cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 2 of Provider Bias in prescribing opioid analgesics: a study of electronic medical Records at a Hospital Emergency Department
Creators: name: Keister, Lisa A.
name: Stecher, Chad
name: Aronson, Brian
name: McConnell, William
name: Hustedt, Joshua
name: Moody, James W.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 2. Logistic regression results for non-opioid prescriptions.
Investigating Two Successive Flux Rope Eruptions In A Solar Active Region
Creators: name: Cheng, X.
name: Zhang, J.
name: Ding, M. D.
name: Olmedo, O.
name: Sun, X. D.
name: Guo, Y.
name: Liu, Y.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: We investigate two successive flux rope (FR1 and FR2) eruptions resulting in two coronal mass ejections (CMEs) on 2012 January 23. Both FRs appeared as an EUV channel structure in the images of high temperature passbands of the Atmospheric Imaging Assembly prior to the CME eruption. Through fitting their height evolution with a function consisting of linear and exponential components, we determine the onset time of the FR impulsive acceleration with high temporal accuracy for the first time. Using this onset time, we divide the evolution of the FRs in the low corona into two phases: a slow rise phase and an impulsive acceleration phase. In the slow rise phase of the FR1, the appearance of sporadic EUV and UV brightening and the strong shearing along the polarity inverse line indicates that the quasi-separatrix-layer reconnection likely initiates the slow rise. On the other hand for the FR2, we mainly contribute its slow rise to the FR1 eruption, which partially opened the overlying field and thus decreased the magnetic restriction. At the onset of the impulsive acceleration phase, the FR1 (FR2) reaches the critical height of 84.4$\pm$11.2 Mm (86.2$\pm$13.0 Mm) where the decline of the overlying field with height is fast enough to trigger the torus instability. After a very short interval ($\sim$2 minutes), the flare emission began to enhance. These results reveal the compound activity involving multiple magnetic FRs and further suggest that the ideal torus instability probably plays the essential role of initiating the impulsive acceleration of CMEs.
description: 9 pages, 5 figures, Accepted for publication in ApJ Letters, Comments are welcome
FSOLab Manual including compilation of tools
Creators: name: Marschalek, ilse
name: Schrammel, Maria
Publisher: name: Zenodo
Year: 2021
Subjects: FSOLab
Process manual
Social Lab

description: This deliverable at hand is a manual for the four FSOLab managers. It is specifically tailored to the FSOlabs implemented in the FoodSafety4EU project. It provides a summary on the concept of social labs, which the FSOLab approach builds on and outlines the concept for experiential learning and the FSOLab process (chapter 2).
Additional file 5 of Large scale genomic rearrangements in selected Arabidopsis thaliana T-DNA lines are caused by T-DNA insertion mutagenesis
Creators: name: Pucker, Boas
name: Kleinbölting, Nils
name: Weisshaar, Bernd
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 5. Read coverage of all analyzed lines in relation to the TAIR9 reference genome sequence.
Observation of resonance-assisted dynamical tunneling in an asymmetric microcavity
Creators: name: Kwak, Hojeong
name: Shin, Younghoon
name: Moon, Songky
name: An, Kyungwon
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We report the first experimental observation of the resonance-assisted dynamical tunneling (RADT) in the inter-mode interaction in an asymmetric-deformed microcavity. A selection rule for strong inter-mode coupling induced by RADT was observed on angular mode numbers as predicted by the RADT theory. In addition, the coupling strength was measured to be proportional to the square of the phase-space area associated with the nonlinear resonance involved in RADT. The proportionality constant was found to depend only on the nonlinear resonance, supporting the semiclassical nature of RADT.
description: 5 pages, 4 figures
Additional file 3 of Provider Bias in prescribing opioid analgesics: a study of electronic medical Records at a Hospital Emergency Department
Creators: name: Keister, Lisa A.
name: Stecher, Chad
name: Aronson, Brian
name: McConnell, William
name: Hustedt, Joshua
name: Moody, James W.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 3. Histogram for previous opioid prescriptions.
Spatial heterogeneity in the radiogenic activity of the lunar interior: Inferences from CHACE and LLRI on Chandrayaan-1
Creators: name: Sridharan, R.
name: Das, Tirtha Pratim
name: Ahmed, S. M.
name: Supriya, Gogulapati
name: Bhardwaj, Anil
name: Kamalakar, J. A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Space Physics (physics.space-ph)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Atomic Physics (physics.atom-ph)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: In the past, clues on the potential radiogenic activity of the lunar interior have been obtained from the isotopic composition of noble gases like Argon. Excess Argon (40) relative to Argon (36), as compared to the solar wind composition, is generally ascribed to the radiogenic activity of the lunar interior. Almost all the previous estimates were based on, 'on-the-spot' measurements from the landing sites. Relative concentration of the isotopes of 40Ar and 36Ar along a meridian by the Chandra's Altitudinal Composition Explorer (CHACE) experiment, on the Moon Impact Probe (MIP) of India's first mission to Moon, has independently yielded clues on the possible spatial heterogeneity in the radiogenic activity of the lunar interior in addition to providing indicative 'antiquity' of the lunar surface along the ground track over the near side of the moon. These results are shown to broadly corroborate the independent topography measurements by the Lunar Laser Ranging Instrument (LLRI) in the main orbiter Chandrayaan-1. The unique combination of these experiments provided high spatial resolution data while indicating the possible close linkages between the lunar interior and the lunar ambience.
The quark masses and meson spectrum: A holographic approach
Creators: name: Afonin, S. S.
name: Pusenkov, I. V.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The spectrum of radially excited unflavored vector mesons is relatively well measured, especially in the heavy-quark sector. This provides a unique opportunity to observe the behavior of the hadron spectrum at fixed quantum numbers as a function of the quark mass. The experimental data suggests the approximately Regge form for the radial spectrum, M_n^2=An+B, where A and B are growing functions of the quark mass. We use the bottom-up holographic approach to find the functions A and B. The obtained result shows a good agreement with the phenomenology and consistency with some predictions of the Veneziano-like dual amplitudes.
description: 17 pages, 3 figures, some clarifying remarks are added, to be published in Phys. Lett. B
Colorful SU(2) center vortices in the continuum and on the lattice
Creators: name: Schweigler, Thomas
name: Höllwieser, Roman
name: Faber, Manfried
name: Heller, Urs M.
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: The spherical vortex as introduced in [Phys. Rev. D77, 014515 (2008)] is generalized. A continuum form of the spherical vortex is derived and investigated in detail. The discrepancy between the gluonic lattice topological charge and the index of the lattice Dirac operator described in previous papers is identified as a discretization effect. The importance of the investigations for Monte Carlo configurations is discussed.
description: 8 pages, 3 figures
Additional file 6 of Large scale genomic rearrangements in selected Arabidopsis thaliana T-DNA lines are caused by T-DNA insertion mutagenesis
Creators: name: Pucker, Boas
name: Kleinbölting, Nils
name: Weisshaar, Bernd
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 6. Structure of genomic locus around one insertion in GK-909H04.
Policy Brief Broadening the Scope in Water Management
Creators: name: Damman, Sigrid
name: Lund, Henrik Brynthe
name: Mäkitie, Tuukka
name: Helness, Herman
Publisher: name: Zenodo
Year: 2022
Subjects: Water recycling and reuse
Environment, resources and sustainability
Circular economy
Sustainability transition
Symbiosis between industry and water utilities

description: Circular economy provides opportunities for value creation from resource recovery and reuse of treated wastewater, contributing to economic, social, and environmental sustainability. However, it also involves several challenges. Some of these are technological, but many are mainly governance related. This brief, targeted to water managers and policy makers, provides five learnings on the kinds of change we need to transition towards water management systems suited for circular economy.
Mayria madagascariensis Forel 1878
Creators: name: Forel, A.
Publisher: name: L'Imprimerie Nationale
Year: 1891
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Mayria
Mayria madagascariensis

description: MAYRIA MADAGASCARIENSIS, Forel.
(Pl. II, fig. 7 et 7a)
Mayria madagascariensis, Forel, Bulletin de la Société entomologique de Belgique (1886).
[[worker]]. Longueur 4,7 mill.
Caractères du genre. Arêtes frontales faiblement recourbées en S, très fortement divergentes et très distantes. Derrière, elles sont bien plus rapprochées du bord de la tête que l'une de l'autre. Tête assez petite, plus ou moins ovale (ouvrière minor?), un peu plus large derrière que devant. Mandibules étroites. Yeux grands, situés en arrière du milieu des cotés de la tête. Epistome caréné, faiblement avancé au milieu en lobe arrondi, entier. Aire frontale large, courte, peu distincte. Thorax comme chez la petite ouvrière d'un Camponotus ordinaire, arqué, élargi devant, rétréci derrière. Pronotum sans épaules, un peu aplati, presque aussi large que la tête. Face déclive du métanotum très courte. Sutures fortement imprimées. N œ ud du pédicule cubique-arrondi, un peu incliné en avant.
Luisante, très finement réticulée. Thorax et abdomen faiblement ridés transversalement (longitudinalement sur les côtés du thorax). Quelques rares poils dressés jaunâtres épars çà et là; une pubescence éparse, mais assez longue, un peu soulevée sur les pattes et les scapes, presque nulle ailleurs. Noire; mandibules d'un brun jaunâtre; antennes et tarses d'un jaune testacé, sauf l'extrémité des scapes et des funicules qui est brunie. Articulations des jambes et bord postérieur des segments abdominaux d'un jaune un peu blanchâtre.
Madagascar (M. Grandidier).
description: Published as part of Forel, A., 1891, Histoire naturelle des Hymenopteres. Deuxieme partie: Les Formicides., pp. 1-231 in Histoire Physique, Naturelle et Politique de Madagascar., Paris :L'Imprimerie Nationale on pages 75-76, DOI: 10.5281/zenodo.9896
Adaptive Query Processing in Link Traversal
Creators: name: Hanski, Jonni
Publisher: name: Zenodo
Year: 2022

description: Extracting a subset or a derived set of data from a larger dataset requires a plan for how to do it efficiently. Creating a good plan, however, requires relevant beforehand knowledge about the data being processed. With traditional databases, sufficient information might be available and up-to-date, however with Linked Data that may not be the case, resulting in inefficient plans that later need to be adjusted. But how to detect when a plan is not efficient enough and needs to be adjusted, when can the plan be adjusted and how can it be adjusted? Has the problem been solved already, or is there something left to explore?
Kurtomathrips morrilli Moulton 1927
Creators: name: Rasool, Iftekhar
name: Alattal, Yehya Zaki
name: Aldhafer, Hathal M.
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Thysanoptera
Thripidae
Kurtomathrips
Kurtomathrips morrilli

description: Kurtomathrips morrilli Moulton Kurtomathrips morrilli Moulton, 1927: 188. This species was described from Arizona in the USA and is widely distributed in southern United States. Unlike other members of the genus, this species has become distributed out of its native range, and is recorded from India (Bhatti et al. 1999), new Saudi Arabia, and although intercepted by plant quarantine in Japan (Masumoto 2010) it is not actually recorded in that country. Material studied. Al Baha. Al Janabeen, two females from Commiphora sp., 22.ix.2020, (BT); Qilwah, five females from Cenchrus pennisetiformis, 25.ix.2020, (BT).
description: Published as part of Rasool, Iftekhar, Alattal, Yehya Zaki & Aldhafer, Hathal M., 2023, Faunistic inventory, identification keys and zoogeographical analysis of the Thysanoptera-Terebrantia of Saudi Arabia, including two new species, pp. 151-200 in Zootaxa 5306 (2) on page 178, DOI: 10.11646/zootaxa.5306.2.1, http://zenodo.org/record/8058749
description: {"references": ["Moulton, D. (1927) Thysanoptera - New species and notes. Bulletin of the Brooklyn Entomological Society, 22, 181 - 202.", "Bhatti, J. S., Veer, V. & Dahiya, A. (1999) The north American species Kurtomathrips morrilli Moulton and Neohydatothrips gracilipes (Hood) (Terebrantia: Thripidae). Have now established large populations from North to South India. Thrips, 1, 54 - 57. https: // doi. org / 10.46318 / Thrips. 1.1999.10 - 14", "Masumoto, M. (2010) Key to genera of the subfamily Thripinae (Thysanoptera: Thripidae) associated with Japanese plant quarantine. Res. Bull. Pl. Prot. Japan, 46, 25 - 59."]}
Atomic Hydrogen in a Galactic Center Outflow
Creators: name: McClure-Griffiths, N. M.
name: Green, J. A.
name: Hill, A. S.
name: Lockman, F. J.
name: Dickey, J. M.
name: Gaensler, B. M.
name: Green, A. J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We describe a population of small, high velocity, atomic hydrogen clouds, loops, and filaments found above and below the disk near the Galactic Center. The objects have a mean radius of 15 pc, velocity widths of $\sim 14$ km/s and are observed at $|z|$ heights up to 700 pc. The velocity distribution of the clouds shows no signature of Galactic rotation. We propose a scenario where the clouds are associated with an outflow from a central star-forming region at the Galactic Center. We discuss the clouds as entrained material traveling at $\sim 200$ km/s in a Galactic wind.
description: Accepted for publication in Astrophysical Journal Letters
Localization at the Edge of 2D Topological Insulator by Kondo Impurities with Random Anisotropies
Creators: name: Altshuler, B. L.
name: Aleiner, I. L.
name: Yudson, V. I.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We consider chiral electrons moving along the 1D helical edge of a 2D topological insulator and interacting with a disordered chain of Kondo impurities. Assuming the electron-spin couplings of random anisotropies, we map this system to the problem of the pinning of the charge density wave by the disordered potential. This mapping proves that arbitrary weak anisotropic disorder in coupling of chiral electrons with spin impurities leads to the Anderson localization of the edge states.
description: Minor revisions; 4 pages, 1 figure
A classical simulation of nonlinear Jaynes--Cummings and Rabi models in photonic lattices
Creators: name: Rodríguez-Lara, B. M.
name: Soto-Eguibar, Francisco
name: Cárdenas, Alejandro Zárate
name: Moya-Cessa, H. M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Optics (physics.optics)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The interaction of a two-level atom with a single-mode quantized field is one of the simplest models in quantum optics. Under the rotating wave approximation, it is known as the Jaynes-Cummings model and without it as the Rabi model. Real-world realizations of the Jaynes-Cummings model include cavity, ion trap and circuit quantum electrodynamics. The Rabi model can be realized in circuit quantum electrodynamics. As soon as nonlinear couplings are introduced, feasible experimental realizations in quantum systems are drastically reduced. We propose a set of two photonic lattices that classically simulates the interaction of a single two-level system with a quantized field under field nonlinearities and nonlinear couplings as long as the quantum optics model conserves parity. We describe how to reconstruct the mean value of quantum optics measurements, such as photon number and atomic energy excitation, from the intensity and from the field, such as von Neumann entropy and fidelity, at the output of the photonic lattices. We discuss how typical initial states involving coherent or displaced Fock fields can be engineered from recently discussed Glauber-Fock lattices. As an example, the Buck-Sukumar model, where the coupling depends on the intensity of the field, is classically simulated for separable and entangled initial states.
description: 13 pages, 3 figures
Fracture and Fatigue Properties of Thick Structural Adhesives
Creators: name: Iyer Kumar, Rahul
name: De Waele, Wim
Publisher: name: Zenodo
Year: 2022

description: As an engineer and researcher, it is important to understand what combination of loading and environmental conditions will cause failure of a component or structure rather than just determining whether failure will be avoided. Future work will focus on an in-depth investigation of failure conditions and mechanisms for various adhesive systems subjected to different load conditions.
Additional file 7 of Large scale genomic rearrangements in selected Arabidopsis thaliana T-DNA lines are caused by T-DNA insertion mutagenesis
Creators: name: Pucker, Boas
name: Kleinbölting, Nils
name: Weisshaar, Bernd
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 7. Analysis results of genomic fusion junction sequences without T-DNA insertion.
Rotating Globular Clusters
Creators: name: Bianchini, P.
name: Varri, A. L
name: Bertin, G.
name: Zocchi, A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Internal rotation is considered to play a major role in the dynamics of some globular clusters. However, in only few cases it has been studied by quantitative application of realistic and physically justified global models. Here we present a dynamical analysis of the photometry and three-dimensional kinematics of omega Cen, 47 Tuc, and M15, by means of a recently introduced family of self-consistent axisymmetric rotating models. The three clusters, characterized by different relaxation conditions, show evidence of differential rotation and deviations from sphericity. The combination of line-of-sight velocities and proper motions allows us to determine their internal dynamics, predict their morphology, and estimate their dynamical distance. The well-relaxed cluster 47 Tuc is very well interpreted by our model; internal rotation is found to explain the observed morphology. For M15, we provide a global model in good agreement with the data, including the central behavior of the rotation profile and the shape of the ellipticity profile. For the partially relaxed cluster omega Cen, the selected model reproduces the complex three-dimensional kinematics; in particular the observed anisotropy profile, characterized by a transition from isotropy, to weakly-radial anisotropy, and then to tangential anisotropy in the outer parts. The discrepancy found for the steep central gradient in the observed line-of-sight velocity dispersion profile and for the ellipticity profile is ascribed to the condition of only partial relaxation of this cluster and the interplay between rotation and radial anisotropy.
description: 19 pages, 14 figures, accepted for publication in the Astrophysical Journal
Floating Wind Turbine Platform in Waves: Computationally-Efficient Algorithm for Numerical Simulation
Creators: name: Pribadi, Ajie B. K
name: Verao Fernandez, Gael
name: Lataire, Evert
Publisher: name: Zenodo
Year: 2022

description: This study has developed a numerical tool capable of performing mooring design optimization analysis for floating wind turbine (FWT) platforms. The numerical model is capable of: i) correctly model the physical behavior of a moored FWT platform and ii) run at a low computational cost (i.e., faster than real-time) allowing for the evaluations of many different mooring configurations. The numerical model is based on the
 Cummins-Ogilvie equation of motion. These hybrid frequency-time-domain approach, allows to perform fast time-domain simulation of floating bodies including external forces such as mooring lines or viscous effects. Firstly, the platform’s excitation force and hydrodynamic coefficients are obtained in the frequency domain utilizing a Boundary Element Method (BEM) solver. Secondly, the results from the BEM solver are converted to the time-domain via convolution integral of the impulse response functions to calculate the radiation force and inverse discrete Fourier transform to compute the excitation force. Thirdly, viscous effect are considered via the Morison Equation using empirical coefficients. Finally, the mooring lines are modelled according to the lumped-mass approach, omitting the coupling between internal nodes allowing the system to be transformed into numerous ordinary differential equations that are solved individually. The established numerical tool can be further coupled with a single and/or multi-objective optimization methods (e.g., genetic algorithm, particle swarm optimization, etc.) to perform a mooring design loop for an FWT platform achieving the optimal configuration in terms of platform motions, mooring line tensions and cost.
Additional file 8 of Large scale genomic rearrangements in selected Arabidopsis thaliana T-DNA lines are caused by T-DNA insertion mutagenesis
Creators: name: Pucker, Boas
name: Kleinbölting, Nils
name: Weisshaar, Bernd
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 8. Visual overview over all insertions detected.
Additional file 9 of Large scale genomic rearrangements in selected Arabidopsis thaliana T-DNA lines are caused by T-DNA insertion mutagenesis
Creators: name: Pucker, Boas
name: Kleinbölting, Nils
name: Weisshaar, Bernd
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 9. Assembly statistics of Col-0_GK-wt.
von Kármán energy decay and heating of protons and electrons in a kinetic turbulent plasma
Creators: name: Wu, P.
name: Wan, M.
name: Matthaeus, W. H.
name: Shay, M. A.
name: Swisdak, M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Decay in time of undriven weakly collisional kinetic plasma turbulence in systems large compared to the ion kinetic scales is investigated using fully electromagnetic particle-in-cell simulations initiated with transverse flow and magnetic disturbances, constant density, and a strong guide field. The observed energy decay is consistent with the von Kármán hypothesis of similarity decay, in a formulation adapted to magnetohydrodyamics (MHD). Kinetic dissipation occurs at small scales, but the overall rate is apparently controlled by large scale dynamics. At small turbulence amplitude the electrons are preferentially heated. At larger amplitudes proton heating is the dominant effect. In the solar wind and corona the protons are typically hotter, suggesting that these natural systems are in large amplitude turbulence regime.
description: Accepted by Phys. Rev. Lett. on August 29, 2013
Classification of 1-Weierstrass points on Kuribayashi quartics, I (with two parameters)
Creators: name: Badr, Eslam E.
name: Saleem, Mohammed A.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: Primary 14H55, 14R20, Secondary 14H37, 14H45, 14H50

description: In this paper, we classify the 1-Weierstrass points of the Kuribayashi quartic curves with two parameters $a$ and $b$ defined by the equation \[C_{a,b}:x^{4}+y^{4}+z^{4}+ax^{2}y^{2}+b(x^{2}+y^{2})z^{2}=0,\] such that $(a^2-4)(b^2-4)(a^2-1)(b^{2}-a-2)\neq0.$ Furthermore, the geometry of these points is investigated.
description: 16 pages, LaTeX file, Presented in "International Conference on Mathematics, Trends, Development (ICMTD12)" held at Cairo, Egypt, December 27-29, 2012. MSC 2010:Primary 14H55, 14R20; Secondary 14H37, 14H45, 14H50 (References have been modified, proofs have been added, conclusions have been extended,...etc)
The potential of sparse photometric data in asteroid shape modeling
Creators: name: Hanuš, J.
name: Ďurech, J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We investigate the potential of the sparse data produced by the Catalina Sky Survey astrometric project (CSS for short) in asteroid shape and rotational state determination by the lightcurve inversion method. We show that although the photometric quality of the CSS data, compared to the dense data, is significantly worse, it is in principle possible that these data are for some asteroids with high lightcurve amplitudes sufficient for a unique shape determination. CSS data are available for $\sim$180 asteroids for which shape models were previously derived from different photometric data sets. For 13 asteroids from this sample, we derive their unique shape models based only on CSS data, compare the two independent shape models together and discuss the reliability of models derived from only CSS data. We also use CSS data to determine shape models for asteroids with already known rotational period values, derive 12 unique models and compare previously published periods with periods determined from the full 3D modeling by the lightcurve inversion method. Finally, we test different shape resolutions used in the lightcurve inversion method in order to find reliable asteroid models.
description: Published in Planetary and Space Science, Volume 73, September 2012
Additional file 1 of Opportunities and limits of combining microbiome and genome data for complex trait prediction
Creators: name: Pérez-Enciso, Miguel
name: Zingaretti, Laura M.
name: Ramayo-Caldas, Yuliaxis
name: de los Campos, Gustavo
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Statistics
subject: FOS: Mathematics

description: Additional file 1: Figure S1. Comparison between flat and informative priors. Posterior distributions of heritability (black line) and microbiability (blue dashed line) in a single replicate of the ‘Joint’ scenario, $$r^{2}$$ r 2 = 0.25. Numbers in the panel titles are predictive accuracies for each prior and method. Overall, mildly informative priors resulted in similar predictive accuracies as for flat priors and more reasonable posterior distributions. Figure S2. Gibbs sampling values of heritability (black line), microbiability (red line), and correlation between genome and microbiome effects (green line) in a single replicate of the ‘Recursive’ scenario ( $$r^{2}$$ r 2 = 0.5). The comparison is between flat and informative priors. Figure S3. Results with the null model using the Bayes C model. This figure shows the results with the null model using the Bayes C model when samples were permuted relative to genotypes and abundances. (A) Prediction accuracy, computed as correlation between predicted and observed phenotypes, for each of the Bayes C analyses: Cgb includes microbiome and genome; Cg includes genome data only, and Cb includes microbiome data only. (B) Estimates of heritability ( $$h^{2}$$ h 2 ) and microbiability ( $$b^{2}$$ b 2 ) for each of the Bayes C analyses. Data are the average of 30 replicates. Figure S4. Plot of the principal component analysis of the original abundance data (top left) and three simulated datasets under the ‘Recursive’ model. Each dot corresponds to a single individual and data are log-transformed. The permutation has a negligible influence on the data structure. Figure S5. Distributions of effects. (A) Observed and fitted (red line) distribution of abundance linear regression effects on methane emissions reported by Difford et al. [4]. (B) Comparison of gamma distributions used for sampling genetic ( $$\alpha$$ α ) and OTUs’ ( $$\omega$$ ω ) effects: $$\alpha \sim {\Gamma }$$ α ∼ Γ ( $$k$$ k = 0.2, $$\theta$$ θ = 5) and $$\omega \sim {\Gamma }$$ ω ∼ Γ (k = 1.4, $$\theta$$ θ = 3.8), plotted in red and black lines, respectively (Eq. 1).
A bright impulsive solar burst detected at 30 THz
Creators: name: Kaufmann, P.
name: White, S. M.
name: Freeland, S. L.
name: Marcon, R.
name: Fernandes, L. O. T.
name: Kudaka, A. S.
name: de Souza, R. V.
name: Aballay, J. L.
name: Fernandez, G.
name: Godoy, R.
name: Marun, A.
name: Valio, A.
name: Raulin, J. -P.
name: de Castro, C. G. Giménez
Publisher: name: arXiv
Year: 2013
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Ground- and space-based observations of solar flares from radio wavelengths to gamma-rays have produced considerable insights but raised several unsolved controversies. The last unexplored wavelength frontier for solar flares is in the range of submillimeter and infrared wavelengths. Here we report the detection of an intense impulsive burst at 30 THz using a new imaging system. The 30 THz emission exhibited remarkable time coincidence with peaks observed at microwave, mm/submm, visible, EUV and hard X-ray wavelengths. The emission location coincides with a very weak white-light feature, and is consistent with heating below the temperature minimum in the atmosphere. However, there are problems in attributing the heating to accelerated electrons. The peak 30 THz flux is several times larger than the usual microwave peak near 9 GHz, attributed to non-thermal electrons in the corona. The 30 THz emission could be consistent with an optically thick spectrum increasing from low to high frequencies. It might be part of the same spectral component found at sub-THz frequencies whose nature remains mysterious. Further observations at these wavelengths will provide a new window for flare studies.
description: 9 pages, 11 figures, accepted by Astrophysical Journal, March 23, 2013
Electrospinning of Silica Nanofibers: How the Sol Viscosity Influences the Taylor Cone
Creators: name: Verschraegen, Sofie
name: De Buysser, Klaartje
name: D'hooge, Dagmar R.
name: De Clerck, Karen
Publisher: name: Zenodo
Year: 2022

description: Silica nanofibrous membranes are flexible, light-weight and porous materials that showcase excellent thermal and chemical resistance. However, the production via a combination of sol-gel synthesis and electrospinning depends on many factors of which the influence is not completely understood. In this work, we investigate the link between the viscosity and the electrospinnability of the tetraethylorthosilicate (TEOS) based spinning solution as a first step in linking the different scales in the process. The viscosity of the silica sol has a clear effect on the behavior of the Taylor cone and hence on the stability of the electrospinning process. Exploiting these insights is of great importance for future chemically driven tuning of silica nanofibrous membranes.
Adaptive Spectral Band Integration in Thermographic Inspection of Composites
Creators: name: Poelman, Gaétan
name: Hedayatrasa, Saeid
name: Kersemans, Mathias
Publisher: name: Zenodo
Year: 2022

description: Internal damage features are a major issue for composites due to their layered structure, and must be detected in a reliable, nondestructive manner. Flash thermography is a promising non-destructive testing (NDT) technique that can be used to rapidly identify such internal anomalies. Advanced data analysis techniques are required to obtain high-quality detection of these damages, especially when concerned with small and deep defects. The most-often used state-of-the-art algorithm, called Pulsed Phase Thermography (PPT), is efficient in enhancing the defect detectability, but is not always straightforward to be interpreted. In order to overcome those limitations, a novel Adaptive Spectral Band Integration (ASBI) technique is proposed.
Fixing the Foundations: Towards Generalization for Machine Learning
Creators: name: Verkerken, Miel
name: D'hooge, Laurens
name: Wauters, Tim
name: Volckaert, Bruno
name: De Turck, Filip
Publisher: name: Zenodo
Year: 2022

description: An intrusion detection system (IDS) is a security monitoring system capable of detecting potential attacks exceeding the firewall. Traditionally, these systems rely on pattern matching and signatures of known attacks, but in the last decades, security researchers have shifted their interest to machine learning (ML) techniques with varying degrees of success. While the published literature reports outstanding results, we are still waiting for the breakthrough of operational ML-IDS in the real world. To address this issue, we investigate the source of the problem, the datasets themselves, and propose guidelines to work with existing benchmark datasets to improve the generalization power of the ML models. This study evaluates the generalization strength of a ML model using the novel inter-dataset evaluation strategy compared to the traditional intra-dataset strategy. The results show high classification performance on the training dataset but fail to transfer this to a second related but unseen dataset with an average drop in accuracy of 25%. The proposed inter-dataset evaluation strategy empowers future research to estimate the generalization strength of ML solutions closer to a real-world setting.
Metallicity Bias in the Kinematics of the Milky Way Stellar Halo
Creators: name: Kafle, P. R.
name: Sharma, S.
name: Lewis, G. F.
name: Bland-Hawthorn, J.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Here we study the metallicity bias in the velocity dispersions, the derived quantity called anisotropy and the mean azimuthal velocity profiles of the Milky Way stellar halo using Blue Horizontal Branch (BHB) stars taken from SDSS/SEGUE survey. The comparatively metal-rich sample ([Fe/H]>-2) has prograde motion and is found to have an offset of 40 km/s in the mean azimuthal velocity with respect to a metal-poor sample ([Fe/H]<=-2) which has retrograde motion. The difference in rotation between the most metal-poor and most metal-rich population was found to be around 65 km/s. For galactocentric distances r<16 kpc, an offset in velocity dispersion profiles and anisotropy can also be seen. In the inner regions, the metal-poor population is in average tangential orbit; however, anisotropy is found to decrease monotonically with radius independent of metallicity. Beyond r = 16 kpc, both the metal-rich and the metal-poor samples are found to have tangential motion. The metallicity bias in the kinematics of the halo stars qualitatively supports the co-existence of at least two-components in the halo having different formation history e.g. in-situ formation and formation by accretion.
description: Accepted for publication in MNRAS (2013 January 14)
Colobopsis Mayr 1861
Creators: name: Forel, A.
Publisher: name: L'Imprimerie Nationale
Year: 1891
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Colobopsis

description: Genre COLOBOPSIS.
Colobopsis, Mayr, Europäische Formiciden (1861).
[[worker]], [[queen]], [[soldier]] et [[male]]. Nymphes nues. Abdomen comme chez les Camponotus, mais plus étroit et plus allongé. La fourmilière présente un trimorphisme de la femelle, c'est-à-dire un soldat à grosse tête tronquée, distinct de l'ouvrière.
[[worker]]. Tête obtuse, mais pas tronquée, très épaisse. Jambes courtes. Du reste identique aux Camponotus, [[worker]] minor.
[[soldier]]. Tête longue, dilatée et tronquée obliquement antérieurement. Les antennes s'insèrent derrière la troncature, qui comprend les mandibules, la partie antérieure des joues et de l'épistome, ainsi que les fossettes clypéales. Du reste comme la [[worker]] et comme elle sans ocelles.
[[queen]]. Comme le soldat. Corps long et étroit; troncature un peu plus faible et tête moins dilatée devant.
[[male]]. Comme chez les Camponotus. Premier article du funicule renflé à l'extrémité, deux fois long et épais comme le suivant.
description: Published as part of Forel, A., 1891, Histoire naturelle des Hymenopteres. Deuxieme partie: Les Formicides., pp. 1-231 in Histoire Physique, Naturelle et Politique de Madagascar., Paris :L'Imprimerie Nationale on pages 76-77, DOI: 10.5281/zenodo.9896
Screening the fifth force in the Horndeski's most general scalar-tensor theories
Creators: name: Kase, Ryotaro
name: Tsujikawa, Shinji
Publisher: name: arXiv
Year: 2013
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study how the Vainshtein mechanism operates in the most general scalar-tensor theories with second-order equations of motion. The field equations of motion, which can be also applicable to most of other screening scenarios proposed in literature, are generally derived in a spherically symmetric space-time with a matter source. In the presence of a field coupling to the Ricci scalar, we clarify conditions under which the Vainshtein mechanism is at work in a weak gravitational background. We also obtain the solutions of the field equation inside a spherically symmetric body and show how they can be connected to exterior solutions that accommodate the Vainshtein mechanism. We apply our general results to a number of concrete models such as the covariant/extended Galileons and the DBI Galileons with Gauss-Bonnet and other terms. In these models the fifth force can be suppressed to be compatible with solar-system constraints, provided that non-linear field kinetic terms coupled to the Einstein tensor do not dominate over other non-linear field self-interactions.
description: 25 pages, 3 figures
Keck II Observations of Hemispherical Differences in H2O2 on Europa
Creators: name: Hand, Kevin P.
name: Brown, Mike E.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present results from Keck II observations of Europa over four consecutive nights using the near-infrared spectrograph (NIRSPEC). Spectra were collected in the 3.14--4.0 micron range, allowing detection and monitoring of the 3.5 micron feature due to hydrogen peroxide. Galileo Near-Infrared Spectrometer (NIMS) results first revealed hydrogen peroxide on Europa in the anti-jovian region of the leading hemisphere at an abundance of 0.13+/-0.07% by number abundance relative to water. We find comparable results for the two nights over which we observed the leading hemisphere. Significantly, we observed a small amount of hydrogen peroxide (~0.04%) during observations of Europa's anti- and sub-Jovian hemispheres. Almost no hydrogen peroxide was detected during observations of just the trailing hemisphere. We conclude that the Galileo observations likely represent the maximum hydrogen peroxide concentration, the exception potentially being the cold water ice regions of the poles, which are not readily observable from the ground. Our mapping of the peroxide abundance across Europa requires revisions to previous estimates for Europa's global surface abundance of oxidants and leads to a reduction in the total oxidant delivery expected for the sub-surface ocean, if exchange of surface material with the ocean occurs.
description: 4 pages, 1 figure
Orbital upper critical field of type-II superconductors with pair breaking
Creators: name: Kogan, V. G.
name: Prozorov, R.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The orbital upper critical field $H_{c2} $ is evaluated for isotropic materials with arbitrary transport and pair-breaking scattering rates. It is shown that unlike transport scattering which enhances $H_{c2} $, the pair breaking suppresses the upper critical field and reduces the dimensionless ratio $h^*(0)=H_{c2}(0)/T_c(dH_{c2}/dT)_{T_c} $ from the Helfand-Werthamer value of $\approx 0.7$ to 0.5 for a strong pair-breaking. $h^*(T)$ is evaluated for arbitrary transport and pair-breaking scattering. A phenomenological model for the pair-breaking suppression by magnetic fields is introduced. It shows qualitative features such as a positive curvature of $H_{c2}(T) $ and the low temperature upturn usually associated with multi-band superconductivity.
Additional file 1 of Identifying trauma patients with benefit from direct transportation to Level-1 trauma centers
Creators: name: Sewalt, Charlie A.
name: Gravesteijn, Benjamin Y.
name: Nieboer, Daan
name: Steyerberg, Ewout W.
name: Den Hartog, Dennis
name: Van Klaveren, David
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1: Table S1. Odds ratios with 95% confidence interval for the three regression models calculating benefit from direct transportation to Level-1 trauma center. For continuous variables the odds ratio of the 75th percentile versus the median and median versus 25th percentile is presented. Continuous variables from interaction terms are centered in order to make the main effects interpretable. Odds ratios above 1 indicate an increase in the probability of mortality. Table S2. Characteristics of patients who benefit from transportation to a Level-1/2 trauma centers, based on predicted absolute benefit from the regression model with interaction terms. Harm was defined as more than 1% absolute harm, while benefit was defined as more than 1% absolute benefit. Table S3. Characteristics of patients who substantially benefit from transportation to a Level-1 trauma centers, based on predicted benefit above 0 in 95% of bootstrapped samples from the regression model with interaction terms.
Prediction of Disassembly Parameters for Process Planning Based on Machine Learning
Creators: name: Blümel, Richard
name: Zander, Niklas
name: Blankemeyer, Sebastian
name: Raatz, Annika
Publisher: name: Cham : Springer
Year: 2023
Subjects: subject: Disassembly planning
subject: Regeneration
subject: Machine learning
subject: Konferenzschrift
subject: Dewey Decimal Classification::600 | Technik

description: The disassembly of complex capital goods is characterized by strong uncertainty regarding the product condition and possible damage patterns to be expected during a regeneration job. Due to the high value of complex capital goods, the disassembly process must be as gentle as possible and being adaptable to the varying und uncertain product's state. While methods based on data mining have already been successfully used to forecast capacity and material requirements, the determination of the product’s or component's condition has become apparent in the recent past. Despite the rapid increase in sensor technology on capital goods such as aircraft engines and their use for condition monitoring due to countless interfering effects, it is only possible to react spontaneously to the product’s condition. So far, we have concentrated on product condition-based prioritization of disassembly operations in a logistics-oriented sequencing strategy. In this article, we present an approach to predict disassembly process-planning parameters based on operational usage data using machine learning. With the prediction of disassembly forces and times, processes, tools and capacities can be efficiently planned. Thus, we can establish a component-friendly disassembly process adaptable to varying product conditions. In this article, we show the successful validation on a replacement model of an aircraft engine.
Additional file 2 of Identifying trauma patients with benefit from direct transportation to Level-1 trauma centers
Creators: name: Sewalt, Charlie A.
name: Gravesteijn, Benjamin Y.
name: Nieboer, Daan
name: Steyerberg, Ewout W.
name: Den Hartog, Dennis
name: Van Klaveren, David
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 2: Figure S1. Calibration of benefit, for both the model with (B) and without interaction terms (A). Calibration of benefit is plotted with the predicted absolute treatment benefit on the x-axis and observed absolute treatment benefit on the y-axis. The study population was therefore divided in 20 equal groups based on the predicted absolute treatment benefit. A predicted absolute benefit of 1% (0.01) for a particular patient means 1% less mortality when this particular patient is brought to a Level-1/2 trauma center instead of a Level-3 trauma center.
Deceleration and trapping of ammonia molecules in a traveling wave decelerator
Creators: name: Jansen, Paul
name: Quintero-Pérez, Marina
name: Wall, Thomas E.
name: Berg, Joost E. van den
name: Hoekstra, Steven
name: Bethlem, Hendrick L.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We have recently demonstrated static trapping of ammonia isotopologues in a decelerator that consists of a series of ring-shaped electrodes to which oscillating high voltages are applied [Quintero-Pérez et al., Phys. Rev. Lett. 110, 133003 (2013)]. In this paper we provide further details on this traveling wave decelerator and present new experimental data that illustrate the control over molecules that it offers. We analyze the performance of our setup under different deceleration conditions and demonstrate phase-space manipulation of the trapped molecular sample.
description: arXiv admin note: text overlap with arXiv:1301.2113