cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Thermoresponsive oil-continous bigels from interpenetrating colloidal particle networks
Creators: name: Macias-Rodriguez, Braulio
name: Gouzy, Roland
name: Coulais, Corentin
name: Velikov, Krassimir
Publisher: name: Zenodo
Year: 2021
Subjects: bigels, apolar, mechanics, silica, lipid

description: Gels comprising binary mixtures of polymers or particles are promising routes to soft materials with vastly improved properties. Recent work has shown the assembly of bigels or double network gels in polar environments; yet the realization of similar systems in apolar solvents has remained elusive. We present a new class of thermo-responsive oil-continuous bigels, formed by sequential assembly of sphere-like silica and platelet-like lipid colloidal particles with short-range attractions, into two discrete percolated gel networks as visualized by confocal microscopy. The ease-of-assembly make bigels suitable for fabrication of 3D-printed soft constructs. Depending on mixture composition, bigels can vastly stiffen, exceeding the elasticity predicted by the sum of the monogels’ elastic moduli by up to an order of magnitude, and toughen, bearing larger strains/stresses prior to induce yielding or material fluidization. The unusual mechanics suggest shear-activated cooperative effects, seemingly arising from mutual steric hindrance and restricted particle mobility due to interpenetration of gel networks.
description: Manuscript form under review
Gas density and X-ray surface brightness profiles of clusters of galaxies from dark matter halo potentials: beyond the isothermal beta model
Creators: name: Suto, Yasushi
name: Sasaki, Shin
name: Makino, Nobuyoshi
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe a theoretical framework to compute the cluster gas distribution in hydrostatic equilibrium embedded in a class of spherical dark matter halo potentials. Unlike the conventional isothermal $β$-model, the present method provides a physical basis to directly probe the shape of dark matter halo from the observed X-ray surface brightness and temperature profiles of clusters of galaxies. Specifically, we examine the extent to which the resulting gas density and X-ray surface brightness profiles are sensitive to the inner slope of the dark matter halo density and other more realistic effects including the self-gravity of the gas and the polytropic equation of state. We also discuss a practical strategy to apply the present methodology to the actual cluster profiles from future X-ray observations.
description: 19 pages, accepted for publication in ApJ, Part 1
Rumex acetosa Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex acetosa

description: Rumex acetosa Linnaeus, Species Plantarum 1: 337. 1753, nom. cons.
"Habitat in Europae pascuis. δ in Alpibus." RCN: 2602.
Conserved type (Jonsell & Nilsson in Taxon 45: 131. 1996): Sweden. Södermanland, Salem, Wiksberg, Jonsell 7110 (UPS; iso- BM, C, H, K, LD, O, S).
Current name: Rumex acetosa L. (Polygonaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 803, DOI: 10.5281/zenodo.291971
Digging Down to the Deep Story: Understanding the Views and Experiences of Aboriginal and Torres Strait Islander Women who Gave Birth during the Baggarrook Yurrongi Project in Naarm, Victoria.
Creators: name: McCalman, Pamela
Publisher: name: La Trobe
Year: 2025
Subjects: classificationCode: 420402
subject: Models of care and place of birth
classificationCode: 420403
subject: Psychosocial aspects of childbirth and perinatal mental health
classificationCode: 420401
subject: Clinical midwifery
classificationCode: 450413
subject: Aboriginal and Torres Strait Islander midwifery and paediatrics
classificationCode: 450414
subject: Aboriginal and Torres Strait Islander mothers and babies health and wellbeing

description: Submitted in total fulfillment of the requirements for the degree of Doctor of Philosophy to the School of Nursing and Midwifery, La Trobe University, Victoria, Australia.
$O(D,D)$-constraint on $D$-dimensional effective actions
Creators: name: Garousi, Mohammad R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Double Field Theory is a manifestly T-duality invariant formulation of string theory in which the effective theory at any order of $α'$ is invariant under global $O(D,D)$ transformations and ought to be invariant under gauge transformations which receive $α'$-corrections. On the other hand, the effective theory in the usual $D$-dimensional formulation of string theory is manifestly gauge invariant and ought to be invariant under T-duality transformations which receive $α'$-corrections. We speculate that the combination of these two constraints may fix both the $2D$-dimensional and the $D$-dimensional effective actions without knowledge of the $α'$-corrections of the gauge and the T-duality transformations. In this paper, using generalized fluxes, we construct arbitrary $O(D,D)$-invariant actions at orders $α'^0$ and $α'$, and then dimensionally reduce them to the $D$-dimensional spacetime. On the other hand, at these orders, we construct arbitrary covariant $D$-dimensional actions. Constraining the two $D$-dimensional actions to be equal up to non-covariant field redefinitions, we find that both actions are fixed up to overall factors and up to field redefinitions.
description: 18 pages, Latex file, no figure; v2: field redefinitions between 2D- and D-dimensional actions are added,v3: the version appears in PRD
Additional file 1: of The housing first technical assistance and training (HFTAT) implementation strategy: outcomes from a mixed methods study of three programs
Creators: name: Watson, Dennis
name: Ahonen, Emily
name: Shuman, Valery
name: Brown, Molly
name: Tsemberis, Sam
name: Huynh, Philip
name: Fangqian Ouyang
name: Huiping Xu
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Computational Biology

description: HFTAT Specifications. This file contains a more detailed description of the HFTATâ s components mapped onto recommended implementation strategy description guidelines. (PDF 71 kb)
The Masses of Nearby Dwarfs can be Determined with Gravitational Microlensing
Creators: name: Paczynski, B.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Microlensing of distant stars in the Milky Way by the nearby high proper motion stars offers a direct way to precisely measure the masses of single lower main sequence stars and brown dwarfs.
description: 4 pages, plain TEX, no figures
Rumex acetosella Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex acetosella

description: Rumex acetosella, spec. nov.
 22. Rumex floribus dioicis, foliis lanceolato-hastatis. Vir. cliff. 32. Hort. cliff. 139. Fl. lapp. 131. Fl. suec. 296. Roy. lugdb. 231. Gron. virg. 153.
 Acetosa arvensis lanceolata. Bauh. pin. 114.
 Oxalis ovina. Tabern. ic. 440.
 β. Acetosa lanceolata angustifolia repens. Bauh. pin. 114. prodr. 55.
 γ. Acetosa arvensis minima non lanceolata. Bauh. pin. 114.
 δ. Acetosa minor erecta, lobis multifidis. Bocc. mus. 164. t. 126.
 Habitat in Europae pascuis & arvis arenosis. ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 338, DOI: 10.5281/zenodo.3931989
Structural properties of Silicon-Germanium and Germanium-Silicon Core-Shell Nanowires
Creators: name: O'Rourke, Conn
name: Mujahed, Shereif Y.
name: Kumarasinghe, Chathurangi
name: Miyazaki, Tsuyoshi
name: Bowler, David R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Core-shell nanowires made of Si and Ge can be grown experimentally with excellent control for different sizes of both core and shell. We have studied the structural properties of Si/Ge and Ge/Si core-shell nanowires aligned along the $[110]$ direction, with diameters up to 10.2~nm and varying core to shell ratios, using linear scaling Density Functional Theory (DFT). We show that Vegard's law, which is often used to predict the axial lattice constant, can lead to an error of up to 1\%, underlining the need for a detailed \emph{ab initio} atomistic treatment of the nanowire structure. We analyse the character of the intrinsic strain distribution and show that, regardless of the composition or bond direction, the Si core or shell always expands. In contrast, the strain patterns in the Ge shell or core are highly sensitive to the location, composition and bond direction. The highest strains are found at heterojunction interfaces and the surfaces of the nanowires. This detailed understanding of the atomistic structure and strain paves the way for studies of the electronic properties of core-shell nanowires and investigations of doping and structure defects.
description: 9 pages, 9 figures, submitted to J. Phys.:Condens. Matter
MOESM1 of MyD88 Signaling Pathway Is Involved in Renal Fibrosis by Favoring a TH2 Immune Response and Activating Alternative M2 Macrophages
Creators: name: Tarcio Braga
name: Matheus Correa-Costa
name: Guise, Yuri
name: Castoldi, Angela
name: Oliveira, Cassiano De
name: Meire Hyane
name: Cenedeze, Marcos
name: Teixeira, Simone
name: Muscara, Marcelo
name: Perez, Katia
name: Cuccovia, Iolanda
name: Pacheco-Silva, Alvaro
name: GonĂ§Alves, Giselle
name: Camara, Niels
Publisher: name: figshare
Year: 2012
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Marine Biology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: Computational Biology

description: Supplementary material, approximately 775 KB.
Avian influenza virus as an oncolytic therapy for pancreatic cancer
Creators: name: Pizzuto, Matteo Samuele
Publisher: name: Imperial College London
Year: 2015

description: Pancreatic ductal adenocarcinoma (PDA) is one of the leading causes of cancer-related deaths worldwide and the development of new treatment strategies for patients suffering from PDA is of crucial importance. Virotherapy uses natural or engineered oncolytic viruses (OVs) to selectively kill tumour cells. Although various OVs are being investigated as agents for pancreatic cancer treatment, due to the genetic heterogeneity of PDA cells and their consequent mixed permissiveness to viruses, virotherapy should not rely on a short list of possible candidates. As such, preliminary data from our group demonstrating the potent pro-apoptotic effect of the low pathogenicity avian influenza virus (LPAIV) H7N3 A/turkey/Italy/2962/03 in PDA cells, previously established to be resistant to other OVs, suggested that this virus might be effective against specific sub-classes of pancreatic cancer. Therefore, in the present studies, the avian isolate was selected for further development. Preferential replication of the H7N3 virus in IFN-deficient cells, a trait of the majority of PDA cell lines, was improved by the truncation of the viral NS1 protein (NS1-77), which compromised the virus’ ability to counteract the IFN-mediated antiviral response and, as bystander effect, enhanced the killing of uninfected cancer cells by stimulating IFN expression from healthy cells. Introduction of L75H mutation within the mitochondrial targeting sequence (MTS) of the viral protein PB1-F2 increased virus replication in permissive IFN deficient cells and also lessened PB1-F2’s ability to counter the IFN response induced by overexpression of mitochondrial antiviral signalling protein (MAVS), further enhancing selectivity for PDA cells. Substitution of the genes expressing avian surface antigens haemagglutinin (HA) and neuraminidase (NA) with those of the well characterized human H1N1 A/Puerto Rico/8/1934 virus eliminated the potential risk of reassortment of the H7N3 virus with circulating human influenza strains that might result in a new pandemic virus, nonetheless, preserving the oncolytic properties of the parental isolate. Finally, to promote anti-tumour immunity, the newly generated PR8 H1/N1-2962 NS1-77 virus was “armed” to express the human granulocyte-macrophage colony-stimulating factor (GM-CSF) gene during infection. Taken together our data demonstrate the possibility to select an IAV from the avian reservoir on the basis of its strain-specific oncolytic skills in PDA cells and, through engineering, improve its selectivity, safety and tumour debulking activity.
Data-driven reduced modelling of turbulent Rayleigh-Benard convection using DMD-enhanced Fluctuation-Dissipation Theorem
Creators: name: Khodkar, M. A.
name: Hassanzadeh, Pedram
Publisher: name: arXiv
Year: 2018
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Dynamical Systems (math.DS)
subject: Chaotic Dynamics (nlin.CD)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: A data-driven, model-free framework is introduced for calculating Reduced-Order Models (ROMs) capable of accurately predicting time-mean responses to external forcings, or forcings needed for specified responses, e.g., for control, in fully turbulent flows. The framework is based on using the Fluctuation-Dissipation Theorem (FDT) in the space of a limited number of modes obtained from Dynamic Mode Decomposition (DMD). Using the DMD modes as the basis functions, rather than the commonly used Proper Orthogonal Decomposition (POD) modes, resolves a previously identified problem in applying FDT to high-dimensional, non-normal turbulent flows. Employing this DMD-enhanced FDT method (FDT$_\mathrm{DMD}$), a 1D linear ROM with horizontally averaged temperature as state vector, is calculated for a 3D Rayleigh-Bénard convection system at the Rayleigh number of $10^6$ using data obtained from Direct Numerical Simulation (DNS). The calculated ROM performs well in various tests for this turbulent flow, suggesting FDT$_\mathrm{DMD}$ as a promising method for developing ROMs for high-dimensional, turbulent systems.
description: revised manuscript (accepted for publication)
GRAIN ALIGNMENT IN THE TAURUS DARK CLOUD
Creators: name: Gerakines, P. A.
name: Whittet, D. C. B.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Variations in polarization efficiency (p/A) of interstellar grains as a function of environment place vital constraints on models for the mechanism of their alignment. We use polarimetry of background field stars to investigate alignment in the Taurus dark cloud as a function of optical depth for extinctions of A_K < 2.5 (A_V < 25). Results show a strong systematic trend in polarization efficiency with extinction. We discuss the possibility of a relationship between p/A and icy grain mantle growth, since mantles are detected in Taurus only for extinctions where p/A is lowest. A simple density model of alignment by paramagnetic alignment (Davis & Greenstein 1951) predicts that the magnetic field strength (B) scales with density to the power k=0.28.
description: 13 pages uuencoded compressed PostScript, submitted to ApJ Letters
Atg8 family proteins, LIR/AIM motifs and other interaction modes.
Creators: name: Rogov, Vladimir V
name: Nezis, Ioannis P
name: Tsapras, Panagiotis
name: Zhang, Hong
name: Dagdas, Yasin
name: Noda, Nobuo N
name: Nakatogawa, Hitoshi
name: Wirth, Martina
name: Mouilleron, Stephane
name: McEwan, David G
name: Behrends, Christian
name: Deretic, Vojo
name: Elazar, Zvulun
name: Tooze, Sharon A
name: Dikic, Ivan
name: Lamark, Trond
name: Johansen, Terje
Publisher: name: The Francis Crick Institute
Year: 2024
Subjects: classificationCode: Signalling & Oncogenes
subject: Signalling & Oncogenes
classificationCode: Chemical Biology & High Throughput
subject: Chemical Biology & High Throughput
classificationCode: Model organisms
subject: Model organisms
classificationCode: Biochemistry & Proteomics
subject: Biochemistry & Proteomics
classificationCode: Structural Biology & Biophysics
subject: Structural Biology & Biophysics
classificationCode: Cell Biology
subject: Cell Biology
classificationCode: Imaging
subject: Imaging

description: The Atg8 family of ubiquitin-like proteins play pivotal roles in autophagy and other processes involving vesicle fusion and transport where the lysosome/vacuole is the end station. Nuclear roles of Atg8 proteins are also emerging. Here, we review the structural and functional features of Atg8 family proteins and their protein-protein interaction modes in model organisms such as yeast, Arabidopsis, C. elegans and Drosophila to humans. Although varying in number of homologs, from one in yeast to seven in humans, and more than ten in some plants, there is a strong evolutionary conservation of structural features and interaction modes. The most prominent interaction mode is between the LC3 interacting region (LIR), also called Atg8 interacting motif (AIM), binding to the LIR docking site (LDS) in Atg8 homologs. There are variants of these motifs like "half-LIRs" and helical LIRs. We discuss details of the binding modes and how selectivity is achieved as well as the role of multivalent LIR-LDS interactions in selective autophagy. A number of LIR-LDS interactions are known to be regulated by phosphorylation. New methods to predict LIR motifs in proteins have emerged that will aid in discovery and analyses. There are also other interaction surfaces than the LDS becoming known where we presently lack detailed structural information, like the N-terminal arm region and the UIM-docking site (UDS). More interaction modes are likely to be discovered in future studies.
Rumex acetosella subsp. acetosella Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex acetosella
Rumex acetosella l. subsp. acetosella

description: Rumex acetosella Linnaeus, Species Plantarum 1: 338. 1753.
"Habitat in Europae pascuis & arvis arenosis." RCN: 2603.
Lectotype (Love in Bot. Helv. 93: 164. 1983): Herb. Linn. No. 464.41 (LINN).
Current name: Rumex acetosella L. subsp. acetosella (Polygonaceae).
Note: Löve indicates the type as "LINN. “22”.”, but on p. 161 mentions that the type sheet bears two specimens. This clearly refers to sheet 464.41, and not to sheet 464.38 (which bears three specimens), subsequently treated as the type by den Nijs (in Feddes Repert. 95: 51-52. 1984). See discussion of this by Wilson (in Telopea 7: 85. 1996).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 803, DOI: 10.5281/zenodo.291971
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Cart. 188 (11 H 73), f. 0276v
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2012
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0276v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0276v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
title: Trade and Sustainable Food Systems
title: Food Systems Summit Brief Prepared by Research Partners of the Scientific Group for the Food Systems Summit June 8, 2021
titleType: Subtitle
Creators: name: Zimmermann, Andrea
name: Rapsomanikis, George
Publisher: name: Center for Development Research (ZEF) in cooperation with the Scientific Group for the UN Food System Summit 2021
Year: 2021
Subjects: subject: FOS: Agriculture, forestry, and fisheries
valueUri: http://www.oecd.org/science/inno/38235147.pdf
classificationCode: 630
subject: Agriculture, Veterinary Medicine
subject: Food systems
subject: Sustainability
subject: Trade

description: Trade is an integral part of our food systems. It connects people at all stages of agricultural and food value chains, linking farmers with consumers across the world. It also links nations to each other and thus scales up from the domestic to global perspective. By moving food from surplus to deficit regions, trade promotes food security, the diversity of foods available, and can affect preferences and diets. Trade impacts food prices and the allocation of resources and thus is inherent with economic growth and interacts with the environment. At the same time, trade can create both winners and losers, resulting in inequality, and can generate negative social and environmental outcomes. This brief provides an overview of the current debate around trade in food and agriculture and illustrates the role that trade can play within food systems in balancing different dimensions of sustainability. While trade openness is generally conducive to food security and promotes economic growth, formulating trade policies to achieve multiple targets, including environmental, nutritional and social objectives, requires careful analysis. Trade policies may not be the best and most efficient instruments to achieve multiple objectives and they should be framed by complementary policies targeting specific aspects of sustainability. For example, in addressing climate change, one of today’s most pressing challenges, a combination of food trade and domestic policy instruments can sharpen the adaptation and mitigation roles of trade and significantly contribute in providing incentives to promote climate-smart technologies. In order to effectively design such policies, a better understanding of both the complex linkages between trade and sustainability outcomes and the simultaneous impacts of policy approaches on all parts of the food system will be necessary.
Gas and multi-species dust dynamics in viscous protoplanetary discs: the importance of the dust back-reaction
Creators: name: Dipierro, Giovanni
name: Laibe, Guillaume
name: Alexander, Richard
name: Hutchison, Mark
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We study the dynamics of a viscous protoplanetary disc hosting a population of dust grains with a range of sizes. We compute steady-state solutions, and show that the radial motion of both the gas and the dust can deviate substantially from those for a single-size dust population. Although the aerodynamic drag from the dust on the gas is weaker than in the case where all grains are optimally coupled to the gas, the cumulative "back-reaction" of the dust particles can still alter the gas dynamics significantly. In typical protoplanetary discs, the net effect of the dust back-reaction decreases the gas accretion flow compared to the dust-free (viscous) case, even for dust-to-gas ratios of order $1\%$. In the outer disc, where dust grains are typically less strongly coupled to the gas and settle towards the midplane, the dust back-reaction can even drive outward gas flow. Moreover, the radial inward drift of large grains is reduced below the gas motion in the inner disc regions, while small dust grains follow the gas dynamics over all the disc extent. The resulting dust and gas dynamics can give rise to observable structures, such as gas and dust cavities. Our results show that the dust back-reaction can play a major role in both the dynamics and observational appearance of protoplanetary discs, and cannot be ignored in models of protoplanetary disc evolution.
description: Accepted for publication in MNRAS, 20 pages, 9 figures
MOESM1 of Psychotic (delusional) depression and completed suicide: a systematic review and meta-analysis
Creators: name: Rossetos Gournellis
name: Tournikioti, Kalliopi
name: Touloumi, Giota
name: Thomadakis, Christos
name: Michalopoulou, Panayiota
name: Michopoulos, Ioannis
name: Christodoulou, Christos
name: Papadopoulou, Athanasia
name: Douzenis, Athanasios
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology

description: Additional file 1. Additional figures.
The electron gas in a magnetic field: the equation of state
Creators: name: Celebonovic, V.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Continuing previous work and using a simple change of variables, an analytical equation of state for a degenerate non-relativistic Fermi gas in a magnetic field is proposed.
description: PDF file,no figures Typos have been corrected and the Journal-ref.added
Some infinite dimensional topics in probability and statistics
Creators: name: Blacque-Florentin, Pierre
Publisher: name: Imperial College London
Year: 2016

description: This thesis comprises two independent parts. In the first part, we develop a pathwise calculus for functionals of integer-valued measures and extend the framework of Functional Itô Calculus to functionals of integer-valued random measures by constructing a ’stochastic derivative’ operator with respect to such integer-valued random measures. This allows us to obtain weak martingale representation formulae holding beyond the class of Poisson random measures, and allowing for random and time-dependent compensators. We study the behaviour of this operator and compare it with other previous approaches in the literature, providing in passing a review of the various Malliavin approaches for jump processes. Finally, some examples of computations are provided. The second part is oriented towards nonparametric statistics, with a financial application as our main goal: we aim at recovering a surface of FX call options on a pegged currency such as the Hong Kong dollar against the U.S. dollar, based on a small number of noisy measurements (the market bid-ask quotes). Inspiring ourselves from the Compressed Sensing literature, we develop a methodology that aims at recovering an arbitrage-free call surface. We first apply this methodology, based on tensor polynomial decomposition of the surface, to a sparse set of call-option prices on the S&P500, recovering the call option prices within desired tolerance, as well as a smooth local-volatility surface. On a pegged currency such as the HKD/USD, it appears that tensor polynomials may not be an adequate way to model the smiles across maturities. Modifying the methodology in favour of structure-preserving functions, we apply the new methodology to our HKD/USD dataset, recovering the smiles, and the corresponding state-price density.
Recruiting for Success. Does Board Diversity Matter?
Creators: name: Cotter Mazzola, Meg E.
name: Pontacolon, Joseph L.
name: Claudio, Angel
name: Salguero, Javier A.
name: James, Marcelles
name: Yawson, Robert
Publisher: name: Zenodo
Year: 2020

description: Nonprofits play an essential role in society. To realize their important missions, nonprofits rely on strong and committed leaders at both the organization level as well as the governance level. Nonprofits are obligated to have an active board of directors to operate. This reliance places the organization in a vulnerable position where they must recruit and engage with external stakeholders and identify individuals with the combination of talent needed to succeed as well as the passion for supporting the organization's vision. Knowing that board members have a long- lasting impact on their organizations, this paper looks at the varying models of governance and the implications for choosing one model over another. Determining the best structure for a governance model represents one component to setting an organization up for success. Equally, if not more important, is ensuring that the board of directors is composed of motivated and committed individuals who are steadfast in their efforts to support the mission of the organization. In order to find the best people for the role, an organization must understand what drives and motivates an individual to serve on a board. The topic of motivation as it relates to governance boards, and how existing boards can use the motivating factors to recruit and retain board members is explored. Finally, we explore the value of diverse board composition and whether certain criteria of diversity carry more weight in terms of impact than others. Keywords:
Decaying $Λ$ cosmologies and statistical properties of gravitational lenses
Creators: name: Torres, L. F. Bloomfield
name: Waga, I.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper we investigate the statistical properties of gravitational lenses for models in which a cosmological term decreases with time as $Λ\propto a^{-m}$, where $a$ is the scale factor and $m$ is a parameter ($0 \leq m < 3$). We show that for given low values of the present matter density parameter $Ω_{m0}$, there is a wide range of values for $m$ for which the lensing rate is significantly smaller than that in cosmological constant ($Λ$) models. We also show that models with low $Ω_{m0}$ and $m\stackrel{>}{\sim}2$ have high likelihood to reproduce the observed lens statistics in the HST snapshot survey.
description: reformated file, 19 pages, Latex, 8 figures available on request
Additional file 1: of Uncovering the mechanisms of research capacity development in health and social care: a realist synthesis
Creators: name: Cooke, Jo
name: Gardois, Paolo
name: Booth, Andrew
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Science Policy

description: The 36 studies describing conceptual models, frameworks or theory for research capacity development. (DOCX 35 kb)
Electrokinetic and electrohydrodynamic problems in multifluid flows
Creators: name: Dubrovina, Elizaveta
Publisher: name: Imperial College London
Year: 2016

description: The present thesis deals with microfluidic systems under the influence of electric fields. The purpose of this research is to identify key behaviours which are highly relevant for applications in lab-on-chip devices such as pH control, patterning, mixing and cell trapping. In the first part of the thesis we consider the electrokinetics of charged, porous membranes and present a mathematical model for the ionic transport under the effects of a horizontal electric field. First, we investigate the behaviour of a system that consists of one anion membrane with two reservoirs and produce numerical solutions with the aim to gain a better understanding of the mechanisms that lead to overlimiting current. We then analyse the features of a system where a bipolar membrane is held in an electrolyte bath with water and a salt. We use our model to confirm findings from experiments such as the hysteretic behaviour of the IV curve and the water splitting phenomenon. In the second part of the thesis we examine the behaviour of interfaces between two fluids that are sandwiched between two electrodes. We find that introducing a constant flow rate into the system leads to time modulated travelling waves. In the case of flat channel walls these look like moving strips which are reminiscent of the patterns found in the no flow case. Adding corrugations on one or both electrodes leads to a rich variety of dynamics. We develop a Floquet stability analysis which takes into account the fact that the base state of the system is nonuniform. This is a very useful tool for identifying the different types of behaviours which arise as we change the applied voltage and the overall flow rate. We examine the streamlines of the fluid to explore the advantages of the different regimes: just by changing the applied voltage it is possible to transition from an environment which is favourable to efficient mixing to one which could enhance cell trapping.
A coherent derivation of the Ewald summation for arbitrary orders of multipoles: The self-terms
Creators: name: Stamm, Benjamin
name: Lagardère, Louis
name: Polack, Étienne
name: Maday, Yvon
name: Piquemal, Jean-Philip
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: In this work, we provide the mathematical elements we think essential for a proper understanding of the calculus of the electrostatic energy of point-multipoles of arbitrary order under periodic boundary conditions. The emphasis is put on the expressions of the so-called self parts of the \Ewald\, summation where different expressions can be found in literature. Indeed, such expressions are of prime importance in the context of new generation polarizable force field where the self field appears in the polarization equations. We provide a general framework, where the idea of the \Ewald\ splitting is applied to the electric potential and subsequently, all other quantities such as the electric field, the energy and the forces are derived consistently thereof. Mathematical well-posedness is shown for all these contributions for any order of multipolar distribution.
Coupling charge-exchange vibrations to nucleons in a relativistic framework: effect on Gamow-Teller transitions and beta-decay half-lives
Creators: name: Robin, Caroline
name: Litvinova, Elena
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The nuclear response theory for isospin-transfer modes in the relativistic particle-vibration coupling framework is extended to include coupling of single nucleons to isospin-flip (charge-exchange) phonons, in addition to the usual neutral vibrations. This new coupling introduces dynamical pion and rho-meson exchange, beyond the Hartree-Fock approximation, up to infinite order. We investigate the impact of this new mechanism on the Gamow-Teller response of a few doubly-magic neutron-rich nuclei, namely $^{48}$Ca, $^{78}$Ni, $^{132}$Sn and $^{208}$Pb. It is found that the coupling to isospin-flip vibrations can have a non negligible impact on the strength distribution and quenching of the giant resonance, globally improving the agreement with the experimental data. The corresponding beta-decay half-lives of $^{78}$Ni and $^{132}$Sn are also calculated, and found to be decreased by a factor $\sim 2$ by the inclusion of the new phonons.
description: 6 pages, 5 figures, v2: accepted version
Superhump period of the black hole X-ray binary GX 339-4
Creators: name: Kosenkov, Ilia A.
name: Veledina, Alexandra
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We investigate variability of optical and near-infrared light curves of the X-ray binary GX 339-4 on a timescale of days. We use the data in four filters from six intervals corresponding to the soft state and from four intervals corresponding to the quiescent state. In the soft state, we find prominent oscillations with the average period P = 1.772 $\pm$ 0.003 d, which is offset from the measured orbital period of the system by 0.7 per cent. We suggest that the measured periodicity originates from the superhumps. In line with this interpretation we find no periodicity in the quiescent state. The obtained period excess $ε$ is below typical values found for cataclysmic variables for the same mass ratio of the binary. We discuss implications of this finding in the context of the superhump theory.
description: 11 pages, 8 figures, 4 tables. Accepted to MNRAS
The formation of extremely diffuse galaxy cores by merging supermassive black holes
Creators: name: Rantala, Antti
name: Johansson, Peter H.
name: Naab, Thorsten
name: Thomas, Jens
name: Frigo, Matteo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Given its velocity dispersion, the early-type galaxy NGC 1600 has an unusually massive ($M_\bullet = 1.7 \times 10^{10} M_\odot$) central supermassive black hole (SMBH), surrounded by a large core ($r_\mathrm{b} = 0.7$ kpc) with a tangentially biased stellar distribution. We present high-resolution equal-mass merger simulations including SMBHs to study the formation of such systems. The structural parameters of the progenitor ellipticals were chosen to produce merger remnants resembling NGC 1600. We test initial stellar density slopes of $ρ\propto r^{-1}$ and $ρ\propto r^{-3/2}$ and vary the initial SMBH masses from $8.5 \times 10^8$ to $8.5 \times 10^9$ $M_\odot$. With increasing SMBH mass the merger remnants show a systematic decrease in central surface brightness, an increasing core size, and an increasingly tangentially biased central velocity anisotropy. Two-dimensional kinematic maps reveal decoupled, rotating core regions for the most massive SMBHs. The stellar cores form rapidly as the SMBHs become bound, while the velocity anisotropy develops more slowly after the SMBH binaries become hard. The simulated merger remnants follow distinct relations between the core radius and the sphere-of-influence, and the SMBH mass, similar to observed systems. We find a systematic change in the relations as a function of the progenitor density slope, and present a simple scouring model reproducing this behavior. Finally, we find the best agreement with NGC 1600 using SMBH masses totaling the observed value of $M_\bullet = 1.7 \times 10^{10} M_\odot$. In general, density slopes of $ρ\propto r^{-3/2}$ for the progenitor galaxies are strongly favored for the equal-mass merger scenario.
description: Accepted for publication in ApJ
Rumex bucephalophorus Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex bucephalophorus

description: Rumex aculeatus Linnaeus, Systema Naturae, ed. 10, 2: 991. 1759.
["Habitat in Creta, Hispania."] Sp. Pl., ed. 2, 1: 482 (1762). RCN: 2604.
Type not designated.
Original material: Herb. Linn. No. 464.39 (LINN); Herb. Linn. No. 464.40 (LINN).
Current name: Rumex bucephalophorus L. (Polygonaceae).
Note: Specific epithet spelled “aculeata” in the protologue. López González (in Anales Jard. Bot. Madrid 44: 589. 1987) treated this name as a synonym of R. bucephalophorus, noting that typification using either 464.39 or 464.40 (LINN) would maintain this position.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 803, DOI: 10.5281/zenodo.291971
The Radio Wavelength Time Delay of Gravitational Lens 0957+561
Creators: name: Haarsma, Deborah B.
name: Hewitt, Jacqueline N.
name: Lehár, Joseph
name: Burke, Bernard F.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The gravitational lens 0957+561 was monitored with the Very Large Array from 1979 to 1997. The 6 cm light curve data from 1995-1997 and the 4 cm data from 1990-1997 are reported here. At 4 cm, the intrinsic source variations occur earlier and are twice as large as the corresponding variations at 6 cm. The VLBI core and jet components have different magnification factors, leading to different flux ratios for the varying and non-varying portions of the VLA light curves. Using both the PRHQ and Dispersion statistical techniques, we determined the time delay, core flux ratio, and excess non-varying B image flux density. The fits were performed for the 4 cm and 6 cm light curves, both individually and jointly, and we used Gaussian Monte Carlo data to estimate 68% statistical confidence levels. The delay estimates from each individual wavelength were inconsistent given the formal uncertainties, suggesting that there are unmodeled systematic errors in the analysis. We roughly estimate the systematic uncertainty in the joint result from the difference between the 6 cm and 4 cm results, giving 409+-30 days for the PRHQ statistic and 397+-20 days for the Dispersion statistic. These results are consistent with the current optical time delay of 417+-3 days, reconciling the long-standing difference between the optical and radio light curves and between different statistical analyses. The unmodeled systematic effects may also corrupt light curves for other lenses, and we caution that multiple events at multiple wavelengths may be necessary to determine an accurate delay in any lens system. Now that consensus has been reached regarding the time delay in the 0957+561 system, the most pressing issue remaining for determining H_0 is a full understanding of the mass distribution in the lens.
description: 20 pages including 4 figures, AASTeX, accepted by ApJ
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VII, Cart. 191 (11 H 76), 199 folios, f. 0004v
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VII, Archives départementales de la Côte-d'Or, Cart. 191 (11 H 76), 199 folios, f. 0004v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VII, Archives départementales de la Côte-d'Or, Cart. 191 (11 H 76), 199 folios, f. 0004v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Substructure in Clusters of Galaxies and the value of ${\bfΩ}$
Creators: name: Dutta, Suvendra N.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the formation of clusters of galaxies in an expanding universe using a new code that regrids at a region of high density. In particular we investigate two models for the initial conditions, both with the standard CDM power spectrum - one has $Ω= 1$ and the other $Ω= 0.2$. Both universes have $H_0 = 100 \kms\mpc^{-1}$ and $Λ= 0$. The level of substructure in the final cluster can be used as a discriminant of the cosmic density. We discuss various statistics which can be measured observationally from clusters of galaxies, that can be used to discriminate between the two models. We find that most of the statistics that use the clusters' member galaxies may not be the best measures of substructure. Statistics that rely more on X-ray maps and other observables depending more directly on the mass distribution could be better discriminants of $Ω$.
description: 7 pages, uuencoded gzipped postscript file, figures included. Accepted for publication to the M.N.R.A.S
Gamma-Ray Bursts and the Cosmic Star Formation Rate
Creators: name: Krumholz, Mark R.
name: Thorsett, S. E.
name: Harrison, Fiona A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have tested several models of GRB luminosity and redshift distribution functions for compatibility with the BATSE 4B number versus peak flux relation. Our results disagree with recent claims that current GRB observations can be used to strongly constrain the cosmic star formation history. Instead, we find that relaxing the assumption that GRBs are standard candles renders a very broad range of models consistent with the BATSE number-flux relation. We explicitly construct two sample distributions, one tracing the star formation history and one with a constant comoving density. We show that both distributions are compatible with the observed fluxes and redshifts of the bursts GRB970508, GRB971214, and GRB980703, and we discuss the measurements required to distinguish the two models.
description: 12 pages, 2 postscript figures, uses AAS LaTex macros v4.0. To be published in Astrophysical Journal Letters, accepted August 20, 1998. Revised for publication