray spectrum of the SNR Cassiopeia A

Morten Bache (DTU Copenhagen)

Ultrafast nonlinear optics with quadratic nonlinearities: prospects for integrated photonics

Rob Grand (HITS)

Disc formation and evolution in cosmological simulations of Milky Way analogues

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