cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
“…Lingua di comunicazione” e “lingua d’approfondimento…”: i bambini migranti e la lingua seconda della scuola ticinese
Creators: name: Rigassi, Tina
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2011

description: Ho preso spunto dalla grounded theory per costruire una teoria a partire dai dati raccolti sul campo. Tramite lo strumento dell’intervista ho raccolto le opinioni di figure professionali attive nel campo dell’educazione in una realtà scolastica particolarmente multiculturale. Il tema del lavoro di ricerca è: “La lingua come elemento di difficoltà all’interno della scuola in una realtà multiculturale” e la domanda di ricerca è: “Che importanza ha una stimolazione linguistica precoce in un contesto dove risalta il trinomio integrazione – lingua – apprendimento?” poiché la preoccupazione principale di un docente di prima elementare intervistato è legata all’apprendimento della lingua seconda degli allievi alloglotti. I bambini migranti della sua classe, anche se per la maggior parte nati in Ticino, hanno un linguaggio molto povero, “di comunicazione” che però con consente di approfondire. Dai dati raccolti, la “lingua di approfondimento” viene percepita come un bagaglio linguistico fondamentale per permettere al bambino migrante di apprendere e riuscire nel suo percorso formativo. Il docente dice che il motivo di questa “povertà” è legato alla mancanza di una stimolazione linguistica precoce. In questo lavoro di ricerca rifletto sull’importanza di una stimolazione linguistica precoce che potrebbe trovare terreno fertile all’interno della scuola dell’infanzia nella quale è in corso una sperimentazione che promuove l’inserimento della figura del docente di lingua e integrazione. Relatore: Fabio Leoni
Treecode and fast multipole method for N-body simulation with CUDA
Creators: name: Yokota, Rio
name: Barba, Lorena
Publisher: name: arXiv
Year: 2010
Subjects: subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: Due to the variety and importance of applications of treecodes and FMM, the combination of algorithmic acceleration with hardware acceleration can have tremendous impact. Alas, programming these algorithms efficiently is no piece of cake. In this contribution, we aim to present GPU kernels for treecode and FMM in, as much as possible, an uncomplicated, accessible way. The interested reader should consult some of the copious literature on the subject for a deeper understanding of the algorithms themselves. Here, we will offer the briefest of summaries. We will focus our attention on achieving a GPU implementation that is efficient in its utilization of the architecture, but without applying the most advanced techniques known in the field (which would complicate the presentation).
The Accreting White Dwarf in SS Cygni Revealed
Creators: name: Sion, Edward
name: Godon, Patrick
name: Myzcka, Janine
name: Blair, William
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have carried out a combined Hubble Space Telescope (HST/GHRS) and Far Ultraviolet Spectroscopic Explorer FUSE) analysis of the prototype dwarf nova SS Cygni during quiescence. The FUSE and HST spectra were obtained at comparable times after outburst and have matching flux levels where the two spectra overlap. In our synthetic spectral analysis, we have used SS Cygni's accurate HST FGS parallax giving d = 166pc, a newly determined mass for the accreting white dwarf (Bitner et al. 2007) of Mwd=0.81Msun (lower than the previous, widely used 1.2 Msun) and the reddening E_{B-V} values 0.04 (Verbunt 1987; La Dous 1991) and 0.07 (Bruch and Engel 1994) derived from the 2175A absorption feature in the IUE LWP spectra. From the best-fit model solutions to the combined HST + FUSE spectral energy distribution, we find that the white dwarf is reaching a temperature Teff of 45-55,000K in quiescence, assuming Log(g)= 8.3 with a solar composition accreted atmosphere. The exact temperature of the WD depends on the reddening assumed and on the inclusion of a quiescent low mass accretion rate accretion disk. Accretion disk models alone fit badly in the FUSE range while, and if we take the distance to be a free parameter, the only accretion disk model which fits well is for a discordant distance of at least several hundred pc and an accretion rate (1.E-8 Msun/yr which is unacceptably high for a dwarf nova in quiescence. We discuss the implications of the white dwarf's temperature on the time-averaged accretion rate and long term compressional heating models.
description: ApJ, accepted
Un palazzo in divenire: vicende costruttive, storia cromatica e studio delle superfici delle ex Scuole Comunali di Locarno
Creators: name: Bordi, Agata
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2016

description: L’edificio del palazzo delle ex Scuole Comunali di Locarno viene costruito nel 1894 ai margini del centro storico di Locarno, sulla via tra l’antico Castello Visconteo e Piazza Grande, secondo il progetto del noto architetto Ferdinando Bernasconi con una pianta a U. Successivamente nel 1932 è soggetto ad un ampliamento, secondo il progetto degli architetti Silverio Rianda e Piero Respini, che allungano e chiudono lo sviluppo del fabbricato creando un edificio con corte centrale chiusa. Attualmente è il luogo per l’edificazione del Palacinema, per il Festival del Film di Locarno; il progetto, ora in corso di realizzazione, ha come obiettivo la totale ristrutturazione degli spazi interni e il mantenimento delle facciate esterne.
The Star Formation Rate Distribution Function of the Local Universe
Creators: name: Bothwell, M. S.
name: Kennicutt, R. C.
name: Johnson, B. D.
name: Wu, Y.
name: Lee, J. C.
name: Dale, D.
name: Engelbracht, C.
name: Calzetti, D.
name: Skillman, E.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present total infrared (IR) and ultraviolet (UV) luminosity functions derived from large representative samples of galaxies at z ~ 0, selected at IR and UV wavelengths from the IRAS IIFSCz catalogue, and the GALEX AIS respectively. We augment these with deep Spitzer and GALEX imaging of galaxies in the 11 Mpc Local Volume Legacy Survey (LVL), allowing us to extend these luminosity functions to lower luminosities (~10^6 L_sun), and providing good constraints on the slope of the luminosity function at the extreme faint end for the first time. Using conventional star formation prescriptions, we generate from our data the SFR distribution function for the local Universe. We find that it has a Schechter form, that the faint-end slope has a constant value (to the limits of our data) of α = -1.51 \pm 0.08, and the 'characteristic' SFR is 9.2 M_sun/yr. We also show the distribution function of the SFR volume density; we then use this to calculate a value for the total SFR volume density at z ~ 0 of 0.025 \pm 0.0016 M_sun/yr/Mpc^-3, of which ~ 20% is occurring in starbursts. Decomposing the total star formation by infrared luminosity, it can be seen that 9 \pm 1% is due to LIRGs, and 0.7 \pm 0.2% is occuring in ULIRGs. By comparing UV and IR emission for galaxies in our sample, we also calculate the fraction of star formation occurring in dust obscured environments, and examine the distribution of dusty star formation: we find a very shallow slope at the highly extincted end, which may be attributable to line of sight orientation effects as well as conventional internal extinction.
description: 14 pages, 10 figures; accepted for publication in MNRAS
title: Ð Ð°ÑÑÑÑ Ð»Ð¾Ð¿Ð°ÑÐºÐ¸ Ð¿Ð°ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ±Ð¸Ð½Ñ, ÑÐ¿ÑÐ¾ÑÐ½ÐµÐ½Ð½Ð¾Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð¿ÑÐµÐ´Ð²Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð¸Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
title: Analysis of the steam turbine blade, hardened by the prestress method
Creators: name: ÐÐ½ÑÐ¾Ð½Ð¾Ð², ÐÐ¸ÐºÐ¸ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019
Subjects: ÐÐ°ÑÐ¾Ð²ÑÐµ ÑÑÑÐ±Ð¸Ð½Ñ
Ð¿ÑÐµÐ´Ð²Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð¸Ðµ
Ð¿Ð¾Ð²ÐµÑÑ Ð½Ð¾ÑÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ¾ÑÐ½ÐµÐ½Ð¸Ðµ
ÑÑÑÐ°Ð»Ð¾ÑÑÐ½Ð°Ñ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑ
ÐºÐ¾ÑÑÐ¾Ð·Ð¸Ð¾Ð½Ð½Ð°Ñ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑ
Ð´Ð¸Ð°Ð³ÑÐ°Ð¼Ð¼Ð° Ð´ÐµÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
ÑÐ¿ÑÑÐ³Ð¾Ð¿Ð»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ
ÑÐ¶Ð¸Ð¼Ð°ÑÑÐ¸Ðµ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ¾ÑÐ½ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð¿ÑÐµÐ´Ð²Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð¸Ñ. Ð¢Ð°ÐºÐ¶Ðµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð´ÑÑÐ³Ð¸Ðµ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ ÑÐ¿ÑÐ¾ÑÐ½ÐµÐ½Ð¸Ñ Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ Ð²ÑÐ±Ð¾Ñ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¼ÐµÑÐ¾Ð´Ð°. ÐÐ»Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐµÐ³Ð¾ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¸ÑÑ ÑÐ¿ÑÑÐ³Ð¾Ð¿Ð»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¿ÑÐ¾ÑÑÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð², ÑÐ°ÐºÐ¸Ñ ÐºÐ°Ðº: ÐºÑÑÐ³Ð»ÑÐ¹ Ð¾Ð±ÑÐ°Ð·ÐµÑ, Ð±ÐµÑÐºÐ¾Ð½ÐµÑÐ½Ð¾-Ð´Ð»Ð¸Ð½Ð½Ð°Ñ ÑÑÑÐ±Ð° Ð¸ Ð¿Ð»Ð°ÑÑÐ¸Ð½Ð° Ñ Ð¾ÑÐ²ÐµÑÑÑÐ¸ÐµÐ¼, Ð¸ ÑÐ»Ð¾Ð¶Ð½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ - ÑÐ°Ð±Ð¾ÑÐ°Ñ Ð»Ð¾Ð¿Ð°ÑÐºÐ° Ð¿Ð°ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ±Ð¸Ð½Ñ Ð¿Ð¾ÑÐ»ÐµÐ´Ð½ÐµÐ¹ ÑÑÑÐ¿ÐµÐ½Ð¸ Ð¦ÐÐ, ÑÐµÐ³Ð¼ÐµÐ½Ñ ÑÐ¾ÑÐ¾ÑÐ°. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¿Ð¾ÐºÐ°Ð·Ð°Ð»Ð¸, Ð½Ð° ÐºÐ°ÐºÐ¸Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÑÑ Ð´ÐµÑÐ°Ð»ÐµÐ¹ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ ÑÐ½Ð¸Ð¶ÐµÐ½Ñ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¿ÑÑÐµÐ¼ Ð½Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ÑÑÐ°ÑÐ¾ÑÐ½ÑÑ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ð¹ ÑÐ¶Ð°ÑÐ¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ´Ð¸Ð»Ð¸ Ð´ÐµÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑ Ð¼ÐµÑÐ¾Ð´Ð° Ð¿ÑÐµÐ´Ð²Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð¸Ñ.
description: In this paper, surface hardening was investigated using the preloading method. Other methods of hardening were also considered . The most performed method of hardening was also chosen. Reasons of used hardening method were also justified. To determine its effectiveness, elastic-plastic calculations were performed for simple objects (dumbbell shaped sample, infinitely long pipe and plate with hole) and complex shaped objects (rotor blade of a steam turbine of the last stage of a low-pressure cylinder, a rotor segment). The results of the calculations showed on which surfaces of the details the stresses can be reduced by resulting residual compressive stresses. Based on the obtained results, effectiveness of preload method was proved.
Spiral structure in nearby galaxies I. Sample, data analysis, and overview of results
Creators: name: Kendall, S.
name: Kennicutt, R. C.
name: Clarke, C.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: This paper, the first of two, introduces an observational study of spiral structure in galaxies chosen from the SINGS survey. Near infrared (NIR) and optical data are used to produce mass surface density maps, and from these the morphology of the disc is examined. The aim of this work is to characterise the prevalence of spiral structure in this sample and, in the cases where a clear spiral pattern is found, include the findings in a comparative study (reported in paper II). A two-armed (`grand design') spiral pattern is found in approximately half the galaxies studied, including all those that are designated as grand design in the optical, but also including some, but not all, optically flocculent galaxies. It is found that the level of non-axisymmetric structure in the galaxies' mass distributions is only modestly higher in those galaxies that are classified as `grand design' compared with those that are not, implying that non-grand design galaxies possess significant power in higher order modes. There is no evidence that bars preferentially trigger the spirals, but they do appear to stir up non-axisymmetric structure in the disc. In contrast, there is evidence that strong/close tidal interactions with companion galaxies are associated with strong two-armed spiral structure in the infrared, though there are a number of galaxies with relatively weak infrared spiral structure that do not possess such companions.
description: 28 pages, 56 figures. Accepted for publication in MNRAS
Phillip Vallentine Tobias - Bibliography from PHILLIP VALLENTINE TOBIAS. 14 October 1925 – 7 June 2012
Creators: name: McKee, Jeffrey K.
Publisher: name: The Royal Society
Year: 2022
Subjects: subject: 40308 Palaeontology (incl. Palynology)
subject: FOS: Earth and related environmental sciences

description: Phillip Tobias was certainly best known as the doyen of African palaeoanthropology, but his interests and accomplishments ranged far beyond that. He was skilled in cytogenetics, human biology and, of course, human anatomy, as a long-time chair of anatomy at his academic home, the University of the Witwatersrand, Johannesburg. The passion of Tobias also made him a leading figure as a warrior for academic freedom and human dignity in the fight against South African apartheid. His oratorical skills gave him power in the classroom and in public, although he was well-known for often going on too long. Fondly known as ‘PVT’, Tobias was a gracious yet demanding scholar, with a work ethic few could attempt to mimic.
From enclosure to exposure to enactment : a phenomenological study on the experiences of 20 Division 1 Black student-athletes abroad
Creators: name: Walker, Devin Leslie
name: 0000-0002-6365-4728
Publisher: name: The University of Texas at Austin
Year: 2018
Subjects: Black student athlete
Student athlete development
International education
Study abroad
CRT

description: This phenomenological study explores the experiences of 20 Division I Black student-athletes who took part in international educational experiences as part of their collegiate careers, as well as the subsequent influence of these experiences on their identities and future orientation. This study utilizes the theoretical framework of Critical Race Theory (CRT) as well as the concept of figured worlds as described by Holland, Lachicotte, Skinner and Cain (1998). Many Black student-athletes suffer from identity foreclosure as they fail to develop salient aspects of their identity outside of the athlete role. International education proffers the opportunity to take advantage of a holistic collegiate experience, which can impede the detrimental effects of the athletic identity foreclosure process that disproportionately affects Black student-athletes. Education abroad can influence student-athletes’ personal, academic, and professional development while stimulating their critical consciousness of the world beyond the gym and campus. The number of college students in international education is increasing. However, most student-athletes are not given access to these opportunities. The 2016 NCAA Goals report highlighted student-athletes desire to have access to international education opportunities. The value of these student-athletes is critical the financial well-being of these institutions, yet they are often denied the invaluable opportunity to experience education abroad. This dissertation examines the process of identity negotiation and development that Black student-athletes experience as they partake in three types of international education: 1) Study Abroad, 2) Competition Abroad, and 3) Service-learning Abroad. This study is solution-oriented. The findings reveal that international education serves as an extracurricular learning experience that enhances the process of identity development and negotiation for Black student-athletes, diminishing the detrimental impact of identity foreclosure. There international learning experiences shaped their future orientation and positively influenced their ability to navigate their lives and careers after their playing days ended.
Additional file 1 of Technology-based health solutions for cancer caregivers to better shoulder the impact of COVID-19: a systematic review protocol
Creators: name: Su, Zhaohui
name: McDonnell, Dean
name: Liang, Bin
name: Kue, Jennifer
name: Li, Xiaoshan
name: Šegalo, Sabina
name: Advani, Shailesh
name: Flores, Bertha E.
name: Wang, Jing
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Additional file 1:. PRISMA-P checklist
Logic-Based Decision Support for Strategic Environmental Assessment
Creators: name: Gavanelli, Marco
name: Riguzzi, Fabrizio
name: Milano, Michela
name: Cagnoli, Paolo
Publisher: name: arXiv
Year: 2010
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences
subject: J.2; I.2.1; I.2.4; I.2.5

description: Strategic Environmental Assessment is a procedure aimed at introducing systematic assessment of the environmental effects of plans and programs. This procedure is based on the so-called coaxial matrices that define dependencies between plan activities (infrastructures, plants, resource extractions, buildings, etc.) and positive and negative environmental impacts, and dependencies between these impacts and environmental receptors. Up to now, this procedure is manually implemented by environmental experts for checking the environmental effects of a given plan or program, but it is never applied during the plan/program construction. A decision support system, based on a clear logic semantics, would be an invaluable tool not only in assessing a single, already defined plan, but also during the planning process in order to produce an optimized, environmentally assessed plan and to study possible alternative scenarios. We propose two logic-based approaches to the problem, one based on Constraint Logic Programming and one on Probabilistic Logic Programming that could be, in the future, conveniently merged to exploit the advantages of both. We test the proposed approaches on a real energy plan and we discuss their limitations and advantages.
description: 17 pages, 1 figure, 26th Int'l. Conference on Logic Programming (ICLP'10)
title: ÐÑÑÐ¾ÑÐ½Ð¸Ðº Ð¾Ð¿Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð½ÐµÐ¹ÑÐ¾ÑÑÐ¸Ð¼ÑÐ»ÑÑÐ¸Ð¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
title: Reference voltage source for the neurostimulation system
Creators: name: ÐÑÐ´Ð¸Ð½, ÐÐ°Ð²ÐµÐ»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2023
Subjects: Ð½ÐµÐ¹ÑÐ¾ÑÑÐ¸Ð¼ÑÐ»ÑÑÐ¾Ñ
Ð¾Ð¿Ð¾ÑÐ½Ð¾Ðµ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ðµ
ÐÐÐÐ
Ð¸ÑÑÐ¾ÑÐ½Ð¸Ðº Ð¾Ð¿Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ
ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½ÑÐ¹ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½Ñ
neurostimulator
reference voltage
CMOS
reference voltage source
temperature coefficient

description: Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð½ÐµÐ¹ÑÐ¾ÑÑÐ¸Ð¼ÑÐ»ÑÑÐ¾ÑÐ¾Ð² Ð¸ ÑÑÐµÐ¼ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¾Ð¿Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð¾Ð¸ÑÐºÐ° Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ, Ð±ÑÐ»Ð¸ ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð»Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð½ÐµÐ¹ÑÐ¾ÑÑÐ¸Ð¼ÑÐ»ÑÑÐ¾ÑÐ° Ð¸ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ° Ð¾Ð¿Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð±Ð»Ð¾ÐºÐ¾Ð², ÑÐ¾ÑÐ¼Ð¸ÑÑÑÑÐ¸Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸Ðº Ð¾Ð¿Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ: Ð¸ÑÑÐ¾ÑÐ½Ð¸Ðº Ð¾Ð¿Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÐºÐ°, ÑÑÐµÐ¼Ñ ÑÐ¼ÐµÑÐµÐ½Ð¸Ñ Ð¸ Ð°ÐºÑÐ¸Ð²Ð½Ð°Ñ Ð½Ð°Ð³ÑÑÐ·ÐºÐ°. ÐÑÐ»Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½ÑÐ¹ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½Ñ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ Ð²ÑÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¾Ñ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ.Â  ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ ÐµÐ³Ð¾ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð²ÑÐ¿Ð¾Ð»Ð½ÑÐ»Ð¸ÑÑ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÑÐµÐ´ÑÑÐ² ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ¸ÑÑÐ¾Ð²ÑÑ Ð¸ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÑ ÑÑÐµÐ¼ Micro-Cap.
description: As a result of the study, a review of currently existing architectures of neurostimulators and schemes of reference voltage sources. As a result, the requirements for the construction of a neurostimulator and a reference voltage source were formulated. The calculation and modeling of the blocks forming the reference voltage source: the reference current source, the bias circuits and the active load are carried out. The temperature coefficient of the device and the dependence of the output voltage on the change in the supply voltage were obtained. Simulations of the device and its characteristics were performed using Micro-Cap digital and analog circuit development tools.
Energetic axion-like particle production in galaxies
Creators: name: Manousos, Athanasios
name: Liolios, Anastasios
name: Eleftheriadis, Christos
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Relativistic axion-like particles (ALPs) originating from the stellar interiors, along with the ones coming from photon-ALP mixing in the galactic magnetic fields, contribute together to make an energetic component of the ALP content of the universe. Considering an isotropic distribution of cosmic gamma rays, it is examined if these high energy axion-like particles could constitute a measurable isotropic "background" for helioscope-type and existing large general-purpose particle experiments, taking into account their sensitivity.
description: To be published in PoS for IDM2010 (Identification of Dark Matter 2010)
How often is a random quantum state k-entangled?
Creators: name: Szarek, Stanislaw J.
name: Werner, Elisabeth
name: Zyczkowski, Karol
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The set of trace preserving, positive maps acting on density matrices of size d forms a convex body. We investigate its nested subsets consisting of k-positive maps, where k=2,...,d. Working with the measure induced by the Hilbert-Schmidt distance we derive asymptotically tight bounds for the volumes of these sets. Our results strongly suggest that the inner set of (k+1)-positive maps forms a small fraction of the outer set of k-positive maps. These results are related to analogous bounds for the relative volume of the sets of k-entangled states describing a bipartite d X d system.
description: 19 pages in latex, 1 figure included
Un método para conocer el estado del arte sobre la aplicación de la innovación educativa. La metáfora del camino
Creators: name: Fidalgo-Blanco, Ángel
Publisher: name: Zenodo
Year: 2019
Subjects: Innovación educativa, profesorado, buena práctica,

description: CAMINANTE Y CAMINO.

1. El caminante. El profesorado que innova.

2. El camino: terreno, etapas y alcance.

3. La meta. Llegar de una pieza.
Additional file 8 of EPHA7 mutation as a predictive biomarker for immune checkpoint inhibitors in multiple cancers
Creators: name: Zhang, Zhen
name: Wu, Hao-Xiang
name: Lin, Wu-Hao
name: Wang, Zi-Xian
name: Yang, Lu-Ping
name: Zeng, Zhao-Lei
name: Luo, Hui-Yan
Publisher: name: figshare
Year: 2021
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 8: Figure S4. Survival analysis of EPHA3 in both discovery and validation cohort.
Relationship between Structure, Entropy and Diffusivity in Water and Water-like Liquids
Creators: name: Agarwal, Manish
name: Singh, Murari
name: Sharma, Ruchi
name: Alam, Mohammad Parvez
name: Chakravarty, Charusita
Publisher: name: arXiv
Year: 2010
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Anomalous behaviour of the excess entropy ($S_e$) and the associated scaling relationship with diffusivity are compared in liquids with very different underlying interactions but similar water-like anomalies: water (SPC/E and TIP3P models), tetrahedral ionic melts (SiO$_2$ and BeF$_2$) and a fluid with core-softened, two-scale ramp (2SRP) interactions. We demonstrate the presence of an excess entropy anomaly in the two water models. Using length and energy scales appropriate for onset of anomalous behaviour, the density range of the excess entropy anomaly is shown to be much narrower in water than in ionic melts or the 2SRP fluid. While the reduced diffusivities ($D^*$) conform to the excess entropy scaling relation, $D^* =A\exp (αS_e)$ for all the systems (Y. Rosenfeld, Phys. Rev. A {\bf 1977}, {\it 15}, 2545), the exponential scaling parameter, $α$, shows a small isochore-dependence in the case of water. Replacing $S_e$ by pair correlation-based approximants accentuates the isochore-dependence of the diffusivity scaling. Isochores with similar diffusivity scaling parameters are shown to have the temperature dependence of the corresponding entropic contribution. The relationship between diffusivity, excess entropy and pair correlation approximants to the excess entropy are very similar in all the tetrahedral liquids.
description: 24 pages, 4 figures, to be published in Journal of Physical Chemistry B
Il Blu Egizio nella Pittura Murale Altomedievale
Creators: name: Alessi, Ilaria
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2019

description: Il presente lavoro di tesi ha come oggetto lo studio del pigmento blu egizio nella pittura murale di età altomedievale, attraverso l’analisi di sei casi studio selezionati e approfonditi in modo differente, riferibili al contesto italo-elvetico. In particolare gli obiettivi preposti includono la caratterizzazione delle superfici dipinte e delle tecniche esecutive (leganti e miscele di pigmenti) e la determinazione delle fonti di approvvigionamento delle materie prime (rame e fondente) impiegate nel processo di produzione del blu egizio. Questi temi sono stati esaminati attraverso confronti tipologici, al fine di evidenziare eventuali corrispondenze o tratti distintivi nei diversi casi studio.
Therapeutic enactment : a case study of the experience of a Canadian military veteran
Creators: name: Kerr, Mark Stuart
Publisher: name: University of British Columbia
Year: 2021

description: Much of the literature on therapeutic treatments for military personnel who have suffered an operational stress injury or PTSD from active duty focuses on individual therapy models. While models of group therapy for military veterans do exist, limited understanding of the impact of their process is known, particularly with Canadian military veterans. This study attempts to understand the experience of one particular type of group therapy called Therapeutic Enactment (TE) through the lens of a Canadian Armed Forces veteran. A case study research design was employed for this study. The participant of this study was a male, Canadian military veteran who had suffered an operational stress injury related to his role in the military and had completed at least one prior Therapeutic Enactment in relation to this difficulty. Data was collected through a 1-hour semi-structured, open-ended interview with a participant via a virtual recorded interview over Zoom. The results of the study were analyzed using the six-phase process of thematic analysis from Braun and Clarke (2006). Four main themes, each with two or three subthemes emerged from this data analysis. The four major themes were: 1) Trust, 2) Beneficial aspects of Therapeutic Enactment, 3) Challenges in Therapeutic Enactment, and 4) Recommendations for future Therapeutic Enactments. This study contributes to our overall understanding of how Therapeutic Enactment is experienced and gives guidance for practical application for clinicians. Implications for future research are also discussed.
СТРУКТУРНО-СЕМАНТИЧЕСКИЕ ОСОБЕННОСТИ ПРИСТАВОЧНЫХ ГЛАГОЛОВ ДВИЖЕНИЯ В РУССКОМ И УЗБЕКСКОМ ЯЗЫКАХ
Creators: name: С.А.Хайруллаева магистрант УзГУМЯ Ташкент, Узбекистан
Publisher: name: Zenodo
Year: 2025

description: В данной статье рассматриваются структурно-семантические особенности приставочных глаголов движения в русском и узбекском языках. А также  глаголы движения в русском языке и их особенности, значение приставок, способы выражения движения в узбекском языке и временные и аспектуальные значения. Настоящая статья посвящена сравнительному анализу структурно-семантических особенностей приставочных глаголов движения в русском и узбекском языках, выявлению их сходств и различий, а также способам передачи значений движения в узбекском языке.

Ключевые слова: Глаголы движения, детерминировать, недетерминировать, приставочные формы, модальные и оценочные, сложные глагольные конструкции
Additional file 3 of EPHA7 mutation as a predictive biomarker for immune checkpoint inhibitors in multiple cancers
Creators: name: Zhang, Zhen
name: Wu, Hao-Xiang
name: Lin, Wu-Hao
name: Wang, Zi-Xian
name: Yang, Lu-Ping
name: Zeng, Zhao-Lei
name: Luo, Hui-Yan
Publisher: name: figshare
Year: 2021
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 3: Figure S1. Violin plot depicting the distribution of TMB and CNA in EPHA7-MUT and EPHA7-WT tumors.
Forcing Adsorption of a Tethered Polymer by Pulling
Creators: name: Osborn, Judy-anne
name: Prellberg, Thomas
Publisher: name: arXiv
Year: 2010
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We present an analysis of a partially directed walk model of a polymer which at one end is tethered to a sticky surface and at the other end is subjected to a pulling force at fixed angle away from the point of tethering. Using the kernel method, we derive the full generating function for this model in two and three dimensions and obtain the respective phase diagrams. We observe adsorbed and desorbed phases with a thermodynamic phase transition in between. In the absence of a pulling force this model has a second-order thermal desorption transition which merely gets shifted by the presence of a lateral pulling force. On the other hand, if the pulling force contains a non-zero vertical component this transition becomes first-order. Strikingly, we find that if the angle between the pulling force and the surface is beneath a critical value, a sufficiently strong force will induce polymer adsorption, no matter how large the temperature of the system. Our findings are similar in two and three dimensions, an additional feature in three dimensions being the occurrence of a reentrance transition at constant pulling force for small temperature, which has been observed previously for this model in the presence of pure vertical pulling. Interestingly, the reentrance phenomenon vanishes under certain pulling angles, with details depending on how the three-dimensional polymer is modeled.
Galaxy Outflows in the Circumgalactic Medium at Cosmic Noon
Creators: name: Nielsen, Nikki
name: None
Publisher: name: Zenodo
Year: 2019

description: The star formation history of the universe reveals that galaxies most actively build their stellar mass at cosmic noon, roughly 10 billion years ago, with a decrease toward present-day. The resulting metal-enriched material ejected from these galaxies due to supernovae and stellar feedback is deposited into the circumgalactic medium (CGM), which is a massive reservoir of diffuse, multiphase gas out to radii of $\sim200$ kpc. The CGM is the interface between the intergalactic medium and the galaxy, through which accreting filaments of near-pristine gas must pass to contribute new star formation material to the galaxy, and outflowing gas is later recycled. Simulating these baryon cycle flows is crucial for accurately modelling galaxy evolution. We examine these multiphase CGM gas flows with the quasar absorption line technique, primarily focusing on the low-ionization MgII absorption doublet (T$\sim10^{4}$ K), with additional multiphase ions such as Lyman alpha, FeII, and CIV. With the combination of HST images, high-resolution UVES/VLT quasar spectra, and cutting-edge IFU data from the Keck Cosmic Web Imager, we quantify the gas kinematics and metallicities of outflowing gas at 69 kpc along the minor axis of an edge-on ($i=85^{\circ}$) galaxy at cosmic noon ($z_{\rm gal}=2.070$). Connecting these results to our Multiphase Galaxy Halos Survey at $z\sim0.3$, we study the evolution of CGM kinematics and metallicities over nearly 10 billion years.
Additional file 9 of EPHA7 mutation as a predictive biomarker for immune checkpoint inhibitors in multiple cancers
Creators: name: Zhang, Zhen
name: Wu, Hao-Xiang
name: Lin, Wu-Hao
name: Wang, Zi-Xian
name: Yang, Lu-Ping
name: Zeng, Zhao-Lei
name: Luo, Hui-Yan
Publisher: name: figshare
Year: 2021
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 9: Figure S5. Association between clinical outcomes and the combination of all 14 EPH genes in the discovery cohort.
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð²Ð¸Ð´ÐµÐ¾Ð¿Ð¾ÑÐ¾ÐºÐ° Ñ Ð¼Ð¸Ð½Ð¸Ð¼Ð°Ð»ÑÐ½ÑÐ¼Ð¸ Ð·Ð°Ð´ÐµÑÐ¶ÐºÐ°Ð¼Ð¸ Ð² ÑÑÐ°Ð½Ð´Ð°ÑÑÐ°Ñ Wi-Fi
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
title: Analysis of video streaming with minimal delays in Wi-Fi standards
Creators: name: Ð¢Ð°ÑÐ»ÑÐºÐ¾Ð²Ð°, ÐÐ»Ð¸Ð·Ð°Ð²ÐµÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019
Subjects: Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½ÑÐµ ÑÐµÑÐ¸
Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð²Ð°Ñ Ð¿ÐµÑÐµÐ´Ð°ÑÐ°
Ð·Ð°Ð´ÐµÑÐ¶ÐºÐ°
Ð²Ð¸Ð´ÐµÐ¾Ð´Ð°Ð½Ð½ÑÐµ
ieee 802.11
Wi-Fi
wireless network
current transfer
delay
udp
tcp
mpeg
qos
video data
802.11n

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð²Ð¸Ð´ÐµÐ¾ÑÐ¸Ð³Ð½Ð°Ð»Ð° Ð² Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½ÑÑ Ð»Ð¾ÐºÐ°Ð»ÑÐ½ÑÑ ÑÐµÑÑÑ, ÑÑÐ°Ð²Ð½Ð¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Wi-Fi. ÐÑÑÐ²Ð»ÑÑÑÑÑ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ Ð·Ð°Ð´ÐµÑÐ¶ÐºÐ¸ Ð² Ð²Ð¸Ð´ÐµÐ¾ÑÑÐ°Ð½ÑÐ»ÑÑÐ¸Ð¸, ÐÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð°Ð´ÐµÑÐ¶ÐµÐº Ð¿ÑÐ¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐµ Ð²Ð¸Ð´ÐµÐ¾ÑÐ¸Ð³Ð½Ð°Ð»Ð° Ð² Ð±ÐµÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¾Ð¹ Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÐµÑÐ¸ Ð½Ð° Ð±Ð°Ð·Ðµ Ð½Ð°Ð¸Ð»ÑÑÑÐµÐ³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð»Ð¾Ð². ÐÑÐ¾Ð¸ÑÑÐ¾Ð´Ð¸Ñ Ð¾ÑÐµÐ½ÐºÐ° Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ Ð·Ð°Ð´ÐµÑÐ¶ÐµÐº Ð¸ Ð´Ð»Ñ Ð¸Ñ Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð²Ð¸Ð´ÐµÐ¾ÑÐ¸Ð³Ð½Ð°Ð»Ð°.
description: In this final work, the peculiarities of video signal transmission in wireless local area networks are considered, the main Wi-Fi standards are compared. The reasons for the delay in video broadcasting are identified, and an analysis of delays in the transmission of video signals in a wireless local area network based on the best standard using various protocols is carried out. There is an estimate of the magnitude of the delays and to minimize them, optimal conditions for the transmission of the video signal are determined.
Exploring the origins of a new, apparently metal-free gas cloud at z = 4.4
Creators: name: Robert, Paul-Frédéric
name: None
Publisher: name: Zenodo
Year: 2019

description: Lyman limit systems (LLSs) are promising probes of pristine or near-pristine environments, being possibly metal-free, or polluted only by the ejecta from PopIII stars. As such, they may prove an important probe of the PopIII star population at redshifts ≥ 15. Such LLSs will have a very-low metallicity, ≤ 1/1000th of the solar value at least, and show weak metal absorption lines against a background quasar's continuum in the near-pristine case. In P. Frédéric Robert et al. 2018 (MNRAS, submitted), I report the discovery and analysis of only the third LLS, LLS1723, in which a high-quality, echelle-resolution spectrum reveals no metal absorption lines, implying a metallicity ≤ 1/10000 solar. Such a low metallicity raises the question of LLS1723's origin and enrichment history. Previous simulations of the circumgalactic medium imply that LLS1723 is a natural candidate for a cold gas stream accreting towards a galaxy. Alternatively, LLS1723 may represent a high-density portion of the intergalactic medium containing either pristine gas – unpolluted by stellar debris for 1.4 Gyr after the Big Bang – or the remnants of low-energy supernovae from (likely low-mass) Population III stars. These possibilities highlight the need for – and opportunity to test – simulations of the frequency with which such high-density, very low-metallicity systems arise in the intergalactic medium. Observationally, mapping the galaxy distribution around such systems may assist in better understanding their origin. New optical integral field spectrographs, such as KCWI, and MUSE are already demonstrating this to be a promising approach (e.g. Fumagalli et al. 2016).
Lifestyle management in polycystic ovary syndrome – beyond diet and physical activity
Creators: name: Cowan, S
name: Lim, S
name: Alycia, C
name: Pirotta, S
name: Thomson, R
name: Gibson-Helm, Melanie
name: Blackmore, R
name: Naderpoor, N
name: Bennett, C
name: Ee, C
name: Rao, V
name: Mousa, A
name: Alesi, S
name: Moran, L
Publisher: name: Open Access Te Herenga Waka-Victoria University of Wellington
Year: 2023
Subjects: subject: 110399 Clinical Sciences not elsewhere classified
subject: FOS: Clinical medicine

description: Polycystic ovary syndrome (PCOS) is a common condition affecting reproductive-aged women with reproductive, metabolic and psychological consequences. Weight and lifestyle (diet, physical activity and behavioural) management are first-line therapy in international evidence-based guidelines for PCOS. While these recommend following population-level diet and physical activity guidelines, there is ongoing interest and research in the potential benefit of including psychological and sleep interventions, as well as a range of traditional, complimentary and integrative medicine (TCIM) approaches, for optimal management of PCOS. There is limited evidence to recommend a specific diet composition for PCOS with approaches including modifying protein, carbohydrate or fat quality or quantity generally having similar effects on the presentations of PCOS. With regards to physical activity, promising evidence supports the provision of vigorous aerobic exercise, which has been shown to improve body composition, cardiorespiratory fitness and insulin resistance. Psychological and sleep interventions are also important considerations, with women displaying poor emotional wellbeing and higher rates of clinical and subclinical sleep disturbance, potentially limiting their ability to make positive lifestyle change. While optimising sleep and emotional wellbeing may aid symptom management in PCOS, research exploring the efficacy of clinical interventions is lacking. Uptake of TCIM approaches, in particular supplement and herbal medicine use, by women with PCOS is growing. However, there is currently insufficient evidence to support integration into routine clinical practice. Research investigating inositol supplementation have produced the most promising findings, showing improved metabolic profiles and reduced hyperandrogenism. Findings for other supplements, herbal medicines, acupuncture and yoga is so far inconsistent, and to reduce heterogeneity more research in specific PCOS populations, (e.g. defined age and BMI ranges) and consistent approaches to intervention delivery, duration and comparators are needed. While there are a range of lifestyle components in addition to population-recommendations for diet and physical activity of potential benefit in PCOS, robust clinical trials are warranted to expand the relatively limited evidence-base regarding holistic lifestyle management. With consumer interest in holistic healthcare rising, healthcare providers will be required to broaden their knowledge pertaining to how these therapies can be safely and appropriately utilised as adjuncts to conventional medical management.
The baryon cycle in the Eagle simulations
Creators: name: Mitchell, Peter
name: None
Publisher: name: Zenodo
Year: 2019

description: Galaxy evolution is to leading order set by the rates of gas inflow and outflow at the boundary of galaxies. I will present a full analysis of gas flows in the Eagle simulation suite, quantifying outflow rates, the rates of inflow split between pristine and recycled accretion, and the important role of feedback in reducing the rate of cosmological gas infall onto dark matter halos. I will explain how these gas flux measurements fit into the larger context of galaxy evolution, for example by setting galaxy star formation rates and metallicities. I will finish by discussing the ongoing task of identifying indirect observable tracers of this baryon cycle to test simulation predictions, emphasising the role that ongoing IFU observations can play.
A Study of Chinese College Students' Plans to Use Blended Learning: a Dual Moderation Model of Student Satisfaction and Social Pressure
Creators: name: Xinyue Li
Publisher: name: DR.KEN Institute of Academic Development and Promotion
Year: 2023
Subjects: Blended Learning
Motivation
Satisfaction
Social influence

description: International Journal of Sociologies and Anthropologies Science Reviews, 3, 3, 1-16
Molecular double core-hole electron spectroscopy for chemical analysis
Creators: name: Tashiro, Motomichi
name: Ehara, Masahiro
name: Fukuzawa, Hironobu
name: Ueda, Kiyoshi
name: Buth, Christian
name: Kryzhevoi, Nikolai V.
name: Cederbaum, Lorenz S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We explore the potential of double core hole electron spectroscopy for chemical analysis in terms of x-ray two-photon photoelectron spectroscopy (XTPPS). The creation of deep single and double core vacancies induces significant reorganization of valence electrons. The corresponding relaxation energies and the interatomic relaxation energies are evaluated by CASSCF calculations. We propose a method how to experimentally extract these quantities by the measurement of single and double core-hole ionization potentials (IPs and DIPs). The influence of the chemical environment on these DIPs is also discussed for states with two holes at the same atomic site and states with two holes at two different atomic sites. Electron density difference between the ground and double core-hole states clearly shows the relaxations accompanying the double core-hole ionization. The effect is also compared with the sensitivity of single core hole ionization potentials (IPs) arising in single core hole electron spectroscopy. We have demonstrated the method for a representative set of small molecules LiF, BeO, BF, CO, N2, C2H2, C2H4, C2H6, CO2 and N2O. The scalar relativistic effect on IPs and on DIPs are briefly addressed.
description: 35 pages, 6 figures. To appear in J. Chem. Phys.
Lattice SU(2) on GPU's
Creators: name: Cardoso, Nuno
name: Bicudo, Pedro
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: We discuss the CUDA approach to the simulation of pure gauge Lattice SU(2). CUDA is a hardware and software architecture developed by NVIDIA for computing on the GPU. We present an analysis and performance comparison between the GPU and CPU with single precision. Analysis with single and multiple GPU's, using CUDA and OPENMP, are also presented. In order to obtain a high performance, the code must be optimized for the GPU architecture, i.e., an implementation that exploits the memory hierarchy of the CUDA programming model. Using GPU texture memory and minimizing the data transfers between CPU and GPU, we achieve a speedup of $200\times$ using 2 NVIDIA 295 GTX cards relative to a serial CPU, which demonstrates that GPU's can serve as an efficient platform for scientific computing. With multi-GPU's we are able, in one day computation, to generate 1 000 000 gauge configurations in a $48^4$ lattice with $β=6.0$ and calculate the mean average plaquette. We present results for the mean average plaquette in several lattice sizes for different $β$. Finally we present results for the mean average Polyakov loop at finite temperature.
description: 7 pages, 6 figures, contribution to the proceedings of the XXVIII International Symposium on Lattice Field Theory - LAT2010, July 14-19 2010, Villasimius, Sadinia, Italy
Green functions of the spectral ball and symmetrized polydisk
Creators: name: Thomas, Pascal J.
name: Van Trao, Nguyen
name: Zwonek, Wlodzimierz
Publisher: name: arXiv
Year: 2010
Subjects: subject: Complex Variables (math.CV)
subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 32U35, 32F45

description: The Green function of the spectral ball is constant over the isospectral varieties, is never less than the pullback of its counterpart on the symmetrized polydisk, and is equal to it in the generic case where the pole is a cyclic (non-derogatory) matrix. When the pole is derogatory, the inequality is always strict, and the difference between the two functions depends on the order of nilpotence of the strictly upper triangular blocks that appear in the Jordan decomposition of the pole. In particular, the Green function of the spectral ball is not symmetric in its arguments. Additionally, some estimates are given for invariant functions in the symmetrized polydisc, e.g. (infinitesimal versions of) the Carathéodory distance and the Green function, that show that they are distinct in dimension greater or equal to $3$.
description: 12 pages
The Neutral Hydrogen Properties of Galaxies in Gas-rich Groups
Creators: name: Dzudzar, Robert
name: None
Publisher: name: Zenodo
Year: 2019

description: The majority of galaxies in the local Universe lie within a group environment - thus it is important to understand the group environmental impact on galaxy evolution. Our multi-wavelength survey of Choir groups probes low mass, gas-rich, late-type dominated groups with one or two giant spirals and a number of dwarf galaxies. These groups are reminiscent of (though more gas-rich) our local group. In this talk I will reveal the neutral hydrgogen (HI) content in the Choir groups. I will show that the majority of galaxies in these groups are gas-rich and that those in non-interacting groups are dominated by their internal galaxy properties rather than the group environment. Only a couple of galaxies are gas-poor which is most likely due to tidal interactions. To place Choir groups in the larger scale context, I will present detailed analysis of two extreme groups: an isolated Choir group, and a cluster infalling Choir group.
I Diritti dei Bambini e delle Bambine
Creators: name: Romanski, Soraya
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2018

description: Questo lavoro vuole dare un contributo alla scarsa presenza di fonti inerenti l’argomento dei diritti affrontato alla scuola dell’infanzia. Partendo dall’ipotesi che sia possibile affrontare la tematica dei diritti a partire da questa fase evolutiva è stato proposto un percorso che ha accompagnato i bambini attraverso l’evoluzione della loro concezione di bisogno per arrivare a costruire quella di diritto. Per rilevare l’evoluzione delle concezioni è stato creato insieme ai bambini un gioco da tavola sul tema dei bisogni e sono state monitorate attraverso una tabella osservativa tutte le scelte effettuate durante le partite. Sono state inoltre effettuate diverse attività incentrate sulla lettura di albi illustrati utilizzati come spunti di discussione ricevuti attraverso la corrispondenza con un giornalista. Sulla base dei dati raccolti attraverso il gioco e all’analisi dei protocolli delle discussioni è stato possibile rilevare la maturazione di specifiche competenze da parte del gruppo che permettono di confermare l’ipotesi iniziale. Relatore: Urs Kocher