cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Equality in the European Union
Creators: name: Michał Piechowicz
Publisher: name: figshare
Year: 2018
Subjects: subject: 160609 Political Theory and Political Philosophy
subject: FOS: Political science
subject: 160699 Political Science not elsewhere classified

description: Equality in the European Union, 2015Gender equality is a vital aspect of the European integration process. Although specific legislation concerning gender issues was included in the establishing Treaties, in the Charter of fundamental rights and in a dozen other directives, non-discriminatory principle has also been strengthened by the jurisdiction of the Court of Justice of the European Union which formed a judgment in more than 200 cases. Nowadays, the EU equality legislation has moved far beyond basic gender issues, and this is also discussed in the article. It focuses not only on the fundamentals of EU legislation concerning gender equality but also on the level of its implementation and its most important limitations. Such considerations are broadened by a discussion on the EU actions which may be also treated as the implementation of non-discriminatory legislation.
Lusthaus Lustgarten Lustwandeln - Cinque Salettln di Josef Hoffmann
Creators: name: Rakowitz, Gundula
Publisher: name: Firenze Architettura
Year: 2019

description: Josef Hoffmann's five Salettln are machines à amuser, they activate emotions and feelings, expressing their most hidden secrets also by using the tricks of artifice and disguise, surprise and charm, seduction and pleasure. This is a time-place that invites us to wander, to “let the soul hang loose”: Lustwandeln in the labyrinth of the Lustgarten reaching the Lusthaus.
description: Firenze Architettura, Vol 23 No 1 (2019)
Statistical analysis of vortex condensate motion in two-dimensional turbulence
Creators: name: Parfenyev, Vladimir
Publisher: name: arXiv
Year: 2023
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: An inverse turbulent cascade in a periodic square box produces a coherent system-sized vortex dipole. We study the statistics of its motion by carrying out direct numerical simulations performed for various bottom friction $α$, pumping intensity $\varepsilon$, and fluid hyperviscosity $ν$. In the main approximation, coherent vortices can be considered as point vortices, and within this model, they drift at the same dipole velocity, which is determined by their circulation and mutual arrangement. The characteristic value of the dipole velocity is more than an order of magnitude smaller than the polar velocity inside coherent vortices. Turbulent fluctuations give rise to a relative velocity between the vortices, which changes the distance between them. We found that for a strong condensate, the probability density function of the vector $\bf ρ$, describing the difference in the mutual arrangement of coherent vortices from half the diagonal of the computational domain, has the form of a ring. The radius of the ring weakly depends on control parameters and the width of the ring is proportional to the dimensionless parameter $δ= ε^{-1/3} L^{2/3} α$, where $ε$ is the inverse energy flux and $L$ is the system size. The random walk around the ring, caused by turbulent fluctuations, has superdiffusion behavior at intermediate times. It results in a finite correlation time of the dipole velocity, which turns out to be of the order of turnover time $τ_K = L^{2/3} ε^{-1/3}$ of system-size eddies produced by an inverse turbulent cascade. The results obtained deepen the understanding of the processes governing the motion of coherent vortices.
Features in the primordial power spectrum of double D-term inflation
Creators: name: Lesgourgues, Julien
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recently, there has been some interest for building supersymmetric models of double inflation. These models, realistic from a particle physics point of view, predict a broken-scale-invariant power spectrum of primordial cosmological perturbations, that may explain eventual non-trivial features in the present matter power spectrum. In previous works, the primordial spectrum was calculated using analytic slow-roll approximations. However, these models involve a fast second-order phase transition during inflation, with a stage of spinodal instability, and an interruption of slow-roll. For our previous model of double D-term inflation, we simulate numerically the evolution of quantum fluctuations, taking into account the spinodal modes, and we show that the semi-classical approximation can be employed even during the transition, due to the presence of a second inflaton field. The primordial power spectrum possesses a rich structure, and possibly, a non-Gaussian spike on observable scales.
description: 42 pages, 8 figures. Minor changes, version accepted in Nucl. Phys. B
Quasi-Normal Modes of Loop Quantum Black Holes Formed from Gravitational Collapse
Creators: name: Zhang, Chao
name: Wang, Anzhong
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper, we study the quasi-normal modes (QNMs) of a scalar field in the background of a large class of quantum black holes that can be formed from gravitational collapse of a dust fluid in the framework of effective loop quantum gravity. The loop quantum black holes (LQBHs) are characterized by three free parameters, one of which is the mass parameter, while the other two are purely due to quantum geometric effects. Among these two quantum parameters, one is completely fixed by black hole thermodynamics and its effects are negligible for macroscopic black holes, while the second parameter is completely free (in principle). In the studies of the QNMs of such LQBHs, we pay particular attention to the difference of the QNMs between LQBHs and classical ones, so that they can be observed for the current and forthcoming gravitational wave observations, whereby place the LQBH theory directly under the test of observations.
description: version published in JCAP 10 (2024) 070
On the origin of force sensitivity in tests of quantum gravity with delocalised mechanical systems
Creators: name: Pedernales, Julen S.
name: Plenio, Martin B.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Physics (quant-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The detection of the quantum nature of gravity in the low-energy limit hinges on achieving an unprecedented degree of force sensitivity with mechanical systems. Against this background, we explore the relationship between the sensitivity of mechanical systems to external forces and the properties of the quantum states they are prepared in. We establish that the main determinant of the force sensitivity in pure quantum states is their spatial delocalisation and we link the force sensitivity to the rate at which two mechanical systems become entangled under a quantum force. We exemplify this at the hand of two commonly considered configurations. One that involves gravitationally interacting objects prepared in non-Gaussian states such as Schrödinger-cat states, where the generation of entanglement is typically ascribed to the accumulation of a dynamical phase between components in superposition. The other prepares particles in Gaussian states that are strongly squeezed in momentum and delocalised in position where entanglement generation is attributed to accelerations. We offer a unified description of these two arrangements using the phase-space representation and link their entangling rate to their force sensitivity, showing that both configurations get entangled at the same rate provided that they are equally delocalised in space. Our description in phase space and the established relation between force sensitivity and entanglement sheds light on the intricacies of why the equivalence between these two configurations holds, something that is not always evident in the literature, due to the distinct physical and analytical methods employed to study each of them. Notably, we demonstrate that while the conventional computation of entanglement via the dynamical phase remains accurate for Schrödinger-cat states, it yields erroneous estimations for systems in squeezed cat states.
description: Invited contribution to Contemporary Physics. 16 pages (+ bibliography), 6 figures
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0587
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0587, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0587, 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
Evaluating surgical skills from kinematic data using convolutional neural networks
Creators: name: Fawaz, Hassan Ismail
name: Forestier, Germain
name: Weber, Jonathan
name: Idoumghar, Lhassane
name: Muller, Pierre-Alain
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: The need for automatic surgical skills assessment is increasing, especially because manual feedback from senior surgeons observing junior surgeons is prone to subjectivity and time consuming. Thus, automating surgical skills evaluation is a very important step towards improving surgical practice. In this paper, we designed a Convolutional Neural Network (CNN) to evaluate surgeon skills by extracting patterns in the surgeon motions performed in robotic surgery. The proposed method is validated on the JIGSAWS dataset and achieved very competitive results with 100% accuracy on the suturing and needle passing tasks. While we leveraged from the CNNs efficiency, we also managed to mitigate its black-box effect using class activation map. This feature allows our method to automatically highlight which parts of the surgical task influenced the skill prediction and can be used to explain the classification and to provide personalized feedback to the trainee.
description: Accepted at MICCAI 2018
Stanze per fare l’amore. Illusione e seduzione in quattro interni del Novecento
Creators: name: Saitto, Viviana
Publisher: name: Firenze Architettura
Year: 2019

description: Four well-known 20th century interiors demonstrate that seduction is the space for play, illusion and challenge. Ettore Sottsass' camera per fare l’amore and the spaces devised for repose at Carlo Mollino's Casa Devalle in Turin, Carlo Scarpa's Casa Ottolonghi in Bardolino and Le Corbusier's Villa Savoye in Poissy, were designed to se-ducere, to lead aside, they are the mirror of the unconscious and of desire.
description: Firenze Architettura, Vol 23 No 1 (2019)
Theory of Rare B Decays
Creators: name: Falk, Adam F.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Theoretical aspects of rare $B$ decays are reviewed. The focus is on the relation between short-distance interactions and physical observables. It is argued that there remain significant uncertainties in the theoretical treatment of certain important quantities. (Talk presented at the International Symposium on Vector Boson Interactions, University of California, Los Angeles, February 1-3, 1995)
description: 12 pages, uses REVTeX with aps.sty, epsf.sty, floats.sty; 10 uuencoded .eps figures included
Stanze tutte per sé. Architettura e piacere negli interni milanesi di Nanda Vigo
Creators: name: Carli, Giovanni
Publisher: name: Firenze Architettura
Year: 2019

description: Nanda Vigo's Milanese interiors show the power of the exotic/erotic and multicultural imaginary of the cosmopolitan city dweller: her clients are art collectors who wish to live the pleasure of the oggetto unico, for a complete synthesis between art and architecture. Nanda Vigo goes beyond the house as a place of dwelling, transforming in into a contemporary scenic spectacle with an elevated technological and symbolic content.
description: Firenze Architettura, Vol 23 No 1 (2019)
Study of the optical to X-ray broad emission lines of Mrk 110
Creators: name: Juráňová, A.
name: Costantini, E.
name: Di Gesu, L.
name: Ebrero, J.
name: Kaastra, J.
name: Korista, K.
name: Kriss, G. A.
name: Mehdipour, M.
name: Piconcelli, E.
name: Rogantini, D.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In order to shed light on the characteristics of the broad line region (BLR) in a narrow-line Seyfert 1 galaxy, we present an analysis of X-ray, UV, and optical spectroscopic observations of the broad emission lines in Mrk 110. For the broad-band modelling of the emission-line luminosity, we adopt the `locally optimally emitting cloud' approach, which allows us to place constraints on the gas radial and density distribution. By exploring additional environmental effects, we investigate the possible scenarios resulting in the observed spectra. We find that the photoionised gas in Mrk 110 responsible for the UV emission can fully account for the observed low-ionisation X-ray lines. The overall ionisation of the gas is lower, and one radial power-law distribution with a high integrated covering fraction $C_{\mathrm{f}} \approx 0.5$ provides an acceptable description of the emission lines spanning from X-rays to the optical band. The BLR is likely more compact than the broad-line Seyfert 1s studied so far, extending from $\sim\!10^{16}$ to $\sim\!10^{18}$ cm, and limited by the dust sublimation radius at the outer edge. Despite the large colour excess predicted by the Balmer ratio, the best fit suggests $E(B-V)\approx0.03$ for both the ionising luminosity and the BLR, indicating that extinction might be uniform over a range of viewing angles. While the adopted data-modelling technique does not allow us to place constraints on the geometry of the BLR, we show that the addition of models with a clumpy, equatorial, wind-like structure may lead to a better description of the observed spectra.
description: Accepted for publication in A&A
Using differential equations to compute two-loop box integrals
Creators: name: Gehrmann, T.
name: Remiddi, E.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The calculation of exclusive observables beyond the one-loop level requires elaborate techniques for the computation of multi-leg two-loop integrals. We discuss how the large number of different integrals appearing in actual two-loop calculations can be reduced to a small number of master integrals. An efficient method to compute these master integrals is to derive and solve differential equations in the external invariants for them. As an application of the differential equation method, we compute the ${\cal O}(ε)$-term of a particular combination of on-shell massless planar double box integrals, which appears in the tensor reduction of $2 \to 2$ scattering amplitudes at two loops.
description: 5 pages, LaTeX, uses espcrc2.sty; presented at Loops and Legs in Quantum Field Theory, April 2000, Bastei, Germany
Bezpieczeństwo dostaw w kontekście rozbudowy infrastruktury przesyłowej w Polsce
Creators: name: Michał Piechowicz
Publisher: name: figshare
Year: 2018
Subjects: subject: 160206 Private Policing and Security Services
subject: FOS: Law

description: Bezpieczeństwo energetyczne rynki surowców i energii, teraźniejszość i przyszłość – gospodarka zasoby naturalne i logistyka, 2014The idea of building interconnectors between the transmission systems of the EU Member States is evolving and getting more visible in Poland. This approach is a part of the implementation of European Energy Policy, which aims to strengthen cooperation between Member States' energy sectors. Combining transmission networks in the EU has also been included as one of the strategic objectives of the national energy policy and a tool of ensuring security of supplies. It is pointed out that the EU needs a fully functioning, connected and integrated internal market of energy, so that no country is isolated from the European network of transmission. The article discusses the grid investments in Poland and make comments on national interconnections in the context of their use of free bandwidth.
Inclusive Decays of B Mesons into D_s and $D_s^{\ast}$ at $O(α_s)$ Including $D_s^{\ast}$ Polarization Effects
Creators: name: Fischer, M.
name: Groote, S.
name: Körner, J. G.
name: Mauser, M. C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The dominant contribution to the inclusive decays of $B$ mesons into the charm-strangeness mesons $D_s$ and $D_s^{\ast}$ is expected to be given by the partonic process $b \to c+(D_s^-,D_s^{\ast -})$. We determine the nonperturbative $O(1/m_b^2)$ and the $O(α_s)$ radiative corrections to $b \to c+(D_s^-,D_s^{\ast -})$ and thereby to the inclusive decays $ \bar{B} \to X_c+(D_s^-,D_s^{\ast -})$. The new feature of our calculation is that we separately determine the nonperturbative and the $O(α_s)$ corrections to the longitudinal ($L$) and transverse ($T$) pieces of the spin 1 $D_s^{\ast -}$ meson. The longitudinal/transverse composition of the $D_s^{\ast -}$ can be probed through its two principal decay modes $D_s^{\ast -} \to D_s^- + γ$ and $D_s^{\ast -} \to D_s^- + π^0$ for which we write down the angular decay distributions.
description: 13 pages, 2 postscript figures added, will be published in Physics Letters B
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Cart. 185 (11 H 70), f. 0236r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0236r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0236r, 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
Novecento d’acqua e di terra. Il Tennis Club di Giovanni Muzio a Milano
Creators: name: Lisini, Caterina
Publisher: name: Firenze Architettura
Year: 2019

description: In Muzio's Tennis Club in Milan there is an evident reference to the classical tradition in architecture and to the use of compositive modules and figures typical of the 20th century in Milan. However, in the swimming pool complex there is also the presence of the contemporary research of metaphysical painting, which results almost in a meeting point between his work from the Twenties and his later mature masterpieces.
description: Firenze Architettura, Vol 23 No 1 (2019)
Superconformal 6D (2,0) theories in superspace
Creators: name: Grojean, C.
name: Mourad, J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A geometrical construction of superconformal transformations in six dimensional (2,0) superspace is proposed. Superconformal Killing vectors are determined. It is shown that the transformation of the tensor multiplet involves a zero curvature non-trivial cochain.
description: 18 pages, LaTeX. Two references added. A comment on superembedding formalism added. Misprints corrected
The onset of stellar multiplicity in massive star formation: A search for low-mass companions of massive young stellar objects with $L'$-band adaptive optics imaging
Creators: name: Bordier, E.
name: de Wit, W. -J.
name: Frost, A. J.
name: Sana, H.
name: Pauwels, T.
name: Koumpia, E.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Given the high incidence of binaries among mature field massive stars, it is clear that multiplicity is an inevitable outcome of high-mass star formation. Understanding how massive multiples form requires the study of the birth environments of massive stars, covering the innermost to outermost regions. We aim to detect and characterise low-mass companions around massive young stellar objects (MYSOs) during and shortly after their formation phase. To investigate large spatial scales, we carried out an $L'$-band high-contrast direct imaging survey seeking low-mass companions (down to $L_{\text{bol}}\approx 10 L_{\odot}$, or late A-type) around thirteen previously identified MYSOs using the VLT/NACO instrument. From those images, we looked for the presence of companions on a wide orbit, covering scales from 300 to 56,000 au. Detection limits were determined for all targets and we tested the gravitational binding to the central object based on chance projection probabilities. We have discovered a total of thirty-nine potential companions around eight MYSOs, the large majority of which have never been reported to date. We derived a multiplicity frequency (MF) of $62\pm13$% and a companion fraction (CF) of $3.0\pm0.5$. The derived MF and CF are compared to other studies for similar separation ranges. The comparisons are effective for a fixed evolutionary stage spanning a wide range of masses and vice versa. We find an increased MF and CF compared to the previous studies targeting MYSOs, showing that the statement in which multiplicity scales with primary mass also extends to younger evolutionary stages. The separations at which the companions are found and their location with relation to the primary star allow us to discuss the implications for the massive star formation theories.
description: 24 pages, 2 Tables, 5 Figures and 4 appendices (containing figures)
Badania dotyczące reprezentacji interesów przedsiębiorstw woj. kujawsko-pomorskiego na poziomie UE - wstęp
Creators: name: Michał Piechowicz
Publisher: name: figshare
Year: 2018
Subjects: subject: 150314 Small Business Management
subject: FOS: Economics and business

description: Badania dotyczące reprezentacji interesów przedsiębiorstw woj. kujawsko-pomorskiego na poziomie UEArticle starts from the exceptionality of lobbying and its related aspects at the supranational level. It also reveals interest representation phenomenon from the perspective of corporate interests and discuss forms of actions and associations of companies on the EU forum. Moreover it defines basic concepts and is an introduction to research project of interest representation of companies from the Kuyavia and Pomerania region in the EU institutions.
The phase function for stellar acoustic oscillations - IV. Solar-like stars
Creators: name: Hernandez, F. Perez
name: Christensen-Dalsgaard, J.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In recent years there has been some progress towards detecting solar-like oscillations in stars. The goal of this challenging project is to analyse frequency spectra similar to that observed for the Sun in integrated light. In this context it is important to investigate what can be learned about the structure and evolution of the stars frIn recent years there has been some progress towards detecting solar-like oscillations in stars. The goal of this challenging project is to analyse frequency spectra similar to that observed for the Sun in integrated light. In this context it is important to investigate what can be learned about the structure and evolution of the stars from such future observations. Here we concentrate on the structure of the upper layers, as reflected in the phase function. We show that it is possible to obtain this function from low-degree p modes, at least for stars on the main sequence. We analyse its dependence on several uncertainties in the structure of the uppermost layers. We also investigate a filtered phase function, which has properties that depend on the layers around the second helium ionization zone.om such future observations. Here we concentrate on the structure of the upper layers, as reflected in the phase function. We show that it is possible to obtain this function from low-degree p modes, at least for stars on the main sequence. We analyse its dependence on several uncertainties in the structure of the uppermost layers. We also investigate a filtered phase function, which has properties that depend on the layers around the second helium ionization zone.
description: 10 pages, 10 figures. Submitted to Mon. Not. R. astr. Soc
Cross-Domain Collaborative Learning via Cluster Canonical Correlation Analysis and Random Walker for Hyperspectral Image Classification
Creators: name: Qin, Yao
name: Bruzzone, Lorenzo
name: Li, Biao
name: Ye, Yuanxin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Image and Video Processing (eess.IV)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: This paper introduces a novel heterogenous domain adaptation (HDA) method for hyperspectral image classification with a limited amount of labeled samples in both domains. The method is achieved in the way of cross-domain collaborative learning (CDCL), which is addressed via cluster canonical correlation analysis (C-CCA) and random walker (RW) algorithms. To be specific, the proposed CDCL method is an iterative process of three main stages, i.e. twice of RW-based pseudolabeling and cross domain learning via C-CCA. Firstly, given the initially labeled target samples as training set ($\mathbf{TS}$), the RW-based pseudolabeling is employed to update $\mathbf{TS}$ and extract target clusters ($\mathbf{TCs}$) by fusing the segmentation results obtained by RW and extended RW (ERW) classifiers. Secondly, cross domain learning via C-CCA is applied using labeled source samples and $\mathbf{TCs}$. The unlabeled target samples are then classified with the estimated probability maps using the model trained in the projected correlation subspace. Thirdly, both $\mathbf{TS}$ and estimated probability maps are used for updating $\mathbf{TS}$ again via RW-based pseudolabeling. When the iterative process finishes, the result obtained by the ERW classifier using the final $\mathbf{TS}$ and estimated probability maps is regarded as the final classification map. Experimental results on four real HSIs demonstrate that the proposed method can achieve better performance compared with the state-of-the-art HDA and ERW methods.
description: 14 pages, 10 figures
Analiza obecnego stanu integracji i możliwe kierunki rozwoju UE
Creators: name: Michał Piechowicz
Publisher: name: figshare
Year: 2018
Subjects: subject: 160699 Political Science not elsewhere classified
subject: FOS: Political science
subject: 160607 International Relations

description: Integracja Europejska - przeszłość, teraźniejszość, przyszłość, 2009This analysis includes main factors which are a creative force of european integration process, discuss main integration theories and deal with the EU as an international organization in the context of international relations
Transient dynamics in strongly nonlinear systems: optimization of initial conditions on the resonant manifold
Creators: name: Perchikov, Nathan
name: Gendelman, O. V.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: We consider a system of two linear and linearly coupled oscillators with ideal impact constraints. Primary resonant energy exchange is investigated by analysis of the slow-flow using the action-angle (AA) formalism. Exact inversion of the action-energy dependence for the linear oscillator with impact constraints is not possible. This difficulty, typical for many models of nonlinear oscillators, is circumvented by matching the asymptotic expansions for the linear and impact limits. The obtained energy-action relation enables the complete analysis of the slow-flow and the accurate description of the critical delocalization transition. The transition from the localization regime to the energy-exchange regime is captured by prediction of the critical coupling value. Accurate prediction of the delocalization transition requires detailed account of the coupling energy with appropriate re-definition and optimization of the limiting phase trajectory on the resonant manifold.
description: 19 pages, 9 figures
Semileptonic Meson Decays in the Quark Model: An Update
Creators: name: Scora, Daryl
name: Isgur, Nathan
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present the predictions of ISGW2, an update of the ISGW quark model for semileptonic meson decays. The updated model incorporates a number of features which should make it more reliable, including the constraints imposed by Heavy Quark Symmetry, hyperfine distortions of wavefunctions, and form factors with more realistic high recoil behaviors.
description: All text and tables contained in the ".latex" file and all figures (14) contained in the ".uu" file.
Magnetic field breakout from white dwarf crystallization dynamos
Creators: name: Blatman, Daniel
name: Ginzburg, Sivan
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: A convective dynamo operating during the crystallization of white dwarfs is one of the promising channels to produce their observed strong magnetic fields. Although the magnitude of the fields generated by crystallization dynamos is uncertain, their timing may serve as an orthogonal test of this channel's contribution. The carbon-oxygen cores of $M\approx 0.5-1.0\,{\rm M}_\odot$ white dwarfs begin to crystallize at an age $t_{\rm cryst}\propto M^{-5/3}$, but the magnetic field is initially trapped in the convection zone - deep inside the CO core. Only once a mass of $m_{\rm cryst}$ has crystallized, the convection zone approaches the white dwarf's helium layer, such that the magnetic diffusion time through the envelope shortens sufficiently for the field to break out to the surface, where it can be observed. This breakout time is longer than $t_{\rm cryst}$ by a few Gyr, scaling as $t_{\rm break}\propto t_{\rm cryst}f^{-1/2}$, where $f\equiv 1-m_{\rm cryst}/M$ depends on the white dwarf's initial C/O profile before crystallization. The first appearance of strong magnetic fields $B\gtrsim 1\textrm{ MG}$ in volume-limited samples approximately coincides with our numerically computed $t_{\rm break}(M)$ - potentially signalling crystallization dynamos as a dominant magnetization channel. However, some observed magnetic white dwarfs are slightly younger, challenging this scenario. The dependence of the breakout process on the white dwarf's C/O profile implies that magnetism may probe the CO phase diagram, as well as uncertainties during the core helium burning phase in the white dwarf's progenitor, such as the $^{12}{\rm C}(α,γ)^{16}{\rm O}$ nuclear reaction.
description: Matches published version
Evaluating Ecological Suitability and Carrying Capacity for Budo's Mangrove Ecosystem: Unveiling Ecotourism Potential and Limits
Creators: name: Oroh, Dannie R. S.
name: Kontu, Tommy M.
name: Lintong, Oktavianus
Publisher: name: Zenodo
Year: 2024

description: Budo Village in North Sulawesi stands out as one of the top 50 recipients of the prestigious 2022Indonesian Tourism Village Award. Notably, Budo is a popular tourist destination with a thrivingmangrove area on Minahasa's northern peninsula. The Budo mangrove area has been designated as atourist attraction since 1994 and garnered increased recognition in 2017, thanks to active promotionalefforts aimed at coastal tourist destinations. Surprisingly, despite its transformation into a touristdestination, research has yet to be undertaken to assess the ecological suitability of mangroves in thiscontext or determine the carrying capacity of the mangrove area. This study seeks to delve into theecological suitability of Budo's mangrove ecological resources and investigate the carrying capacity of thearea as a tourist destination. The results of this analysis categorize the Budo mangrove tourist destinationas 'unsuitable,' as indicated by an IKW score of 1.5. Consequently, a comprehensive restoration approachis required to render this mangrove area suitable and viable for tourism. Mangrove restoration initiatives,coupled with more stringent adherence to ecotourism principles in the Budo mangrove area, along withconsiderations for its carrying capacity, could serve as vital steps towards achieving this objective.
Photoevaporation of protoplanetary discs with PLUTO+PRIZMO I. Lower X-ray-driven mass-loss rates due to enhanced cooling
Creators: name: Sellek, Andrew D.
name: Grassi, Tommaso
name: Picogna, Giovanni
name: Rab, Christian
name: Clarke, Cathie J.
name: Ercolano, Barbara
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Context: Photoevaporation is an important process for protoplanetary disc dispersal but there has so far been a lack of consensus from simulations over the mass-loss rates and the most important part of the high-energy spectrum for driving the wind. Aims: We aim to isolate the origins of these discrepancies through carefully-benchmarked hydrodynamic simulations of X-ray photoevaporation with time-dependent thermochemistry calculated on the fly. Methods: We conduct hydrodynamic simulations with pluto where the thermochemistry is calculated using prizmo. We explore the contribution of certain key microphysical processes and the impact of using different spectra used previously in literature studies. Results: We find that additional cooling results from the excitation of O by neutral H, which leads to dramatically reduced mass-loss across the disc compared to previous X-ray photoevaporation models, with an integrated rate of 10^-9 Msun/yr. Such rates would allow for longer-lived discs than previously expected from population synthesis. An alternative spectrum with less soft X-ray produces mass-loss rates around a factor of 2-3 times lower. The chemistry is significantly out of equilibrium, with the survival of H2 into the wind aided by advection. This leads to its role as the dominant coolant at 10s au - thus stabilising a larger radial temperature gradient across the wind - as well as providing a possible wind tracer.
description: 26 pages, 16 figures, Accepted 31st July 2024 for publication in A&A
Trivero, la Panoramica Zegna. Una visione calvinistica del piacere
Creators: name: Zilio, Luca
Publisher: name: Firenze Architettura
Year: 2019

description: This brief essay attempts, through the figure of Ermenegildo Zegna, the industrialist who in 1910 founded a textile industry with the aim of excelling with English-quality textiles, to analyse the role played by the landscape, during the second after-war period, in the definition of a new type of entrepreneurship and in the design of work-spaces, trying to show how the attention and care for the territory can become the basis for the management and culture of an Italian fashion company.
description: Firenze Architettura, Vol 23 No 1 (2019)
Retrofuturismo?
Creators: name: Rossi Prodi, Fabrizio
Publisher: name: Firenze Architettura
Year: 2019

description: With curiosity due to its karstic reemergence, and some perplexity, this article explores Retrofuturism, an art movement – not mainly architectural – that investigates the influence of future representations produced in past eras, expressing a nostalgia for the memory of those anticipations, balanced between past and future, alienation and the promises of redemption offered by new technologies.
description: Firenze Architettura, Vol 23 No 1 (2019)
Dalla cattedrale al pop-up. Prospettive di tutela e salvaguardia del patrimonio delle sale cinematografiche
Creators: name: Caccia Gherardini, Susanna
Publisher: name: Firenze Architettura
Year: 2019

description: The heritage represented by movie theaters has been in gradual decline for some time now. The barbaric transformation undergone by many of these buildings over the years has caused, often fortuitously, the definitive loss of many of the most significant examples of this cultural patrimony. Only an informed awareness can and should guide the mindful restoration choices for preventing additional alterations and pillage.
description: Firenze Architettura, Vol 23 No 1 (2019)
The Infrared Surface Brightness technique applied to RR Lyrae stars from the solar neighborhood
Creators: name: Zgirski, Bartłomiej
name: Gieren, Wolfgang
name: Pietrzyński, Grzegorz
name: Górski, Marek
name: Wielgórski, Piotr
name: Storm, Jesper
name: Bras, Garance
name: Kervella, Pierre
name: Nardetto, Nicolas
name: Hajdu, Gergely
name: Chini, Rolf
name: Haas, Martin
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The Baade-Wesselink method allows us to estimate distances to individual pulsating stars. Accurate geometric parallaxes obtained by the Gaia mission serve us in the calibration of the method and in the determination of its precision. The method also provides a way of determining mean radii of pulsating stars. The main aim of this work is to determine the scatter and possible dependence of p- factors of RR Lyrae stars on their pulsation periods. The secondary objective is to determine mean radius - period relations for these stars. Our calibrations for RR Lyrae stars are based on photometric data gathered at the Cerro Murphy Observatory. We obtained spectroscopic data specifically for this project using high resolution spectrographs. We use the Infrared Surface Brightness (IRSB) version of the method that relies on a surface brightness - color relation dependent on the (V-K) color. We obtain the spread of p- factors of around 0.07-0.08 for our sample of 9 RR Lyrae stars from the solar neighborhood. However, we also find relations between the p-factor and the pulsation period for RRab stars with the rms scatter around the relation of around 0.05, but with relatively large uncertainty of relations' parameters. We present relations between the mean radius and period for RR Lyrae pulsating in the fundamental mode with the rms scatter around the relation of $0.012R_{\odot}$. We observe a clear offset between p- factors obtained using the IRSB technique (with mean p between 1.39 and 1.45) and values inferred by Bras et al. (2024) using the SPIPS tool (Mérand et al. 2015). On the other hand, we obtain a similar scatter of p of as observed by Bras et al. (2024). Our period-radius relations are in a good agreement with both the inference of Bras et al. (2024) based on SPIPS and theoretical predictions of Marconi et al. (2005, 2015)
description: accepted for publication in A&A
A Brief Introduction to Chiral Perturbation Theory
Creators: name: Holstein, Barry R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A brief introduction to the subject of chiral perturbation theory ($χ$pt) is presented, including a discussion of effective field theory and applications of $χ$pt in the arena of purely mesonic interactions as well as in the $πN$ sector.
description: 15 pages, talk given at TAPS detector workshop, Rez, Czech Republic, Sept. 1999, to be published in Czech. J. Phys
Nanoscale Quantum Calorimetry with Electronic Temperature Fluctuations
Creators: name: Brange, F.
name: Samuelsson, P.
name: Karimi, B.
name: Pekola, J. P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Motivated by the recent development of fast and ultra-sensitive thermometry in nanoscale systems, we investigate quantum calorimetric detection of individual heat pulses in the sub-meV energy range. We propose a hybrid superconducting injector-calorimeter set-up, with the energy of injected pulses carried by tunneling electrons. Treating all heat transfer events microscopically, we analyse the statistics of the calorimeter temperature fluctuations and derive conditions for an accurate measurement of the heat pulse energies. Our results pave the way for novel, fundamental quantum thermodynamics experiments, including calorimetric detection of single microwave photons.
description: 6 pages, 3 figures plus supplemental material, 8 pages, 1 figure
COSMOS Brightest Group Galaxies -- III: Evolution of stellar ages
Creators: name: Gozaliasl, G.
name: Finoguenov, A.
name: Babul, A.
name: Ilbert, O.
name: Sargent, M.
name: Vardoulaki, E.
name: Faisst, A. L.
name: Liu, Z.
name: Shuntov, M.
name: Cooper, O.
name: Dolag, K.
name: Toft, S.
name: Magdis, G. E.
name: Toni, G.
name: Mobasher, B.
name: Barré, R.
name: Cui, W.
name: Rennehan, D.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The unique characteristics of the brightest group galaxies (BGGs) link the evolutionary continuum between galaxies like the Milky Way and more massive BCGs in dense clusters. This study investigates the stellar properties of BGGs over cosmic time (z = 0.08-1.30), extending our previous work (Gozaliasl et al. 2016, 2018; Paper I and Paper II). We analyze data of 246 BGGs from our X-ray galaxy group catalog in the COSMOS field, examining stellar age, mass, star formation rate (SFR), specific SFR (sSFR), and halo mass. Comparisons are made with Millennium and Magneticum simulations. We explore the variation of stellar properties with the projected offset from the X-ray peak or host halo center. Using a mock galaxy catalog, we evaluated the accuracy of SED-derived stellar ages, finding a mean absolute error of about one Gyr. Observed BGG age distributions show a bias towards younger ages compared to semi-analytical models and the Magneticum simulation. Our analysis of stellar age versus mass reveals trends with a positive slope, suggesting complex evolutionary pathways across redshifts. We observe a negative correlation between stellar age and SFR across all redshift ranges. Using a cosmic-time-dependent main sequence framework, we identify star-forming BGGs, finding that about 20% of BGGs in the local universe exhibit star-forming characteristics, increasing to 50% at $z=1.0$. Our findings support an inside-out formation scenario for BGGs, where older stellar populations are near the X-ray peak and younger populations at larger offsets indicate ongoing star formation. The distribution of stellar ages for lower-mass BGGs ($10^{10-11} M_\odot$) deviates from constant ages predicted by models, highlighting current models' limitations in capturing galaxies' complex star formation histories.
description: 24 Pages, 45 figures
Vec2SPARQL: integrating SPARQL queries and knowledge graph embeddings
Creators: name: Kulmanov, Maxat
name: Şenay Kafkas
name: Karwath, Andreas
name: Malic, Alexander
name: Gkoutos, Georgios V
name: Dumontier, Michel
name: Hoehndorf, Robert
Publisher: name: Semantic Web Applications and Tools for Healthcare and Life Sciences
Year: 2018
Subjects: subject: 80301 Bioinformatics Software
subject: FOS: Computer and information sciences

description: Recent developments in machine learning have led to a rise of largenumber of methods for extracting features from structured data. The featuresare represented as vectors and may encode for some semantic aspects of data.They can be used in a machine learning models for different tasks or to com-pute similarities between the entities of the data. SPARQL is a query languagefor structured data originally developed for querying Resource Description Frame-work (RDF) data. It has been in use for over a decade as a standardized NoSQLquery language. Many different tools have been developed to enable data shar-ing with SPARQL. For example, SPARQL endpoints make your data interopera-ble and available to the world. SPARQL queries can be executed across multi-ple endpoints. We have developed a Vec2SPARQL, which is a general frame-work for integrating structured data and their vector space representations.Vec2SPARQL allows jointly querying vector functions such as computing sim-ilarities (cosine, correlations) or classifications with machine learning modelswithin a single SPARQL query. We demonstrate applications of our approachfor biomedical and clinical use cases. Our source code is freely available athttps://github.com/bio-ontology-research-group/vec2sparql and we make aVec2SPARQL endpoint available at http://sparql.bio2vec.net/
Cherenkov radio pulses from EeV neutrino interactions: the LPM effect
Creators: name: Alvarez-Muñiz, J.
name: Zas, E.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the implications of the LPM effect for the Cherenkov radiation of EeV electromagnetic showers in the coherent radiowave regime for ice. We show that for showers above 100~PeV the electric field scales with shower energy but has a markedly narrower angular distribution than for lower energy showers. We give an electric field frequency and angular spectrum parameterization valid for showers having energy up to the EeV regime and discuss the implications for neutrino detectors based on arrays of radio antennas. Implications of the LPM effect for under water neutrino detectors in project are also briefly addressed.
description: 15 pages, 2 tables, 3 postscript figures