Investigation of the Impacts of Parental Chronic Illness on Youth Caregiving Experiences and Psychosocial Adjustment.

Objective: Parental chronic illness has an impact on several aspects of offspring’s life. Three major impediments to research progress in this field are undeveloped and untested theoretical frameworks, no clear conceptualization of youth caregiving, and no available instrument to assess such construct in Italian. To address these weaknesses, the aims of this PhD dissertation were: (1) to investigate the psychometric properties of the Italian version of the Young Caregiver of Parents Inventory-Revised (YCOPI-R); (2) to empirically examine a model of the effects of parental illness on youth and family functioning innovatively analyzing the role of psychological flexibility; (3) to test a refined conceptualization of youth caregiving. Methods: A total of 501 adolescents aged 11 to 24 (295 young caregivers and 206 young noncaregivers) completed a questionnaire regarding youth caregiving, parental illness, and youth adjustment. In the first study, young caregivers were compared to noncaregivers, while the other studies used only the young carers subgroup. Results: The first study indicated that the Italian version of the YCOPI-R demonstrated sound psychometric and was able to discriminate between young caregivers and noncaregivers. The second study underlined the key protective role of psychological flexibility in shaping youth adjustment and family functioning in the context of parental illness. The third study innovatively clarified the nature of youth caregiving, indicating that it is a tripartite construct related to both positive and negative youth adjustment outcomes. Conclusions. This PhD project drew attention towards youth of chronically ill parents, a segment of the young population which is presently almost completely neglected in Italy by health policies and healthcare providers. This PhD project ultimately shed light into the processes through which parental illness results in detrimental youth outcomes and highlighted avenues for interventions that target empirically supported mechanisms which ameliorate the detrimental effects of parental illness on youth.

Obscured AGN in deep fields: tracing accretion and star-formation up to z ∼ 5

The discovery of scaling relations between the mass of the SMBH and some key physical properties of the host galaxy suggests that the growth of the SMBH and that of the galaxy are coupled, with the AGN activity and the star-formation (SF) processes influencing each other. Although the mechanism of this co-evolution are still a matter of debate, all scenarios agree that a key phase of the co-evolution is represented by the obscured accretion phase. This phase is of the co-evolution is the least studied, mostly due to the challenge in detecting and recognizing such obscured AGN. My thesis aims at investigating the AGN-galaxy co-evolution paradigm by identifying and studying AGN in the obscured accretion phase. The study of obscured AGN is key for our understanding of the feedback processes and of the mutual influence of the SF and the AGN activity. Moreover, these obscured and elusive AGN are needed to explain the X-ray background spectrum and to reconcile the measurements and the theoretical prediction of the BH accretion rate density. In this thesis, we firstly investigate the synergies between IR and X-ray missions in detecting and characterizing AGN, with a particular focus on the most obscured ones. We exploited UV/optical emission lines to select high-redshift obscured AGN at the cosmic noon, where the highest SFR density and BH accretion rate density are expected. We provide X-ray spectral analysis and UV-to-far-IR SED-fitting. We show that our samples host a significant fraction of very obscured sources; many of these are highly accreting. Finally, we performe a thoughtful investigation of a galaxy at z~5 with unusual and peculiar features, that lead us to identify a second extremely young population of stars and hidden AGN activity.

Cross-population radio galaxies as a test of the jet-accretion relationship

Radio galaxies (RGs) are extremely relevant in addressing important unknowns concerning the interaction among black hole accretion, radio jets, and the environment. In the classical scheme, their accretion rate and ejection of relativistic jets are directly linked: efficient accretion (HERG) is associated with powerful edge-brightened jets (FRIIs); inefficient accretion (LERG) is associated with weak edge-darkened jets (FRIs). The observation of RGs with an inefficient engine associated with edge-brightened radio emission (FRII-LERGs) broke this scheme. FRII-LERGs constitute a suitable population to explore how accretion and ejection are linked and evaluate the environment's role in shaping jets. To this aim, we performed a multiwavelength study of different RGs catalogs spanning from Jy to mJy flux densities. At first, we investigated the X-ray properties of a sample of 51 FRIIs belonging to the 3CR catalog at z<0.3. Two hypotheses were invoked to explain FRII-LERGs behavior: evolution from classical FRIIs; the role of the environment. Next, we explored the mJy sky by studying the optical-radio properties of hundreds of RGs at z<0.15 (Best & Heckman 2012 sample). FRII-LERGs appear more similar to the old FRI-LERGs than to the young FRII-HERGs. These results point towards an evolutive scenario, however, nuclear time scale changes, star population aging, and kpc-Mpc radio structure modification do not agree. The role of the Mpc environment was then investigated. The Wen et al. 2015 galaxy clusters sample, built exploiting the SDSS survey, allowed us to explore the habitat of 7219 RGs at z<0.3. Most RGs are found to live in outside clusters. For these sources, differences among RG classes are still present. Thus, the environment is not the key parameter, and the possibility of intrinsic differences was reconsidered: we speculated that different black hole properties (spin and magnetic field at its horizon) could determine the observed spread in jet luminosity.