cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
THE URGENCY OF ENSURING INFORMATION SECURITY
Creators: name: Saidova Nigina Sirojiddin qizi sdvangn21@gmail.com Master, Faculty of International Law University of World Economy and Diplomacy/Tashkent/ Uzbekistan
Publisher: name: Zenodo
Year: 2023

description: this scientific article is based on the theoretical data analysis of the information security system, and highlights the relevance of information security issues in the current era.  The main principles of the information security system and the legal measures available in the country are discussed.

Key words: information, information security, public information, confidential information, documented information, confidential information.
objective
Creators: name: Da Costa Neto, Raimundo Euzebio
Publisher: name: Open Science Framework
Year: 2023

description: The objective of this systematic review is to examine the epidemiological aspects of Cryptococcus-related meningitis in the Northeast region of Brazil. The aim is to identify the risk factors, modes of transmission, and clinical and epidemiological characteristics of the disease in this geographic area. The review will involve a comprehensive synthesis of existing literature, including studies, reports, and relevant data sources, to provide a comprehensive understanding of the epidemiology of Cryptococcus-related meningitis in the Northeast of Brazil. The findings of this review will contribute to the knowledge base on Cryptococcus-related meningitis in this specific region, guiding future research, prevention strategies, and healthcare interventions.
Photosynthesis, photorespiration and related aspects of CO2 exchange by wheat, corn and Amaranthus edulis
Creators: name: Jolliffe, Peter Alfred
Publisher: name: University of British Columbia
Year: 2011

description: Certain aspects of CO₂ exchange by wheat (Triticum aestivum L.), corn (Zea mays L.) and the grain Amaranth (Amaranthus edulis Speg.) were investigated. The effects of O₂ concentration on apparent photosynthesis of juvenile wheat and corn shoots were measured at different temperatures, CO₂ concentrations and light intensities using infra-red CO₂ analysis and both open and closed gas-flow systems. The only condition in which apparent photosynthesis of wheat was not inhibited by O₂ was in 20.8% O₂ when the CO₂ concentration was saturating and the temperature was 30° C or less. The degree of inhibition increased with increasing O₂ concentration, increasing temperature, and decreasing CO₂ concentration and was independent of the light intensity. During some of the growing season in temperate regions, the effect of atmospheric O₂ on the photosynthetic productivity of wheat may be negligible. The effect of O₂ on wheat was ascribed to both a stimulation of photorespiration and an inhibition of photosynthesis by O₂. In corn, which apparently lacks photorespiration, photosynthesis was also inhibited by 99% O₂- No inhibition occurred at 20.8% O₂, however, and the stability and reversibility of the inhibition observed at 99% O₂ differed from that found with wheat. These differences between wheat and corn are correlated with differences in leaf anatomy and photosynthetic carbon metabolism and with differences in the response of apparent photosynthesis and the CO₂ compensation point to environmental conditions. Many of the gas exchange characteristics of corn and similar plants seem to be advantageous for the warm dry areas they often inhabit. Initially high rates of CO₂ production are exhibited by wheat immediately following illumination, and it has been suggested that this post-illumination CO₂ burst is an extension of photorespiration into the dark period. In accord with this, CO₂ concentration was found to influence both the post-illumination CO₂ burst and the inhibition of apparent photosynthesis by O₂ in a similar way. Except for Amaranthus edulis, plants which lack photorespiration also lack significant post-illumination CO₂ bursts. On the basis of its response to O₂ concentration, however, the burst of Amaranthus edulis is concluded to be unrelated to photorespiration. Measurements of ¹²CO₂ and ¹⁴CO₂ exchange were used to estimate the quantity of carbon in wheat and corn shoots which was in free exchange with atmospheric CO₂. The free exchange pool size was found to be very small and it cannot be an important factor in the CO₂ concentration response of photosynthesis or in the post-illumination CO₂ burst.
Bringing new works to life : collaboration and interpretation in the performance, recording and editing of new works for guitar
Creators: name: Malone, DF
Publisher: name: University Of Tasmania
Year: 2023

description: This project aims to make clear the nature of collaboration between performer and composer. Whereas the roles of composer and interpreter are essentially sequential, the roles of collaborators are, by definition, interactive. While an interpreter comes to a score as a finished piece of work, a collaborative performer is involved with the composer's creative process before the musical score obtains its final form. As an intermediary between the composer and the audience, the interpreter must balance the literal requirements of the printed score with his or her own understanding of the composer's intentions and the needs of the performance. The printed score is a necessarily limited medium and interpreters define the extent of their own creative freedom in relation to its constraints and their understanding of its meaning. The purpose of this Master of Music project is to demonstrate my creative contribution, as both interpreter and collaborative performer, to the realisation of new musical works for guitar that were written between 1995 and 2002 by composers resident in Tasmania. The project consists of a recital of works by Graham Southwell Brown, Russell Gilmour, Maria Grenfell, Don Kay, John Lockwood and Raffaele Marcellino with a master recording of performances of these works for later release on CD or for broadcast. These are accompanied by a performance edition of the works by Brown, Gilmour, Grenfell and Kay that includes my fingerings, editorial marks and the revisions that have arisen from the process of collaborating with these composers. The exegesis outlines my collaboration with the composers of the works, and places the project in the context of writings by performers, composers, and musicologists on the interpretive role of the performer and the nature of collaboration between performer and composer.
Additional file 1 of Inhibition of LRRK2 kinase activity promotes anterograde axonal transport and presynaptic targeting of α-synuclein
Creators: name: Brzozowski, Charlotte F.
name: Hijaz, Baraa A.
name: Singh, Vijay
name: Gcwensa, Nolwazi Z.
name: Kelly, Kaela
name: Boyden, Edward S.
name: West, Andrew B.
name: Sarkar, Deblina
name: Volpicelli-Daley, Laura A.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 1: Fig. S1. No change in glutamatergic terminal density upon LRRK2 kinase inhibitor treatment. A) Shown are confocal images of primary hippocampal neurons stained for vLGUT1 (red), the above-threshold signal (black) and counted particles (bright blue) per frame. The obtained data is quantified in the graph of the right. No change in glutamatergic terminal density was observed for LRRK2 kinase inhibitor treatment. (Nested t-test; t = (58) = 1.16, p = 0.25, n=3, 10 measurements per sample) B) Confocal images of glutamatergic terminals in coronal sections of the mouse striatum, the above-threshold signal (black) and counted particles (bright blue). No change of glutamatergic terminal density was observed upon LRRK2 kinase inhibitor treatment (PF-360). (Nested t-test; t = (58) = 0.88, p = 0.38, n=3, 10 measurements per sample) C) Shows are confocal images of the dorsal mouse striatum stained for DAT (red) and the above threshold signal (black) for control (left) and PF-360 treated animals (right). LRRK2 kinase inhibitor treatment significantly increased the integrated density of DAT signal compared to control, as visualized in the graph on the right. (Nested t-test; t = (4) = 2.99, p = 0.04, *p
External and internal security in the Australian colonies from their founding to the end of the Macquarie era
Creators: name: McMahon, JF
Publisher: name: University Of Tasmania
Year: 2023

description: This thesis considers external and internal security in the Australian colonies from the founding of New South Wales to the end of the Macquarie era. As history is a continuum, matters outside the nominated time frame of 1788 to 1821 are, where relevant, considered. This study is not a sociological history of British forces, nor concerned with their many roles, unless applicable. However, to appreciate European concepts of sovereignty which influenced Pitt's government in selecting secure colonial borders, consideration is given to the discovery of New Holland and New South Wales. New South Wales lay athwart zones of strategic interest to the Dutch in the East Indies and the Spanish in the Pacific. Spanish claims were ignored, but to prevent international tension with Holland, Britain selectively prescribed the colony's western border. Additionally, with France, under the Bourbons and Napoleon, apparently planning settlements in Australia, Britain established outposts at Norfolk Island, Risdon Cove and Port Phillip, After 1815, possible Dutch and French intrusion in the region saw the establishment of outposts at Melville Island, Albany and Westernport. At Swan River in 1829, sovereignty was proclaimed and a settlement established, ensuring the whole of Australia became a British domain. The garrisons' internal security role was to support and defend the civil power. From the arrival of the Second Fleet in 1790, until 1810, the New South Wales Corps carried out these duties (receiving historical notoriety for their insurrection in 1808). Thereafter, other regiments were posted to the colony for shorter periods. Tasks included guarding convicts, hunting bushrangers, and protecting settlers on the spreading colonial borders. The Castle Hill Rebellion of 1804, was the most serious internal security situation faced. After the Napoleonic Wars, economic stringencies seriously limited the garrison's strength, yet the number of convicts transported significantly increased, placing a heavy load on the security forces. Until 1810, internal security was weakened by a long running struggle for domination between the military and civil powers. This commenced with Marine officers' dissatisfaction with Phillip's government and culminated with the New South Wales Corps mutiny against Bligh. From 1810, Macquarie established the primacy of the civil over the military power. By his departure in 1821, Sydney Cove had developed from a penal settlement into a colony ready for civic reforms resulting from the Bigge Inquiry. Maintenance of internal security allowed colonial development to take place, whilst threats to external security were the prime reason for the continent of Australia coming under British sovereignty.
An introduction to hyperlinear and sofic groups
Creators: name: Pestov, Vladimir G.
name: Kwiatkowska, Aleksandra
Publisher: name: arXiv
Year: 2009
Subjects: subject: Group Theory (math.GR)
subject: FOS: Mathematics
subject: 03C20, 20F69, 37B10, 46L10

description: This is an edited write-up of lecture notes of the 7-th Appalachian set theory workshop of the same title led by the first named author at the Cornell University on November 22, 2008. A draft version of the notes was prepared by the second named author. This presentation is largely complementary to the earlier survey by the first-named author (Hyperlinear and sofic groups: a brief guide, Bull. Symb. Logic 14 (2008), pp. 449-480; arXiv:0804.3968v8 [math.GR]).
description: 30 pages, 1 figure, latex 2e; a final revision for the volume "Appalachian Set Theory 2006-2009" (James Cummings and Ernest Schimmerling, eds.), to appear in the London Mathematical Society Lecture Notes Series, Cambridge University Press (2012). Compared to the previous version, a few references were added, and a misstated result by Osin and Thomas was corrected
Relatório Queimadas 2022 no Estado do Acre
Creators: name: Silva, Sonaira
name: De Melo, Antonio Willian Flores
name: Reis, João Dos
name: De Paula, Yara
name: Anderson, Liana
Publisher: name: Zenodo
Year: 2023

description: As queimadas são monitoradas operacionalmente pelos focos de calor, que são pontos quentes na superfície terrestre detectadas por sensores remotos e indicam a ocorrência de fogo ativo naquele momento e local. Entretanto, com estes dados não é possível saber a extensão das áreas afetadas pelas queimadas. Neste contexto, o Projeto Acre Queimadas (CNPq/Prevfogo - Ibama Nº 33/2018, processo: 442650/2018-3), tem como um dos objetivos quantificar áreas queimadas do estado do Acre através de técnicas de mapeamento utilizando imagens satelitais, trazendo informações sobre a extensão das áreas afetadas pelo fogo e sua localização.queimadas do estado do Acre através de técnicas de mapeamento utilizando imagens satelitais, trazendo informações sobre a extensão das áreas afetadas pelo fogo e sua localização.
The technical and environmental efficiency of the Australian irrigation schemes
Creators: name: Liu, Gang
Publisher: name: University Of Tasmania
Year: 2023

description: Water resource management reform occupies a prominent place in Australia because deficiencies in the management of water and salinity are rapidly moving Australia towards a serious shortage of quality water. The objective of this study is to develop a comprehensive index to identify a best practice as benchmark for the Australian irrigation industry in relation to irrigation water delivery and the treatment of salinity. The efficiency performance of the sampled irrigation schemes is measured against the benchmark which will also provide information on an scheme's managerial capacity and operating environment. This information can help scheme managers and government agencies and policy makers to identify clear targets management improvements and effective policy. The sampled schemes involved in this study are mainly drawn from the Murray Darling Basin (MDB) which constitutes seventy five percent of Australia's irrigated area. Over ninety five percent water resources in the basin are used for irrigation activities. More than twenty five percent of irrigation water is lost in the conveyance system through seepage, leakage and evaporation. The MDB has also long been recognised as one of Australia's most important environmental concerns. The improvement of the productive efficiency of water delivery off-farm and the efficiency in treating salt emissions in the MDB is important to Australia. This study develops a panel data modelling framework using stochastic frontier analysis and data envelopment analysis techniques, which are used to assess the efficiency of the major Australian irrigation schemes. Although the efficiency measures obtained from the stochastic frontier analysis and the data envelopment analysis are correlated with respect to efficiency scores ranking, there is strong evidence of the presence of random noise in data set applied to the study. Thus, the conclusions in relation to policy implication are drawn from the stochastic frontier analysis which does accommodate random noise. The results reveal the following: (1) there is evidence of some technical and environmental inefficiency in the operation of Australia's irrigation system in each of the years 98/99, 99/00 and 00/01; (2) both technical and environmental efficiency appear to be improving over time; (3) the potential savings of the water resource and potential reductions in salt emissions are substantial if the industry can achieve full technical and environmental efficiency; (4) NSW and Victorian schemes outperform Queensland schemes with respect to technical efficiency but there is no evidence that privately run schemes operate significantly more efficiently than publicly run schemes; (5) the operating environment is not conductive to the achievement of efficiency improvements.
Additional file 2 of Inhibition of LRRK2 kinase activity promotes anterograde axonal transport and presynaptic targeting of α-synuclein
Creators: name: Brzozowski, Charlotte F.
name: Hijaz, Baraa A.
name: Singh, Vijay
name: Gcwensa, Nolwazi Z.
name: Kelly, Kaela
name: Boyden, Edward S.
name: West, Andrew B.
name: Sarkar, Deblina
name: Volpicelli-Daley, Laura A.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 2: Fig. S2. Reduction of LRRK2 immunofluorescence signal in LRRK2 KO mice. A) LRRK2 immunofluorescence in C57BL/6J LRRK2 KO mice (kindly provided by Dr. Matthew Goldberg, UAB) is visibly reduced in the striatum and cortex compared to wildtype mice. B) Confocal images of mouse brain sections immunostained for LRRK2 (green) and presynaptic markers (vLGUT1 in red, VAMP2 in blue) show colocalization, especially for glutamatergic terminals in the striatum.
SN 1999ga: a low-luminosity linear type II supernova?
Creators: name: Pastorello, A.
name: Crockett, R. M.
name: Martin, R.
name: Smartt, S. J.
name: Altavilla, G.
name: Benetti, S.
name: Botticella, M. T.
name: Cappellaro, E.
name: Mattila, S.
name: Maund, J. R.
name: Ryder, S. D.
name: Salvo, M.
name: Taubenberger, S.
name: Turatto, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Type II-linear supernovae are thought to arise from progenitors that have lost most of their H envelope by the time of the explosion, and they are poorly understood because they are only occasionally discovered. It is possible that they are intrinsically rare, but selection effects due to their rapid luminosity evolution may also play an important role in limiting the number of detections. In this context, the discovery of a subluminous type II-linear event is even more interesting. We investigate the physical properties and characterise the explosion site of the type II SN 1999ga, which exploded in the nearby spiral galaxy NGC 2442. Spectroscopic and photometric observations of SN 1999ga allow us to constrain the energetics of the explosion and to estimate the mass of the ejected material, shedding light on the nature of the progenitor star in the final stages of its life. The study of the environment in the vicinity of the explosion site provides information on a possible relation between these unusual supernovae and the properties of the galaxies hosting them. Despite the lack of early-time observations, we provide reasonable evidence that SN 1999ga was probably a type II-linear supernova that ejected a few solar masses of material, with a very small amount of radioactive elements of the order of 0.01 solar masses.
description: 11 pages, 9 figures. Accepted for publication in A&A (March 28, 2009)
Mapping 6D N = 1 supergravities to F-theory
Creators: name: Kumar, Vijay
name: Morrison, David R.
name: Taylor, Washington
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We develop a systematic framework for realizing general anomaly-free chiral 6D supergravity theories in F-theory. We focus on 6D (1, 0) models with one tensor multiplet whose gauge group is a product of simple factors (modulo a finite abelian group) with matter in arbitrary representations. Such theories can be decomposed into blocks associated with the simple factors in the gauge group; each block depends only on the group factor and the matter charged under it. All 6D chiral supergravity models can be constructed by gluing such blocks together in accordance with constraints from anomalies. Associating a geometric structure to each block gives a dictionary for translating a supergravity model into a set of topological data for an F-theory construction. We construct the dictionary of F-theory divisors explicitly for some simple gauge group factors and associated matter representations. Using these building blocks we analyze a variety of models. We identify some 6D supergravity models which do not map to integral F-theory divisors, possibly indicating quantum inconsistency of these 6D theories.
description: 37 pages, no figures; v2: references added, minor typos corrected; v3: minor corrections to DOF counting in section 5
Studies of Parton Propagation and Hadron Formation in the Space-Time Domain
Creators: name: Brooks, W. K.
name: Hakobyan, H.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Over the past decade, new data from HERMES, Jefferson Lab, Fermilab, and RHIC that connect to parton propagation and hadron formation have become available. Semi-inclusive DIS on nuclei, the Drell-Yan reaction, and heavy-ion collisions all bring different kinds of information on parton propagation within a medium, while the most direct information on hadron formation comes from the DIS data. Over the next decade one can hope to begin to understand these data within a unified picture. We briefly survey the most relevant data and the common elements of the physics picture, then highlight the new Jefferson Lab data, and close with a prospective for the future.
description: Invited talk delivered at the Sixth International Conference on Perspectives in Hadronic Physics, ICTP, Trieste, Italy, 12-16 May 2008. 8 pages, 5 figures
Spectroscopic study of the N159/N160 complex in the Large Magellanic Cloud
Creators: name: Fariña, Cecilia
name: Bosch, Guillermo L.
name: Morrell, Nidia I.
name: Barbá, Rodolfo H.
name: Walborn, Nolan R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present a spectroscopic study of the N159/N160 massive-star forming region south of 30 Doradus in the Large Magellanic Cloud, classifying a total of 189 stars in the field of the complex. Most of them belong to O and early B spectral classes; we have also found some uncommon and very interesting spectra, including members of the Onfp class, a Be P Cygni star, and some possible multiple systems. Using spectral types as broad indicators of evolutionary stages, we considered the evolutionary status of the region as a whole. We infer that massive stars at different evolutionary stages are present throughout the region, favoring the idea of a common time for the origin of recent star formation in the N159/N160 complex as a whole, while sequential star formation at different rates is probably present in several subregions.
description: 36 pages, 24 figures (127 spectra mostly OB stars, 4 field images). Published in The Astronomical Journal
Additional file 3 of Inhibition of LRRK2 kinase activity promotes anterograde axonal transport and presynaptic targeting of α-synuclein
Creators: name: Brzozowski, Charlotte F.
name: Hijaz, Baraa A.
name: Singh, Vijay
name: Gcwensa, Nolwazi Z.
name: Kelly, Kaela
name: Boyden, Edward S.
name: West, Andrew B.
name: Sarkar, Deblina
name: Volpicelli-Daley, Laura A.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 3: Fig. S3. No change of localization of synapsin-1 upon LRRK2 kinase inhibitor treatment. A) Colocalization analysis of a mouse cohort treated with LRRK2 kinase inhibitor PF-360 and control mice showed no significant difference in overlap of vGLUT1 (red) and Synapsin-1 (green). Confocal images of the dorsal striatum as well as colocalized pixel maps are shown for visualization. (Nested t-test t = (2) = 0.43. p = 0.71, n = 2, 9 measurements per sample). B) High resolution imaging analysis with ExPath (Expansion Pathology, protocol adapted from Bucur et al. (2020), Nature Protocols) showed no significant change of synapsin-1 (blue) localization at the presynaptic terminal between control animals and PF-360 treated animals. Shown are confocal images of ExPath samples stained for presynaptic markers vGLUT1 (red) and Synapsin-1 (blue) and postsynaptic marker Homer1 (green). (Nested t-test: vGLUT1/Homer1: t = (2) = 0.74, p = 0.54, vGLUT1/synapsin-1: t = (2) = 1.05, p = 0.40, n = 2, 10 measurements per sample).
Fate of Z(N) walls in hot holographic QCD
Creators: name: Yee, Ho-Ung
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We first study Z(N) walls in a deconfined phase of Witten's D4-brane background of pure SU(N) Yang-Mills theory, motivated by a recent work in the case of N=4 SYM. Similarly to it, we propose that for a large wall charge k ~ N, it is described by k D2-branes blown up into a NS5-brane wrapping S^3 inside S^4 via Myers effect, and we calculate the tension by suitable U-duality. We find a precise Casimir scaling for the tension formula. We then study the fate of Z(N)-vacua in a presence of fundamental flavors in quenched approximation via gauge/gravity correspondence. In the case of D3/D7 system where one can vary the mass m_q of flavors, we show that there is a phase transition at T_c ~ m_q, below which the Z(N)-vacua survive while they are lifted above the critical temperature. We analytically calculate the energy lift of k'th vacua in the massless case, both in the D3/D7 system and in the Sakai-Sugimoto model.
description: 24 pages, v2: references updated, v3: A clarification on the meaning of Z(N) walls in Euclidean space added, citations updated
On reductions of soliton solutions of multi-component NLS models and spinor Bose-Einstein condensates
Creators: name: Gerdjikov, V. S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: We consider a class of multicomponent nonlinear Schrodinger equations (MNLS) related to the symmetric BD.I-type symmetric spaces. As important particular case of these MNLS we obtain the Kulish-Sklyanin model. Some new reductions and their effects on the soliton solutions are obtained by proper modifying the Zakahrov-Shabat dressing method.
description: AIP AMiTaNS'09 Proceedings,
UBVRI Photometric Standard Stars Around the Celestial Equator: Updates and Additions
Creators: name: Landolt, Arlo U.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: New broadband UBVRI photoelectric observations on the Johnson-Kron-Cousins photometric system have been made of 202 stars around the sky, and centered at the celestial equator. These stars constitute both an update of and additions to a previously published list of equatorial photometric standard stars. The list is capable of providing, for both celestial hemispheres, an internally consistent homogeneous broadband standard photometric system around the sky. When these new measurements are included with those previously published by Landolt (1992), the entire list of standard stars in this paper encompasses the magnitude range 8.90 < V < 16.30, and the color index range -0.35 < (B - V) < +2.30.
description: 66 pages, 11 figures; complete version (including finding charts) to appear in May issue of AJ (2009, 137, 4186)
On volumes of hyperbolic orbifolds
Creators: name: Adeboye, Ilesanmi
name: Wei, Guofang
Publisher: name: arXiv
Year: 2009
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 57N15, 57M50

description: In this paper we derive an explicit lower bound on the volume of a hyperbolic $n$-orbifold for dimensions greater than or equal to four. Our main tool is H. C. Wang's bound on the radius of a ball embedded in the fundamental domain of a discrete subgroup of a semisimple Lie group.
description: 19 pages, LaTeX; typos added, Section 5 revised
Additional file 1 of Quantifying contact patterns in response to COVID-19 public health measures in Canada
Creators: name: Brankston, Gabrielle
name: Merkley, Eric
name: Fisman, David N.
name: Tuite, Ashleigh R.
name: Poljak, Zvonimir
name: Loewen, Peter J.
name: Greer, Amy L.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1.
The Motion of Water Masers in the Pre-Planetary Nebula IRAS 16342-3814
Creators: name: Claussen, M. J
name: Sahai, R.
name: Morris, M. R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present high angular resolution observations, using the Very Long Baseline Array (VLBA) of the NRAO, of the high-velocity water masers toward the "water-fountain" pre-planetary nebula, IRAS 16342-3814. The detailed structure of the water masers appears to be that of bow shocks on either side of a highly collimated jet. The proper motions of the water masers are approximately equal to the radial velocities; the three-dimensional velocities are approximately +/-180 km/s, which leads to a very short dynamical time-scale of ~100 years. Although we do not find direct evidence for precession of the fast collimated jet, there may be indirect evidence for such precession.
description: Accepted by the Astrophysical Journal
The effect of temperature on protein synthesis and growth efficiency in juvenile barramundi, Lates calcarifer
Creators: name: Katersky, Robin Sue
Publisher: name: University Of Tasmania
Year: 2023

description: Temperature has a marked and direct effect on key physiological processes in fish, each species has a range of temperatures over which it survives (thermal tolerance range) and where growth occurs. Culture of barramundi, Lates calcarifer, is occurring at temperatures across the thermal tolerance (15-40¬¨‚àûC). Consequently, this thesis examined the effect of temperature on protein metabolism: feed intake (FI, g.d‚ÄövÖ¬™¬¨œÄ), growth (SGR, %.d‚ÄövÖ¬™¬¨œÄ), growth efficiency (in relation to protein and energy retention) and protein synthesis (ks, %.d‚ÄövÖ¬™¬¨œÄ) were measured. Fish were fed to satiation daily on the same diet. Protein synthesis was determined using the flooding dose method with ¬¨‚â•H-phenylalanine. Models of Fl, SGR and growth efficiency were developed from two experiments. The first examined temperatures from 21-33¬¨‚àûC at 3¬¨‚àûC intervals and the second looked at temperatures 27, 33, 36 and 39 ¬¨‚àûC. These models calculate the optimal temperature for each parameter to be 31¬¨‚àûC. However, the optimal range for maximum growth efficiency (both PPV and PEV) is estimated to be 10 times wider than for Fl or SGR. These models also predict an optimal temperature which is ‚ÄövÑvÆ4¬¨‚àûC higher than what has been previously determined for barramundi. The broad optimal range for growth efficiency is much more extensive than previously recognized for barramundi. Experiments were conducted to quantify the effect of temperature on protein synthesis (ks). The first experiment examined white muscle (WM) and whole body (WB) lc, from 21-33¬¨‚àûC, at 3¬¨‚àûC intervals, 24 h after feeding. No significant differences existed between temperatures, however regardless of temperature WBk, was ‚ÄövÑvÆ4 times greater than WMIcs. A second experiment was conducted at 21, 27 and 33¬¨‚àûC on the WM, Liver and WBk, at times 0, 4, 8, 12 and 24 h after feeding. At the 27 and 33¬¨‚àûC WMks peaked 6 h after feeding and remained significantly elevated over the initial 12 h. A final experiment was conducted at 27, 33, 36 and 39¬¨‚àûC on the WM, Liver, stomach, digestive tract and WBks at times 0, 2, 4, 6, 8, 12, and 24 h after feeding. No differences occur between WBk, at 27 and 33¬¨‚àûC and peaks occur ‚ÄövÑvÆ3 h after feeding; liver ks peaks 2 h after feeding and is an order of magnitude higher than WBks. At 21 and 39¬¨‚àûC, WBIcs is not affected by feeding and this corresponds to the low growth rates observed at these temperatures. The results of the three protein synthesis experiments have been combined with protein growth data to model protein turnover over the thermal tolerance range for juvenile barramundi.
MASTER prompt and follow-up GRB observations
Creators: name: Tyurina, Nataly
name: Lipunov, Vladimir
name: Kornilov, Victor
name: Gorbovskoy, Evgeny
name: Shatskij, Nikolaj
name: Kuvshinov, Dmitry
name: Balanutsa, Pavel
name: Belinski, Alexander
name: Krushinsky, Vadim
name: Zalozhnyh, Ivan
name: Tlatov, Andrey
name: Parkhomenko, Alexander
name: Ivanov, Kirill
name: Yazev, Sergey
name: Kortunov, Petr
name: Sankovich, Anatoly
name: Kuznetsov, Artem
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: There are the results of gamma-ray bursts observations obtained using the MASTER robotic telescope in 2007 - 2009. We observed 20 error-boxes of gamma-ray bursts this period.The limits on their optical brightnesses have been derived. There are 5 prompt observations among them, obtained at our very wide field cameras. Also we present the results of the earliest observations of the optical emission of the gamma-ray bursts GRB 050824 and GRB 060926.
description: 10 pages, 2 figures
The distribution of stellar mass in the low-redshift Universe
Creators: name: Li, Cheng
name: White, Simon D. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use a complete and uniform sample of almost half a million galaxies from the Sloan Digital Sky Survey to characterise the distribution of stellar mass in the low-redshift Universe. Galaxy abundances are well determined over almost four orders of magnitude in stellar mass, and are reasonably but not perfectly fit by a Schechter function with characteristic stellar mass m* = 6.7 x 10^10 M_sun and with faint-end slope α= -1.155. For a standard cosmology and a standard stellar Initial Mass Function, only 3.5% of the baryons in the low-redshift Universe are locked up in stars. The projected autocorrelation function of stellar mass is robustly and precisely determined for r_p < 30 Mpc/h. Over the range 10 kpc/kpc < r_p < 10 Mpc/h it is extremely well represented by a power law. The corresponding three-dimensional autocorrelation function is ξ*(r) = (r/6.1 Mpc/h)^{-1.84}. Relative to the dark matter, the bias of the stellar mass distribution is approximately constant on large scales, but varies by a factor of five for r_p < 1 Mpc/h. This behaviour is approximately but not perfectly reproduced by current models for galaxy formation in the concordance LCDM cosmology. Detailed comparison suggests that a fluctuation amplitude σ_8 ~ 0.8 is preferred to the somewhat larger value adopted in the Millennium Simulation models with which we compare our data. This comparison also suggests that observations of stellar mass autocorrelations as a function of redshift might provide a powerful test for the nature of Dark Energy.
description: 12 pages, 11 figures, accepted for publication in Monthly Notices, two appendices added to explore possible systematic biases due to the stellar mass definition and surface density limits
СИСТЕМА ПЛАНИРОВАНИЯ И УПРАВЛЕНИЯ В МЕЛКОСЕРИЙНОМ И ЕДИНИЧНОМ ПРОИЗВОДСТВЕ
Creators: name: Каландаров Илёс Ибодуллаевич
Publisher: name: TECHика
Year: 2020
Subjects: система планирования
календарное планирование
единичное производства
производственный цикл
эвристический метод

description: Система планирования и управления должны быть адаптивной, с изменяющейся производственной ситуацией, иметь возможность подстраиваться под ситуации на участке и на производстве в целом. В этих условиях требуется разрабатывать новые подходы и методы решения задач планирования и управления. В данной работе рассматривается повышение эффективности производства с помощью первого способа, реализованного путем управления организацией производства и оперативным управлением производственного подразделения.
Saint Sebastian and the wounded forest : personal relationship with the tasmanian landscape
Creators: name: Lendis, Andrew John
Publisher: name: University Of Tasmania
Year: 2023

description: Saint Sebastian and the Wounded Forest is a project that sets out to show that painting has the ability to evoke a truly emotional, poetic, connection with the Tasmanian wilderness because it has the capacity to create, and exist within, its own space and time. Through an investigation into the way that icons operate and into the way that the presentation of space and time in the construction of a painting can affect whether a painting is experienced on an intellectual or an emotional level, I have come to an understanding of how certain painters such as Albrecht Altdorfer and more recently Stanley Spencer and Peter Booth, control the viewers' response to their work. This project is an investigation into, and an attempt to prove through practice, the proposition that painting is different from other art practices such as photography in that it can exist outside of time, and thus can be free of time. It is able to manipulate and conjecture its own laws of temporality. This project also investigates the proposition that a painting can exist as a place (that is to say: a space to be in) on its own terms precisely because it possesses the ability to define and control its own space in the world and can construct and collapse space in the same way that it can collapse time. This project proposes that the effect produced by this ability has the capacity to produce a sense of transcendence in the beholder, an impression that could be described as time standing still or as an unexplainable response that elicits deep emotion (a half- remembered memory of a place or time, or both, known from long ago). The outcome of the research project is a series of paintings that aims to disrupt the viewer's ability to undertake an intellectual reading of the manifest subject in the work and, rather, force the viewer to experience the works on a purely emotional level. It is intended that this emotional engagement might form a bridge between the viewer's own experience and what they seek within the image, which is something invisible and hidden behind the painting's skin and is also a re-enactment of my own process of painting.
PEDOMAN WAWANCARA.docx
Creators: name: Nining, Sri
Publisher: name: figshare
Year: 2023
Subjects: classificationCode: 420502
subject: Aged care nursing
classificationCode: 420503
subject: Community and primary care
classificationCode: 420504
subject: Mental health nursing
classificationCode: 420505
subject: Nursing workforce

description: Include:Demographi data and interview questions
The Enrichment of the Intracluster Medium
Creators: name: Sivanandam, Suresh
name: Zabludoff, Ann I.
name: Zaritsky, Dennis
name: Gonzalez, Anthony H.
name: Kelson, Dan D.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: To determine the relative contributions of galactic and intracluster stars to the enrichment of the intracluster medium (ICM), we present X-ray surface brightness, temperature, and Fe abundance profiles for a set of twelve galaxy clusters for which we have extensive optical photometry. Assuming a standard IMF and simple chemical evolution model scaled to match the present-day cluster early-type SN Ia rate, the stars in the brightest cluster galaxy (BCG) plus the intracluster stars (ICS) generate 31^{+11}_{-9}%, on average, of the observed ICM Fe within r_{500} (~ 0.6 times r_{200}, the virial radius). An alternate, two-component SN Ia model (including both prompt and delayed detonations) produces a similar BCG+ICS contribution of 22^{+9}_{-9}%. Because the ICS typically contribute 80% of the BCG+ICS Fe, we conclude that the ICS are significant, yet often neglected, contributors to the ICM Fe within r_{500}. However, the BCG+ICS fall short of producing all the Fe, so metal loss from stars in other cluster galaxies must also contribute. By combining the enrichment from intracluster and galactic stars, we can account for all the observed Fe. These models require a galactic metal loss fraction (0.84^{+0.11}_{-0.14}) that, while large, is consistent with the metal mass not retained by galactic stars. The SN Ia rates, especially as a function of galaxy environment and redshift, remain a significant source of uncertainty in further constraining the metal loss fraction. For example, increasing the SN Ia rate by a factor of 1.8 -- to just within the 2 sigma uncertainty for present-day cluster early-type galaxies -- allows the combined BCG + ICS + cluster galaxy model to generate all the ICM Fe with a much lower galactic metal loss fraction (~ 0.35).
description: 27 pages, 9 figures, 7 tables. Accepted for publication in ApJ
Additional file 2 of Quantifying contact patterns in response to COVID-19 public health measures in Canada
Creators: name: Brankston, Gabrielle
name: Merkley, Eric
name: Fisman, David N.
name: Tuite, Ashleigh R.
name: Poljak, Zvonimir
name: Loewen, Peter J.
name: Greer, Amy L.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 2.
On Magnesium Sulfide as the Carrier of the 30micron Emission Feature in Evolved Stars
Creators: name: Zhang, Ke
name: Jiang, Biwei
name: Li, Aigen
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A large number of carbon-rich evolved objects (asymptotic giant branch stars, protoplanetary nebulae, and planetary nebulae) in both the Milky Way galaxy and the Magellanic Clouds exhibit an enigmatic broad emission feature at 30 micron. This feature, extending from 24 micron to 45 micron, is very strong and accounts for up to 30% of the total infrared luminosity of the object. In literature it is tentatively attributed to magnesium sulfide (MgS) dust. Using the prototypical protoplanetary nebula around HD 56126 for illustrative purpose, however, in this work we show that in order for MgS to be responsible for the 30 micron feature, one would require an amount of MgS mass substantially exceeding what would be available in this source. We therefore argue that MgS is unlikely the carrier of the 30 micron feature seen in this source and in other sources as well.
description: 16 pages, 3 figures, accepted by ApJ
RESEARCH OF THE OXIDATIVE PROCESS OF GOLD-CONTAINING SULFIDE MATERIALS ROASTING FOR THE DEVELOPMENT OF AN OPTIMAL MODE
Creators: name: Tolibov Behzod
Publisher: name: TECHика
Year: 2020
Subjects: oxidative calcination
drying
fluidized bed furnace
sulfides
suspended calcination
refractory ores
gold-arsenic ores
biooxidation cake
desulfurization
recovery
fluidized bed
humidity
pyrometallurgy
undeoxidation
sintering of pieces.

description: Now, in world practice, sulphide refractory gold-containing materials are subjected to oxidative roasting mainly with low productivity and subsequent cyanidation provides a high degree of metal recovery. Of particular importance is oxidative calcination to increase the extraction of valuable components (Au, Ag, Mo, W, Cu, Zn) from metal-containing intermediate products. Today, new technologies and technological schemes are being developed around the world in the field of processing gold-bearing ores to increase the degree of extraction and reduce processing costs in order to reduce the cost of the product, and special attention is paid to reducing the content of a valuable component in the tailings of processes, as well as special attention paid to reduce the content of a valuable component in the tailings of production processes. In this aspect, the development of new technologies and the improvement of existing technologies to increase the extraction of valuable components are urgent tasks of the science and practice of the mining and metallurgical industry. The aim of the research was to develop an effective technology for processing sulfide materials in suspension in a kiln to intensify the process and increase the yield of valuable components.
Eta Carinae across the 2003.5 Minimum: Analysis in the visible and near infrared spectral region
Creators: name: Nielsen, K. E.
name: Kober, G. Vieira
name: Weis, K.
name: Gull, T. R.
name: Stahl, O.
name: Bomans, D. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present an analysis of the visible through near infrared spectrum of Eta Carinae and its ejecta obtained during the "Eta Carinae Campaign with the UVES at the ESO VLT". This is a part of larger effort to present a complete Eta Carinae spectrum, and extends the previously presented analyses with the HST/STIS in the UV (1240-3159 A) to 10,430 A. The spectrum in the mid and near UV is characterized by the ejecta absorption. At longer wavelengths, stellar wind features from the central source and narrow emission lines from the Weigelt condensations dominate the spectrum. However, narrow absorption lines from the circumstellar shells are present. This paper provides a description of the spectrum between 3060 and 10,430 A, including line identifications of the ejecta absorption spectrum, the emission spectrum from the Weigelt condensations and the P-Cygni stellar wind features. The high spectral resolving power of VLT/UVES enables equivalent width measurements of atomic and molecular absorption lines for elements with no transitions at the shorter wavelengths. However, the ground based seeing and contributions of nebular scattered radiation prevent direct comparison of measured equivalent widths in the VLT/UVES and HST/STIS spectra. Fortunately, HST/STIS and VLT/UVES have a small overlap in wavelength coverage which allows us to compare and adjust for the difference in scattered radiation entering the instruments' apertures. This paper provides a complete online VLT/UVES spectrum with line identifications and a spectral comparison between HST/STIS and VLT/UVES between 3060 and 3160 A.
description: 13 pages, 11 figures + atlas. The paper accepted for the ApJS and is accompanied with an atlas in the online edition paper
Simulink File For: " A Method for Charging Electric Vehicles with Battery-supercapacitor Hybrid Energy Storage Systems to Improve Voltage Quality and Battery Lifetime in Islanded Building-level DC Microgrids"
Creators: name: Abadi, Seyyed Ali Ghorashi Khalil
Publisher: name: Zenodo
Year: 2023
Subjects: Electric Vehicle Charging
Microgrids
Voltage Control
Battery Energy Storage
Supercapacitor

description: This package includes MATLAB Simulink files related to the paper entitled "A Method for Charging Electric Vehicles with Battery-supercapacitor Hybrid Energy Storage Systems to Improve Voltage Quality and Battery Lifetime in Islanded Building-level DC Microgrids." published in IEEE Transactions on Sustainable Energy. Click on Link to the paper to see the publication. DOI of the paper: https://doi.org/10.1109/TSTE.2023.3254597
description: Please read the readme.txt file first.