Prof. Dr. Monica Colpi

University of Milan, Italy

Expertise in gravitational waves, eLISA, black hole binaries. More info.

Prof. Dr. Shep Doeleman

Harvard-Smithsonian Center for Astrophysics and MIT, Cambridge, USA

Expertise in Sgr A*, Event Horizon Telescope, accretion of supermassive black holes. More info.

Dr. Tommaso Grassi

Ludwig-Maxwellian University, Munich, Germany

Expertise in chemistry and microphysics of different enviroments, ranging from the interstellar medium in galaxy to primordial gas. More info.

Prof. Dr. Kayhan Gultekin

Michigan University, Department of Astronomy, Ann Arbor, USA

Expertise in supermassive black holes, galaxy nuclei, host galaxies. More info.

Prof. Dr. Ralf Klessen

Institute for Theoretical Astrophysics, University of Heidelberg, Germany

Expertise in gravitational collapse, numerical simulations, star formation, formation of massive objects. More info.

Prof. Dr. Muhammad Latif

COMSATS, Islamabad, Pakistan

Expertise in formation of the first stars and black holes, numerical simulations. More info.

Dr. Alessandro Lupi

Institute for Astrophysics, Paris, France

Expertise in Computational Astrophysics, numerical simulations of black holes formation and accretion. More info.

Prof Dr. Lucio Mayer

Center for Theoretical Astrophysics and Cosmology, Zurich, Switzerland

Expertise in formation of supermassive black holes, galaxies, numerical simulations, gravitational waves. More info.

Prof Dr. Priyamvada Natarajan

Yale University, USA

Expertise in formation and accretion of supermassive black holes, theoretical models.More info.

Prof. Dr. Kevin Schawinski

ETH, Zurich, Switzerland

Expertise in supermassive black holes, accretion, X-ray observations, NuSTAR.More info.

Prof. Dr. Raffaella Schneider

Sapienza University of Rome, Italy

Expertise in supermassive black holes, host galaxies, seed formation, gravitational waves.More info.

Dr. Daniel Stern

Jet Propulsory Laboratory, USA

NuSTAR project scientist.More info.

Prof Dr. Daniel Wang

Massachussets

Expertise in supermassive black holes, high-energy feedback, hot gas, radio, infrared, ultraviolet and X-ray observations.More info.