Costado Dios
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Massive stars, resolved stellar populations in nearby galaxies |
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X-ray and multi-wavelength studies of X-ray binaries |
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Infrared Astrophysics, star-formation, AGN activity |
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Evangelia Ntormousi studied Physics at the University of Thessaloniki. She obtained her Ph.D. in Astrophysics in 2012, from the Ludwig-Maximillians University of Munich, as part of the International Max-Planck Research School in Astrophysics. |
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She was a postdoctoral fellow at the CEA (Commissariat à l'Énergie Atomique et aux énergies alternatives) in Saclay, France until 2017. She then moved, as a Marie-Curie postdoctoral fellow at FORTH, where is is collaborating with Prof. Konstantinos Tassis. |
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Magnetic fields; Interstellar turbulence; Galactic dynamics; Star formation; Stellar feedback |
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237 Physics Bldg
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(+30) 2810 39-4173
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Paolo Bonfini obtained his MSc in Astrophysics at the University of Milan-Bicocca (Italy) in 2008, and his PhD in Physics at the University of Crete (Greece) in 2013. |
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After the PhD, he obtained a postdoctoral position at the Centre for Astrophysics and Supercomputing (CAS) of the Swinburne University of Technology (Australia) during 2013-2015. Then, during 2015-2017, he was awarded a Mexican postdoctoral fellowship to work at the Instituto de Radioastronomia y Astrofisica (IRyA) of the National Autonomous University of Mexico (UNAM). In 2018 returned to IA-FORTH as a postdoc. From July 2018 until February 2020 he was a postdoc affiliated with the National Observatory of Athens. |
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Spectral properties of nearby galaxies, scaling relations between Super-Massive Black Holes (SMBHs) and their host galaxies, morphological modelling and evolution of nearby galaxies, dust rings in early-type galaxies, extragalactic Globular Cluster (GC) populations. |
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232 Physics Bldg
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(+30) 2810 39-4200
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Lankeswar Dey earned his B.Sc. in Physics from the University of Kalyani, India, in 2015. He then pursued an Integrated M.Sc.-Ph.D. program at the Tata Institute of Fundamental Research (TIFR), India, completing his doctoral degree in 2022. |
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Following his Ph.D., Lankeswar briefly worked at the National Centre for Radio Astrophysics (NCRA), India, before joining West Virginia University (WVU) as a Postdoctoral Fellow in September 2022. At WVU, he was an active member of the NANOGrav collaboration, contributing to pulsar timing array research. In September 2025, he joined the Institute of Astrophysics, Foundation for Research and Technology–Hellas (IA-FORTH), as a Postdoctoral Researcher on the MMMonsters project, focusing on the first multi-messenger detection of a supermassive black hole binary in collaboration with Maria Charisi. |
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Gravitational Waves, Supermassive Black Hole Binaries, Pulsar Timing Arrays, Multi-messenger Astronomy |
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114β Physics Bldg
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(+30) 281039 4154
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