cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: 01_1813
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
NGC1614: A Laboratory for Starburst Evolution
Creators: name: Alonso-Herrero, A.
name: Engelbracht, C. W.
name: Rieke, M. J.
name: Rieke, G. H.
name: Quillen, A. C.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The modest extinction and reasonably face-on viewing geometry make the luminous IR galaxy NGC1614 an ideal laboratory for study of a powerful starburst. HST/NICMOS observations show: 1.) deep CO stellar absorption, tracing a starburst nucleus about 45 pc in diameter; 2.) surrounded by a ~600 pc diameter ring of supergiant HII regions revealed in Pa$α$ line emission; 3.) lying within a molecular ring indicated by its extinction shadow in H-K; 4.) all at the center of a disturbed spiral galaxy. The luminosities of the giant HII regions in the ring are extremely high, an order of magnitude brighter than 30 Doradus. The relation of deep stellar CO bands to surrounding ionized gas ring to molecular gas indicates that the luminous starburst started in the nucleus and is propagating outward into the surrounding molecular ring. This hypothesis is supported by evolutionary starburst modeling that shows that the properties of NGC1614 can be fitted with two short-lived bursts of star formation separated by 5 Myr. The total dynamical mass of the starburst region of 1.3x10^9 Msol is mostly accounted for by the old pre-star burst stellar population. Although our starburst models use a modified Salpeter IMF, the tight mass budget suggests that the IMF may contain relatively more 10-30 Msol stars and fewer low mass stars than the Salpeter function. The dynamical mass is nearly 4 times smaller than the mass of molecular gas estimated from the standard ratio of 12CO(1-0) to H2. A number of arguments place the mass of gas in the starburst region at ~25% of the dynamical mass, nominally about 1/15 and with an upper limit of 1/10 of the amount estimated from 12CO and the standard ratio. (Abridged)
description: Accepted for publication in ApJ. 20 pages (uses emulateapj)
title: wala
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Japhug
subject: jya

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Nucleation Kinetics in Al-Sm Metallic Glasses
Creators: name: Zhao, L.
name: Bokas, G. B.
name: Perepezko, J. H.
name: Szlufarska, I.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The isothermal nucleation kinetics in Al-Sm metallic glasses with low Sm concentrations (xSm) was studied using molecular dynamics simulations in order to calculate time-temperature-transformation curves. The average delay time of Al nanocrystal nucleation was found to increase exponentially with xSm, whereas the estimated critical cooling rate necessary to avoid crystallization decreases exponentially with xSm. Sm solutes were found to suppress Al nucleation by increasing the attachment barrier and therefore by reducing the attachment frequency. The analysis shows that the attachment of Al to the evolving nucleus has the same characteristics as Al diffusion within the amorphous matrix and they both take place heterogeneously via collective movement of a group of Al atoms.
title: poucet1
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Japhug
subject: jya

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Memoria Curso Académico 2011-2012
Creators: name: CSIC-JA-UPO-Centro Andaluz De Biología Del Desarrollo (CABD)
Publisher: name: CSIC-JA-UPO - Centro Andaluz de Biología del Desarrollo (CABD)
Year: 2012

description: El CABD está especializado en el estudio de la Biología del Desarrollo. Esta especialidad investiga los mecanismos genéticos y moleculares que controlan cómo las células crecen, se comunican y se diferencian formando órganos complejos. Se ha comprobado que el funcionamiento anómalo de los genes que controlan el desarrollo de los organismos causa numerosas enfermedades. Por tanto, el conocimiento de la función normal de estos genes ayudará a diseñar nuevas estrategias para prevenir o curar estos problemas. Actualmente el centro lo ocupan 17 grupos trabajando en desarrollo de ratón, pez cebra, Xenopus, Drosophila y Caenorhabditis, así como estudiando control del ciclo celular en levaduras, regulación génica en bacterias y estrés oxidativo. El Centro está cofinanciado por el Consejo Superior de Investigaciones Científicas (CSIC), la Junta de Andalucía y la Universidad Pablo de Olavide (UPO), de Sevilla. La edificación y el equipamiento fueron costeados con fondos de la Unión Europea.
Characterizing magnetic field morphologies in Class 0 protostellar cores with ALMA
Creators: name: Le Gouellec, Valentin
Publisher: name: Zenodo
Year: 2019

description: Recent ALMA observations have continued to clarify the role of the magnetic field in the earliest phase of star formation. Here I will present new ALMA dust polarization observations of a small sample of Class 0 protostellar cores; the high angular resolution of these observations reveals several unexpected phenomena. First, we see unpredicted, very high polarization fractions along the outflow cavity walls surrounding the extremely high velocity (EHV) molecular jet of Serpens Emb 8(N). Our investigations of outflow and dense-gas properties, and their correlation with the polarized emission in this source, allow us to better understand the local conditions necessary for the occurrence of Radiative Alignment Torques (RATs), which align dust grains with respect to the magnetic field. Second, maps of the intermediate-mass protostar Serpens SMM1, and in particular the inner core of SMM1-a, present a polarization pattern that exhibits a poloidal magnetic field at the bases of the two lobes of the bipolar outflow. Notably, at the base of the EHV jet in the redshifted lobe, there is a highly polarized spot with a local magnetic field aligned with the direction of the jet. The high polarization fractions encountered in these two protostars lead us to propose that additional grain-alignment mechanisms may be causing this enhanced polarization. We propose that the enhanced polarization seen along outflow cavity walls in Class 0 protostars is caused by irradiation of the cavities by accretion processes and outflow shocks. However, to align dust grains deep in the walls of the cavity and to cause the high polarization fraction that we see, we find that longer-wavelength (i.e., (sub)millimeter) photons may be necessary, which implies a degree of grain growth that is unexpected in Class 0 sources. Our observations allow us not only to constrain the different magnetic field morphologies within the central cores, along the outflow cavity walls, and in possible accretion streamers in our sources, but also to better understand grain alignment and grain growth in young star-forming sources.
Probabilistic eccentricity bifurcation for stars around shrinking massive black hole binaries
Creators: name: Iwasa, Mao
name: Seto, Naoki
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Based on the secular theory, we discuss the orbital evolution of stars in a nuclear star cluster to which a secondary massive black hole is infalling with vanishing eccentricity. We find that the eccentricities of the stars could show sharp transitions, depending strongly on their initial conditions. By examining the phase-space structure of an associated Hamiltonian, we show that these characteristic behaviors are partly due to a probabilistic bifurcation at a separatrix crossing, resulting from the retrograde apsidal precession by the cluster potential. We also show that separatrix crossings are closely related to realization of a large eccentricity and could be important for astrophysical phenomena such as tidal disruption events or gravitational wave emissions.
description: 19 pages, 20 figures, 4 tables. Accepted for publication in MNRAS
Additional file 2: of Expected and unexpected evolution of plant RNA editing factors CLB19, CRR28 and RARE1: retention of CLB19 despite a phylogenetically deep loss of its two known editing targets in Poaceae
Creators: name: Hein, Anke
name: Knoop, Volker
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Phylogeny of the RARE1 orthologs in angiosperms. Shown is a Maximum Likelihood tree (see Methods). (PDF 468Â kb)
Clustering of Galaxies with f(R) gravity
Creators: name: Capozziello, Salvatore
name: Faizal, Mir
name: Hameeda, Mir
name: Pourhassan, Behnam
name: Salzano, Vincenzo
name: Upadhyay, Sudhaker
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Based on thermodynamics, we discuss the galactic clustering of expanding Universe by assuming the gravitational interaction through the modified Newton's potential given by $f(R)$ gravity. We compute the corrected $N$-particle partition function analytically. The corrected partition function leads to more exact equations of states of the system. By assuming that system follows quasi-equilibrium, we derive the exact distribution function which exhibits the $f(R)$ correction. Moreover, we evaluate the critical temperature and discuss the stability of the system. We observe the effects of correction of $f(R)$ gravity on the power law behavior of particle-particle correlation function also. In order to check feasibility of an $f(R)$ gravity approach to the clustering of galaxies, we compare our results with an observational galaxy cluster catalog.
description: 14 pages, 8 figures, 1 table; accepted for publication on MNRAS
title: nWNa
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Japhug
subject: jya

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Properties of giant molecular clouds in a strongly barred galaxy NGC 1300
Creators: name: Maeda, Fumiya
Publisher: name: Zenodo
Year: 2019

description: Recent studies show that star formation efficiency (SFE) depends on galactic-scale environments. However, what controls the SFE within galaxies is still unclear. To clear the SF mechanism, it is important to study on extreme environments as a pilot study. Thus, we focus on a prototype strongly barred galaxy NGC 1300 which hosts extreme environments; the SFE of total molecular gas in the bar is 5 times smaller than that in the arm. In ALMA Cycle 5, we carried out 12CO(1−0) observations toward the western bar and arm regions of NGC 1300 with the 12-m array at a high angular resolution of ~40 pc to investigate the impact of the galactic environment on the properties of GMCs. We detected the GMC-like gas clouds associated with the dark lanes. We used the CPROPS package to identify GMCs and measured their physical properties. The parameters of CPROPS are the same as those used in the previous GMC study on a typical spiral galaxy M51 (Colombo et al. 2014). Typical values of basic properties of the GMCs are radius of 45 pc, velocity dispersion of 5 km/s, molecular gas mass of 6 × 10^5 Msun and virial parameter of 1.5, and these values are not significantly different in the bar, arm and bar end regions based on two-sided K-S test. This result suggests GMC properties themselves are unlikely to be the cause for the low SF efficiency in the bar. To further study on the cause of low SFE in bar regions, we compared the CO(1-0) data with Nobeyama 45-m single dish telescope and the12-m array data. We find that the recovery fraction of the molecular gases, or flux derived from the 12-m array/ flux derived from Nobeyama 45-m, tends to be smaller in the bar region (~0.4) than arm region (~0.9). Due to the lack of ACA (7m array + Total Power) data, the 12-m array data has no sensitivity on a large- scale structure; 50 % (10 %) flux for a Gaussian component with a FWHM of 500 pc (1 kpc) cannot be recovered based on the CASA simulation. Therefore, the tendency of the recovery fraction suggests that a large amount of extended molecular gas exists in the bar which would make the SFE low.
New concepts of inertial measurements with multi-species atom interferometry
Creators: name: Bonnin, Alexis
name: Diboune, Clément
name: Zahzam, Nassim
name: Bidel, Yannick
name: Cadoret, Malo
name: Bresson, Alexandre
Publisher: name: arXiv
Year: 2017
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: In the field of cold atom inertial sensors, we present and analyze innovative configurations for improving their measurement range and sensitivity, especially attracting for onboard applications. These configurations rely on multi-species atom interferometry, involving the simultaneous manipulation of different atomic species in a unique instrument to deduce inertial measurements. Using a dual-species atom accelerometer manipulating simultaneously both isotopes of rubidium, we report a preliminary experimental realization of original concepts involving the implementation of two atom interferometers first with different interrogation times and secondly in phase quadrature. These results open the door to a new generation of atomic sensors relying on high performance multi-species atom interferometric measurements.
Aspect-Based Relational Sentiment Analysis Using a Stacked Neural Network Architecture
Creators: name: Jebbara, Soufian
name: Cimiano, Philipp
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: Sentiment analysis can be regarded as a relation extraction problem in which the sentiment of some opinion holder towards a certain aspect of a product, theme or event needs to be extracted. We present a novel neural architecture for sentiment analysis as a relation extraction problem that addresses this problem by dividing it into three subtasks: i) identification of aspect and opinion terms, ii) labeling of opinion terms with a sentiment, and iii) extraction of relations between opinion terms and aspect terms. For each subtask, we propose a neural network based component and combine all of them into a complete system for relational sentiment analysis. The component for aspect and opinion term extraction is a hybrid architecture consisting of a recurrent neural network stacked on top of a convolutional neural network. This approach outperforms a standard convolutional deep neural architecture as well as a recurrent network architecture and performs competitively compared to other methods on two datasets of annotated customer reviews. To extract sentiments for individual opinion terms, we propose a recurrent architecture in combination with word distance features and achieve promising results, outperforming a majority baseline by 18% accuracy and providing the first results for the USAGE dataset. Our relation extraction component outperforms the current state-of-the-art in aspect-opinion relation extraction by 15% F-Measure.
title: ADCO, Cartulaire de l'abbaye de Saint-Seine (XIIIe siècle), Cart. 165 (10 H 6, ms. 139), 354 pages, f. 0216
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/2009
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de l'abbaye de Saint-Seine (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 165 (10 H 6, ms. 139), 354 pages, f. 0216, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'abbaye de Saint-Seine (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 165 (10 H 6, ms. 139), 354 pages, f. 0216, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Saint-Seine
description: Provenance: http://www.wikidata.org/entity/Q2820709
Additional file 1: of Information standards for recording alcohol use in electronic health records: findings from a national consultation
Creators: name: Haroon, Shamil
name: Wooldridge, Darren
name: Hoogewerf, Jan
name: Krishnarajah Nirantharakumar
name: Williams, John
name: Martino, Lina
name: Bhala, Neeraj
Publisher: name: figshare
Year: 2018
Subjects: Medicine
Molecular Biology
Biotechnology
Marine Biology
Cancer
Science Policy

description: This includes the survey questions and selected quotes (DOCX 33 kb)
title: qaprANar
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Japhug
subject: jya

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
title: VERTICAL DISPERSION AND OXYGEN DEMAND OF DEICING
Creators: name: Pereira, Marina S.
Publisher: name: University of Massachusetts Amherst
Year: 2008
Subjects: subject: DEICING AGENT CONTAMINANTS
subject: Environmental Engineering
subject: FOS: Environmental engineering

description: The research site is located in Plymouth, Massachusetts, above the Plymouth Carver Aquifer. It is positioned along side State Route 25 which opened in the summer of 1987 in order to extend Interstate 495 to the Bourne Bridge. Snow/ice removing measures using salt, and an alternate deicing agent, CMA have been practiced since the winter of 1987. The highway runoff is collected into an infiltration basin, allowing salt and CMA to infiltrate the sandy aquifer below. The salt and CMA increase the specific conductivity of the groundwater while, the infiltrated acetate is biodegraded, leading to DO depletion within the aquifer. Once anoxic conditions are reached, any further acetate loaded into the aquifer is degraded anaerobically. The objective of this research was to develop and calibrate, steady state, analytical models of specific conductivity and DO transport through the aquifer. The models feature advection, vertical dispersion and for the dissolved oxygen, first order decay. The vertical dispersivity parameter results would be used in the reactive model because it contributes to the mixing of the plume, therefore accounting for the microbial activity. The data used to calibrate the model included monthly groundwater measurements of specific conductivity and dissolved oxygen collected and analyzed from October 1999 - October 2007. Groundwater quality data were obtained from four clusters of a total of 3 7 monitoring wells that allowed for a more detailed study of the vertical variation of parameters. Other data used in this research included monthly rain data and the Massachusetts Highway Department reports of deicing agent solids applied over seven complete road-deicing seasons. The specific conductivity data calibrate the elevation of the plume bottom, the source concentration C~, and the vertical dispersivity. The bottom elevation decreases with distance from the basin as expected. The result for the second parameter searched in the transport model, C infinity was checked against the expected values based on the average amount of deicing agent applied yearly in the research area section ofSR-25. If the model is correct and the average C infinity predicted is as much as 1200 microsiemens / cm, then 56% of the deicing agent material drifted off the highway. The average vertical dispersivity result for all of the well clusters used in this project was 0.77 m. The first order decay rates results from the reactive transport model, suggest that the decay rate is zero order near the source and first order within time and distance away from the source. This behavior is exhibited in a Michaelis-Menten kinetics model.
Properties of the multicritical point of +/- J Ising spin glasses on the square lattice
Creators: name: Lessa, Jean C.
name: de Queiroz, S. L. A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We use numerical transfer-matrix methods to investigate properties of the multicriticalpoint of binary Ising spin glasses on a square lattice, whose location we assume to be given exactly by a conjecture advanced by Nishimori and Nemoto. We calculate the two largest Lyapunov exponents, as well as linear and non-linear zero-field uniform susceptibilities, on strip of widths $4 \leq L \leq 16$ sites, from which we estimate the conformal anomaly $c$, the decay-of-correlations exponent $η$, and the linear and non-linear susceptibility exponents $γ/ν$ and $γ^{nl}/ν$, with the help of finite-size scaling and conformal invariance concepts. Our results are: $c=0.46(1)$; $0.187 \lesssim η\lesssim 0.196$; $γ/ν=1.797(5)$; $γ^{nl}/ν=5.59(2)$. A direct evaluation of correlation functions on the strip geometry, and of the statistics of the zeroth moment of the associated probability distribution, gives $η=0.194(1)$, consistent with the calculation via Lyapunov exponents. Overall, these values tend to be inconsistent with the universality class of percolation, though by small amounts. The scaling relation $γ^{nl}/ν=2 γ/ν+d$ (with space dimensionality $d=2$) is obeyed to rather good accuracy, thus showing no evidence of multiscaling behavior of the susceptibilities.
description: RevTeX 4, 7 pages, 4 .eps figures; final version, to be published in Physical Review B (2006)
Condensates and Singularities in String Theory
Creators: name: Kostelecky, Alan
name: Perry, Malcolm
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We derive a class of solutions to the string sigma-model equations for the closed bosonic string. The tachyon field is taken to form a constant condensate and the beta-function equations at one-loop level are solved for the evolution of the metric and the dilaton. The solutions represent critical string theories in arbitrary dimensions. The spectrum of the subclass of models with a linearly rising asymptotic dilaton is found using the Feigin-Fuks method. Certain approximate solutions arising in string field theory are used to illustrate the results explicitly. An argument based on conformal invariance leads to the conjecture that that stringy corrections to at least some singular spacetimes in general relativity result in non-singular metrics. We use the singularities of the big-bang/crunch type appearing in our models to examine this conjecture.
description: 20 pages, DAMTP-R92-40, IUHET 242
Fully differential NNLO computations with MATRIX
Creators: name: Grazzini, Massimiliano
name: Kallweit, Stefan
name: Wiesemann, Marius
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present the computational framework MATRIX which allows us to evaluate fully differential cross sections for a wide class of processes at hadron colliders in next-to-next-to-leading order (NNLO) QCD. The processes we consider are $2\to 1$ and $2\to 2$ hadronic reactions involving Higgs and vector bosons in the final state. All possible leptonic decay channels of the vector bosons are included for the first time in the calculations, by consistently accounting for all resonant and non-resonant diagrams, off-shell effects and spin correlations. We briefly introduce the theoretical framework MATRIX is based on, discuss its relevant features and provide a detailed description of how to use MATRIX to obtain NNLO accurate results for the various processes. We report reference predictions for inclusive and fiducial cross sections of all the physics processes considered here and discuss their corresponding uncertainties. MATRIX features an automatic extrapolation procedure that allows us, for the first time, to control the systematic uncertainties inherent to the applied NNLO subtraction procedure down to the few permille level (or better).
description: 76 pages, 2 figures, 11 tables
Aspect-Based Sentiment Analysis Using a Two-Step Neural Network Architecture
Creators: name: Jebbara, Soufian
name: Cimiano, Philipp
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: The World Wide Web holds a wealth of information in the form of unstructured texts such as customer reviews for products, events and more. By extracting and analyzing the expressed opinions in customer reviews in a fine-grained way, valuable opportunities and insights for customers and businesses can be gained. We propose a neural network based system to address the task of Aspect-Based Sentiment Analysis to compete in Task 2 of the ESWC-2016 Challenge on Semantic Sentiment Analysis. Our proposed architecture divides the task in two subtasks: aspect term extraction and aspect-specific sentiment extraction. This approach is flexible in that it allows to address each subtask independently. As a first step, a recurrent neural network is used to extract aspects from a text by framing the problem as a sequence labeling task. In a second step, a recurrent network processes each extracted aspect with respect to its context and predicts a sentiment label. The system uses pretrained semantic word embedding features which we experimentally enhance with semantic knowledge extracted from WordNet. Further features extracted from SenticNet prove to be beneficial for the extraction of sentiment labels. As the best performing system in its category, our proposed system proves to be an effective approach for the Aspect-Based Sentiment Analysis.
Geometric properties of Cesaro averaging operators
Creators: name: Sangal, Priyanka
name: Swaminathan, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Complex Variables (math.CV)
subject: FOS: Mathematics
subject: 30C45, 00A30

description: In this paper, using positivity of trigonometric cosine and sine sums whose coefficients are generalization of Vietoris numbers, we find the conditions on the coefficient $\{a_k\}$ to characterize the geometric properties of the corresponding analytic function $f(z)=z+\displaystyle\sum_{k=2}^{\infty} a_kz^k$ in the unit disc $\mathbb{D}$. As an application we also find geometric properties of a generalized Cesàro type polynomials.
description: 15 pages
title: Testing of $31cm times 31cm$ GEM Chamber at COSY
Creators: name: Adak, R. P.
name: Dubey, A. K.
name: Saini, J.
name: Jain, V.
name: Chattopadhyay, S.
name: Das, S.
name: Frankefeld, U.
name: Henner, J.
name: Niebur, W.
name: Sorokin, I.
name: Blog, T.
name: Uhlig, F.
name: Friese, V.
name: Ghosh, P.
name: Heuser, J.
Publisher: name: GSI Helmholtzzentrum fuer Schwerionenforschung, Darmstadt
Year: 2014
Subjects: Physics

description: GSI Scientific Report 2013 - GSI Report 2014-1
The EU's Clean Industrial Deal: A Defining Moment for Europe's Industrial Future
Creators: name: Orayeva, Jennet
Publisher: name: Zenodo
Year: 2025

description: The EU Commission recently announced the Clean Industrial Deal to claim global leadership in the race for industrial decarbonisation. What does this mean for Europe's industrial future, and how can EU-funded R&I projects contribute to its success? Find out in this article authored by RTDS communication expert Jennet Orayeva. The original article is available on the RTDS Group website: https://www.rtds-group.com/news/eu-clean-industrial-deal/
title: Candidature projet QUAETMARMED 2015
Creators: name: MMSH (USR 3125) / CNE (UMR 8562)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2019

description: Projet Questionner le monde méditerranéen : les outils qui ont fait les sciences sociales en Méditerranée, porté par Véronique Ginouvès (MMSH) et Christelle Rabier (Centre Norbert Elias), en 2015
title: Distributed practice in mathematics: Recommendable especially for students on a medium performance level?
Creators: name: Barzagar Nazari, Katharina
name: Ebersbach, Mirjam
Publisher: name: Universität Kassel
Year: 2019
Subjects: subject: desirable difficulties
subject: distributed practice
subject: spacing effect
subject: mathematics
subject: school
subject: 150
subject: Mathematikunterricht
subject: Lerntechnik
subject: Experimentelle Psychologie

description: This research was funded by the LOEWE Excellence Initiative of the State of Hesse, Germany, as part of the project “Desirable Difficulties in Learning” (2015–2018)
Hyperbolic relaxation of the 2D Navier-Stokes equations in a bounded domain
Creators: name: Ilyin, Alexei
name: Rykov, Yuri
name: Zelik, Sergey
Publisher: name: arXiv
Year: 2017
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35B40, 35B45

description: A hyperbolic relaxation of the classical Navier-Stokes problem in 2D bounded domain with Dirichlet boundary conditions is considered. It is proved that this relaxed problem possesses a global strong solution if the relaxation parameter is small and the appropriate norm of the initial data is not very large. Moreover, the dissipativity of such solutions is established and the singular limit as the relaxation parameter tends to zero is studied
The dark matter effect on realistic equation of state in neutron stars
Creators: name: Panotopoulos, Grigoris
name: Lopes, Ilidio
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this work we apply relativistic mean-field theory in neutron stars assuming that fermionic dark matter is trapped inside the star and interacts directly with neutrons by exchanging Standard Model Higgs bosons. For realistic values of the parameters of the model we compute numerically the equation of state, and we compare it to the standard one. Furthermore, the mass-to-radius relation for both equations of state (pure neutron matter as well as admixed DM-neutron star) is shown, and the highest star mass for both cases is reported.
description: 6 pages, 3 figures, to appear in PRD
Transition from synchronous to asynchronous superfluid phase slippage in an aperture array
Creators: name: Sato, Y.
name: Hoskinson, E.
name: Packard, R. E.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We have investigated the dynamics of superfluid phase slippage in an array of apertures. The magnitude of the dissipative phase slips shows that they occur simultaneously in all the apertures when the temperature is around 10 mK below the superfluid transition, and subsequently lose their simultaneity as the temperature is lowered. We find that when periodic synchronous phase slippage occurs, the synchronicity exists from the very first phase slip, and therefore is not due to mode locking of interacting oscillators. When the system is allowed to relax freely from a given initial energy, the total number of phase slips that occur and the energy left in the system after the last phase slip depends reproducibly on the initial energy. We find the energy remaining after the final phase slip is a periodic function of the initial system energy. This dependence directly reveals the discrete and dissipative nature of the phase slips and is a powerful diagnostic for investigation of synchronicity in the array. When the array slips synchronously, this periodic energy function is a sharp sawtooth. As the temperature is lowered and the degree of synchronicity drops, the peak of this sawtooth becomes rounded, suggesting a broadening of the time interval over which the array slips. The underlying mechanism for the higher temperature synchronous behavior and the following loss of synchronicity at lower temperatures is not yet understood. We discuss the implications of our measurements and pose several questions that need to be resolved by a theory explaining the synchronous behavior in this quantum system. An understanding of the array phase slip process is essential to the optimization of superfluid `dc-SQUID' gyroscopes and interferometers.
description: 10 pages, 4 figures
Mechanisms of Lipid Modulation and Agonist Activation in the Muscle Nicotinic Acetylcholine Receptor
Creators: name: Thompson, Mackenzie
Publisher: name: Université d'Ottawa / University of Ottawa
Year: 2024
Subjects: Biophysics
Electrophysiology
Cryo-EM
nAChR
Lipid modulation
Activation

description: The muscle nicotinic acetylcholine receptor (nAChR) is a synaptic receptor that mediates neuromuscular communication by allowing cations to flow into a skeletal muscle cell in response to acetylcholine (ACh) binding. ACh binding transiently converts the nAChR from a non-conductive resting state to a conductive open state, increasing the intracellular voltage, ultimately leading to muscle contraction. The composition of the surrounding lipid environment also influences the stabilities of these, and other, conformational states to modulate nAChR function. While there is a reasonable understanding of what conformational states agonists and lipids stabilize to exert their effects, the mechanisms by which they do so remain enigmatic. In this thesis, the structural mechanisms of agonist activation and lipid modulation are explored using a combination of screening mutagenesis and electrophysiology. In manuscripts 1 and 2 extensive functional characterization of the peripheral M4 α-helices in the nAChR transmembrane domain (TMD) is used to explore different potential pathways of lipid modulation. Lipid modulation is suggested to occur through unique and independent mechanisms in each nAChR subunit that add together to account for the dramatic effects of lipids on nAChR function. In manuscript 3 new nAChR structures in apo and agonist bound states are used to guide a functional characterization of the interface between the extracellular domain (ECD) and the TMD, which is responsible for coupling agonist binding to channel gating. The new structures, which contradict previously reported mechanisms of nAChR activation, highlight conformational asymmetry at the ECD - TMD interface in α versus non-α subunits. We propose that agonist binding allows local "tension" at the ECD - TMD interfaces of the α subunits to "relax" to a conformationally symmetric active state. The results of these studies enhance our understanding of the mechanisms that underly allosteric transitions in the nAChR.
Turbulent density fluctuations and proton heating rate in the solar wind from 9-20~R_{\odot}
Creators: name: Raja, K. Sasikumar
name: Subramanian, Prasad
name: Ramesh, R.
name: Vourlidas, Angelos
name: Ingale, Madhusudan
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We obtain scatter broadened images of the Crab Nebula at 80 MHz as it transits through the inner solar wind in June 2016 and 2017. These images are anisotropic, with the major axis oriented perpendicular to the radially outward coronal magnetic field. Using these data, we deduce that the density modulation index (δN_e/N_e) caused by turbulent density fluctuations in the solar wind ranges from 1.9 \times 10^{-3} to 7.7 \times 10^{-3} between 9-20 R_{\odot}. We also find that the heating rate of solar wind protons at these distances ranges from 2.2 \times 10^{-13} to 1.0 \times 10^{-11} ~erg~cm^{-3}~s^{-1}. On two occasions, the line of sight intercepted a coronal streamer. We find that the presence of the streamer approximately doubles the thickness of the scattering screen.
description: to appear in The Astrophysical Journal
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Cart. 185 (11 H 70), f. 0062r
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: 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 général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0062r, 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 I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0062r, 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
A waveform model for eccentric binary black hole based on effective-one-body-numerical-relativity (EOBNR) formalism
Creators: name: Cao, Zhoujian
name: Han, Wen-Biao
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Binary black hole systems are among the most important sources for gravitational wave detection. And also they are good objects for theoretical research for general relativity. Gravitational waveform template is important to data analysis. Effective-one-body-numerical-relativity (EOBNR) model has played an essential role in the LIGO data analysis. For future space-based gravitational wave detection, many binary systems will admit somewhat orbit eccentricity. At the same time the eccentric binary is also an interesting topic for theoretical study in general relativity. In this paper we construct the first eccentric binary waveform model based on effective-one-body-numerical-relativity framework. Our basic assumption in the model construction is that the involved eccentricity is small. We have compared our eccentric EOBNR model to the circular one used in LIGO data analysis. We have also tested our eccentric EOBNR model against to another recently proposed eccentric binary waveform model; against to numerical relativity simulation results; and against to perturbation approximation results for extreme mass ratio binary systems. Compared to numerical relativity simulations with eccentricity as large as about 0.2, the overlap factor for our eccentric EOBNR model is better than 0.98 for all tested cases including spinless binary and spinning binary; equal mass binary and unequal mass binary. Hopefully our eccentric model can be the start point to develop a faithful template for future space-based gravitational wave detectors.
title: Modeling the Wachusett Reservoir, Central Massachusetts, Tributaries for Improved Watershed Management
Creators: name: Fiedler, Erich
Publisher: name: University of Massachusetts Amherst
Year: 2009
Subjects: subject: Environmental Engineering
subject: FOS: Environmental engineering

description: The Wachusett Reservoir watershed is an integral component of the Metropolitan Boston water supply. The Massachusetts Department of Conservation and Recreation (DCR) is responsible for water resource management and water quality protection and has implemented extensive environmental monitoring and modeling programs. These efforts have been used to identify and direct management priorities. Also, a long term collaborative effort with the University of Massachusetts, Amherst has focused on improving data collection and watershed modeling. From the environmental monitoring program, annual nutrient fluxes for total phosphorus (TP), nitrate (NO3-N), and total organic carbon (TOC) have been estimated. These annual nutrient fluxes have assisted DCR to direct water quality management spatially throughout the monitoring period. However, the program has had limited success in identifying the fluxes temporally due to budgetary restrictions on frequent routine sampling. In order to more effectively utilize resources, collaborative research projects with the University of Massachusetts Amherst have been funded to investigate the potential for modeling hydrological variability in the Wachusett Reservoir sub basins to more effectively utilize available data. Several methods to estimate nutrient flux were investigated to evaluate the potential to interpolate a more complete and useful nutrient and hydrologic dataset. These included multiple regression and mechanistic methods. The regression methods utilized a geographical information system (GIS) and generated nutrient loading estimates at annual and monthly timescales. Lumped mechanistic methods were used to generate daily hydrologic and nutrient loading estimates to more accurately capture temporal variability. The methods were compared to evaluate both accuracy and applicability of modeling at the various subbasins. Application of the mechanistic models toward watershed management was another goal of the modeling project. The model dataset generated was applied to optimize the DCR routine monitoring program. Several potential improvements toward watershed monitoring were recommended to more accurately capture hydrologic and nutrient loading variability in the Wachusett Reservoir Watershed.
On the finiteness of the BRS modulo-d cocycles
Creators: name: Piguet, Olivier
name: Sorella, Silvio P.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Ladders of field polynomial differential forms obeying systems of descent equations and corresponding to observables and anomalies of gauge theories are renormalized. They obey renormalized descent equations. Moreover they are shown to have vanishing anomalous dimensions. As an application a simple proof of the nonrenormalization theorem for the nonabelian gauge anomaly is given.
description: 21 p., UGVA-DPT 1992/03-759, Publ. in Nucl Phys. B381 (1992) 373
Exploring the Complex Chemistry of Young Solar Systems
Creators: name: Jørgensen, Jes
Publisher: name: Zenodo
Year: 2019

description: Studies of the complex organic chemistry in regions of star and planet formation have taken a tremendous step forward with data from ALMA. With its unprecedented sensitivity and angular resolution, ALMA has made it possible to zoom in on the gas surrounding deeply embedded protostars on Solar System scales. Such observations reveal the details of the rich complex organic chemistry taking place there - and, in particular, the physical and chemical evolution taking place while the young protoplanetary disks are being assembled. As part of the Protostellar Interferometric Line Survey (PILS), we have performed an unbiased spectral line survey in ALMA's Band 7 of the deeply embedded low-mass protostar IRAS 16293-2422, one of the template sources for star formation and astrochemistry. The survey has yielded a large number of new detections of molecules in the ISM, including key species in the chemical networks of prebiotic molecules. Also, the data show the presence of numerous rare isotopologues of complex organics and other species providing new constraints on their formation paths. The exact measurements of the abundances of the complex organic molecules and their isotopologues are compared to cometary measurements, i.p., from the Rosetta mission, providing the chemical link between the embedded protostellar stages and objects in our own Solar System. Finally, the PILS program outlines some of the paths forward in terms of future systematic ALMA surveys of the organic chemistry in star- and planet-forming regions.
Influencing Health Equity Throughout the Emergency Management Cycle: A Scoping Review
Creators: name: Coderre, Katrina
Publisher: name: Université d'Ottawa / University of Ottawa
Year: 2024
Subjects: Health Equity
Emergency Management
Public Health
Priority Populations
Health Disparity
Disaster
Crisis

description: This thesis sought to gain a better global understanding of how public health can influence health equity throughout the emergency management cycle that includes prevention, mitigation, preparedness, response, and recovery through a scoping review. Seven articles met inclusion criteria, all focused on prevention, which aligns well with public health practices. Interventions such as accommodations for functional needs such as low vision, reduced hearing, limited proficiency in the language which services are provided, or use of assistive devices for mobility and providing training and education to priority populations may influence health equity; however, the evidence is limited, and further research is needed. Due to the intricate challenges that emergencies present and the many factors influencing health equity, there is a need to unravel complexities to guide comprehensive research and intervention design.
title: shayijingbai
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Japhug
subject: jya

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7