Study of the impact from nonlinear distortion in radio receiver architectures

A dissertação de doutoramento apresentada insere-se na área de electrónica não-linear de rádio-frequência (RF), UHF e microondas, tendo como principal campo de acção o estudo da distorção nãolinear em arquitecturas de recepção rádio, nomeadamente receptores de conversão directa como Power Meters, RFID (Radio Frequency IDentification) ou SDR (Software Define Radio) front-ends. Partindo de um estudo exaustivo das actuais arquitecturas de recepção de radiofrequência e revendo todos os conceitos teóricos relacionados com o desempenho não-linear dos sistemas/componentes electrónicos, foram desenvolvidos algoritmos matemáticos de modulação dos comportamentos não-lineares destas arquitecturas, simulados e testados em laboratório e propostas novas arquitecturas para a minimização ou cancelamento do impacto negativo de grandes interferidores em frequências vizinhas ao do sistema pretendido.

Characterisation of ZG16p, a unique mammalian lectin from pancreatic zymogen granules

The mechanisms of secretory granule biogenesis and regulated secretion of digestive enzymes in pancreatic acinar cells are still not well understood. To shed light on these processes, which are of biological and clinical importance (e.g., pancreatitis), a better molecular understanding of the components of the granule membrane, their functions and interactions is required. The application of proteomics has largely contributed to the identification of novel zymogen granule (ZG) proteins but was not yet accompanied by a better characterization of their functions. In this study we aimed at a) isolation and identification of novel membrane-associated ZG proteins; b) characterization of the biochemical properties and function of the secretory lectin ZG16p, a membrane-associated protein; c) exploring the potential of ZG16p as a new tool to label the endolysosomal compartment. First, we have performed a suborganellar proteomics approach by combining protein analysis by 2D-PAGE and identification by mass spectrometry, which has led to the identification of novel peripheral ZGM proteins with proteoglycan-binding properties (e.g., chymase, PpiB). Then, we have unveiled new molecular properties and (multiple) functions of the secretory lectin ZG16p. ZG16p is a unique mammalian lectin with glycan and proteoglycan binding properties. Here, I revealed for the first time that ZG16p is highly protease resistant by developing an enterokinase-digestion assay. In addition I revealed that ZG16p binds to a high molecular weight complex at the ZGM (which is also protease resistant) and forms highly stable dimers. In light of these findings I suggest that ZG16p is a key component of a predicted submembranous granule matrix attached to the luminal side of the ZGM that fulfils important functions during sorting and packaging of zymogens. ZG16p, may act as a linker between the matrix and aggregated zymogens due to dimer formation. Furthermore, ZG16p protease resistance might be of higher importance after secretion since it is known that ZG16p binds to pathogenic fungi in the gut. I have further investigated the role of ZG16p binding motifs in its targeting to ZG in AR42J cells, a pancreatic model system. Point mutations of the glycan and the proteoglycan binding motifs did not inhibit the targeting of ZG16p to ZG in AR42J cells. I have also demonstrated that when ZG16p is present in the cytoplasm it interacts with and modulates the endo-lysosomal compartment. Since it is known that impaired autophagy due to lysosomal malfunction is involved in the course of pancreatitis, a potential role of ZG16p in pancreatitis is discussed.

Nonlinear periodic problems with a jumping reaction

We consider a periodic problem driven by the scalar $p-$Laplacian and with a jumping (asymmetric) reaction. We prove two multiplicity theorems. The first concerns the nonlinear problem ($1

An extreme planetary system around HD 219828: one long-period super Jupiter to a hot-Neptune host star

Context. With about 2000 extrasolar planets confirmed, the results show that planetary systems have a whole range of unexpected properties. This wide diversity provides fundamental clues to the processes of planet formation and evolution. Aims: We present a full investigation of the HD 219828 system, a bright metal-rich star for which a hot Neptune has previously been detected. Methods: We used a set of HARPS, SOPHIE, and ELODIE radial velocities to search for the existence of orbiting companions to HD 219828. The spectra were used to characterise the star and its chemical abundances, as well as to check for spurious, activity induced signals. A dynamical analysis is also performed to study the stability of the system and to constrain the orbital parameters and planet masses. Results: We announce the discovery of a long period (P = 13.1 yr) massive (m sini = 15.1 MJup) companion (HD 219828 c) in a very eccentric orbit (e = 0.81). The same data confirms the existence of a hot Neptune, HD 219828 b, with a minimum mass of 21 M⊕ and a period of 3.83 days. The dynamical analysis shows that the system is stable, and that the equilibrium eccentricity of planet b is close to zero. Conclusions: The HD 219828 system is extreme and unique in several aspects. First, ammong all known exoplanet systems it presents an unusually high mass ratio. We also show that systems like HD 219828, with a hot Neptune and a long-period massive companion are more frequent than similar systems with a hot Jupiter instead. This suggests that the formation of hot Neptunes follows a different path than the formation of their hot jovian counterparts. The high mass, long period, and eccentricity of HD 219828 c also make it a good target for Gaia astrometry as well as a potential target for atmospheric characterisation, using direct imaging or high-resolution spectroscopy. Astrometric observations will allow us to derive its real mass and orbital configuration. If a transit of HD 219828 b is detected, we will be able to fully characterise the system, including the relative orbital inclinations. With a clearly known mass, HD 219828 c may become a benchmark object for the range in between giant planets and brown dwarfs.