IRAS 00183-7111: ALMA and X-ray view of an ultra luminous infrared galaxy

The aim of this Thesis work is to study the multi-frequency properties of the Ultra Luminous Infrared Galaxy (ULIRG) IRAS 00183-7111 (I00183) at z = 0.327, connecting ALMA sub-mm/mm observations with those at high energies in order to place constraints on the properties of its central power source and verify whether the gas traced by the CO may be responsible for the obscuration observed in X-rays. I00183 was selected from the so-called Spoon diagnostic diagram (Spoon et al. 2007) for mid-infrared spectra of infrared galaxies based on the equivalent width of the 6.2 μm Polycyclic Aromatic Hydrocarbon (PAH) emission feature versus the 9.7 μm silicate strength. Such features are a powerful tool to investigate the contribution of star formation and AGN activity in this class of objects. I00183 was selected from the top-left region of the plot where the most obscured sources, characterized by a strong Si absorption feature, are located. To link the sub-mm/mm to the X-ray properties of I00183, ALMA archival Cycle 0 data in Band 3 (87 GHz) and Band 6 (270 GHz) have been calibrated and analyzed, using CASA software. ALMA Cycle 0 was the Early Science program for which data reprocessing is strongly suggested. The main work of this Thesis consisted in reprocessing raw data to provide an improvement with respect to the available archival products and results, which were obtained using standard procedures. The high-energy data consists of Chandra, XMM-Newton and NuSTAR observations which provide a broad coverage of the spectrum in the energy range 0.5 − 30 keV. Chandra and XMM archival data were used, with an exposure time of 22 and 22.2 ks, respectively; their reduction was carried out using CIAO and SAS software. The 100 ks NuSTAR are still private and the spectra were obtained by courtesy of the PI (K. Iwasawa). A detailed spectral analysis was done using XSPEC software; the spectral shape was reproduced starting from simple phenomenological models, and then more physical models were introduced to account for the complex mechanisms that involve this source. In Chapter 1, an overview of the scientific background is discussed, with a focus on the target, I00183, and the Spoon diagnostic diagram, from which it was originally selected. In Chapter 2, the basic principles of interferometry are briefly introduced, with a description of the calibration theory applied to interferometric observations. In Chapter 3, ALMA and its capabilities, both current and future, are shown, explaining also the complex structure of the ALMA archive. In Chapter 4, the calibration of ALMA data is presented and discussed, showing also the obtained imaging products. In Chapter 5, the analysis and discussion of the main results obtained from ALMA data is presented. In Chapter 6, the X-ray observations, data reduction and spectral analysis are reported, with a brief introduction to the basic principle of X-ray astronomy and the instruments from which the observations were carried out. Finally, the overall work is summarized, with particular emphasis on the main obtained results and the possible future perspectives.

Distribuzione, prevalenza e host range della Skeleton Eroding Band nell'atollo di Faafu, Repubblica delle Maldive

Lo studio delle malattie che colpiscono i coralli rappresenta un campo di ricerca nuovo e poche sono le ricerche concentrate nell’Oceano Indo-Pacifico, in particolare nella Repubblica delle Maldive. Lo scopo di questa ricerca è stato approfondire le conoscenze riguardo distribuzione, prevalenza e host range della Skeleton Eroding Band (SEB) nell’atollo di Faafu. Durante il lavoro, svolto in campo tra il novembre e il dicembre 2013, sono state indagate le isole di: Magoodhoo, Filitheyo e Adangau al fine di rilevare differenze nei livelli di prevalenza della SEB in relazione ai diversi gradi di utilizzo da parte dell’uomo delle 3 isole. Il piano di campionamento ha previsto la scelta casuale, in ciascuna delle isole, di 4 siti in cui sono stati realizzati 3 belt transect e 3 point intercept transect a 2 profondità predefinite. La SEB è stata ritrovata con una prevalenza media totale di 0,27%. Dai risultati dell’analisi statistica le differenze fra le isole non sono apparse significative, facendo ipotizzare che i livelli di prevalenza differiscano a causa di oscillazioni casuali di carattere naturale e che quindi non siano dovute a dinamiche legate al diverso sfruttamento da parte dell’uomo. I generi Acropora e Pocillopora sono risultati quelli maggiormente colpiti con valori di prevalenza totale di 0,46% e 1,33%. Infine è stata rilevata una correlazione positiva tra il numero di colonie di madrepore affette dalla SEB e il numero di colonie in cui la malattia è associata alla presenza di lesioni provocate da danni meccanici. I dati di prevalenza ottenuti e le previsioni di cambiamenti climatici in grado di aumentare distribuzione, host range, abbondanza della patologia, pongono l’accento sulla necessità di chiarire il ruolo delle malattie dei coralli nel deterioramento, resilienza e recupero dei coral reefs, al fine di attuare politiche di gestione adatte alla protezione di questi fragili ecosistemi.