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University of Bordeaux

EducationBordeaux, France
About: University of Bordeaux is a education organization based out in Bordeaux, France. It is known for research contribution in the topics: Population & Laser. The organization has 28811 authors who have published 55536 publications receiving 1619635 citations. The organization is also known as: UB.


Papers
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Journal ArticleDOI
TL;DR: Factors involved in Bax conformational change and the function(s) of the distinct domains controlling the addressing and the insertion of Bax into mitochondria are described in this review.

252 citations

Journal ArticleDOI
TL;DR: By working at the level of expressions, a notion of graph rewriting is derived which is as powerful as the usual one (based on a categorical approach) introduced by Ehrig, Pfender, and Schneider.
Abstract: We define an algebraic structure for the set of finite graphs, a notion of graph expression for defining them, and a complete set of equational rules for manipulating graph expressions. (By agraph we mean an oriented hypergraph, the hyperedges of which are labeled with symbols from a fixed finite ranked alphabet and that is equipped with a finite sequence of distinguished vertices). The notion of a context-free graph grammar is introduced (based on the substitution of a graph for a hyperedge in a graph). The notion of an equational set of graphs follows in a standard way from the algebraic structure. As in the case of context-free languages, a set of graphs is contextfree iff it is equational. By working at the level of expressions, we derive from the algebraic formalism a notion of graph rewriting which is as powerful as the usual one (based on a categorical approach) introduced by Ehrig, Pfender, and Schneider.

252 citations

Journal ArticleDOI
TL;DR: In this article, the authors presented a compact source catalogue extracted from the APEX Telescope Large Area Survey of the GALaxy (ATLASGAL), which provides an unbiased database of dusty clumps in the inner Galaxy.
Abstract: Context. The APEX Telescope Large Area Survey of the GALaxy (ATLASGAL) is the first systematic survey of the inner Galactic plane in the sub-millimetre. The observations were carried out with the Large APEX Bolometer Camera (LABOCA), an array of 295 bolometers observing at 870 μ m (345 GHz). Aims. Here we present a first version of the compact source catalogue extracted from this survey. This catalogue provides an unbiased database of dusty clumps in the inner Galaxy. Methods. The construction of this catalogue was made using the source extraction routine SExtractor. We have cross-associated the obtained sources with the IRAS and MSX catalogues, in order to constrain their nature.Results. We have detected 6639 compact sources in the range from 330 ≤ l ≤ 21 degrees and |b | ≤ 1.5 degrees. The catalogue has a 99% completeness for sources with a peak flux above 6σ , which corresponds to a flux density of ~0.4 Jy beam-1 . The parameters extracted for sources with peak fluxes below the 6σ completeness threshold should be used with caution. Tests on simulated data find the uncertainty in the flux measurement to be ~12%, however, in more complex regions the flux values can be overestimated by a factor of 2 due to the additional background emission. Using a search radius of 30′′ we found that 40% of ATLASGAL compact sources are associated with an IRAS or MSX point source, but, ~50% are found to be associated with MSX 21 μ m fluxes above the local background level, which is probably a lower limit to the actual number of sources associated with star formation. Conclusions. Although infrared emission is found towards the majority of the clumps detected, this catalogue is still likely to include a significant number of clumps that are devoid of star formation activity and therefore excellent candidates for objects in the coldest, earliest stages of (high-mass) star formation.

252 citations

Journal ArticleDOI
TL;DR: The need for further inquiry into the relationship between climate and demographic/cultural change is demonstrated in order to better understand the mechanisms of cultural transmission at work in Neanderthals and early Homo sapiens populations.
Abstract: Crucial questions in the debate on the origin of quintessential human behaviours are whether modern cognition and associated innovations are unique to our species and whether they emerged abruptly, gradually or as the result of a discontinuous process. Three scenarios have been proposed to account for the origin of cultural modernity. The first argues that modern cognition is unique to our species and the consequence of a genetic mutation that took place approximately 50 ka in Africa among already evolved anatomically modern humans. The second posits that cultural modernity emerged gradually in Africa starting at least 200 ka in concert with the origin of our species on that continent. The third states that innovations indicative of modern cognition are not restricted to our species and appear and disappear in Africa and Eurasia between 200 and 40 ka before becoming fully consolidated. We evaluate these scenarios in the light of new evidence from Africa, Asia and Europe and explore the mechanisms that may have led to modern cultures. Such reflections will demonstrate the need for further inquiry into the relationship between climate and demographic/cultural change in order to better understand the mechanisms of cultural transmission at work in Neanderthals and early Homo sapiens populations.

252 citations

Journal ArticleDOI
A. Abramowski1, Fabio Acero2, Felix Aharonian3, Felix Aharonian4  +207 moreInstitutions (28)
TL;DR: In this article, the authors measured the imprint of the EBL opacity to gamma-rays on the spectra of the brightest extragalactic sources detected with the High Energy Stereoscopic System (H.E.S.).
Abstract: The extragalactic background light (EBL) is the diffuse radiation with the second highest energy density in the Universe after the cosmic microwave background. The aim of this study is the measurement of the imprint of the EBL opacity to gamma-rays on the spectra of the brightest extragalactic sources detected with the High Energy Stereoscopic System (H.E.S.S.). The originality of the method lies in the joint fit of the EBL optical depth and of the intrinsic spectra of the sources, assuming intrinsic smoothness. Analysis of a total of ~10^5 gamma-ray events enables the detection of an EBL signature at the 8.8 std dev level and constitutes the first measurement of the EBL optical depth using very-high energy (E>100 GeV) gamma-rays. The EBL flux density is constrained over almost two decades of wavelengths (0.30-17 microns) and the peak value at 1.4 micron is derived as 15 +/- 2 (stat) +/- 3 (sys) nW / m^2 sr.

252 citations


Authors

Showing all 28995 results

NameH-indexPapersCitations
Nicholas G. Martin1921770161952
George F. Koob171935112521
Daniel J. Jacob16265676530
Arthur W. Toga1591184109343
James M. Tour14385991364
Floyd E. Bloom13961672641
Herbert Y. Meltzer137114881371
Jean-Marie Tarascon136853137673
Stanley Nattel13277865700
Michel Haïssaguerre11775762284
Liquan Chen11168944229
Marion Leboyer11077350767
Jean-François Dartigues10663146682
Alexa S. Beiser10636647457
Robert Dantzer10549746554
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
202378
2022393
20213,110
20203,362
20193,245
20183,143