Évolution et transmission des savoir-faire céramiques au cours du Sylvicole (-1000 à 1550 de notre ère) : la station 3-avant de Pointe-du-Buisson (BhFl-1d), Haut-Saint-Laurent, Québec

La station 3-avant de Pointe-du-Buisson (Beauharnois, Haut-Saint-Laurent, Québec) représente la plus importante collection de récipients de terre cuite datant du Sylvicole moyen ancien (-400 à 500 de notre ère) dans le Nord-Est américain. De plus, on trouve sur ce site une série continue d’occupations couvrant l’ensemble de la période Sylvicole. En dépit de complications d’ordre stratigraphique (terreau homogène et pédoturbations), des concepts et des méthodes évolutionnaires tirés de la théorie de l’hérédité duelle sont appliqués à l’étude de cet assemblage. D’un point de vue anthropologique, que nous apprend l’étude de l’évolution et de la transmission des savoir-faire d’une technologie que nous assumons exclusivement féminine au cours de la période Sylvicole? L’auteur défend que l’archéologie évolutionnaire permet de détecter le contexte de la transmission, c’est-à-dire l’organisation socioéconomique des populations du passé. L’examen des traits stylistiques suggère que la sédentarisation estivale des bandes amérindiennes à partir du Sylvicole moyen tardif favorise une homogénéisation des productions céramiques dans un contexte virilocal qui est la conséquence d’une transmission de type conformiste opérant sur un axe horizontal (entre pairs). Cependant, le passage probable des tribus iroquoiennes à l’uxorilocalité et à la matrilinéarité à la fin du Sylvicole se traduit par une saisissante hétérogénéisation des pots, qui s’explique possiblement par une sélection de marqueurs identitaire d’ordre clanique (transmission verticale entre parents et descendants). L’étude des traits techno-fonctionnels indique une diversification de la vaisselle de terre cuite à mesure que les populations intensifient leurs expériences sur les cultigènes. Dans l’ensemble, cette évolution trahit une attention accrue conférée à la performance des pots en tant que récipients culinaires. Par ailleurs, le concours de la sériation et de datations AMS permet la reconnaisance d’un taxon « Sylvicole moyen moyen » caractérisé par une modification morphologique et décorative des vases. Une enquête comparative portant sur un échantillon de 27 sites archéologiques de l’horizon Pseudo-scallop-shell démontre que la variation populationnelle est structurée en fonction de la localisation des communautés dans un bassin hydrographique spécifique. Par conséquent, l’auteur soumet des pistes en vue de l’élaboration d’une taxonomie robuste et propre au Sylvicole moyen ancien et au Sylvicole moyen moyen. Enfin, des indices de natures diverses (archéologiques, paléoethnobotaniques, ethnolinguistiques, paléoanthropologiques, et d’autres issus de la génétique des populations) suggèrent une identité proto-algonquienne des bandes des deux sous-périodes susmentionnées.Station 3-avant at Pointe-du-Buisson (Beauharnois, Haut-Saint-Laurent, Quebec) has produced the most important collection of Early Middle Woodland (400 B.C. – A.D. 500) earthen ware in Northeastern North America. It also contains an uninterrupted sequence of occupations throughout the Woodland Period. Notwithstanding several stratigraphic complications (homogeneous soil and pedoturbations), evolutionary concepts and methods drawn from the Dual Inheritance Theory are applied to this assemblage. From an anthropological standpoint, what does the study of the evolution and the transmission of know-how pertaining to a Woodland period technology, which we assume to be exclusively feminine, tell us? The author defends that evolutionary archaeology may help detect the context of transmission, i.e. the socioeconomic organization of past populations. The examination of stylistic traits suggests that the progressive summertime sedentarization of amerindian bands, starting around the Late Middle Woodland period, favours a homogenization of ceramics in the context of virilocality, which is the consequence of a conformist-biased transmission operating on a horizontal axis (between peers). However, the probable transition to uxorilocality and to matrilinearity by Iroquoian tribes at the end of the Woodland Period manifests itself through an obvious heterogenization of ceramics, which is likely to reflect a form of cultural selection targeting clanic markers (vertical transmission between parents and offsprings). The study of techno-functional traits indicates a diversification of the ceramic tool-kit following an intensification of experimentation with cultigens. Overall, this evolution underlines a greater attention given to the performance of pots as culinary tools. Additionally, the recourse to seriation and AMS datation allows for the recognition of a Middle Middle Woodland taxon that is characterized by both morphological and decorative modifications of pots. A comparative analysis involving a sample of 27 archaeological sites belonging in the Pseudo-scallop-shell Horizon further demonstrates that the populational variation comprised within this dataset is structured according to the geographic localization of sites in specific drainages. Consequently, the author outlines guidelines for the elaboration of a proper taxonomy with respect to both Early Middle Woodland and Middle Middle Woodland taxa. Finally, arguments drawn from diverse fields (archaeology, palaeoethnobotany, ethnolinguistics, palaeonanthropology and population genetics) point towards a proto-algonquian identity for the aforementioned taxa

Variabilité stylistique des occupations du Sylvicole moyen ancien (400 av. n.è. – 500 de n.è.) sur la station 3-arrière de Pointe-du-Buisson : approche typologique

Ce mémoire porte sur la variabilité observée dans un assemblage, composé à la fois d’artéfacts lithiques et céramiques, représentatif de la plus grande collection archéologique dominée par une composante du Sylvicole moyen ancien connue au Québec. Les traits caractéristiques des poteries qui ont été transportées, abandonnées, et en partie manufacturées sur la station 3-arrière du complexe de Pointe-du-Buisson, sont appréhendés à travers une acception holistique de la notion de «style», qui inclut tous les aspects des attributs qu’elle couvre, à savoir les technologiques, les morphologiques, les décoratifs et les fonctionnels. Grâce à l’application d’une méthode typologique, une approche peu utilisée depuis plusieurs décennies, du moins dans le Nord-Est américain, et dont le mérite propre réside dans sa capacité à traiter l’artéfact dans son ensemble, des schémas comportementaux (cognitifs et procéduraux) visibles sur les tessons de bord décorés ont été mis en lumière. Ces derniers sont intimement liés aux techniques décoratives employées par les potières, et semblent s’être modifiés au fil du temps de la manière suivante : type «sigillé» précédant les types plus récents «repoussé» et «basculant». Une analyse comparative, basée sur un échantillon de sites localisés dans la région de Haut-Saint-Laurent et dans celles avoisinantes, a par ailleurs souligné d’importantes similarités entre l’assemblage céramique de la composante du Sylvicole moyen ancien de BhFl-1d’ et ceux des sites de Vieux-Pont (Estrie), d’Oka (rivière des Outaouais), de Pointe-du-Gouvernement (Haut-Richelieu) et de Winooski (aux abords du Lac Champlain dans le Vermont). Ces résultats appuient l’identification d’une manifestation culturelle qui est très étroitement connectée aux phases Canoe Point et Winooski de la tradition Point Peninsula. Résultant des conclusions susmentionnées, et d’autres issues d’enquêtes récentes, des considérations d’ordre taxonomique s’ensuivent. Bien qu’une refonte complète du taxon «Sylvicole moyen» soit prématurée, une critique de ce taxon s’avère nécessaire. Aussi des taxons tels que l’Early Horticultural Period de Snow ou le «Sylvicole initial» de Wright et Clermont sont discutés, dans la mesure où ils pourraient renvoyer à une définition plus générale, mais aussi peut-être plus fidèle, des caractéristiques anthropologiques propres aux populations qui ont vécu le long du Saint-Laurent et de ses tributaires depuis le Sylvicole inférieur jusqu’à la fin du Sylvicole moyen tardif.This thesis focuses on the variability observed within an assemblage, made up of lithic and ceramic artefacts, that is felt to be representative of the largest collection dominated by an Early Middle Woodland component known in Quebec. The characteristic traits of the pots transported, discarded, and partly manufactured on the station 3-arrière of the Pointe-du-Buisson complex, are apprehended via a holistic understanding of the notion of «style» which includes all aspects of the attributes it covers, i.e. technological, morphological, decorative and functional ones. Thanks to the application of a typological method, a long forsaken approach, at least in eastern north America, whose specific merit resides in its ability to treat the artefact as a whole, behavioural (cognitive and procedural) patterns visible on the decorated rim sherds have been identified. These are intimately related to the decorative techniques used by the makers, and seem to have changed through time as follows: «vertical or simple» type, preceding the more recent «push-pull» and «rocker-stamp» types. A comparative analysis, based on a sample of sites located in the Upper St-Lawrence and neighbouring regions, has also revealed great similarities between the ceramic assemblage of the Early Middle Woodland component of BhFl-1d’ and those of Vieux-Pont (Eastern Townships, QC), Oka (Ottawa River), Pointe-du-Gouvernement (Upper Richelieu) and Winooski (Lake Champlain area, Vermont) sites. These results argue for the existence of a cultural manifestation that is very closely related to both the Canoe Point and Winooski phases of the Point Peninsula tradition. Following the aforementioned conclusions and based on others resulting from recent inquiries, further taxonomic considerations have emerged. While a complete overhaul of the Middle Woodland pattern would be premature, rethinking this taxon appears necessary. Therefore, taxa such as Early Horticultural Period (Snow) or Initial Woodland (Wright, Clermont) are revived and discussed since they may prove to be useful in defining more general, but also maybe more appropriate, anthropological traits concerning the populations that lived along the Saint Lawrence River and its tributaries from the Early Woodland to the end of the Late Middle Woodland

The exceptionally powerful TeV gamma-ray emitters in the Large Magellanic Cloud

The Large Magellanic Cloud, a satellite galaxy of the Milky Way, has been observed with the High Energy Stereoscopic System (H.E.S.S.) above an energy of 100 billion electron volts for a deep exposure of 210 hours. Three sources of different types were detected: the pulsar wind nebula of the most energetic pulsar known N 157B, the radio-loud supernova remnant N 132D and the largest non-thermal X-ray shell - the superbubble 30 Dor C. The unique object SN 1987A is, surprisingly, not detected, which constrains the theoretical framework of particle acceleration in very young supernova remnants. These detections reveal the most energetic tip of a gamma-ray source population in an external galaxy, and provide via 30 Dor C the unambiguous detection of gamma-ray emission from a superbubble.Comment: Published in Science Magazine (Jan. 23, 2015). This ArXiv version has the supplementary online material incorporated as an appendix to the main pape

Constraints on axionlike particles with H.E.S.S. from the irregularity of the PKS 2155-304 energy spectrum

Axionlike particles (ALPs) are hypothetical light (sub-eV) bosons predicted in some extensions of the Standard Model of particle physics. In astrophysical environments comprising high-energy gamma rays and turbulent magnetic fields, the existence of ALPs can modify the energy spectrum of the gamma rays for a sufficiently large coupling between ALPs and photons. This modification would take the form of an irregular behavior of the energy spectrum in a limited energy range. Data from the H.E.S.S. observations of the distant BL Lac object PKS 2155-304 (z=0.116) are used to derive upper limits at the 95% C.L. on the strength of the ALP coupling to photons, ggammaa<2.1×10-11GeV-1 for an ALP mass between 15 and 60 neV. The results depend on assumptions on the magnetic field around the source, which are chosen conservatively. The derived constraints apply to both light pseudoscalar and scalar bosons that couple to the electromagnetic fieldFil: Medina, Maria Clementina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); ArgentinaFil: H.E.S. S. collaboration

Diffuse Galactic gamma-ray emission with H.E.S.S

Diffuse γ-ray emission is the most prominent observable signature of celestial cosmic-ray interactions at high energies. While already being investigated at GeV energies over several decades, assessments of diffuse γ-ray emission at TeV energies remain sparse. After completion of the systematic survey of the inner Galaxy, the H.E.S.S. experiment is in a prime position to observe large-scale diffuse emission at TeV energies. Data of the H.E.S.S. Galactic Plane Survey are investigated in regions off known γ-ray sources. Corresponding γ-ray flux measurements were made over an extensive grid of celestial locations. Longitudinal and latitudinal profiles of the observed γ-ray fluxes show characteristic excess emission not attributable to known γ-ray sources. For the first time large-scale γ-ray emission along the Galactic plane using imaging atmospheric Cherenkov telescopes has been observed. While the background subtraction technique limits the ability to recover modest variation on the scale of the H.E.S.S. field of view or larger, which is characteristic of the inverse Compton scatter-induced Galactic diffuse emission, contributions of neutral pion decay as well as emission from unresolved γ-ray sources can be recovered in the observed signal to a large fraction. Calculations show that the minimum γ-ray emission from π0 decay represents a significant contribution to the total signal. This detection is interpreted as a mix of diffuse Galactic γ-ray emission and unresolved sources

Probing the gamma-ray emission from HESS J1834-087 using H.E.S.S. and Fermi LAT observations

Aims. Previous observations with the High Energy Stereoscopic System (H.E.S.S.) have revealed an extended very-high-energy (VHE; E> 100 GeV) γ-ray source, HESS J1834−087, coincident with the supernova remnant (SNR) W41. The origin of the γ-ray emission was investigated in more detail with the H.E.S.S. array and the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope. Methods. The γ-ray data provided by 61 h of observations with H.E.S.S., and four years with the Fermi LAT were analyzed, covering over five decades in energy from 1.8 GeV up to 30 TeV. The morphology and spectrum of the TeV and GeV sources were studied and multiwavelength data were used to investigate the origin of the γ-ray emission toward W41. Results. The TeV source can be modeled with a sum of two components: one point-like and one significantly extended (σTeV = 0.17° ± 0.01°), both centered on SNR W41 and exhibiting spectra described by a power law with index ΓTeV ≃ 2.6. The GeV source detected with Fermi LAT is extended (σGeV = 0.15° ± 0.03°) and morphologically matches the VHE emission. Its spectrum can be described by a power-law model with an index ΓGeV = 2.15 ± 0.12 and smoothly joins the spectrum of the whole TeV source. A break appears in the γ-ray spectra around 100 GeV. No pulsations were found in the GeV range. Conclusions. Two main scenarios are proposed to explain the observed emission: a pulsar wind nebula (PWN) or the interaction of SNR W41 with an associated molecular cloud. X-ray observations suggest the presence of a point-like source (a pulsar candidate) near the center of the remnant and nonthermal X-ray diffuse emission that could arise from the possibly associated PWN. The PWN scenario is supported by the compatible positions of the TeV and GeV sources with the putative pulsar. However, the spectral energy distribution from radio to γ-rays is reproduced by a one-zone leptonic model only if an excess of low-energy electrons is injected following a Maxwellian distribution by a pulsar with a high spin-down power (>1037 erg s-1). This additional low-energy component is not needed if we consider that the point-like TeV source is unrelated to the extended GeV and TeV sources. The interacting SNR scenario is supported by the spatial coincidence between the γ-ray sources, the detection of OH (1720 MHz) maser lines, and the hadronic modeling

Discovery of the Hard Spectrum VHE γ-Ray Source HESS J1641-463

This Letter reports the discovery of a remarkably hard spectrum source, HESS J1641−463, by the High Energy Stereoscopic System (H.E.S.S.) in the very high energy (VHE) domain. HESS J1641−463 remained unnoticed by the usual analysis techniques due to confusion with the bright nearby source HESS J1640−465. It emerged at a significance level of 8.5 standard deviations after restricting the analysis to events with energies above 4 TeV. It shows a moderate flux level of phgr(E>1 TeV) = (3.64 ± 0.44stat ± 0.73sys) × 10−13 cm−2 s−1, corresponding to 1.8% of the Crab Nebula flux above the same energy, and a hard spectrum with a photon index of Γ = 2.07 ± 0.11stat ± 0.20sys. It is a point-like source, although an extension up to a Gaussian width of σ = 3 arcmin cannot be discounted due to uncertainties in the H.E.S.S. point-spread function. The VHE γ-ray flux of HESS J1641−463 is found to be constant over the observed period when checking time binnings from the year-by-year to the 28 minute exposure timescales. HESS J1641−463 is positionally coincident with the radio supernova remnant SNR G338.5+0.1. No X-ray candidate stands out as a clear association; however, Chandra and XMM-Newton data reveal some potential weak counterparts. Various VHE γ-ray production scenarios are discussed. If the emission from HESS J1641−463 is produced by cosmic ray protons colliding with the ambient gas, then their spectrum must extend close to 1 PeV. This object may represent a source population contributing significantly to the galactic cosmic ray flux around the knee

The 2010 very high energy gamma-ray flare & 10 years of multi-wavelength observations of M 87

Abridged: The giant radio galaxy M 87 with its proximity, famous jet, and very massive black hole provides a unique opportunity to investigate the origin of very high energy (VHE; E>100 GeV) gamma-ray emission generated in relativistic outflows and the surroundings of super-massive black holes. M 87 has been established as a VHE gamma-ray emitter since 2006. The VHE gamma-ray emission displays strong variability on timescales as short as a day. In this paper, results from a joint VHE monitoring campaign on M 87 by the MAGIC and VERITAS instruments in 2010 are reported. During the campaign, a flare at VHE was detected triggering further observations at VHE (H.E.S.S.), X-rays (Chandra), and radio (43 GHz VLBA). The excellent sampling of the VHE gamma-ray light curve enables one to derive a precise temporal characterization of the flare: the single, isolated flare is well described by a two-sided exponential function with significantly different flux rise and decay times. While the overall variability pattern of the 2010 flare appears somewhat different from that of previous VHE flares in 2005 and 2008, they share very similar timescales (~day), peak fluxes (Phi(>0.35 TeV) ~= (1-3) x 10^-11 ph cm^-2 s^-1), and VHE spectra. 43 GHz VLBA radio observations of the inner jet regions indicate no enhanced flux in 2010 in contrast to observations in 2008, where an increase of the radio flux of the innermost core regions coincided with a VHE flare. On the other hand, Chandra X-ray observations taken ~3 days after the peak of the VHE gamma-ray emission reveal an enhanced flux from the core. The long-term (2001-2010) multi-wavelength light curve of M 87, spanning from radio to VHE and including data from HST, LT, VLA and EVN, is used to further investigate the origin of the VHE gamma-ray emission. No unique, common MWL signature of the three VHE flares has been identified.Comment: 19 pages, 5 figures; Corresponding authors: M. Raue, L. Stawarz, D. Mazin, P. Colin, C. M. Hui, M. Beilicke; Fig. 1 lightcurve data available online: http://www.desy.de/~mraue/m87