cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Best Portfolio Management Strategies For Synthetic and Real Assets
Creators: name: Gruszka, Jarosław
name: Szwabiński, Janusz
Publisher: name: arXiv
Year: 2019
Subjects: subject: Portfolio Management (q-fin.PM)
subject: FOS: Economics and business
subject: 91G10, 91G60

description: Managing investment portfolios is an old and well know problem in multiple fields including financial mathematics and financial engineering as well as econometrics and econophysics. Multiple different concepts and theories were used so far to describe methods of handling with financial assets, including differential equations, stochastic calculus and advanced statistics. In this paper, using a set of tools from the probability theory, various strategies of building financial portfolios are analysed in different market conditions. A special attention is given to several realisations of a so called balanced portfolio, which is rooted in the natural "buy-low-sell-high" principle. Results show that there is no universal strategy, because they perform differently in different circumstances (e.g. for varying transaction costs). Moreover, the planned time of investment may also have a significant impact on the profitability of certain strategies. All methods have been tested with both simulated trajectories and real data from the Polish stock market.
description: 19 pages, 8 figures
Additional file 1: of Evaluation of treatment response in adults with relapsing MOG-Ab-associated disease
Creators: name: Cobo-Calvo, Alvaro
name: Sepúlveda, María
name: Rollot, Fabien
name: Thais Armangué
name: Ruiz, Anne
name: Maillart, Elisabeth
name: Papeix, Caroline
name: Audoin, Bertrand
name: Zephir, Helene
name: Biotti, Damien
name: Ciron, Jonathan
name: Francoise Durand-Dubief
name: Collongues, Nicolas
name: Ayrignac, Xavier
name: Labauge, Pierre
name: Thouvenot, Eric
name: Bourre, Bertrand
name: Montcuquet, Alexis
name: Cohen, Mikael
name: Deschamps, Romain
name: Solà-Valls, Nuria
name: Llufriu, Sara
name: Seze, Jerome De
name: Blanco, Yolanda
name: Vukusic, Sandra
name: Saiz, Albert
name: Marignier, Romain
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Marine Biology
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences
subject: Computational Biology

description: Table S1.Treatment regimens and intervals. Table S2 Characteristics in patients with MOG antibodies and multiple sclerosis. Table S3 Comparison of baseline possible confounders between treated and non-treated patients in the original sample. Table S4 Comparison of baseline possible confounders between treated and non-treated patients in the pseudo-population. Table S5 Patients who received combined drugs and reasons for inclusion/exclusion in different analyses. (DOCX 28 kb)
The effect of rotation on the thermal instability of stratified galactic atmospheres - I. Local analysis
Creators: name: Sobacchi, Emanuele
name: Sormani, Mattia
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Observations show that (i) multiple gas phases can coexist in the atmospheres of galaxies and clusters; (ii) these atmospheres may be significantly rotating in the inner parts, with typical velocities that approach or even exceed the local sound speed. The thermal instability is a natural candidate to explain the formation of cold structures via condensation of a hotter gas phase. Here we systematically study the effect of rotation on the thermal stability of stratified plane-parallel atmospheres, using both analytical arguments and numerical simulations. We find that the formation of cold structures starting from small isobaric perturbations is enhanced in the regions where the rotation of the system is dynamically important (i.e. when the rotational velocity becomes comparable to the sound speed). In particular, the threshold value of the ratio between the cooling and dynamical time $t_{\rm cool}/t_{\rm dyn}$ below which condensations can form is increased by a factor up to $\sim 10$ in the presence of significant rotation. We briefly discuss the implications of our results for galaxies and clusters.
description: Accepted for publication in MNRAS. Animations of all the simulations in the paper can be downloaded at the following url: https://www.ita.uni-heidelberg.de/~mattia/download/therm/paper_I.zip
Additional file 4: of PHF8 upregulation contributes to autophagic degradation of E-cadherin, epithelial-mesenchymal transition and metastasis in hepatocellular carcinoma
Creators: name: Zhou, Wuhua
name: Gong, Li
name: Wu, Qinchuan
name: Xing, Chunyang
name: Wei, Bajin
name: Chen, Tianchi
name: Zhou, Yuan
name: Yin, Shengyong
name: Jiang, Bin
name: Xie, Haiyang
name: Zhou, Lin
name: Zheng, Shusen
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Cancer

description: Table S3. Oligonucleotide sequences of primers for ChIP. (DOCX 16 kb)
High Energy Spectral Components in Gamma-Ray Burst Afterglows
Creators: name: Zhang, Bing
name: Meszaros, Peter
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate two high energy radiation mechanisms, the proton synchrotron and the electron inverse Compton emission, and explore their possible signatures in the broad-band spectra and in the keV to GeV light curves of gamma-ray burst afterglows. We develop a simple analytical approach, allowing also for the effects of photon-photon pair production, and explore the conditions under which one or the other of these components dominates. We identify three parameter space regions where different spectral components dominate: (I) a region where the proton synchrotron and other hadron-related emission components dominate, which is small; (II) a region where the electron inverse Compton component dominates, which is substantial; (III) a third substantial region where electron synchrotron dominates. We discuss the prospects and astrophysical implications of directly detecting the inverse Compton and the proton high energy components in various bands, in particular in the GeV band with future missions such as GLAST, and in the X-ray band with Chandra. We find that regime II parameter space is the most favorable regime for high energy emission. The inverse Compton component is detectable by GLAST within hours for bursts at typical cosmological distances, and by Chandra in days if the ambient density is high.
description: ApJ in press; revised version with slight changes, aastex, 26 pages, 6 figures
Additional file 1: of Ultrasound inflammatory parameters and Treg/Th17 cell profiles in established rheumatoid arthritis
Creators: name: Prado, Aline
name: Bisi, Melissa
name: Deise Piovesan
name: Bredemeier, Markus
name: Talita Baptista
name: Petersen, Laura
name: Bauer, Moises
name: Silveira, Inês
name: Mendonça, José
name: Staub, Henrique
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Figure S1. Association of percentage of Th-17 lymphocytes and 10-joint pD score.(rS = Spearman correlation coefficient, n = 90). (DOC 48 kb)
Additional file 10 of circEXOC6B interacting with RRAGB, an mTORC1 activator, inhibits the progression of colorectal cancer by antagonizing the HIF1A-RRAGB-mTORC1 positive feedback loop
Creators: name: Li, Xiaomin
name: Wang, Jianjun
name: Lin, Weihao
name: Yuan, Qinzi
name: Lu, Yanxia
name: Wang, Haowei
name: Chen, Yujia
name: Chen, Lixia
name: Dai, Peiling
name: Long, Huaicheng
name: Li, Xuenong
Publisher: name: figshare
Year: 2022
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 10: Supplementary Table S1. Primer sequences are used in PCR or RT- qPCR.
title: Dietary, Pharmacological, and Physiological Strategies to Manipulate Acute Energy Balance
Creators: name: Schubert, Matthew M
Publisher: name: Griffith University
Year: 2015
Subjects: subject: Obesity
subject: Weight gain
subject: Pharmacological strategies
subject: Dietary strategies
subject: Caffiene and diet
subject: Coffee and diet
subject: Hormones related to appetite

description: Weight gain and obesity are significant public health problems. Weight gain results from a shift in energy balance, when an individual consumes more energy than required for their given energy expenditure. As such, health professionals, scientists, and governing bodies are striving to find effective interventions that will return the energy balance equation to neutral levels, or manipulate the equation in a negative direction to induce weight loss. Physiological manipulations, such as exercise, are inexpensive and effective at influencing energy balance. Pharmacological and dietary strategies, such as caffeine and coffee, have been less examined. Exercise, coffee, and caffeine are relatively prevalent in modern societies. Therefore, improving our understanding of how these manipulations interact with respect to factors influencing energy balance is of high importance. This thesis comprises a series of studies that aim to examine the influence of exercise, nutritional (coffee/caffeine) manipulations, and their combination, on factors that influence energy balance. The specific aims are to 1) determine how acute exercise influences subsequent energy intake over a period of less than 24 h; 2) determine how acute exercise influences hormones related to appetite (acylated ghrelin, peptide YY, pancreatic polypeptide, and glucagon-like peptide-1) and whether these hormonal changes relate to post-exercise alterations in energy intake; 3) examine how caffeine and/or coffee influence appetite, gastric emptying, and energy intake; and 4) determine how caffeine consumed before and after a bout of exercise influences acute energy balance.
Stellar Populations and Star Cluster Formation in Interacting Galaxies with the Advanced Camera for Surveys
Creators: name: de Grijs, Richard
name: Lee, Jessica T.
name: Herrera, M. Clemencia Mora
name: Alvensleben, Uta Fritze-v.
name: Anders, Peter
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Pixel-by-pixel colour-magnitude and colour-colour diagrams - based on a subset of the Hubble Space Telescope Advanced Camera for Surveys Early Release Observations - provide a powerful technique to explore and deduce the star and star cluster formation histories of the Mice and the Tadpole interacting galaxies. In each interacting system we find some 40 bright young star clusters (20 <= F606W (mag) <= 25, with a characteristic mass of ~3 x 10^6 Msun), which are spatially coincident with blue regions of active star formation in their tidal tails and spiral arms. We estimate that the main events triggering the formation of these clusters occurred ~(1.5-2.0) x 10^8 yr ago. We show that star cluster formation is a major mode of star formation in galaxy interactions, with >= 35% of the active star formation in encounters occurring in star clusters. This is the first time that young star clusters have been detected along the tidal tails in interacting galaxies. The tidal tail of the Tadpole system is dominated by blue star forming regions, which occupy some 60% of the total area covered by the tail and contribute ~70% of the total flux in the F475W filter (decreasing to ~40% in F814W). The remaining pixels in the tail have colours consistent with those of the main disk. The tidally triggered burst of star formation in the Mice is of similar strength in both interacting galaxies, but it has affected only relatively small, spatially coherent areas.
description: 23 pages in preprint form, 6 (encapsulated) postscript figures; accepted for publication in New Astronomy; ALL figures (even the grey-scale ones) need to be printed on a colour printer style files included; for full-resolution paper, see http://www.ast.cam.ac.uk/STELLARPOPS/ACSpaper/
Coelogyne simplicissima M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne simplicissima

description: Coelogyne simplicissima (J.J.Sm.) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum simplicissimum J.J.Sm., Bull. Jard. Bot. Buitenzorg, sér. 2, 25: 15 (1917).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 127, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
Using Acoustic Perturbations to Dynamically Tune Shear Thickening in Colloidal Suspensions
Creators: name: Sehgal, Prateek
name: Ramaswamy, Meera
name: Cohen, Itai
name: Kirby, Brian J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Colloidal suspensions in industrial processes often exhibit shear thickening that is difficult to control actively. Here, we use piezoelectric transducers to apply acoustic perturbations to dynamically tune the suspension viscosity in the shear-thickening regime. We attribute the mechanism of dethickening to the disruption of shear-induced force chains via perturbations that are large relative to the particle roughness scale. The ease with which this technique can be adapted to various flow geometries makes it a powerful tool for actively controlling suspension flow properties and investigating system dynamics.
description: 21 pages, 14 figures
Additional file 1: of Quadriceps muscle activity during commonly used strength training exercises shortly after total knee arthroplasty: implications for home-based exercise-selection
Creators: name: Jakobsen, Thomas
name: Jakobsen, Markus
name: Andersen, Lars
name: Husted, Henrik
name: Kehlet, Henrik
name: Bandholm, Thomas
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Plant Biology

description: Exercise description. (DOCX 1742 kb)
The triggered star formation in rotating disks
Creators: name: Palous, J.
name: Ehlerova, S.
name: Elmegreen, B. G.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The gravitational instability of expanding shells triggering the formation of clouds and stars is analyzed. Disks with different scale-heights, ambient and shell velocity dispersions, mid-plane densities, rotation rates and shear rates are explored with three dimensional numerical simulations in the thin shell approximation. Three conditions for the shell collapse are specified: the first is that it happens before a significant blow-out, the second requires that the shell collapses before it is distorted by Coriolis forces and shear, and the third requires that the internal pressure in the accumulated gas is small and the fragmentation is achieved within the expansion time. The gas-rich and slowly rotating galaxies are the best sites of the triggered star formation, concluding that its importance has been much larger at the times of galaxy formation compared to the present epoch.
description: 4 pages, to be published in the proceedings of the Euroconference "The Evolution of Galaxies II - Basic building blocks", ed. M. Sauvage, G. Stasinska, L. Vigroux, D. Schaerer, S. Madden
Routine SARS‐CoV‐2 vaccination for all children
Creators: name: De Paris, Kristina
name: Permar, Sallie R.
Publisher: name: Wiley
Year: 2022

description:
The SARS-CoV-2 pandemic has resulted in unprecedented health and economic losses. Children generally present with less severe disease from this virus compared with adults, yet neonates and children with COVID-19 can require hospitalization, and older children can develop severe complications, such as the multisystem inflammatory syndrome, resulting in >1500 deaths in children from COVID-19 since the onset of the pandemic. The introduction of effective SARS-CoV-2 vaccines in school-age children and adult populations combined with the emergence of new, more highly transmissible SARS-CoV-2 variants has resulted in a proportional increase of infections in young children. Here, we discuss (1) the current knowledge on pediatric SARS-CoV-2 infection and pathogenesis in comparison with adults, (2) the data on vaccine immunogenicity and efficacy in children, and (3) the benefits of early life SARS-CoV-2 vaccination.
"Hunt Takes Hare": Theming Games Through Game-Word Vector Translation
Creators: name: Younès, Rabii
name: Michael, Cook
Publisher: name: arXiv
Year: 2024
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Computation and Language (cs.CL)
subject: FOS: Computer and information sciences

description: A game's theme is an important part of its design -- it conveys narrative information, rhetorical messages, helps the player intuit strategies, aids in tutorialisation and more. Thematic elements of games are notoriously difficult for AI systems to understand and manipulate, however, and often rely on large amounts of hand-written interpretations and knowledge. In this paper we present a technique which connects game embeddings, a recent method for modelling game dynamics from log data, and word embeddings, which models semantic information about language. We explain two different approaches for using game embeddings in this way, and show evidence that game embeddings enhance the linguistic translations of game concepts from one theme to another, opening up exciting new possibilities for reasoning about the thematic elements of games in the future.
description: 7 pages, PCG Workshop at FDG 2024
Stability of Accretion Disks in Presence of Nucleosynthesis
Creators: name: Mukhopadhyay, Banibrata
name: Chakrabarti, Sandip K.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the effect of nuclear reaction on a thin, axisymmetric, differentially rotating, inviscid, steady accretion flow around a black hole from an analytical point of view. We find that for most of the reasonable disk parameters, when $p-p$-reaction, dissociation of deuterium and helium are taken into account, the transonic region of the disk continues to have the inner sonic point and if the temperature of the flow at the injection sonic point could be raised (by say, some heating processes) the flow would to pass through this inner sonic point. Otherwise, the flow may be unstable. We use the sonic point analysis to study the solution. In the rest of the disk parameters the inner sonic point is absent altogether and the flow will definitely be unstable.
description: 18 Latex pages, 6 figures; Accepted for publication in ApJ; aaspp4.sty
Zinc in cereal grains: Concentration, distribution, speciation, bioavailability, and barriers to transport from roots to grains in wheat
Creators: name: Aiqing, Zhao
name: Zhang, Liansheng
name: Ning, Peng
name: Chen, Qin
name: Wang, Bini
name: Zhang, Fuxin
name: Yang, Xingbin
name: Zhang, Youlin
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Plant Biology

description: Zinc (Zn) is an essential micro-nutrient for humans, and Zn deficiency is of global concern. In addition to inherited and pathological Zn deficiencies, insufficient dietary intake is leading cause, especially in those consuming cereal grains as a stable food, in which Zn concentration and bioavailability are relatively low. To improve Zn levels in the human body, it is important to understand the accumulation and bioavailability of Zn in cereal grains. In recent years, knowledge on the molecular mechanisms underlying Zn uptake, transport, homeostasis, and deposition within cereal crops has been accumulating, paving the way for a more targeted approach to improving the nutrient status of crop plants. In this paper, we briefly review existing studies on the distribution and transport pathways of Zn in major small-grained cereals, using wheat as a case study. The findings confirm that Zn transport in plants is a complex physiological process mainly governed by Zn transporters and metal chelators. This work reviews studies on Zn uptake, transport, and deposition in wheat plants, summarizes the possible barriers impairing Zn deposition in wheat grains, and describes strategies for increasing Zn concentration in wheat grains.
title: Frankfurt am Main im Klimawandel
title: eine Untersuchung zur städtischen Wärmebelastung
titleType: Subtitle
Creators: name: Früh, Barbara
name: Koßmann, Meinolf
name: Roos, Marita
Publisher: name: Freie Universität Berlin
Year: 2011
Subjects: subject: Klima
subject: Klimawandel
subject: Frankfurt am Main
subject: Stadt
subject: 500 Naturwissenschaften und Mathematik::550 Geowissenschaften, Geologie::551 Geologie, Hydrologie, Meteorologie

description: Ziel der Untersuchung war es, auf der Basis von Projektionen regionaler Klimamodelle die Auswirkungen des Klimawandels für detaillierte Stadtstrukturen aufzuzeigen. Mit Hilfe der am Beispiel Frankfurt/Main entwickelten sogenannten "Quadermethode" konnte erstmals sowohl die vergangene als auch die zukünftige Wärmebelastung für Frankfurt am Main unter Berücksichtigung der vielfältigen Bebauungsstrukturen und sonstiger Flächennutzungen simuliert werden. Auch die klimatischen Auswirkungen der größeren Planungsvorhaben der Stadt wurden in diesem Zusammenhang untersucht.
Coelogyne smithiana M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne smithiana

description: Coelogyne smithiana (Ames) M.W.Chase & Schuit., comb. nov.
 Basionym: Acoridium smithianum Ames, Blumea, Suppl. 1: 74 (1937).
 Homotypic synonym: Dendrochilum smithianum (Ames) L.O.Williams, Philipp. J. Sci. 80: 311 (1952).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 127, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
title: Allegorical and Cultural Landscapes in the Novels of Nathaniel Hawthorne and Al- Nahda Arab Writers
Creators: name: Faiq, Tatheer Assim
Publisher: name: Griffith University
Year: 2015
Subjects: subject: Nathaniel Hawthorne 1804-1864
subject: Mohammadd al-Muwaylihi 1868-1930
subject: Kahlil Gibran 1883-1931
subject: Cultural landscapes in literature
subject: Al- Nahda Arab writers
subject: Arab renaissance

description: The fictional works of American author Nathaniel Hawthorne and the Arab writers, Mohammadd al-Muwaylihi and Kahlil Gibran share an interest in allegorical landscapes which respond to political and religious tyranny. Throughout their novels, we encounter historically specific images of political corruption and religious oppression located among the urban settings of Salem, Rome, Cairo, Paris, Baalbek, and Beirut. In this thesis, these settings are considered as cultural landscapes: geographical sites which are perceived and presented allegorically within a socio-political frame. These landscapes are drawn on both realist and symbolic levels. Nathaniel Hawthorne presents the shameful burden of religious and political oppression. In works such as The Scarlet Letter and The Marble Faun where is characters are engaged in a rebellion against their cultural institutions to show the defects of such religious and political institutions. For Hawthorne, Boston forest becomes a place that witnesses the birth of the new female rebel to defy the very foundations of the Puritan society. Rome becomes a historical setting where crime survives during the course of the rise and fall of civilisations as reflected in art galleries, churches and ruins: a reality of human destruction that is equally recognized by American and European characters. Al- Muwaylihi’s Hadith Isa Ibn Hisham draws a socio political picture of Egyptian life through the representation of nineteenth century Cairo with its complex streets and buildings. In his second part of the book, al- Muwaylihi presents a journey from Cairo to Paris in which his characters, brutalized by colonial practices, seek the values of modernity at the heart of Europe. Such a journey defied the political and Islamic institutions of his age. For al- Muwaylihi, Parisian sites are symbols of technology and modernity, while Cairo emblematizes the city of conflict as the inhabitants face new social changes through encounters with the European colonizers.
Galaxy Formation: Warm Dark Matter, Missing Satellites, and the Angular Momentum Problem
Creators: name: Goetz, Martin
name: Sommer-Larsen, Jesper
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present warm dark matter (WDM) as a possible solution to the missing satellites and angular momentum problem in galaxy formation and introduce improved initial conditions for numerical simulations of WDM models, which avoid the formation of unphysical haloes found in earlier simulations. There is a hint, that the mass function of satellite haloes has been overestimated so far, pointing to higher values for the WDM particle mass.
description: 5 pages, 2 figures, submitted to the proceedings of the Euroconference "Galaxy Evolution - III. From simple approaches to self-consistent models", Kiel, 2002. A high-quality version of Fig. 1 can be downloaded from http://www.tac.dk/~gotz/goetz.fig1.eps; some minor and a major typo corrected
Probing the local electronic structure of isovalent Bi atoms in InP
Creators: name: Krammel, C. M.
name: da Cruz, A. R.
name: Flatté, M. E.
name: Roy, M.
name: Maksym, P. A.
name: Zhang, L. Y.
name: Wang, K.
name: Li, Y. Y.
name: Wang, S. M.
name: Koenraad, P. M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Cross-sectional scanning tunneling microscopy (X-STM) is used to experimentally study the influence of isovalent Bi atoms on the electronic structure of InP. We map the spatial pattern of the Bi impurity state, which originates from Bi atoms down to the sixth layer below the surface, in topographic, filled state X-STM images on the natural $\{110\}$ cleavage planes. The Bi impurity state has a highly anisotropic bowtie-like structure and extends over several lattice sites. These Bi-induced charge redistributions extend along the $\left\langle 110\right\rangle$ directions, which define the bowtie-like structures we observe. Local tight-binding calculations reproduce the experimentally observed spatial structure of the Bi impurity state. In addition, the influence of the Bi atoms on the electronic structure is investigated in scanning tunneling spectroscopy measurements. These measurements show that Bi induces a resonant state in the valence band, which shifts the band edge towards higher energies. This is in good agreement to first principles calculations. Furthermore, we show that the energetic position of the Bi induced resonance and its influence on the onset of the valence band edge depend crucially on the position of the Bi atoms relative to the cleavage plane.
Convection physics and tidal synchronization of the subdwarf binary NY Virginis
Creators: name: Preece, Holly P.
name: Tout, Christopher A.
name: Jeffery, C. Simon
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Asteroseismological analysis of NY Vir suggests that at least the outer 55 per cent of the star (in radius) rotates as a solid body and is tidally synchronized to the orbit. Detailed calculation of tidal dissipation rates in NY Vir fails to account for this synchronization. Recent observations of He core burning stars suggest that the extent of the convective core may be substantially larger than that predicted with theoretical models. We conduct a parametric investigation of sdB models generated with the Cambridge STARS code to artificially extend the radial extent of the convective core. These models with extended cores still fail to account for the synchronization. Tidal synchronization may be achievable with a non-MLT treatment of convection.
description: 7 Pages, 7 Figures, 1 Table, Submitted 21/12/2018, Accepted 20/02/2019 MNRAS
Additional file 2 of Intratumor heterogeneity and T cell exhaustion in primary CNS lymphoma
Creators: name: Heming, Michael
name: Haessner, Svea
name: Wolbert, Jolien
name: Lu, I-Na
name: Li, Xiaolin
name: Brokinkel, Benjamin
name: Müther, Michael
name: Holling, Markus
name: Stummer, Walter
name: Thomas, Christian
name: Schulte-Mecklenbeck, Andreas
name: de Faria, Flavia
name: Stoeckius, Marlon
name: Hailfinger, Stephan
name: Lenz, Georg
name: Kerl, Kornelius
name: Wiendl, Heinz
name: Meyer zu Hörste, Gerd
name: Grauer, Oliver M.
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 2: Supplementary Methods.
Additional file 1: of From bench to bedside: in vitro and in vivo evaluation of a neonate-focused nebulized surfactant delivery strategy
Creators: name: F. Bianco
name: F. Ricci
name: C. Catozzi
name: X. Murgia
name: M. Schlun
name: A. Bucholski
name: U. Hetzer
name: S. Bonelli
name: M. Lombardini
name: E. Pasini
name: M. Nutini
name: M. Pertile
name: S. Minocchieri
name: M. Simonato
name: B. Rosa
name: G. Pieraccini
name: G. Moneti
name: L. Lorenzini
name: S. Catinella
name: G. Villetti
name: M. Civelli
name: B. Pioselli
name: P. Cogo
name: V. Carnielli
name: C. Dani
name: F. Salomone
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer

description: Table S1. Baseline and post lung injury (Post-BAL) characteristics of surfactant-depleted adult rabbits treated with nasal continuous positive pressure ventilation (nCPAP), with intratracheal surfactant (Inst-SURF), or with different doses of nebulized surfactant (Neb-SURF100, Neb-SURF200, Neb-SURF400, and Neb-SURF600. Figure S1. PrINT cast with silicon-coated nostrils. Figure S2. Nebulizer output assessment. (DOCX 239 kb)
Anatheta planulicollis
Creators: name: Ashe, James S.
name: Gusarov, Vladimir I.
Publisher: name: Zenodo
Year: 2003
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Anatheta
Anatheta planulicollis

description: Anatheta planulicollis (Casey 1910)
(Figs. 1–17)
description: Published as part of Ashe, James S. & Gusarov, Vladimir I., 2003, Review of Anatheta Casey (Staphylinidae: Aleocharinae: Athetini), with Notes on Synonymy of Canastota Casey and Silusida Casey, pp. 27-36 in The Coleopterists Bulletin 57 (1) on page 32, DOI: 10.1649/0010-065X(2003)057[0027:ROACSA]2.0.CO;2, http://zenodo.org/record/10103389
Eigenfunctions of Galactic Phase Space Spirals from Dynamic Mode Decomposition
Creators: name: Darling, Keir
name: Widrow, Lawrence M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate the spatiotemporal structure of simulations of the homogeneous slab and isothermal plane models for the vertical motion in the Galactic disc. We use Dynamic Mode Decomposition (DMD) to compute eigenfunctions of the simulated distribution functions for both models, referred to as DMD modes. In the case of the homogeneous slab, we compare the DMD modes to the analytic normal modes of the system to evaluate the feasibility of DMD in collisionless self gravitating systems. This is followed by the isothermal plane model, where we focus on the effect of self gravity on phase mixing. We compute DMD modes of the system for varying relative dominance of mutual interaction and external potential, so as to study the corresponding variance in mode structure and lifetime. We find that there is a regime of relative dominance, at approximately $ 4:1 $ external potential to mutual interaction where the DMD modes are spirals in the $ (z,v_z) $ plane, and are nearly un-damped. This leads to the proposition that a system undergoing phase mixing in the presence of weak to moderate self gravity can have persisting spiral structure in the form of such modes. We then conclude with the conjecture that such a mechanism may be at work in the phase space spirals observed in Gaia Data Release 2, and that studying more complex simulations with DMD may aid in understanding both the timing and form of the perturbation that lead to the observed spirals.
description: 8 pages, 6 figures
Holographic Entropy Relations Repackaged
Creators: name: He, Temple
name: Headrick, Matthew
name: Hubeny, Veronika E.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We explore the structure of holographic entropy relations (associated with 'information quantities' given by a linear combination of entanglement entropies of spatial sub-partitions of a CFT state with geometric bulk dual). Such entropy relations can be recast in multiple ways, some of which have significant advantages. Motivated by the already-noted simplification of entropy relations when recast in terms of multipartite information, we explore additional simplifications when recast in a new basis, which we dub the K-basis, constructed from perfect tensor structures. For the fundamental information quantities such a recasting is surprisingly compact, in part due to the interesting fact that entropy vectors associated to perfect tensors are in fact extreme rays in the holographic entropy cone (as well as the full quantum entropy cone). More importantly, we prove that all holographic entropy inequalities have positive coefficients when expressed in the K-basis, underlying the key advantage over the entropy basis or the multipartite information basis.
description: 38 pages, 1 pdf figure; v2: fixed minor typos and added clarification comments, JHEP version
Measured Mass Loss Rates of Solar-like Stars as a Function of Age and Activity
Creators: name: Wood, Brian E.
name: Mueller, Hans-Reinhard
name: Zank, Gary P.
name: Linsky, Jeffrey L.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Collisions between the winds of solar-like stars and the local ISM result in a population of hot hydrogen gas surrounding these stars. Absorption from this hot H I can be detected in high resolution Lyman-alpha spectra of these stars from the Hubble Space Telescope. The amount of absorption can be used as a diagnostic for the stellar mass loss rate. We present new mass loss rate measurements derived in this fashion for four stars (Epsilon Eri, 61 Cyg A, 36 Oph AB, and 40 Eri A). Combining these measurements with others, we study how mass loss varies with stellar activity. We find that for the solar-like GK dwarfs, the mass loss per unit surface area is correlated with X-ray surface flux. Fitting a power law to this relation yields Mdot ~ Fx^(1.15+/-0.20). The active M dwarf Proxima Cen and the very active RS CVn system Lambda And appear to be inconsistent with this relation. Since activity is known to decrease with age, the above power law relation for solar-like stars suggests that mass loss decreases with time. We infer a power law relation of Mdot ~ t^(-2.00+/-0.52). This suggests that the solar wind may have been as much as 1000 times more massive in the distant past, which may have had important ramifications for the history of planetary atmospheres in our solar system, that of Mars in particular.
description: 34 pages, 9 figures; AASTEX v5.0 plus EPSF extensions in mkfig.sty; accepted by ApJ
Evidence for a Molecular Cloud Origin for Gamma-Ray Bursts: Implications for the Nature of Star Formation in the Universe
Creators: name: Reichart, Daniel E.
name: Price, Paul A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It appears that the majority of rapidly-, well-localized gamma-ray bursts with undetected, or dark, optical afterglows, or `dark bursts' for short, occur in clouds of size R > 10L_{49}^{1/2} pc and mass M > 3x10^5L_{49} M_{sun}, where L is the isotropic-equivalent peak luminosity of the optical flash. We show that clouds of this size and mass cannot be modeled as a gas that is bound by pressure equilibrium with a warm or hot phase of the interstellar medium (i.e., a diffuse cloud): Such a cloud would be unstable to gravitational collapse, resulting in the collapse and fragmentation of the cloud until a burst of star formation re-establishes pressure equilibrium within the fragments, and the fragments are bound by self-gravity (i.e., a molecular cloud). Consequently, dark bursts probably occur in molecular clouds, in which case dark bursts are probably a byproduct of this burst of star formation if the molecular cloud formed recently, and/or the result of lingering or latter generation star formation if the molecular cloud formed some time ago. We then show that if bursts occur in Galactic-like molecular clouds, the column densities of which might be universal, the number of dark bursts can be comparable to the number of bursts with detected optical afterglows: This is what is observed, which suggests that the bursts with detected optical afterglows might also occur in molecular clouds. We confirm this by modeling and constraining the distribution of column densities, measured from absorption of the X-ray afterglow, of the bursts with detected optical afterglows: We find that this distribution is consistent with the expectation for bursts that occur in molecular clouds, and is not consistent with the expectation for bursts that occur in diffuse clouds. More...
description: Accepted to The Astrophysical Journal, 22 pages, 6 figures, LaTeX
title: Navigating the Health Care System: Movement and Meaning for Older People with Dementia
Creators: name: Namiki, Satoko
Publisher: name: Griffith University
Year: 2014
Subjects: subject: Dementia
subject: Health care system
subject: Aged care
subject: Acute care system

description: Older people with dementia are significant users of both long-term care and acute care services. The transitions between these services are not always smooth and very little is known about the meaning that such transitions have for people with dementia. This study aimed to explore the journeys of residential aged care facility (RACF) residents with dementia as they transition through the acute care system, and to investigate the system features and continuity of care (COC) issues that serve to shape the meanings that these transitions have for these people. The study addresses the following two research questions: 1. What meanings do people with dementia construct from their multiple transition experiences? 2. What are the factors that affect COC, and therefore, have an impact on the transition experiences of people with dementia through the system? This study was guided by a critical social constructionism paradigm and employed a whole-system design and narrative methods. This approach enabled the researcher to explore ‘the person in the system’. Data were collected through mixed methods including transfer tracking, formal interviews, observations, chart audit, and document review. Data analysis was undertaken using a narrative analysis approach that acknowledged people’s ability to construct their own meaning within particular contexts.
A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes
Creators: name: Freundlich, Jonathan
name: Dekel, Avishai
name: Jiang, Fangzhou
name: Ishai, Guy
name: Cornuault, Nicolas
name: Lapiner, Sharon
name: Dutton, Aaron A.
name: Maccio, Andrea V.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a simple model for the response of a dissipationless spherical system to an instantaneous mass change at its center, describing the formation of flat cores in dark matter haloes and ultra-diffuse galaxies (UDGs) from feedback-driven outflow episodes in a specific mass range. This model generalizes an earlier simplified analysis of an isolated shell into a system with continuous density, velocity and potential profiles. The response is divided into an instantaneous change of potential at constant velocities due to a given mass loss or gain, followed by energy-conserving relaxation to a new Jeans equilibrium. The halo profile is modeled by a two-parameter function with a variable inner slope and an analytic potential profile (Dekel et al. 2017), which enables determining the associated kinetic energy at equilibrium. The model is tested against NIHAO cosmological zoom-in simulations, where it successfully predicts the evolution of the inner dark-matter profile between successive snapshots in about 75% of the cases, failing mainly in merger situations. This model provides a simple understanding of the formation of dark-matter halo cores and UDGs by supernova-driven outflows, and a useful analytic tool for studying such processes.
description: 27 pages, 22 figures, accepted by MNRAS
Remarks on the Cosmic Density of Degenerate Neutrinos
Creators: name: Ichikawa, Kazuhide
name: Kawasaki, M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We re-investigate the evolution of the strongly degenerate neutrinos in the early universe. With the larger degeneracy, the neutrino number freezes at higher temperatures because the neutrino annihilation rate decreases. We consider very large degeneracy so large that the neutrino number freezes before events in which the particle degrees of freedom in the universe decrease (e.g. the muon annihilation and the quark-hadron phase transition). In such a case, the degeneracy by the time of nucleosynthesis becomes smaller than the initial degeneracy. We calculate how much it decreases from the initial value on the basis of the conservation of the neutrino number and the total entropy. We found a large drop in the degeneracy but it is not large enough to affect the current constraints on the neutrino degeneracy from BBN and CMBR.
description: 14 pages, 5 figures
title: Controlling Non-Classical States of Light: Experimental Techniques in Quantum Information Science
Creators: name: Kocsis, Alexander (Sacha) Julien
Publisher: name: Griffith University
Year: 2014
Subjects: subject: Optical quantum information science
subject: Quantum information science
subject: Photonic quantum information science
subject: Quantum networks
subject: Non-classical states of light

description: The key task of transmitting quantum states encompasses a diverse array of tech- niques and applications. This thesis presents experimental work in optical quantum information science, focused on strategies for transmitting quantum states with high fidelity and security. The majority of the work in this thesis is in photonic quantum information science, although one experiment used continuous–variable states. In the first experiment, the noiseless amplification of a photon polarisation qubit was realised, using delocalised single photon ancilla states and two single–mode amplification stages operating coherently. Artificial loss was applied to a single photon, to simulate a loss in a long–distance quantum transmission channel, and for the highest gain setting that was investigated, the qubit amplifier achieved a five–fold increase in transmission fidelity. In the second experiment, linear optical techniques for distributing mode entangle- ment in a quantum network were studied. Quantum networks are based on a series of nodes, potentially separated by significant distances, and connected via quantum repeaters. Different quantum repeater architectures have been proposed, but they all include embedded distillation stages, which are based on linear optical techniques. We simulate two distinct quantum repeater scenarios, using different configurations of an entanglement swapping stage, a noiseless single–mode amplification stage, and loss. The performance of the amplification stage in overcoming the loss is characterised in both configurations. Significant distillation of mode entanglement is achieved in one configuration, and an increase in mode coherence is achieved in the other configuration.