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Calendar overview of all LAIP-events

18 May: Starry night in Babelsberg

Jonay I. González Hernández (IAC)

High precision spectroscopy with HARPS-LFC: the solar gravitational redshift

Cancelled!

Cameron Bell (AIP)

A revised age scale for young Galactic clusters

Tim Beers (University of Notre Dame)

Carbon in the Early Universe and Observational Constraints on First-Star Nucleosynthesis

Aline Vidotto (Trinity College Dublin)

Stellar magnetic activity and their effects on planets (and vice-versa)

Kathryn Kreckel (MPIA Heidelberg)

The ISM in Nearby Galaxies: An Optical IFU Perspective

Bridget Falck (Institute of Theoretical Astrophysics, University of Oslo)

Simulating the Large Scale Structure of the Universe

Mahmoudreza Oshagh (University Goettingen)

Impact of stellar surface inhomogeneities on the determination of exoplanet's parameters

L.C. Popovic (Astronomical Observatory, Belgrade)

Spectropolarimetry of Type 1 AGNs: AGN central structure and mass of black hole

Chervin Laporte (Columbia University)

The response of the Milky Way to the Large Magellanic Cloud and Sagittarius

Claudia Reinlein (Fraunhofer Institute Jena)

Active and Adaptive Optics at the Fraunhofer IOF

Marco Potenza and Mirko Siano (University of Milano)

From light scattering to hyperspectral imaging: optical analogical simulations

Marco Potenza and Mirko Siano (University of Milano)

Wavefront characterization of partially coherent light

Alexander Kolodzig (Kavli Institute, Beijing)

Can AGN, galaxy clusters, and WHIM explain the surface brightness fluctuations of the cosmic X-ray background?

Travis Metcalfe

The rotation and magnetic activity of Kepler field stars

Chris Brook (IAC, Tenerife)

Abundance Matching in the Local Volume

Kevin Schawinski (ETH, Zurich)

Supermassive black holes: from deep fields to deep minds

Alessandra Buonanno (Albert Einstein Institute, Potsdam)

The New Era of Precision Gravitational-Wave Astrophysics

Jochen Liske (Hamburg)

The low-redshift universe as seen by the Galaxy And Mass Assembly survey

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