bluuebunny/crossref_metadata_2025_split huggingface dataset:
Preferensi Pemilihan Tipe Rumah dan Lokasi Perumahan Pada Masyarakat Menengah ke Atas di Daerah Pinggiran Kota Yogyakarta
Authors: Leo Kristina Sryla Dhiu 
Published: May 2020

Pemenuhan akan tempat tinggal di area pusat Kota Yogyakarta semakin hari semakin terbatas sejalan dengan meningkatnya jumlah penduduk kota dan keterbatasan lahan untuk membangun tempat tinggal membuat warga kota memilih untuk mencari tempat tinggal di daerah pinggiran kota. Hal ini berdampak pada tumbuhnya perumahan-perumahan formal di pinggiran kota yang menjadi daya tarik masyarakat khususnya masyarakat menengah ke atas dalam memilih hunian sesuai dengan preferensi dan kriteria yang diinginkan. Tujuan penelitian ini adalah untuk mengetahui preferensi pemilihan lokasi perumahan dan tipe hunian pada masyarakat menengah ke atas dan mengetahui hubungan antara karakteristik sosial ekonomi individu/rumah tangga dengan pemilihan tipe rumah. Metode yang digunakan adalah menggunakan pendekatan deduktif dengan analisis deskriptif guna mengetahui preferensi pemilihan lokasi perumahan dan analisis tabulasi silang untuk mengetahui hubungan antara status sosial masyarakat dengan tipe rumah di wilayah penelitian. Teknik Pengumpulan data menggunakan kuesioner dan observasi lapangan. Hasil akhir penelitian ini menyatakan bahwa faktor keamanan dan kenyamanan merupakan faktor yang paling berpengaruh dalam memilih lokasi perumahan bagi masyarakat menengah keatas, faktor selanjutnya adalah kondisi fisik perumahan dan investasi. Karakteristik kondisi sosial ekonomi yang memiliki korelasi dengan pemilihan tipe rumah pada masyarakat menengah ke atas adalah tingkat pendapatan.
The Evolutionary Development of Transit Transport of Temperature-Sensitive Goods
Authors: Tsvetkov V. A. , Zoidov K. Kh. , Medkov A. A. 
Published: May 2020

The presented study identifies modern organizational and institutional trends in the evolutionary development of transit transport of temperature-sensitive goods.Aim. The study aims to determine the place and role of transit transport of temperature-sensitive goods across Russia and within the Eurasian space via global communication lines as an efficient direction for the development of transit economy, an innovative method of transport, and a highly profitable form of export for transport services.Tasks. The authors examine, systematize, and analyze the organizational and institutional directions for the evolutionary development of transit transport of temperature-sensitive goods and formulate proposals for implementing the most efficient corporate mechanisms for the development of transit economy in Russia and formation of a global Eurasia.Methods. This study uses the methods of evolutionary-institutional theory, systems analysis, theory of engineering and manufacturing balance, and historical approach.Results. It is determined that the development of transport of temperature-sensitive and other sensitive goods should be evolutionary. In the early 21st century, the transport of fish and seafood from the Asia-Pacific region to the European Union is becoming increasingly important for meeting the demands of retail trade and the food service industry. The benefits (competitive advantages) and shortcomings (market problems) of transit transport of temperature-sensitive goods by different modes of transport are identified. A set of organizational and institutional measures has been developed to improve the traceability of movement of Russian food products for the purpose of development, dispatch, and regular operation of a fleet of “cold express trains”.Conclusions. One of the organizational and institutional directions for the evolutionary development of transit transport of temperature-sensitive goods involves the activity of supranational political and integration entities, primarily the Eurasian Economic Union (EAEU) and the Shanghai Cooperation Organisation (SCO), and their efforts to create a unified transport space and to combine infrastructure and integration projects. The establishment of a supranational Eurasian Transit Transport Company (ETTC) should serve as a corporate framework for integration processes within the global Eurasian space in terms of linking transport and communication systems.
SE NON ESISTESSE UN LUOGO DOVE STARE AL SICURO? TERREMOTO E SUBLIME: DAGLI SCRITTI PRE-CRITICI ALLA KRITIK DER URTEILSKRAFT
Authors: CARAMEL Niccolò , POGGI Davide 
Published: May 2020

Lo spaventoso sisma di Lisbona, verificatosi il 1° novembre 1755, non comportò solo incalcolabili devastazioni sul piano socio-economico, ma andò a colpire profondamente tanto l’immaginario popolare (minandone le certezze quotidiane), quanto i savants dell’Europa settecentesca, stimolando un’intensa riflessione (che coprì l’intero spettro dei punti di vista, da quello teologico, a quello scientifico). Il giovane Kant è chiaro exemplum dell’interesse suscitato dall’eccezionale fenomeno tellurico presso gli illuministi: tra il gennaio e l’aprile del 1756, egli dette alle stampe tre brevi saggi interamente dedicati alla descrizione scientifica del terremoto portoghese, saggi che si inseriscono nel contesto degli studi del pensatore di Königsberg riguardanti la filosofia della natura e, nello specifico, l’età, l’origine e la costituzione della terra (oggetto dei saggi del 1754 e del 1755). Con il presente lavoro, si intende portare all’attenzione del lettore quella che pare essere una precisa evoluzione della concezione dell’utilità del terremoto, nel passaggio dal periodo pre-critico a quello critico, in particolare nella Kritik der Urteilskraft (1790). Qui l’Autore pare escludere il terremoto dall’elenco degli eventi naturali catastrofici la cui esperienza, “se ci troviamo al sicuro”, genera nell’uomo il concetto di sublime dinamico (KU, AA 05: 261). Quali sono le ragioni per cui il terremoto non trova spazio in questo discorso? Il sisma perde cioè i caratteri di catastrofe agli occhi di Kant, oppure è giudicato così terrificante da togliere ogni razionalità all’uomo e impedire ogni spiraglio interpretativo?
The effect of study abroad on intercultural competence: Results from a longitudinal quasi-experimental study
Authors: Heinzmann Sybille , Künzle Roland , Schallhart Nicole , Müller Marianne 
Published: May 2020

This study analyses the impact of short-term study abroad experiences on upper secondary school students’ intercultural competence by means of an experimental design including an intervention and a control group who are studied longitudinally by means of a pre-test, post-test and delayed post-test. In recent years there has been an increasing effort to evaluate the success of study abroad programs not only in terms of number of participants, but in terms of academic, intercultural and linguistic development. Nevertheless, few studies have employed the experimental designs needed to gauge the impact of study abroad programs and even fewer have included a delayed posttest which may shed light on the sustainability of identified effects. The present study includes a broad range of study abroad programs which differ in terms of certain key characteristics, such as duration, type of accommodation or target language. In this way, it is possible to analyse the effect of different parameters on the student’s intercultural development and, ultimately, to identify key factors for successful programs.
The paper starts by discussing different models of intercultural competence before outlining the model used in this study. This is followed by a presentation of the participants and the key characteristics of their individual study abroad programs. Analyses of covariance are used to examine the intercultural competence of the students in the control group and the intervention group at the time of the post-test and the delayed posttest and to identify key factors that contribute to the explanation of their intercultural competence. The findings indicate that short-term study abroad experiences have a positive influence on young people’s intercultural competence both short-term and longer-term. The most crucial factors for the explanation of the participants’ intercultural competence are their starting conditions, the duration of their stay, the amount of interaction with representatives of the target culture, and the regular use of the target language. The paper finishes with a discussion of implications for program design and of the limitations of the study.
UMA ANÁLISE RETÓRICO-LINGUÍSTICA DO DISCURSO DE PROCLAMAÇÃO DA INDEPENDÊNCIA DA GUINE-BISSAU
Authors: Menezes Léia Cruz de , Danfá Abdulai 
Published: May 2020

A partir da proposta de Menezes (2006, 2011) de estudo das expressões linguísticas modalizadoras deônticas na construção da argumentação em discursos políticos, empreendemos análise retórico-linguística dos modos de atuação das expressões deônticas constitutivas do discurso de proclamação da independência da Guiné-Bissau. Tendo em vista a missão da Universidade da Integração Internacional da Lusofonia Afro-Brasileira (UNILAB), como instituição de ensino internacional, valorizamos o debruçar-se sobre os textos entendidos como marcos históricos dos países que habitam a UNILAB, sob os mais diversos vieses. Entendemos que o estudo deste documento histórico sob o ponto de vista retórico-linguístico auxilia às reflexões acerca do próprio conceito de nação guineense, construído linguisticamente no discurso de proclamação da independência. Analisamos a íntegra do discurso de independência da Guiné-Bissau com base nos parâmetros “alvo” e “fonte” dos valores semânticos deônticos instaurados no discurso, bem como consideramos as partes constitutivas do discurso conforme delineadas pela retórica a fim de compreendermos os efeitos de sentido gerados pelas expressões linguísticas modalizadoras deônticas na construção da argumentação. Constatamos, ao longo de um discurso de sete páginas, a presença de vinte e nove expressões modalizadoras deônticas, localizadas nas partes do discurso destinadas à apresentação de provas e ao epílogo, cuja fonte emana de valores morais como a lealdade e que constroem um conceito de nação independente do julgo colonial que só alcançou e manterá tal configuração se mantiver estrutura monopartidária.
Palavras-chave: Modalidade deôntica. Leiturar e tórico-linguística. Discurso de independência da Guiné-Bissau.
GRAMÁTICA, FUNCIONALISMO E ENSINO DE LÍNGUA
Authors: Ferreira Ediene Pena , Lima Leydiane Sousa 
Published: May 2020

Com o objetivo de apresentar contribuições do paradigma funcionalista para o ensino de fatos gramaticais de língua portuguesa, propomos, neste trabalho, alguns modelos de exercícios com os verbos parecer, acabar, pegar e querer, que possibilitam a reflexão sobre língua portuguesa por meio de usos reais dessa língua. Para que esse objetivo pudesse ser alcançado, discorremos sobre diferentes conceitos de gramática e esclarecemos que compreendemos gramática como regularidade que estrutura o funcionamento da língua e que ensinar gramática é fazer com que o aluno reflita sobre esse funcionamento e compreenda a língua que tem. Esse conceito de gramática nos é apresentado pela abordagem funcionalista de linguagem, eleita para subsidiar nossa discussão. Dentre os temas de interesse do funcionalismo, e que nos deu subsídios para propor as atividades com os verbos, destacamos o paradigma da gramaticalização, compreendido como o processo pelo qual itens lexicais tornam-se gramaticais ou itens e construções já gramaticais tornam-se ainda mais gramaticais. Em outras palavras, gramaticalização é o processo de mudança linguística responsável pelo fazer-se da gramática.
Palavras-chave: funcionalismo, gramática, ensino.
The Effect of Vitamin B3 and Humic Acid on Flowering Traits and Roots Growth of Geranium Pelargonium hortorum L.
Authors: Al-Yasiri Khansaa A.A. , Khudair Thaer Y. , Abdul Albbas Fakhria A. 
Published: May 2020

The current study was conducted during the agricultural season (2019-2020) in the lath house that (covered with Saran and cloth) belonging to the Agricultural Research and Experiment Station at the College of Agriculture, University of Basrah, We sprayed Geranium Pelargonium hortorum L. with three a concentrations (0, 50, 100) mg. L-1 of the organic fertilizer humic acid as well as three concentrations (0, 40, 80) mg. L-1 of vitamin B3 nicotine amide. Then, we investigated the response of Geranium plant for two treatments in n the vegetative ,flowering and root growth after three sprays of each treatment fertilizer humic acid and nicotine amide at (100 and 80) mg. L-1 respectively caused led to the improvement of flowering and root growth indicators, which included (flowering date, the length stalk of inflorescence, percentage of dry matter in inflorescences, length of main roots, number of main roots, percentage of dry matter in the root system). The present study indicated the important role of humic acid and nicotine amide in the amelioration of flowering and root growth of geranium plant.
A Cross-correlation Study of High-energy Neutrinos and Tracers of Large-scale Structure
Authors: Fang Ke , Banerjee Arka , Charles Eric , Omori Yuuki 
Published: May 2020

Abstract
The origin of the bulk of the astrophysical neutrinos detected by the IceCube Observatory remains a mystery. Previous source-finding analyses compared the directions of IceCube events and individual sources in astrophysical catalogs. The source association method is technically challenging when the number of source candidates is much larger than the number of the observed astrophysical neutrinos. We show that in this large source number regime, a two-point cross-correlation analysis of neutrino data and source catalog can instead be used to constrain potential source populations for the high-energy astrophysical neutrinos, and provide spatial evidence for the existence of astrophysical neutrinos. We present an analysis of the cross-correlation of the IceCube 2010–2012 point-source data and a WISE–2MASS galaxy sample. While we find no significant detection of cross-correlation with the publicly available neutrino data set, we show that, when applied to the full IceCube data, which has a longer observation time and higher astrophysical neutrino purity, our method has sufficient statistical power to detect a cross-correlation signal if the neutrino sources trace the large-scale structure of the universe.
Disentangling Dust Components in SN 2010jl: The First 1400 Days
Authors: Bevan A. M. , Krafton K. , Wesson R. , Andrews J. E. , Montiel E. , Niculescu-Duvaz M. , Barlow M. J. , De Looze I. , Clayton G. C. 
Published: May 2020

Abstract
The luminous Type IIn SN 2010jl shows strong signs of interaction between the SN ejecta and dense circumstellar material. Dust may be present in the unshocked ejecta; the cool, dense shell (CDS) between the shocks in the interaction region; or in the circumstellar medium (CSM). We present and model new optical and infrared photometry and spectroscopy of SN 2010jl from 82 to 1367 days since explosion. We evaluate the photometric and spectroscopic evolution using the radiative transfer codes mocassin and damocles, respectively. We propose an interaction scenario and investigate the resulting dust formation scenarios and dust masses. We find that SN 2010jl has been continuously forming dust based on the evolution of its infrared emission and optical spectra. There is evidence for preexisting dust in the CSM as well as new dust formation in the CDS and/or ejecta. We estimate that 0.005–0.01 M
⊙ of predominantly carbon dust grains has formed in SN 2010jl by ∼1400 days post-outburst.
Star–Gas Misalignment in Galaxies. I. The Properties of Galaxies from the Horizon-AGN Simulation and Comparisons to SAMI
Authors: Khim Donghyeon J. , Yi Sukyoung K. , Dubois Yohan , Bryant Julia J. , Pichon Christophe , Croom Scott M. , Bland-Hawthorn Joss , Brough Sarah , Choi Hoseung , Devriendt Julien , Groves Brent , Owers Matt S. , Richards Samuel N. , Sande Jesse van de , Sweet Sarah M. 
Published: May 2020

Abstract
Recent integral field spectroscopy observations have found that about 11% of galaxies show star–gas misalignment. The misalignment possibly results from external effects such as gas accretion, interaction with other objects, and other environmental effects, hence providing clues to these effects. We explore the properties of misaligned galaxies using Horizon-AGN, a large-volume cosmological simulation, and compare the results with those of the Sydney-AAO Multi-object integral field spectrograph (SAMI) Galaxy Survey. Horizon-AGN can match the overall misalignment fraction and reproduces the distribution of misalignment angles found by observations surprisingly closely. The misalignment fraction is found to be highly correlated with galaxy morphology both in observations and in the simulation: early-type galaxies are substantially more frequently misaligned than late-type galaxies. The gas fraction is another important factor associated with misalignment in the sense that misalignment increases with decreasing gas fraction. However, there is a significant discrepancy between the SAMI and Horizon-AGN data in the misalignment fraction for the galaxies in dense (cluster) environments. We discuss possible origins of misalignment and disagreement.
Emission Signatures from Subparsec Binary Supermassive Black Holes. III. Comparison of Models with Observations
Authors: Nguyen Khai , Bogdanović Tamara , Runnoe Jessie C. , Eracleous Michael , Sigurdsson Steinn , Boroson Todd 
Published: May 2020

Abstract
We present a method for comparing the Hβ emission-line profiles of observed supermassive black hole (SBHB) candidates and models of subparsec SBHBs in circumbinary disks. Using the approach based on principal component analysis, we infer the values of the binary parameters for the spectroscopic SBHB candidates and evaluate the parameter degeneracies, representative of the uncertainties intrinsic to such measurements. We find that as a population, the SBHB candidates favor the average value of the semimajor axis corresponding to log(a/M) ≈ 4.20 ± 0.42 and comparable mass ratios, q > 0.5. If the SBHB candidates considered are true binaries, this result would suggest that there is a physical process that allows initially unequal-mass systems to evolve toward comparable mass ratios (e.g., accretion that occurs preferentially onto the smaller of the black holes) or point to some, yet unspecified, selection bias. Our method also indicates that the SBHB candidates equally favor configurations in which the mini-disks are coplanar or misaligned with the binary orbital plane. If confirmed for true SBHBs, this finding would indicate the presence of a physical mechanism that maintains misalignment of the mini-disks down to subparsec binary separations (e.g., precession driven by gravitational torques). The probability distributions of the SBHB parameters inferred for the observed SBHB candidates and our control group of AGNs are statistically indistinguishable, implying that this method can in principle be used to interpret the observed emission-line profiles once a sample of confirmed SBHBs is available but cannot be used as a conclusive test of binarity.
Star Formation Occurs in Dense Gas, but What Does “Dense” Mean?
Authors: Evans Neal J. , Kim Kee-Tae , Wu Jingwen , Chao Zhang , Heyer Mark , Liu Tie , Nguyen-Lu’o’ng Quang , Kauffmann Jens 
Published: May 2020

Abstract
We report results of a project to map HCN and

emission toward a sample of molecular clouds in the inner Galaxy, all containing dense clumps that are actively engaged in star formation. We compare these two molecular line tracers with millimeter continuum emission and extinction, as inferred from 13CO, as tracers of dense gas in molecular clouds. The fraction of the line luminosity from each tracer that comes from the dense gas, as measured by

mag, varies substantially from cloud to cloud. In all cases, a substantial fraction (in most cases, the majority) of the total luminosity arises in gas below the

mag threshold and outside the region of strong millimeter continuum emission. Measurements of

toward other galaxies will likely be dominated by such gas at lower surface densities. Substantial, even dominant, contributions to the total line luminosity can arise in gas with densities typical of the cloud as a whole (n ∼ 100 cm−3). Defining the dense clump from the HCN or

emission itself, similarly to previous studies, leads to a wide range of clump properties, with some being considerably larger and less dense than in previous studies. HCN and

have a similar ability to trace dense gas for the clouds in this sample. For the two clouds with low virial parameters, 13CO is definitely a worse tracer of the dense gas, but for the other four, it is equally good (or bad) at tracing dense gas.
Energetic Neutral Atom Flux from the Inner Heliosheath and Its Connection to Termination Shock Properties
Authors: Shrestha Bishwas L. , Zirnstein Eric J. , Heerikhuisen Jacob 
Published: May 2020

Abstract
We present statistical comparisons between energetic neutral atom (ENA) fluxes obtained using a global simulation of the heliosphere and data collected by the Interstellar Boundary Explorer (IBEX) spacecraft. The simulation of the inner heliosheath (IHS) ENA flux is based on a 3D steady-state heliosphere, while the data are from the IBEX-Hi instrument over the time period 2009–2015. The statistical comparison is performed by calculating the chi-square value between the simulated ENA fluxes and the data for each line of sight in the sky. A comparison with exposure-averaged data for solar minimum and solar maximum conditions is also performed to see the effect of solar wind (SW) properties on the IHS ENA fluxes. The model matches well with the data in the flanks and parts of the nose of the heliosphere, whereas the match is poor in the downwind tail, ribbon, and polar regions. We interpret these results to mean that (i) heliosheath plasma in the polar region consists of advected fast (or slow) SW during the solar minimum (or maximum) condition, and (ii) heliospheric termination shock parameters are likely different over the poles. A poor match at around 30° north and south of the downwind direction is likely due to the existence of a mixture of plasma that comes from fast and slow SW. While our results are consistent with a single heliotail, the shape of the heliosphere continues to be an area of active research, and more data and further modeling are needed to determine its true structure.
Chemical Composition of Bright Stars in the Continuous Viewing Zone of the TESS Space Mission
Authors: Tautvaišienė G. , Mikolaitis Š. , Drazdauskas A. , Stonkutė E. , Minkevičiūtė R. , Kjeldsen H. , Brogaard K. , von Essen C. , Grundahl F. , Pakštienė E. , Bagdonas V. , Vázquez C. Viscasillas 
Published: May 2020

Abstract
Accurate atmospheric parameters and chemical composition of stars play a vital role in characterizing physical parameters of exoplanetary systems and understanding of their formation. A full asteroseismic characterization of a star is also possible if its main atmospheric parameters are known. The NASA Transiting Exoplanet Survey Satellite (TESS) space telescope will play a very important role in searching of exoplanets around bright stars and stellar asteroseismic variability research. We have observed all 302 bright (V < 8 mag) and cooler than F5 spectral class stars in the northern TESS continuous viewing zone with a 1.65 m telescope at the Molėtai Astronomical Observatory of Vilnius University and the high-resolution Vilnius University Echelle Spectrograph. We uniformly determined the main atmospheric parameters, ages, orbital parameters, velocity components, and precise abundances of 24 chemical species (C(C2), N(CN), [O i], Na i, Mg i, Al i, Si i, Si ii, Ca i, Ca ii, Sc i, Sc ii, Ti i, Ti ii, V i, Cr i, Cr ii, Mn i, Fe i, Fe ii, Co i, Ni i, Cu i, and Zn i) for 277 slowly rotating single stars in the field. About 83% of the sample stars exhibit the Mg/Si ratios greater than 1.0 and may potentially harbor rocky planets in their systems.