Student

In February of 2024, he started working on his senior thesis under the supervision of Prof. Iossif Papadakis, titled "Study of the temperature radial dependence in X-ray illuminated accretion discs".

In February of 2024, he started working on his senior thesis under the supervision of Prof. Iossif Papadakis, titled "Study of the temperature radial dependence in X-ray illuminated accretion discs".

In 2024 he started working on his bachelor’s thesis titled  “X-ray Variability Studies of NGC 4051” under the supervision of professor Iossif Papadakis, which he presented in October of the same year.

In 2023 she joined the Institute of Astrophysics at FORTH, when she started working on her senior thesis studying the timing and spectral variability of Be/X-ray binaries under the supervision of Dr. Pablo Reig.

In the summer of 2023 she completed her internship at Skinakas Observatory. At the beginning of the academic year she started working on her senior thesis which is centered around the spatially resolved dust attenuation in Luminous Infrared Galaxies (LIRGs). Throughout autumn of 2023 she worked on supernovae and transient astronomy at the University of Kyoto and Okayama Observatory.

In the summer of 2022, he completed his internship at Skinakas Observatory and the following summer worked there voluntarily. In the fall of 2023, he started working on his senior thesis studying the long term optical variability of Be/X-ray binaries under the supervision of Dr. Reig, which completed in the autumn of 2024. Afterwards, he started working on his thesis studying secondary standard stars in the field of view of Be/X-ray binary systems, again under the supervision of Dr. Reig.

In the summer of 2022, he completed his internship at Skinakas Observatory and the following summer worked there voluntarily. In the fall of 2023, he started working on his senior thesis studying the long term optical variability of Be/X-ray binaries under the supervision of Dr.Reig.

During her Master's Thesis « Impact of the distortion of time on the galaxy angular power spectrum » she worked on forecasting the signal to noise ratio for the SKA experiment by considering the observation of two different populations of galaxies (bright and faint), with the goal of testing General Relativity at large scales of the Universe, under the supervision of Prof. C. Bonvin and Sveva Castello at the University of Geneva. 

During her PhD studies, she will work on « Higher-order statistics for neutral hydrogen intensity mapping » as a member of the TITAN project.

For her PhD studies, she is using radio observations to study compact symmetric objects and supermassive black hole binaries. She is also a member of the PASIPHAE Collaboration, working on the mapping of the galactic magnetic field. Her research interests also include cosmological structure formation.

In 2023 he worked and completed his undergraduate thesis, titled “Warm Molecular Gas in Hot Dust-Obscured Quasars”, under the supervision of Dr. Tanio Diaz-Santos. During the summer of 2022, he completed his 3-month internship as an observant in Skinakas Observatory. He is now working on his master thesis under the supervision of Prof. I. Papadakis. For his MSc thesis he will study the flux variability of the accretion discs in Active Galactic Nuclei.