cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Cartulaire de Cîteaux dit Cartularium Vetus (milieu XIIIe siècle) et Notices du XIIe siècle, Cart. 169 (11 H 63), f. 0053r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2011
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de Cîteaux dit Cartularium Vetus (milieu XIIIe siècle) et Notices du XIIe siècle, Archives départementales de la Côte-d'Or, Cart. 169 (11 H 63), f. 0053r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux dit Cartularium Vetus (milieu XIIIe siècle) et Notices du XIIe siècle, Archives départementales de la Côte-d'Or, Cart. 169 (11 H 63), f. 0053r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Towards an Understanding of the Globular Cluster Over--abundance around the Central Giant Elliptical NGC 1399
Creators: name: Kissler-Patig, Markus
name: Grillmair, Carl J.
name: Meylan, Georges
name: Brodie, Jean P.
name: Minniti, Dante
name: Goudfrooij, Paul
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the kinematics of a combined sample of 74 globular clusters around NGC 1399. Their high velocity dispersion, increasing with radius, supports their association with the gravitational potential of the galaxy cluster rather than with that of NGC 1399 itself. We find no evidence for rotation in the full sample, although some indication for rotation in the outer regions. The data do not allow us to detect differences between the kinematics of the blue and red sub-populations of globular clusters. A comparison between the globular cluster systems of NGC 1399 and those of NGC 1404 and NGC 1380 indicates that the globular clusters in all three galaxies are likely to have formed via similar mechanisms and at similar epochs. The only property which distinguishes the NGC 1399 globular cluster system from these others is that it is ten times more abundant. We summarize the evidence for associating these excess globulars with the galaxy cluster rather than with NGC 1399 itself, and suggest that the over-abundance can be explained by tidal stripping, at an early epoch, of neighboring galaxies and subsequent accumulation of globulars in the gravitational potential of the galaxy cluster.
description: AJ accepted (March issue), 27 pages (6 figures included), AAS style, two columns. Also available at http://www.eso.org/~mkissler
Unusual Multiple Magnetic Transitions and Anomalous Hall Effect Observed in Antiferromagnetic Weyl Semimetal, Mn$_{2.94}$Ge (Ge-rich)
Creators: name: Ghosh, Susanta
name: Low, Achintya
name: Changdar, Susmita
name: Purwar, Shubham
name: Thirupathaiah, Setti
Publisher: name: arXiv
Year: 2024
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report on the magnetic and Hall effect measurements of the magnetic Weyl semimetal, Mn$_{2.94}$Ge (Ge-rich) single crystal. From the magnetic properties study, we identify unusual multiple magnetic transitions below the N$\acute{e}$el temperature of 353 K, such as the spin-reorientation ($T_{SR}$) and ferromagnetic-like transitions. Consistent with the magnetic properties, the Hall effect study shows unusual behavior around the spin-reorientation transition. Specifically, the anomalous Hall conductivity (AHC) increases with increasing temperature, reaching a maximum at $T_{SR}$, which then gradually decreases with increasing temperature. This observation is quite in contrast to the Mn$_{3+δ}$Ge (Mn-rich) system, though both compositions share the same hexagonal crystal symmetry. This study unravels the sensitivity of magnetic and topological properties on the Mn concentration.
description: 15 pages, 6 figures, Accepted-In Press
Quantification of post-translationally modified p53 in single cells
Creators: name: Squires, James Alexander
Publisher: name: Imperial College London
Year: 2017

description: This work outlines efforts towards the development of immunosorbent assays for quantifying post-translationally modified p53, a key tumour suppressor protein, in single cancer cells. These assays utilised the microfluidic antibody capture (MAC) chip to selectively detect post-translationally modified p53 at single molecule sensitivity. Three assays for post-translationally modified p53 were developed; for acetylated-p53, ubiquitinated-p53 and phosphorylated-p53. The assay for acetylated p53, utilising click chemistry, was unsuccessful, as was an approach using antibodies. The assay for ubiquitinated p53 was successful in cell lysate, though could not be made successful in single cells. However, an assay for phosphorylated-p53 was successful and was multiplexed alongside a previously developed total p53 assay to elucidate the effects of a range of drugs on the phosphorylation and total p53 expression in single cells from immortalised cancer cell lines. This assay was then successfully applied, alongside the total p53 assay, to clinically relevant patient-derived xenograft material, the results of which were published in the peer-reviewed literature due to its novelty. This constituted one of the first examples of the measurement of a potentially clinically relevant biomarker in tumour derived material at single cell sensitivity. Further development of the MAC chip aimed at improving its throughput and range of accessible analytes could allow its use as a diagnostic or prognostic device when linked to clinically relevant outcomes such as remission, progression free survival, overall survival or measures of quality of life. This would be a significant contribution towards the personalisation of cancer treatment.
Models of technological polymers
Creators: name: Molinari, Nicola
Publisher: name: Imperial College London
Year: 2018

description: Polymers are widely adopted in many industrial sectors, where they usually constitute small but crucial technological components. In the oil and gas industry, polymer seals should act as impermeable barriers to protect sophisticated downhole equipment from corrosion. Additionally, their mechanical properties play an important role in communicating information from the bottom of the well to the surface. However, costly permeation-driven failures are observed. In the energy storage sector, polymers are promising candidates for safer electrolytes that do not suffer from safety issues related to leakage, shorting and combustible reactions. However, cation mobility in polymer-based electrolytes must be improved to attain commercial viability. Finally, nanoparticles have been recently suggested as universal and inexpensive polymer adhesives, possibly solving the century-old problem of adhering soft matter together. The common thread is that significant insight can be gained through a molecular-level understanding of the underlying mechanisms. Using a molecular-simulation-based approach, I have investigated the trends in, and the fundamental drivers of, the properties of these three technology-relevant polymer systems. In the oil and gas industry, hydrogenated nitrile butadiene rubber is widely adopted, and I have developed and validated a molecular model for it based on the OPLS-AA force-field. I have also studied the mechanical properties of filled elastomers using a coarse-grained model, and have uncovered important connections between filler loading, polymer-fillers network, and the stress-strain response of the material. In battery technology, poly(ethylene)oxide/Li/bis(trifluoromethane)sulfonimide is a promising electrolyte system, and I have demonstrated the central role of the anion in coordinating lithium atoms and the appearance of asymmetrical cation/anion clusters. Finally, I have investigated the use of nanoparticles as universal glue by studying the effects on the stress-strain response of nanoparticles’ size, nanoparticle-polymer interaction strength and density. The latter influences the organisation of the nanoparticles at the interface, which results in a non-monotonous mechanical reinforcement.
Alauda Linnaeus, 1758, gen. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Alaudidae
Alauda

description: Alauda [gen. nov.]
Rostrum cylindrico-subulatum, rectum, recta protensum: Mandibulis aequalibus, basi deorsum dehiscentibus.
Lingua bifida.
Unguis posticus rectior, digito longior.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 165, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The X-ray properties of the nearby LINER galaxy, NGC 4736
Creators: name: Roberts, T. P.
name: Warwick, R. S.
name: Ohashi, T.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: NGC 4736 is a nearby Sab spiral galaxy, hosting one of the closest examples of a LINER nucleus. We have utilized recent observations by ROSAT and ASCA to characterise the X-ray properties of this galaxy. Twelve discrete X-ray sources are detected within the region subtended by its optical disk, the majority of which are likely to be X-ray binaries associated with the galaxy. By far the brightest source in the X-ray band is positionally coincident with the nucleus of the galaxy and is spatially resolved into a component with a radial extent of ~ 3 kpc plus a point-like core. The broad band (0.1-10 keV) spectrum of this nuclear source is composed of a hard continuum with a spectral slope characteristic of that observed in classical Seyfert nuclei (i.e. power-law photon index, Gamma ~ 1.7), with thermal emission (kT = 0.1-0.6 keV) dominant below 2 keV. An Fe K alpha line may also be present at ~ 6.8 keV. There is no evidence for X-ray temporal variability on timescales of hours to years. A plausible model is that the hard continuum originates in a near-quiescent active galactic nucleus (with L_x ~ 6 x 10^39 erg/s, 0.5-10 keV) embedded in the LINER at the centre of NGC 4736. However, an alternative explanation, namely that the LINER is the site of a dense population of X-ray binary sources, cannot be completely excluded.
description: 11 pages including 4 embedded figures, uses graphicx.sty and mn.sty, accepted for publication in MNRAS
High energy protons from PKS 1333-33
Creators: name: Anchordoqui, L. A.
name: Romero, G. E.
name: Bergliaffa, S. E. Perez
name: Combi, J. A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this letter we give an account of the possible acceleration of protons in the outer radio lobes of the active galaxy PKS 1333-33. We also make estimates of the arrival energy spectrum.
description: 3 pages revtex, two figures, to appear in Mod. Phys. Lett. A
Search for line signal candidates in the Fermi-LAT data
Creators: name: Li, Shang
name: Xia, Zi-Qing
name: Liang, Yun-Feng
name: Duan, Kai-Kai
name: Shen, Zhao-Qiang
name: Li, Xiang
name: Feng, Lei
name: Yuan, Qiang
name: Fan, Yi-Zhong
name: Chang, Jin
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In order to search for the line-like signals in the Fermi-LAT data, we have analyzed totally 49152 regions of interest (ROIs) that cover the whole sky. No ROI displays a line signal with test statistic (TS) value above 25, while for 50 ROIs weak line-like excesses with ${\rm TS}>16$ are presented. The intrinsic significances of these potential signals are further reduced by the large trial factor introduced in such kind of analysis. For the largest TS value of 24.3 derived in our analysis, the corresponding global significance is only $0.54σ$. We thus do not find any significant line-like signal and set up constraints on the cross section of dark matter annihilating to gamma-ray lines, $\left_{γγ}$.
description: 10 pages, 6 figures, accepted by PRD
Additional file 3: of Trends in healthcare utilization and costs associated with pneumonia in the United States during 2008â 2014
Creators: name: Tong, Sabine
name: Amand, Caroline
name: Kieffer, Alexia
name: Kyaw, Moe
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Table S3. Frequency of index pneumonia visits per 1000 person-years by age group and year (DOCX 13 kb)
An Integrated computational & mammalian synthetic biology framework for engineering turing patterns
Creators: name: Scholes, Natalie
Publisher: name: Imperial College London
Year: 2018

description: Turing patterns are thought to underlie the formation of many tissue structures during development. First proposed by Alan Turing, two key properties are known to affect the formation of patterns: the fine balance of the interaction parameters and the differential diffusion of an activating and inhibiting species. Despite many experimental examples, it has been difficult to determine if Turing patterns alone suffice to generate patterns in vivo. Engineering Turing patterns, in the absence of any endogenous patterning networks, may shed light on how they function in nature. Here I combined a computational and mammalian synthetic biology approach into a unified framework for engineering Turing patterns. Through theoretical analysis of a wide range of networks (15,514 networks with two and three interacting species), I found that ≈60% of all networks tested can achieve Turing patterns. However, features beyond structure determine a network's Turing patterning capability. Even though individual networks with three interacting molecules are more likely to form Turing patterns than two species networks, the parameter space always remains very limited (<1% of the explored parameter space). To enable the precise parameter tuning required, I therefore developed an in vivo platform to integrate and exchange DNA in a pre-defined genomic locus, using CRISPR/Cas9. This platform ensures the functionality of the regulatory circuits by making use of endogenous gene regulatory elements. Moreover, the theoretical analysis revealed that differential diffusion remains advantageous, albeit not absolutely necessary, for Turing pattern formation. Hence, I engineered a 90-fold slower diffusing activator variant. Factors such as intracellular negative feedbacks complicated the system and ultimately led to the conclusion that these components are unsuitable for supporting Turing patterns. Nonetheless, the general results from the theoretical analysis, and the generation of a novel platform for generating inducible systems in mammalian cell lines, show promise for future Turing pattern generation.
Interacting quantum walk on a graph
Creators: name: Verga, Alberto D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We introduce an elementary quantum system consisting of a set of spins on a graph and a particle hopping between its nodes. The quantum state is build sequentially, applying a unitary transformation that couples neighboring spins and, at a node, the local spin with the particle. We observe the relaxation of the system towards a stationary paramagnetic or ferromagnetic state, and demonstrate that it is related to eigenvectors thermalization and random matrix statistics. The relation between these macroscopic properties and interaction generated entanglement is discussed.
description: 15 pages, 11 figures (v2 extended version)
Vertical Structure of Accretion Discs with Hot Coronae in AGN
Creators: name: Różańska, A.
name: Czerny, B.
name: Życki, P. T.
name: Pojmański, G.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study vertical structure of radiation pressure dominated disc with a hot corona. We include all the relevant processes like bound--free opacity and convection. We show that the presence of the corona modifies considerably the density and the opacity of the disc surface layers which are important from the point of view of spectrum formation. The surface of the disc with a corona is much denser and less ionized than the surface of a bare disc. Such a disc is likely to produce a neutral reflection and a local spectrum close to a black body. This effect will help to reconcile the predictions of accretion disc models with the observational data since a neutral reflection and a lack of Lyman edge are generally seen in AGN.
description: 10 pages, 9 figures, submitted to MNRAS
The origin of the Narrow Line Region of Mrk 3: an overpressured jet cocoon
Creators: name: Capetti, A.
name: Axon, D. J.
name: Macchetto, F. D.
name: Marconi, A.
name: Winge, C.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained HST FOC long-slit optical spectroscopy of the Narrow Line Region of the Seyfert 2 galaxy Mrk 3. In the region cospatial with the radio-jet the velocity field is highly perturbed and shows two velocity systems separated by as much as 1700 km/s. We interpret this to be the consequence of the rapid expansion of a cocoon of hot gas, shocked and heated by the radio-emitting outflow, which compresses and accelerates the ambient gas. The NLR itself is essentially a cylindrical shell expanding supersonically. From the size and velocity of the expanding region, we derive an upper limit to the radio-source age, ~< 1.5 E5 years, and a lower limit for the jet power, ~> 2 E42 erg/s required to inflate the cocoon and estimate that the jet minimum advance speed is 3 E-3 pc per year. The total kinetic energy of the high velocity NLR gas can be estimated as ~6 E54 erg, comparable to the total energy carried by the jet over its lifetime and this quantitatively supports the idea that the NLR gas is accelerated by the jet. If the advance speed of Mrk 3 is representative of the Seyfert population then these sources must also be short lived and probably recurrent. The jet kinetic luminosity of Mrk 3 is between 2 and 3 orders of magnitude smaller than that derived for radio-loud AGNs with similar emission-line luminosity. On the other hand, the fraction of jet power dissipated in radio-emission is similar. We speculate that the main distinction between radio-quiet and radio-loud AGN is ascribed to a difference in jet power rather than to a different efficiency in synchrotron emission production.
description: 13 pages, 8 figures, Astrophysical Journal in press
Pore-scale imaging and analysis of carbonate dissolution during reservoir-condition CO2-acidified brine flow: Influence of chemical and physical heterogeneity
Creators: name: Al-Khulaifi, Yousef
Publisher: name: Imperial College London
Year: 2018

description: The sequestration of carbon dioxide (CO2) into geologic formations is one of the long-term solutions proposed to mitigate atmospheric CO2 concentrations [1]. Potential storage sites include deep saline aquifers and depleted hydrocarbon reservoirs. In the case of carbonate reservoirs, the possibility of significant dissolution reaction taking place between CO2, in situ brines and rock is very real. Proposed in this thesis is a method to dynamically image reactive transport in carbonates at subsurface conditions, representing the movement of CO2 saturated brine in the reservoir. The work will focus on understanding reactive transport in carbonate reservoirs by imaging changes in the pore structure, porosity and permeability in representative rock samples induced by the simultaneous flow and reaction of CO2 saturated brine at reservoir conditions. X-ray micro-tomography will be the imaging tool of choice to investigate pore structure changes during reactive transport experiments. Effluent from the dissolution reactions will be collected for analysis via inductively coupled plasma mass spectrometry (ICP-MS) to monitor the preferential dissolution of different minerals in the rock. Direct simulation on 3D images from micro-tomography (μCT) and network modelling tools will be used for further analysis of the rock property evolution. In this thesis we study dissolution of carbonate minerals with an increasing level of complexity to observe the effect of chemical and physical heterogeneity. We start with a single mineral dolomite case where we investigate the impact of rock heterogeneity and flowrate on reaction rates and dissolution dynamics. Next we study dissolution in a chemically heterogeneous medium consisting of two minerals with contrasting initial structure and transport properties, but with uniform spatial distribution. Finally, we studied a heterogeneous reservoir sample consisting of dolomite and calcite (having the ratio 8 to 1) which had a non-uniform spatial distribution.
Additional file 1 of Automated cardiovascular magnetic resonance image analysis with fully convolutional networks
Creators: name: Wenjia Bai
name: Sinclair, Matthew
name: Tarroni, Giacomo
name: Oktay, Ozan
name: Rajchl, Martin
name: Vaillant, Ghislain
name: Lee, Aaron
name: Aung, Nay
name: Lukaschuk, Elena
name: Mihir Sanghvi
name: Zemrak, Filip
name: Fung, Kenneth
name: Paiva, Jose
name: Carapella, Valentina
name: Kim, Young
name: Suzuki, Hideaki
name: Kainz, Bernhard
name: Matthews, Paul
name: Petersen, Steffen
name: Piechnik, Stefan
name: Neubauer, Stefan
name: Glocker, Ben
name: Rueckert, Daniel
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Image demonstrating visual assessment and comparison between automated segmentation and manual segmentation. (PDF 210 kb)
Group actions on treelike compact spaces
Creators: name: Glasner, Eli
name: Megrelishvili, Michael
Publisher: name: arXiv
Year: 2018
Subjects: subject: Dynamical Systems (math.DS)
subject: Functional Analysis (math.FA)
subject: General Topology (math.GN)
subject: FOS: Mathematics
subject: 37Bxx, 54H20, 54H15, 22A25

description: We show that group actions on many treelike compact spaces are not too complicated dynamically. We first observe that an old argument of Seidler implies that every action of a topological group $G$ on a regular continuum is null and therefore also tame. As every local dendron is regular, one concludes that every action of $G$ on a local dendron is null. We then use a more direct method to show that every continuous group action of $G$ on a dendron is Rosenthal representable, hence also tame. Similar results are obtained for median pretrees. As a related result we show that Helly's selection principle can be extended to bounded monotone sequences defined on median pretrees (e.g., dendrons or linearly ordered sets). Finally, we point out some applications of these results to continuous group actions on dendrites.
description: 22 pages
Lithium Production in Companions of Accreting X-Ray Binaries by Neutron Spallation of C,N,O Elements
Creators: name: Guessoum, Nidhal
name: Kazanas, Demosthenes
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the processes which could lead to the observed enhancement of Li and possibly other light elements (Be, B) in the companions of a number of X-ray novae. We conclude that one of the most promising mechanisms is the spallation of CNO elements on the surface of the companion induced by the neutron flux produced in the hot accretion flow onto the compact object. Direct production of the observed Li and its deposition onto the dwarf companion seem less likely, mainly because of the possibility of its destruction in the production region itself and difficulties in its deposition associated with the configuration of the companion's magnetic field. We discuss other potential observables of the above scenario.
description: 23 pages Latex, of which 5 pages of tables, to appear in the Astrophysical Journal, Vol 512, Feb 10 issue
Additional file 2: of Trends in healthcare utilization and costs associated with pneumonia in the United States during 2008â 2014
Creators: name: Tong, Sabine
name: Amand, Caroline
name: Kieffer, Alexia
name: Kyaw, Moe
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Table S2. Demographic characteristics of pneumonia patients by year. (DOCX 15 kb)
Orthosymplectic $Z_2\times Z_2$-graded Lie superalgebras and parastatistics
Creators: name: Stoilova, N. I.
name: Van der Jeugt, J.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Group Theory (math.GR)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: A $Z_2\times Z_2$-graded Lie superalgebra $g$ is a $Z_2\times Z_2$-graded algebra with a bracket $[.,.]$ that satisfies certain graded versions of the symmetry and Jacobi identity. In particular, despite the common terminology, $g$ is not a Lie superalgebra. We construct the most general orthosymplectic $Z_2\times Z_2$-graded Lie superalgebra $osp(2m_1+1,2m_2|2n_1,2n_2)$ in terms of defining matrices. A special case of this algebra appeared already in work of Tolstoy in 2014. Our construction is based on the notion of graded supertranspose for a $Z_2\times Z_2$-graded matrix. Since the orthosymplectic Lie superalgebra $osp(2m+1|2n)$ is closely related to the definition of parabosons, parafermions and mixed parastatistics, we investigate here the new parastatistics relations following from $osp(2m_1+1,2m_2|2n_1,2n_2)$. Some special cases are of particular interest, even when one is dealing with parabosons only.
Alauda arvensis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Alaudidae
Alauda
Alauda arvensis

description: Alauda arvensis [spec. nov.]
A. rectricibus extimis duabus extrorsum longitudinaliter albis: intermediis interiori latere ferrugineis. Fn. svec. 190.
Alauda non cristata. Gesn. av. 78. Aldr. orn. l. 18. c. 12.
Alauda vulgaris. Will. orn. 149. t. 40. Raj. av. 69. n. 1. Alb. av. 1. p. 39. t. 41.
Alauda arvorum. Frisch. av. 3. t. 15. f. 1.
Alauda coelipeta. Klein. av. 71.
Habitat in Europae apricis.
Volata perpendiculari in a�re suspensa cantillat:
Ecce suum tirile, tirile, suum tirile tractat;
Autumno sole occidente in retia compellitur.
Hyeme pinguescit in australioribus carne sapidissima zj.
Calculosis noxia.
Columbas ad Passeres nec ad Gallinas pertinere, docet monogamia, osculatio, incubatus alternus, nutritio pulli, Ova pauca, nidificatio, locus in altis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 165, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Obscuration of the Parsec Scale Jets in the Compact Symmetric Object 1946+708
Creators: name: Peck, A. B.
name: Taylor, G. B.
name: Conway, J. E.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results of VLA and VLBA observations of the 1.420 GHz neutral hydrogen absorption associated with the Compact Symmetric Object 1946+708 (z=0.101). We find significant structure in the gas on parsec scales. The peak column density in the HI (N_HI~2.2x10^23 cm^-2 (T_s/8000K)) occurs toward the center of activity of the source, as does the highest velocity dispersion (FWHM~350 \kms). In addition, we find that the continuum spectra of the various radio components associated with these jets strongly indicate free-free absorption. This effect is particularly pronounced toward the core and inner components of the receding jet, suggesting the presence of a screen local to the source, perhaps part of an obscuring torus.
description: revised version, some text added, 1 figure changed; accepted to Astrophysical Journal, 22 page LaTeX document includes 8 postscript figures
The origin and early evolution of a bipolar magnetic region in the solar photosphere
Creators: name: Getling, A. V.
name: Buchnev, A. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Finding the formation mechanisms for bipolar configurations of strong local magnetic field under control of the relatively weak global magnetic field of the Sun is a key problem of the physics of solar activity. This study is aimed at discriminating whether the magnetic field or fluid motion plays a primary, active role in this process. The very origin and early development stage of Active Region 12548 are investigated based on SDO/HMI observations of 2016 May 20--25. Full-vector magnetic and velocity fields are analyzed in parallel. The leading and trailing magnetic polarities are found to grow asymmetrically in terms of their amplitude, magnetic flux, and the time variation of these quantities. The leading-polarity magnetic element originates as a compact feature against the background of a distributed trailing-polarity field, with an already existing trailing-polarity magnetic element. No signs of strong horizontal magnetic fields are detected between the two magnetic poles. No predominant upflow between their future locations precedes the origin of this bipolar magnetic region (BMR); instead, upflows and downflows are mixed, with some prevalence of downflows. Any signs of a large-scale horizontal divergent flow from the area where the BMR develops are missing; in contrast, a normal supergranulation and mesogranulation pattern is preserved. This scenario of early BMR evolution is in strong contradiction with the expectations based on the model of a rising $Ω$-shaped loop of a flux tube of strong magnetic field, and an \emph{in situ} mechanism of magnetic-field amplification and structuring should operate in this case.
description: 11 pages, 5 figures
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Cart. 193 (11 H 78), f. 0041r
Creators: name: de la Côte d'Or, Archives départementales
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: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Archives départementales de la Côte-d'Or, Cart. 193 (11 H 78), f. 0041r, 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 IX, Archives départementales de la Côte-d'Or, Cart. 193 (11 H 78), f. 0041r, 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
Show, Attend and Translate: Unsupervised Image Translation with Self-Regularization and Attention
Creators: name: Yang, Chao
name: Kim, Taehwan
name: Wang, Ruizhe
name: Peng, Hao
name: Kuo, C. -C. Jay
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Image translation between two domains is a class of problems aiming to learn mapping from an input image in the source domain to an output image in the target domain. It has been applied to numerous domains, such as data augmentation, domain adaptation, and unsupervised training. When paired training data is not accessible, image translation becomes an ill-posed problem. We constrain the problem with the assumption that the translated image needs to be perceptually similar to the original image and also appears to be drawn from the new domain, and propose a simple yet effective image translation model consisting of a single generator trained with a self-regularization term and an adversarial term. We further notice that existing image translation techniques are agnostic to the subjects of interest and often introduce unwanted changes or artifacts to the input. Thus we propose to add an attention module to predict an attention map to guide the image translation process. The module learns to attend to key parts of the image while keeping everything else unaltered, essentially avoiding undesired artifacts or changes. The predicted attention map also opens door to applications such as unsupervised segmentation and saliency detection. Extensive experiments and evaluations show that our model while being simpler, achieves significantly better performance than existing image translation methods.
description: Accepted at IEEE Transactions on Image Processing (TIP)
SOSA: A Lightweight Ontology for Sensors, Observations, Samples, and Actuators
Creators: name: Janowicz, Krzysztof
name: Haller, Armin
name: Cox, Simon J D
name: Phuoc, Danh Le
name: Lefrancois, Maxime
Publisher: name: arXiv
Year: 2018
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: The Sensor, Observation, Sample, and Actuator (SOSA) ontology provides a formal but lightweight general-purpose specification for modeling the interaction between the entities involved in the acts of observation, actuation, and sampling. SOSA is the result of rethinking the W3C-XG Semantic Sensor Network (SSN) ontology based on changes in scope and target audience, technical developments, and lessons learned over the past years. SOSA also acts as a replacement of SSN's Stimulus Sensor Observation (SSO) core. It has been developed by the first joint working group of the Open Geospatial Consortium (OGC) and the World Wide Web Consortium (W3C) on \emph{Spatial Data on the Web}. In this work, we motivate the need for SOSA, provide an overview of the main classes and properties, and briefly discuss its integration with the new release of the SSN ontology as well as various other alignments to specifications such as OGC's Observations and Measurements (O\&M), Dolce-Ultralite (DUL), and other prominent ontologies. We will also touch upon common modeling problems and application areas related to publishing and searching observation, sampling, and actuation data on the Web. The SOSA ontology and standard can be accessed at \url{https://www.w3.org/TR/vocab-ssn/}.
Heavy element abundances in blue compact galaxies
Creators: name: Izotov, Y. I.
name: Thuan, T. X.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present high-quality ground-based spectroscopic observations of 54 supergiant H II regions in 50 low-metallicity blue compact galaxies with oxygen abundances 12 + log O/H between 7.1 and 8.3. We use the data to determine abundances for the elements N, O, Ne, S, Ar and Fe. We also analyze Hubble Space Telescope (HST) Faint Object Spectrograph archival spectra of 10 supergiant H II regions to derive C and Si abundances in a subsample of 7 BCGs. The main result of the present study is that none of the heavy element-to-oxygen abundance ratios studied here (C/O, N/O, Ne/O, Si/O, S/O, Ar/O, Fe/O) depend on oxygen abundance for BCGs with 12 + log O/H < 7.6 (Z < Zsun/20). This constancy implies that all these heavy elements have a primary origin and are produced by the same massive (M > 10Msun) stars responsible for O production. The dispersion of the C/O and N/O ratios in these galaxies is found to be remarkably small, being only +/-0.03 dex and +/-0.02 dex respectively. This very small dispersion is strong evidence against any time-delayed production of C and primary N in the lowest-metallicity BCGs (secondary N production is negligible at these low metallicities). The absence of a time-delayed production of C and N is consistent with the scenario that galaxies with 12 + log O/H < 7.6 are undergoing now their first burst of star formation, and that they are therefore young, with ages not exceeding 40 Myr. If very low metallicities BCGs are indeed young, this would argue against the commonly held belief that C and N are produced by intermediate-mass (3Msun < M < 9Msun) stars at very low metallicities, as these stars would not have yet completed their evolution in these lowest metallicity galaxies.
description: 37 pages, 5 EPS figures, to appear in ApJ, February 1999
Propositional fuzzy logics: Tableaux and strong completeness
Creators: name: Kulacka, Agnieszka
Publisher: name: Imperial College London
Year: 2017

description: In his famous book Mathematical Fuzzy Logic, Petr Hajek defined a new fuzzy logic, which he called BL. It is weaker than the three fundamental fuzzy logics Product, Lkasiewicz and Godel, which are in turn weaker than classical logic, but axiomatic systems for each of them can be obtained by adding axioms to BL. Thus, Hajek placed all these logics in a unifying axiomatic framework. In this dissertation, two problems concerning BL and other fuzzy logics have been considered and solved. One was to construct tableaux for BL and for BL with additional connectives. Tableaux are automatic systems to verify whether a given formula must have given truth values, or to build a model in which it does not have these specific truth values. The other problem that was solved is to construct strongly standard complete axiomatic systems for BL, Lukasiewicz and Product logics, which was done by extending Hajek's axiomatic systems for them by an infinitary rule.
Alauda pratensis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Alaudidae
Alauda
Alauda pratensis

description: Alauda pratensis [spec. nov.]
A. rectricibus extimis duabus extrorsum albis, linea superciliorum alba. Fn. svec. 191.
Alauda pratorum. Aldr. orn. l. 18. c. 15. Will. orn. 150. Raj. av. 69. n. 3. Olin. av. 27.
Alauda sylvestris. Alb. av. 1. p. 40. t. 42.
Habitat in Europae pratis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 166, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
ASCA Discovery of an X-ray Pulsar in the Error Box of SGR1900+14
Creators: name: Hurley, K.
name: Li, P.
name: Kouveliotou, C.
name: Murakami, T.
name: Ando, M.
name: Strohmayer, T.
name: van Paradijs, J.
name: Vrba, F.
name: Luginbuhl, C.
name: Yoshida, A.
name: Smith, I.
name: Kulkarni, S.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a 2 - 10 keV ASCA observation of the field around the soft gamma repeater SGR1900+14. One quiescent X-ray source was detected in this observation, and it was in the SGR error box. In 2 - 10 keV X-rays, its spectrum may be fit by a power law with index -2.2, and its unabsorbed flux is 9.6 x 10^-12 erg cm^-2 s^-1. We also find a clear 5.16 s period. The properties of the three well-studied soft gamma repeaters are remarkably similar to one another, and provide evidence that all of them are associated with young, strongly magnetized neutron stars in supernova remnants.
description: Accepted for publication in the Astrophysical Journal Letters
Additional file 2: of Reduced intrinsic DNA curvature leads to increased mutation rate
Creators: name: Chaorui Duan
name: Huan, Qing
name: Xiaoshu Chen
name: Shaohuan Wu
name: Carey, Lucas
name: Xionglei He
name: Wenfeng Qian
Publisher: name: figshare
Year: 2018
Subjects: Biophysics
Medicine
Developmental Biology

description: Review history. (DOCX 41 kb)
Toughening of unsaturated polyester resin by solid elastomers and liquid rubbers_A Review.pdf
Creators: name: M. P., Chandresh
name: Dechamma C. D.,, Ani
name: M., Bhavana
name: N., Rameshwara
name: S., Roopa
Publisher: name: figshare
Year: 2021
Subjects: subject: 91209 Polymers and Plastics
subject: FOS: Materials engineering

description: Unsaturated polyester (USP) resins are thermosetting polymers that have been known for many years for its thermal and chemical resistance. They are widely used matrices for composite applications. However, their low toughness makes them limited for the applications where toughness becomes a critical property. Thus, these resins need to be modified by toughening agents (tougheners) to improve their fracture toughness or increase their impact resistance. In order to improve the toughness of USP resins, researchers have used different material incorporations viz. elastomers, thermoplastics, and particulate / fibrous fillers into the USP matrix. The intent of this paper is to review the varied research that has been performed to improve the toughness of USP resin by elastomer modification. This review summarizes the effect of various elastomers (both solid elastomers and liquid rubbers) on the toughness of the USP resin. It also covers the chemical modifications employed with those elastomeric tougheners, and the additional incorporation of certain fillers, which have resulted in much higher toughness along with combating other property reduction due to softer elastomeric inclusions.
Additional file 1: of Trends in healthcare utilization and costs associated with pneumonia in the United States during 2008â 2014
Creators: name: Tong, Sabine
name: Amand, Caroline
name: Kieffer, Alexia
name: Kyaw, Moe
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Table S1. International Classification of Diseases, 9th revision, Clinical Modification (ICD-9-CM) codes used. (DOCX 13 kb)
Investigating Functional Redundancies in the Context of Vehicle Automation - A Trajectory Tracking Perspective
Creators: name: Stolte, Torben
name: Liao, Tianyu
name: Nee, Matthias
name: Nolte, Marcus
name: Maurer, Markus
Publisher: name: arXiv
Year: 2018
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Level 3+ automated driving implies highest safety demands for the entire vehicle automation functionality. For the part of trajectory tracking, functional redundancies among all available actuators provide an opportunity to reduce safety requirements for single actuators. Yet, the exploitation of functional redundancies must be well argued if employed in a safety concept as physical limits can be reached. In this paper, we want to examine from a trajectory tracking perspective whether such a concept can be used. For this, we present a model predictive fault-tolerant trajectory tracking approach for over-actuated vehicles featuring wheel individual all-wheel drive, brakes, and steering. Applying this approach exemplarily demonstrates for a selected reference trajectory that degradations such as missing or undesired wheel torques as well as reduced steering dynamics can be compensated. Degradations at the physical actuator limits lead to significant deviations from the reference trajectory while small constant steering angles are partially critical.
description: 8 pages, 6 figures, 3 tables, presented at the 2018 21st International Conference on Intelligent Transportation Systems (ITSC), Maui, HI, USA
Diffuse Gamma-Ray Emission from Starburst Galaxies and M31
Creators: name: Blom, Jan J.
name: Paglione, Timothy A. D.
name: Carraminana, Alberto
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a search for high energy gamma-ray emission from 9 nearby starburst galaxies and M31 with the EGRET instrument aboard CGRO. Though the diffuse gamma-ray emission from starburst galaxies was suspected to be detectable, we find no emission from NGC 253, M82 nor from the average of all 9 galaxies. The 2 sigma upper limit for the EGRET flux above 100 MeV for the averaged survey observations is 1.8 x 10-8 ph cm-2 s-1. From a model of the expected radio and gamma-ray emission, we find that the magnetic field in the nuclei of these galaxies is > 25 micro Gauss, and the ratio of proton and electron densities is < 400. The EGRET limits indicate that the rate of massive star formation in the survey galaxies is only about an order of magnitude higher than in the Milky Way. The upper limit to the gamma-ray flux above 100 MeV for M31 is 1.6 x 10-8 ph cm-2 s-1. At the distance of M31, the Milky Way flux would be over twice this value, indicating higher gamma-ray emissivities in our Galaxy. Therefore, since the supernova rate of the Milky Way is higher than in M31, our null detection of M31 supports the theory of the supernova origin of cosmic rays in galaxies.
description: 17 pages, plus 1 Postscript figure, AAS Latex macros v4.0, accepted for publication in ApJ Main Journal