cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 3: of Results of a feasibility cluster randomised controlled trial of a peer-led school-based intervention to increase the physical activity of adolescent girls (PLAN-A)
Creators: name: Sebire, Simon
name: Jago, Russell
name: Banfield, Kathryn
name: Edwards, Mark
name: Campbell, Rona
name: Kipping, Ruth
name: Blair, Peter
name: Bryar Kadir
name: Garfield, Kirsty
name: Matthews, Joe
name: Lyons, Ronan
name: Hollingworth, William
Publisher: name: figshare
Year: 2018
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: Plant Biology

description: Baseline descriptive statistics of peer-supporter and non-peer-supporter students. Descriptive data for peer-supporters and non-peer-supporters at baseline. (DOCX 15 kb)
Fast and stable method for simulating quantum electron dynamics
Creators: name: Watanabe, Naoki
name: Tsukada, Masaru
Publisher: name: arXiv
Year: 2000
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: A fast and stable method is formulated to compute the time evolution of a wavefunction by numerically solving the time-dependent Schr{ö}dinger equation. This method is a real space/real time evolution method implemented by several computational techniques such as Suzuki's exponential product, Cayley's form, the finite differential method and an operator named adhesive operator. This method conserves the norm of the wavefunction, manages periodic conditions and adaptive mesh refinement technique, and is suitable for vector- and parallel-type supercomputers. Applying this method to some simple electron dynamics, we confirmed the efficiency and accuracy of the method for simulating fast time-dependent quantum phenomena.
description: 10 pages, 35 eps figures
Efficient, portable and extensible packet inspection with eBPF
Creators: name: Repetto, Matteo
name: Zuppelli, Marco
name: Carrega, Alessandro
Publisher: name: Zenodo
Year: 2021
Subjects: Network covert channels
cloud computing
eBPF
amplification attacks
Kubernetes

description: The availability of virtualization technologies and cloud models has made possible an effective decoupling of applications and services from the underlying infrastructure, which eventually allows far more flexibility in deployment and operation processes than in the past. However, this also means that hardware acceleration will be available ever more seldom, which may jeopardize the efficiency of computing-intensive tasks, including network monitoring and packet inspection in cyber- security appliances. In ASTRID, we investigated the usage of the extended Berkeley Packet Filter (eBPF) for effective and efficient packet inspection. Our goal is the implementation of a tool that provides similar information as existing cyber-security appliances but with a reduced execution footprint, in order to be easily integrated in cloud-native applications without any hardware or software dependency on the underlying infrastructure. In this paper, we discuss the main results of our work with respect to two challenging use cases, namely amplification attacks and network covert channels.
Dirac-Surface-State-Dominated Spin to Charge Current Conversion in the Topological Insulator $(Bi_{0.22}Sb_{0.78})_2Te_3$ Films at Room Temperature
Creators: name: Mendes, J. B. S.
name: Alves-Santos, O.
name: Holanda, J.
name: Loreto, R. P.
name: de Araujo, C. I. L.
name: Chang, Cui-Zu
name: Moodera, J. S.
name: Azevedo, A.
name: Rezende, S. M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report the spin to charge current conversation in an intrinsic topological insulator (TI) $(Bi_{0.22}Sb_{0.78})_2Te_3$ film at room temperature. The spin currents are generated in a thin layer of permalloy (Py) by two different processes, spin pumping (SPE) and spin Seebeck effects (SSE). In the first we use microwave-driven ferromagnetic resonance of the Py film to generate a SPE spin current that is injected into the TI $(Bi_{0.22}Sb_{0.78})_2Te_3$ layer in direct contact with Py. In the second we use the SSE in the longitudinal configuration in Py without contamination by the Nernst effect made possible with a thin NiO layer between the Py and $(Bi_{0.22}Sb_{0.78})_2Te_3$ layers. The spin-to-charge current conversion is attributed to the inverse Edelstein effect (IEE) made possible by the spin-momentum locking in the electron Fermi contours due to the Rashba field. The measurements by the two techniques yield very similar values for the IEE parameter, which are larger than the reported values in the previous studies on topological insulators.
description: 18 pages and 7 figures
A STUDY ON RELATIONSHIP BETWEEN CAREER MATURITY AND SELF-ESTEEM AMONG SENIOR SECONDARY STUDENTS
Creators: name: Arundeep Kour*, Dr. Kuldeep Kaur Grewal** &  Dr. Rajnish Sharma**
Publisher: name: Zenodo
Year: 2024

description: Career maturity is crucial at every stage of life. However, secondary school students have a lot of difficulty selecting a career. The primary goal of schooling is the "improvement of vocational efficiency." Career-ready people are needed if we are to accomplish these goals. Students' self-esteem is also influenced by their career maturity. The goal of the current study was to investigate the relationship between secondary school students' self-esteem and professional maturity. The J&K Board of School Education's Dhounthly Educational Block provided a sample of 50 secondary school pupils for the study. The data was gathered using the Career Maturity Inventory by Crites and Savickas from 2011, the Self Esteem Inventory by Drs. Santosh Dhar and UpinderDhar from 2015, and other sources. The association between career maturity and self-esteem was determined using the coefficient of correlation, and the difference in career maturity between male and female secondary school students was determined using the t-value. The study came to the conclusion that self esteem and career maturity are positively correlated. Compared to women, men are more career-savvy.
Blind line search in ALMA deep fields as pathfinders for future synergies with ngVLA, JWST, SPICA
Creators: name: Andreani, Paola
Publisher: name: Zenodo
Year: 2019

description: The results of a blind search for emission lines in several ALMA datacubes at different depths - undertaken with the aim to construct a luminosity function of the FIR ([CII], [OIII]) and molecular lines at various redshifts - will be presented and discussed with a look at their role as reference for future ground-based and space mission at longer (ngVLA) and shorter (JWST and SPICA) wavelengths. We have used a few different - both empirical and statistical - methods to extract sources with a high level of reliability. The main target of this project are the FIR lines which are responsible for the cooling of the interstellar medium (ISM) and which are directly connected to the star formation processes in galaxies. The individual study of these lines allows to investigate also the physical properties of the ISM. For instance, the [CII] 158 μm line mainly arises from cold neutral gas heated by massive stars and the [OIII] 88 μm line arises only from ionised gas. The [CII]/[OIII] luminosity ratio shows a transition from above unity at z = 0 to less at z ≥ 7 indicating that targeting [CII] and [OIII] lines will enable us to study the transition of properties of the ISM at various redshifts. However any other line (for instance various CO transition, water) may be identified with our methods. Once consolidated the physical properties of the high-z sources blindly discovered will constitute a database which will be used both as follow-up and synergies at longer and shorter wavelengths. The exploitation of their characteristics allows similar searches at larger redshift with ngVLA and at the same time studying their counterpart at mid- and far-IR with JSWT and SPICA.
Look Wider to Match Image Patches with Convolutional Neural Networks
Creators: name: Park, Haesol
name: Lee, Kyoung Mu
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: When a human matches two images, the viewer has a natural tendency to view the wide area around the target pixel to obtain clues of right correspondence. However, designing a matching cost function that works on a large window in the same way is difficult. The cost function is typically not intelligent enough to discard the information irrelevant to the target pixel, resulting in undesirable artifacts. In this paper, we propose a novel learn a stereo matching cost with a large-sized window. Unlike conventional pooling layers with strides, the proposed per-pixel pyramid-pooling layer can cover a large area without a loss of resolution and detail. Therefore, the learned matching cost function can successfully utilize the information from a large area without introducing the fattening effect. The proposed method is robust despite the presence of weak textures, depth discontinuity, illumination, and exposure difference. The proposed method achieves near-peak performance on the Middlebury benchmark.
description: published in SPL
title: Histoire : abide he mogui
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Characterizing outflows from low-mass object Chamaeleon-MMS1
Creators: name: Allen, Veronica
Publisher: name: Zenodo
Year: 2019

description: In the study of low-mass star formation, a pivotal object is being sought: the first hydrostatic core (FSHC). Theoretical models predict that FSHCs are the direct precursors of protostars prior to the onset of nuclear fusion, are extremely short-lived, very faint (0.01-0.1 Lsun), and drive a very weak molecular outflow. Several candidates have been identified in recent years, one of which is Chalmaeleon-MMS1 (Cha-MMS1). We have studied this object using moderately-high resolution (~0.5'' or 75 au) Cycle 2 ALMA observations of outflow and dense gas tracers. We find clear evidence of weak outflows in CO and 13CO, and of their interactions with the surrounding cloud through CS, H2CO and CH3OH emission. H2CO is detected toward the continuum source with a rotational temperature of ~70K, but CH3OH is not detected toward the source, indicating a very weak protostar. The outflows have several orders of magnitude lower kinetic energy and mechanical luminosity than Class 0 objects and even fellow FSHC candidate L1448, making this among the earliest protostellar object detected. The red and blue components are also very disorganized implying that the early years are a chaotic period for outflows.
Galaxy And Mass Assembly: Automatic Morphological Classification of Galaxies Using Statistical Learning
Creators: name: Sreejith, Sreevarsha
name: Pereverzyev, Sergiy
name: Kelvin, Lee S.
name: Marleau, Francine
name: Haltmeier, Markus
name: Ebner, Judith
name: Bland-Hawthorn, Joss
name: Driver, Simon P.
name: Graham, Alister W.
name: Holwerda, Benne W.
name: Hopkins, A. M.
name: Liske, J.
name: Loveday, Jon
name: Moffett, Amanda J.
name: Pimbblet, K. A.
name: Taylor, Edward N.
name: Wang, Lingyu
name: Wright, Angus H.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We apply four statistical learning methods to a sample of $7941$ galaxies ($z<0.06$) from the Galaxy and Mass Assembly (GAMA) survey to test the feasibility of using automated algorithms to classify galaxies. Using $10$ features measured for each galaxy (sizes, colours, shape parameters \& stellar mass) we apply the techniques of Support Vector Machines (SVM), Classification Trees (CT), Classification Trees with Random Forest (CTRF) and Neural Networks (NN), returning True Prediction Ratios (TPRs) of $75.8\%$, $69.0\%$, $76.2\%$ and $76.0\%$ respectively. Those occasions whereby all four algorithms agree with each other yet disagree with the visual classification (`unanimous disagreement') serves as a potential indicator of human error in classification, occurring in $\sim9\%$ of ellipticals, $\sim9\%$ of Little Blue Spheroids, $\sim14\%$ of early-type spirals, $\sim21\%$ of intermediate-type spirals and $\sim4\%$ of late-type spirals \& irregulars. We observe that the choice of parameters rather than that of algorithms is more crucial in determining classification accuracy. Due to its simplicity in formulation and implementation, we recommend the CTRF algorithm for classifying future galaxy datasets. Adopting the CTRF algorithm, the TPRs of the 5 galaxy types are : E, $70.1\%$; LBS, $75.6\%$; S0-Sa, $63.6\%$; Sab-Scd, $56.4\%$ and Sd-Irr, $88.9\%$. Further, we train a binary classifier using this CTRF algorithm that divides galaxies into spheroid-dominated (E, LBS \& S0-Sa) and disk-dominated (Sab-Scd \& Sd-Irr), achieving an overall accuracy of $89.8\%$. This translates into an accuracy of $84.9\%$ for spheroid-dominated systems and $92.5\%$ for disk-dominated systems.
description: 30 pages, 21 figures, accepted for publication in MNRAS
title: 03_0464
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/
title: Histoire : mutong de disheng
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
title: Space Inventory and Preliminary Marketing Recommendations
Creators: name: (:Unkn) Unknown
Publisher: name: University of Massachusetts Amherst
Year: 1995
Subjects: subject: Waterfront
subject: Architecture
subject: FOS: Civil engineering
subject: Yankee Publishing
subject: Economic History
subject: Economics
subject: Growth and Development
subject: Public Economics
subject: Public Policy
subject: Urban, Community and Regional Planning
subject: Urban Studies
subject: Urban Studies and Planning

description: The Center for Economic Development at the University of Massachusetts, in Amherst, is part of the Landscape Architecture and Regional Planning Department, and is funded by the Economic Development Administration of the U.S. Department of Commerce, and the University of Massachusetts.
description: This report was designed to assist further economic development of Gloucester, Massachusetts’s working waterfront and downtown commercial district. This market and economic development plan was meant to provide the Gloucester Community Development Office with some key ingredients for the success of their overall economic revitalization plan that was being prepared for the entire city.
Chromospheric Inversions of a Micro-flaring Region
Creators: name: Reid, A.
name: Henriques, V.
name: Mathioudakis, M.
name: Doyle, J. G.
name: Ray, T.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We use spectropolarimetric observations of the Ca II 8542~Å line, taken from the Swedish 1-m Solar Telescope (SST), in an attempt to recover dynamic activity in a micro-flaring region near a sunspot via inversions. These inversions show localized mean temperature enhancements of $\sim$1000~K in the chromosphere and upper photosphere, along with co-spatial bi-directional Doppler shifting of 5 - 10 km s$^{-1}$. This heating also extends along a nearby chromospheric fibril, co-spatial to 10 - 15 km s$^{-1}$ down-flows. Strong magnetic flux cancellation is also apparent in one of the footpoints, concentrated in the chromosphere. This event more closely resembles that of an Ellerman Bomb (EB), though placed slightly higher in the atmosphere than is typically observed.
description: 9 pages, 9 figures, accepted in ApJ. Movies are stored here: https://star.pst.qub.ac.uk/webdav/public/areid/Microflare/
The fate of vacancy-induced supersolidity in 4He
Creators: name: Boninsegni, Massimo
name: Kuklov, Anatoly
name: Pollet, Lode
name: Prokof'ev, Nikolay
name: Svistunov, Boris
name: Troyer, Matthias
Publisher: name: arXiv
Year: 2006
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: The supersolid state of matter, exhibiting non-dissipative flow in solids, has been elusive for thirty five years. The recent discovery of a non-classical moment of inertia in solid 4He by Kim and Chan provided the first experimental evidence, although the interpretation in terms of supersolidity of the ideal crystal phase remains subject to debate. Using quantum Monte Carlo methods we investigate the long-standing question of vacancy-induced superflow and find that vacancies in a 4He crystal phase separate instead of forming a supersolid. On the other hand, non-equilibrium vacancies relaxing on defects of poly-crystalline samples could provide an explanation for the experimental observations.
description: 4 pages,4 figures. Replaced with published version
A project based on Multi-Configuration Dirac-Fock calculations for plasma spectroscopy
Creators: name: Comet, Maxime
name: Pain, Jean-Christophe
name: Gilleron, Franck
name: Piron, Robin
Publisher: name: arXiv
Year: 2017
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We present a project dedicated to hot plasma spectroscopy based on a Multi-Configuration Dirac-Fock (MCDF) code, initially developed by J. Bruneau. The code is briefly described and the use of the transition-state method for plasma spectroscopy is detailed. Then an opacity code for local-thermodynamic-equilibrium plasmas using MCDF data, named OPAMCDF, is presented. Transition arrays for which the number of lines is too large to be handled in a Detailed-Line-Accounting calculation can be modeled within the Partially-Resolved-Transition-Array method or using the Unresolved-Transition-Arrays formalism in jj-coupling. An improvement of the original Partially-Resolved-Transition-Array method is presented which gives a better agreement with Detailed-Line-Accounting computations. Comparisons with some absorption and emission experimental spectra are shown. Finally, the capability of the MCDF code to compute atomic data required for collisional-radiative modeling of plasma at non local thermodynamic equilibrium is illustrated. Additionally to photoexcitation, this code can be used to calculate photoionization, electron impact excitation and ionization cross-sections as well as autoionization rates in the Distorted-Wave or Close Coupling approximations. Comparisons with cross-sections and rates available in the literature are discussed.
description: submitted to High Energy Density Physics
Renormalization-group improved effective potential for gauge theories in curved spacetime
Creators: name: Elizalde, E.
name: Odintsov, S. D.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The renormalization-group improved effective potential for an arbitrary renormalizable massless gauge theory in curved spacetime is found,thus generalizing Coleman-Weinberg's approach corresponding to flat space.Some explicit examples are considered,among of them:scalar self-interacting theory,scalar electrody namics,the asymptotically-free SU(2) gauge model,and the SU(5) GUT theory. The possibility of curvature-induced phase transitions is analyzed.It is shown that such a phase transition may take place in a SU(5) inflationary universe.The inclusion of quantum gravity effects isbriefly discussed.
description: Latex file,11pages
Additional file 2: of Results of a feasibility cluster randomised controlled trial of a peer-led school-based intervention to increase the physical activity of adolescent girls (PLAN-A)
Creators: name: Sebire, Simon
name: Jago, Russell
name: Banfield, Kathryn
name: Edwards, Mark
name: Campbell, Rona
name: Kipping, Ruth
name: Blair, Peter
name: Bryar Kadir
name: Garfield, Kirsty
name: Matthews, Joe
name: Lyons, Ronan
name: Hollingworth, William
Publisher: name: figshare
Year: 2018
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy

description: Template for Intervention Description and Replication (TIDieR) checklist for PLAN-A.Completed TIDieR Checklist describing the PLAN-A intervention. (DOCX 16 kb)
Observational signatures of cloud-cloud collision in the extended star-forming region S235
Creators: name: Dewangan, L. K.
name: Ojha, D. K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a multi-wavelength data analysis of the extended star-forming region S235 (hereafter E-S235), where two molecular clouds are present. In E-S235, using the 12CO (1-0) and 13CO (1-0) line data, a molecular cloud linked with the site "S235main" is traced in a velocity range [-24, -18] km s^{-1}, while the other one containing the sites S235A, S235B, and S235C (hereafter "S235ABC") is depicted in a velocity range [-18, -13] km s^{-1}. In the velocity space, these two clouds are separated by ~4 km s^{-1}, and are interconnected by a lower intensity intermediate velocity emission, tracing a broad bridge feature. In the velocity channel maps, a possible complementary molecular pair at [-21, -20] km s^{-1} and [-16, -15] km s^{-1} is also evident. The sites, "S235ABC", East 1, and South-West are spatially seen in the interface of two clouds. Together, these observed features are consistent with the predictions of numerical models of the cloud-cloud collision (CCC) process, favoring the onset of the CCC in E-S235 about 0.5 Myr ago. Deep UKIDSS near-infrared photometric analysis of point-like sources reveals significant clustering of young stellar populations toward the sites located at the junction, and the "S235main". The sites, "S235ABC" harbor young compact H II regions having dynamical ages of ~0.06-0.22 Myr, and these sites (including South-West and East 1) also contain dust clumps (having M_clump ~40 to 635 M_sun). Our observational findings suggest that the star formation activities (including massive stars) appear to be influenced by the CCC mechanism at the junction.
description: 16 pages, 12 figures, Accepted for publication in The Astrophysical Journal
The MACHO Project Hubble Space Telescope Follow-Up: Preliminary Results on the Location of the Large Magellanic Cloud Microlensing Source Stars
Creators: name: Alcock, C.
name: Allsman, R. A.
name: Alves, D. R.
name: Axelrod, T. S.
name: Becker, A. C.
name: Bennett, D. P.
name: Cook, K. H.
name: Dalal, N.
name: Drake, A. J.
name: Freeman, K. C.
name: Geha, M.
name: Griest, K.
name: Lehner, M. J.
name: Marshall, S. L.
name: Minniti, D.
name: Nelson, C. A.
name: Peterson, B. A.
name: Popowski, P.
name: Pratt, M. R.
name: Quinn, P. J.
name: Stubbs, C. W.
name: Sutherland, W.
name: Tomaney, A. B.
name: Vandehei, T.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We attempt to determine whether the MACHO microlensing source stars are drawn from the average population of the LMC or from a population behind the LMC by examining the HST color-magnitude diagram (CMD) of microlensing source stars. We present WFPC2 HST photometry of eight MACHO microlensing source stars and the surrounding fields in the LMC. The microlensing source stars are identified by deriving accurate centroids in the ground-based MACHO images using difference image analysis (DIA) and then transforming the DIA coordinates to the HST frame. We consider in detail a model for the background population of source stars based on that presented by Zhao, Graff & Guhathakurta. In this model, the source stars have an additional reddening = 0.13 mag and a slightly larger distance modulus ~ 0.3 mag than the average LMC population. We also investigate a series of source star models, varying the relative fraction of source stars drawn from the average and background populations and the displacement of the background population from the LMC. Due to the small number of analyzed events the distribution of probabilities of different models is rather flat. A shallow maximum occurs at a fraction s_LMC ~ 0.8 of the source stars in the LMC. This is consistent with the interpretation that a significant fraction of observed microlensing events are due to lenses in the Milky Way halo, but does not definitively exclude other models.
description: revised version, results slightly changed, accepted by ApJ
title: Histoire : qianshang he xiaotou
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Bayesian Reconstraction with Adaptive Image Notion
Creators: name: Guglielmetti, Fabrizia
Publisher: name: Zenodo
Year: 2019

description: Bayesian probability theory is employed to provide a stable and unique solution to the ill-posed inverse problem of image analysis applied to ALMA calibrated interferometric data sets. The novel algorithm, Bayesian Reconstruction with Adaptive Image Notion (BRAIN), is under development aiming at detecting the weak signal in the presence of varying noise also in extreme cases as sparse data and mosaic of images. The technique makes use of Gaussian statistics for a joint source detection and background estimation through a probabilistic mixture-model technique. Statistics is rigorously applied throughout the algorithm, so pixels with low intensity can be handled optimally and accurately, without binning and loss of resolution. BRAIN makes use of a 2D adaptive kernel deconvolution method to prevent spurious signal that may arise from the deconvolution process of the dirty image from the well-known dirty beam. Continuum, emission and absorption lines detection occurs without an explicit subtraction. An automated decision in the separation between different kind of signals is developed while minimizing spurious detections. BRAIN has the objective to become a new CASA task. Preliminary results are shown on the application of BRAIN to ALMA simulated data.
title: 02_1181
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: Laboratoire de Médiévistique Occidentale de Paris
subject: LaMOP

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/
Additional file 1: of The inference of gray whale (Eschrichtius robustus) historical population attributes from whole-genome sequences
Creators: name: Brüniche-Olsen, Anna
name: Westerman, Rick
name: Kazmierczyk, Zuzanna
name: Vertyankin, Vladimir
name: Celine Godard-Codding
name: Bickham, John
name: J. DeWoody
Publisher: name: figshare
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: Computational Biology

description: Table S1. Information on raw reads filtering statistics. Paired-end libraries were sequenced on an Illumina HiSeq 2500. Table S2. Environmental variables used in AQUAMAPS to generate maps of suitable habitat for gray whales during the Holocene. Table S3. The D–test statistic evaluates the number (n) of ABBA and BABA sites (D = (nABBA - nBABA) / (nABBA + nBABA)) and D 0 indicates that P2 is more closely related to P3 than P1. The significance of the D test was evaluated with a Z-score, where |Z-scores| > 3 was used as the critical value for a significant test. Figure S1. Inferred effective population sizes (Ne) over time. Estimates are averages based on 11 autosomal scaffolds larger than 30 Mb. A substitution rate of a) 10 × 10− 10 bp− 1 year− 1 and b) 1.5 × 10− 10 bp− 1 year− 1 were used. (DOCX 446 kb)
title: Histoire : shenqi de feitan
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Supplementary Material: Detailed examples and proofs from Unstable cores are the source of instability in chemical reaction networks
Creators: name: Vassena, Nicola
name: Stadler, Peter F.
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 340699
subject: Physical chemistry not elsewhere classified
classificationCode: 490199
subject: Applied mathematics not elsewhere classified
classificationCode: 490303
subject: Numerical solution of differential and integral equations
classificationCode: 490409
subject: Ordinary differential equations, difference equations and dynamical systems
classificationCode: 490410
subject: Partial differential equations

description: The file integrates the main text (i) by providing a thorough discussion of the examples presented in the main text, (ii) by including all detailed proofs of cited results in the present paper's setting, (iii) by expanding on generalized-unstable-feedbacks: a minor point in the main text.
Water lines and multiple ring and gap structures of the protoplanetary disk around HD 163296
Creators: name: Notsu, Shota
Publisher: name: Zenodo
Year: 2019

description: Observationally locating the position of the H2O snowline (=the sublimation front of water molecules) in protoplanetary disks is crucial because it will constrain the dust-grain evolution and planet formation, and the origin of water on terrestrial planets. Water lines from disks have been detected through recent space infrared spectroscopic observations, such as Spitzer and Herschel. However, these lines mainly trace the disk surface and the cold water reservoir outside the H2O snowline. In our previous papers (Notsu et al. 2016&2017&2018, ApJ), on the basis of our calculations of disk chemical structures and water line profiles, we proposed how to identify the position of the H2O snowline in the disk midplane by analyzing the Keplerian profiles of water lines, which can be obtained by high-dispersion spectroscopic observations across a wide range of wavelengths. We concluded that water lines that have small Einstein A coefficients and relatively high excitation energies trace the hot water gas inside the H2O snowline. In ALMA Cycle 3, we conducted the high-spatial resolution continuum and water line observations at Band 7 for the disk around the Herbig Ae star HD163296 (Notsu et al. 2019, ApJ, 875, 96). The targeted lines are considered to be the candidate submillimeter water lines to locate the position of the H2O snowline, on the basis of our model calculations. We compared the upper limit fluxes with the values calculated by our model calculations with dust emission included, and we constrained the line emitting region (the position of the H2O snowline) and the dust opacities from the observations. We conclude that, if the outer edge of the region with a high water abundance and the position of the water snowline are both beyond 8 au, then the millimeter dust opacity will have a value larger than 2.0 cm^2 g^-1. In addition, the position of the water snowline must lie inside 20 au if the millimeter dust opacity is 2.0 cm^2 g^-1. Moreover, we also reported multiple ring and gap patterns in the Band 7 dust continuum emission with around 15 au resolution. The positions of bright rings and dust depleted dark gaps are consistent with those indicated by the previous ALMA observations (e.g., Isella et al. 2016, 2018). Future observations of the dust continuum emission at higher angular resolution and water lines with longer observation time are required to clarify the detailed structures and the position of the H2O snowline in the disk midplane
Finite element approach for simulating quantum electron dynamics in a magnetic field
Creators: name: Watanabe, Naoki
name: Tsukada, Masaru
Publisher: name: arXiv
Year: 2000
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: A fast and stable numerical method is formulated to compute the time evolution of a wave function in a magnetic field by solving the time-dependent Schroedinger equation. This computational method is based on the finite element method in real space to improved accuracy without any increase of computational cost. This method is also based on Suzuki's exponential product theory to afford an efficient way to manage the TD-Schroedinger equation with a vector potential. Applying this method to some simple electron dynamics, we have confirmed its efficiency and accuracy.
description: 7 pages, 30 eps figures
Mobility in excess of $10^{6}$ cm$^2$/Vs in InAs quantum wells grown on lattice mismatched InP substrates
Creators: name: Hatke, A. T.
name: Wang, T.
name: Thomas, 2 C.
name: Gardner, G.
name: Manfra, M. J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: InAs-based two-dimensional electron systems grown on lattice mismatched InP substrates offer a robust platform for the pursuit of topologically protected quantum computing. We investigated strained composite quantum wells of In$_{0.75}$Ga$_{0.25}$As/InAs/In$_{0.75}$Ga$_{0.25}$As with In$_{0.75}$Al$_{0.25}$As barriers. By optimizing the widths of the In$_{0.75}$Ga$_{0.25}$As layers, the In$_{0.75}$Al$_{0.25}$As barrier, and the InAs quantum well we demonstrate mobility in excess of $1 \times 10^{6}\,$cm$^{2}/$Vs. Mobility vs. density data indicates that scattering is dominated by a residual three dimensional distribution of charged impurities. We extract the Rashba parameter and spin-orbit length as important material parameters for investigations involving Majorana zero modes.
Collaboration in the context of industry convergence - an overview
Creators: name: Kohut, Magdalena
Publisher: name: Institut für betriebswirtschaftliches Management im Fachbereich Chemie und Pharmazie
Year: 2019
Subjects: subject: 330 Economics

description: Recent literature on organizational features and activities along the phases of convergent value chains is gathered in a classification framework. It is emphasized that within convergent value chains organizations lack certain competences and hence need to collaborate in order to close their competence gaps. These collaborations are also discussed in regard to the intensity of resource and competence integration, ranging from licensing agreements to mergers and acquisitions. Strategic alliances, joint ventures as well as mergers and acquisitions in the biotechnology sector undergoing convergent processes are analyzed over the 20-year period, 1997-2016. Subsequently, the biopharmaceutical sector is chosen as a convergent industry case example and its value chain analyzed using the classification framework developed. The position of the incumbent firms is shown to shift from spanning the entire value chain in a fully-integrated business model, to being pushed towards the market end of the value chain by the industry new entrants, to finally trying to regain a stronger position by adapting a coordinating hub business model.
WZW-Toda Reduction using the Casimir Operator
Creators: name: Jack, I.
name: Panvel, J.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We construct a quantum Hamiltonian operator for the Wess-Zumino-Witten (WZW) model in terms of the Casimir operator. This facilitates the discussion of the reduction of the WZW model to Toda field theory at the quantum level and provides a very straightforward derivation of the quantum central charge for the Toda field theory.
description: 16pp, uses harvmac, LTH 304 (Revised version with improved discussion of non-perturbative effects)
title: Histoire : sWNgWrmABja2
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Iterative Supervised Principal Components
Creators: name: Piironen, Juho
name: Vehtari, Aki
Publisher: name: arXiv
Year: 2017
Subjects: subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences

description: In high-dimensional prediction problems, where the number of features may greatly exceed the number of training instances, fully Bayesian approach with a sparsifying prior is known to produce good results but is computationally challenging. To alleviate this computational burden, we propose to use a preprocessing step where we first apply a dimension reduction to the original data to reduce the number of features to something that is computationally conveniently handled by Bayesian methods. To do this, we propose a new dimension reduction technique, called iterative supervised principal components (ISPC), which combines variable screening and dimension reduction and can be considered as an extension to the existing technique of supervised principal components (SPCs). Our empirical evaluations confirm that, although not foolproof, the proposed approach provides very good results on several microarray benchmark datasets with very affordable computation time, and can also be very useful for visualizing high-dimensional data.
Additional file 18: of Proteomic analysis of Medulloblastoma reveals functional biology with translational potential
Creators: name: Rivero-Hinojosa, Samuel
name: Lau, Ling
name: Stampar, Mojca
name: Staal, Jerome
name: Huizhen Zhang
name: Gordish-Dressman, Heather
name: Northcott, Paul
name: Pfister, Stefan
name: Taylor, Michael
name: Brown, Kristy
name: Rood, Brian
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Figure S10. EIF4 inhibitor concentration dependent cell death in medulloblastoma cells. a) MB002, MB004 and D556 cells were treated with the EIF4F inhibitors 4E1RCat for 72Â h at the indicated concentrations. In all cell lines we found concentration-dependent cell death when treated with EIF4F inhibitors. D556 at normal (10ûS) and nutrient deprivation (2% FBS) conditions (b) and D556 and primary human cerebellar astrocytes cells (c) were treated with the EIF4F inhibitor 4E1RCat for 72Â h at the indicated concentrations. Error bars indicate the standard variation deviation. d) Treatment of D556 and primary human cerebellar astrocytes cells with 4E1RCat in combination with cisplatin at the indicated concentrations. (PDF 975 kb)
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Cart. 192 (11 H 77), 295 folios, f. 0080v
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0080v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0080v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Additional file 1: of Results of a feasibility cluster randomised controlled trial of a peer-led school-based intervention to increase the physical activity of adolescent girls (PLAN-A)
Creators: name: Sebire, Simon
name: Jago, Russell
name: Banfield, Kathryn
name: Edwards, Mark
name: Campbell, Rona
name: Kipping, Ruth
name: Blair, Peter
name: Bryar Kadir
name: Garfield, Kirsty
name: Matthews, Joe
name: Lyons, Ronan
name: Hollingworth, William
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy

description: Consort 2010 extension for pilot and feasibility trials checklist. Completed CONSORT checklist (version adapted for reporting pilot and feasibility studies). (DOC 225 kb)