bluuebunny/crossref_metadata_2025_split huggingface dataset:
“New Normal”: Analisis Penerimaan Menggunakan Balance Score Card
Authors: Maria Florentina Rumba  , Margaretha P.N Rozady  , Theresia W. Mado  
Published: August 2020

Abstrak: Kebiasaan manusia berubah karena adanya wabah COVID-19, hal ini berpengaruh ketika manusia masuk ke dalam fase new normal. New normal diartikan sebagai keadaan yang tidak biasa dilakukan sebelumnya, yang kemudian dijadikan sebagai standar atau kebiasaan baru yang mesti dilakukan manusia untuk dirinya sendiri maupun untuk bersosialisasi dengan orang lain. Kebiasaan baru ini pun menimbulkan pro dan kontra seiring dengan dampak yang timbul. Lembaga pendidikan tinggi merupakan salah satu yang merasakan dampak penerapan new normal. Perkuliahan yang selama ini dilakukan secara online/daring, akan kembali dilakukan secara luring/tatap muka, dengan tetap menerapkan protokol COVID-19 seperti mengenakan masker, menjaga jarak, mengenakan sarung tangan, serta tidak melakukan kontak fisik seperti berjabat tangan. Masalah yang muncul bukan hanya kecemasan orang tua terhadap anak – anaknya, tetapi bagaimana lembaga pendidikan tinggi mengatur segala sumber daya yang dimiliki agar memenuhi standar penerapan new normal. penelitian ini bertujuan untuk mengetahui penerimaan terhadap kondisi normal yang baru menggunakan Perspektif balance score card.
Abstract: Human habits change because of the COVID-19 outbreak, this affects when humans enter the new normal phase. New normal is defined as a condition that is not normally done before, which is then used as a standard or new habits that must be done by humans for themselves or to socialize with others. This new habit also raises the pros and cons along with the impact arising with the new normal. Higher education institutions are the ones who feel the impact of implementing new normal. Lectures that have been conducted online / online will be re-done offline / face to face, while still applying the COVID-19 protocol such as wearing a mask, keeping a distance, wearing gloves, and not making physical contact such as shaking hands. The problem that arises is not only parents' anxiety about their children, but how higher education institutions regulate all available resources to meet new normal implementation standards. This study aims to determine acceptance of new normal conditions using the balance score card Perspective.
Trying To Fit A Square Peg In A Round Hole: Is Community Interpreting Just Too Big For Public Policy? The Canadian Experience A Provocation
Authors: Sasso Angela , Malli Kiran 
Published: August 2020

Abstract: A public policy that obliges the public sector to use the services of a properly trained community interpreter builds a framework for equity, and strengthens the interpreting industry. Public policy does not prescribe a centralized national government budget; instead, each public sector service would define their own budget reinforcing a rigor applied in utilizing interpreters. The current absence of political commitment leaves Community Interpreting vulnerable to shifts, and in turn, jeopardizes access to proper training for interpreters and access to public services for minority language speakers. Lack of public policy on access to health, legal and civil services for the minority language speakers impedes equity, and inhibits the delivery of effective public services. But is Community Interpreting just too big for public policy? This paper will explore:1) Brief evolution of community interpreting in the Canadian context2) Models of public policy3) The relationship between community interpreting and public policy4) Whether public policy is a professional necessityResumen: Una política pública que obliga al sector público a utilizar los servicios de un intérprete social formado adecuadamente construye una estructura para la equidad y fortalece la industria de la interpretación. La política pública no impone un presupuesto de gobierno centralizado. En su lugar, cada servicio del sector público define su propio presupuesto reforzando un rigor aplicado a la utilización de intérpretes. La ausencia actual de compromiso deja a la interpretación social indefensa ante los cambios y, a su vez, pone en peligro el acceso a una formación adecuada para los intérpretes y el acceso a los servicios públicos para los hablantes de lenguas minoritarias. La falta de política pública de acceso a servicios sanitarios, jurídicos y civiles para los hablantes de lenguas minoritarias impide la equidad e inhibe el desarrollo de servicios públicos efectivos. Pero, ¿es la interpretación social demasiado grande para la política pública? Este trabajo hablará de los siguientes temas1) Breve evolución de la interpretación social en el contexto canadiense2) Modelos de política pública3) La relación entre interpretación social y política pública4) Si la política pública constituye una necesidad profesional
Diseño de Nuevos Materiales para la Formación de Intérpretes en el Ámbito Sanitario (Especialidad: Español - Chino)
Authors: Wang Xi 
Published: August 2020

Resumen: En los últimos años, han llegado abundantes extranjeros a España importando sus lenguas y culturas, de los cuales muchos son de origen chino. Teniendo en cuenta las grandes distancias lingüísticas y culturales que existen entre dicha población y la población mayoritaria en el país de acogida, surgen problemas específicos cuando acuden al servicio sanitario. Ante esta situación actual la formación de intérpretes profesionales en el ámbito sanitario es un tema urgente. Los materiales para la formación en interpretación en el ámbito sanitario se caracterizan, hoy en día, por su escasez en comparación con otros ámbitos profesionales y, más aún, en la combinación lingüística español-chino. El uso de materiales adecuados puede promover el desarrollo de la formación y, en consecuencia, la profesionalización de la interpretación en el ámbito sanitario. Para llevar a cabo el trabajo, se han analizado los materiales existentes y descrito las competencias requeridas por la profesión, con el fin de identificar los aspectos más relevantes de la formación en la interpretación en el ámbito sanitario, en general, como los de la combinación lingüística y cultural, en particular, proponiendo criterios que se pueden aplicar en el diseño de nuevos materiales.Abstract: In recent years, the number of immigrants in Spain has increased considerably, particularly those who come from China. Due to the differences and distance between Spanish and Chinese languages and cultures, serious access problems arise when Chinese migrants want to use the Spanish healthcare system. In this case, the importance of training professional medical interpreters is particularly important. Compared with other professions, materials available to medical interpreters are scarce, even more regarding the Spanish-Chinese language combination. Suitable materials contribute to promote the development of quality training, so as to achieve the purpose of advancing the process of professionalisation. An analysis about the existing materials has been performed and the competences students need to achieve have been described. The ultimate goal of this analysis is to provide criteria for the design of training materials for Spanish-Chinese medical interpreters.
Análisis de los Errores de Traducción de los Alumnos Tailandeses en la Traducción del Texto con Elementos Culturales (Español-Tailandés)
Authors: Sirinit Thanita 
Published: August 2020

Resumen: En este artículo presentamos un análisis de los errores de traducción cometidos por los alumnos tailandeses en la traducción del texto con elementos culturales del español al tailandés. Los datos obtenidos han permitido identificar los problemas y dificultades persistentes de los alumnos a la hora de traducir, y han confirmado la necesidad de integrar objetivos de aprendizaje específicos para desarrollar la competencia traductora en los alumnos. Abstract: The aim this paper is to present an analysis of the translation errors committed by the Thai students in the translation of the text with cultural elements from Spanish to Thai. The data obtained have allowed us to identify the persistent problems and difficulties of the students when translating, and have confirmed the need to integrate specific learning objectives in order to develop the translator competence in the students.
Public Service Interpreting and Cultural Mediation in the Region of Valencia: Strengths, Weaknesses and Recommendations for Improvement in the Healthcare Setting
Authors: Sánchez Pérez Marta Isabel 
Published: August 2020

Abstract: This article aims at approaching the state of the art of Cultural Mediation (CM) and Public Service Interpreting (PSI) in healthcare settings in the Valencian Region by analysing the strengths and weaknesses of the current issues regulating PSI and CM focusing on its legislation, accreditation criteria and implementation of services and suggesting measures that have proven effective in other territories with a larger tradition of PSI and CM services in order to advance towards a health system that ensures equal access and medical care to everyone regardless of the patient’s culture of origin or language.Resumen: Este artículo ofrece una panorámica del estado de la cuestión de la Mediación Intercultural (MI) y la Interpretación en los Servicios Públicos (ISP) en el ámbito sanitario de la Comunitat Valenciana analizando sus fortalezas y debilidades, y centrándose en la legislación, criterios de acreditación e implementación de servicios linguisticos y culturales. Asímismo ofrece una serie de recomendaciones de mejora para contribuir a avanzar hacia un sistema sanitario que garantice un acceso y una atención sanitaria igualitarios independientemente del origen cultural del paciente y su lengua.
Interpreters Banks as a Response To a Multilingual Europe's Needs
Authors: Burdeus-Domingo Noelia 
Published: August 2020

Abstract: Globalisation urges governments to address equality in access to public services. Even though Public Service Interpreting (PSI) helps allophones to overcome the breach in communication, such services need a solid, organised structure to effectively respond to the current linguistic needs. This article presents the results of a comparative study of the healthcare interpreting services provided in Barcelona and Montreal which, by applying an indirect method of observation (interviews) to examine the aforementioned services, describes the existing PSI structures and organisations as narrated by their managers. Our conclusions draw attention to certain aspects of Barcelona’s interpreting services which, should they be modified, could be beneficial. Finally, the interpreters bank model settled in Montreal (and throughout Quebec) is suggested as a role model for Barcelona, that could contribute to structuring PSI services in Europe.Resumen: La globalización insta a los gobiernos a abordar el problema de la igualdad de acceso a los servicios públicos. Si bien los servicios de Interpretación en los Servicios Públicos (ISP) ayudan a los alófonos a vencer barreras comunicativas, estos necesitan una estructura sólida organizada para responder con eficacia a las necesidades lingüísticas actuales. Este artículo presenta los resultados de un estudio comparativo de los servicios de interpretación médica de Barcelona y Montreal que, mediante la aplicación de un método de observación indirecto (entrevistas), examina los servicios mencionados, describiendo las estructuras y organizaciones existentes tal y como las definen sus propios gestores. Las conclusiones se centran en aspectos de los servicios de interpretación de Barcelona que convendría modificar y sugieren el modelo de banco de intérpretes instaurado en la provincia de Quebec como un ejemplo a seguir en Barcelona, que podría contribuir a la estructuración de servicios de ISP en Europa.
Rekayasa Perangkat Lunak Pengenal Binatang Menggunakan Metode CART
Authors: Shandi Yusup Jauhari 
Published: August 2020

Semakin berkembangnya teknologi informasi, menyebabkan kebutuhan akan informasi sudah tidak lagi membutuhkan alat peraga. Berbagai bentuk informasi terhadap objek atau benda yang ditemukan ingin langsung didapatkan, akan tetapi masalah seringkali muncul karena pengenalan suatu objek yang dikenali terbatas.
Artikel ini memaparkan desain sistem untuk menghasilkan informasi tanpa alat peraga secara fisik, dan secara khusus bertujuan mempermudah seseorang untuk mengenal suatu binatang yang ditemukan secara langsung atau tiba-tiba. Pemilihan binatang sebagai objek yang dikenal, karena memiliki bentuk objek yang tergolong konsisten sehingga dapat meningkatkan nilai keakuratan dalam melakukan penelitian.
Pemilihan Metode Classification And Regression Tree (CART) yang digunakan, karena memiliki performa yang akurat dalam pengambilan keputusan. Adapun pemilihan Clarifai API sebagai sistem pendukung perangkat lunak ini, karena memiliki kemampuan baik dalam computer vision untuk mengidentifikasi dan menganalisis suatu objek melalui gambar atau video.
Photospheric Emission in Gamma-Ray Bursts. I. Variability
Authors: Wang Kai , Lin Da-Bin , Wang Yun , Jiang Lu-Yao , Du Shen-Shi , Li Xiao-Yan , Ren Jia , Wang Xiang-Gao , Liang En-Wei 
Published: August 2020

Abstract
It is generally believed that the variability of photospheric emission in gamma-ray bursts (GRBs) traces that of the jet power. This work further investigates the variability of photospheric emission in a variable jet. By setting a constant η (dimensionless entropy of the jet), we find that the light curve of the photospheric emission shows a “tracking” pattern on the time profile of jet power. However, the relative variability is significantly low in the photospheric emission compared with that in the jet power. If the η is genetic variable, the variability of the photospheric emission is not only limited by the jet power but also affected by η strongly. It becomes complex and is generally different from that of the jet power. Moreover, the opposite phase may stand in the variabilities of the photospheric emission at different photon energies. We also find that the relative variability does not remain constant over the photon energies with an obvious reduction at a certain energy. This is consistent with the analysis of GRB 090902B in which an appreciable thermal component has been detected in a wide energy range. For several other GRBs coupling with the thermal component, we conservatively evaluate the variability of the thermal and nonthermal emission, respectively. Our results show that the relative variability of the thermal emission is likely comparable to that of the nonthermal emission for these bursts. In addition, the analysis of GRB 120323A reveals that the variability of the photospheric emission may be of the opposite phase from that of the nonthermal emission.
Differential Rotation of the Halo Traced by K-giant Stars
Authors: Tian Hao , Liu Chao , Wang Yougang , Xu Yan , Yang Chengqun , Zhang Bo , Xue Xiang-Xiang 
Published: August 2020

Abstract
We use K-giant stars selected from the LAMOST DR5 to study the variation of the rotational velocity of the Galactic halo at different space positions. Modeling the rotational velocity distribution with both the halo and disk components, we find that the rotational velocity of the halo population decreases almost linearly with increasing vertical distance to the Galactic disk plane, Z, at fixed galactocentric radius, R. The samples are separated into two parts with

and

. We derive that the decreasing rates along Z for the two subsamples are −3.07 ± 0.63 and −1.89 ± 0.37 km s−1 kpc−1, respectively. Comparing with the TNG simulations, we suggest that this trend is caused by the interaction between the disk and halo. The results from the simulations show that only an oblate halo can provide a decreasing rotational velocity with increasing Z. This indicates that the Galactic halo is oblate with galactocentric radius

. On the other hand, the flaring of the disk component (mainly the thick disk) is clearly traced by this study; with R between 12 and 20 kpc, the disk can vertically extend to

above the disk plane. What is more interesting is that we find the Gaia–Enceladus–Sausage component has a significant contribution only in the halo with

, i.e., a fraction of 23%–47%, while in the outer subsample, the contribution is too low to be well constrained.
On the Magnetospheric Origin of Repeating Fast Radio Bursts
Authors: Wang Wei-Yang , Xu Renxin , Chen Xuelei 
Published: August 2020

Abstract
A bright radio burst was newly discovered in SGR 1935+2154, which exhibits some fast radio burst (FRB)-like temporal and frequency properties, suggesting a neutron star (NS)/magnetar magnetospheric origin of FRBs. We propose an explanation of the temporal and frequency properties of sub-pulses of repeating FRBs based on the generic geometry within the framework of charged-bunching coherent curvature radiation in the magnetosphere. The sub-pulses in a radio burst come from bunches of charged particles moving along different magnetic field lines. Their radiation beams sweep across the line of sight at different times, and those radiating at the more curved part tend to be seen earlier and at higher frequency. However, by considering bunches generated at slightly different times, we find there is also a small probability that the emission from the less curved part can be seen earlier. We simulate the time–frequency structures by deriving various forms of the electric acceleration field in the magnetosphere. This structure of sub-pulses is a natural consequence of coherent curvature radiation from an NS/magnetar magnetosphere with suddenly and violently triggered sparks. We apply this model to explain the time–frequency structure within a specific dipolar configuration by invoking the transient pulsar-like sparking from the inner gap of a slowly rotating NS, and we have also applied it to more generic configurations.
Massive Galaxies Impede Massive Outflows
Authors: Tanner Ryan 
Published: August 2020

Abstract
A set of 66 3D hydrodynamical simulations explores how galactic stellar mass affects three-phase, starburst-driven outflows. Simulated velocities are compared to two basic analytic models: with and without a gravitational potential. For stellar mass <1010
M
⊙, simulated velocities match those of both analytical models and are unaffected by the potential; above they reduce significantly as expected from the analytic model with gravity. Gravity also affects total outflow mass and each of the three phases differently. Outflow masses in the hot, warm, and cold phases each scale with stellar mass as

−0.25, −0.97, and −1.70, respectively. Thus, the commonly used Chevalier & Clegg analytic model should be modified to include gravity when applied to higher-mass galaxies. In particular, using M82 as the canonical galaxy to interpret hydrodynamical simulations of starburst-driven outflows from higher-mass galaxies will underestimate the retarding effect of gravity. Using the analytic model of Johnson & Axford with realistic thermalization efficiency and mass loading, I find that only galaxy masses ≲1011.5
M
⊙ can outflow.
GRB 170817A as a Refreshed Shock Afterglow Viewed Off-axis
Authors: Lamb Gavin P. , Levan Andrew J. , Tanvir Nial R. 
Published: August 2020

Abstract
Energy injection into the external shock system that generates the afterglow to a gamma-ray burst (GRB) can result in a rebrightening of the emission. Here we investigate the off-axis view of a rebrightened refreshed shock afterglow. We find that the afterglow light curve, when viewed from outside of the jet opening angle, could be characterized by a slow rise, or long plateau, with a maximum flux determined by the total system energy. Using the broadband afterglow data for GRB 170817A, associated with the gravitational-wave-detected binary neutron star merger GW170817, we show that a refreshed shock model with a simple top-hat jet can reproduce the observed afterglow features. We consider two refreshed shock models: a single episode of energy injection, and an episode of continuous energy injection. The best-fit model parameters give a jet opening angle for our first and second models, respectively, of θ

j
= 5.°

and 6.°

, an inclination to the line of sight ι = 16.°

and 17.°

, an initial on-axis isotropic equivalent kinetic energy

and

erg, and a total/final, on-axis isotropic equivalent refreshed shock energy

and

erg. The first model fitting prefers an initial bulk Lorentz factor Γ0,1 < 60, with a comparatively low central value of Γ0,1 = 19.5, indicating that, in this case, the on-axis jet could have been a “failed GRB.” Alternatively, our second model is consistent with a bright GRB for an on-axis observer, with

. Due to the low Lorentz factor and/or the jet opening angles at θ

j
∼ ι/3, both models are unable to reproduce the γ-ray emission observed in GRB 170817A, which would therefore require an alternative explanation such as cocoon shock breakout.
Pulsar Candidate Sifting Using Multi-input Convolution Neural Networks
Authors: Lin Haitao , Li Xiangru , Zeng Qingguo 
Published: August 2020

Abstract
Pulsar candidate sifting is an essential process for discovering new pulsars. It aims to search for the most promising pulsar candidates from an all-sky survey, such as the High Time Resolution Universe (HTRU), Green Bank Northern Celestial Cap (GBNCC), Five-hundred-meter Aperture Spherical Radio Telescope, etc. Recently, machine learning (ML) has become a hot topic in investigations of pulsar candidate sifting. However, one typical challenge in ML for pulsar candidate sifting comes from the learning difficulty arising from the high class imbalance between the observed numbers of pulsars and non-pulsars. Therefore, this work proposes a novel framework for candidate sifting, named Multi-input Convolutional Neural Networks (MICNN). MICNN is an architecture of deep learning with four diagnostic plots of a pulsar candidate as its inputs. To train our MICNN on a highly class-imbalanced data set, a novel image augmentation technique is proposed, as well as a three-stage training strategy. Experiments on observations from HTRU and GBNCC show the effectiveness and robustness of these proposed techniques. In the experiments on HTRU, our MICNN model achieves a recall rate of 0.962 and a precision rate of 0.967 even in a highly class-imbalanced test data set.
The Case for an Early Solar Binary Companion
Authors: Siraj Amir , Loeb Abraham 
Published: August 2020

Abstract
We show that an equal-mass, temporary binary companion to the Sun in the solar birth cluster at a separation of ∼103 au would have increased the likelihood of forming the observed population of outer Oort Cloud objects and of capturing Planet Nine. In particular, the discovery of a captured origin for Planet Nine would favor our binary model by an order of magnitude relative to a lone stellar history. Our model predicts an overabundance of dwarf planets, discoverable by Legacy Survey of Space and Time, with similar orbits to Planet Nine, which would result from capture by the stellar binary.