cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Search for the Hypothetical pi -> mu x Decay
Creators: name: Bilger, R.
name: Clement, H.
name: Denig, A.
name: Fohl, K.
name: Hautle, P.
name: Kluge, W.
name: Konter, J. A.
name: Kurz, G.
name: Mango, S.
name: Schapler, D.
name: Schonleber, F.
name: Siodlaczek, U.
name: Brandt, B. van den
name: Wagner, G. J.
name: Wieser, R.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The KARMEN collaboration has reported the possible observation of a hitherto unknown neutral and weakly interacting particle x, which is produced in the decay pi -> mu + x with a mass m(x) = 33.9 MeV. We have searched for this hypothetical decay branch by studying muons from pion decay in flight with the LEPS spectrometer at the piE3 channel at PSI and find branching ratios BR(pi- to mu- anti-x) < 4e-7 and BR(pi+ to mu+ x) < 7e-8 (95\% C.L.). Together with the limit BR > 2e-8 derived in a recent theoretical paper our result would leave only a narrow region for the existence of x if it is a heavy neutrino.
description: 10 pages, TeX (uses epsf), 3 Postscript figures uu-encoded
Radio, Hard X-Ray, and Gamma-Ray Emissions Associated with a Far-Side Solar Event
Creators: name: Grechnev, V. V.
name: Kiselev, V. I.
name: Kashapova, L. K.
name: Kochanov, A. A.
name: Zimovets, I. V.
name: Uralov, A. M.
name: Nizamov, B. A.
name: Grigorieva, I. Yu.
name: Golovin, D. V.
name: Litvak, M. L.
name: Mitrofanov, I. G.
name: Sanin, A. B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The SOL2014-09-01 far-side solar eruptive event produced hard electromagnetic and radio emissions observed with detectors at near-Earth vantage points. Especially challenging was a long-duration >100 MeV $γ$-ray burst probably produced by accelerated protons exceeding 300 MeV. This observation raised a question of how high-energy protons could reach the Earth-facing solar surface. Some preceding studies discussed a scenario in which protons accelerated by a CME-driven shock high in the corona return to the solar surface. We continue with the analysis of this challenging event, involving radio images from the Nançay Radioheliograph and hard X-ray data from the High Energy Neutron Detector (HEND) of the Gamma-Ray Spectrometer onboard the Mars Odyssey space observatory located near Mars. HEND recorded unocculted flare emission. The results indicate that the emissions observed from the Earth's direction were generated by flare-accelerated electrons and protons trapped in static long coronal loops. Their reacceleration is possible in these loops by a shock wave, which was excited by the eruption, being initially not CME-driven. The results highlight the ways to address remaining questions.
description: 36 pages, 11 figures. For associated movie file, see http://ssrt.iszf.irk.ru/~grechnev/papers/2014-09-01/ Accepted for publication in Solar Physics
YUFERING Report on Trainings
Creators: name: Lorenzo Costumato
name: Fabiana Scalabrini
name: Chiara Fantauzzi
Publisher: name: Zenodo
Year: 2024

description: This deliverable aims to report on the training delivered in the context of the YUFERING project. Providing high-quality training was one of the main goals of the project. For this reason, this report is crucial to represent the expected value creation of the consortium’s activities. Indeed, the report published by the European Commission in April 2023 includes insights from the YUFERING project, and describes the following YUFERING experiences as best practices to be mentioned. In detail: • Engaging Non-Academic Actors, 5.2. Good practices, page 29 (Flipped Knowledge Transfer (FKT)) • Mainstreaming Open Science, 6.2. Good practices, page 32 (Open Science Calendar 2022) • Citizen and Societal Engagement, 7.2. Good practices, page 36 (Community Engaged Research and Innovation (CERI) agenda setting)

As highlighted in the following sections, YUFERING training offer insights on several competences, such as those related to the Competence Framework, and topics, such as circular economy, arts and open science. To achieve a high-quality training offer that can generate a significant social impact throughout Europe, it becomes of primary importance to undertake a coherent path of identification, development and rewarding talents. The urgency of this offer is not limited to European borders but goes beyond them, becoming a global urgency.
Redundant Perception and State Estimation for Reliable Autonomous Racing
Creators: name: Gosala, Nikhil Bharadwaj
name: Bühler, Andreas
name: Prajapat, Manish
name: Ehmke, Claas
name: Gupta, Mehak
name: Sivanesan, Ramya
name: Gawel, Abel
name: Pfeiffer, Mark
name: Bürki, Mathias
name: Sa, Inkyu
name: Dubé, Renaud
name: Siegwart, Roland
Publisher: name: arXiv
Year: 2018
Subjects: subject: Robotics (cs.RO)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: In autonomous racing, vehicles operate close to the limits of handling and a sensor failure can have critical consequences. To limit the impact of such failures, this paper presents the redundant perception and state estimation approaches developed for an autonomous race car. Redundancy in perception is achieved by estimating the color and position of the track delimiting objects using two sensor modalities independently. Specifically, learning-based approaches are used to generate color and pose estimates, from LiDAR and camera data respectively. The redundant perception inputs are fused by a particle filter based SLAM algorithm that operates in real-time. Velocity is estimated using slip dynamics, with reliability being ensured through a probabilistic failure detection algorithm. The sub-modules are extensively evaluated in real-world racing conditions using the autonomous race car "gotthard driverless", achieving lateral accelerations up to 1.7G and a top speed of 90km/h.
description: 7 pages, 21 figures, submitted to the International Conference on Robotics and Automation 2019, for accompanying video visit https://www.youtube.com/watch?v=ir_uqEYuT84
Additional file 1: of Budgeting for a billion: applying health technology assessment (HTA) for universal health coverage in India
Creators: name: Saudamini Dabak
name: Songyot Pilasant
name: Mehndiratta, Abha
name: Downey, Laura
name: Francoise Cluzeau
name: Kalipso Chalkidou
name: Luz, Alia
name: Sitaporn Youngkong
name: Yot Teerawattananon
Publisher: name: figshare
Year: 2018
Subjects: subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Questionnaire. Survey on health technology assessment in India. (DOCX 31 kb)
A bound on superconducting $T_c$'s
Creators: name: Esterlis, I.
name: Kivelson, S. A.
name: Scalapino, D. J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: It is notoriously difficult to make quantitative theoretical predictions of the superconducting $T_c$, either from first-principles or even from a knowledge of normal state properties. Ultimately, this reflects the fact that the energy scales involved in the superconducting state are extremely small in natural units, and that $T_c$ depends exponentially on a subtle interplay between different interactions so that small uncertainties in microscopic processes can lead to order 1 effects on $T_c$. However, in some circumstances, it may be possible to determine (approximate) bounds on $T_c$. Here, we propose such a bound for the conventional phonon-mediated mechanism of pairing with strongly retarded interactions, i.e. in the case in which $\hbar\bar ω\ll E_F$ where $\bar ω$ is an appropriate characteristic phonon frequency and $E_F$ is the Fermi energy. Specifically, drawing on both empirical results (shown in Figure 2 below) and recent results[1] of determinant quantum Monte Carlo (DQMC) studies of the paradigmatic Holstein model, we propose that \begin{equation} k_B T_c \leq A_{max} \ \hbar \bar ω\end{equation} where $A_{max}$ is a dimensionless number of order one that we estimate to be \begin{equation} A_{max} \approx 1/10. \end{equation}
description: 7 pages, 2 figures
El uso de la web en la solución de problemas profesionales del estudiante universitario
Creators: name: Martínez Ibarra, Oriniel
name: López Fernández, José Manuel
Publisher: name: figshare
Year: 2021
Subjects: subject: 130202 Curriculum and Pedagogy Theory and Development
subject: FOS: Educational sciences

description: El presente trabajo ofrece una valoración teórico-práctica de la necesidad del estudio, elaboración y aplicación del uso de las Web con interés educativo. Se parte de sus antecedentes enfatizando su problemática en el contexto de la Educación Superior. Se defiende la idea de que estos espacios Web pueden contribuir a la solución de diversos problemas profesionales a los que se enfrentan los estudiantes de carreras pedagógicas durante la práctica laboral investigativa.
WEBINAR: Getting started with command line bioinformatics
Creators: name: Brandies, Parice
Publisher: name: Zenodo
Year: 2021
Subjects: subject: Bioinformatics
subject: FOS: Computer and information sciences
subject: Command line
subject: Workflows
subject: Bash
subject: Computational biology
subject: http://edamontology.org/topic_0091
subject: http://edamontology.org/topic_0769

description: This record includes training materials associated with the Australian BioCommons webinar ‘Getting started with command line bioinformatics’. This webinar took place on 22 June 2021. Bioinformatics skills are in demand like never before and biologists are stepping up to the challenge of learning to analyse large and ever growing datasets. Learning how to use the command line can open up many options for data analysis but getting started can be a little daunting for those without a background in computer science. Parice Brandies and Carolyn Hogg have recently put together ten simple rules for getting started with command-line bioinformatics to help biologists begin their computational journeys. In this webinar Parice walks you through their hints and tips for getting started with the command line. She covers topics like learning tech speak, evaluating your data and workflows, assessing computational requirements, computing options, the basics of software installation, curating and testing scripts, a bit of bash and keeping good records. The webinar will be followed by a short Q&A session. The slides were created by Parice Brandies and are based on the publication ‘Ten simple rules for getting started with command-line bioinformatics’ (https://doi.org/10.1371/journal.pcbi.1008645). The slides are shared under a Creative Commons Attribution 4.0 International unless otherwise specified and were current at the time of the webinar. Files and materials included in this record: Event metadata (PDF): Information about the event including, description, event URL, learning objectives, prerequisites, technical requirements etc. Index of training materials (PDF): List and description of all materials associated with this event including the name, format, location and a brief description of each file. Getting started with command line bioinformatics - slides (PDF): Slides presented during the webinar Materials shared elsewhere: A recording of the webinar is available on the Australian BioCommons YouTube Channel https://youtu.be/p7pA4OLB2X4
description: {"references": ["Brandies PA, Hogg CJ (2021) Ten simple rules for getting started with command-line bioinformatics. PLoS Comput Biol 17(2): e1008645. https://doi.org/10.1371/journal.pcbi.1008645"]}
Tachyon-free Non-supersymmetric Type IIB Orientifolds via Brane-Antibrane Systems
Creators: name: Aldazabal, G.
name: Uranga, A. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We derive the rules to construct type IIB compact orientifolds in six and four dimensions including D-branes and anti-D-branes. Even though the models are non-supersymmetric due to the presence of the anti-D-branes, we show that it is easy to construct large classes of models free of tachyons. Brane-antibrane annihilation can be prevented for instance by considering models with branes and antibranes stuck at different fixed points in the compact space. We construct several anomaly-free and tachyon-free six-dimensional orientifolds containing D9-branes and anti-D5-branes. This setup allows to construct four-dimensional chiral models with supersymmetry unbroken in the bulk and in some D-brane sectors, whereas supersymmetry is broken (at the string scale) in some `hidden' anti-D-brane sector. We present several explicit models of this kind. We also comment on the role of the non-cancelled attractive brane-antibrane forces and the non-vanishing cosmological constant, as providing interesting dynamics for the geometric moduli and the dilaton, which may contribute to their stabilization.
description: 30 pages, Latex, no figures. Minor corrections
Modeling OWL with Rules: The ROWL Protege Plugin
Creators: name: Sarker, Md. Kamruzzaman
name: Carral, David
name: Krisnadhi, Adila A.
name: Hitzler, Pascal
Publisher: name: arXiv
Year: 2018
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: In our experience, some ontology users find it much easier to convey logical statements using rules rather than OWL (or description logic) axioms. Based on recent theoretical developments on transformations between rules and description logics, we develop ROWL, a Protege plugin that allows users to enter OWL axioms by way of rules; the plugin then automatically converts these rules into OWL DL axioms if possible, and prompts the user in case such a conversion is not possible without weakening the semantics of the rule.
description: Accepted at ISWC 2016
Polyrhachis (Myrma) laboriosa var. architecta Santschi, 1924, n. var.
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1924
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Polyrhachis
Polyrhachis laboriosa
Polyrhachis (myrma) laboriosa sm. var. architecta

description: 132. - Polyrhachis (Myrma) laboriosa Sm. var. architecta n. var.
[[worker]] Differe du type par ses epines de l'ecaille qui sont beaucoup plus ecartees, bien plus espacees au bout que longues. Le gastre est aussi plus volumineux, depourvu de poils dresses dessus et de cote, puis la pubescence en est plus courte et d'un gris jaunatre comme le thorax. Le mesotonum est distinctement plus long que chez le type et l'epinotum un peu plus large.
Congo belge: Kondue (Luja) 2 [[worker]] recues de Mr. Reichensperger.
description: Published as part of Santschi, F., 1924, Descriptions de nouveaux formicides africains et notes diverses. - II., pp. 195-224 in Revue de Zoologie Africaine 12 on page 224
An Imaging Polarimeter(IMPOL) for multi-wavelength observations
Creators: name: Ramaprakash, A. N.
name: Gupta, Ranjan
name: Sen, A. K.
name: Tandon, S. N.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Taking advantage of the advances in array detector technology, an imaging polarimeter (IMPOL) has been constructed for measuring linear polarization in the wavelength band from 400-800 nm. It makes use of a Wollaston prism as the analyser to measure simultaneously the two orthogonal polarization components that define a Stoke's parameter. An achromatic half-wave plate is used to rotate the plane of polarization with respect to the axis of the analyser so that the second Stoke's parameter also can be determined. With a field of view correponding to about 30x30 sq. mm for a 1.2 m, f/13 telescope, a sensitive, liquid-nitrogen cooled CCD camera as the detector and a built-in acquisition and guidance unit, the instrument can be used for studying stellar fields or extended objects with an angular resolution close to 2 arcsec. The instrumental polarization is less than 0.05% and the accuracies of measurement are primarily limited by photon noise for typical observations.
description: 10 pages including 5 embedded figures; submitted to Astronomy and Astrophysics Supplement Series; available on request to A. N. Ramaprakash (anr@iucaa.ernet.in or preprn@iucaa.ernet.in); quote report no
MOESM7 of Prevalence of autoimmune thyroid diseases among the Turner Syndrome patients: meta-analysis of cross sectional studies
Creators: name: Sagad Mohamed
name: Elkhidir, Ibrahim
name: Abdelhamid Abuzied
name: Noureddin, Ahmed
name: Gehad Ibrahim
name: Mahmoud, Ahmed
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 60506 Virology
subject: Computational Biology

description: Additional file 7: Fig S7 Pooled prevalence of ATDs among patients with monosomy 45, X karyotype of Turner Syndrome.
Report on the YUFE community-engagement based R&I pilot
Creators: name: Bruno Hoste
name: Anne Adams
Publisher: name: Zenodo
Year: 2024
Subjects: Community Engaged R&I

description: As part of the YUFE model towards a community engagement-based research & innovation agenda, an approach was developed to foster research collaboration between de YUFE partners, venturing towards defining strategic research strengths, and underneath the emergence of so-called research nodes.  This objective was tackled by two flight paths: 1. In order to identify potential future YUFE R&I nodes, an extensive analysis was carried out, focusing on acquired EU project funding by the YUFE universities and on their publication output. Potential research strengths (clusters) were identified, and strategic options mapped. This effort resulted in datasets that can be used for future strategic guidance and decision making on alliance level. In addition to this top-down analysis, a bottom-up initiative was supported and used as a testcase to develop a YUFE R&I node (YUFERING pilot BioYUFE on ‘Biodiversity’). This pilot focused on education, research collaboration and innovation and the continuum between these three aspects, which was considered to emphasize the strength of a community engaged (CERI) research & innovation node pilot. This pilot was then used to extract and test a methodology and to define lessons to inspire the development of future R&I nodes within the YUFE alliance. 2. A Horizon Europe (HE) Marie Sklodowska-Curie (MSCA) COFUND proposal was written and submitted with an explicit objective to foster research collaboration within the alliance, triggered by postdocs. Initiated and steered by the University of Antwerp, it was developed in collaboration with a dedicated Project Group of (R&I support staff) of the YUFE partners. At the heart of this project lies an overarching training programme focusing on stakeholder interaction and community engagement, fuelling a CERI approach across the partner universities. This project started on 1st of January 2023.
Vacuum structure of a modified MIT Bag
Creators: name: Hofmann, R.
name: Gutsche, T.
name: Schumann, M.
name: Viollier, R. D.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: An alternative to introducing and subsequently renormalizing classical parameters in the expression for the vacuum energy of the MIT bag for quarks is proposed in the massless case by appealing to the QCD trace anomaly and scale separation due to asymptotic freedom. The explicit inclusion of gluons implies an unrealistically low separation scale.
description: 5 pages, 2 figures
NGC 3105: a young open cluster with low metallicity
Creators: name: Alonso-Santiago, J.
name: Marco, A.
name: Negueruela, I.
name: Tabernero, H. M.
name: Castro, N.
name: McBride, V. A.
name: Rajoelimanana, A. F.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: NGC 3105 is a young open cluster hosting blue, yellow and red supergiants. This rare combination makes it an excellent laboratory to constrain evolutionary models of high-mass stars. It is poorly studied and fundamental parameters such as its age or distance are not well defined. We intend to characterize in an accurate way the cluster as well as its evolved stars, for which we derive for the first time atmospheric parameters and chemical abundances. We identify 126 B-type likely members within a radius of 2.7$\pm$0.6 arcmin, which implies an initial mass, $M_{cl}\approx$4100 M$_{\odot}$. We find a distance of 7.2$\pm$0.7 kpc for NGC 3105, placing it at $R_{GC}$=10.0$\pm$1.2 kpc. Isochrone fitting supports an age of 28$\pm$6 Ma, implying masses around 9.5 M$_{\odot}$ for the supergiants. A high fraction of Be stars ($\approx$25 %) is found at the top of the main sequence down to spectral type b3. From the spectral analysis we estimate for the cluster a $v_{rad}$=+46.9$\pm$0.9 km s$^{-1}$ and a low metallicity, [Fe/H]=-0.29$\pm$0.22. We also have determined, for the first time, chemical abundances for Li, O, Na, Mg, Si, Ca, Ti, Ni, Rb, Y, and Ba for the evolved stars. The chemical composition of the cluster is consistent with that of the Galactic thin disc. An overabundance of Ba is found, supporting the enhanced $s$-process. NGC 3105 has a low metallicity for its Galactocentric distance, comparable to typical LMC stars. It is a valuable spiral tracer in a very distant region of the Carina-Sagittarius spiral arm, a poorly known part of the Galaxy. As one of the few Galactic clusters containing blue, yellow and red supergiants, it is massive enough to serve as a testbed for theoretical evolutionary models close to the boundary between intermediate and high-mass stars.
description: 18 pages, 13 figures. Accepted for publication in A&A
Report on Collaboration with other consortia of European Universities
Creators: name: Andreas Bressler
Publisher: name: Zenodo
Year: 2024

description: The purpose of this document is to report on the task for exploitation of project results through exchange of best practices with other funded European University consortia. The focus of this document is to report on the outcomes for the different subtasks. This task is a deliverable of YUFERING WP6 ‘dissemination, exploitation, communication’. The main objective of this task was to deepen the connections and collaboration with other funded European University consortia.
Anoplolepis
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1926
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Anoplolepis
Formica
Formica longipes

description: 1. Subgenus Anoplolepis Santschi sensu str.
[[worker]]. Monomorphes; assez grandes. Les 4 premiers articles du funicule subegaux, le 3 e plutot plus long que le premier. Ocelles absents.
[[male]]. Beaucoup plus petits que les [[queen]].
Type: Formica longipes Jerdon, 1851.
Autres especes: Plagiolepis carinata Emery, 1899. P. braunsi Forel 1913.
description: Published as part of Santschi, F., 1926, Trois notes myrmécologiques., pp. 13-28 in Annales de la Société Entomologique de France 95 on page 13
Strategy for a European Career Track System
Creators: name: Ilaria Boncori
name: Jenny Wilders
name: Charlotte Simmat
Publisher: name: Zenodo
Year: 2024

description: The Young Universities for the Future of Europe (YUFE) share the vision of a European Research Area with free circulation of researchers, scientific knowledge, and technology. Work is being completed within YUFE to develop common tools to enable professional development exchanges and upward career paths such as joint YUFE Career Tracks. However, our academic YUFE partners all have different national systems featuring different national regulations towards research, careers, mobility, selection procedures for entry and advance in positions, and assessment criteria. To make the YUFE career paths aligned and to foster mobility, we needed a better understanding of the YUFE partners’ national career systems and the national and local research training and research funding landscape. Therefore, we aim to explore academic career systems in more detail to identify challenges and potential solutions to enhance researcher mobility and a YUFE Career Track. The work is structured in sub-tasks as follows: 1. Mapping of academic career paths in the eight YUFE universities (entry and exit points); hiring practices and official requirements of skills and qualifications; evidencing research development and teaching skills; as well as the range of selection criteria for academic positions and tenure in YUFE partner countries. 2. Mapping of all researcher competency frameworks already in place at our ten YUFE universities. 3. Establish recommendations at European, national, and institutional level to overcome the obstacles for talent circulation. 4. Advice to develop a Strategy for a European Career Track System, making references to the ERA Policy developments.
Small-scale magnetic flux emergence in the quiet Sun
Creators: name: Moreno-Insertis, F.
name: Martinez-Sykora, J.
name: Hansteen, V. H.
name: Muñoz, D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Small bipolar magnetic features are observed to appear in the interior of individual granules in the quiet Sun, signaling the emergence of tiny magnetic loops from the solar interior. We study the origin of those features as part of the magnetoconvection process in the top layers of the convection zone. Two quiet-Sun magnetoconvection models, calculated with the radiation-magnetohydrodynamic (MHD) Bifrost code and with domain stretching from the top layers of the convection zone to the corona, are analyzed. Using 3D visualization as well as a posteriori spectral synthesis of Stokes parameters, we detect the repeated emergence of small magnetic elements in the interior of granules, as in the observations. Additionally, we identify the formation of organized horizontal magnetic sheets covering whole granules. Our approach is twofold, calculating statistical properties of the system, like joint probability density functions (JPDFs), and pursuing individual events via visualization tools. We conclude that the small magnetic loops surfacing within individual granules in the observations may originate from sites at or near the downflows in the granular and mesogranular levels, probably in the first 1 or 1.5 Mm below the surface. We also document the creation of granule-covering magnetic sheet-like structures through the sideways expansion of a small subphotospheric magnetic concentration picked up, and pulled out of the interior, by a nascent granule. The sheet-like structures we found in the models may match the recent observations of Centeno et al. (2017).
description: 9 pages, 5 figures, Published in The Astrophysical Journal Letters
The Status of Supersymmetry
Creators: name: Bagger, Jonathan A.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Supersymmetry searches are about to enter an important new era. With LEP 200 and the Main Injector, they will, for the first time, begin to probe significant regions of the supersymmetric parameter space. There is a real chance that supersymmetry might indeed be found before the advent of the LHC.
description: Invited talk given at PbarP95, May 9-13, 1995, Fermilab. This summary is intended for experimentalists
OWLAx: A Protege Plugin to Support Ontology Axiomatization through Diagramming
Creators: name: Sarker, Md. Kamruzzaman
name: Krisnadhi, Adila A.
name: Hitzler, Pascal
Publisher: name: arXiv
Year: 2018
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Databases (cs.DB)
subject: FOS: Computer and information sciences

description: Once the conceptual overview, in terms of a somewhat informal class diagram, has been designed in the course of engineering an ontology, the process of adding many of the appropriate logical axioms is mostly a routine task. We provide a Protege plugin which supports this task, together with a visual user interface, based on established methods for ontology design pattern modeling.
description: Poster in ISWC 2016
Anoplolepis (Mesanoplolepis) Santschi, 1926, n. subg.
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1926
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Anoplolepis
Plagiolepis
Plagiolepis simulans

description: 3. Subgenus Mesanoplolepis, n. subg.
[[worker]]. Monomorphes, taille mediocre. Yeux en arriere du milieu des cotes de la tete. Ecaille plus ou moins inclinee en avant. Ensemble des articles 2 et 3 du funicule pas beaucoup plus long que le premier. [[male]] de meme taille que la [[worker]], [[queen]] beaucoup plus grande. Ocelles distincts.
Type: Plagiolepis simulans Santschi, 1908.
Autres especes: P. (A.) deceptor Arnold, 1922 P. decolor Em. 1910, melanaria Arnold.
description: Published as part of Santschi, F., 1926, Trois notes myrmécologiques., pp. 13-28 in Annales de la Société Entomologique de France 95 on page 14
Solutions of the Modified Chiral Model in (2+1) Dimensions
Creators: name: Ioannidou, Theodora
name: Zakrzewski, Wojtek
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: This paper deals with classical solutions of the modified chiral model on $R^{2+1}$. Such solutions are shown to correspond to products of various factor which we call time-dependent unitons. Then the problem of solving the system of second-order partial differential equations for the chiral field is reduced to solving a sequence of systems of first-order partial differential equations for the unitons.
description: 11 pages + 3 figures, Latex, to appear in Journal of Mathematical Physics
MOESM6 of Prevalence of autoimmune thyroid diseases among the Turner Syndrome patients: meta-analysis of cross sectional studies
Creators: name: Sagad Mohamed
name: Elkhidir, Ibrahim
name: Abdelhamid Abuzied
name: Noureddin, Ahmed
name: Gehad Ibrahim
name: Mahmoud, Ahmed
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy
subject: 60506 Virology
subject: Computational Biology

description: Additional file 6: Fig S6. Pooled prevalence of ATDs among patients with Iso-Xq karyotype of Turner Syndrome.
Coherence of the Borromean three-body Förster resonances in Rydberg atoms
Creators: name: Ryabtsev, I. I.
name: Beterov, I. I.
name: Tretyakov, D. B.
name: Yakshina, E. A.
name: Entin, V. M.
name: Cheinet, P.
name: Pillet, P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We have observed recently the Stark-tuned three-body Förster resonances ${\rm 3}\times nP_{3/2} (|M|)\to nS_{1/2} +(n+1)S_{1/2} +nP_{3/2} (|M^{*} |)$ at long-range interactions of a few cold Rb Rydberg atoms [D.B.Tretyakov et al., Phys. Rev. Lett. 119, 173402 (2017)]. The three-body resonance appears at a different dc electric field with respect to the ordinary two-body resonance ${\rm 2}\times nP_{3/2} (|M|)\to nS_{1/2} +(n+1)S_{1/2} $ and corresponds to a transition when the three interacting atoms change their states simultaneously (two atoms go to the $S$ states, and the third atom remains in the $P$ state but changes its moment projection), with the negligible contribution of the two-body resonance to the population transfer. It thus has a Borromean character and represents an effective three-body operator, which can be used to directly control the three-body interactions in quantum simulations and quantum gates implemented with Rydberg atoms. In this paper we theoretically investigate the coherence of such three-body resonances and we show that high-contrast Rabi-like population oscillations are possible for the localized Rydberg atoms in a certain spatial configuration. This paves the way to implementing three-qubit quantum gates and quantum simulations based on three-body Rydberg interactions.
description: 14 pages, 5 figures. arXiv admin note: substantial text overlap with arXiv:1707.01636
Report on legal, regulatory and financial barriers and recommendations
Creators: name: Martin Unfried
Publisher: name: Zenodo
Year: 2024

description: Most of the partner universities admit that a broader analysis of legal, regulatory barriers to research collaboration within and outside the YUFE network cannot be complete. One reason is that some of them do not have one single practice but very diverse practices in accordance with the different faculties and research groups. Hence, it was difficult to find experts within the partner universities who have an overview and the full picture of the different conditions of research collaboration and contractual instruments. This means that it is not easy to analyse a ‘common’ practice even within one university. So far, the view on research collaboration of YUFE partners is not different from the exchange with other universities. Basic questions are whether a researcher comes from an EU or third country and what type of contract or hosting schemes is applied, not whether a researcher is employed by a YUFE partner. The findings of this study indicate that YUFE should aim at developing specific arrangements for the exchange of staff amongst YUFE partners in the field of research collaboration. Based on the findings, recommendations are made for a “privileged framework for the exchange of staff”. That could for instance mean to develop an innovative instrument that would broaden the scope of internal vacancies to the YUFE partner university for certain research projects (beyond todays YUFE staff programme). One could define what projects fall under YUFE research collaboration with a privileged access for researchers employed by a YUFE university leading the way to internal vacancies of YUFE as a European University. A privileged framework could also include a tailor- made YUFE “secondment tool”. YUFE could agree on framework conditions for the secondment of YUFE research personnel to other YUFE universities. Such a “privileged” framework has to take into account the legal problems of YUFE partners due to restrictive national legislation. The question of special arrangements or a “privileged framework” is not that obvious in the case of financial and ethical aspects of research collaboration that were also part of the study. The partner universities today have a certain routine how to deal with intellectual property rights questions in transnational research projects, data protection or the assessment of ethical questions. In the case of data protection and ethical standards, it is obvious that compliance with European legislation and joint European Ethical Codes are providing a rather strong common framework where specific YUFE agreements are possible but less urgent.
Status of Neutrino Astronomy: The Quest for Kilometer-Scale Instruments
Creators: name: Halzen, F.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This is a (very) personal attempt to summarize the status of neutrino astronomy: its scientific motivations, our understanding of natural water and ice as particle detectors and, finally, the detector technology.
description: Latex 2.09 using epsf.sty, 13 pages, 5 postscript figures. Postscript version of complete paper available soon at http://phenom.physics.wisc.edu/pub/preprints/1996/madph-96-981.ps.Z or at ftp://phenom.physics.wisc.edu/pub/preprints/1996/madph-96-981.ps.Z
MOESM5 of Prevalence of autoimmune thyroid diseases among the Turner Syndrome patients: meta-analysis of cross sectional studies
Creators: name: Sagad Mohamed
name: Elkhidir, Ibrahim
name: Abdelhamid Abuzied
name: Noureddin, Ahmed
name: Gehad Ibrahim
name: Mahmoud, Ahmed
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 60506 Virology
subject: Computational Biology

description: Additional file 5: Fig S5. Pooled prevalence of hyperthyroidism among patients with Turner Syndrome diagnosed with ATDs.
Plagiolepis
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1926
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Plagiolepis

description: Genre Plagiolepis Mayr.
Ce genre reste ainsi limite a de petites especes comme chez Brachymyrmex et ne depassant que rarement 2 mm. chez la [[worker]]. Le mesonotum est ici-tres apparent. Ocelles absents ou peu developpes. [[worker]] isomorphes ou presque.
description: Published as part of Santschi, F., 1926, Trois notes myrmécologiques., pp. 13-28 in Annales de la Société Entomologique de France 95 on page 14
Deep HST/FOC Imaging of the Central Density Cusp of the Globular Cluster M15
Creators: name: Sosin, Craig
name: King, Ivan R.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the Faint Object Camera on the repaired Hubble Space Telescope, we have observed two fields in the globular cluster M15: the central density cusp, and a field at r = 20''. These are the highest-resolution images ever taken of this cluster's dense core, and are the first to probe the distribution of stars well below the main-sequence turnoff. After correction for incompleteness, we measure a logarithmic cusp slope (d log σ/ d log r) of -0.70 +- 0.05 (1-sigma) for turnoff (~ 0.8 \Msun) stars over the radial range from 0.3'' to 10''; this slope is consistent with previous measurements. We also set an approximate upper limit of ~1.5'' (90% confidence limit) on the size of any possible constant-surface-density core, but discuss uncertainties in this limit that arise from crowding corrections. We find that fainter stars in the cusp also have power-law density profiles: a mass group near 0.7 \Msun has a logarithmic slope of -0.56 +- 0.05 (1-sigma) over the radial range from 2'' to 10''. Taken together, the two slopes are not well matched by the simplest core-collapse or black-hole models. We also measure a mass function at r = 20'', outside of the central cusp. Both of the FOC fields show substantial mass segregation, when compared with a mass function measured with the WFPC2 at r = 5'. In comparing the overall mass functions of the two FOC fields and the r = 5' field, we find that the radial variation of the mass function is somewhat less than that predicted by a King-Michie model of the cluster, but greater than that predicted by a Fokker-Planck model taken from the literature.
description: 40 pages single-spaced, including 12 figures; to appear in AJ, April 1997
Reanalysis of the EMC charm production data with extrinsic and intrinsic charm at NLO
Creators: name: Harris, B. W.
name: Smith, J.
name: Vogt, R.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A calculation of the next-to-leading order exclusive extrinsic charm quark differential distributions in deeply inelastic electroproduction has recently been completed. Using these results we compare the NLO extrinsic contributions to the charm structure function $F_2(x,Q^2,m_c^2)$ with the corresponding NLO intrinsic contributions. The results of this analysis are compared with the EMC DIS charm quark data and evidence for an intrinsic charm component in the proton is found.
description: Latex with 7 figures in seperate file. Revised version to appear in Nuclear Physics B. Conclusions unchanged
The Galactic Census of High- and Medium-mass Protostars. IV. Molecular Clump Radiative Transfer, Mass Distributions, Kinematics, and Dynamical Evolution
Creators: name: Barnes, Peter J.
name: Hernandez, Audra K.
name: Muller, Erik
name: Pitts, Rebecca L.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present $^{12}$CO, $^{13}$CO, and C$^{18}$O data as the next major release for the CHaMP project, an unbiased sample of Galactic molecular clouds in $l$ = 280$^{\circ}$-300$^{\circ}$. From a radiative transfer analysis, we self-consistently compute 3D cubes of optical depth, excitation temperature, and column density for $\sim$300 massive clumps, and update the $I_{\rm CO}$-dependent CO$\rightarrow$H$_2$ conversion law of Barnes et al (2015). For $N$ $\propto$ $I^p$, we find $p$ = 1.92$\pm$0.05 for the velocity-resolved conversion law aggregated over all clumps. A practical, integrated conversion law is $N_{\rm CO}$ = (4.0$\pm$0.3)$\times$10$^{19}$m$^{-2}$ $I_{\rm CO}^{1.27\pm0.02}$, confirming an overall 2$\times$ higher total molecular mass for Milky Way clouds, compared to the standard $X$ factor. We use these laws to compare the kinematics of clump interiors with their foreground $^{12}$CO envelopes, and find evidence that most clumps are not dynamically uniform: irregular portions seem to be either slowly accreting onto the interiors, or dispersing from them. We compute the spatially-resolved mass accretion/dispersal rate across all clumps, and map the local flow timescale. While these flows are not clearly correlated with clump structures, the inferred accretion rate is a statistically strong function of the local mass surface density $Σ$, suggesting near-exponential growth or loss of mass over effective timescales $\sim$30-50 Myr. At high enough $Σ$, accretion dominates, suggesting gravity plays an important role in both processes. If confirmed by numerical simulations, this sedimentation picture would support arguments for long clump lifetimes mediated by pressure confinement, with a terminal crescendo of star formation, suggesting a resolution to the 40-yr-old puzzle of the dynamical state of molecular clouds and their low star formation efficiency.
description: Accepted to ApJ. Main paper is 19 pages, plus 4 Appendices which are available from the links on pg.20
title: 02_0816
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/
Report on the accreditation pilot based in Open Science criteria
Creators: name: Jouni Kekäle
name: Maria Pietilä
name: Katri Rintamäki
Publisher: name: Zenodo
Year: 2024

description: The work package four (WP4) of YUFERING (YUFE Transforming Research and In- novation through Europe-wide Knowledge Transfer) has focused on the transformation of recognition, reward and circulation of talents and teams across Europe. It has aimed at finding solutions for increasing research mobility, identifying the skills for a new gen- eration of researchers, and training researchers on these skills. Task 4.3, titled ‘Novel recognition and reward scheme for researchers’, has been dedicated to developing tools for piloting novel recognition and reward schemes for re- searchers, and to pilot these in the selection of researchers for YUFE postdocs. As outlined in the project proposal, these schemes aim to acknowledge researchers’ efforts and performance beyond traditional quantitative criteria and metrics. Up to date, research funding organizations have been active in piloting new assessment methods. There is a call also for universities to pilot such approaches. The EC’s Scoping report ‘Towards a Reform of the Research Assessment System’ (EC 2021, 8) identified European Universities Alliances as important testbeds for reforms and pilot projects. YUFE has taken an active role in creating and piloting new approaches.
Plagiolepis (Acantholepis)
Creators: name: Santschi, F.
Publisher: name: Zenodo
Year: 1926
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Plagiolepis

description: Genre Acantholepis Mayr.
Ce genre parait au premier abord tres facile a distinguer des Plagiolepis, par l'epinotum tres anguleux au-dessus des stomates et l'ecaille ordinairement bicuspide, mais les passages au sous-genre Anacantholepis sont frequents et alors la distinction ne repose plus que sur le developpement accentue des ocelles, la variabilite de la taille ou la forme plus anguleuse de l'epinotum.
description: Published as part of Santschi, F., 1926, Trois notes myrmécologiques., pp. 13-28 in Annales de la Société Entomologique de France 95 on page 15
Weakly coupled system of semilinear wave equations with distinct scale-invariant terms in the linear part
Creators: name: Chen, Wenhui
name: Palmieri, Alessandro
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35L52 (Primary), 35B33, 35B44 (Secondary)

description: In this work we determine the critical exponent for a weakly coupled system of semilinear wave equations with distinct scale-invariant lower order terms, when these terms make both equations in some sense parabolic-like. For the blow-up result the test functions method is applied, while for the global existence (in time) results we use L2-L2 estimates with additional L1 regularity.
description: 19 pages