cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1 of Participation of women in the health workforce in the fragile and conflict-affected countries: a scoping review
Creators: name: Ayaz, Basnama
name: Martimianakis, Maria Athina
name: Muntaner, Carles
name: Nelson, Sioban
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Biotechnology
Science Policy

description: Additional file 1. Sex-segregated data from global health observatory, WHO for the identified FCASs in different years.
Ages of A-type Vega-like stars from uvby$β$ Photometry
Creators: name: Song, Inseok
name: Caillault, J. -P.
name: Navascués, David Barrado y
name: Stauffer, John R.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have estimated the ages of a sample of A-type Vega-like stars by using Strömgren \emph{uvby$β} photometric data and theoretical evolutionary tracks. We find that 13 percent of these A stars have been reported as Vega-like stars in the literature and that the ages of this subset run the gamut from very young (50~Myr) to old (1~Gyr), with no obvious age difference compared to those of field A stars. We clearly show that the fractional IR luminosity decreases with the ages of Vega-like stars.
description: 4pages text, 3 tables, 3 figures, Accepted in ApJ
Shadow bands in single-layered Bi_2Sr_2CuO_6 studied by angle-resolved photoemission spectroscopy
Creators: name: Nakayama, K.
name: Sato, T.
name: Dobashi, T.
name: Terashima, K.
name: Souma, S.
name: Matsui, H.
name: Takahashi, T.
name: Campuzano, J. C.
name: Kudo, K.
name: Sasaki, T.
name: Kobayashi, N.
name: Kondo, T.
name: Takeuchi, T.
name: Kadowaki, K.
name: Kofu, M.
name: Hirota, K.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We have performed systematic angle-resolved photoemission spectroscopy (ARPES) on single-layered cuprate superconductor Bi2Sr2CuO6 to elucidate the origin of shadow band. We found that the shadow band is exactly the c(2x2) replica of the main band irrespective of the carrier concentration and its intensity is invariable with respect to temperature, doping, and substitution constituents of block layers. This result rules out the possibility of antiferromagnetic correlation and supports the structural origin of shadow band. ARPES experiments on optimally doped La1.85Sr0.15CuO4 also clarified the existence of the c(2x2) shadow band, demonstrating that the shadow band is not a unique feature of Bi-based cuprates. We conclude that the shadow band is related to the orthorhombic distortion at the crystal surface.
description: 6 pages, 4figures
Print versus digital reading preferences of university students in Australia
Creators: name: Johnston, Nicole
name: Salaz, A. M.
Publisher: name: Carnegie Mellon University
Year: 2018
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences
subject: 130103 Higher Education
subject: FOS: Educational sciences

description: This paper presents findings of a survey that investigated the reading preferences of university students at Edith Cowan University (ECU) in Perth, Australia. This survey is being undertaken as part of the Academic Reading Format International Study (ARFIS), which is investigating print versus digital reading preferences in 31 countries. A total of 582 students completed the survey. Results from the survey indicate a strong preference for reading in print because of issues such as eyestrain, tactile features, better focus, and an ability to highlight and take notes. Issues such as cost, usability, and accessibility also impacted on students' reading decisions.

Presented at VALA 2018, Melbourne, Australia
The Rotation of M Dwarfs Observed by the Apache Point Galactic Evolution Experiment
Creators: name: Gilhool, Steven H.
name: Blake, Cullen H.
name: Terrien, Ryan C.
name: Bender, Chad
name: Mahadevan, Suvrath
name: Deshpande, Rohit
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the results of a spectroscopic analysis of rotational velocities in 714 M dwarf stars observed by the SDSS III Apache Point Galactic Evolution Experiment (APOGEE) survey. We use a template fitting technique to estimate $v\sin{i}$ while simultaneously estimating $\log{g}$, $[\text{M}/\text{H}]$, and $T_{\text{eff}}$. We conservatively estimate that our detection limit is 8 km s$^{-1}$. We compare our results to M dwarf rotation studies in the literature based on both spectroscopic and photometric measurements. Like other authors, we find an increase in the fraction of rapid rotators with decreasing stellar temperature, exemplified by a sharp increase in rotation near the M$4$ transition to fully convective stellar interiors, which is consistent with the hypothesis that fully convective stars are unable to shed angular momentum as efficiently as those with radiative cores. We compare a sample of targets observed both by APOGEE and the MEarth transiting planet survey and find no cases were the measured $v\sin{i}$ and rotation period are physically inconsistent, requiring $\sin{i}>1$. We compare our spectroscopic results to the fraction of rotators inferred from photometric surveys and find that while the results are broadly consistent, the photometric surveys exhibit a smaller fraction of rotators beyond the M$4$ transition by a factor of $\sim 2$. We discuss possible reasons for this discrepancy. Given our detection limit, our results are consistent with a bi-modal distribution in rotation that is seen in photometric surveys.
description: 31 pages, 11 figures, 4 tables. Accepted for publication by AJ
Research Data and Software Management Policy of Vrije Universiteit Amsterdam
Creators: name: Scholten, Jolien
name: Bosch, Sander Erik
name: Heijnen, Sam
name: Hofstra, Tycho
name: Ras, Marcel
name: Vermaas, Meron
name: Unger, Dimitri
Publisher: name: Zenodo
Year: 2025
Subjects: Research Data Management
Research Software Management
Open Science
FAIR data
Data stewardship
policy
Vrije Universiteit Amsterdam

description: The Research Data and Software Management Policy of Vrije Universiteit Amsterdam articulates how to handle research data and software at this Dutch university. The policy lists the responsibilities regarding research data and software management for researchers, department heads, faculty boards and the university as a whole.

This version of the policy (3.0) was approved by the VU Executive Board on December 17, 2024.

This university-wide policy is worked out in more detailed policies and guidelines at faculty level.
Coherent States, Dynamics and Semiclassical Limit on Quantum Groups
Creators: name: Aref'eva, I. Ya.
name: Parthasarathy, R.
name: Viswanathan, K. S.
name: Volovich, I. V.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Coherent states on the quantum group $SU_q(2)$ are defined by using harmonic analysis and representation theory of the algebra of functions on the quantum group. Semiclassical limit $q\rightarrow 1$ is discussed and the crucial role of special states on the quantum algebra in an investigation of the semiclassical limit is emphasized. An approach to $q$-deformation as a $q$-Weyl quantization and a relavence of contact geometry in this context is pointed out. Dynamics on the quantum group parametrized by a real time variable and corresponding to classical rotations is considered.
description: 20 pages in latex, SFU-HEP-108-93
Medium response in JEWEL and its impact on jet shape observables in heavy ion collisions
Creators: name: Elayavalli, Raghav Kunnawalkam
name: Zapp, Korinna Christine
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Realistic modeling of medium-jet interactions in heavy ion collisions is becoming increasingly important to successfully predict jet structure and shape observables. In JEWEL, all partons belonging to the parton showers initiated by hard scattered partons undergo collisions with thermal partons from the medium, leading to both elastic and radiative energy loss. The recoiling medium partons carry away energy and momentum from the jet. Since the thermal component of these recoils' momenta is part of the soft background activity, comparison with data requires the implementation of a subtraction procedure. We present two independent procedures through which background subtraction can be performed and discuss the impact of the medium recoil on jet shape observables. Keeping track of the medium response significantly improves the JEWEL description of jet shape measurements.
description: 23 pages, 16 figures
Additional file 2 of Participation of women in the health workforce in the fragile and conflict-affected countries: a scoping review
Creators: name: Ayaz, Basnama
name: Martimianakis, Maria Athina
name: Muntaner, Carles
name: Nelson, Sioban
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Biotechnology
Science Policy

description: Additional file 2. World Bank’s (WB) harmonized lists of FCASs for 2018 and 2019.
Fracture and Fatigue Mechanism of Cast Iron Water Mains
Creators: name: RUI JIANG
Publisher: name: Monash University
Year: 2018
Subjects: subject: 90505 Infrastructure Engineering and Asset Management
subject: FOS: Civil engineering
subject: 90501 Civil Geotechnical Engineering
subject: 90509 Water Resources Engineering
subject: 90506 Structural Engineering

description: Cast iron pipelines buried between the 1840s and 1980s account for a significant proportion of urban water supply systems. Bursts of large-diameter cast iron water mains cause extensive financial losses and impacts on transportation and society. This study introduced methodologies to quantify the impact of cyclic pressures on corroded pipes and leak-before-break analysis for preventing pipe bursts.
On the Mass-Donating Star in GRS 1915+105
Creators: name: Eikenberry, Stephen S.
name: Bandyopadhyay, Reba M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an analysis of constraints on the companion mass for the Galactic microquasar GRS 1915+105. Using the known inclination angle and stability of the jet axis, we can rule out massive ($M_s \ga 3 M_{\sun}$) companions with orbital axes not aligned with the jet axis. For an aligned orbital axis, we constrain the ratio of the stellar radius to the binary semi-major axis to be $R_s/a <0.342$, based on the lack of X-ray eclipses. We then show that these constraints together with the X-ray luminosity, approximate black hole mass, and observations of the X-ray absorbing column density towards GRS 1915+105 rule out accretion via stellar wind from a massive companion, implying that accretion occurs via Roche-lobe overflow. In that case, the constraint on $R_s/a$ rules out any companion with $M_s > 19.4 M_{\sun}$ for a black hole mass of $M_{BH} \simeq 30 M_{\sun}$. The lack of significant X-ray reprocessing in the infrared from GRS 1915+105 also provides constraints on the mass and temperature range of a Roche-lobe-filling mass donor.
description: 18 pages, including 2 figures; to appear in ApJ Letters
The infrared-radio correlation of spheroid- and disc-dominated star-forming galaxies to z $\sim$ 1.5 in the COSMOS field
Creators: name: Molnar, Daniel Cs.
name: Sargent, Mark T.
name: Delhaize, Jacinta
name: Delvecchio, Ivan
name: Smolcic, Vernesa
name: Novak, Mladen
name: Schinnerer, Eva
name: Zamorani, Giovanni
name: Bondi, Marco
name: Herrera-Ruiz, Noelia
name: Murphy, Eric J.
name: Vardoulaki, Eleni
name: Karim, Alexander
name: Leslie, Sarah
name: Magnelli, Benjamin
name: Carollo, C. Marcella
name: Middelberg, Enno
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Using infrared data from the Herschel Space Observatory and Karl G. Jansky Very Large Array (VLA) 3 GHz observations in the COSMOS field, we investigate the redshift evolution of the infrared-radio correlation (IRRC) for star-forming galaxies (SFGs) we classify as either spheroid- or disc-dominated based on their morphology. The sample predominantly consists of disc galaxies with stellar mass ${\gtrsim}10^{10}\,M_{\odot}$, and residing on the star-forming main sequence (MS). After the removal of AGN using standard approaches, we observe a significant difference between the redshift-evolution of the median IR/radio ratio $\overline{q}_{\mathrm{TIR}}$ of (i) a sample of ellipticals, plus discs with a substantial bulge component (`spheroid-dominated' SFGs) and, (ii) virtually pure discs and irregular systems (`disc-dominated' SFGs). The spheroid-dominated population follows a declining $\overline{q}_{\mathrm{TIR}}$ vs. $z$ trend similar to that measured in recent evolutionary studies of the IRRC. However, for disc-dominated galaxies, where radio and IR emission should be linked to star formation in the most straightforward way, we measure very little change in $\overline{q}_{\mathrm{TIR}}$. This suggests that low-redshift calibrations of radio emission as an SFR-tracer may remain valid out to at least $z\,{\simeq}\,1\,{-}\,1.5$ for pure star-forming systems. We find that the different redshift-evolution of $q_{\rm TIR}$ for the spheroid- and disc-dominated sample is mainly due to an increasing radio excess for spheroid-dominated galaxies at $z\,{\gtrsim}\,$0.8, hinting at some residual AGN activity in these systems. This finding demonstrates that in the absence of AGN the IRRC is independent of redshift, and that radio observations can therefore be used to estimate SFRs at all redshifts for genuinely star-forming galaxies.
description: Resubmitted to MNRAS after addressing reviewer feedback
Rotational Energy Transfer in H2+H2
Creators: name: Sultanov, Renat A.
name: Guster, Dennis
Publisher: name: arXiv
Year: 2006
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: FOS: Physical sciences

description: Quantum-mechanical close-coupling calculations for state-to-state cross sections and thermal rates are reported for H2+H2 collisions. Two recently developed potential energy surfaces (PES) for the H2-H2 system are applied, namely, the global potential surface from the work of A.I. Boothroyd, P.G. Martin, W.J. Keogh, M.J. Peterson, J. Chem. Phys., 116 (2002) 666, and a restricted, model surface from the works of P. Diep, J.K. Johnson, J. Chem. Phys., 113 (2000) 3480; ibid. 112, 4465. The low temperature limit is investigated. We found significant differences in cross sections and corresponding thermal rates calculated with these two PESs.
description: 4 Figures, 1 Table
Improved Modelling of Long-Span Highway Bridge Traffic Loading
Creators: name: DONG GUO
Publisher: name: Monash University
Year: 2018
Subjects: subject: 90599 Civil Engineering not elsewhere classified
subject: FOS: Civil engineering

description: Traffic load modelling on the bridges plays an important role in the bridge design and assessment, but they are not well represented in the current national standards, especially for long-span bridges. This thesis investigates fundamental aspects of a realistic and efficient modelling of the traffic load in three aspects.
title: 01_2296
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/
Electric Dipole Spin Resonance for Heavy Holes in Quantum Dots
Creators: name: Bulaev, Denis V.
name: Loss, Daniel
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We propose and analyze a new method for manipulation of a heavy hole spin in a quantum dot. Due to spin-orbit coupling between states with different orbital momenta and opposite spin orientations, an applied rf electric field induces transitions between spin-up and spin-down states. This scheme can be used for detection of heavy-hole spin resonance signals, for the control of the spin dynamics in two-dimensional systems, and for determining important parameters of heavy-holes such as the effective $g$-factor, mass, spin-orbit coupling constants, spin relaxation and decoherence times.
description: 5 pages, 3 figures
D2.2: Second Report on Users' Needs
Creators: name: Geser, Guntram
name: Selhofer, Hannes
Publisher: name: Zenodo
Year: 2015
Subjects: subject: Archaeology

description: Background and objectives

This document is a deliverable (D2.2) of the ARIADNE project (“Advanced Research Infrastructure for Archaeological Dataset Networking in Europe”) which is funded under the European Community's Seventh Framework Programme. It presents results of the work carried out in Task 2.1 “Survey of users’ needs and community building”. The foundation of this document is the earlier deliverable D2.1 (First Report on Users’ Needs), which presented the results of a large international online survey among about 700 archaeological researchers and data centre managers.

The main objective of this report is to provide additional, more detailed evidence about user requirements of key target groups (“users”) of the project with regard to the ARIADNE data portal. A panel of about 25 researchers was asked to describe in detail their use of digital data archives, to evaluate existing archives and other portals and to highlight useful features of these portals which could serve as “good practices” when creating a new research data portal. This information shall support the ARIADNE project in taking informed decisions regarding the specification of the e-infrastructure and services so that they are developed in a way that corresponds to perceived and actual research needs. The mandate was to provide evidence on these issues, notably through collecting feed-back from the ARIADNE community by way of a user survey.
Additional file 3 of Participation of women in the health workforce in the fragile and conflict-affected countries: a scoping review
Creators: name: Ayaz, Basnama
name: Martimianakis, Maria Athina
name: Muntaner, Carles
name: Nelson, Sioban
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Biotechnology
Science Policy

description: Additional file 3. PRISMA-ScR checklist.
Spectroscopic data for synthesised compounds from Metal-free selective mono-halodecarboxylation of heteroarenes under mild conditions
Creators: name: Henderson, Scott H.
name: West, Ryan A.
name: Ward, Simon E.
name: Honey, Mark A.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Organic Chemistry
subject: FOS: Chemical sciences
subject: 30306 Synthesis of Materials
subject: 30503 Organic Chemical Synthesis

description: The halodecarboxylation of heteroarene carboxylic acids by treatment with N-bromosuccinimide (NBS) or N-chlorosuccinimide (NCS) was performed. This procedure provides a convenient route to synthetically useful mono-halogenated heteroarene intermediates such as halo-indoles, -aza-indoles, -indazoles and -aza-indazoles. The mild conditions employed and simple protocol provides an advantage over traditional halodecarboxylation procedures that require expensive and toxic metal catalysts, basic conditions, time-consuming intermediate isolation and elevated reaction temperatures.
Relativistic dynamics without conservation laws
Creators: name: Rothenstein, Bernhard
name: Popescu, Stefan
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: We show that relativistic dynamics can be approached without using conservation laws (conservation of momentum, of energy and of the centre of mass). Our approach avoids collisions that are not easy to teach without mnemonic aids. The derivations are based on the principle of relativity and on its direct consequence, the addition law of relativistic velocities.
Additional file 4 of Participation of women in the health workforce in the fragile and conflict-affected countries: a scoping review
Creators: name: Ayaz, Basnama
name: Martimianakis, Maria Athina
name: Muntaner, Carles
name: Nelson, Sioban
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Biotechnology
Science Policy

description: Additional file 4. The search strategy of the review and number of resulted sources from MEDLINE and CINHAL databases.
The importance of anisotropic interstellar turbulence and molecular-cloud magnetic mirrors for galactic cosmic-ray propagation
Creators: name: Chandran, Benjamin D. G.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent studies suggest that when magnetohydrodynamic (MHD) turbulence is excited by stirring a plasma at large scales, the cascade of energy from large to small scales is anisotropic, in the sense that small-scale fluctuations satisfy the inequality k_parallel << k_perp, where k_parallel and k_perp are, respectively, the components of a fluctuation's wave vector parallel and perpendicular to the background magnetic field. Such anisotropic fluctuations are very inefficient at scattering cosmic rays. Results based on the quasilinear approximation for scattering of cosmic rays by anisotropic MHD turbulence are presented and explained. The important role played by molecular-cloud magnetic mirrors in confining and isotropizing cosmic rays when scattering is weak is also discussed.
description: 5 pages, 5 figures. To appear in the Proceedings of the International Space Science Institute (ISSI) Conference on the Astrophysics of Galactic Cosmic Rays, Bern, Switzerland, 2000
Additional file 1 of A quantitative analysis of extension and distribution of lung injury in COVID-19: a prospective study based on chest computed tomography
Creators: name: Pellegrini, Mariangela
name: Larina, Aleksandra
name: Mourtos, Evangelos
name: Frithiof, Robert
name: Lipcsey, Miklos
name: Hultström, Michael
name: Segelsjö, Monica
name: Hansen, Tomas
name: Perchiazzi, Gaetano
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer

description: Additional file 1. For additional information about Materials and methods
Multiplicity fluctuation and correlation of mesons and baryons in ultra-relativistic heavy-ion collisions at LHC
Creators: name: Li, Hai-hong
name: Shao, Feng-lan
name: Song, Jun
Publisher: name: arXiv
Year: 2017
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We study the multiplicity fluctuation and correlation of identified mesons and baryons formed at the hadronization by the quark combination mechanism in the context of ultra-relativistic heavy-ion collisions. Based on the statistical method of free quark combination, we derive the two-hadron multiplicity correlations such as meson-meson and meson-baryon correlations, and take the effects of quark number fluctuation at hadronization into account by a Taylor expansion method. After including the decay contributions, we calculate the dynamical fluctuation observable $ν_{dyn}$ for $\text{K}π$, $pπ$ and $\text{K}p$ pairs and discuss what underlying physics can be obtained by comparing with the data in Pb-Pb collisions at $\sqrt{s_{NN}}=2.76$ TeV and the simulations from HIJING and AMPT event generators.
description: 8 pages, 3 figures
Manual do SysPerf
Creators: name: Lobo, Gilberto
name: Gomes, Raphael
name: Martins, Nathan
Publisher: name: Zenodo
Year: 2023

description: Manual do software SysPerf, uma ferramenta para identificar gargalos e ineficiências na infraestrutura de software, sugerindo melhorias com base em métricas coletadas e análises realizadas. O objetivo é auxiliar os administradores de sistemas na tomada de decisões para aprimorar a infraestrutura.
Table S4 from What is cumulative cultural evolution?
Creators: name: Mesoudi, Alex
name: Thornton, Alex
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 60801 Animal Behaviour

description: Human experimental studies of cumulative cultural evolution that feature our core and extended criteria
Additional file 1 of Hospital nurses’ knowledge regarding older patients: a multicenter study
Creators: name: Derks, Christel T. A. J.
name: Hutten - van den Elsen, Marjo M. G. M.
name: Hakvoort, Lysette J.
name: van Mersbergen, Mariëlle P. J.
name: Schuurmans, Marieke J.
name: Dikken, Jeroen
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Cancer
subject: Science Policy

description: Additional file 1. Number of nurses related to norm group scores on ward and hospital level.
Connecting X-ray absorption and 21cm neutral hydrogen absorption in obscured radio AGN
Creators: name: Moss, V. A.
name: Allison, J. R.
name: Sadler, E. M.
name: Urquhart, R.
name: Soria, R.
name: Callingham, J. R.
name: Curran, S. J.
name: Musaeva, A.
name: Mahony, E. K.
name: Glowacki, M.
name: Farrell, S. A.
name: Bannister, K. W.
name: Chippendale, A. P.
name: Edwards, P. G.
name: Harvey-Smith, L.
name: Heywood, I.
name: Hotan, A. W.
name: Indermuehle, B. T.
name: Lenc, E.
name: Marvil, J.
name: McConnell, D.
name: Reynolds, J. E.
name: Voronkov, M. A.
name: Wark, R. M.
name: Whiting, M. T.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Many radio galaxies show the presence of dense and dusty gas near the active nucleus. This can be traced by both 21cm HI absorption and soft X-ray absorption, offering new insight into the physical nature of the circumnuclear medium of these distant galaxies. To better understand this relationship, we investigate soft X-ray absorption as an indicator for the detection of associated HI absorption, as part of preparation for the First Large Absorption Survey in HI (FLASH) to be undertaken with the Australian Square Kilometre Array Pathfinder (ASKAP). We present the results of our pilot study using the Boolardy Engineering Test Array, a precursor to ASKAP, to search for new absorption detections in radio sources brighter than 1 Jy that also feature soft X-ray absorption. Based on this pilot survey, we detected HI absorption towards the radio source PKS 1657-298 at a redshift of z = 0.42. This source also features the highest X-ray absorption ratio of our pilot sample by a factor of 3, which is consistent with our general findings that X-ray absorption predicates the presence of dense neutral gas. By comparing the X-ray properties of AGN with and without detection of HI absorption at radio wavelengths, we find that X-ray hardness ratio and HI absorption optical depth are correlated at a statistical significance of 4.71σ. We conclude by considering the impact of these findings on future radio and X-ray absorption studies.
description: 22 pages, 20 figures, accepted for publication in MNRAS
Bond electronic polarization induced by spin
Creators: name: Jia, Chenglong
name: Onoda, Shigeki
name: Nagaosa, Naoto
name: Han, Jung Hoon
Publisher: name: arXiv
Year: 2006
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study theoretically the electric polarization induced by noncollinear spin configurations in the limit of strong Hund coupling. We employ a model of two magnetic ions sandwitching an oxygen ion. It is shown that there appears a longitudinal polarization P_x along the bond, which is roughly proportional to (m_r^x)^2-(m_l^x)^2 where m_{r(l)}^x is the x-component of the spin orientation vector at right (left) magnetic ion. A numerical study of the model Hamiltonian yields both longitudinal and transverse electric dipole moments. The transverse polarization is shown to have a non-uniform as well as a uniform component, with the latter being consistent with the previous theory. The longitudinal polarization is non-uniform and oscillating with the period half that of the spin order, but the local magnitude is typically much larger than the uniform transverse polarization and may be detected by X-ray/neutron scattering experiments.
description: 8 pages including 6 figures; discussion on experiments in multiferroics added
Reconstruction of cosmological matter perturbations in Modified Gravity
Creators: name: Gonzalez, J. E.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The analysis of perturbative quantities is a powerful tool to distinguish between different Dark Energy models and gravity theories degenerated at the background level. In this work, we generalise the integral solution of the matter density contrast for General Relativity gravity to a wide class of Modified Gravity (MG) theories. To calculate this solution is necessary prior knowledge of the Hubble rate, the density parameter at the present epoch ($Ω_{m0}$) and the functional form of the effective Newton's constant that characterises the gravity theory. We estimate in a model-independent way the Hubble expansion rate by applying a non-parametric reconstruction method to model-independent cosmic chronometer data and high-$z$ quasar data. In order to compare our generalised solution of the matter density contrast, using the non-parametric reconstruction of $H(z)$ from observational data, with purely theoretical one, we choose a parameterisation of the Screened MG and the $Ω_{m0}$ from WMAP-9 collaborations. Finally, we calculate the growth index for the analysed cases, finding very good agreement between theoretical values and the obtained ones using the approach presented in this work.
description: 8 pages, 3 figures
Special Theory of Relativity through the Doppler Effect
Creators: name: Moriconi, M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: We present the special theory of relativity taking the Doppler effect as the starting point, and derive several of its main effects, such as time dilation, length contraction, addition of velocities, and the mass-energy relation, and assuming energy and momentum conservation, we discuss how to introduce the 4-momentum in a natural way. We also use the Doppler effect to explain the "twin paradox", and its version on a cylinder. As a by-product we discuss Bell's spaceship paradox, and the Lorentz transformation for arbitrary velocities in one dimension.
description: 20 pages, 1 figure
Table S3 from What is cumulative cultural evolution?
Creators: name: Mesoudi, Alex
name: Thornton, Alex
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 60801 Animal Behaviour

description: Evidence for our core and extended criteria in non-human animal studies of cumulative cultural evolution
Statistical Self-Similar Properties of Complex Networks
Creators: name: Lee, Chang-Yong
name: Jung, Sunghwan
Publisher: name: arXiv
Year: 2006
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: It has been shown that many complex networks shared distinctive features, which differ in many ways from the random and the regular networks. Although these features capture important characteristics of complex networks, their applicability depends on the type of networks. To unravel ubiquitous characteristics that complex networks may have in common, we adopt the clustering coefficient as the probability measure, and present a systematic analysis of various types of complex networks from the perspective of statistical self-similarity. We find that the probability distribution of the clustering coefficient is best characterized by the multifractal; moreover, the support of the measure had a fractal dimension. These two features enable us to describe complex networks in a unified way; at the same time, offer unforeseen possibilities to comprehend complex networks.
description: 11 pages, 4 figures
Key Insights from the EuroPotent Therapeutics Summit on HPAPI Trends
Creators: name: ayesha
Publisher: name: Zenodo
Year: 2025

description: The development of HPAPIs involves intricate processes that must balance both effectiveness and safety. Manufacturers are required to implement advanced containment strategies to prevent cross-contamination and protect workers, patients, and the surrounding environment. Cutting-edge containment technologies and rigorous safety procedures are essential to mitigating the risks associated with HPAPI production.

Containment and Cross-Contamination Prevention

Robust containment measures are fundamental in HPAPI manufacturing. Facilities must be designed to prevent the escape of potent compounds, ensuring both personnel safety and product purity. Key strategies include specialized equipment, controlled production environments, and stringent cleaning protocols to reduce cross-contamination risks.

Environmental, Health, and Safety (EHS) Compliance

Due to the high potency of HPAPIs, strict adherence to Environmental, Health, and Safety (EHS) regulations is imperative. Implementing a comprehensive EHS framework ensures regulatory compliance while fostering a strong culture of safety within manufacturing facilities. Essential components of an effective EHS strategy include routine risk assessments, continuous employee training, and ongoing safety monitoring.

EuroPotent Therapeutics Summit

To explore the latest developments and challenges in HPAPI production, the EuroPotent Therapeutics Summit will take place on May 22-23, 2025, in Frankfurt, Germany. This event will bring together industry leaders and experts to discuss regulatory changes, innovative containment technologies, and best practices in HPAPI manufacturing. Attendees will gain valuable insights into the evolving landscape of potent therapeutic development.

Register Now at https://veridonglobal.com/events/europotent-therapeutics-summit/register-europotent/

Conclusion

Manufacturing HPAPIs requires strict containment, proactive cross-contamination control, and unwavering adherence to EHS guidelines. Staying informed through industry events like the EuroPotent Therapeutics Summit offers valuable opportunities to learn from experts and stay connected within this specialized field.
Archives d'enfance (1939-1942). Explorations Journal des voyages. Le Petit Voyageur
Creators: name: Http://Www.Idref.Fr/026708647 Bastaire, Jean (1927-2013)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023

description: Numérisation ICB CollEx-Persée AAP20212022
description: Contient des numéros d'un journal manuscrit créé par Jean Bastaire et ses compagnons de jeu d'enfants ainsi que d'autres documents ayant probablement servi à la rédaction de ce périodique.
description: Source: Fonds Bastaire Université Clermont Auvergne (A1.0388-0403)
description: Relation: http://www.calames.abes.fr/pub/ms/Calames-202012217123954326
description: created: 194007/194109
Charge densities above pulsar polar caps
Creators: name: Jessner, A.
name: Lesch, H.
name: Kunzl, T.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The ability of the neutron star surface to supply all or only part of the charges filling the pulsar magnetosphere is crucial for the physics prevailing within it, with direct consequences for the possible formation of pair creation regions. We evaluate the conditions for $e^-$ emission from pulsar surfaces for a simple Goldreich-Julian geometry taking both thermal and field emission processes into account. Using recently published estimates for the equation of state at the neutron star's surface, we show, that for a large range of $T_{\rm surf}, B$ and $P$, the liberated charges will fully screen the accelerating B-parallel electric field ${\rm E_\|}$. For surface temperatures $T_{\rm surf}<2\cdot 10^5 $K a balance between field emission of electrons and shielding of the field will occur. Even in the overidealised case of $T_{\rm surf}=0$ one can expect a prodigious supply of electrons which will weaken the accelerating ${\rm E_\|}$. We calculated the motion of electrons along selected polar field lines numerically for the low temperature, field emission scenario yielding their Lorentz factors as well as the produced radiation densities. Inverse Compton and later curvature losses are seen to balance the acceleration by the residual electric fields. We found that the conditions for magnetic pair production are not met anywhere along the field lines up to a height of 1500 pulsar radii. We did not {\it a priori} assume an "inner gap", and our calculations did not indicate the formation of one under realistic physical conditions without the introduction of further assumptions.
description: 11 pages, 7 latex figures, accepted for publication in ApJ
Additional file 1: of Sex and cardiovascular disease status differences in attitudes and willingness to participate in clinical research studies/clinical trials
Creators: name: Gruca, Thomas
name: Hottel, Wesley
name: Comstock, Janine
name: Olson, Anna
name: Rosenthal, Gary
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: Science Policy

description: Survey ICTS - V2. (DOCX 22Â kb)
Additional file 2 of Hospital nurses’ knowledge regarding older patients: a multicenter study
Creators: name: Derks, Christel T. A. J.
name: Hutten - van den Elsen, Marjo M. G. M.
name: Hakvoort, Lysette J.
name: van Mersbergen, Mariëlle P. J.
name: Schuurmans, Marieke J.
name: Dikken, Jeroen
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Cancer
subject: Science Policy

description: Additional file 2. Questions of the knowledge about Older Patient – Quiz [15] and percentage of Dutch hospital nurses (n = 1743) who answered the question correct – wrong.
The Origin of the Charge Ordering and Its Relevance to Superconductivity in $θ$-(BEDT-TTF)$_2$X: The Effect of the Fermi Surface Nesting and the Distant Electron-Electron Interactions
Creators: name: Kuroki, Kazuhiko
Publisher: name: arXiv
Year: 2006
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The origin of the charge ordering in organic compounds $θ$-(BEDT-TTF)$_2 X$ ($X=MM'$(SCN)$_4$, $M=$Tl,Rb,Co, $M'=$Cs,Zn) is studied using an extended Hubbard model. Calculating the charge susceptibility within random phase approximation (RPA), we find that the $(3\times 3)\sim (3\times 4)$ charge ordering observed at relatively high temperatures can be considered as a consequence of a cooperation between the Fermi surface nesting, controlled by the hopping integral in the $c$ direction, and the electron-electron interactions, where the distant (next nearest neighbor) interactions that have not been taken into account in most of the previous studies play an important role.Mean field analysis at T=0 also supports the RPA results, and further shows that in the $3\times 3$ charge ordered state, some portions of the Fermi surface remain ungapped and are nested with a nesting vector close to the modulation wave vector of the horizontal stripe ordering observed at low temperatures in $X=MM'$(SCN)$_4$. We further study the possibility of superconductivity by taking into account the distant off-site repulsions and the band structure corresponding to $X=$I$_3$, in which superconductivity is experimentally observed. We find that there is a close competition between $d_{xy}$-wave-like singlet pairing and $p_{x+2y}$-wave-like triplet pairing due to a cooperation between the charge and the spin fluctuations. The present analysis provides a possible unified understanding of the experimental phase diagram of the $θ$-(BEDT-TTF)$_2 X$ family, ranging from a charge ordered insulator to a superconductor.
description: 13 pages, 18 figures (Figs.5,6,7,14,15,18 compressed using jpeg2ps)
A New Model for the Evolution of Light Elements in an Inhomogeneous Galactic Halo
Creators: name: Suzuki, Takeru Ken
name: Yoshii, Yuzuru
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present predictions of the evolution of the light elements, Li, Be, and B, in the early epochs of the Galactic halo, using a model of supernova-induced chemical evolution based on contributions from supernovae (SNe) and cosmic rays (CRs). The most important prediction from our model is that the abundances of light elements in extremely metal-poor stars might be used as age indicators in the very early stages of an evolving halo population, at times when metallicity in most stars are dominated by local metal enrichment due to nearby SN events, and is poorly correlated with age. Our results show that the best ``cosmic clock'' is the $^6$Li abundance. We have derived relationships among various cosmic-ray parameters. Although our model is successful for certain sets of cosmic-ray parameters, larger energy should be absorbed by energetic particles from each SN than required to the current situation of Galactic disk. We discuss an alternative hypothesis of AGN activity in the early Galaxy as another possible accelerator of CRs.
description: ApJ in press, 32 pages including 8 figures (3 fiures, fig.3,5,& 7 in color)
Additional file 1: of Validation of two short questionnaires assessing physical activity in colorectal cancer patients
Creators: name: Henriksen, Hege
name: Berntsen, Sveinung
name: Paur, Ingvild
name: Zucknick, Manuela
name: Skjetne, Anne
name: Bøhn, Siv
name: Henriksen, Christine
name: Smeland, Sigbjørn
name: Carlsen, Monica
name: Blomhoff, Rune
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Physical activity, all participants in total and stratified by sex. Physical activity levels based on Norwegian Food Based Dietary Guideline (i.e. moderate intensity physical activity and vigorous intensity physical activity) are presented in minutes per week as both self-reported by NORDIET-FFQ and objectively measured by SenseWear Armband (SWA). (DOCX 18 kb)
Spin diffusion/transport in $n$-type GaAs quantum wells
Creators: name: Cheng, J. L.
name: Wu, M. W.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: The spin diffusion/transport in $n$-type (001) GaAs quantum well at high temperatures ($\ge120$ K) is studied by setting up and numerically solving the kinetic spin Bloch equations together with the Poisson equation self-consistently. All the scattering, especially the electron-electron Coulomb scattering, is explicitly included and solved in the theory. This enables us to study the system far away from the equilibrium, such as the hot-electron effect induced by the external electric field parallel to the quantum well. We find that the spin polarization/coherence oscillates along the transport direction even when there is no external magnetic field. We show that when the scattering is strong enough, electron spins with different momentums oscillate in the same phase which leads to equal transversal spin injection length and ensemble transversal injection length. It is also shown that the intrinsic scattering is already strong enough for such a phenomena. The oscillation period is almost independent on the external electric field which is in agreement with the latest experiment in bulk system at very low temperature [Europhys. Lett. {\bf 75}, 597 (2006)]. The spin relaxation/dephasing along the diffusion/transport can be well understood by the inhomogeneous broadening, which is caused by the momentum-dependent diffusion and the spin-orbit coupling, and the scattering. The scattering, temperature, quantum well width and external magnetic/electric field dependence of the spin diffusion is studied in detail.
description: 12 pages, 6 figures, to be published in J Appl. Phys
A Large Class of New Gravitational and Axionic Backgrounds for Four-Dimensional Superstrings
Creators: name: Kiritsis, E.
name: Kounnas, C.
name: Lust, D.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A large class of new 4-D superstring vacua with non-trivial/singular geometries, spacetime supersymmetry and other background fields (axion, dilaton) are found. Killing symmetries are generic and are associated with non-trivial dilaton and antisymmetric tensor fields. Duality symmetries preserving N=2 superconformal invariance are employed to generate a large class of explicit metrics for non-compact 4-D Calabi-Yau manifolds with Killing symmetries.
description: LateX file, 34pp., (v5) Some misprints corrected in sections 3.1, 3.2 as pointed out in the paper of Hori and Kapustin (hep-th/0203147). Some comsetic changes also made in the same sections
Additional file 1 of Modelling of soil characteristics as basis for projections of potential future forest ecosystem development under climate change and atmospheric nitrogen deposition
Creators: name: Schlutow, Angela
name: Schröder, Winfried
name: Jenssen, Martin
name: Nickel, Stefan
Publisher: name: figshare
Year: 2021
Subjects: subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 1. Data used and characteristics of modelling regions and modelling sites.