999 resultados para Escriptors valencians-s. XIV-XVI-Bibliografies


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Mémoire numérisé par la Division de la gestion de documents et des archives de l'Université de Montréal

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Depuis les années 1980, les archéologues ont remarqué l'originalité des collections de céramiques trouvées sur des sites occupés par les pêcheurs basques au cours du XVIe au XVIIIe siècle sur les côtes atlantiques du Canada. Le site de Red Bay (Labrador) a été le premier à fournir une riche collection de terre cuites communes, majoliques et grès, qui ont permis aux archéologues de reconnaître une tradition céramique distincte. Pendant plus de deux siècles, ces céramiques constituent un fil conducteur qui montre la permanence des activités commerciales basques au Canada. En utilisant une approche mutualiste et comparative de quatre sites de pêche basque (Red Bay (1530-1580), Anse-à-la-Cave (1580-1630), Petit-Mécatina (1630-1713), Pabos (1713- 1760)) et leurs ports d’attache dans l’Europe atlantique, nous observons comment à partir du milieu du XVIe siècle, l’ensemble des céramiques se transforme d'un endroit à l’autre sans perdre son air distinctif jusqu'au début du XVIIIe siècle quand les témoins des céramiques basques changent radicalement. Finalement, une perspective globale qui relie les deux côtes atlantiques par le biais de ces matériaux céramiques nous aide à mieux connaître les réseaux d'approvisionnement liés aux traversées de pêche et l’espace économique complexe qui s’articule aux routes maritimes et de l’intérieur. Ces deux éléments se veulent essentiels à la compréhension de l'expansion outremers, ses materiaux laissés et son rôle dans l'économie mondiale au début de l'époque moderne.

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Cet essai aborde la Bible comme nourriture essentielle de l’expérience de foi chrétienne, en particulier chez les personnes engagées dans la formation à la vie chrétienne. On y explore les questions suivantes : Qu’est-ce que la Parole de Dieu ? Quel est le rapport entre la Bible et la Parole de Dieu ? Comment la Bible peut-elle nourrir l’expérience chrétienne aujourd’hui ? Quelles implications pour la formation à la vie chrétienne ? Après avoir exploré la perspective de l'exhortation Verbum, Domini du pape Benoît XVI sur ces questions, on fait appel aux réflexions de Sandra Schneiders dans Le texte de la rencontre (1991) avant de conclure par quelques remarques empruntées à Joël Molinario dans Parole de Dieu et Écriture en catéchèse (2011) et à André Fossion dans Dieu désirable (2010). Intervention lors des 8e Journées de réflexion en formation à la vie chrétienne de Montréal, tenues les 14-15 mars 2013 à l’Institut de pastorale des Dominicains.

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Study on variable stars is an important topic of modern astrophysics. After the invention of powerful telescopes and high resolving powered CCD’s, the variable star data is accumulating in the order of peta-bytes. The huge amount of data need lot of automated methods as well as human experts. This thesis is devoted to the data analysis on variable star’s astronomical time series data and hence belong to the inter-disciplinary topic, Astrostatistics. For an observer on earth, stars that have a change in apparent brightness over time are called variable stars. The variation in brightness may be regular (periodic), quasi periodic (semi-periodic) or irregular manner (aperiodic) and are caused by various reasons. In some cases, the variation is due to some internal thermo-nuclear processes, which are generally known as intrinsic vari- ables and in some other cases, it is due to some external processes, like eclipse or rotation, which are known as extrinsic variables. Intrinsic variables can be further grouped into pulsating variables, eruptive variables and flare stars. Extrinsic variables are grouped into eclipsing binary stars and chromospheri- cal stars. Pulsating variables can again classified into Cepheid, RR Lyrae, RV Tauri, Delta Scuti, Mira etc. The eruptive or cataclysmic variables are novae, supernovae, etc., which rarely occurs and are not periodic phenomena. Most of the other variations are periodic in nature. Variable stars can be observed through many ways such as photometry, spectrophotometry and spectroscopy. The sequence of photometric observa- xiv tions on variable stars produces time series data, which contains time, magni- tude and error. The plot between variable star’s apparent magnitude and time are known as light curve. If the time series data is folded on a period, the plot between apparent magnitude and phase is known as phased light curve. The unique shape of phased light curve is a characteristic of each type of variable star. One way to identify the type of variable star and to classify them is by visually looking at the phased light curve by an expert. For last several years, automated algorithms are used to classify a group of variable stars, with the help of computers. Research on variable stars can be divided into different stages like observa- tion, data reduction, data analysis, modeling and classification. The modeling on variable stars helps to determine the short-term and long-term behaviour and to construct theoretical models (for eg:- Wilson-Devinney model for eclips- ing binaries) and to derive stellar properties like mass, radius, luminosity, tem- perature, internal and external structure, chemical composition and evolution. The classification requires the determination of the basic parameters like pe- riod, amplitude and phase and also some other derived parameters. Out of these, period is the most important parameter since the wrong periods can lead to sparse light curves and misleading information. Time series analysis is a method of applying mathematical and statistical tests to data, to quantify the variation, understand the nature of time-varying phenomena, to gain physical understanding of the system and to predict future behavior of the system. Astronomical time series usually suffer from unevenly spaced time instants, varying error conditions and possibility of big gaps. This is due to daily varying daylight and the weather conditions for ground based observations and observations from space may suffer from the impact of cosmic ray particles. Many large scale astronomical surveys such as MACHO, OGLE, EROS, xv ROTSE, PLANET, Hipparcos, MISAO, NSVS, ASAS, Pan-STARRS, Ke- pler,ESA, Gaia, LSST, CRTS provide variable star’s time series data, even though their primary intention is not variable star observation. Center for Astrostatistics, Pennsylvania State University is established to help the astro- nomical community with the aid of statistical tools for harvesting and analysing archival data. Most of these surveys releases the data to the public for further analysis. There exist many period search algorithms through astronomical time se- ries analysis, which can be classified into parametric (assume some underlying distribution for data) and non-parametric (do not assume any statistical model like Gaussian etc.,) methods. Many of the parametric methods are based on variations of discrete Fourier transforms like Generalised Lomb-Scargle peri- odogram (GLSP) by Zechmeister(2009), Significant Spectrum (SigSpec) by Reegen(2007) etc. Non-parametric methods include Phase Dispersion Minimi- sation (PDM) by Stellingwerf(1978) and Cubic spline method by Akerlof(1994) etc. Even though most of the methods can be brought under automation, any of the method stated above could not fully recover the true periods. The wrong detection of period can be due to several reasons such as power leakage to other frequencies which is due to finite total interval, finite sampling interval and finite amount of data. Another problem is aliasing, which is due to the influence of regular sampling. Also spurious periods appear due to long gaps and power flow to harmonic frequencies is an inherent problem of Fourier methods. Hence obtaining the exact period of variable star from it’s time series data is still a difficult problem, in case of huge databases, when subjected to automation. As Matthew Templeton, AAVSO, states “Variable star data analysis is not always straightforward; large-scale, automated analysis design is non-trivial”. Derekas et al. 2007, Deb et.al. 2010 states “The processing of xvi huge amount of data in these databases is quite challenging, even when looking at seemingly small issues such as period determination and classification”. It will be beneficial for the variable star astronomical community, if basic parameters, such as period, amplitude and phase are obtained more accurately, when huge time series databases are subjected to automation. In the present thesis work, the theories of four popular period search methods are studied, the strength and weakness of these methods are evaluated by applying it on two survey databases and finally a modified form of cubic spline method is intro- duced to confirm the exact period of variable star. For the classification of new variable stars discovered and entering them in the “General Catalogue of Vari- able Stars” or other databases like “Variable Star Index“, the characteristics of the variability has to be quantified in term of variable star parameters.

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Todas las cartas se presentan en su idioma original (francés) y su traducción al castellano. - Contiene índice onomástico, de cartas, reseñas biográficas de personajes citados en la correspondencia y a modo de epílogo una reflexión sobre la Restauración Borbónica en España 175 años después

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Incluye conclusiones y propuestas de mejora

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La construcción territorial del reino de Murcia en la Edad Moderna constituye un tema transversal dentro del currículo regional de la Educación Secundaria Obligatoria (ESO) y Bachillerato, que ofrece la posibilidad de comprender cómo se fue formando aquella entidad político-cultural en los siglos modernos y las consecuencias administrativas que hoy presenta la Comunidad Autónoma de la Región de Murcia..

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Es presenta el dibuix d’un centre assistencial que ha crescut i canviat amb la seva ciutat: ahir a la vora de l’Onyar, avui a tocar de la Gran Via i demà a Salt, l’hospital encara es mostra lligat a les necessitats socials d’aquells qui li donen raó de ser, els ciutadans

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Repàs de la història dels certàmens literaris a Barcelona fins a l’entrada de l’època contemporània, des del s. XIV fins al XVIII

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Article que es refereix a la XVI Olimpíada Nacional de Química (2002 – 2003), celebrada el 9-12 de maig de 2003, al Seminari Menor de Tarazona (Saragossa). L’ olimpíada consisteix en dues proves: la primera consisteix en la resolució de 4 problemes llargs, i la segona en 45 preguntes de resposta múltiple (tipus test) que contenen qüestions teòriques i problemes curt. En aquest article s’ esmenten els alumnes que han obtingut alguna mena de distinció, els classificats per a la Fase Nacional, els problemes proposats i les característiques de les preguntes del test

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Estudi de l’obra de Benet Sanxes Galindo, conegut en castellà com Benito Sánchez Galindo. Poeta i pintor del s. XVI, ha estat poc conegut i estudiat. L’autor aprofita per fer un repàs de les obres que l’han tractat. L’article s’emmarca en un número monogràfic amb el títol “Miscel•lània d’homenatge a Modest Prats”

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L'articulació política del pla de Barcelona en l'època medieval es va basar en l'existència de dos territoris: d'una banda, una gran àrea que va coincidir amb la plana entre les desembocadures del Llobregat i del Besòs, on les autoritats locals exerciren alguna funció de control judicial. D'altra banda, un territori molt més petit, anomenat Hort i Vinyet (Parròquia de Sants i Sarrià Sant Martí Provençals), on la jurisdicció civil i penal del Consell de Cent era absoluta. L'objectiu d'aquest treball és mostrar, en primer lloc, que el territori anomenat Hort i Vinyet no existia i, d'altra banda, que l'extens territori no era subjecte a la jurisdicció municipal

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A l’article es pretén traçar una primera cronologia de l’evolució de les competències fiscals del municipi barceloní fins a la consolidació d’un veritable sistema fiscal. Més que conclusions definitives, el treball vol establir unes primeres hipòtesis dins d’una investigació pròpia en curs sobre la fiscalitat reial a la ciutat de Barcelona que, fins al moment, s’havia centrat sobretot en l’anàlisi del patrimoni reial

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Exposició de com foren vistos els pagesos per aquells que no ho eren durant l’època medieval i moderna, tot recollint els prejudicis i malentesos relacionats amb aquest punt de vista

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Aproximació al funcionament de la mostassafia barcelonina medieval, i a la creació d’un dret municipal encarregat de regular la vida ciutadana. Aquesta aproximació es fa a partir d’un aspecte relativament simple: el control de la qualitat de les espècies i les drogues. L’anàlisi de les ordinacions de mercaderies encamerades serveix per veure com els consellers aprofitaren la creació de la figura del mostassaf i l’establiment de les seves àmplies atribucions normatives per controlar l’activitat mercantil barcelonina