cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Topic Detection and Tracking Pilot Study Final Report
Creators: name: Allan, James
name: Carbonell, Jaime G.
name: Doddington, George
name: Yamron, Jonathan
name: Yiming  Yang
Publisher: name: Carnegie Mellon University
Year: 2003
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Topic Detection and Tracking (TDT) is a DARPA-sponsored initiative to investigate the state of the art in finding and following new events in a stream of broadcast news stories. The TDT problem consists of three major tasks: (1) segmenting a stream of data, especially recognized speech, into distinct stories; (2) identifying those news stories that are the first to discuss a new event occurring in the news; and (3) given a small number of sample news stories about an event, finding all following stories in the stream. The TDT Pilot Study ran from September 1996 through October 1997. The primary participants were DARPA, Carnegie Mellon University, Dragon Systems, and the University of Massachusetts at Amherst. This report summarizes the findings of the pilot study.
Meyer, B., de R
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Luzern
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Fractional Non-Linear, Linear and Sublinear Death Processes
Creators: name: Orsingher, Enzo
name: Polito, Federico
name: Sakhno, Ludmila
Publisher: name: arXiv
Year: 2013
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics

description: This paper is devoted to the study of a fractional version of non-linear $\mathpzc{M}^ν(t)$, $t>0$, linear $M^ν(t)$, $t>0$ and sublinear $\mathfrak{M}^ν(t)$, $t>0$ death processes. Fractionality is introduced by replacing the usual integer-order derivative in the difference-differential equations governing the state probabilities, with the fractional derivative understood in the sense of Dzhrbashyan--Caputo. We derive explicitly the state probabilities of the three death processes and examine the related probability generating functions and mean values. A useful subordination relation is also proved, allowing us to express the death processes as compositions of their classical counterparts with the random time process $T_{2 ν} (t)$, $t>0$. This random time has one-dimensional distribution which is the folded solution to a Cauchy problem of the fractional diffusion equation.
Relativistic Radiation Hydrodynamical Accretion Disk Winds
Creators: name: Fukue, Jun
name: Akizuki, Chizuru
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Accretion disk winds browing off perpendicular to a luminous disk are examined in the framework of fully special relativistic radiation hydrodynamics. The wind is assumed to be steady, vertical, and isothermal. %and the gravitational fields is approximated by a pseudo-Newtonian potential. Using a velocity-dependent variable Eddington factor, we can solve the rigorous equations of relativistic radiative hydrodynamics, and can obtain radiatively driven winds accelerated up to the {\it relativistic} speed. For less luminous cases, disk winds are transonic types passing through saddle type critical points, and the final speed of winds increases as the disk flux and/or the isothermal sound speed increase. For luminous cases, on the other hand, disk winds are always supersonic, since critical points disappear due to the characteristic nature of the disk gravitational fields. The boundary between the transonic and supersonic types is located at around $\hat{F}_{\rm c} \sim 0.1 (ε+p)/(ρc^2)/γ_{\rm c}$, where $\hat{F}_{\rm c}$ is the radiative flux at the critical point normalized by the local Eddington luminosity, $(ε+p)/(ρc^2)$ is the enthalpy of the gas divided by the rest mass energy, and $γ_{\rm c}$ is the Lorentz factor of the wind velocity at the critical point. In the transonic winds, the final speed becomes 0.4--0.8$c$ for typical parameters, while it can reach $\sim c$ in the supersonic winds.
description: 6 pages, 5 figures; PASJ 59 (2007) in press
The massless Dirac-Weyl equation with deformed extended complex potentials
Creators: name: Yesiltas, O.
name: Cagatay, B.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mathematical Physics (math-ph)
subject: Quantum Algebra (math.QA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Basically (2 + 1) dimensional Dirac equation with real deformed Lorentz scalar potential is investi gated in this study. The position dependent Fermi velocity function transforms Dirac Hamiltonian into a Klein-Gordon-like effective Hamiltonian system. The complex Hamiltonian and its real energy spectrum and eigenvectors are obtained analytically. Moreover, the Lie algebraic analysis is performed.
description: 7pages, to be published in Canadian Journal of Physics in the special issue: Turkish Physical Society 32nd International Physics Congress (TPS32) : 6-9 September 2016, Bodrum, Turkey
Meyer, Franz Jakob, Erben
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Luzern
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
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The Effect of Composite Resonances on Higgs decay into two photons
Creators: name: Hernández, A. E. Cárcamo
name: Dib, Claudio O.
name: Zerwekh, Alfonso R.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In scenarios of strongly coupled electroweak symmetry breaking, heavy composite particles of different spin and parity may arise and cause observable effects on signals that appear at loop levels. The recently observed process of Higgs to $γγ$ at the LHC is one of such signals. We study the new constraints that are imposed on composite models from $H\to γγ$, together with the existing constraints from the high precision electroweak tests. We use an effective chiral Lagrangian to describe the effective theory that contains the Standard Model spectrum and the extra composites below the electroweak scale. Considering the effective theory cutoff at $Λ= 4πv \sim 3 $ TeV, consistency with the $T$ and $S$ parameters and the newly observed $H\to γγ$ can be found for a rather restricted range of masses of vector and axial-vector composites from $1.5$ TeV to $1.7$ TeV and $1.8$ TeV to $1.9$ TeV, respectively, and only provided a non-standard kinetic mixing between the $W^{3}$ and $B^{0}$ fields is included.
description: 30 pages, 10 figures. Version for publication in European Physical Journal C
Michelletti, P. G
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Lugano
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
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Top-down influence in early visual processing: a Bayesian perspective
Creators: name: Lee, Tai Sing
Publisher: name: Carnegie Mellon University
Year: 1965
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Traditional views of visual processing suggest that early visual neurons are static spatiotemporal filters that extract local features by feedforward computation. The extracted information is then fed forward through a chain of modules to successively higher visual areas for further analysis. Recording from early visual neurons in awake behaving monkeys, we revealed there are many levels of complexity in the information processing of the early visual cortex. We found that the early visual neurons not only are sensitive to features within their receptive fields (RFs) but also to the global context of a visual scene, the behavioral relevance of the stimuli and the experience of the animals. These findings suggest that the early visual cortex (V1 and V2) is tightly coupled to and highly interactive with the rest of the visual system. The top-down interaction, mediated by recurrent feedback connections, introduces contextual information to influence the perceptual inference in the early visual cortex.
Radiative Transfer in Relativistic Accretion-Disk Winds
Creators: name: Fukue, Jun
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Radiative transfer in a relativistic accretion disk wind is examined under the plane-parallel approximation in the fully special relativistic treatment. For an equilibrium flow, where the flow speed and the source function are constant, the emergent intensity is analytically obtained. In such an equilibrium flow the usual limb-darkening effect does not appear, since the source function is constant. Due to the Doppler and aberration effects associated with the relativistic motion of winds, however, the emergent intensity is strongly enhanced toward the flow direction. This is the {\it relativistic peaking effect}. We thus carefully treat and estimate the appearance of relativistic winds and jets, when we observe them in an arbitrary direction.
description: 8 pages, 4 figures; PASJ 60 (2008) in press
LabVIEW and HIL for Power Electronics and Drives Applications
Creators: Alessandro Lidozzi
Marco di Benedetto
Publisher: name: IEEE
Year: 2024

The course will cover the methodologies to switch to new graphical programming development environments, starting with a review and going into the most promising solutions.
Nowadays, even a typical power converter can exhibit more active devices and higher switching frequency than ever to satisfy a higher control performance demand. This increases complexity related to the control board, where usually a combined μC (or μP, DSP) and FPGA are installed. Those two ‘actors’ require a completely different programming approach and development tools from traditional boards.

Accordingly, control algorithm development is considered a ‘time consuming’ task within a research or industrial project. The Integrated Development Environments provided by the control platforms manufacturers, or third parties constantly move from the classical, old, text-based approach to a new, fast, and simple-to-learn graphical programming method. Moreover, a high level of abstraction is usually demanded to accelerate the learning time, even for non-specialist workers. However, full control of the hardware is still mandatory.

The course will cover the methodologies to switch to new graphical programming development environments, starting with a review and going into the most promising solutions.
Code splitting between targets, best practices, and code efficiency will be part of the course.

Alessandro Lidozzi received the Electronic Engineering degree and the Ph.D. degree from the Roma Tre University, Rome, Italy, in 2003 and 2007, respectively. Since 2017, he has been Associate Professor with the C-PED, ROMA TRE University. His research interests are mainly focused on power converters and electrical machines modeling and control, Hardware-In-the-Loop real-time simulators and Power-Hardware-In-the-Loop emulators, graphical programming of FPGA and development of high-performance control platforms based on combined DSP-FPGA targets.

Marco di Benedetto received the M.Eng. degree in Electronic Engineering from the University of Roma Tor Vergata, Rome, Italy, in 2014, and the Ph.D. in Mechanical and Industrial Engineering from the Roma Tre University, Rome, Italy, in 2018. Since November 2018, he has been a Research Fellow with the Center of Power Electronics and Drives at Roma Tre University. In October 2022, he was appointed to position of Assistant Professor at Roma Tre University. His research interests mainly focus on hardware and FPGA control design for multilevel power converter topologies.
Reanalysis of LIGO black-hole coalescences with alternative prior assumptions
Creators: name: Gerosa, Davide
name: Vitale, Salvatore
name: Haster, Carl-Johan
name: Chatziioannou, Katerina
name: Zimmerman, Aaron
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present a critical reanalysis of the black-hole binary coalescences detected during LIGO's first observing run under different Bayesian prior assumptions. We summarize the main findings of Vitale et al. (2017) and show additional marginalized posterior distributions for some of the binaries' intrinsic parameters.
description: Proceedings of IAU Symposium 338: Gravitational Wave Astrophysics (Baton Rouge, LA, October 2017)
Meyer, Willer
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Endingen
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Circuit Integration of Liquid Metal: Terminator-Inspired Electrical-Thermal Co-Design for Power Electronics -Slides
Creators: Jin Wang
Publisher: name: IEEE
Year: 2024

PELS Webinar Slides

Abstract: This webinar will start with a brief introduction of a few key power electronics research initiatives at the Ohio State University in recent years. The applications of these initiatives span industrial motor drives, electric propulsion for aircraft, and power distribution on the moon's surface. Then, most part of this webinar will concentrate on integrated liquid metal-based cooling for power electronic circuits. The basics of liquid metal-based cooling, principles of pumps, including two circuit-integrated pumps, and the performance, benefits, and remaining challenges of liquid metal-based cooling will be discussed in detail.
Metz, J. J
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Kandern
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
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La previsione dell’insolvenza ex art. 13 co. 3 C.c.i.: efficacia del test di classificazione binario e dell’analisi discriminante lineare
Creators: name: Danovi, Alessandro
name: D'Amico, Alessandro
Publisher: name: Department of Economics and Business Studies, University of Genoa
Year: 2020
Subjects: Accounting and Business Adm.

description: We argue that a multivariate dichotomous classification test is the best tool when forecasting bankruptcy in the context of the upcoming reform of the Italian law on insolvency and restructuring (d.lgs. 14/2019 – Codice della crisi d’impresa e dell’insolvenza). To back our claim, we show an empirical comparison between the ability of the univariate dichotomous classification test and linear discriminant analysis to predict bankruptcy, and discuss the results with respect to the limitations of the two approaches. The tested models are designed based on their features, considering the scope of application of the new legislation, and the evolution over time of the many bankruptcy prediction techniques.
title: 01_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/
Deep neutral hydrogen observations of Leo T with the Westerbork Synthesis Radio Telescope
Creators: name: Adams, Elizabeth A. K.
name: Oosterloo, Tom A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Leo T is the lowest mass gas-rich galaxy currently known and studies of its gas content help us understand how such marginal galaxies survive and form stars. We present deep neutral hydrogen (HI) observations from the Westerbork Synthesis Radio Telescope in order to understand its HI distribution and potential for star formation. We find a larger HI line flux than the previously accepted value, resulting in a 50% larger HI mass of 4.1 x 10^5 Msun. The additional HI flux is from low surface brightness emission that was previously missed; with careful masking this emission can be recovered even in shallower data. We perform a Gaussian spectral decomposition to find a cool neutral medium component (CNM) with a mass of 3.7 x 10^4 Msun, or almost 10% of the total HI mass. Leo T has no HI emission extending from the main HI body, but there is evidence of interaction with the Milky Way circumgalactic medium in both a potential truncation of the HI body and the offset of the peak HI distribution from the optical center. The CNM component of Leo T is large when compared to other dwarf galaxies, even though Leo T is not currently forming stars and has a lower star formation efficiency than other gas-rich dwarf galaxies. However, the HI column density associated with the CNM component in Leo T is low. One possible explanation is the large CNM component is not related to star formation potential but rather a recent, transient phenomenon related to the interaction of Leo T with the Milky Way circumgalactic medium.
description: accepted for publication in A&A; 12 pages, 13 figures
Tolerating Dependences Between Large Speculative Threads Via Sub-Threads
Creators: name: Colohan, Christopher B.
name: Ailamaki, Anastassia
name: J. Gregory Steffan
name: Mowry, Todd C.
Publisher: name: Carnegie Mellon University
Year: 1987
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Thread-level speculation (TLS) has proven to be a promising method of extracting parallelism from both integer and scientific workloads, targeting speculative threads that range in size from hundreds to several thousand dynamic instructions and have minimal dependences between them. Recent work has shown that TLS can offer compelling performance improvements for database workloads, but only when targeting much larger speculative threads of more than 50,000 dynamic instructions per thread, with many frequent data dependences between them. To support such large and dependent speculative threads, hardware must be able to buffer the additional speculative state, and must also address the more challenging problem of tolerating the resulting cross-thread data dependences In this paper we present hardware support for large speculative threads that integrates several previous proposals for TLS hardware. We also introduce support for subthreads: a mechanism for tolerating cross-thread data dependences by checkpointing speculative execution. When speculation fails due to a violated data dependence, with sub-threads the failed thread need only rewind to the checkpoint of the appropriate sub-thread rather than rewinding to the start of execution; this significantly reduces the cost of mis-speculation. We evaluate our hardware support for large and dependent speculative threads in the database domain and find that the transaction response time for three of the five transactions from TPC-C (on a simulated 4- processor chip-multiprocessor) speedup by a factor of 1.9 to 2.9.
Meyer, Friedrich
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Waldenburg
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Numerical simulations of particle sedimentation using the immersed boundary method
Creators: name: Ghosh, Sudeshna
name: Stockie, John M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences
subject: 74F10, 76D05, 76M20, 76T20

description: We study the settling of solid particles within a viscous incompressible fluid contained in a two-dimensional channel, where the mass density of the particles is slightly greater than that of the fluid. The fluid-structure interaction problem is simulated numerically using the immersed boundary method, with an added mass term that is incorporated using a Boussinesq approximation. Simulations are performed with a single circular particle, and also with two particles in various initial configurations. The terminal settling velocities for the particles correspond closely with both theoretical and experimental results, and the single-particle dynamics reproduce expected behavior qualitatively. The two-particle simulations exhibit drafting-kissing-tumbling dynamics that is similar to what is observed in other experimental and numerical studies.
Three-body recombination near a narrow Feshbach resonance in $^6$Li
Creators: name: Li, Jiaming
name: Liu, Ji
name: Luo, Le
name: Gao, Bo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We experimentally measure, and theoretically analyze the three-atom recombination rate, $L_3$, around a narrow $s$ wave magnetic Feshbach resonance of $^6$Li-$^6$Li at 543.3 Gauss. By examining both the magnetic field dependence and especially the temperature dependence of $L_3$ over a wide range of temperatures from a few $μ$K to above 200 $μ$K, we show that three-atom recombination through a narrow resonance follows a universal behavior determined by the long-range van der Waals potential, and can be described by a set of rate equations in which three-body recombination proceeds via successive pairwise interactions. We expect the underlying physical picture to be applicable not only to narrow $s$ wave resonances, but also to resonances in nonzero partial waves, and not only at ultracold temperatures, but also at much higher temperatures.
description: 6 pages,7 figures, 1 table
Reddened Dimming of Boyajian's Star Supports Internal Storage of Its "Missing" Flux
Creators: name: Foukal, Peter
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Two recent short term dimmings of KIC 8462852 (Boyajian's Star) exhibit clear reddening in the B, r' and i' photometric passbands. We show that the intensity ratios of the three pass bands agree well with cooling of an approximately 6800 K black body by about 30K. This agreement, together with other recent findings on the timing and longer term dimmings of this star, support our previous argument that the star's photometric behavior is caused by internal storage of impeded convective flux, rather than by external sources of obscuration such the ISM or circumstellar material.
Oppenheimer, Abraham Isaac
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Frankfurt a. M.
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Spherical Relativistic Radiation Flows with Variable Eddington Factor
Creators: name: Akizuki, Chizuru
name: Fukue, Jun
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We solve spherically symmetric radiation flows under full special relativity with the help of a variable Eddington factor $f(τ, β)$, where $τ$ is the optical depth and $β$ is the flow velocity normalized by the speed of light. Relativistic radiation hydrodynamics under the moment formalism has several complex problems, such as a closure relation. Conventional moment equations closed with the traditional Eddington approximation in the comoving frame have singularity, beyond which the flow cannot be accelerated. In order to avoid such a pathological behavior inherent in the relativistic moment formalism, we propose a variable Eddington factor, which depends on the flow velocity as well as the optical depth, for the case of the sperically symmertic one-dimensional flow. We then calculate the relaticistic spherical flow with such variable Eddington factors to investigate the case that gas is accelerated by radiative force. As a result, it is shown that the gas speed reaches around the speed of light by radiation pressure.
description: 7 pages, 5 figures; PASJ 60 (2008) in press
title: ADCO, Cart. 186 (11 H 71), f. 0445v
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/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: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la Côte-d'Or, C
art. 186 (11 H 71). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la
 Côte-d'Or, Cart. 186 (11 H 71), f. 0445v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-
project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Title Generation for Spoken Broadcast News using a Training Corpus
Creators: name: Jin, Rong
name: Hauptmann, 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: The problem of title generation involves finding the essence of a document and expressing it in only a few words. The results of a query to the Informedia Digital Video Library are summarized through an automatically generated title for each retrieved news story. When the document is errorful, as with speech-recognized broadcast news stories, the title creation challenge becomes even greater. We implemented a set of title word selection strategies and evaluated them on an independent test corpus of 579 broadcast news documents, comparing manual transcription results to automatically recognized speech using the CMU Sphinx speech recognition system with a 64000-word broadcast news language model. Using a training collection of 21190 transcribed broadcast news stories, we trained several systems to produce appropriate title words, i.e. Naïve Bayesian approach with full vocabulary, Naïve Bayesian approach with limited vocabulary, nearest neighbor approach and extractive approach. The F1 results shows that the nearest neighbor approach is a quick and easy way of generating good titles for speech recognized documents (F1 = 15.2%), while a Nave Bayesian approach with limited vocabulary also does well on our F1 measure (F1 = 21.6%), which ignores word order in the titles. Overall, the results show that title generation for speech recognized news documents is possible at a level approaching the accuracy of titles generated for perfect text transcriptions. One surprising phenomenon is that extractive approach performances slightly better for speech recognized documents than for manual transcripts.
Ott-Escher, Caspar, zur Engelburg
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Zürich
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Orbital misalignment of the Neptune-mass exoplanet GJ 436b with the spin of its cool star
Creators: name: Bourrier, Vincent
name: Lovis, Christophe
name: Beust, Hervé
name: Ehrenreich, David
name: Henry, Gregory W.
name: Astudillo-Defru, Nicola
name: Allart, Romain
name: Bonfils, Xavier
name: Ségransan, Damien
name: Delfosse, Xavier
name: Cegla, Heather M.
name: Wyttenbach, Aurélien
name: Heng, Kevin
name: Lavie, Baptiste
name: Pepe, Francesco
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The angle between the spin of a star and its planets' orbital planes traces the history of the planetary system. Exoplanets orbiting close to cool stars are expected to be on circular, aligned orbits because of strong tidal interactions with the stellar convective envelope. Spin-orbit alignment can be measured when the planet transits its star, but such ground-based spectroscopic measurements are challenging for cool, slowly-rotating stars. Here we report the characterization of a planet three-dimensional trajectory around an M dwarf star, derived by mapping the spectrum of the stellar photosphere along the chord transited by the planet. We find that the eccentric orbit of the Neptune-mass exoplanet GJ 436b is nearly perpendicular to the stellar equator. Both eccentricity and misalignment, surprising around a cool star, can result from dynamical interactions (via Kozai migration) with a yet-undetected outer companion. This inward migration of GJ 436b could have triggered the atmospheric escape that now sustains its giant exosphere. Eccentric, misaligned exoplanets orbiting close to cool stars might thus hint at the presence of unseen perturbers and illustrate the diversity of orbital architectures seen in exoplanetary systems.
description: Published in Nature on 18 Decembre 2017. Preprint is 25 pages, 12 figures, 2 tables
Nicolier, Jean Etienne
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Vevey
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FigureS2-6.pdf from Behavioural red-light sensitivity in fish according to the optomotor response
Creators: name: Matsuo, Megumi
name: Kamei, Yasuhiro
name: Fukamachi, Shoji
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: 60801 Animal Behaviour
subject: FOS: Biological sciences

description: The four parameters for mbuna in second-round OMR assay. The quantified OMR of mbuna. The four parameters of OMR, i.e., (A) Delay, (B) Duration, (C) Angular Velocity, (D) Distance, are shown. Values represent means. Error bars are standard errors (SEs).
title: ADCO, Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Cart. 181 (11 H 754), 165 folios, f. 0222
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/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 181 (11 H 754), 165 folios, f. 0222, 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. 181 (11 H 754), 165 folios, f. 0222, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Catalytic Coherence
Creators: name: Aberg, Johan
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Due to conservation of energy we cannot directly turn a quantum system with a definite energy into a superposition of different energies. However, if we have access to an additional resource in terms of a system with a high degree of coherence, as for standard models of laser light, we can overcome this limitation. The question is to what extent coherence gets degraded when utilized. Here it is shown that coherence can be turned into a catalyst, meaning that we can use it repeatedly without ever diminishing its power to enable coherent operations. This finding stands in contrast to the degradation of other quantum resources, and has direct consequences for quantum thermodynamics, as it shows that latent energy that may be locked into superpositions of energy eigenstates can be released catalytically.
description: Added material, journal reference
MPEC 2024-U107 : 2024 UU2
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 UU2

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Measurement of $\hat{q}$ in RHI collisions using di-hadron correlations
Creators: name: Tannenbaum, M. J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: In the BDMPSZ model, the energy loss of an outgoing parton in a medium $-dE/dx$ is the transport coefficient $\hat{q}$ times $L$ the length traveled. This results in jet quenching, which is well established. However BDMPSZ also predicts an azimuthal broadening of di-jets also proportional to $\hat{q}L$ which has so far not been observed. The broadening should produce a larger $k_T$ in A$+$A than in p$+$p collisions. This presentation introduces the observation that the $k_T$ measured in p$+$p collisions for di-hadrons with $p_{Tt}$ and $p_{Ta}$ must be reduced to compensate for the energy loss of both the trigger and away parent partons when comparing to the $k_T$ measured with the same di-hadron $p_{Tt}$ and $p_{Ta}$ in A$+$A collisions. This idea is applied to a recent STAR di-hadron measurement in Au$+$Au at $\sqrt{s_{NN}}$=200 GeV, [Phys. Lett. B760 (2016) 689], with result $=2.1\pm 0.6$ GeV$^2$. This is more precise but in agreement with a theoretical calculation of $=14^{+42}_{-14}$ GeV$^2$ using the same data. Assuming a length $\approx 7$ fm for central Au$+$Au collisions the present result gives $\hat{q}\approx 0.30\pm 0.09$ GeV$^2$/fm, in fair agreement with the JET collaboration result from single hadron suppression of $\hat{q}\approx 1.2\pm 0.3$ GeV$^2$/fm at an initial time $τ_0=0.6$ fm/c in Au$+$Au collisions at $\sqrt{s_{NN}}=200$ GeV. There are several interesting details to be discussed: for a given $p_{Tt}$ the $$ seems to decrease then vanish with increasing $p_{Ta}$; the di-jet spends a much longer time in the medium ($\approx 7$ fm/c) then $τ_0=0.6$ fm/c which likely affects the value of $\hat{q}$ that would be observed.
description: 6 text pages plus abstract, 6 figures, 1 table, Proceedings of the 12th International Workshop on High-pT Physics in the RHIC/LHC Era, 2-5 October, 2017 University of Bergen, Bergen, Norway. To appear in Proceedings of Science
FigureS1-3.pdf from Behavioural red-light sensitivity in fish according to the optomotor response
Creators: name: Matsuo, Megumi
name: Kamei, Yasuhiro
name: Fukamachi, Shoji
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: 60801 Animal Behaviour
subject: FOS: Biological sciences

description: The four parameters for zebrafish in first-round OMR assay. The quantified OMR of zebrafish. The four parameters of OMR, i.e., (A) Delay, (B) Duration, (C) Angular Velocity, (D) Distance, are shown. Values represent means. Error bars are standard errors (SEs).
From Rota-Baxter Algebras to Pre-Lie Algebras
Creators: name: An, Huihui
name: Bai, Chengming
Publisher: name: arXiv
Year: 2007
Subjects: subject: Mathematical Physics (math-ph)
subject: Quantum Algebra (math.QA)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 17B, 81R

description: Rota-Baxter algebras were introduced to solve some analytic and combinatorial problems and have appeared in many fields in mathematics and mathematical physics. Rota-Baxter algebras provide a construction of pre-Lie algebras from associative algebras. In this paper, we give all Rota-Baxter operators of weight 1 on complex associative algebras in dimension $\leq 3$ and their corresponding pre-Lie algebras.
description: 23 pages, appear in Journal of Physics A; Mathematical and Theoretical
Koencke, Heinrich, & Edlefsen
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Hamburg
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
title: 03_0167
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/
Ripples and Charge Puddles in Graphene on a Metallic Substrate
Creators: name: Martin, S. C.
name: Samaddar, S.
name: Sacépé, B.
name: Kimouche, A.
name: Coraux, J.
name: Fuchs, F.
name: Grévin, B.
name: Courtois, H.
name: Winkelmann, C. B.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Graphene on a dielectric substrate exhibits spatial doping inhomogeneities, forming electron-hole puddles. Understanding and controlling the latter is of crucial importance for unraveling many of graphene's fundamental properties at the Dirac point. Here we show the coexistence and correlation of charge puddles and topographic ripples in graphene decoupled from the metallic substrate it was grown on. The analysis of interferences of Dirac fermion-like electrons yields a linear dispersion relation, indicating that graphene on a metal can recover its intrinsic electronic properties.
description: 4 figures
The Star Formation Demographics of Galaxies in the Local Volume
Creators: name: Lee, Janice C.
name: Kennicutt, Robert C.
name: Funes, Jose G.
name: J., S.
name: Sakai, Shoko
name: Akiyama, Sanae
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the connections between the current global star formation activity, luminosity, dynamical mass and morphology of galaxies in the Local Volume, using H-alpha data from the 11 Mpc H-alpha and Ultraviolet Galaxy Survey (11HUGS). Taking the equivalent width (EW) of the H-alpha emission line as a tracer of the specific star formation rate, we analyze the distribution of galaxies in the M_B-EW and rotational velocity (V_{max})-EW planes. Star-forming galaxies show two characteristic transitions in these planes. A narrowing of the galaxy locus occurs at M_B~-15 and V_{max}~50 km/s, where the scatter in the logarithmic EWs drops by a factor of two as the luminosities/masses increase, and galaxy morphologies shift from predominately irregular to late-type spiral. Another transition occurs at M_B~-19 and V_{max}~120 km/s, above which the sequence turns off toward lower EWs and becomes mostly populated by intermediate and early-type bulge-prominent spirals. Between these two transitions, the mean logarithmic EW appears to remain constant at 30 A. We comment on how these features reflect established empirical relationships, and provide clues for identifying the large-scale physical processes that both drive and regulate star formation, with emphasis on the low-mass galaxies that dominate our approximately volume-limited sample.
description: 5 pages, accepted for publication in ApJL pending editing for length
Aristotle on the limits of final causes. The case of extended teleology
Creators: name: Hernández Villarreal, Andrés
Publisher: name: University of St Andrews
Year: 2021

description: In this thesis, I discuss the concept of Aristotelian extended teleology (i.e., non-theistic teleological causation in which more than one substance is involved). I argue that some passages of Aristotle’s corpus and Theophrastus’ Metaphysics can be read as arguments of extended teleology. To interpret those passages, I introduce the concept of “axiarchism”, according to which X is actual because X is good. The thesis is composed of five chapters. In chapter 1, I introduce both the doctrine of Aristotle’s four causes and the discussion of the reach of final causes according to the second book of the Physics. In chapter 2, I discuss the teleological arguments that can be found in the first book of Aristotle’s Politics. I argue that some of these arguments can be read as arguments for extended teleology. In chapter 3, I argue that it is reasonable to suppose that, for Aristotle, the sublunary is not a random result of the superlunary and that, therefore, there is some form of order in all the parts of the universe. In this chapter, I focus particularly on Physics VIII, Generation and Corruption II 10. In the fourth chapter, I discuss Metaphysics XII. I defend the view that the tenth chapter of book Lambda can be read as an explicit question about the order and unity of all the parts of the world. In chapter 5, I discuss Theophrastus’ Metaphysics. I argue that Theophrastus is pointing towards the need for an account of extended teleology. He claims that not everything can be the result of a final cause, because some natural phenomena (e.g., the rotation of the sun that causes the yearly seasons) cannot be explained in teleological terms. In questioning the possibility of explaining these phenomena in teleological terms, however, Theophrastus is already thinking in terms of extended teleology.
Dimensionality Reduction in Deep Learning for Chest X-Ray Analysis of Lung Cancer
Creators: name: Gordienko, Yu.
name: Kochura, Yu.
name: Alienin, O.
name: Rokovyi, O.
name: Stirenko, S.
name: Gang, Peng
name: Hui, Jiang
name: Zeng, Wei
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (cs.LG)
subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: Efficiency of some dimensionality reduction techniques, like lung segmentation, bone shadow exclusion, and t-distributed stochastic neighbor embedding (t-SNE) for exclusion of outliers, is estimated for analysis of chest X-ray (CXR) 2D images by deep learning approach to help radiologists identify marks of lung cancer in CXR. Training and validation of the simple convolutional neural network (CNN) was performed on the open JSRT dataset (dataset #01), the JSRT after bone shadow exclusion - BSE-JSRT (dataset #02), JSRT after lung segmentation (dataset #03), BSE-JSRT after lung segmentation (dataset #04), and segmented BSE-JSRT after exclusion of outliers by t-SNE method (dataset #05). The results demonstrate that the pre-processed dataset obtained after lung segmentation, bone shadow exclusion, and filtering out the outliers by t-SNE (dataset #05) demonstrates the highest training rate and best accuracy in comparison to the other pre-processed datasets.
description: 6 pages, 14 figures