cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Emergence of the Planck Scale
Creators: name: Sidharth, B. G.
Publisher: name: arXiv
Year: 2000
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: In this paper we first observe some interesting parallels between Planck scale considerations and elementary particle Compton wavelength scale considerations, particularly in the context of Wheeler's space time foam and a space time arising out of a stochastic random heap of elementary particles discussed in previous papers. These parallels lead to a semi qualitative picture which shows how the short lived Planck scale arises from the Compton wavelength considerations.
description: 9 pages, TeX
Research Through Design as a Method for Interaction Design Research in HCI
Creators: name: Zimmerman, John
name: Forlizzi, Jodi
name: Evenson, Shelley
Publisher: name: Carnegie Mellon University
Year: 2007
Subjects: Applied Computer Science

description: For years the HCI community has struggled to integrate design in research and practice. While design has gained a strong foothold in practice, it has had much less impact on the HCI research community. In this paper we propose a new model for interaction design research within HCI. Following a research through design approach, designers produce novel integrations of HCI research in an attempt to make the right thing: a product that transforms the world from its current state to a preferred state. This model allows interaction designers to make research contributions based on their strength in addressing under-constrained problems. To formalize this model, we provide a set of four lenses for evaluating the research contribution and a set of three examples to illustrate the benefits of this type of research.
An analytical method to simulate the HI 21-cm visibility signal for intensity mapping experiments
Creators: name: Sarkar, Anjan Kumar
name: Bharadwaj, Somnath
name: Marthi, Visweshwar Ram
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Simulations play a vital role in testing and validating HI 21-cm power spectrum estimation techniques. Conventional methods use techniques like N-body simulations to simulate the sky signal which is then passed through a model of the instrument. This makes it necessary to simulate the HI distribution in a large cosmological volume, and incorporate both the light-cone effect and the telescope's chromatic response. The computational requirements may be particularly large if one wishes to simulate many realizations of the signal. In this paper we present an analytical method to simulate the HI visibility signal. This is particularly efficient if one wishes to simulate a large number of realizations of the signal. Our method is based on theoretical predictions of the visibility correlation which incorporate both the light-cone effect and the telescope's chromatic response. We have demonstrated this method by applying it to simulate the HI visibility signal for the upcoming Ooty Wide Field Array Phase I.
description: 11 pages, 6 figures, MNRAS, stx2344
Additional file 7 of Disruption of ruminal homeostasis by malnutrition involved in systemic ruminal microbiota-host interactions in a pregnant sheep model
Creators: name: Xue, Yanfeng
name: Lin, Limei
name: Hu, Fan
name: Zhu, Weiyun
name: Mao, Shengyong
Publisher: name: figshare
Year: 2020
Subjects: subject: Microbiology
subject: FOS: Biological sciences

description: Additional file 7:. Supplementary Table S3 Gene primers used for quantitative real time-PCR.
Analysis of M-stationary points to an EPEC modeling oligopolistic competition in an electricity spot market
Creators: name: Henrion, René
name: Outrata, Jiří
name: Surowiec, Thomas
Publisher: name: Weierstrass Institute
Year: 2009
Subjects: subject: Equilibrium problems with equilibrium constraints
subject: EPEC
subject: $M$-stationary solutions
subject: electricity spot market
subject: calmness
subject: 90C30
subject: 49J53

description: We consider an equilibrium problem with equilibrium constraints (EPEC) as it arises from modeling competition in an electricity spot market (under ISO regulation). For a characterization of equilibrium solutions, so-called $M$-stationarity conditions are derived. This requires a structural analysis of the problem first (constraint qualifications, strong regularity). Second, the calmness property of a certain multifunction has to be verified in order to justify $M$-stationarity. Third, for stating the stationarity conditions, the co-derivative of a normal cone mapping has to be calculated. Finally, the obtained necessary conditions are made fully explicit in terms of the problem data for one typical constellation. A simple two-settlements example serves as an illustration.
Stable Crank--Nicolson discretisation for incompressible miscible displacement problems of low regularity
Creators: name: Jensen, Max
name: Müller, Rüdiger
Publisher: name: Weierstrass Institute
Year: 2009
Subjects: subject: discontinuous Galerkin
subject: low regularity
subject: Crank-Nicolson
subject: 65M60
subject: 65M12
subject: 76S05

description: In this article we study the numerical approximation of incompressible miscible displacement problems with a linearised Crank-Nicolson time discretisation, combined with a mixed finite element and discontinuous Galerkin method. At the heart of the analysis is the proof of convergence under low regularity requirements. Numerical experiments demonstrate that the proposed method exhibits second-order convergence for smooth and robustness for rough problems.
Solar flare radio pulsations as a signature of dynamic magnetic reconnection
Creators: name: Kliem, B.
name: Karlicky, M.
name: Benz, A. O.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Decimetric radio observations of the impulsive solar flare on October 5, 1992, 09:25 UT show a long series of quasi-periodic pulsations deeply modulating a continuum in the 0.6-2 GHz range that is slowly drifting toward lower frequencies. We propose a model in which the pulsations of the radio flux are caused by quasi-periodic particle acceleration episodes that result from a dynamic phase of magnetic reconnection in a large-scale current sheet. The reconnection is dominated by repeated formation and subsequent coalescence of magnetic islands (known as ``secondary tearing'' or ``impulsive bursty'' regime of reconnection), while a continuously growing plasmoid is fed by newly coalescing islands. Such a model, involving a current sheet and a growing plasmoid, is consistent with the Yohkoh observations of the same flare (Ohyama & Shibata 1998). We present two-dimensional MHD simulations of dynamic magnetic reconnection that support the model. Within the framework of the proposed interpretation, the radio observations reveal details of plasmoid formation in flares.
description: A file with full-quality figures is available at http://www.aip.de/~preprint/preprints/2000/2000_23.html
Everyday life of women in Nyamayara
Creators: name: Vydrina, Alexandra
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2019
Subjects: subject: Kakabe
subject: kke

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
description: conversation with women of Nyamayara about their everyday life
title: ADCO, Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Cart. 29 (G 134), 996 folios, f. 0675
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: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0675, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0675, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
title: JFR - Journal of Family Research, Vol 31 No 2 (2019): Families, health, and well-being
title: Families, health, and well-being
titleType: AlternativeTitle
Creators: name: JFR-Journal Of Family Research
Publisher: name: JFR - Journal of Family Research
Year: 2019

description: Editorial...p. 130 Introduction to the Special Issue “Families, health, and well-being”...p. 131-137 Couple relationships and health: The role of the individual’s and the partner’s education...p. 138-154 Mental health dynamics around marital dissolution. Moderating effects of parenthood and children’s age...p. 155-179 Exploring the role of family ties on life satisfaction in later life in Europe...p. 180-198 Offspring and later-life loneliness in Eastern and Western Europe...p. 199-215 Grandparenthood, grandchild care and depression among older people in 18 countries...p. 216-239
Research Issues for Privacy in a Ubiquitously Connected World
Creators: name: Hong, Jason
Publisher: name: Carnegie Mellon University
Year: 2014
Subjects: Applied Computer Science

description: In just the past decade, we have seen the invention and adoption of wireless networking, smartphones, big data and predictive analytics, wearable computing, autonomous vehicles, sensor networks, social media sites, massive open online courses (MOOCs), and an array of many other wondrous technologies. We are now at a major inflection point, as computation, communication, and sensing are woven into our everyday lives. A very likely scenario is that, in the near future, our computing systems will know everything about us. A fundamental problem, however, is that these same technologies also introduce many new privacy risks, often at a rate faster than legal mechanisms and social norms can adapt. In this position paper, I sketch out several major research challenges for privacy. I present two different scenarios for privacy, probing the confluence of smart devices and inferencing, as well as issues in social media and big data. I also present some ongoing work my team is doing in investigating social influences on privacy, which I use as an example of how more social scientists can be brought on board to study issues of privacy
EOSC Front-Office Design, Functional and Technical Specification
Creators: name: Wilk, Roksana
name: Hienola, Anca
name: Wolski, Marcin
name: Shepherdson, John
name: Wilk, Bartosz
name: Tuminauskas, Raimundas
name: Walter, Bartosz
Publisher: name: Zenodo
Year: 2024
Subjects: open science
user environments
EOSC

description: Research and analysis on the functional and technical specification of a possible user environment in an infrastructure implementing open science paradigma.

 

It's a deliverable is the first step in defining the boundaries for the EOSC Platform Front-Office development within the scope of the EOSC Future project. The summary presented in the following sections describes the main goals of WP5, the typology of the Front-Office users, the state-of-play of the Front-Office architecture and technical specification (including the relevant supporting components), and the initial functional design. In addition, there is an analysis of the gaps that need to be bridged by the Front-Office development teams. The assumptions used in this deliverable will be updated during the EOSC Future project to reflect the feedback from users and additional needs.
Deformed defects for scalar fields with polynomial interactions
Creators: name: Bazeia, D.
name: León, M. A. González
name: Losano, L.
name: Guilarte, J. Mateos
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper we use the deformation procedure introduced in former work on deformed defects to investigate several new models for real scalar field. We introduce an interesting deformation function, from which we obtain two distinct families of models, labeled by the parameters that identify the deformation function. We investigate these models, which identify a broad class of polynomial interactions. We find exact solutions describing global defects, and we study the corresponding stability very carefully.
description: 8 pages, 5 eps figures, to appear in PRD
Toward High-Precision Astrometry with WFPC2. I. Deriving an Accurate PSF
Creators: name: Anderson, Jay
name: King, Ivan R.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The first step toward doing high-precision astrometry is the measurement of individual stars in individual images, a step that is fraught with dangers when the images are undersampled. The key to avoiding systematic positional error in undersampled images is to determine an extremely accurate point-spread function (PSF). We apply the concept of the {\it effective} PSF, and show that in images that consist of pixels it is the ePSF, rather than the often-used instrumental PSF, that embodies the information from which accurate star positions and magnitudes can be derived. We show how, in a rich star field, one can use the information from dithered exposures to derive an extremely accurate effective PSF by iterating between the PSF itself and the star positions that we measure with it. We also give a simple but effective procedure for representing spatial variations of the HST PSF. With such attention to the PSF, we find that we are able to measure the position of a single reasonably bright star in a single image with a precision of 0.02 pixel (2 mas in WF frames, 1 mas in PC), but with a systematic accuracy better than 0.002 pixel (0.2 mas in WF, 0.1 mas in PC), so that multiple observations can reliably be combined to improve the accuracy by $\surd N$.
description: 33 pp. text + 15 figs.; accepted by PASP
"Research Support From Libraries For All". Unterstützung für alle! VDB Kommission für forschungsnahe Dienste.
Creators: name: Strauch, Annette
Publisher: name: Zenodo
Year: 2019
Subjects: VDB
Bibliothekare
Bibliothekarinnen
Bibliotheken
Bibliotheken als Partner der Forschung
Forschung
Forscher
Forscherinnen
Kommission für forschungsnahe Dienste

description: Die Kommission für forschungsnahe Dienste existiert seit 2018 und ist die jüngste Kommission des VDB. Forschungsnahe Dienste werden von Bibliotheken in immer größerem Maße wahrgenommen, z.B. in folgenden Bereichen wie die des Open Access und Publikationsdienstleistungen, Forschungsdatenmanagement und Forschungsinformationssysteme, Bibliometrieservices. Kolleginnen und Kollegen, die in die Erstellung von forschungsnahen Dienstleistungen eingebunden sind, sollen durch entsprechende Fortbildungs- und Vernetzungsangebote der Kommission für forschungsnahe Dienste besser unterstützt werden. Die Arbeit der Kommission wurde während der Präsentation vorgestellt sowie Veranstaltungen beim Bibliothekskongress in Leipzig 2019, und es gab einen Bericht über den vorher stattgefundenen VDB-Workshop "Was ist Forschung?" in Darmstadt. Die Präsentation finden Sie auch auf dieser Seite zur Jahrestagung 2019 des Leibniz-Arbeitskreises Bibliotheken und Informationseinrichtungen: http://ak-bib.leibniz-arbeitskreise.de/jahrestagung-2019/praesentationen/
Conversation about celebration of the end of Ramadan
Creators: name: Vydrina, Alexandra
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2019
Subjects: subject: Kakabe
subject: kke

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
description: conversation with women of Gnamayara about their everyday life
Nonequilibrium Steady States and Fano-Kondo Resonances in an AB Ring with a Quantum Dot
Creators: name: Takahashi, Junko
name: Tasaki, Shuichi
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Electron transport through a strongly correlated quantum dot (QD) embedded in an Aharonov-Bohm (AB) ring is investigated with the aid of the finite-U slave-boson mean-field (SBMF) approach extended to nonequilibrium regime. A nonequilibrium steady state (NESS) of the mean-field Hamiltonian is constructed with the aid of the C*-algebraic approach for studying infinitely extended systems. In the linear response regime, the Fano-Kondo resonances and AB oscillations of the conductance obtained from the SBMF approach are in good agreement with those from the numerical renormalization group technique (NRG) by Hofstetter et al. by using twice larger Coulomb interaction. At zero temperature and finite bias voltage, the resonance peaks of the differential conductance tend to split into two. At low bias voltage, the split of the asymmetric resonance can be observed as an increase of the conductance plateau. We also found that the differential conductance has zero-bias maximum or minimum depending on the background transmission via direct tunneling between the electrodes.
description: 24 pages,17 figures
Requirements for Automatically Generating Multi-Modal Interfaces for Complex Appliances
Creators: name: Nichols, Jeffrey
name: Myers, Brad
name: Harris, Thomas K.
name: Rosenfeld, Roni
name: Shriver, Stefanie
name: HIggins, Michael
name: Hughes, Joseph
Publisher: name: Carnegie Mellon University
Year: 2002
Subjects: Applied Computer Science

description: Several industrial and academic research groups are working to simplify the control of appliances and services by creating a truly universal remote control. Unlike the preprogrammed remote controls available today, these new controllers download a specification from the appliance or service and use it to automatically generate a remote control interface. This promises to be a useful approach because the specification can be made detailed enough to generate both speech and graphical interfaces. Unfortunately, generating good user interfaces can be difficult. Based on user studies and prototype implementations, this paper presents a set of requirements that we have found are needed for automatic interface generation systems to create high-quality user interfaces.
Conversation about going to the market
Creators: name: Vydrina, Alexandra
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2019
Subjects: subject: Kakabe
subject: kke

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
description: conversation with women of Gnamayara about their everyday life
CO line emission from galaxies in the Epoch of Reionization
Creators: name: Vallini, L.
name: Pallottini, A.
name: Ferrara, A.
name: Gallerani, S.
name: Sobacchi, E.
name: Behrens, C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the CO line luminosity ($L_{\rm CO}$), the shape of the CO Spectral Line Energy Distribution (SLED), and the value of the CO-to-$\rm H_2$ conversion factor in galaxies in the Epoch of Reionization (EoR). To this aim, we construct a model that simultaneously takes into account the radiative transfer and the clumpy structure of giant molecular clouds (GMCs) where the CO lines are excited. We then use it to post-process state-of-the-art zoomed, high resolution ($30\, \rm{pc}$), cosmological simulation of a main-sequence ($M_{*}\approx10^{10}\, \rm{M_{\odot}}$, $SFR\approx 100\,\rm{M_{\odot}\, yr^{-1}}$) galaxy, "Althæa", at $z\approx6$. We find that the CO emission traces the inner molecular disk ($r\approx 0.5 \,\rm{kpc}$) of Althæa with the peak of the CO surface brightness co-located with that of the [CII] 158$\rm μm$ emission. Its $L_{\rm CO(1-0)}=10^{4.85}\, \rm{L_{\odot}}$ is comparable to that observed in local galaxies with similar stellar mass. The high ($Σ_{gas} \approx 220\, \rm M_{\odot}\, pc^{-2}$) gas surface density in Althæa, its large Mach number (\mach$\approx 30$), and the warm kinetic temperature ($T_{k}\approx 45 \, \rm K$) of GMCs yield a CO SLED peaked at the CO(7-6) transition, i.e. at relatively high-$J$, and a CO-to-$\rm H_2$ conversion factor $α_{\rm CO}\approx 1.5 \, \rm M_{\odot} \rm (K\, km\, s^{-1}\, pc^2)^{-1} $ lower than that of the Milky Way. The ALMA observing time required to detect (resolve) at 5$σ$ the CO(7-6) line from galaxies similar to Althæa is $\approx13$ h ($\approx 38$ h).
description: 16 pages, 14 figures, accepted for publication in MNRAS
Dielectronic recombination of lithium-like Ni25+ ions - high resolution rate coefficients and influence of external crossed E and B fields
Creators: name: Schippers, Stefan
name: Bartsch, Timo
name: Brandau, Carsten
name: Mueller, Alfred
name: Gwinner, Gerald
name: Wissler, Goetz
name: Beutelspacher, Michael
name: Grieser, Manfred
name: Wolf, Andreas
name: Phaneuf, Ronal
Publisher: name: arXiv
Year: 2000
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Astrophysics (astro-ph)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Absolute dielectronic recombination (DR) rates for lithium-like Ni$^{25+}$($1s^2 2s$) ions were measured at high-energy resolution at the Heidelberg heavy-ion storage ring TSR. We studied the center-of-mass energy range 0--130 eV which covers all $Δn$=0 core excitations. The influence of external crossed electric (0--300 V/cm) and magnetic (41.8--80.1 mT) fields was investigated. For the measurement at near-zero electric field resonance energies and strengths are given for Rydberg levels up to n$=$32; also Maxwellian plasma rate coefficients for the $Δn$=0 DR at electron temperatures between 0.5 and 200 eV are provided. For increasing electric field strength we find that for both the $2p_{1/2}$ and the $2p_{3/2}$ series of Ni$^{24+}$($1s^2 2p_j n\ell$) Rydberg resonances with n>30 the DR rate coefficient increases approximately linearly by up to a factor of 1.5. The relative increase due to the applied electric field for Ni$^{25+}$ is remarkably lower than that found in previous measurements with lighter isoelectronic Si$^{11+}$, Cl$^{14+}$ and also Ti$^{19+}$ ions, [T. Bartsch et al, Phys. Rev. Lett. {\bf 79}, 2233 (1997); {\bf 82}, 3779 (1999) and to be published] and in contrast to the results for lighter ions no clear dependence of the electric field enhancement on the magnetic field strength is found. The Maxwellian plasma rate coefficients for $Δn$=0 DR of Ni$^{25+}$ are enhanced by at most 11% in the presence of the strongest experimentally applied fields.
description: 14 pages, 12 figures, 4 tables
SARS‑CoV‑2 RNA polymerase as target for antiviral therapy
Creators: name: Buonaguro, Luigi
name: Tagliamonte, Maria
name: Tornesello, Maria Lina
name: Buonaguro, Franco
Publisher: name: Zenodo
Year: 2020

description: A new human coronavirus named SARS-CoV-2 was identified in several cases of acute respiratory syndrome in
Wuhan, China in December 2019. On March 11 2020, WHO declared the SARS-CoV-2 infection to be a pandemic,
based on the involvement of 169 nations. Specific drugs for SARS-CoV-2 are obviously not available. Currently, drugs
originally developed for other viruses or parasites are currently in clinical trials based on empiric data. In the quest of
an effective antiviral drug, the most specific target for an RNA virus is the RNA-dependent RNA-polymerase (RdRp)
which shows significant differences between positive-sense and negative-sense RNA viruses. An accurate evaluation
of RdRps from different viruses may guide the development of new drugs or the repositioning of already approved
antiviral drugs as treatment of SARS-CoV-2. This can accelerate the containment of the SARS-CoV-2 pandemic and,
hopefully, of future pandemics due to other emerging zoonotic RNA viruses.
Medium resolution near-infrared spectroscopy of Massive Young Stellar Objects
Creators: name: Pomohaci, R.
name: Oudmaijer, R. D.
name: Lumsden, S. L.
name: Hoare, M. G.
name: Mendigutia, I.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present medium-resolution (R~7000) near-infrared echelle spectroscopic data for 36 MYSOs drawn from the Red MSX Source (RMS) survey. This is the largest sample observed at this resolution at these wavelengths of MYSOs to date. The spectra are characterized mostly by emission from hydrogen recombination lines and accretion diagnostic lines. One MYSO shows photospheric HI absorption, a comparison with spectral standards indicates that the star is an A type star with a low surface gravity, implying that the MYSOs are probably swollen, as also suggested by evolutionary calculations. An investigation of the Br$γ$ line profiles shows that most are in pure emission, while 13$\pm$5 % display P Cygni profiles, indicative of outflow, while less than 8$\pm$4 % have inverse P Cygni profiles, indicative of infall. These values are comparable with investigations into the optically bright Herbig Be stars, but not with those of Herbig Ae and T Tauri stars, consistent with the notion that the more massive stars undergo accretion in a different fashion than lower mass objects which are undergoing magnetospheric accretion. Accretion luminosities and rates as derived from the Br$γ$ line luminosities agree with results for lower mass sources, providing tentative evidence for massive star formation theories based on scaling of low-mass scenarios. We present Br$γ$/Br12 line profile ratios exploiting the fact that optical depth effects can be traced as a function of Doppler shift across the lines. These show that the winds of MYSOs in this sample are nearly equally split between constant, accelerating, and decelerating velocity structures. There are no trends between the types of features we see and bolometric luminosities or near-infrared colours.
description: 30 pages, 21 figures (with appendices). Accepted for publication in Monthly Notices of the Royal Astronomical Society
Perturbative Calculation of Quasinormal Modes of $d$--Dimensional Black Holes
Creators: name: Shu, Fu-Wen
name: Shen, You-Gen
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study analytically quasinormal modes in a wide variety of black hole spacetimes, including $d$--dimensional asymptotically flat spacetimes and non-asymptotically flat spacetimes (particular attention has been paid to the four dimensional case). We extend the analytical calculation to include first-order corrections to analytical expressions for quasinormal mode frequencies by making use of a monodromy technique. All possible type perturbations are included in this paper. The calculation performed in this paper show that systematic expansions for uncharged black holes include different corrections with the ones for charged black holes. This difference makes them have a different $n$--dependence relation in the first-order correction formulae. The method applied above in calculating the first-order corrections of quasinormal mode frequencies seems to be unavailable for black holes with small charge. This result supports the Neitzke's prediction. On what concerns quantum gravity we confirm the view that the $\ln3$ in $d=4$ Schwarzschild seems to be nothing but some numerical coincidences.
description: 49 pages, 5 figures
Regulating Behavior in Online Communities
Creators: name: Yuqing  Ren
name: Kraut, Robert
name: Kiesler, Sara
name: Resnick, Paul
Publisher: name: Carnegie Mellon University
Year: 2010
Subjects: Applied Computer Science

description: In thriving communities, a rough consensus eventually emerges about the range of behaviors the managers and most members consider acceptable, what we will call normative behaviors, and another range of behaviors that are beyond the pale. A Rape In Cyberspace, the newspaper report by Julian Dibbell (1993), describes a classic example of unacceptable behavior in LamdaMoo, an early virtual environment. Mr. Bungle, an avatar in the online community, wrote a program that forced two avatars controlled by other participants to have virtual sex with him and with each other, and to do brutal things to their own bodies. In describing the event online the next day, one of the victims begged “"I am requesting that Mr. Bungle be toaded for raping Starsinger and I [stet],” where “toad” is the command that would turn Bungle’s avatar into a toad, annihilating the character’s original description and attributes. Within 24 hours, 50 other characters also called for his toading. Three days later the community had a real-time discussion of the issue. An system administrator who observed this discussion eventually ran the toad command to eliminate the Mr. Bungle character. Although LamdaMoo did not have a policy against cyberrape, when one occurred in its midst, this action instigated widespread discussion and crystallized a view among many inhabitants of what were correct and incorrect types of behavior in this community.
Magnetization of nanoparticle systems in a rotating magnetic field
Creators: name: Denisov, S. I.
name: Lyutyy, T. V.
name: Hänggi, P.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The investigation of a sizable thermal enhancement of magnetization is put forward for uniaxial ferromagnetic nanoparticles that are placed in a rotating magnetic field. We elucidate the nature of this phenomenon and evaluate the resonant frequency dependence of the induced magnetization. Moreover, we reveal the role of magnetic dipolar interactions, point out potential applications and reason the feasibility of an experimental observation of this effect.
description: 10 pages, 2 figures
Additional file 1 of Therapeutic mechanism of Toujie Quwen granules in COVID-19 based on network pharmacology
Creators: name: Huang, Ying
name: Zheng, Wen-jiang
name: Ni, Yong-shi
name: Li, Mian-sha
name: Chen, Jian-kun
name: Liu, Xiao-hong
name: Tan, Xing-hua
name: Li, Ji-qiang
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1.
title: Soft Rock Studio: Exploring a “Soft Systems” Approach to “Artificial Rock”
Creators: name: Forren, James
Publisher: name: University of Massachusetts Amherst
Year: 2021
Subjects: subject: Soft systems
subject: Artificial rock
subject: Natural materials
subject: Green concrete
subject: Materially-driven design
subject: Morphogenetic design
subject: Architectural Engineering
subject: Architectural Technology
subject: Architecture
subject: FOS: Civil engineering
subject: Construction Engineering and Management
subject: Engineering Education
subject: Structural Engineering

description: This paper discusses a study aimed at shifting disciplinary norms in construction materials. The study, conducted in a graduate level design-build studio, approached precast concrete construction through the lens of “artificial rock”: a composite material that can use cement, sand, aggregate, and reinforcing supplements and alternatives like flax, calcium carbonate, pyrolyzed biomass, soil, alginates, gelatin, and bacteria. Taught as “The Soft Rock Studio”, the course positioned artificial rock within the larger conceptual framework of “soft systems” - adaptive, networked part-to-whole relationships engaged in feedback loops with the environment. The Soft Rock Studio designed and prototyped components and assemblies for an alignment structure – or sky room - for a coastal site. Alignment structures are landscape and architecture constructions that align with the daytime and evening events in the sky: equinoxes, cardinal directions, constellations and solar orientations. The study design integrated empirical making, material testing and computational simulation in an iterative design methodology. The design methodology was tailored for a remote learning context and included the design and distribution of a material kit for at-home experimentation. Integrated with the methodology were process portfolios documenting student research and reflection, including responses to technology and humanities literature. Outcomes discussed in this paper are: material experimentations and iterative design possibilities of two student projects; evidence of student uptake; and reflections on the iterative design methodology. Observations and findings from alignment structure strategies are not included in the scope of this paper.
Conversation about how children go hunting and playing in the bush
Creators: name: Vydrina, Alexandra
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2019
Subjects: subject: Kakabe
subject: kke

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
description: conversation with women of Gnamayara about their everyday life
The covariant Tolman-Oppenheimer-Volkoff equations II: The anisotropic case
Creators: name: Carloni, Sante
name: Vernieri, Daniele
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We generalise the covariant Tolman-Oppenheimer-Volkoff equations proposed in arXiv:1709.02818 [gr-qc] to the case of static and spherically symmetric spacetimes with anisotropic sources. The extended equations allow a detailed analysis of the role of the anisotropic terms in the interior solution of relativistic stars and lead to the generalisation of some well known solutions of this type. We show that, like in the isotropic case, one can define generating theorems for the anisotropic Tolman-Oppenheimer-Volkoff equations. We also find that it is possible to define a reconstruction algorithm able to generate a double infinity of interior solutions. Among these, we derive a class of solutions that can represent "quasi-isotropic" stars.
description: 14 pages, 6 figures
Reflections of Everyday Activities in Spending Data
Creators: name: Schwarz, Julia
name: Mankoff, Jennifer
name: H. Scott  Matthews
Publisher: name: Carnegie Mellon University
Year: 2009
Subjects: Applied Computer Science

description: In this paper we show that financial information can be used to sense many aspects of human activity. This simple technique gives people information about their daily lives, is easily accessible to many at no extra cost, requires little setup, and does not require the manufacture of any external devices. We will focus on how financial data can be used to show users where they spend their time, when they accomplish certain habits, and what the impact of their activities is on the environment. We validate our idea by implementing three demonstration applications intended for personal use. Finally, this paper discusses limitations of sensing using financial data and possible solutions.
The Metallicity Distribution Function of Red Giants in the LMC
Creators: name: Cole, A. A.
name: Smecker-Hane, T. A.
name: Gallagher, J. S.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report new metallicity determinations for 39 red giants in a 220 square arcminute region, 1.8 degrees southwest of the bar of the Large Magellanic Cloud. These abundance measurements are based on spectroscopy of the Ca II infrared triplet. The metallicity distribution function (MDF) shows a strong peak at [Fe/H] = -0.57 +/- 0.04. Half the red giants in our field fall within the range -0.83 < [Fe/H] < -0.41. We find a striking contrast in the shape of the MDF below [Fe/H] < -1 between our inner disk field and the distant outer field studied by Olszewski (1993). Our field-star MDF seems similar to that of the intermediate-age (1-3 Gyr) star clusters. We have also obtained abundance estimates using Stromgren photometry for ~1000 red giants in the same field. The Stromgren measurements, which are sensitive to a combination of cyanogen and iron lines, correlate well with the Ca II measurements, but a metallicity-dependent offset is found (abridged).
description: 55 pages, 16 figures, AASTeX v5.0, extended data table not included, to appear in the October, 2000 issue of The Astronomical Journal
Metal abundances in hot white dwarfs with signatures of a superionized wind
Creators: name: Werner, K.
name: Rauch, T.
name: Kruk, J. W
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: About a dozen hot white dwarfs with effective temperatures Teff = 65,000-120,000 K exhibit unusual absorption features in their optical spectra. These objects were tentatively identified as Rydberg lines of ultra-high excited metals in ionization stages V-X, indicating line formation in a dense environment with temperatures near one million Kelvin. Since some features show blueward extensions, it was argued that they stem from a superionized wind. A unique assignment of the lines to particular elements is not possible, although they probably stem from C, N, O, and Ne. To further investigate this phenomenon, we analyzed the ultraviolet spectra available from only three stars of this group; that is, two helium-rich white dwarfs, HE 0504-2408 and HS 0713+3958 with spectral type DO, and a hydrogen-rich white dwarf, HS 2115+1148 with spectral type DAO. We identified light metals (C, N, O, Si, P, and S) with generally subsolar abundances and heavy elements from the iron group (Cr, Mn, Fe, Co, Ni) with solar or oversolar abundance. The abundance patterns are not unusual for hot WDs and can be interpreted as the result of gravitational settling and radiative levitation of elements. As to the origin of the ultra-high ionized metals lines, we discuss the possible presence of a multicomponent radiatively driven wind that is frictionally heated.
description: Accepted for publication in A&A
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Cart. 192 (11 H 77), 295 folios, f. 0062r
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
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. 0062r, 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. 0062r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Mendeleev's "Family": The Actinides
Creators: name: Orna, Mary Virginia
name: Fontani, Marco
Publisher: name: Substantia
Year: 2019

description: When Dmitri Mendeleev laid out his ordered grid of the then-known elements in 1869, he could not have predicted the overwhelming and all-encompassing effect that his idea would have on scientific theory for the next 150 years. Nevertheless, he knew, presciently and from the start that he had conceived and laid claim to a powerful predictive tool that would bring some kind of order to a seemingly random set of fundamental substances. It is not within the scope of this paper to detail how the thought currents of his day were converging, little by little, on the realization that the universe was an intrinsically ordered one, nor is it our purpose to award to Mendeleev the title of sole “discoverer” of the periodic system. We wish merely to point out that he now occupies a well-deserved place within the system under the title of “mendelevium,” element 101, and that, by this attribution, he belongs to a special “family,” the actinides. How this family was uncovered, grew, and developed is the topic of this essay.
description: Substantia, Vol 3 No 2 Suppl. 5 (2019)
Mendeleev at Home
Creators: name: Orna, Mary Virginia
Publisher: name: Substantia
Year: 2019

description: Dmitri Mendeleev was “at home” at the St. Petersburg State University for forty years. The museum set up in his former place of work/living quarters is well worth a visit.
description: Substantia, Vol 3 No 2 Suppl. 5 (2019)
Setting the Table: A Retrospective and Prospective of the Periodic Table of the Elements.
Creators: name: Orna, Mary Virginia
name: Fontani, Marco
Publisher: name: Substantia
Year: 2019

description: The major theme of this special issue volume is “The History of The Periodic Table, the Discovery of the Elements, and of the Materials that Changed the Course of History: The Development of the Periodic System and Its Consequences.” After a brief chronological retrospective on the development of the periodic table, each paper contributed to this volume will be summarized, with some editorial comments.
description: Substantia, Vol 3 No 2 Suppl. 5 (2019)
The AMBRE project: a study of Li evolution in the Galactic thin and thick discs
Creators: name: Prantzos, N.
name: de Laverny, P.
name: Guiglion, G.
name: Recio-Blanco, A.
name: Worley, C. C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Recent observations suggest a "double-branch" behaviour of Li/H versus metallicity in the local thick and thin discs. This is reminiscent of the corresponding O/Fe versus Fe/H behaviour, which has been explained as resulting from radial migration in the Milky Way disc. We use a semi-analytical model of disc evolution with updated chemical yields and parameterised radial migration. We explore the cases of long-lived (red giants of a few Gy lifetime) and shorter-lived (Asymptotic Giant Branch stars of several 10$^8$ yr) stellar sources of Li, as well as those of low and high primordial Li. We show that both factors play a key role in the overall Li evolution. We find that the observed "two-branch" Li behaviour is only directly obtained in the case of long-lived stellar Li sources and low primordial Li. In all other cases, the data imply systematic Li depletion in stellar envelopes, thus no simple picture of the Li evolution can be obtained. This concerns also the reported Li/H decrease at supersolar metallicities.
description: 8 pages, 4 figures, Astronomy and Astrophysics in press
Shaping the Periodic Classification in Portugal through (text)books and charts
Creators: name: Malaquias, Isabel
name: Oliveira, João A. B. P.
Publisher: name: Substantia
Year: 2019

description: In the current paper, we present an investigation carried out to map the reception and use of Mendeleev’s periodic classification in the Portuguese education system, from 1850 to 1975 while being confronted with other classifications. We present protagonists and documents to demonstrate the attention that the topic received. The research involved the identification of textbooks, programs and graphic presentations used in higher and secondary education levels within this time frame. During the 1880s, Mendeleev’s classification appears in higher-level (text)books and programs. Secondary school textbooks however remained faithful to earlier classifications for some more decades, with the exception of the first occurrence found in a textbook for advanced high school in 1906. It does not seem that the periodic system was integrated in the official secondary programs before 1938. The oldest use of periodic charts seems to be from after 1891 at the University of Coimbra, the oldest surviving one dating back to the second quarter of the twentieth century. The periodic table wall charts seem to have entered the secondary classroom in Portugal by the 1960s. This survey of the use of the Periodic System in Portugal demonstrates how the different context of reception have shaped its introduction in the educational system of what we now regard as the indispensable tool for chemistry. While there was relatively little scientific debate on the periodic law and system, as far as it was found, Mendeleev’s classification was appropriated at different speed and stages through textbooks and charts, responding to different pedagogical needs and usage.
description: Substantia, Vol 3 No 2 Suppl. 4 (2019)
Role of electron-electron and electron-phonon interaction effect in the optical conductivity of VO2
Creators: name: Okazaki, K.
name: Sugai, S.
name: Muraoka, Y.
name: Hiroi, Z.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We have investigated the charge dynamics of VO2 by optical reflectivity measurements. Optical conductivity clearly shows a metal-insulator transition. In the metallic phase, a broad Drude-like structure is observed. On the other hand, in the insulating phase, a broad peak structure around 1.3 eV is observed. It is found that this broad structure observed in the insulating phase shows a temperature dependence. We attribute this to the electron-phonon interaction as in the photoemission spectra.
description: 6 pages, 8 figures, accepted for publication in Phys. Rev. B
Fairy tale about an orphan and the figtree
Creators: name: Vydrina, Alexandra
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2019
Subjects: subject: Kakabe
subject: kke

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
description: conversation with women of Gnamayara about their everyday life
Additional file 1 of Is social camouflaging associated with anxiety and depression in autistic adults?
Creators: name: Hull, Laura
name: Levy, Lily
name: Lai, Meng-Chuan
name: Petrides, K. V.
name: Baron-Cohen, Simon
name: Allison, Carrie
name: Smith, Paula
name: Mandy, Will
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health

description: Additional file 1: Bivariate correlations between all variables and hierarchical regression analyses in sample split by gender identity.