Basilakos Spyros

Spyros Basilakos is a cosmologist with a career spanning scientific research, academic teaching and science communication. He has held a number of academic positions at various universities around Europe. Spyros Basilakos is the head of the Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing (IAASARS) at the National Observatory of Athens. He is President of the Greek National Committee for Astronomy that advises the Greek government for issues which are related with Astronomy and Astrophysics. Also, he is the National Delegate in the International Astronomical Union (IAU). Since 09/02/2021 Dr. S. Basilakos also serves the governing board of NOA from the post of Vice-President.

He completed his PhD studies in Cosmology at the University of Athens. During the period 1999-2002, he worked as a PPARC fellow at the Imperial College (UK). From 2002 to 2005, he worked within NOA’s (National observatory of Athens) program searching for the clustering properties of the large scale structures. In 2005 he joined the astrophysics group at the University of Groningen (The Netherlands) as a NOVA fellow. For the period 2006-2014 he was a faculty member (Senior Researcher) at the Academy of Athens (RCAAM) and a Visiting Professor at the University of Barcelona (2011-2012). Today he is Director of Research at the Academy of Athens and head of IAASARS. In 2013, 2014, 2017 and 2019 he participated in the international Gravity competition organized by the Gravity Research Foundation (GRF-USA) and his scientific works received honorable mentions by GRF. Moreover, he supervised a large number of PhD and MSc theses and he participated in several international collaborations and scientific programs. His research work has led to ~220 scientific articles. Currently, he gives lectures in Cosmology and General Relativity at the University of Athens and contributes to public engagement events in science.


Cosmological tests of General Relativity, constraints on the cosmological parameters using observational data, nature of dark energy and the accelerating Universe, the physics of inflation and the evolution of matter perturbations, statistical and geometrical measures for quantifying large-scale structures.