Tracing AGN accretion and star formation in Herschel galaxies

In this Thesis, we study the physical properties and the cosmic evolution of AGN and their host galaxies since z∼3. Our analysis exploits samples of star forming galaxies detected with Herschel at far-IR wavelengths (from 70 up to 500 micron) in different extragalactic surveys, such as COSMOS and the deep GOODS (South and North) fields. The broad-band ancillary data available in COSMOS and the GOODS fields, allows us to implement Herschel and Spitzer photometry with multi-wavelength ancillary data. We perform a multicomponent SED-fitting decomposition to decouple the emission due to star formation from that due to AGN accretion, and to estimate both host-galaxy parameters (such as stellar mass, M* and star formation rate, SFR), and nuclear intrinsic bolometric luminosities. We use the individual estimates of AGN bolometric luminosity obtained through SED-fitting decomposition to reconstruct the redshit evolution of the AGN bolometric luminosity function since z∼3. The resulting trends are used to estimate the overall AGN accretion rate density at different cosmic epochs and to trace the first ever estimate of the AGN accretion history from an IR survey. Later on, we focus our study on the connection between AGN accretion and integrated galaxy properties. We analyse the relationships of AGN accretion with galaxy properties in the SFR-M* plane and at different cosmic epochs. Finally, we infer what is the parameter that best correlates with AGN accretion, comparing our results with previous studies and discussing their physical implications in the context of current scenarios of AGN/galaxy evolution.

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.

Study of two novel streptococcus pneumoniae operons: pilus islet 2 and the lantibiotic operon

Analysis of publicly available genomes of Streptococcus pneumoniae has led to the identification of a new genomic element resembling gram-positive pilus islets (PIs). Here, we demonstrate that this genomic region, herein referred to as PI-2 (containing the genes pitA, sipA, pitB, srtG1, and srtG2) codes for a novel functional pilus in pneumococcus. Therefore, there are two pilus islets identified so far in this pathogen (PI-1 and PI-2). Polymerization of the PI-2 pilus requires the backbone protein PitB as well as the sortase SrtG1 and the signal peptidase-like protein SipA. PI-2 is associated with serotypes 1, 2, 7F, 19A, and 19F, considered to be emerging in both industrialized and developing countries. Interestingly, strains belonging to clonal complex 271 (CC271) contain both PI-1 and PI-2, as revealed by genome analyses. In these strains both pili are surface exposed and independently assembled. Furthermore, in vitro experiments provide evidence that the pilus encoded by PI-2 of S. pneumoniae is involved in adherence. Thus, pneumococci encode at least two types of pili that may play a role in the initial host cell contact to the respiratory tract. In addition, the pilus proteins are potential antigens for inclusion in a new generation of pneumococcal vaccines. Adherence by pili could represent important factor in bacterial community formation, since it has been demonstrated that bacterial community formation plays an important role in pneumococcal otitis media. In vitro quantification of bacterial community formation by S. pneumoniae was performed in order to investigate the possible role of pneumococcal pili to form communities. By using different growth media we were not able to see clear association between pili and community formation. But our findings revealed that strains belonging to MLST clonal complex CC15 efficiently form bacterial communities in vitro in a glucose dependent manner. We compared the genome of forty-four pneumococcal isolates discovering four open reading frames specifically associated with CC15. These four genes are annotated as members of an operon responsible for the biosynthesis of a putative lanctibiotic peptide, described to be involved in bacterial community formation. Our experiments show that the lanctibiotic operon deletion affects glucose mediated community formation in CC 15 strain INV200. Moreover, since glucose consumption during bacterial growth produce an acidic environment, we tested bacterial community formation at different pH and we showed that the lanctibiotic operon deletion affected pH mediated community formation in CC 15 strain INV200. In conclusion, these data demonstrate that the putative lanctibiotic operon is associated with pneumococcal CC 15 strains in vitro bacterial community formation.