cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1: of Matrix metalloproteinase activity in the lung is increased in Hermansky-Pudlak syndrome
Creators: name: Summer, Ross
name: Rachana Krishna
name: DeLeila Schriner
name: Cuevas-Mora, Karina
name: Sales, Dominic
name: Para, Rachel
name: Roman, Jesse
name: Nieweld, Carl
name: Gochuico, Bernadette
name: Romero, Freddy
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Computational Biology

description: Clinical Demographics of HPS and control subjects. (PDF 133 kb)
The X-ray Source at the Center of the Cassiopeia A Supernova Remnant
Creators: name: Mereghetti, S.
name: Tiengo, A.
name: Israel, G. L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the first results of an XMM-Newton observation of the central X-ray source in the Cas A supernova remnant. The spectrum can be fit equally well with an absorbed steep power law (alpha~3, N_H~1.5x10^22 cm^-2) or with a bremsstrahlung with temperature kT~2.4 keV and N_H~10^22 cm^-2. A blackbody model (kT~0.7 keV) gives a slightly worse fit and requires a column density N_H~5x10^21 cm^-2 and an emitting area with radius ~0.3 km (for d=3.4 kpc). A search for pulsations for periods longer than 150 ms gave negative results. The 3 sigma upper limits on the pulsed fraction are ~13% for P>0.3 s and ~7% for P>3 s. The overall properties of the central X-ray source in Cas A are difficult to explain in terms of a rapidly spinning neutron star with a canonical magnetic field of ~10^12 G, and are more similar to those of slowly rotating neutron stars such as the Anomalous X-ray Pulsars.
description: 15 pages, latex, 3 figures, to appear in The Astrophysical Journal; Revised version with more details on spectral analysis, fig. 1 and 2 slightly changed, revised flux values
Intermediate Luminosity Optical Transients (ILOTs) from merging giants
Creators: name: Segev, Ran
name: Sabach, Efrat
name: Soker, Noam
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We suggest and study the formation of intermediate luminosity optical transients (ILOTs) from the merger of two cool giant stars. For the two stars to merge when both are in their giant phases the stars must have close masses at their zero age main sequence, and the orbital separation must be in the right range. After the two giants merge, the two cores spiral-in toward each other within a common envelope. We study the energy sources of radiation in this process that include the ejection of mass that powers radiation by both recombination and by collision with previously ejected mass. This process includes no jets, unlike many other types of ILOTs, hence the event will not form a bipolar nebula. Using the stellar evolution numerical code mesa for two binary systems with stellar masses of (15Mo, 15.75Mo) and (31Mo, 31.5Mo), we find that the merger of the two cores releases gravitational energy that marginally ejects the entire common envelope. This implies that in many cases the two cores merge, i.e., a fatal common envelope evolution, leading to a somewhat more luminous ILOT. A typical ILOT from merger of two cool giant stars lasts for several months to several years and has a typical average luminosity of L(ILOT)~=10^6(M_{CE}/10Mo)Lo, where M_{CE} is the ejected common envelope mass. The merger-driven massive outflow forms dust, hence leading to a very red ILOT, possibly even infrared luminous and undetectable in the visible.
description: Accepted for publication in The Astrophysical Journal
The transition from Population III to normal galaxies: Ly-a and HeII 1640 emission and the ionising properties of high redshift starburst galaxies
Creators: name: Schaerer, Daniel
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine spectral properties of the ionising continua, the Lyman-break, and the Ly-a and HeII 1640 recombination lines in starbursts. The transition from primordial galaxies to currently observed metallicities, is examined. For the average properties of starbursts, the main findings are: 1) The Lyman continuum flux increases with decreasing metallicity. For a universal Salpeter IMF from 1-100 Msun the enhancement reaches typically a factor of ~3 between solar metallicity and Pop III objects. 2) While for metallicities Z >~ 1/50 Zsun the amplitude of the Lyman-break depends little on Z, a reduction by a factor ~2 is found at lower Z, due to the strong increase of the average stellar temperature. 3) Using theoretical models and empirical constraints we discuss the expected evolution of the hardness of He+ to H ionising photons with metallicity and possible uncertainties. We also provide a simple estimate of the possible impact of hot WR like stars on Q(He+)/Q(H) at very low metallicities. 4) Calibrations for star formation rate determinations from various recombination lines at all metallicities and for various IMFs are derived. For young bursts the maximum Ly-a equivalent width is shown to increase strongly with decreasing metallicity for the same IMF. However, for well known reasons, the Ly-a emission predicted likely represents an upper limit. Non-negligible HeII 1640 emission due to stellar photoionisation appears to be limited to very low metallicities and Population III objects.(abridged abstract)
description: Accepted for publication in A&A. LaTeX, 14 pages including figures. Model predictions available at http://webast.ast.obs-mip.fr/sfr
A laser-microfabricated electrohydrodynamic thruster for centimeter-scale aerial robots
Creators: name: Prasad, Hari Krishna Hari
name: Vaddi, Ravi Sankar
name: Chukewad, Yogesh M
name: Dedic, Elma
name: Novosselov, Igor
name: Fuller, Sawyer B
Publisher: name: arXiv
Year: 2019
Subjects: subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: To date, insect scale robots capable of controlled flight have used flapping wings for generating lift, but this requires a complex and failure-prone mechanism. A simpler alternative is electrohydrodynamic (EHD) thrust, which requires no moving mechanical parts. In EHD, corona discharge generates a flow of ions in an electric field between two electrodes; the high-velocity ions transfer their kinetic energy to neutral air molecules through collisions, accelerating the gas and creating thrust. We introduce a fabrication process for EHD thruster based on 355 nm laser micromachining and our approach allows for greater flexibility in materials selection. Our four-thruster device measures 1.8 x 2.5 cm and is composed of steel emitters and a lightweight carbon fiber mesh. The current and thrust characteristics of each individual thruster of the quad thruster is determined and agrees with Townsend relation. The mass of the quad thruster is 37 mg and the measured thrust is greater than its weight (362.6 uN). The robot is able to lift off at a voltage of 4.6 kV with a thrust to weight ratio of 1.38.
description: Co-primary authors: Hari Krishna Hari Prasad, Ravi Sankar Vaddi, and Yogesh M Chukewad Submitted to PLOS ONE
Magnetic Helix Formation Driven by Keplerian Disk Rotation in an External Plasma Pressure --- The Initial Expansion Stage
Creators: name: Li, H.
name: Lovelace, R. V. E.
name: Finn, J. M.
name: Colgate, S. A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the evolution of a magnetic arcade that is anchored to an accretion disk and is sheared by the differential rotation of a Keplerian disk. By including an extremely low external plasma pressure at large distances, we obtain a sequence of axisymmetric magnetostatic equilibria and show that there is a fundamental difference between field lines that are affected by the plasma pressure and those are not (i.e., force-free). Force-free fields, while being twisted by the differential rotation of the disk, expand outward at an angle of $\sim 60^\circ$ away from the rotation axis, consistent with the previous studies. These force-free field lines, however, are enclosed by the outer field lines which originate from small disk radii and come back to the disk at large radii. These outer fields experience most of the twist, and they are also affected most by the external plasma pressure. At large cylindrical radial distances, magnetic pressure and plasma pressure are comparable so that any further radial expansion of magnetic fields is prevented or slowed down greatly by this pressure. This hindrance to cylindrical radial expansion causes most of the added twist to be distributed on the ascending portion of the field lines, close to the rotation axis. Since these field lines are twisted most, the increasing ratio of the toroidal $B_ϕ$ component to the poloidal component $B_{R,z}$ eventually results in the collimation of magnetic energy and flux around the rotation axis. We discuss the difficulty with adding a large number of twists within the limitations of the magnetostatic approximation.
description: 9 pages text, 7 figures (fig7 in color), accepted to ApJ
title: Notions of Home: Constant, Fluid, and Mobile
Creators: name: Nakamura-Mather, Mika
Publisher: name: Griffith University
Year: 2017
Subjects: subject: Art Objects
subject: Cultural Dislocation
subject: Memory Influence
subject: Emotion Response

description: I have spent more than a quarter of a century living outside my homeland of Japan. In recent visits to Japan, I have noticed that my sense of belonging is growing stronger. This has caused me to question whether this is simply nostalgia or something deeper. I wonder whether my prolonged exposure to other cultures has enhanced my appreciation of my own, or whether I am losing my cultural identity and the idea of home is becoming more attractive because it feels familiar and safe. Through my studio work, I seek to juxtapose the present with the past, to examine the role that memory plays in our notions of home, and particularly to discover how my memories influence my emotional response to geographical and cultural dislocation. In this exegesis, I examine the nature of memory and the idea that home is not merely a place on a map. My research investigates whether a particular material associated with a specific place—in my case, wood—can be fundamental to developing a better understanding of who we are, where we come from, and why we call one place home over another.
Additional file 1 of Cerebrovascular complications in patients with community-acquired bacterial meningitis: occurrence and associated factors in the COMBAT multicenter prospective cohort
Creators: name: Benadji, Amine
name: Debroucker, Thomas
name: Martin-Blondel, Guillaume
name: Argaud, Laurent
name: Vitrat, Virginie
name: Biron, Charlotte
name: Wolff, Michel
name: Hoen, Bruno
name: Duval, Xavier
name: Tubiana, Sarah
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Neuroscience
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Supplementary Material 1
Dynamically generated inflationary two-field potential via non-Riemannian volume forms
Creators: name: Benisty, David
name: Guendelman, Eduardo I.
name: Nissimov, Emil
name: Pacheva, Svetlana
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider a simple model of modified gravity interacting with a single scalar field $φ$ with weakly coupled exponential potential within the framework of non-Riemannian spacetime volume-form formalism. The specific form of the action is fixed by the requirement of invariance under global Weyl-scale symmetry. Upon passing to the physical Einstein frame we show how the non-Riemannian volume elements create a second canonical scalar field $u$ and dynamically generate a non-trivial two-scalar-field potential $U_{\rm eff}(u,φ)$ with two remarkable features: (i) it possesses a large flat region for large $u$ describing a slow-roll inflation; (ii) it has a stable low-lying minimum w.r.t. $(u,φ)$ representing the dark energy density in the "late universe". We study the corresponding two-field slow-roll inflation and show that the pertinent slow-roll inflationary curve $φ= φ(u)$ in the two-field space $(u,φ)$ has a very small curvature, i.e., $φ$ changes very little during the inflationary evolution of $u$ on the flat region of $U_{\rm eff}(u,φ)$. Explicit expressions are found for the slow-roll parameters which differ from those in the single-field inflationary counterpart. Numerical solutions for the scalar spectral index and the tensor-to-scalar ratio are derived agreeing with the observational data.
description: 13 pages. 2 Fig. arXiv admin note: text overlap with arXiv:1906.06691 , v.2 14 pages, typos corrected, additional explanations
Trichoderma erinaceum Bissett, Kubicek & Szackacs, Can. J. Bot.
Creators: name: Thokala, Prameeladevi
name: Narayanasamy, Prabhakaran
name: Kamil, Deeba
name: Choudhary, Shiv Pratap
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Fungi
Ascomycota
Sordariomycetes
Hypocreales
Hypocreaceae
Trichoderma
Trichoderma erinaceum

description: 7. Trichoderma erinaceum Bissett, Kubicek & Szackacs, Can. J. Bot. 8: 8, 00. Figure 9
Section— Trichoderma
Description:
Colony: 7.0– 8.5 cm growth was observed in 4 days on PDA medium. White mycelium producing yellow pustules turning to dark green color with the age. The pustules uniformly spread throughout the plate leaving a concentric green ring at the center. The reverse of the plate is colorless.
Conidiophores: The main axis terminates in a septate elongation with a single phialide at its tip and fertile branches arising near the base. Conidiophore branches arising at angles of 90° or less concerning the main axis, paired or not, rebranching sparingly to produce phialides directly or at the tips of short secondary branches.
Phialides: Phialides arising from branches are solitary or in whorls of 2 or 3, straight, cylindrical, flask-shaped and swollen in the middle.
Conidia: Ellipsoidal to broadly ellipsoidal, 4.00–5.50 × 3.5–4.5 µm, green.
Chlamydospores: Chlamydospores terminal to intercalary, globose to subglobose, 8.00–13.00 µm.
 Cultures examined: ITCC 7287 (Withania somnifera rhizosphere, Delhi); ITCC 7288 (Groundnut rhizosphere, Tirupati, AP); ITCC 7289 (Soil, SUKAST, Jammu, J&K).
Diagnostic features: Conidiophores arising at 90° and ends with a single phialide with the fertile branches at the base and produce solitary and flask-shaped phialides directly on secondary branches.
 Ecology and habitats: Soil, endophyte of woody tissue of Theobroma cacao in Peru.
description: Published as part of Thokala, Prameeladevi, Narayanasamy, Prabhakaran, Kamil, Deeba & Choudhary, Shiv Pratap, 2021, Polyphasic taxonomy of Indian Trichoderma species, pp. 1-27 in Phytotaxa 502 (1) on page 11, DOI: 10.11646/phytotaxa.502.1.1, http://zenodo.org/record/5424892
Additional file 1 of Preimplantation genetic testing for Aicardi–Goutières syndrome induced by novel compound heterozygous mutations of TREX1: an unaffected live birth
Creators: name: Xu, Huiling
name: Pu, Jiajie
name: Lin, Suiling
name: Hu, Rui
name: Yao, Jilong
name: Li, Xuemei
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. Table S1. Variants classification following ACMG guidelines.
UU Aqr from high to low state
Creators: name: Vrielmann, Sonja
name: Baptista, Raymundo
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper we present Physical Parameter Eclipse Mapping (PPEM) of UBVRI eclipse light curves of UU Aqr from high to low states. We used a simple, pure hydrogen LTE model to derive the temperature and surface density distribution in the accretion disc. The reconstructed effective temperatures in the disc range between 9000K and 15000K in the inner part of the disc and below 7000K in the outer parts. In the higher states it shows a more or less prominent bright spot with T_eff between about 7000K and 8000K. The inner part of the disc (R < 0.3R_L1) is optically thick at all times, while the outer parts of the disc up to the disc edge (0.51+-0.04R_L1 in the high state and 0.40+-0.03R_L1 in the low state) deviate from a simple black body spectrum indicating that either the outer disc is optically thin or it shows a temperature inversion in the vertical direction. While during high state the disc is variable, it appears rather stable in low state. The variation during high state affects the size of the optically thick part of the disc, the white dwarf or boundary layer temperature and the uneclipsed component (originating in a disc chromosphere and/or cool disc wind), while the actual size of the disc remains constant. The difference between high and low state is expressed as a change in disc size that also affects the size of the optically thick part of the disc and the presence of the bright spot. Using the PPEM method we retrieve a distance for UU Aqr of 207+-10pc, compatible with previous estimates.
description: 13 pages, 8 figures, uses aa.cls, accepted for publication in AN, for associated postscript files, see http://www/DE/Ins/Per/Vrielmann/uuaqrmaps.html
Additional file 1: of Leukemia relapse following unmanipulated haploidentical transplantation: a risk factor analysis on behalf of the ALWP of the EBMT
Creators: name: Piemontese, Simona
name: Boumendil, Ariane
name: Labopin, Myriam
name: Schmid, Christoph
name: Ciceri, Fabio
name: Arcese, William
name: Koc, Yener
name: Gulbas, Zafar
name: Tischer, Johanna
name: Bruno, Benedetto
name: Depei Wu
name: Blaise, Didier
name: Beelen, Dietrich
name: Irrera, Giuseppe
name: Ruggeri, Annalisa
name: Houhou, Mohamed
name: Mohty, Mohamad
name: Nagler, Arnon
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Developmental Biology
subject: Marine Biology
subject: Cancer
subject: Science Policy
subject: Hematology
subject: Plant Biology
subject: FOS: Biological sciences
subject: 60506 Virology

description: Table S1. Characteristic of the 587 patients included in our analysis and the 1065 patients transplanted in the same years in the EBMT centres but not included in the final analysis due to incomplete data. (DOCX 19 kb)
Trichoderma ghanense Doi, Abe & J. Sugiyama, Bull. Natl. Sci. Mus. Ser. B (Bot.
Creators: name: Thokala, Prameeladevi
name: Narayanasamy, Prabhakaran
name: Kamil, Deeba
name: Choudhary, Shiv Pratap
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Fungi
Ascomycota
Sordariomycetes
Hypocreales
Hypocreaceae
Trichoderma
Trichoderma ghanense

description: 8. Trichoderma ghanense Doi, Abe & J. Sugiyama, Bull. Natl. Sci. Mus. Ser. B (Bot.):, 987. Figure 0
Section—Longibrachiatum
Description:
 Colony: 7 – 8.5 cm in four days. Aerial hyphae cottony grown throughout the plate. Artemisia green white cushionlike small pustules formed throughout the plate but concentrating more than 2 cm away from the edge of the plate. The white pustules turned to green after conidiation. Reverse of the plate was colorless.
Conidiophores: Conidiophores typically consisting of a strongly developed central axis from which arise, toward the tip, solitary phialides and further from the tip progressively longer, often paired, secondary branches. Phialides arising directly from secondary branches, typically not in whorls.
Phialides: Phialides cylindrical or straight or hooked.
Conidia: Conidia green, ellipsoidal, 6.0–7.5× 4.0–4.5 µm and smooth.
 FIGURE 0. Trichoderma ghanense ( A ) Growth on PDA, ( B ) Pustules with ooze, ( C ) Reverse of the plate, ( D ) Conidiophore branching, ( E,F,G ) Phialide disposition, ( H ) Spores, ( I ) Chlamydospores.
Chlamydospores: Chlamydospores abundant, globose, 7.0–12.0 µm in dia. and smooth.
Culture Examined: ITCC 7279 (Soil, Arunachal Pradesh).
Diagnostic features: Greenish white cushion-like small pustules, Conidiophore bearing cylindrical or straight or looked solitary phialides. Chlamydospores are abundant and globose.
Ecology and habitats: Soil.
 FIGURE. Trichoderma harzianum ( A ) Growth on PDA, ( B ) Pustules, ( C ) Reverse of the plate; ( D, E ) Conidiophore branching, ( F,G ) ampulliform phialides, ( H ) Spores, ( I ) Spores under SEM, ( J ) Chlamydospores.
 FIGURE. Trichoderma hamatum ( A ) Growth on PDA, ( B ) Pustules, ( C ) Reverse of the plate, ( D ) pustule, ( E.F ) Conidiophore branching, ( G,H,I ) Phialide disposition, ( J ) Spores, ( K ) Chlamydospores.
description: Published as part of Thokala, Prameeladevi, Narayanasamy, Prabhakaran, Kamil, Deeba & Choudhary, Shiv Pratap, 2021, Polyphasic taxonomy of Indian Trichoderma species, pp. 1-27 in Phytotaxa 502 (1) on pages 11-13, DOI: 10.11646/phytotaxa.502.1.1, http://zenodo.org/record/5424892
Dynamic management for business processes modeling & execution in workflows
Creators: name: Golani, Mati
Publisher: name: Freie Universität Berlin
Year: 2001
Subjects: subject: 000 Informatik, Informationswissenschaft, allgemeine Werke::000 Informatik, Wissen, Systeme::004 Datenverarbeitung; Informatik

description: Contemporary workflow-management systems cannot represent change or evolution of business processes. When a change is needed due to external reason, an offline procedure is invoked in order to create a new workflow engine template for the future instances in the workflow enactment module. The standard interfaces do not deal with the business process metadata in a way that can actually change it as a reaction to inbound knowledge. There are many relevant cases, especially in the virtual enterprise arena, where the business process is not deterministic and is influenced by external parameters (such as the selection of virtual partners), so the knowledge of what should be done is available, however it is external to the system. There is a need to develop a modeling mechanism that enables to transfer process definitions in an automatic way, without the need for human interference. One way of confronting with these issues is the use of a rule-based engine to monitor business process execution. This engine will contain internal meta-rules that refer to metadata entities, i.e. rules that describe how to act on other rules (business process routing) when a change is detected, while executing all needed consistency checks.
Rhagiosoma Chapuis 1878
Creators: name: Sekerka, Lukáš
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Rhagiosoma

description: Rhagiosoma Chapuis, 1878, stat. restit.
 Rhagiosoma Chapuis, 1878: cxliii (type species R. madagascariense Chapuis, 1878 nec. Heyden, 1877 (= Rhagiosoma chapuisi nom. nov.), by monotypy).
 Rhagiosoma: MONRÓS (1956): 106 (as synonym of Megamerus Mac Leay, 1827).
description: Published as part of Sekerka, Lukáš, 2007, On the genus Rhagiosoma and the identity of R. madagascariense (Coleoptera: Chrysomelidae: Sagrinae: Megamerini), pp. 195-202 in Acta Entomologica Musei Nationalis Pragae 47 on page 196, DOI: 10.5281/zenodo.5328315
Vaccine Hesitancy Under the Magnifying Glass: A Systematic Review of the Uses and Misuses of an Increasingly Popular Construct
Creators: name: Lokmanoglu, Ayse D.
name: Velho, Raphaela M.
name: Walter, Nathan
name: Andrews, Emily A.
name: Ophir, Yotam
name: Walter, Dror
name: Pruden, Meredith L.
Publisher: name: Taylor & Francis
Year: 2022

description:
Resistance to vaccines has hindered attempts to contain and prevent outbreaks of infectious diseases for centuries. More recently, however, the term "vaccine hesitancy" has been used to describe not necessarily outright resistance but also a delay in acceptance or uncertainty regarding vaccines. Given concerns about hesitancy and its impact on vaccine uptake rates, researchers increasingly shifted the focus from resistance to vaccines toward vaccine hesitancy. Acknowledging the urgency to accurately assess the phenomenon, it is critical to understand the state of the literature, focusing on issues of conceptualization and operationalization. To carry out this systematic review, we collected and analyzed all published empirical articles from 2000 to 2021 that explicitly included quantitative self-report measures of vaccine hesitancy (k = 86). Using a mixed-method approach, the review demonstrates and quantifies crucial inconsistencies in the measurement of the construct, lack of clarity in regard to the determination of who should or should not be defined as hesitant, and overreliance on unrepresentative samples. Crucially, our analysis points to a potential systematic bias toward exaggerating the level of hesitancy in the population. Modeling a vaccine hesitancy co-citation network, the analysis also points to the existence of insular academic silos that make it harder to achieve a unified measurement tool. Theoretical and practical implications for academics, practitioners, and policymakers are discussed.
THE USE OF METAPHOR AND SYMBOLIC MEANING IN LITERARY WORKS
Creators: name: Abdullayeva, Yulduz
Publisher: name: Zenodo
Year: 2025

description: This article analyzes the use of metaphor and symbolism in literary works. It examines the function of metaphor as a means of expression within literary texts and evaluates its effectiveness. The article also highlights the emergence of symbolic images, their range of meanings, and their influence on readers' perception. The stylistic features of artistic devices are analyzed based on examples from various literary works.
Effects of pairing, continuum, and deformation on particles in the classically forbidden regions for Mg isotopes
Creators: name: Zhang, Kaiyuan
name: Wang, Dongyang
name: Zhang, Shuangquan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Particles in the classically forbidden regions are studied based on the deformed relativistic Hartree-Bogoliubov theory in continuum with PC-PK1 for magnesium isotopes. By analyzing the neutron and proton radii, it is found that the largest deviations from the empirical values appear at the predicted neutron halo nuclei $^{42}$Mg and $^{44}$Mg. Consistently, notable increases at $^{42}$Mg and $^{44}$Mg are found in the total number of neutrons in the classically forbidden regions that includes the number of neutrons in continuum. It is shown that the deformation effect, in general, increases the number of particles in the classically forbidden regions below the continuum threshold. The most deeply bound single-particle states play the dominant roles in the increase caused by deformation.
description: 18 pages, 6 figures. Accepted for publication in Physical Review C
Trichoderma hamatum Bain., Bull. Soc. Mycol.
Creators: name: Thokala, Prameeladevi
name: Narayanasamy, Prabhakaran
name: Kamil, Deeba
name: Choudhary, Shiv Pratap
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Fungi
Ascomycota
Sordariomycetes
Hypocreales
Hypocreaceae
Trichoderma
Trichoderma hamatum

description: 9. Trichoderma hamatum (Bon.) Bain., Bull. Soc. Mycol. France:, 906. Figure
Section— Pachybasium
Description:
Colony:7.0– 8.5 cm growth was observed in 4 days on PDA medium. Mycelium is mostly submerged, less aerial mycelium which is floccose and white. Compact cushioned pustules looking velvety due to the presence of numerous, flexuous sterile conidiophore apices. These pustules are white at first, becoming yellow, then pea-green followed by olive green. Colorless at the reverse of the Petri plate.
 Conidiophores: Conidiophores in pustules are broad, comprising a regular, undulate and humate sterile elongation with the phialides arising near the base. The lateral branches typically comprise one or a few, broad cells with phialides arising at the tip and along the length. The internodes between branches are short and the phialides densely clustered. Phialides: Phialides are short, broadly ellipsoidal to ovoidal, pyriform and ampulliform, formed on small branches, smooth - walled, hyaline or pale green color.
Conidia: Oblong to ellipsoidal and smooth, 5.0–6.0 × 3.0–4.0 µm, green.
Chlamydospores: Chlamydospores terminal and intercalary, globose, 4.0–8.0 µm diam.
Cultures examined: ITCC 7271 (Rice soil, Cuttack, Odisha); ITCC 7272 (Soil, Kochi, Kerala); ITCC 7270 (Soil, Dehradun, Uttarakhand).
Diagnostic features: Compact cushioned pustules white at first, becoming yellow, then green in colour. Conidiophores with non-fertile, stout, hamate and undulate elongations, with the short, ovoidal or pyriform densely clustered phialides near the base.
Ecology and habitats: Soil.
description: Published as part of Thokala, Prameeladevi, Narayanasamy, Prabhakaran, Kamil, Deeba & Choudhary, Shiv Pratap, 2021, Polyphasic taxonomy of Indian Trichoderma species, pp. 1-27 in Phytotaxa 502 (1) on page 14, DOI: 10.11646/phytotaxa.502.1.1, http://zenodo.org/record/5424892
Gallup Poll # 694
Creators: name: Gallup
Publisher: name: Roper Center for Public Opinion Research
Year: 2021

description: Most important problem facing the country (1); civil rights (1); business conditions (1); Democratic vs. Republican (3); changing proportion of representatives (1); possible presidential candidates for 1964 election (1); William Scranton vs. Richard Nixon (1); Richard Nixon vs. Barry Goldwater (1); Barry Goldwater vs. William Scranton (1); Richard Nixon vs. Lyndon Baines Johnson (1); Barry Goldwater vs. Lyndon Baines Johnson (1); William Scranton vs. Lyndon Baines Johnson (1); Barry Goldwater vs. Lyndon Baines Johnson vs. George Wallace (1); certainty of vote (1); Liberal vs. Conservative (1); President Lyndon Baines Johnson job performance (1); vote in 1960 (1).
A new approach to the problem of modes in the Mestel disk
Creators: name: Demleitner, Markus
name: Fuchs, Burkhard
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the modes admitted by the Mestel disk, a disk with a globally flat rotation curve. In contrast to previous analyses of this problem by Zang (\cite{1976PhDT........26Z}) and Evans & Read (\cite{1998MNRAS.300...83E}, \cite{1998MNRAS.300..106E}), we approximate the orbits to obtain almost closed expressions for the kernel of the integral equation governing the behaviour of the modes. Otherwise we, like them, follow Kalnajs' programme to simultaneously solve the Boltzmann and Poisson equations. We investigate the modes admitted by both the self-consistent and a cut-out Mestel disk, the difference being that in the latter, a part of the matter in the disk is immobilised. This breaks the self-similarity and produces a pronouncedly different picture, both technically and in terms of the disk properties. The self-consistent disk is governed by a Cauchy integral equation, the cut-out disk by an integral equation that can be treated as a Fredholm equation of the second kind. In general, our approximation reproduces the results of the previous works remarkably well, yielding quantities mostly within 5% of the values reported by Zang and Evans & Read and thus also the basic result that in a ``standard'' cut-out disk, only one-armed modes are unstable at the limit of axisymmetric stability. In the self-consistent disk, relatively compact expressions for the kernel allow an intuitive understanding of most of the properties of neutral (non-rotating, non-growing) modes there. We finally show that self-consistent Mestel disks do not admit growing or rotating modes in this sort of stellar-dynamical analysis.
description: 10 pages, 1 figure; accepted for publication in A&A
PyRod -- Tracing Water Molecules in Molecular Dynamics Simulations
Creators: name: Schaller, David
name: Pach, Szymon
name: Wolber, Gerhard
Publisher: name: arXiv
Year: 2019
Subjects: subject: Biomolecules (q-bio.BM)
subject: FOS: Biological sciences

description: Ligands entering a protein binding pocket essentially compete with water molecules for binding to the protein. Hence, the location and thermodynamic properties of water molecules in protein structures have gained increased attention in the drug design community. Including corresponding data into 3D pharmacophore modeling is essential for efficient high throughput virtual screening. Here, we present PyRod, a free and open-source python software that allows for visualization of pharmacophoric binding pocket characteristics, identification of hot spots for ligand binding and subsequent generation of pharmacophore features for virtual screening. The implemented routines analyze the protein environment of water molecules in molecular dynamics (MD) simulations and can differentiate between hydrogen bonded waters as well as waters in a protein environment of hydrophobic, charged or aromatic atom groups. The gathered information is further processed to generate dynamic molecular interaction fields (dMIFs) for visualization and pharmacophoric features for virtual screening. The described software was applied to 5 therapeutically relevant drug targets and generated pharmacophores were evaluated using DUD-E benchmarking sets. The best performing pharmacophore was found for the HIV1 protease with an early enrichment factor of 54.6. PyRod adds a new perspective to structure-based screening campaigns by providing easy-to-interpret dMIFs and purely protein-based 3D pharmacophores that are solely based on tracing water molecules in MD simulations. Since structural information about co-crystallized ligands is not needed, screening campaigns can be followed, for which less or no ligand information is available. PyRod is freely available at https://github.com/schallerdavid/pyrod.
Ανάπτυξη τμήματος εφαρμογής πλοήγησης σε εξωτερικό χώρο με φωνητική εντολή μέσω έξυπνων κινητών τηλέφωνων
Creators: name: Δεμένεγας, Παντελεήμων
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2021
Subjects: subject: Εφαρμογή πλοήγησης
subject: Προβλήματα όρασης

description: Η εργασία αφορά στην ανάπτυξη εφαρμογής (application) που λειτουργεί σε περιβάλλον android , με την υποστήριξη των εφαρμογών Google Maps, Google speech to text και text to speech, και στόχο έχει στην αυτόνομη διαβίωση των χρηστών με αναπηρία. Αρχικά, παρουσιάζονται οι αρχές που διέπουν τη σχέση Τεχνολογίας και Αναπηρίας. Η τεχνολογία διευκολύνει τη ζωή των αναπήρων όταν αποκαθιστά την προσβασιμότητα. ΄Οσον αφορά τη θεσμική ρύθμιση της τεχνολογίας, παρατηρείται ότι παραμένει ζητούμενο η διασφάλιση ότι η χρήση της τεχνολογίας θα υπηρετεί τα ανθρώπινα δικαιώματα, στοχεύοντας στην εξάλειψη του ψηφιακού χάσματος μεταξύ του γενικού πληθυσμού και των αναπήρων. Στη συνέχεια, γίνεται ανάλυση της ομάδας- στόχου της παρούσας εργασίας, δηλαδή τα άτομα με μερική ή ολική απώλεια όρασης, καθώς και άλλα εμποδιζόμενα άτομα, που αντιμετωπίζουν παρεμφερείς δυσκολίες και μπορούν να επωφεληθούν από τις ίδιες τεχνολογικές εφαρμογές. Στο σημείο αυτό, επισημαίνεται ότι η βαρύτητα της αναπηρία εξαρτάται από την ύπαρξη ή όχι προσαρμογών στο περιβάλλον διαβίωσης. Για το λόγο αυτόν, γίνονται εξατομικευμένες εύλογες προσαρμογές , και παράγονται διάφορα τεχνικά βοηθήματα για αναπήρους που βελτιώνουν τις λειτουργικές ικανότητες τους. Ειδική κατηγορία βοηθημάτων αποτελούν τα προϊόντα υποστηρικτικής (assistive technologies) και προσαρμοστικής τεχνολογίας (adaptive technologies) που έχουν αναπτυχθεί για τα άτομα με περιορισμένη όραση ή τυφλά άτομα. Στα πλαίσια της εφαρμογής, γίνεται αναφορά στο Παγκόσμιο Σύστημα Στιγματοθέτησης, ή Θεσιθεσίας GPS (Global Positioning System) καθώς και σε εμπορικές ή ερευνητικές εφαρμογές πλοήγησης σε συσκευές κινητής τηλεφωνίας για άτομα με περιορισμένη όραση ή τυφλά. Τέλος, αναλύεται ο κώδικας της εφαρμογής που βασίστηκε στην αρχιτεκτονική Model-View-View Model. Αποτελείται από 3 activities οι οποίες υλοποιούν τις βασικές λειτουργικότητες, ενώ η υλοποίηση των σημαντικότερων λειτουργικοτήτων γίνεται σε αντίστοιχα View Models. Ξεκινά από μια Main Activity και περιμένει ως ότου ακούσει τη λέξη πλοήγηση .Τότε προχωρά στη Navigation Activity , όπου ρωτά το χρήστη “πού θα ήθελε να πάει” . Μέχρις ότου ο χρήστης δώσει μια έγκυρη διεύθυνση και να επιβεβαιώσει ότι όντως αυτή είναι η διεύθυνση όπου θα ήθελε να πάει επαναλαμβάνονται τα βήματα της διαδικασίας. Σε επόμενο στάδιο , η εφαρμογή μπορεί να καλύπτει επιπλέον καθήκοντα και σε συνεργασία με σύστημα GPS να αποτελέσει μιαν ανεξάρτητη εφαρμογή για smartphone σε περιβάλλον android ή σε κάποια ανεξάρτητη συσκευή για την πλοήγηση των ατόμων με περιορισμένη ή καθόλου όραση, και άλλων ομάδων που αντιμετωπίζουν παρεμφερείς δυσκολίες.
An electrically powered binary star?
Creators: name: Wu, Kinwah
name: Cropper, Mark
name: Ramsay, Gavin
name: Sekiguchi, Kazuhiro
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose a model for stellar binary systems consisting of a magnetic and a non-magnetic white-dwarf pair which is powered principally by electrical energy. In our model the luminosity is caused by resistive heating of the stellar atmospheres due to induced currents driven within the binary. This process is reminiscent of the Jupiter-Io system, but greatly increased in power because of the larger companion and stronger magnetic field of the primary. Electrical power is an alternative stellar luminosity source, following on from nuclear fusion and accretion. We find that this source of heating is sufficient to account for the observed X-ray luminosity of the 9.5-min binary RX J1914+24, and provides an explanation for its puzzling characteristics.
description: accepted by MNRAS
Additional file 2 of Cerebrovascular complications in patients with community-acquired bacterial meningitis: occurrence and associated factors in the COMBAT multicenter prospective cohort
Creators: name: Benadji, Amine
name: Debroucker, Thomas
name: Martin-Blondel, Guillaume
name: Argaud, Laurent
name: Vitrat, Virginie
name: Biron, Charlotte
name: Wolff, Michel
name: Hoen, Bruno
name: Duval, Xavier
name: Tubiana, Sarah
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Neuroscience
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Supplementary Material 2
Abundance analysis of targets for the COROT / MONS asteroseimology missions I. Semi-automatic abundance analysis of the gamma Dor star HD 49434
Creators: name: Bruntt, H.
name: Catala, C.
name: Garrido, R.
name: Rodriguez, E.
name: Bouret, J. C.
name: Hua, T.
name: Lignieres, F.
name: Charpinet, S.
name: Veer-Menneret, C. Van't
name: Ballereau, D.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: One of the goals of the ground-based support program for the COROT and MONS/Roemer satellite missions is to select and characterise suitable target stars for the part of the missions dedicated to asteroseismology. While the global atmospheric parameters may be determined with good accuracy from the Stromgren indices, careful abundance analysis must be made for the proposed main targets. This is a time consuming process considering the long list of primary and secondary targets. We have therefore developed new software called VWA for this task. The VWA automatically selects the least blended lines from the atomic line database VALD, and consequently adjusts the abundance in order to find the best match between the calculated and observed spectra. The variability of HD 49434 was discovered as part of COROT ground-based support observations. Here we present a detailed abundance analysis of HD 49434 using VWA. For most elements we find abundances somewhat below the Solar values, in particular we find [Fe/H] = -0.13(14). We also present the results from the study of the variability that is seen in spectroscopic and photometric time series observations. From the characteristics of the variation seen in photometry and in the line profiles we propose that HD 49434 is a variable star of the gamma Doradus type.
description: 10 pages, 6 figures
Main-sequence stellar eruption model for V838 Mon
Creators: name: Soker, Noam
name: Tylenda, Romuald
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose that the energy source of the outburst of V838 Mon and similar objects is an accretion event, i.e., gravitational energy rather than thermonuclear runaway. We show that the merger of two main sequence stars, of masses 1.5 Mo and 0.1-0.5 Mo can account for the luminosity, large radius, and low effective temperture of V838 Mon and similar objects. Subsequent cooling and gravitational contraction lead such objects to move along the Hayashi limit, as observed. By varying the masses and types of the merging stars, and by considering slowly expanding, rather than hydrostatic, envelopes, this model can account for a large range in luminosities and radii of such outburst events.
description: 9 pages
The evolution of the galaxy distribution
Creators: name: Benson, A. J.
name: Frenk, C. S.
name: Baugh, C. M.
name: Cole, S.
name: Lacey, C. G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We follow the evolution of the galaxy population in a Lambda-CDM cosmology by means of high-resolution N-body simulations in which the formation of galaxies and their observable properties are calculated using a semi-analytic model. We display images of the spatial distribution of galaxies in the simulations that illustrate its evolution and provide a qualitative understanding of the processes responsible for various biases that develop. We consider three specific statistical measures of clustering at z=1 and z=0: the correlation length (in real- and redshift-space) of galaxies of different luminosity, the morphology-density relation and the genus curve of the topology of galaxy isodensity surfaces. For galaxies with luminosity below L*, the z=0 correlation length depends very little on the luminosity of the sample, but for brighter galaxies it increases very rapidly, reaching values in excess of 10Mpc/h. The "accelerated" dynamical evolution experienced by galaxies in rich clusters, which is partly responsible for this effect, also results in a strong morphology-density relation. Remarkably, this relation is already well-established at z=1. The genus curves of the galaxies are significantly different from the genus curves of the dark matter but this is not due to genuine topological differences but rather to the sparse sampling of the density field provided by galaxies. The predictions of our model at z=0 will be tested by forthcoming data from the 2dF and Sloan galaxy surveys, and those at z=1 by the DEEP and VIRMOS surveys.
description: 18 pages, 9 figures. Submitted to MNRAS. High-resolution copies of the colour figures can be found at http://www.astro.caltech.edu/~abenson/Mocks/mocks.html
Rhagiosoma chapuisi Sekerka, 2007, nom. nov.
Creators: name: Sekerka, Lukáš
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Rhagiosoma
Rhagiosoma chapuisi

description: Rhagiosoma chapuisi nom. nov.
(Figs. 2 a-c)
 Rhagiosoma madagascariense Chapuis, 1878: cxliv (nec Mecynodera madagascariensis Heyden, 1877). Megamerus madagascariensis: MONRÓS (1956): 107, MONRÓS (1958): 5.
 Type locality. ‘Madagascar’.
 Type material. LECTOTYPE (designated here): J, ‘Coll.et.detrm. / Dr.Chapuis [w, p, bb, h] // Coll. Chapuis [w, p, s] // 1590 [w, p, s] // Madagascar [violet, p, s] // Type [w, p, s] // Coll. R. I. Sc. N. B. [blue, p, h; preceding two labels glued on this label] // TYPE [red, p, bb, h]’ (IRSN). PARALECTOTYPES: J, ‘Coll.et.detrm. / Dr.Chapuis [w, p, bb, h] // Coll. Chapuis [w, p, s] // 1592 [w, p, s] // Madagascar [violet, p, s] // M.R.Belg. [w, p, s] // Coll. R. I. Sc. N. B. [blue, p, h; preceding two labels glued on this label] // Para- / type [orange, p, bb, h]’ (IRSN); J, ‘Coll.et.detrm. / Dr.Chapuis [w, p, bb, h] // v. Krogh [w, hw, bb, s] // Coll. Chapuis [w, p, s] // 1590 [w, p, s] // Madagascar [violet, p, s] // M.R.Belg. [w, p, s] // Coll. R. I. Sc. N. B. [blue, p, h; preceding two labels glued on this label] // Para- / type [orange, p, bb, h]’ (IRSN); ♀, ‘Coll.et.detrm. / Dr.Chapuis [w, p, bb, h] // Coll. Chapuis [w, p, s] // Madagascar [violet, p, s] // Type. [w, p, s] // Coll. R. I. Sc. N. B. [blue, p, h; preceding two labels glued on this label] // Allo- / TYPE [red, p, bb, h, first row hw]’ (IRSN); J, ‘TYPE [red, p, bb, h] // TYPE [r, p, h] // MUSÉE DU CONGO / Madagascar / Coll. Clavareau [w, p, h, middle row hw] // Madagascar / Coll. Chapuis [w, hw, h] // Rhagiosoma / madagascariense / TYPE Chp. [w, hw, h] // R. DÉT. / C / 1795 [w, p, h, middle row hw] // J [w, p, h]’ (MRAC). The specimens are provided with the following label: ‘ LECTOTYPUS [or PARALECTOTYPUS] / Rhagiosoma / madagascariense / Chapuis, 1878 / L. Sekerka des. 2006 [red, p, bb, h]’.
 Distribution. Madagascar.
 Comments. Based on the examination of the type material, Mecynodera madagascariensis fully corresponds with the generic characters of Rhagiosoma, and I propose a new combination, R. madagascariense (Heyden, 1877), comb. nov. Thus, R. madagascariense Chapuis, 1878, nec Heyden, 1877, becomes its junior secondary homonym. Rhagiosoma chapuisi nom. nov. is proposed here as a new substitute name for R. madagascariense Chapuis, 1878, nec Heyden, 1877.
 I found constant differences between R. madagascariense and R. chapuisi nom. nov. based on the study of the type material. Differential diagnosis and additional comments are given under R. madagascariense.
description: Published as part of Sekerka, Lukáš, 2007, On the genus Rhagiosoma and the identity of R. madagascariense (Coleoptera: Chrysomelidae: Sagrinae: Megamerini), pp. 195-202 in Acta Entomologica Musei Nationalis Pragae 47 on pages 197-198, DOI: 10.5281/zenodo.5328315
A quantum emitter coated with graphene interacting in the strong coupling regime
Creators: name: Günay, Mehmet
name: Karanikolas, Vasilios
name: Sahin, Ramazan
name: Ovali, Rasim Volga
name: Bek, Alpan
name: Tasgin, Mehmet Emre
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: Plasma Physics (physics.plasm-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We demonstrate the strong coupling of a quantum dot and a graphene spherical shell coating it. Our simulations are the exact solutions of 3D Maxwell equations. Interaction produces sharp hybrid modes, even when the two are off-resonant, which are voltage-tunable (continuously) in an 80 meV interval. Despite a voltage-tunable quantum dot, the coupling of the light to these "very sharp" plexcitonic resonances is an order of magnitude larger than its coupling to a quantum dot. Hence, our results are very attractive for sensing applications and graphene display technologies with sharper colors. Moreover, on a simple theoretical model, we explain why such sharp, highly tunable, resonances emerge.
description: 7 pages, 7 figures