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Institution

Université libre de Bruxelles

EducationBrussels, Belgium
About: Université libre de Bruxelles is a education organization based out in Brussels, Belgium. It is known for research contribution in the topics: Population & Breast cancer. The organization has 24974 authors who have published 56969 publications receiving 2084303 citations. The organization is also known as: ULB.


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Journal ArticleDOI
TL;DR: Autocatalytic interactions between the members of an animal group or society, and particularly chemically or visually mediated allelomimesis, can be an important factor in the organisation of their collective activity.
Abstract: Autocatalytic interactions between the members of an animal group or society, and particularly chemically or visually mediated allelomimesis, can be an important factor in the organisation of their collective activity. Furthermore, the interactions between the individuals and the environment allow different collective patterns and decisions to appear under different conditions, with the same individual behaviour. While most clearly demonstrable in social insects, these principles are fundamental to schools of fishes, flocks of birds, groups of mammals, and many other social aggregates. The analysis of collective behaviour in these terms implies detailed observation of both individual and collective behaviour, combined with mathematical modelling to link the two.

699 citations

Journal ArticleDOI
23 Aug 2012-Nature
TL;DR: Surprisingly, it is found that the majority of labelled tumour cells in benign papilloma have only limited proliferative potential, whereas a fraction has the capacity to persist long term, giving rise to progeny that occupy a significant part of the tumour.
Abstract: Recent studies using the isolation of a subpopulation of tumour cells followed by their transplantation into immunodeficient mice provide evidence that certain tumours, including squamous skin tumours, contain cells with high clonogenic potential that have been referred to as cancer stem cells (CSCs). Until now, CSC properties have only been investigated by transplantation assays, and their existence in unperturbed tumour growth is unproven. Here we make use of clonal analysis of squamous skin tumours using genetic lineage tracing to unravel the mode of tumour growth in vivo in its native environment. To this end, we used a genetic labelling strategy that allows individual tumour cells to be marked and traced over time at different stages of tumour progression. Surprisingly, we found that the majority of labelled tumour cells in benign papilloma have only limited proliferative potential, whereas a fraction has the capacity to persist long term, giving rise to progeny that occupy a significant part of the tumour. As well as confirming the presence of two distinct proliferative cell compartments within the papilloma, mirroring the composition, hierarchy and fate behaviour of normal tissue, quantitative analysis of clonal fate data indicates that the more persistent population has stem-cell-like characteristics and cycles twice per day, whereas the second represents a slower cycling transient population that gives rise to terminally differentiated tumour cells. Such behaviour is shown to be consistent with double-labelling experiments and detailed clonal fate characteristics. By contrast, measurements of clone size and proliferative potential in invasive squamous cell carcinoma show a different pattern of behaviour, consistent with geometric expansion of a single CSC population with limited potential for terminal differentiation. This study presents the first experimental evidence for the existence of CSCs during unperturbed solid tumour growth.

698 citations

Journal ArticleDOI
Markus Ackermann, J. Ahrens1, Xinhua Bai2, M. Bartelt, S. W. Barwick3, R. C. Bay4, T. Becka1, J. K. Becker, K.-H. Becker5, P. Berghaus6, Elisa Bernardini, D. Bertrand6, D. J. Boersma7, S. Böser, Olga Botner8, Adam Bouchta8, Othmane Bouhali6, C.P. Burgess9, T. Burgess9, T. Castermans10, Dmitry Chirkin11, B. Collin12, Jan Conrad8, Jodi Cooley7, D. F. Cowen12, Anna Davour8, C. De Clercq13, C.P. de los Heros8, Paolo Desiati7, Tyce DeYoung12, P. Ekström9, T. Feser1, Thomas K. Gaisser2, R. Ganugapati7, Heiko Geenen5, L. Gerhardt3, A. Goldschmidt11, Axel Groß, Allan Hallgren8, Francis Halzen7, Kael Hanson7, D. Hardtke4, Torsten Harenberg5, T. Hauschildt2, K. Helbing11, M. Hellwig1, P. Herquet10, G. C. Hill7, Joseph T. Hodges7, D. Hubert13, B. Hughey7, P. O. Hulth9, K. Hultqvist9, S. Hundertmark9, Janet Jacobsen11, Karl-Heinz Kampert5, Albrecht Karle7, M. Kestel12, G. Kohnen10, L. Köpke1, Marek Kowalski, K. Kuehn3, R. Lang, H. Leich, Matthias Leuthold, I. Liubarsky14, Johan Lundberg8, James Madsen15, Pawel Marciniewski8, H. S. Matis11, C. P. McParland11, T. Messarius, Y. Minaeva9, P. Miocinovic4, R. Morse7, K. Münich, R. Nahnhauer, J. W. Nam3, T. Neunhöffer1, P. Niessen2, D. R. Nygren11, Ph. Olbrechts13, A. C. Pohl8, R. Porrata4, P. B. Price4, Gerald Przybylski11, K. Rawlins7, Elisa Resconi, Wolfgang Rhode, M. Ribordy10, S. Richter7, J. Rodríguez Martino9, H. G. Sander1, S. Schlenstedt, David A. Schneider7, R. Schwarz7, A. Silvestri3, M. Solarz4, Glenn Spiczak15, Christian Spiering, Michael Stamatikos7, D. Steele7, P. Steffen, R. G. Stokstad11, K. H. Sulanke, Ignacio Taboada4, O. Tarasova, L. Thollander9, S. Tilav2, Wolfgang Wagner, C. Walck9, M. Walter, Yi Wang7, C. H. Wiebusch5, R. Wischnewski, H. Wissing, Kurt Woschnagg4 
TL;DR: In this article, the authors used pulsed and continuous light sources embedded with the AMANDA neutrino telescope, an array of more than six hundred photomultiplier tubes buried deep in the ice.
Abstract: We have remotely mapped optical scattering and absorption in glacial ice at the South Pole for wavelengths between 313 and 560 nm and depths between 1100 and 2350 m. We used pulsed and continuous light sources embedded with the AMANDA neutrino telescope, an array of more than six hundred photomultiplier tubes buried deep in the ice. At depths greater than 1300 m, both the scattering coefficient and absorptivity follow vertical variations in concentration of dust impurities, which are seen in ice cores from other Antarctic sites and which track climatological changes. The scattering coefficient varies by a factor of seven, and absorptivity (for wavelengths less than ∼450 nm) varies by a factor of three in the depth range between 1300 and 2300 m, where four dust peaks due to stadials in the late Pleistocene have been identified. In our absorption data, we also identify a broad peak due to the Last Glacial Maximum around 1300 m. In the scattering data, this peak is partially masked by scattering on residual air bubbles, whose contribution dominates the scattering coefficient in shallower ice but vanishes at ∼1350 m where all bubbles have converted to nonscattering air hydrates. The wavelength dependence of scattering by dust is described by a power law with exponent -0.90 ± 0.03, independent of depth. The wavelength dependence of absorptivity in the studied wavelength range is described by the sum of two components: a power law due to absorption by dust, with exponent -1.08 ± 0.01 and a normalization proportional to dust concentration that varies with depth; and a rising exponential due to intrinsic ice absorption which dominates at wavelengths greater than ∼500 nm. Copyright 2006 by the American Geophysical Union.

697 citations

Journal ArticleDOI
Nasim Azani1, Marielle Babineau2, C. Donovan Bailey3, Hannah Banks4, Ariane R. Barbosa5, Rafael Barbosa Pinto6, James S. Boatwright7, Leonardo Maurici Borges8, Gillian K. Brown9, Anne Bruneau2, Elisa Silva Candido6, Domingos Cardoso10, Kuo-Fang Chung11, Ruth Clark4, Adilva de Souza Conceição, Michael D. Crisp12, Paloma Cubas13, Alfonso Delgado-Salinas14, Kyle G. Dexter, Jeff J. Doyle15, Jérôme Duminil16, Ashley N. Egan17, Manuel de la Estrella4, Marcus J. Falcao, Dmitry A. Filatov18, Ana Paula Fortuna-Perez19, Renee Hersilia Fortunato20, Edeline Gagnon2, Peter Gasson4, Juliana Gastaldello Rando21, Ana Maria Goulart de Azevedo Tozzi6, Bee F. Gunn12, David Harris22, Elspeth Haston22, Julie A. Hawkins23, Patrick S. Herendeen, Colin E. Hughes24, João Ricardo Vieira Iganci25, Firouzeh Javadi26, Sheku Alfred Kanu27, Shahrokh Kazempour-Osaloo28, Geoffrey C. Kite4, Bente B. Klitgaard4, Fabio J. Kochanovski6, Erik J. M. Koenen24, Lynsey Kovar3, Matt Lavin29, M. Marianne le Roux30, Gwilym P. Lewis4, Haroldo Cavalcante de Lima, Maria Cristina Lopez-Roberts5, Barbara A. Mackinder22, Vitor Hugo Maia31, Valéry Malécot32, Vidal de Freitas Mansano, Brigitte Marazzi, Sawai Mattapha23, Joseph T. Miller33, Chika Mitsuyuki26, Tania M. Moura34, Daniel J. Murphy4, Madhugiri Nageswara-Rao3, Bruno Nevado18, Danilo M. Neves4, Dario I. Ojeda16, R. Toby Pennington22, Darirn E. Prado35, Gerhard Prenner4, Luciano Paganucci de Queiroz5, Gustavo Ramos10, Fabiana L. Ranzato Filardi, Pétala Gomes Ribeiro5, María de Lourdes Rico-Arce4, Michael J. Sanderson36, Juliana Santos-Silva, Wallace M. B. São-Mateus37, Marcos J. S. Silva38, Marcelo F. Simon39, Carole Sinou2, Cristiane Snak5, Élvia R. de Souza, Janet I. Sprent40, Kelly P. Steele41, Julia E. Steier42, Royce Steeves2, Charles H. Stirton43, Shuichiro Tagane26, Benjamin M. Torke44, Hironori Toyama26, Daiane Trabuco da Cruz5, Mohammad Vatanparast17, Jan J. Wieringa45, Michael Wink46, Martin F. Wojciechowski42, Tetsukazu Yahara26, Ting-Shuang Yi47, Erin Zimmerman2 
01 Feb 2017-Taxon
TL;DR: The classification of the legume family proposed here addresses the long-known non-monophyly of the traditionally recognised subfamily Caesalpinioideae, by recognising six robustly supported monophyletic subfamilies and reflects the phylogenetic structure that is consistently resolved.
Abstract: The classification of the legume family proposed here addresses the long-known non-monophyly of the traditionally recognised subfamily Caesalpinioideae, by recognising six robustly supported monophyletic subfamilies. This new classification uses as its framework the most comprehensive phylogenetic analyses of legumes to date, based on plastid matK gene sequences, and including near-complete sampling of genera (698 of the currently recognised 765 genera) and ca. 20% (3696) of known species. The matK gene region has been the most widely sequenced across the legumes, and in most legume lineages, this gene region is sufficiently variable to yield well-supported clades. This analysis resolves the same major clades as in other phylogenies of whole plastid and nuclear gene sets (with much sparser taxon sampling). Our analysis improves upon previous studies that have used large phylogenies of the Leguminosae for addressing evolutionary questions, because it maximises generic sampling and provides a phylogenetic tree that is based on a fully curated set of sequences that are vouchered and taxonomically validated. The phylogenetic trees obtained and the underlying data are available to browse and download, facilitating subsequent analyses that require evolutionary trees. Here we propose a new community-endorsed classification of the family that reflects the phylogenetic structure that is consistently resolved and recognises six subfamilies in Leguminosae: a recircumscribed Caesalpinioideae DC., Cercidoideae Legume Phylogeny Working Group (stat. nov.), Detarioideae Burmeist., Dialioideae Legume Phylogeny Working Group (stat. nov.), Duparquetioideae Legume Phylogeny Working Group (stat. nov.), and Papilionoideae DC. The traditionally recognised subfamily Mimosoideae is a distinct clade nested within the recircumscribed Caesalpinioideae and is referred to informally as the mimosoid clade pending a forthcoming formal tribal and/or cladebased classification of the new Caesalpinioideae. We provide a key for subfamily identification, descriptions with diagnostic charactertistics for the subfamilies, figures illustrating their floral and fruit diversity, and lists of genera by subfamily. This new classification of Leguminosae represents a consensus view of the international legume systematics community; it invokes both compromise and practicality of use.

697 citations

Journal ArticleDOI
TL;DR: To understand the subclonal structure of primary breast cancer, whole-genome and targeted sequencing was applied to multiple samples from each of 50 patients' tumors, finding thatLandmarks of disease progression arose within detectable subclones of antecedent lesions.
Abstract: The sequencing of cancer genomes may enable tailoring of therapeutics to the underlying biological abnormalities driving a particular patient's tumor. However, sequencing-based strategies rely heavily on representative sampling of tumors. To understand the subclonal structure of primary breast cancer, we applied whole-genome and targeted sequencing to multiple samples from each of 50 patients' tumors (303 samples in total). The extent of subclonal diversification varied among cases and followed spatial patterns. No strict temporal order was evident, with point mutations and rearrangements affecting the most common breast cancer genes, including PIK3CA, TP53, PTEN, BRCA2 and MYC, occurring early in some tumors and late in others. In 13 out of 50 cancers, potentially targetable mutations were subclonal. Landmarks of disease progression, such as resistance to chemotherapy and the acquisition of invasive or metastatic potential, arose within detectable subclones of antecedent lesions. These findings highlight the importance of including analyses of subclonal structure and tumor evolution in clinical trials of primary breast cancer.

695 citations


Authors

Showing all 25206 results

NameH-indexPapersCitations
Karl J. Friston2171267217169
Yi Chen2174342293080
David Miller2032573204840
Jing Wang1844046202769
H. S. Chen1792401178529
Jie Zhang1784857221720
Jasvinder A. Singh1762382223370
D. M. Strom1763167194314
J. N. Butler1722525175561
Andrea Bocci1722402176461
Bradley Cox1692150156200
Marc Weber1672716153502
Hongfang Liu1662356156290
Guenakh Mitselmakher1651951164435
Yang Yang1642704144071
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
2023119
2022412
20213,195
20203,051
20192,751
20182,609