The J1030 field: a new window on early large scale structures and faint radio-galaxy populations

The correlations between the evolution of the Super Massive Black Holes (SMBHs) and their host galaxies suggests that the SMBH accretion on sub-pc scales (active galactice nuclei, AGN) is linked to the building of the galaxy over kpc scales, through the so called AGN feedback. Most of the galaxy assembly occurs in overdense large scale structures (LSSs). AGN residing in powerful sources in LSSs, such as the proto-brightest cluster galaxies (BCGs), can affect the evolution of the surrounding intra-cluster medium (ICM) and nearby galaxies. Among distant AGN, high-redshift radio-galaxies (HzRGs) are found to be excellent BCG progenitor candidates. In this Thesis we analyze novel interferometric observations of the so-called "J1030" field centered around the z = 6.3 SDSS Quasar J1030+0524, carried out with the Atacama large (sub-)millimetre array (ALMA) and the Jansky very large array (JVLA). This field host a LSS assembling around a powerful HzRG at z = 1.7 that shows evidence of positive AGN feedback in heating the surrounding ICM and promoting star-formation in multiple galaxies at hundreds kpc distances. We report the detection of gas-rich members of the LSS, including the HzRG. We showed that the LSS is going to evolve into a local massive cluster and the HzRG is the proto-BCG. we unveiled signatures of the proto-BCG's interaction with the surrounding ICM, strengthening the positive AGN feedback scenario. From the JVLA observations of the "J1030" we extracted one of the deepest extra-galactic radio surveys to date (~12.5 uJy at 5 sigma). Exploiting the synergy with the X-ray deep survey (~500 ks) we investigated the relation of the X-ray/radio emission of a X-ray-selected sample, unveiling that the radio emission is powered by different processes (star-formation and AGN), and that AGN-driven sample is mostly composed by radio-quiet objects that display a significant X-ray/radio correlation.

Disorders of arousal: a physiopathological window to explore the mechanisms regulating sleep arousal

Disorders of Arousal (DoA) belong to NREM parasomnias and are characterized by motor and emotional episodes arising from incomplete awakenings from NREM sleep. DoA episodes embody at the same time the double nature of the arousal process, that is preserving sleep as well as respond to sleep perturbations, thus being an ideal model to study sleep arousal. In the first part of this work, we performed a spectral whole scalp EEG analysis exploring the neurophysiologic correlates of the pre-motor onset of the episodes in a large sample of patients with DoA, disclosing the co-existence of both slow and fast EEG frequencies over overlapping areas before DoA episodes, suggesting an alteration of local sleep mechanisms. Episodes of different complexity were preceded by a similar EEG activation, implying that they possibly share a similar pathophysiology. In the second part of this work, we performed a spectral whole scalp EEG analysis comparing the pre-motor onset of the episodes and normal arousals from healthy sleepers, disclosing the persistence of slow frequencies as well as sigma band (expression of sleep spindles) in DoA episodes. Overall, these results might subtend a higher tendence to preserve sleep and a more defective mechanism toward developing a complete arousal in patients with DoA. In the last part of our work, we evaluated 15 patients with DoA with 15 controls in a functional MRI study during wakefulness in addition to a proton magnetic resonance spectroscopy (1H-MRS) focused on cingulate cortex. We disclosed subtle alterations on posterior cingulate cortex as well as an increased connectivity in sensory-motor network, possibly representing a trait-functional feature responsible for the dysfunctional arousal process in DoA patients