Procedures of quality control and data analysis of multi-site ground-based observations for the absolute flux calibration of Gaia

The Gaia space mission is a major project for the European astronomical community. As challenging as it is, the processing and analysis of the huge data-flow incoming from Gaia is the subject of thorough study and preparatory work by the DPAC (Data Processing and Analysis Consortium), in charge of all aspects of the Gaia data reduction. This PhD Thesis was carried out in the framework of the DPAC, within the team based in Bologna. The task of the Bologna team is to define the calibration model and to build a grid of spectro-photometric standard stars (SPSS) suitable for the absolute flux calibration of the Gaia G-band photometry and the BP/RP spectrophotometry. Such a flux calibration can be performed by repeatedly observing each SPSS during the life-time of the Gaia mission and by comparing the observed Gaia spectra to the spectra obtained by our ground-based observations. Due to both the different observing sites involved and the huge amount of frames expected (≃100000), it is essential to maintain the maximum homogeneity in data quality, acquisition and treatment, and a particular care has to be used to test the capabilities of each telescope/instrument combination (through the “instrument familiarization plan”), to devise methods to keep under control, and eventually to correct for, the typical instrumental effects that can affect the high precision required for the Gaia SPSS grid (a few % with respect to Vega). I contributed to the ground-based survey of Gaia SPSS in many respects: with the observations, the instrument familiarization plan, the data reduction and analysis activities (both photometry and spectroscopy), and to the maintenance of the data archives. However, the field I was personally responsible for was photometry and in particular relative photometry for the production of short-term light curves. In this context I defined and tested a semi-automated pipeline which allows for the pre-reduction of imaging SPSS data and the production of aperture photometry catalogues ready to be used for further analysis. A series of semi-automated quality control criteria are included in the pipeline at various levels, from pre-reduction, to aperture photometry, to light curves production and analysis.

Homogeneous analysis of a sample of Open Clusters in the context of the BOCCE project and the Gaia-ESO Survey

The open clusters (OC) are gravitationally bound systems of a few tens or hundreds of stars. In our Galaxy, the Milky Way, we know about 3000 open clusters, of very different ages in the range of a few millions years to about 9 Gyr. OCs are mainly located in the Galactic thin disc, with distances from the Galactic centre in the range 4-22 kpc and a height scale on the disc of about 200 pc. Their chemical properties trace those of the environment in which they formed and the metallicity is in the range -0.5<[Fe/H]<+0.5 dex. Through photometry and spectroscopy it is possible to study relatively easily the properties of the OCs and estimate their age, distance, and chemistry. For these reasons they are considered primary tracers of the chemical properties and chemical evolution of the Galactic disc. The main subject of this thesis is the comprehensive study of several OCs. The research embraces two different projects: the Bologna Open Cluster Chemical Evolution project (BOCCE) and the Gaia-ESO Survey. The first is a long-term programme, aiming at studying the chemical evolution of the Milky Way disc by means of a homogeneous sample of OCs. The latter is a large public spectroscopy survey, conducted with the high-resolution spectrograph FLAMES@VLT and targeting about 10^5 stars in different part of the Galaxy and 10^4 stars in about 100 OCs. The common ground between the two projects is the study of the properties of the OCs as tracers of the disc's characteristics. The impressive scientific outcome of the Gaia-ESO Survey and the unique framework of homogeneity of the BOCCE project can propose, especially once combined together, a much more accurate description of the properties of the OCs. In turn, this will give fundamental constraints for the interpretation of the properties of the Galactic disc.

Pulsating variable stars as tracers of galactic structure and interaction mechanisms

My PhD project has been focused on the study of the pulsating variable stars in two ultra-faint dwarf spheroidal satellites of the Milky Way, namely, Leo IV and Hercules; and in two fields of the Large Magellanic Cloud (namely, the Gaia South Ecliptic Pole calibration field, and the 30 Doradus region) that were repeatedly observed in the KS band by the VISTA Magellanic Cloud (VMC, PI M.R. Cioni) survey of the Magellanic System.

I controlli sulla tutela interinale della crisi della famiglia

La tesi affronta il tema dei controlli avverso i provvedimenti nell’interesse della prole e dei coniugi resi nell’ambito dei procedimenti di separazione e di divorzio, dapprima fornendo un inquadramento storico della problematica, attraverso la disamina delle posizioni dottrinali e giurisprudenziali formatesi con riferimento alla natura ed al regime impugnatorio di tali provvedimenti dall’entrata in vigore del codice di rito del 1865 ad oggi, dopodiché analizzando le numerose questioni interpretative cui l’attuale quadro normativo, risultante dalla stratificazione legislativa operata dalla L. 14 maggio 2005, n. 80 e dalla L. 8 febbraio 2006, n. 54, dà origine. In particolare la tesi, dopo aver delineato la struttura del reclamo di cui all’art. 708 c.p.c., cercando di fornire una soluzione ai dubbi che la scarna disciplina contenuta nella menzionata norma solleva, si occupa dei rapporti tra gli istituti del reclamo alla Corte d’appello e della revoca e modifica ad opera del giudice istruttore, riepilogando le varie teorie elaborate dalla dottrina e dalla giurisprudenza sul tema e cercando di individuare quale sia l’ambito di applicazione di ciascuno strumento di controllo. La tesi affronta poi, a fronte della mancata previsione di una forma di riesame avanti ad un organo superiore avverso i provvedimenti resi dal giudice istruttore ai sensi dell’art. 709, ultimo comma, c.p.c., la questione della reclamabilità di tali provvedimenti, cercando di individuare quale sia lo strumento più idoneo cui fare ricorso per colmare la lacuna che si dovesse ritenere esistente nel dato normativo. Il lavoro si conclude con la disamina, in una prospettiva de iure condendo, dei progetti di riforma che sono stati elaborati con riferimento al tema dei controlli avverso i provvedimenti temporanei e urgenti.

Tecnica, stile e ideologia nella musica sinfonica in video: la Quinta Sinfonia di Beethoven

Oggetto di questo lavoro è un’analisi dettagliata di un campione ristretto di riprese televisive della Quinta Sinfonia di Beethoven, con l’obiettivo di far emergere il loro meccanismo costruttivo, in senso sia tecnico sia culturale. Premessa dell’indagine è che ciascuna ripresa sia frutto di un’autorialità specifica che si sovrappone alle due già presenti in ogni esecuzione della Quinta Sinfonia, quella del compositore e quella dell’interprete, definita perciò «terza autorialità» riassumendo nella nozione la somma di contributi specifici che portano alla produzione di una ripresa (consulente musicale, regista, operatori di ripresa). La ricerca esamina i rapporti che volta a volta si stabiliscono fra i tre diversi piani autoriali, ma non mira a una ricostruzione filologica: l’obiettivo non è ricostruire le intenzioni dell’autore materiale quanto di far emergere dall’esame della registrazione della ripresa, così com’è data a noi oggi (spesso in una versione già più volte rimediata, in genere sotto forma di dvd commercializzato), scelte tecniche, musicali e culturali che potevano anche essere inconsapevoli. L’analisi dettagliata delle riprese conferma l’ipotesi di partenza che ci sia una sorta di sistema convenzionale, quasi una «solita forma» o approccio standardizzato, che sottende la gran parte delle riprese; gli elementi che si possono definire convenzionali, sia per la presenza sia per la modalità di trattamento, sono diversi, ma sono soprattutto due gli aspetti che sembrano esserne costitutivi: il legame con il rito del concerto, che viene rispettato e reincarnato televisivamente, con la costruzione di una propria, specifica aura; e la presenza di un paradigma implicito e sostanzialmente ineludibile che pone la maggior parte delle riprese televisive entro l’alveo della concezione della musica classica come musica pura, astratta, che deve essere compresa nei suoi propri termini.

Improving the cosmic distance ladder. Distance and structure of the Large Magellanic Cloud

The Large Magellanic Cloud (LMC) is widely considered as the first step of the cosmological distance ladder, since it contains many different distance indicators. An accurate determination of the distance to the LMC allows one to calibrate these distance indicators that are then used to measure the distance to far objects. The main goal of this thesis is to study the distance and structure of the LMC, as traced by different distance indicators. For these purposes three types of distance indicators were chosen: Classical Cepheids,``hot'' eclipsing binaries and RR Lyrae stars. These objects belong to different stellar populations tracing, in turn, different sub-structures of the LMC. The RR Lyrae stars (age >10 Gyr) are distributed smoothly and likely trace the halo of the LMC. Classical Cepheids are young objects (age 50-200 Myr), mainly located in the bar and spiral arm of the galaxy, while ``hot'' eclipsing binaries mainly trace the star forming regions of the LMC. Furthermore, we have chosen these distance indicators for our study, since the calibration of their zero-points is based on fundamental geometric methods. The ESA cornerstone mission Gaia, launched on 19 December 2013, will measure trigonometric parallaxes for one billion stars with an accuracy of 20 micro-arcsec at V=15 mag, and 200 micro-arcsec at V=20 mag, thus will allow us to calibrate the zero-points of Classical Cepheids, eclipsing binaries and RR Lyrae stars with an unprecedented precision.

Global and regional sea level variations in the recent past and future: insight from observations and modeling

This work is focused on the analysis of sea–level change (last century), based mainly on instrumental observations. During this period, individual components of sea–level change are investigated, both at global and regional scales. Some of the geophysical processes responsible for current sea-level change such as glacial isostatic adjustments and current melting terrestrial ice sources, have been modeled and compared with observations. A new value of global mean sea level change based of tide gauges observations has been independently assessed in 1.5 mm/year, using corrections for glacial isostatic adjustment obtained with different models as a criterion for the tide gauge selection. The long wavelength spatial variability of the main components of sea–level change has been investigated by means of traditional and new spectral methods. Complex non–linear trends and abrupt sea–level variations shown by tide gauges records have been addressed applying different approaches to regional case studies. The Ensemble Empirical Mode Decomposition technique has been used to analyse tide gauges records from the Adriatic Sea to ascertain the existence of cyclic sea-level variations. An Early Warning approach have been adopted to detect tipping points in sea–level records of North East Pacific and their relationship with oceanic modes. Global sea–level projections to year 2100 have been obtained by a semi-empirical approach based on the artificial neural network method. In addition, a model-based approach has been applied to the case of the Mediterranean Sea, obtaining sea-level projection to year 2050.