Cross-population radio galaxies as a test of the jet-accretion relationship

Radio galaxies (RGs) are extremely relevant in addressing important unknowns concerning the interaction among black hole accretion, radio jets, and the environment. In the classical scheme, their accretion rate and ejection of relativistic jets are directly linked: efficient accretion (HERG) is associated with powerful edge-brightened jets (FRIIs); inefficient accretion (LERG) is associated with weak edge-darkened jets (FRIs). The observation of RGs with an inefficient engine associated with edge-brightened radio emission (FRII-LERGs) broke this scheme. FRII-LERGs constitute a suitable population to explore how accretion and ejection are linked and evaluate the environment's role in shaping jets. To this aim, we performed a multiwavelength study of different RGs catalogs spanning from Jy to mJy flux densities. At first, we investigated the X-ray properties of a sample of 51 FRIIs belonging to the 3CR catalog at z<0.3. Two hypotheses were invoked to explain FRII-LERGs behavior: evolution from classical FRIIs; the role of the environment. Next, we explored the mJy sky by studying the optical-radio properties of hundreds of RGs at z<0.15 (Best & Heckman 2012 sample). FRII-LERGs appear more similar to the old FRI-LERGs than to the young FRII-HERGs. These results point towards an evolutive scenario, however, nuclear time scale changes, star population aging, and kpc-Mpc radio structure modification do not agree. The role of the Mpc environment was then investigated. The Wen et al. 2015 galaxy clusters sample, built exploiting the SDSS survey, allowed us to explore the habitat of 7219 RGs at z<0.3. Most RGs are found to live in outside clusters. For these sources, differences among RG classes are still present. Thus, the environment is not the key parameter, and the possibility of intrinsic differences was reconsidered: we speculated that different black hole properties (spin and magnetic field at its horizon) could determine the observed spread in jet luminosity.

Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse flux of tau neutrinos in the cosmic radiation. Earth-skimming nu(tau) may interact in the Earth's crust and produce a tau lepton by means of charged-current interactions. The tau lepton may emerge from the Earth and decay in the atmosphere to produce a nearly horizontal shower with a typical signature, a persistent electromagnetic component even at very large atmospheric depths. The search procedure to select events induced by tau decays against the background of normal showers induced by cosmic rays is described. The method used to compute the exposure for a detector continuously growing with time is detailed. Systematic uncertainties in the exposure from the detector, the analysis, and the involved physics are discussed. No tau neutrino candidates have been found. For neutrinos in the energy range 2x10(17) eV < E(nu)< 2x10(19) eV, assuming a diffuse spectrum of the form E(nu)(-2), data collected between 1 January 2004 and 30 April 2008 yield a 90% confidence-level upper limit of E(nu)(2)dN(nu tau)/dE(nu)< 9x10(-8) GeV cm(-2) s(-1) sr(-1).

The Fornax spectroscopic survey I. Survey strategy and preliminary results on the redshift distribution of a complete sample of stars and galaxies

The Fornax Spectroscopic Survey will use the Two degree Field spectrograph (2dF) of the Angle-Australian Telescope to obtain spectra for a complete sample of all 14000 objects with 16.5 less than or equal to b(j) less than or equal to 19.7 in a 12 square degree area centred on the Fornax Cluster. The aims of this project include the study of dwarf galaxies in the cluster (both known low surface brightness objects and putative normal surface brightness dwarfs) and a comparison sample of background field galaxies. We will also measure quasars and other active galaxies, any previously unrecognised compact galaxies and a large sample of Galactic stars. By selecting all objects-both stars and galaxies-independent of morphology, we cover a much larger range of surface brightness and scale size than previous surveys. In this paper we first describe the design of the survey. Our targets are selected from UK Schmidt Telescope sky survey plates digitised by the Automated Plate Measuring (APM) facility. We then describe the photometric and astrometric calibration of these data and show that the APM astrometry is accurate enough for use with the 2dF. We also describe a general approach to object identification using cross-correlations which allows us to identify and classify both stellar and galaxy spectra. We present results from the first 2dF field. Redshift distributions and velocity structures are shown for all observed objects in the direction of Fornax, including Galactic stars? galaxies in and around the Fornax Cluster, and for the background galaxy population. The velocity data for the stars show the contributions from the different Galactic components, plus a small tail to high velocities. We find no galaxies in the foreground to the cluster in our 2dF field. The Fornax Cluster is clearly defined kinematically. The mean velocity from the 26 cluster members having reliable redshifts is 1560 +/- 80 km s(-1). They show a velocity dispersion of 380 +/- 50 km s(-1). Large-scale structure can be traced behind the cluster to a redshift beyond z = 0.3. Background compact galaxies and low surface brightness galaxies are found to follow the general galaxy distribution.

A catalog of HI-selected galaxies from the south celestial cap region of sky

The first deep catalog of the H I Parkes All Sky Survey (HIPASS) is presented, covering the south celestial cap (SCC) region. The SCC area is similar to2400 deg(2) and covers delta < -62&DEG;. The average rms noise for the survey is 13 mJy beam(-1). Five hundred thirty-six galaxies have been cataloged according to their neutral hydrogen content, including 114 galaxies that have no previous cataloged optical counterpart. This is the largest sample of galaxies from a blind H I survey to date. Most galaxies in optically unobscured regions of sky have a visible optical counterpart; however, there is a small population of low-velocity H I clouds without visible optical counterparts whose origins and significance are unclear. The rms accuracy of the HIPASS positions is found to be 1.'9. The H I mass range of galaxies detected is from &SIM;10(6) to &SIM;10(11) M-.. There are a large number of late-type spiral galaxies in the SCC sample (66%), compared with 30% for optically selected galaxies from the same region in the NASA Extragalactic Database. The average ratio of H I mass to B luminosity of the sample increases according to optical type, from 1.8 M-./L-. for early types to 3.2 M-./L-. for late-type galaxies. The H I-detected galaxies tend to follow the large-scale structure traced by galaxies found in optical surveys. From the number of galaxies detected in this region of sky, we predict the full HIPASS catalog will contain &SIM;5000 galaxies, to a peak flux density limit of &SIM;39 mJy (3 σ), although this may be a conservative estimate as two large voids are present in the region. The H I mass function for this catalog is presented in a subsequent paper.

The 1000 brightest HIPASS galaxies: Newly cataloged galaxies

The H I Parkes All-Sky Survey (HIPASS) is a blind 21 cm survey for extragalactic neutral hydrogen, covering the whole southern sky. The HIPASS Bright Galaxy Catalog (BGC) is a subset of HIPASS and contains the 1000 H I brightest (peak flux density) galaxies. Here we present the 138 HIPASS BGC galaxies that had no redshift measured prior to the Parkes multibeam H I surveys. Of the 138 galaxies, 87 are newly cataloged. Newly cataloged is defined as having no optical ( or infrared) counterpart in the NASA/IPAC Extragalactic Database. Using the Digitized Sky Survey, we identify optical counterparts for almost half of the newly cataloged galaxies, which are typically of irregular or Magellanic morphological type. Several H I sources appear to be associated with compact groups or pairs of galaxies rather than an individual galaxy. The majority ( 57) of the newly cataloged galaxies lie within 10degrees of the Galactic plane and are missing from optical surveys as a result of confusion with stars or dust extinction. This sample also includes newly cataloged galaxies first discovered by Henning et al. in the H I shallow survey of the zone of avoidance. The other 30 newly cataloged galaxies escaped detection because of their low surface brightness or optical compactness. Only one of these, HIPASS J0546-68, has no obvious optical counterpart, as it is obscured by the Large Magellanic Cloud. We find that the newly cataloged galaxies with -b->10degrees are generally lower in H I mass and narrower in velocity width compared with the total HIPASS BGC. In contrast, newly cataloged galaxies behind the Milky Way are found to be statistically similar to the entire HIPASS BGC. In addition to these galaxies, the HIPASS BGC contains four previously unknown H I clouds.

CALIBRATION AND USE OF AN IN-HOUSE ANTI-MEASLES IgG STANDARD SERUM

For the purpose of research a large quantity of anti-measles IgG working reference serum was needed. A pool of sera from five teenagers was prepared and named Alexandre Herculano (AH). In order to calibrate the AH serum, 18 EIA assays were performed testing in parallel AH and the 2nd International Standard 1990, Anti-Measles Antibody, 66/202 (IS) in a range of dilutions (from 1/50 to 1/25600). A method which compared parallel lines resulting from the graphic representation of the results of laboratory tests was used to estimate the power of AH relative to IS. A computer programme written by one of the authors was used to analyze the data and make potency estimates. Another method of analysis was used, comparing logistic curves relating serum concentrations with optical density by EIA. For that purpose an existing computer programme (WRANL) was used. The potency of AH relative to IS, by either method, was estimated to be 2.4. As IS has 5000 milli international units (mIU) of anti-measles IgG per millilitre (ml), we concluded that AH has 12000 mIU/ml.

Search for very high energy Gamma radiation from the Starburst Galaxy IC 342

This thesis describes a search for very high energy (VHE) gamma-ray emission from the starburst galaxy IC 342. The analysis was based on data from the 2003 — 2004 observing season recorded using the Whipple 10-metre imaging atmospheric Cherenkov telescope located on Mount Hopkins in southern Arizona. IC 342 may be classed as a non-blazar type galaxy and to date only a few such galaxies (M 87, Cen A, M 82 and NGC 253) have been detected as VHE gamma-ray sources. Analysis of approximately 24 hours of good quality IC 342 data, consisting entirely of ON/OFF observations, was carried out using a number of methods (standard Supercuts, optimised Supercuts, scaled optimised Supercuts and the multivariate kernel analysis technique). No evidence for TeV gamma-ray emission from IC 342 was found. The significance was 0.6 a with a nominal rate of 0.04 ± 0.06 gamma rays per minute. The flux upper limit above 600 GeV (at 99.9 % confidence) was determined to be 5.5 x 10-8 m-2 s-1, corresponding to 8 % of the Crab Nebula flux in the same energy range.

Chronic Stress Improves NO- and Ca2+ Flux-Dependent Vascular Function: A Pharmacological Study

Background: Stress is associated with cardiovascular diseases. Objective: This study aimed at assessing whether chronic stress induces vascular alterations, and whether these modulations are nitric oxide (NO) and Ca2+ dependent. Methods: Wistar rats, 30 days of age, were separated into 2 groups: control (C) and Stress (St). Chronic stress consisted of immobilization for 1 hour/day, 5 days/week, 15 weeks. Systolic blood pressure was assessed. Vascular studies on aortic rings were performed. Concentration-effect curves were built for noradrenaline, in the presence of L-NAME or prazosin, acetylcholine, sodium nitroprusside and KCl. In addition, Ca2+ flux was also evaluated. Results: Chronic stress induced hypertension, decreased the vascular response to KCl and to noradrenaline, and increased the vascular response to acetylcholine. L-NAME blunted the difference observed in noradrenaline curves. Furthermore, contractile response to Ca2+ was decreased in the aorta of stressed rats. Conclusion: Our data suggest that the vascular response to chronic stress is an adaptation to its deleterious effects, such as hypertension. In addition, this adaptation is NO- and Ca2+-dependent. These data help to clarify the contribution of stress to cardiovascular abnormalities. However, further studies are necessary to better elucidate the mechanisms involved in the cardiovascular dysfunction associated with stressors. (Arq Bras Cardiol. 2014; [online].ahead print, PP.0-0)

Calibration of CES functions for real-world multisectoral modeling

We show how to calibrate CES production and utility functions when indirect taxation affecting inputs and consumption is present. These calibrated functions can then be used in computable general equilibrium models. Taxation modifies the standard calibration procedures since any taxed good has two associated prices and a choice of reference value units has to be made. We also provide an example of computer code to solve the calibration of CES utilities under two alternate normalizations. To our knowledge, this paper fills a methodological gap in the CGE literature.

Calibración TLR y LRM en MATLAB para medidas con guías de onda

En este proyecto, lo primero que hemos hecho ha sido desarrollar un algoritmo en Matlab que implementara el método de calibración TRL, el funcionamiento del cual hemos comprobado en primera instancia mediante simulaciones y, posteriormente, mediante un ejemplo real. Posteriormente, hemos desarrollado otro algoritmo en Matlab para implementar el método de calibración LRM. Este algoritmo sólo lo hemos podido comprobar a nivel de simulación. A continuación, mediante los dos algoritmos, hemos realizado una comparación entre ambos sistemas de calibración a través de simulaciones. Finalmente, analizando los resultados de varias simulaciones calibradas con nuestro programa del método TRL, hemos buscado cuáles pueden ser los motivos para la aparición de picos indeseados y hemos encontrado uno de ellos.

Caracterització d'oscil·ladors basats en CMOS-M/NEMS i la seva aplicació com a sensors de massa

El present projecte tracta sobre la caracterització d'oscil·ladors basats en ressonadors micro/nanoelectromecànics (M/NEMS) i la seva aplicació com a sensors de massa. Els oscil·ladors utilitzats es basen en un pont i una palanca ressoants M/NEMS, integrats en tecnologia CMOS. En primer lloc s'ha fet una introducció teòrica als conceptes utilitzats per a entendre el funcionament i la caracterització dels dispositius. A continuació s'han realitzat proves per tal de caracteritzar els paràmetres importants per a l'ús dels oscil·ladors com a sensors de massa, com la seva estabilitat en freqüència. Per acabar s'han aplicat aquests sensors en la caracterització i modelització del flux de massa a través d'obertures de dimensions micromètriques.

Implicacions del factor tissular en l'activació plaquetària: mecanismes d'acció

La formació de trombus està mediada per dos sistemes paral•lels: el sistema de la coagulació i agregació plaquetària. El prinicipal inciador de la cascada de la coagulació in vivo és el factor tissular (FT). La hipòtesi del present treball és que el FT és capaç d’induir agregació i activació plaquetària independentment del seu paper en la coagulació. Mitjançant estudis d’agregació hem vist que el FT indueix activació i agregació plaquetària. A més també hem pogut veure que en un sistema que simula el flux sanguini, les plaquetes són capaces d’adherir-se a una superfície coberta per FT, de manera similar al que s’espera en una placa ateroscleròtica trencada. Hem trobat que el FT indueix activació plaquetària per vies de senyalització que involucren la PKC, PI3K, tirosin quinases i Ser/Tre fosfatases. Per últim hem generat una línia cel•lular que expressa FT a la membrana. Aquesta línia cel•lular permetrà futurs estudis de la funció del FT en la seva forma nativa, és a dir, com a proteïna transmembrana enlloc de proteïna soluble purificada. En resum, aquests estudis han permès veure com el FT és capaç d’activar directament les plaquetes i induir la seva agregació jugant així un doble paper en els mecanismes de trombosi i hemostàsia.

Comparació dels sistemes "ribosome skipping" i "splicing acceptor" per a l'expressió de transgenes en adenovirus oncolítics

Report for the scientific sojourn carried out at the University of St. Andrews, United Kingdom, from November 2007 until January 2008. Therapeutic transgene expression is a valuable strategy to counteract the limitations associated with oncolytic adenoviruses. Late phase expression is desirable to avoid early cell death for proper virus production. In this 3 months-collaboration, we have constructed a late expression system based on ribosome skipping downstream fiber protein and compared it with a splicing-based method of late gene expression. Despite expressing high amounts of the transgene when utilizing the ribosome skipping-system, flow cytomety assays indicate a delayed transgene-expression kinetics compared with the splicing-based one. Furthermore, when using the ribosome skipping system not only fiber protein expression is more altered but also viral production. These results suggest splicing-based expression strategy as a more suitable system for expression of transgenes late in the viral life cycle of an oncolytic adenovirus.

Identificació de noves dianes terapèutiques en neoplàsies limfoides

El limfoma de cèl•lules de mantell (LCM) és un limfoma de cèl•lules B incurable que presenta sobreexpressió de ciclina D1. Això fa necessari el desenvolupament de noves teràpies. Els gens supressors de tumors estan alterats en càncer pel silenciament epigenètic aberrant, com a conseqüència de la desacetilació de les histones dels seus promotors. Els inhibidors de les desacetilases d'histones (HDACi) són nous compostos amb resultats prometedors per al tractament de tumors. L'objectiu principal, i que ha durat 7 mesos, va ser analitzar l'activitat antitumoral de l'àcid hidroxàmic suberoilanílid (SAHA, vorinostat), un HDACi en fase d'assajos clínics per al tractament de varis tumors, en cèl•lules de LCM. Es va analitzar la sensibilitat al SAHA (Merck Pharmaceuticals) en nou línies cel•lulars humanes de LCM, que es diferenciaven en les alteracions genètiques, les característiques replicatives i la sensibilitat als fàrmacs; i cèl•lules primàries de 6 pacients. El SAHA va presentar un efecte citotòxic heterogeni amb DL50 (Dosi Letal 50) de 3.25 μM a &25 μM amb 24 d'incubació. Aquest efecte citotòxic s'incrementava notablement després de 48 hores d'incubació assolint una DL50 de 0.34 a 5.69 μM. Cal destacar que 5 dels 6 casos de les mostres primàries de LCM van mostrar una elevada sensibilitat (DL50 & 8.07 μM). A nivell mecanistic, el SAHA va augmentar l'acetilació de les histones H3 i H4, i va disminuir els nivells de proteïna de la ciclina D1 i c-Flip. La citometria de flux i els anàlisis per Western Blot van posar de manifest que l'efecte citotòxic del SAHA es dóna a través de l'activació de la via mitocondrial de mort cel•lular i la cascada de caspases. El SAHA indueix l'expressió transcripcional de la proteïna proapoptòtica Bmf. Aquests resultats suggereixen que el SAHA podria ser una nova teràpia prometedora per al tractament del LCM.

Plan de gestión de energías renovables en el Monasterio Sakya Tashi Ling del Garraf

En el presente estudio se han analizado las posibilidades de reducción del impacto ambiental que genera el consumo de energía en el Monasterio budista Sakya Tashi Ling del Parque del Garraf, mediante la mejora de la eficiencia energética de los edificios y la producción de la energía consumida a partir de fuentes de energía renovables. Se ha realizado un inventario exhaustivo de los flujos energéticos de entrada del Monasterio: electricidad y combustibles fósiles, y el análisis de estos datos ha permitido observar que la mayor parte del consumo energético del Monasterio tiene como uso final la iluminación. El consumo total de energía se ha cuantificado en 138 kWh/m2/año y la emisiones de CO2 en 177 kg CO2/m2/año. A partir de estos datos se ha estudiado la posibilidad de reducir el consumo y abastecer la demanda energética del Monasterio a través de fuentes de energía renovable como las placas solares fotovoltaicas o las calderas de biomasa. Para alcanzar este objetivo se han propuesto tres escenarios posibles con costes económicos y resultados muy distintos. A diferencia de los escenarios “Edificio Energía Plus” y “Edificio Energía 0”, el tercer escenario propuesto, que trataba de alcanzar el triple objetivo del Plan 20/20/20 (producir a partir de fuentes renovables el 20% de la energía consumida, aumentar en una 20% la eficiencia energética y reducir en un 20% las emisiones de CO2 derivadas del uso de la energía) ha resultado ser muy viable económicamente: la inversión necesaria se amortizaría en tan sólo 5 años.