The high velocity tail of the total velocity distribution of stars provides essential insight into fundamental properties of the Galaxy. Hypervelocity stars (HVSs), travelling on unbound orbits... Show moreThe high velocity tail of the total velocity distribution of stars provides essential insight into fundamental properties of the Galaxy. Hypervelocity stars (HVSs), travelling on unbound orbits coming from the Galactic Centre, are powerful tracers of the underlying Galactic gravitational potential, and can shed light on the stellar population in the proximity of our massive black hole. Runaway stars, ejected from the stellar disk, provide information on binary evolution and stellar clusters' dynamical processes. The advent of the data from the European Space Agency satellite Gaia has revolutionized our knowledge on high velocity stars. In my PhD thesis entitled "Hunting for the fastest stars in the Milky Way" I present my work on searching for the fastest stars in the Milky Way. I start by presenting our modelling work on predicting the HVS population expected to be contained in the Gaia catalogue. Then I illustrate the data mining techniques built and implemented to find these rare objects in the first and second data release of Gaia. Finally, I conclude discussing how HVSs can be used to constrain the Galactic dark matter halo and the binary population in the Galactic Centre. Show less
The work presented in this thesis is part of an on-going effort to understand and mitigate the effects of radiation damage in astronomical CCDs. My research was motivated by and took place in the... Show moreThe work presented in this thesis is part of an on-going effort to understand and mitigate the effects of radiation damage in astronomical CCDs. My research was motivated by and took place in the challenging context of the European Space Agency__s (ESA) astrometric mission, Gaia, for which radiation damage has been considered since its conception as one of the most important threats to its scientific performance. In this context my research focused primarily on the modelling of the effects of radiation-induced Charge Transfer Inefficiency (CTI) supported by the analysis of the experimental test data. I developed the most detailed model to date of CTI in CCDs that enables simulating the operation of irradiated devices (Chapter 2). Using this model I have been able to verify and enhance our current understanding of CTI as well as support the characterization of CCDs and the understanding of experimental results (Chapters 3 and 6). As part of this research I conducted the comprehensive re-assessment of the performance of Gaia taking into account radiation damage (Chapters 3 and 4). Finally I took part in the effort of countering CTI by elaborating, testing, and improving a forward modelling approach at the image processing level to mitigate the CTI effects on the Gaia easurements (Chapters 3 and 5), as well as test and explore the potential of a specific hardware mitigation tool (Chapter 6). Show less
