cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 790
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
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 790, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 790, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Optimal control of nonlinear elliptic problems with sparsity
Creators: name: Ponce, Augusto C.
name: Wilmet, Nicolas
Publisher: name: arXiv
Year: 2017
Subjects: subject: Analysis of PDEs (math.AP)
subject: Optimization and Control (math.OC)
subject: FOS: Mathematics
subject: 49K20 (Primary) 35J20, 35J91, 49J20, 49J52 (Secondary)

description: We study the minimization of the cost functional \[ F(μ) = \lVert u - u_d \rVert_{L^p(Ω)} + α\lVert μ\rVert_{\mathcal{M}(Ω)}, \] where the controls $μ$ are taken in the space of finite Borel measures and $u \in W_0^{1, 1}(Ω)$ satisfies the equation $- Δu + g(u) = μ$ in the sense of distributions in $Ω$ for a given nondecreasing continuous function $g : \mathbb{R} \to \mathbb{R}$ such that $g(0) = 0$. We prove that $F$ has a minimizer for every desired state $u_d \in L^1(Ω)$ and every control parameter $α> 0$. We then show that when $u_d$ is nonnegative or bounded, every minimizer of $F$ has the same property.
description: 25 pages
Correlated X-ray and Optical Variability in Mkn 509
Creators: name: Marshall, Kevin
name: Ryle, Wesley T.
name: Miller, H. Richard
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results of a 3 year monitoring campaign of the Seyfert 1 galaxy Markarian 509, using X-ray data from the Rossi X-ray Timing Explorer (RXTE) and optical data taken by the SMARTS consortium. Both light curves show significant variations, and are strongly correlated with the optical flux leading the X-ray flux by 15 days. The X-ray power spectrum shows a steep high-frequency slope of -2.0, breaking to a slope of -1.0 at at timescale of 34 days. The lag from optical to X-ray emission is most likely caused by variations in the accretion disk propagating inward.
description: 13 pages, 3 figures. Accepted for publication in the Astrophysical Journal
Using Theorem Provers to Guarantee Closed-Loop System Properties
Creators: name: Arechiga, Nikos
name: Loos, Sarah M.
name: Platzer, Andre
name: Krogh, Bruce H.
Publisher: name: Carnegie Mellon University
Year: 1985
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: This paper presents a new approach for leveraging the power of theorem provers for formal verification to provide sufficient conditions that can be checked on embedded control designs. Theorem provers are often most efficient when using generic models that abstract away many of the controller details, but with these abstract models very general conditions can be verified under which desirable properties such as safety can be guaranteed for the closed-loop system. We propose an approach in which these sufficient conditions are static conditions that can be checked for the specific controller design, without having to include the dynamics of the plant. We demonstrate this approach using the KeYmaera theorem prover for differential dynamic logic for two examples: an intelligent cruise controller and a cooperative intersection collision avoidance system (CICAS) for left-turn assist. In each case, safety of the closed-loop system proved using KeYmaera provides static sufficient conditions that are checked for the controller design.
High Reynolds number magnetohydrodynamic turbulence using a Lagrangian model
Creators: name: Graham, J. Pietarila
name: Mininni, P. D.
name: Pouquet, A.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: With the help of a model of magnetohydrodynamic (MHD) turbulence tested previously, we explore high Reynolds number regimes up to equivalent resolutions of 6000^3 grid points in the absence of forcing and with no imposed uniform magnetic field. For the given initial condition chosen here, with equal kinetic and magnetic energy, the flow ends up being dominated by the magnetic field, and the dynamics leads to an isotropic Iroshnikov-Kraichnan energy spectrum. However, the locally anisotropic magnetic field fluctuations perpendicular to the local mean field follow a Kolmogorov law. We find that the ratio of the eddy turnover time to the Alfven time increases with wavenumber, contrary to the so-called critical balance hypothesis. Residual energy and helicity spectra are also considered; the role played by the conservation of magnetic helicity is studied, and scaling laws are found for the magnetic helicity and residual helicity spectra. We put these results in the context of the dynamics of a globally isotropic MHD flow which is locally anisotropic because of the influence of the strong large-scale magnetic field, leading to a partial equilibration between kinetic and magnetic modes for the energy and the helicity.
description: 11 pages, 7 figures, submitted to Phys. Rev. E
Detecting Low Rapport During Natural Interactions in Small Groups from Non-Verbal Behaviour
Creators: name: Müller, Philipp
name: Huang, Michael Xuelin
name: Bulling, Andreas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences
subject: H.5.m

description: Rapport, the close and harmonious relationship in which interaction partners are "in sync" with each other, was shown to result in smoother social interactions, improved collaboration, and improved interpersonal outcomes. In this work, we are first to investigate automatic prediction of low rapport during natural interactions within small groups. This task is challenging given that rapport only manifests in subtle non-verbal signals that are, in addition, subject to influences of group dynamics as well as inter-personal idiosyncrasies. We record videos of unscripted discussions of three to four people using a multi-view camera system and microphones. We analyse a rich set of non-verbal signals for rapport detection, namely facial expressions, hand motion, gaze, speaker turns, and speech prosody. Using facial features, we can detect low rapport with an average precision of 0.7 (chance level at 0.25), while incorporating prior knowledge of participants' personalities can even achieve early prediction without a drop in performance. We further provide a detailed analysis of different feature sets and the amount of information contained in different temporal segments of the interactions.
description: 12 pages, 6 figures
Spectroscopic vetting of TESS planet candidates
Creators: name: Nielsen, Louise Dyregaard
Publisher: name: Zenodo
Year: 2021
Subjects: Exoplanets

description: Since the release of the first TESS sectors, the high resolution spectrograph CORALIE on the Swiss 1.2 m Euler telescope has observed more than 300 TESS Objects of Interest (TOIs). This work has been conducted in collaboration with the TESS Follow-up Programme to best support exoplanet-observations with larger telescopes, such as HARPS and Espresso. Within a wide range of science cases, we have covered a diverse set of TOIs spanning stellar types, orbital periods and transit depths. Amongst our sample of TOIs, we find that 43% are still unresolved planet candidates, 26% have been confirmed as planets, 2.5% are brown dwarfs and 20% have been identified as eclipsing stellar binaries.
 We wish to present an overview of the first three years of spectroscopic vetting and follow-up observations. We will also demonstrate our latest data release of spectra, cross-correlation functions and radial velocities, which are publicly available through the DACE platform (dace.unige.ch).
Additional file 2 of The metagenomic next-generation sequencing in diagnosing central nervous system angiostrongyliasis: a case report
Creators: name: Feng, Li
name: Zhang, Aiwu
name: Que, Jiali
name: Zhou, Hongyan
name: Wang, Haiyan
name: Guan, Yuanlin
name: Shen, Cunzhou
name: Sun, Xunsha
name: Lai, Rong
name: Peng, Fuhua
name: Feng, Huiyu
name: Chen, Ling
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Mental Health
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 2. Procedure of mNGS and PCR. Additional file 2 provided detailed procedure of mNGS and PCR.
Sojourn times of the Hadamard walk in one dimension
Creators: name: Konno, Norio
Publisher: name: arXiv
Year: 2011
Subjects: subject: Quantum Physics (quant-ph)
subject: Combinatorics (math.CO)
subject: Probability (math.PR)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: The Hadamard walk is a typical model of the discrete-time quantum walk. We investigate sojourn times of the Hadamard walk on a line by a path counting method.
description: 14 pages, title changed, minor corrections, Quantum Information Processing (in press)
Using the Amazon Mechanical Turk for Transcription of Spoken Language
Creators: name: Marge, Matthew R
name: Satanjeev  Banerjee
name: Rudnicky, Alexander
Publisher: name: Carnegie Mellon University
Year: 2008
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: We investigate whether Amazon's Mechanical Turk (MTurk) service can be used as a reliable method for transcription of spoken language data. Utterances with varying speaker demographics (native and non-native English, male and female) were posted on the MTurk marketplace together with standard transcription guidelines. Transcriptions were compared against transcriptions carefully prepared in-house through conventional (manual) means. We found that transcriptions from MTurk workers were generally quite accurate. Further, when transcripts for the same utterance produced by multiple workers were combined using the ROVER voting scheme, the accuracy of the combined transcript rivaled that observed for conventional transcription methods. We also found that accuracy is not particularly sensitive to payment amount, implying that high quality results can be obtained at a fraction of the cost and turnaround time of conventional methods.
title: 02_0442
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/
Using Tensor Analysis to characterize Contact-map Dynamics of Proteins
Creators: name: Ramanathan, Arvind
name: Pratul K. Agarwal
name: Langmead, Christopher J.
Publisher: name: Carnegie Mellon University
Year: 2004
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Molecular dynamics simulations provide vast amount of information about a protein’s dynamics. To interpret a protein’s dynamics and how it may relate to its function, traditionally, two-way analysis techniques such as principal component analysis have been used. However, two-way analysis techniques are usually limited by the fact that they have to be done post-process, i.e., after the simulations have been run and also cannot provide insights into temporal behavior of a protein. To overcome these limitations, we are proposing to use multi-way analysis techniques to understand and interpret protein dynamics as and when the simulations are progressing i.e., online. We model MD simulations in terms of a collection of contact maps and then modeling them as tensors to capture multiple dependencies. Using two recently developed techniques to perform online analysis of streaming data, we illustrate the use of this technique to describe and interpret the behavior of a protein complex in real time. We provide both experimental evidence to support our claims and also discuss the potential advantages and disadvantages of using tensor analysis techniques.
A warm Neptune around the G5V dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
Creators: name: König, Pierre-Cécil
name: Damasso, Mario
name: Hébrard, Guillaume
name: Naponiello, Luca
name: Et Al., Including SOPHIE
Publisher: name: Zenodo
Year: 2021
Subjects: Exoplanets
Stellar Astrophysics
Planetary Systems
Techniques: Photometric
Techniques: Spectroscopic
Techniques: Radial Velocities

description: We report the detection and characterization of the new transiting extrasolar planet TOI-1710 b. It was first identified as a promising candidate by the Transiting Exoplanet Survey Satellite (TESS). Its planetary nature has been established from HARPS-N and SOPHIE spectroscopic observations via the radial velocity method. The stellar parameters for the host star are derived from the spectra and a joint Markov chain Monte-Carlo (MCMC) adjustment of the spectral energy distribution and evolutionary tracks of TOI-1710. Performed in a combined MCMC and quasi-periodic Gaussian process method, a simultaneous analysis of the TESS light curve and the radial velocity evolution concomitantly allows us to determine the planetary properties and inspect the stellar magnetic activity jitter. TOI-1710 b is a massive warm Neptune (30.0 ± 5.7 M_Earth and 5.84 ± 0.30 R_Earth) orbiting a G5V dwarf star on a 24.3 days circular compatible orbit (e = 0.13 ± 0.09).
description: König, Pierre-Cécil, et al., A&A, in prep.
description: {"references": ["Foreman-Mackey, Daniel, et al. (2017). Exoplanet Python Package associated to DOI:10.3847/1538-3881/aa9332"]}
The user's guide project: giving experiential context to research papers
Creators: name: Malkiewich, Cary
name: Merling, Mona
name: White, David
name: Wolcott, Luke
name: Yarnall, Carolyn
Publisher: name: arXiv
Year: 2018
Subjects: subject: History and Overview (math.HO)
subject: FOS: Mathematics

description: This paper was written in 2015, and published in the Journal of Humanistic Mathematics. This paper announces the first issue (2015) of Enchiridion: Mathematics User's Guides, a project to produce peer-reviewed User's Guides as companions to published papers. These User's Guides are meant to explain the key insights and organizing principles in their companion papers, the metaphors and imagery used by the authors, the story of the development of the companion papers, and a colloquial summary appropriate for a non-mathematical audience. Examples of User's Guides can be found at https://mathusersguides.com/
Using Style to Understand Descriptions of Software Architecture
Creators: name: Abowd, Gregory
name: Allen, Robert
name: Garlan, David
Publisher: name: Carnegie Mellon University
Year: 1965
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: The software architecture of most systems is described informally and diagrammatically. In order for these descriptions to be meaningful at all, figures are understood by interpreting the boxes and lines in specific, conventionalized ways[5]. The imprecision of these interpretations has a number of limitations. In this paper we consider these conventionalized interpretations as architectural styles and provide a formal framework for their uniform definition. In addition to providing a template for precisely defining new architectural styles, this framework allows for the proof that the notational constraints on a style are sufficient to guarantee the meanings of all described systems and provides a unified semantic base through which different stylistic interpretations can be compared.
Near-infrared cross-dispersed spectroscopy of brown dwarf candidates in the Upper Sco association
Creators: name: Lodieu, N.
name: Hambly, N. C.
name: Jameson, R. F.
name: Hodgkin, S. T.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present near-infrared (1.15-2.50 microns) medium-resolution (R = 1700) spectroscopy of a sample of 23 brown dwarf candidates in the young Upper Sco association. We confirm membership of 21 brown dwarfs based on their spectral shape, comparison with field dwarfs, and presence of weak gravity-sensitive features. Their spectral types range from M8 to L2 with an uncertainty of a subclass, suggesting effective temperatures between 2700 and 1800 K with an uncertainty up to 300 K and masses in the 30-8 Mjup range. Among the non-members, we have uncovered a field L2 dwarf at a distance of 120-140 pc, assuming that it is single. The success rate of our photometric selection based on five photometric passbands and complemented partly by proper motion is over 90%, a very promising result for future studies of the low-mass star and brown dwarf populations in young open clusters by the UKIDSS Galactic Cluster Survey. We observe a large dispersion in the magnitude versus spectral-type relation which is likely the result of the combination of several effects including age dispersion, extent and depth of the association, a high degree of multiplicity and the occurrence of disks.
description: 13 pages, 7 figures, 3 tables, accepted to MNRAS
Linked stage graph
Creators: name: Tietz, Tabea
name: Waitelonis, J.
name: Zhou, Kanran
name: Felgentreff, P.
name: Meyer, N.
name: Weber, A.
name: Sack, Harald
Publisher: name: Karlsruhe
Year: 2019
Subjects: cultural heritage
linked data
knowledge graph
UL

description: Archives today are publishing their cultural heritage data on the Web for exploration. However, for archive novices the traditional archival structures often are not intuitive and difficult to understand, and thus challenges data access and consumption. To tackle this problem, Linked Stage Graph was developed, a knowledge graph (KG) on the foundation of historical data about the Stuttgart State Theater. The data was made available by the Baden-Wuerttemberg State Archives for the Coding da Vinci hackathon. This demo paper contributes the KG,a SPARQL endpoint, named entity extraction and linking to existing authoritative KGs as well as a dedicated user interface for exploration.
Self Assembly of Soft Matter Quasicrystals and Their Approximants
Creators: name: Iacovella, Christopher R.
name: Keys, Aaron S.
name: Glotzer, Sharon C.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The surprising recent discoveries of quasicrystals and their approximants in soft matter systems poses the intriguing possibility that these structures can be realized in a broad range of nano- and micro-scale assemblies. It has been theorized that soft matter quasicrystals and approximants are largely entropically stabilized, but the thermodynamic mechanism underlying their formation remains elusive. Here, we use computer simulation and free energy calculations to demonstrate a simple design heuristic for assembling quasicrystals and approximants in soft matter systems. Our study builds on previous simulation studies of the self-assembly of dodecagonal quasicrystals and approximants in minimal systems of spherical particles with complex, highly-specific interaction potentials. We demonstrate an alternative entropy-based approach for assembling dodecagonal quasicrystals and approximants based solely on particle functionalization and shape, thereby recasting the interaction-potential-based assembly strategy in terms of simpler-to-achieve bonded and excluded-volume interactions. Here, spherical building blocks are functionalized with mobile surface entities to encourage the formation of structures with low surface contact area, including non-close-packed and polytetrahedral structures. The building blocks also possess shape polydispersity, where a subset of the building blocks deviate from the ideal spherical shape, discouraging the formation of close-packed crystals. We show that three different model systems with both of these features -- mobile surface entities and shape polydispersity -- consistently assemble quasicrystals and/or approximants. We argue that this design strategy can be widely exploited to assemble quasicrystals and approximants on the nano- and micro- scales. In addition, our results further elucidate the formation of soft matter quasicrystals in experiment.
description: 12 pages 6 figures
Additional file 1 of Assessing healthcare access using the Levesque’s conceptual framework– a scoping review
Creators: name: Cu, Anthony
name: Meister, Sofia
name: Lefebvre, Bertrand
name: Ridde, Valéry
Publisher: name: figshare
Year: 2021
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences

description: Additional file 1.
Barrier to recombination of oppositely charged large polarons
Creators: name: Emin, David
Publisher: name: arXiv
Year: 2017
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: Electronic charge carriers in ionic materials can self-trap to form large polarons. Interference between the ionic displacements associated with oppositely charged large polarons increases as they approach one another. Initially this interference produces an attractive potential that fosters their merger. However, for small enough separations this interference generates a repulsive interaction between oppositely charged large polarons. In suitable circumstances this repulsion can overwhelm their direct Coulomb attraction. Then the resulting net repulsion between oppositely charged large polarons constitutes a potential barrier which impedes their recombination.
description: 10 pages, 2 figures
Bright OB stars in the Galaxy IV. Stellar and wind parameters of early to late B supergiants
Creators: name: Markova, N.
name: Puls, J.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We apply the NLTE atmosphere code FASTWIND to perform a spectroscopic study of a small sample of Galactic B-supergiants from B0 to B9. By means of the resulting data and incorporating additional datasets from alternative studies, we investigate the properties of OB-supergiants and compare our findings with theoretical predictions. As a result we find that due to the combined effects of line- and wind-blanketing, the temperature scale of Galactic B-supergiants needs to be revised downwards, by 10 to 20 percent, the latter value being appropriate for stronger winds. In fair accordance with recent results, our sample furthermore indicates a gradual decrease in wind terminal velocities over the bi-stability region, where the limits of this region are located at lower temperatures than the predicted ones. Introducing a distance-independent quantity Q' related to wind-strength, we also show that this quantity is a well defined, monotonically increasing function of Teff outside this region. Inside and from hot to cool, the mass loss rate changes by a factor (in between 0.4 and 2.5) which is (much) smaller than the predicted factor of 5. All this indicates that the decrease in wind terminal velocity over the bi-stability region is not over-compensated by an increase of mass loss rate, as frequently argued (provided the wind-clumping properties on both sides of this region do not differ substantially).
description: 23 pages and 14 figures accepted for publication in A & A; the Fig. 1 title and the last para of Sec. 4.1 modified; a new reference added
Automated stellar variability classification using TESS light curves
Creators: name: Chickles, Emma
name: Daylan, Tansu
name: Gordon, Lindsey
Publisher: name: Zenodo
Year: 2021
Subjects: Stellar Astrophysics

description: Stellar variability is driven by various processes occurring at the stellar surface and in the stellar interior, such as due to stellar eclipses, flares, tidal interactions, pulsations, spots, and rotation. We use unsupervised machine learning on photometric light curves observed by the Transiting Exoplanet Survey Satellite (TESS) to conduct a census of different types of stellar variability. Towards this purpose, we use a one-dimensional convolutional autoencoder and feature engineering, which yields compressed, low-dimensional representations of the data. We use the learned representations to perform large-scale classification and novelty detection using TESS light curves. We validate our pipeline using cataloged eclipsing binaries in ASAS-SN, the General Catalogue of Variable Stars, and SIMBAD. The indiscriminate survey produced by TESS offers a unique opportunity to investigate the relationships between light curve features and underlying stellar characteristics such as type, age, metallicity, and mass. Our homogeneous census of stellar variability will lead to a better understanding of the underlying demographics.
Low Complexity Kolmogorov-Smirnov Modulation Classification
Creators: name: Wang, Fanggang
name: Xu, Rongtao
name: Zhong, Zhangdui
Publisher: name: arXiv
Year: 2011
Subjects: subject: Information Theory (cs.IT)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Kolmogorov-Smirnov (K-S) test-a non-parametric method to measure the goodness of fit, is applied for automatic modulation classification (AMC) in this paper. The basic procedure involves computing the empirical cumulative distribution function (ECDF) of some decision statistic derived from the received signal, and comparing it with the CDFs of the signal under each candidate modulation format. The K-S-based modulation classifier is first developed for AWGN channel, then it is applied to OFDM-SDMA systems to cancel multiuser interference. Regarding the complexity issue of K-S modulation classification, we propose a low-complexity method based on the robustness of the K-S classifier. Extensive simulation results demonstrate that compared with the traditional cumulant-based classifiers, the proposed K-S classifier offers superior classification performance and requires less number of signal samples (thus is fast).
description: This paper is accepted by IEEE WCNC 2011
Bolsonaro’s Congressional Cheerleaders in the Post-Truth Era: Demagoguery as communication, and YouTube as the Tool.pdf
Creators: name: Kissock, Tom
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 470102
subject: Communication technology and digital media studies
classificationCode: 441099
subject: Sociology not elsewhere classified
classificationCode: 440899
subject: Political science not elsewhere classified
classificationCode: 400699
subject: Communications engineering not elsewhere classified
classificationCode: 430204
subject: Digital heritage

description:   
This paper examines a Press Conference (PC) which took place on the 29th of April 2020 at the Palacio Do Alvorado in Brazil. President Jair Bolsonaro and his congressional deputies (his Congressional Cheerleaders) spoke to their civilian fans and took turns berating Journalists who were at the same location. Videos of the episode were posed to YouTube from numerous smartphones and television cameras and thus was subsequently covered by traditional media. What this paper explores is how Bolsonaro and his Congressional Cheerleaders, bypassed legacy media as an accountability mechanism, to post videos of their own version of the events straight to their echo chambers on YouTube. By conducting thematic content and affordance analysis of the event across YouTube videos, this paper finds that these Congressional Cheerleaders purposely used violent rhetoric to circumvent traditional media, and subsequently argues that Brazil’s traditional media outlets then failed to hold each actor accountable. This paper adds to the scholarship on demagoguery and how agents of populism like Bolsonaro’s and his Congressional Cheerleaders in Brazil interact with traditional and social media. Thus, this paper sets out a conceptual framework for understanding how modern populism shouldn’t empathise a cult of personality. In fact, it is extremely nuanced, driven by a network of political agents who are able leverage the power of video to disseminate violent political messaging. Furthermore, with the growing trend of video used by politicians across social media this research can also be translated to other regions experiencing demagoguery and populism outside of Brazil.
title: ADCO, Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Cart. 180 (11 H 755), 83 folios, f. 0147
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/2017
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 pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 180 (11 H 755), 83 folios, f. 0147, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 180 (11 H 755), 83 folios, f. 0147, 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
Using Story Topics For Language Model Adaptation
Creators: name: Seymore, Kristie
name: Rosenfeld, Roni
Publisher: name: Carnegie Mellon University
Year: 2008
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: The subject matter of any conversation or document can typically be described as some combination of elemental topics. We have developed a language model adaptation scheme that takes a piece of text, chooses the most similar topic clusters from a set of over 5000 elemental topics, and uses topic specific language models built from the topic clusters to rescore N-best lists. We are able to achieve a 15% reduction in perplexity and a small improvement in WER by using this adaptation. We also investigate the use of a topic tree, where the amount of training data for a specific topic can be judiciously increased in cases where the elemental topic cluster has too few word tokens to build a reliably smoothed and representative language model. Our system is able to fine-tune topic adaptation by interpolating models chosen from thousands of topics, allowing for adaptation to unique, previously unseen combinations of subjects.
Using State Space Exploration and a Natural Deduction Style Message Derivation Engine to Verify Security Protocols
Creators: name: Clarke, Edmund M
name: Somesh  Jha
name: Marrero, Will
Publisher: name: Carnegie Mellon University
Year: 2002
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: As more resources are added to computer networks, and as more vendors look to the World Wide Web as a viable marketplace, the importance of being able to restrict access and to ensure some kind of acceptable behavior even in the presence of malicious adversaries becomes paramount.
The Spin-Statistics Theorem in Arbitrary Dimensions
Creators: name: Boya, Luis J.
name: Sudarshan, E. C. G.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate the spin-statistics connection in arbitrary dimensions for hermitian spinor or tensor quantum fields with a rotationally invariant bilinear Lagrangian density. We use essentially the same simple method as for space dimension D = 3. We find the usual connection (tensors as bosons and spinors as fermions) for D = 8n + 3; 8n + 4; 8n + 5, but only bosons for spinors and tensors in dimensions 8n +/- 1 and 8n. In dimensions 4n + 2 the spinors may be chosen as bosons or fermions. The argument hinges on finding the identity representation of the rotation group either on the symmetric or the antisymmetric part of the square of the field representation.
description: 14 pages. To be published in International Journal of Theoretical Physics
Direct observation of surface state thermal oscillation in SmB6 oscillators
Creators: name: Casas, Brian
name: Stern, Alex
name: Efimkin, Dmitry K.
name: Fisk, Zachary
name: Xia, Jing
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: SmB6 is a mixed valence Kondo insulator that exhibits a sharp increase in resistance following an activated behavior that levels off and saturates below 4K. This behavior can be explained by the proposal of SmB6 representing a new state of matter, a Topological Kondo insulator, in which a Kondo gap is developed and topologically protected surface conduction dominates low-temperature transport. Exploiting its non-linear dynamics, a tunable SmB6 oscillator device was recently demonstrated, where a small DC current generates large oscillating voltages at frequencies from a few Hz to hundreds of MHz. This behavior was explained by a theoretical model describing the thermal and electronic dynamics of coupled surface and bulk states. However, a crucial aspect of this model, the predicted temperature oscillation in the surface state, hasn't been experimentally observed to date. This is largely due to the technical difficulty of detecting an oscillating temperature of the very thin surface state. Here we report direct measurements of the time-dependent surface state temperature in SmB6 with a RuO micro-thermometer. Our results agree quantitatively with the theoretically simulated temperature waveform, and hence support the validity of the oscillator model, which will provide accurate theoretical guidance for developing future SmB6oscillators at higher frequencies.
description: 6 pages, 6 figures
Using Simple Speech–Based Features to Detect the State of a Meeting and the Roles of the Meeting Participants
Creators: name: Satanjeev  Banerjee
name: Rudnicky, Alexander
Publisher: name: Carnegie Mellon University
Year: 2006
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: We introduce a simple taxonomy of meeting states and participant roles. Our goal is to automatically detect the state of a meeting and the role of each meeting participant and to do so concurrent with a meeting. We trained a decision tree classiﬁer that learns to detect these states and roles from simple speech–based features that are easy to compute automatically. This classiﬁer detects meeting states 18% absolute more accurately than a random classiﬁer, and detects participant roles 10% absolute more accurately than a majority classiﬁer. The results imply that simple, easy to compute features can be used for this purpose.
Asymmetric access to information impacts the power-law exponent in networks
Creators: name: Cao, Zhenfeng
name: He, Zhou
name: Johnson, Neil F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: FOS: Physical sciences

description: The preferential attachment (PA) process is a popular theory for explaining network power-law degree distributions. In PA, the probability that a new vertex adds an edge to an existing vertex depends on the connectivity of the target vertex. In real-world networks, however, each vertex may have asymmetric accessibility to information. Here we address this issue using a new network-generation mechanism that incorporates asymmetric accessibility to upstream and downstream information. We show that this asymmetric information accessibility directly affects the power-law exponent, producing a broad range of values that are consistent with observations. Our findings shed new light on the possible mechanisms in three important real-world networks: a citation network, a hyperlink network, and an online social network.
description: 4 pages, 3 figures
Identify Transit Signals with Object Detection Algorithm
Creators: name: Cui, Kaiming
name: Liu, Junjie
name: Feng, Faobo
name: Liu, Jifeng
Publisher: name: Zenodo
Year: 2021
Subjects: Exoplanets
Data Analysis Techniques

description: Deep learning algorithms are widely used in many fields of astronomy, and have a wide range of applications in transiting exoplanet detection and classification. We have trained an neural network using two-dimensional object detection algorithm with Kepler and TESS light curves. Our network outputs excellent performance on Kepler and TESS data. The detected transits can amplify their periodicity and our network can be easily used to find single transiting events and cluster multiple transits.
description: {"references": ["Pearson, K. A., Palafox, L., & Griffith, C. A. 2018, MNRAS, 474, 478, doi: 10.1093/mnras/stx2761", "Zucker, S., & Giryes, R. 2018, AJ, 155, 147, doi: 10.3847/1538-3881/aaae05", "Shallue, C. J., & Vanderburg, A. 2018, AJ, 155, 94, doi: 10.3847/1538-3881/aa9e09", "Ansdell, M., Ioannou, Y., Osborn, H. P., et al. 2018, ApJL, 869, L7, doi: 10.3847/2041-8213/aaf23b", "Dattilo, A., Vanderburg, A., Shallue, C. J., et al. 2019, AJ, 157, 169, doi: 10.3847/1538-3881/ab0e12", "Yu, L., Vanderburg, A., Huang, C., et al. 2019, AJ, 158, 25, doi: 10.3847/1538-3881/ab21d6", "Osborn, H. P., Ansdell, M., Ioannou, Y., et al. 2020, A&A, 633, A53, doi: 10.1051/0004-6361/201935345", "Schanche, N., Collier Cameron, A., H\u00e9brard, G., et al. 2019, MNRAS, 483, 5534, doi: 10.1093/mnras/sty3146", "Chaushev, A., Raynard, L., Goad, M. R., et al. 2019, MNRAS, 488, 5232, doi: 10.1093/mnras/stz2058", "Olmschenk, G., Ishitani Silva, S., Rau, G., et al. 2021, AJ, 161, 273, doi: 10.3847/1538-3881/abf4c6"]}
A Hydrodynamic Model of Alfvénic Wave Heating in a Coronal Loop and its Chromospheric Footpoints
Creators: name: Reep, Jeffrey W.
name: Russell, Alexander J. B.
name: Tarr, Lucas A.
name: Leake, James E.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Alfvénic waves have been proposed as an important energy transport mechanism in coronal loops, capable of delivering energy to both the corona and chromosphere and giving rise to many observed features, of flaring and quiescent regions. In previous work, we established that resistive dissipation of waves (ambipolar diffusion) can drive strong chromospheric heating and evaporation, capable of producing flaring signatures. However, that model was based on a simplified assumption that the waves propagate instantly to the chromosphere, an assumption which the current work removes. Via a ray tracing method, we have implemented traveling waves in a field-aligned hydrodynamic simulation that dissipate locally as they propagate along the field line. We compare this method to and validate against the magnetohydrodynamics code Lare3D. We then examine the importance of travel times to the dynamics of the loop evolution, finding that (1) the ionization level of the plasma plays a critical role in determining the location and rate at which waves dissipate; (2) long duration waves effectively bore a hole into the chromosphere, allowing subsequent waves to penetrate deeper than previously expected, unlike an electron beam whose energy deposition rises in height as evaporation reduces the mean-free paths of the electrons; (3) the dissipation of these waves drives a pressure front that propagates to deeper depths, unlike energy deposition by an electron beam.
description: Accepted to ApJ
Double Stage Delay Multiply and Sum Beamforming Algorithm Applied to Ultrasound Medical Imaging
Creators: name: Mozaffarzadeh, Moein
name: Sadeghi, Masume
name: Mahloojifar, Ali
name: Orooji, Mahdi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: In Ultrasound (US) imaging, Delay and Sum (DAS) is the most common beamformer, but it leads to low quality images. Delay Multiply and Sum (DMAS) was introduced to address this problem. However, the reconstructed images using DMAS still suffer from level of sidelobes and low noise suppression. In this paper, a novel beamforming algorithm is introduced based on the expansion of DMAS formula. It is shown that there is a DAS algebra inside the expansion, and it is proposed to use DMAS instead of the DAS algebra. The introduced method, namely Double Stage DMAS (DS-DMAS), is evaluated numerically and experimentally. The quantitative results indicate that DS-DMAS results in about 25% lower level of sidelobes compared to DMAS. Moreover, the introduced method leads to 23%, 22% and 43% improvement in Signal-to-Noise Ratio, Full-Width-Half-Maximum and Contrast Ratio, respectively, in comparison with DMAS beamformer.
description: This paper is accepted in "Ultrasound in Medicine and Biology" journal
Study of vector meson fragmentation using a broken SU(3) model
Creators: name: Indumathi, D.
name: Saveetha, H.
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Inclusive hadro production in e^+ e^- annihilation processes is examined to study the fragmentation process. A broken SU(3) model is used to determine the quark and gluon fragmentation functions of octet vector mesons, ρand K^*, in a simple way with an SU(3) breaking parameter λ. These are expressed in terms of just two light quark fragmentation functions, V(x, Q2) and γ(x, Q2) and the gluon fragmentation function Dg(x, Q2). These functions are parameterized at the low input scale of Q0^2 = 1.5 GeV2, evolved through LO DGLAP evolution including charm and bottom flavour at appropriate thresholds, and fitted by comparison with data at the Z-pole. The model is extended with the introduction of a few additional parameters to include a study of singlet--octet mixing and hence ωand ϕfragmentation. The model gives good fits to the available data for x >~ 0.01, where x is the scaled energy of the hadron. The model is then applied successfully to ω, ϕproduction in pp collisions at the Relativistic Heavy Ion Collider, RHIC; these data form an important base-line for the study of Quark Gluon Plasma in heavy nucleus collisions at RHIC, and also in future at the LHC.
description: 27 pages PRD-latex with 10 eps figure files; modified to include an analysis of RHIC pp data
Multicolor Variability of Young Stars with Disks: Insights from Coordinated Space and Ground Observations
Creators: name: Venuti, Laura
name: Cody, Ann Marie
name: Rebull, Luisa M.
name: Beccari, Giacomo
name: Irwin, Mike J.
name: Thanvantri, Sowmya
name: Howell, Steve B.
name: Barentsen, Geert
Publisher: name: Zenodo
Year: 2021
Subjects: Stellar Astrophysics
YSOs
Observations

description: Space telescopes have provided unprecedented depictions of the manifold variability behaviors typical of young stellar objects (YSOs). However, the lack of coordinated, multiband data often limited our understanding of the observed flux patterns. We conducted a comprehensive variability survey of 278 B-to-K YSOs in the 1-2 Myr-old cluster NGC 6530. Our sample was monitored with Kepler/K2, and simultaneous u,g,r,i,Halpha time series were acquired with VST/OmegaCAM. We detected substantially lower variability on B/A stars than on G/K stars for any light curve morphology, and a dearth of some distinctive disk-driven behaviors among stars earlier than G. We could also pinpoint distinct contributions to the leading day-to-week variability timescales, from intense accretion triggered by inner disk instabilities, to variable accretion efficiency in the outer magnetosphere. On the heels of that project, we are undertaking a new survey of the Taurus star forming region, coupling high-precision photometry from TESS with simultaneous u,g,r,i data from the Las Cumbres Observatory. This program will provide unique constraints on the physical drivers of YSO variability, and on the mid- to long-term stability of inner disks around young stars.
description: {"references": ["Allen et al. (2004), ApJS, 154, 363", "Cody et al. (2014), AJ, 147, 82", "Cody et al. (2018), AJ, 156, 71", "Damiani et al. (2019), A&A, 623, A25", "Sergison et al. (2020), MNRAS, 491"]}