Forecasting a language shift based on cellular automata

Language extinction as a consequence of language shifts is a widespread social phenomenon that affects several million people all over the world today. An important task for social sciences research should therefore be to gain an understanding of language shifts, especially as a way of forecasting the extinction or survival of threatened languages, i.e., determining whether or not the subordinate language will survive in communities with a dominant and a subordinate language. In general, modeling is usually a very difficult task in the social sciences, particularly when it comes to forecasting the values of variables. However, the cellular automata theory can help us overcome this traditional difficulty. The purpose of this article is to investigate language shifts in the speech behavior of individuals using the methodology of the cellular automata theory. The findings on the dynamics of social impacts in the field of social psychology and the empirical data from language surveys on the use of Catalan in Valencia allowed us to define a cellular automaton and carry out a set of simulations using that automaton. The simulation results highlighted the key factors in the progression or reversal of a language shift and the use of these factors allowed us to forecast the future of a threatened language in a bilingual community.

Transport Resource Management within UMTS Radio Network Subsystem

Tällä hetkellä haastavin telekommunikaatioteollisuuden tutkimus – ja kehitystoiminta on keskittynyt kolmannen sukupolven matkapuhelinjärjestelmien ympärille. Järjestelmien standardointityössä on saatu aikaiseksi ensimmäiset vakaat spesifikaatioversiot ja kaupallista toimintaa ollaan parhaillaan aloittelemassa Japanissa ja Euroopassa. Eräs kolmannen sukupolven järjestelmistä on UMTS (Universal Mobile Telecommunications System). Tämä diplomityö antaa yleiskuvan UMTS järjestelmästä ja sen eri verkkoelementtien toiminnallisuuksista. Päähuomio on kiinnitetty radioverkkojärjestelmään (UMTS Terrestrial Radio Access Network) ja erityisesti sen radioaliverkkojärjestelmään (Radio Network Subsystem), joka koostuu radioverkonohjaimesta (Radio Network Controller) ja joukosta siihen kuuluvia tukiasemia (Node B). Radioverkonohjain ja tukiasemat on yhdistetty avoimen rajapinnan kautta jota kutsutaan Iub -rajapinnaksi. Rajapinta tarjoaa radioverkonohjaimelle mahdollisuuden kontrolloida tukiasemia signalointiviestien avulla ja mahdollistaa tehokkaan ja luotettavan käyttäjätiedon siirron radioaliverkkojärjestelmän sisällä. Tämän diplomityön pääasiallinen sisältö on siirtoresurssien hallinta Iub -rajapinnan ylitse. Työssä esitellään ja selitetään siirtoverkon arkkitehtuuri. Myös kaikki Iub:ssä sijaitsevat protokollat ja toiminnalliset yksiköt jotka vaikuttavat siirtoresurssien hallintaan esitellään ja kuvataan yksityiskohtaisesti. Päähuomio on kiinnitetty sovellusprotokolliin sekä rajapinnan siirtoverkko- että radioverkkokerroksella sekä näiden protokollien väliseen vuorovaikutukseen. Kyseiset protokollat ovat Node B Application Part (NBAP) ja Access Link Control Application Part (ALCAP). Työn toteutusosassa käydään lävitse NBAP –protokollan prototyypin ja Node B Manager –toiminnallisen yksikön prototyypin implementaatio.

Review of quantitative phase-digital holographic microscopy: promising novel imaging technique to resolve neuronal network activity and identify cellular biomarkers of psychiatric disorders.

Quantitative phase microscopy (QPM) has recently emerged as a new powerful quantitative imaging technique well suited to noninvasively explore a transparent specimen with a nanometric axial sensitivity. In this review, we expose the recent developments of quantitative phase-digital holographic microscopy (QP-DHM). Quantitative phase-digital holographic microscopy (QP-DHM) represents an important and efficient quantitative phase method to explore cell structure and dynamics. In a second part, the most relevant QPM applications in the field of cell biology are summarized. A particular emphasis is placed on the original biological information, which can be derived from the quantitative phase signal. In a third part, recent applications obtained, with QP-DHM in the field of cellular neuroscience, namely the possibility to optically resolve neuronal network activity and spine dynamics, are presented. Furthermore, potential applications of QPM related to psychiatry through the identification of new and original cell biomarkers that, when combined with a range of other biomarkers, could significantly contribute to the determination of high risk developmental trajectories for psychiatric disorders, are discussed.

Radio Imaging of the Very-High-Energy γ-Ray Emission Region in the Central Engine of a Radio Galaxy

The accretion of matter onto a massive black hole is believed to feed the relativistic plasma jets found in many active galactic nuclei (AGN). Although some AGN accelerate particles to energies exceeding 1012 electron volts and are bright sources of very-high-energy (VHE) γ-ray emission, it is not yet known where the VHE emission originates. Here we report on radio and VHE observations of the radio galaxy Messier 87, revealing a period of extremely strong VHE γ-ray flares accompanied by a strong increase of the radio flux from its nucleus. These results imply that charged particles are accelerated to very high energies in the immediate vicinity of the black hole.

Product Definition Process for Mobile Radio System Product

Työn tarkoituksena oli tutkia tuotteen määrittelyyn liittyvää kirjallisuutta ja perehtyä tuotteen määrittelytyön nykytilaan kohdeyrityksessä. Näihin molempiin perustuen muodostetaan prosessimalli tuotteen määrittelytyölle kohdeyrityksessä. Työssä käsitellään prosessijohtamisen pääperiaatteet sekä tuotteen määrittelyä koskevaa kirjallisuutta ja tutkimuksia. Koska kysessä oleva tuote on suurelta osalta ohjelmistotuote, ohjelmistojen suunnittelua, erityisesti ohjelmistovaatimusten hallintaa ja ohjelmistojen määrittelyä, on myös tarkasteltu työssä. Tuotteen määrittelyn haasteita on käsitelty yksityiskohtaisemmin, esimerkiksi dokumentointia, prosessin kulkua, vaatimusten epävakaisuutta sekä muutoksia. Kohdeyritys ja sen ongelmakohdat esitellään ja luodaan prosessimalli. Tämä malli esittelee seuraavat prosessit: raakavaatimusten hallinta -prosessin, roadmapping -prosessin, esisuunnittelu- ja spesifikaatioprosessin ja julkaisun suunnittelu -prosessin. Kaikki nämä ovat vaiheita ennen varsinaisen tuotekehitysprojektin aloittamista. Työssä esitellään myös kolmetasoinen dokumentaatiomalli.

The 2010 May Flaring Episode of Cygnus X-3 in Radio, X-rays, and γ-rays

In 2009, Cygnus X-3 (Cyg X-3) became the first microquasar to be detected in the GeV γ-ray regime, via the satellites Fermi and AGILE. The addition of this new band to the observational toolbox holds promise for building a more detailed understanding of the relativistic jets of this and other systems. We present a rich data set of radio, hard and soft X-ray, and γ-ray observations of Cyg X-3 made during a flaring episode in 2010 May. We detect a ~3 day softening and recovery of the X-ray emission, followed almost immediately by a ~1 Jy radio flare at 15 GHz, followed by a 4.3σ γ-ray flare (E > 100 MeV) ~1.5 days later. The radio sampling is sparse, but we use archival data to argue that it is unlikely the γ-ray flare was followed by any significant unobserved radio flares. In this case, the sequencing of the observed events is difficult to explain in a model in which the γ-ray emission is due to inverse Compton scattering of the companion star's radiation field. Our observations suggest that other mechanisms may also be responsible for γ-ray emission from Cyg X-3.

Deep radio images of the HEGRA and Whipple TeV sources in the Cygnus OB2 region.

The modern generation of Cherenkov telescopes has revealed a new population of gamma-ray sources in the Galaxy. Some of them have been identified with previously known X-ray binary systems while other remain without clear counterparts a lower energies. Our initial goal here was reporting on extensive radio observations of the first extended and yet unidentified source, namely TeV J2032+4130. This object was originally detected by the HEGRA telescope in the direction of the Cygnus OB2 region and its nature has been a matter of debate during the latest years. The situation has become more complex with the Whipple and MILAGRO telescopes new TeV detections in the same field which could be consistent with the historic HEGRA source, although a different origin cannot be ruled out. Aims.We aim to pursue our radio exploration of the TeV J2032+4130 position that we initiated in a previous paper but taking now into account the latest results from new Whipple and MILAGRO TeV telescopes. The data presented here are an extended follow up of our previous work. Methods.Our investigation is mostly based on interferometric radio observations with the Giant Metre Wave Radio Telescope (GMRT) close to Pune (India) and the Very Large Array (VLA) in New Mexico (USA). We also conducted near infrared observations with the 3.5 m telescope and the OMEGA2000 camera at the Centro Astronómico Hispano Alemán (CAHA) in Almería (Spain). Results.We present deep radio maps centered on the TeV J2032+4130 position at different wavelengths. In particular, our 49 and 20 cm maps cover a field of view larger than half a degree that fully includes the Whipple position and the peak of MILAGRO emission. Our most important result here is a catalogue of 153 radio sources detected at 49 cm within the GMRT antennae primary beam with a full width half maximum (FWHM) of 43 arc-minute. Among them, peculiar sources inside the Whipple error ellipse are discussed in detail, including a likely double-double radio galaxy and a one-sided jet source of possible blazar nature. This last object adds another alternative counterpart possibility to be considered for both the HEGRA, Whipple and MILAGRO emission. Moreover, our multi-configuration VLA images reveal the non-thermal extended emission previously reported by us with improved angular resolution. Its non-thermal spectral index is also confirmed thanks to matching beam observations at the 20 and 6 cm wavelengths.

Deep GMRT radio observations and a multi-wavelength study of the region around HESS J1858+020

Context. There are a number of very high energy sources in the Galaxy that remain unidentified. Multi-wavelength and variability studies, and catalogue searches, are powerful tools to identify the physical counterpart, given the uncertainty in the source location and extension. Aims. This work carries out a thorough multi-wavelength study of the unidentified, very high energy source HESS J1858+020 and its environs. Methods. We have performed Giant Metrewave Radio Telescope observations at 610 MHz and 1.4 GHz to obtain a deep, low-frequency radio image of the region surrounding HESS J1858+020. We analysed archival radio, infrared, and X-ray data as well. This observational information, combined with molecular data, catalogue sources, and a nearby Fermi gamma-ray detection of unidentified origin, are combined to explore possible counterparts to the very high energy source. Results. We provide with a deep radio image of a supernova remnant that might be related to the GeV and TeV emission in the region. We confirm the presence of an H ii region next to the supernova remnant and coincident with molecular emission. A potential region of star formation is also identified. We identify several radio and X-ray sources in the surroundings. Some of these sources are known planetary nebulae, whereas others may be non-thermal extended emitters and embedded young stellar objects. Three old, background Galactic pulsars also neighbour HESS J1858+020 along the line of sight. Conclusions. The region surrounding HESS J1858+020 is rich in molecular structures and non-thermal objects that may potentially be linked to this unidentified very high energy source. In particular, a supernova remnant interacting with nearby molecular clouds may be a good candidate, but a star forming region, or a non-thermal radio source of yet unclear nature, may also be behind the gamma-ray source. The neighbouring pulsars, despite being old and distant, cannot be discarded as candidates. Further observational studies are needed, however, to narrow the search for a counterpart to the HESS source.

Characterization of the HIV protease inhibitor Nelfinavir cellular targets

The HIV protease inhibitors (HIV-PIs) are among the most potent antiviral drugs for the HIV infection. Treatment of patients with HIV-PIs has been linked with development of side effects including dyslipidemia, lipodystrophy syndrome and cardiovascular complications. Moreover, these drugs have shown anti-tumoral activity in non-infected patients but little is known about the involved molecular mechanism for these off-target effects. Here we propose that the HIV-PI Nelfinavir could block a cellular protease thus causing the observed phenotypes. We firstly focus our attention on a cellular protein, DDI2, showing sequence and structural conservation with the HIV protease. We applied cellular and in vitro approaches to produce a correctly folded recombinant protein in order to investigate the presence of a proteolytic activity. Despite the fact that we could identify two techniques that can be applied to produce a folded recombinant DDI2, no proteolytic activity has been identified in the present study. However, we could observe that decreasing the DDI2 levels recapitulated some phenotype observed in presence of HIV-PIs, including the phosphorylation of the protein translation regulators eIF2a and eEF2. As an alternative approach to identify cellular targets for HIV-PIs, we applied a proteomic screening called Slice-SILAC. We focused our attention on the defective maturation of Lamin A, a member of the nuclear lamina, induced by the block of the cellular protease Zmpste24. We demonstrated that Nelfinavir induced accumulation of Prelamin A and nuclear shape defects and in addition caused presence of cytosolic DNA, probably due to TREX1 downregulation. We showed that these phenotypes correlated with activation of the AIM2 inflammasome and IL-lß release. These findings suggest that DDI2 and Zmpste24 are direct or indirect cellular targets for the HIV-PIs and indicate a possible role for these proteins in promoting off-target effects and anti¬tumoral activity observed in HIV-PI treated patients. -- Les inhibiteurs de la protéase du VIH (IP-VIH) sont parmi les médicaments antiviraux les plus efficaces pour l'infection par le VIH. Le traitement des patients avec les IP-VIH cause des effets secondaires comprenant la dyslipidémie, le syndrome de lipodystrophie et les complications cardio-vasculaires. De plus, ces médicaments ont montré une activité anti-tumorale chez les patients non infectés, toutefois le mécanisme moléculaire impliqué dans ces effets hors-cible reste inconnu. Nous proposons que l'IP-VIH Nelfinavir puisse bloquer une protéase cellulaire provoquant les phénotypes observés. De ce fait, nous avons concentré notre attention sur une protéine cellulaire, DDI2, qui possède une séquence et une structure proche de celle de la protéase du VIH. Nous avons appliqué des approches cellulaire et in vitro pour produire une protéine recombinante correctement repliée afin d'étudier son activité protéolytique. Malgré le fait que nous avons pu identifier deux techniques qui peuvent être appliquées pour produire une protéine DDI2 recombinante correctement repliée, aucune activité protéolytique n'a été identifiée dans la présente étude. De plus, nous avons pu observer que la réduction de DDI2 récapitule les phénotypes observé avec le IP-VIH, y compris les phosphorylations de eIF2a et eEF2, impliquées dans la régulation de la traduction protéique. Une approche alternative, appelée Slice-SILAC, a été utilisée afin d'identifier de nouvelles cibles cellulaires du Nelfinavir. Nous avons concentré notre attention sur la maturation défectueuse de la Lamine A, un membre de la lamine nucléaire, induite par l'inhibition de la protéase cellulaire Zmpste24. Nous avons démontré que le Nelfinavir induit une accumulation de Prélamine A déformant la membrane nucléaire et la présence d'ADN cytosolique, probablement en raison de la régulation négative de TREX1. Nous avons montré que ces phénotypes causent l'activation de l'inflammasome AIM2 et la sécrétion d'IL-lß. Ces résultats suggèrent que DDI2 et Zmpste24 sont des cibles cellulaires pour les IP-VIH et indiquent un possible rôle pour ces protéines dans l'apparition d'effets secondaires ainsi que dans l'activité anti-tumorale observée chez les patients traités avec les IP-VIH.

Spontaneous cell polarization: Feedback control of Cdc42 GTPase breaks cellular symmetry.

Spontaneous polarization without spatial cues, or symmetry breaking, is a fundamental problem of spatial organization in biological systems. This question has been extensively studied using yeast models, which revealed the central role of the small GTPase switch Cdc42. Active Cdc42-GTP forms a coherent patch at the cell cortex, thought to result from amplification of a small initial stochastic inhomogeneity through positive feedback mechanisms, which induces cell polarization. Here, I review and discuss the mechanisms of Cdc42 activity self-amplification and dynamic turnover. A robust Cdc42 patch is formed through the combined effects of Cdc42 activity promoting its own activation and active Cdc42-GTP displaying reduced membrane detachment and lateral diffusion compared to inactive Cdc42-GDP. I argue the role of the actin cytoskeleton in symmetry breaking is not primarily to transport Cdc42 to the active site. Finally, negative feedback and competition mechanisms serve to control the number of polarization sites.