bluuebunny/crossref_metadata_2025_split huggingface dataset:
Prototipe Cscm (Coin Sorting And Counting Machine) Berbasis Arduino Uno R3 Studi Kasus : Koperasi Melati
Authors: Suheri Agus , Setiawan Widi Juniarti 
Published: August 2020

Arduino merupakan perangkat keras sekaligus perangkat lunak yang memungkinkan siapa saja melakukan pembuatan prototipe suatu rangkaian elektronika yang berbasis mikrokontroler dengan mudah dan cepat. Arduino Integrated Development Equipment (Arduino IDE) adalah perangkat lunak yang digunakan untuk mengembangkan program dan memungkinkan program diunggah ke papan Arduino. Papan arduino merupakan papan elektronis yang berisi mikrokontroler berbasis ATMega, sedangkan mikrokontroler adalah sebuah keping (integrated circuit) yang mengandung prosesor alias sang pemroses dan sekaligus memori yang berguna untuk menyimpan data. Transaksi yang menggunakan uang koin biasanya membutuhkan waktu yang lebih lama dan tingkat kerumitan yang lebih tinggi dibandingkan dengan menggunakan uang kertas biasa. Sebab lebih banyaknya elemen yang dihitung. Bahkan sering sekali terjadi kesalahan dalam penghitungan dan penyortiran uang koin tersebut. Dengan memanfaatkan teknologi mikrokontroler, yaitu menggabungkan Arduino dengan Sensor Infrared, Motor Servo, Motor DC, LCD 20x4, I2C, dan Keypad 4x4 nantinya akan menjadi CSCM (Coin Sorting and Counting Machine) yang dapat menghitung dan menyortir uang koin secara otomatis. Hasil penghitungan dan penyortiran uang koin akan ditampilkan pada LCD.Pada penelitian ini diharapkan dapat membantu transaksi menggunakan uang koin menjadi lebih cepat dan mudah sehingga waktu dan tenaga yang digunakan lebih sedikit. Serta mengurangi tingkat kesalahan dalam penghitungan dan penyortiran uang koin.
HUBUNGAN ANTARA PENERIMAAN DIRI DAN DUKUNGAN SOSIAL ORANG TUA ANAK AUTIS DENGAN INTERAKSI SOSIAL ANAK AUTIS
Authors: Suyanti Suyanti , Faizah Kurniyatul 
Published: August 2020

This study aims to determine how much influence social acceptance and support for parents of autistic children with social interaction of children with autism. The population is 30 parents of autistic children and the closestpeople who attend in PAUD Inklusi Anggrek MandiriSitubondo and the sample is the whole of the population of some 30 people. This study is correlational; the subject is determined by purposive sampling technique. Results of the study showed that the regression analysis coefficient on F = 17.839, p = 0.000 (p <0.05) so that there is a significant relationship between self-acceptance and social support for parents of autistic children with social l interactionautistic children is received. Partially there is a significant correlation between self-acceptance with social interaction shown by prices at t = 5.018, p = 0.000, so the hypothesis is accepted. In parsal also shown at t = 1.613 p = 0.118 (p> 0.05), so the research hypothesis that says there is a relationship of social support with social interaction rejected. So overall derived price Sguare R = 0.569 which shows variable acceptance of self and social support contributed 56.9% effective this further strengthensacceptance your self parents with autistic children and social support autistic children associated with autistic children social interaction. So H0 rejected, which means acceptance of self and relationship betweensocial parents support correlated with sociall interactionautistic children.
MEMBENTUK BUDAYA ORGANISASI DI LINGKUNGAN LEMBAGA PENDIDIKAN ISLAM
Authors: Arfandi Arfandi , Iffah Ukhtul 
Published: August 2020

Organizational culture is the shared values and beliefs that underlying organizational identity. That is an invisible social force that can move people in organization to carry out work activities. Persons in organization learns the culture unconsciously that applies within an organization. Culture is also the main determinant of someone’s wishes and behaviours. Human behaviors are usually influenced by the surrounding environment, so that the values, perceptions, preferences, and behaviors between persons who live in a certain environment can be different from other peoples in other environments. Culture encompasses all knowledges, beliefs, skills, arts, morals, laws, customs, and human habits, as members of society. Culture that consists of ideas, attitudes, values and habits of individuals are learned from their lives in the social environment.
I Illness Belief dan Illness Representation pada Pasien Diabetes Mellitus: Study Phenomenologhy
Authors: Arif Nisak 
Published: August 2020

Latar Belakang: Diabetes Mellitus (DM) merupakan salah satu penyakit kronis yang membutuhkan strategi untuk dalam pengelolaan penyakitnya. Berbagai pengalaman dan pengetahuan pasien selama sakit dapat membentuk illness belief dan illness representation yang berbeda-beda pada pasien. Kesesuaian illness belief dan illness representation dapat menjadi salah satu kunci keberhasilan dalam pengelolaan penyakit ini. Tujuan: Studi ini merupakan studi pendahuluan yang bertujuan untuk mengetahui illness belief dan illness representation pada pasien DM. Metode: Metode dalam studi pendahuluan ini menggunakan design kualitatif dengan pendekatan phenomenology yang melibatkan sepuluh perawat dan sepuluh pasien di di Rumah Sakit Umum Daerah Dr. Soeroto Ngawi dan Rumah Sakit Widodo Ngawi. Pengambilan data dilakukan dengan indepth interview semistructure selanjutnya dianalisa menggunakan content analysis. Hasil: Tiga tema telah dididapatkan dalam studi ini, yaitu persepsi pasien tentang illness belief dan illness representation vs kelalaian pasien, persepsi perawat tentang illness belief dan illness representation vs tindakan mandiri perawat, serta dampak positif illness belief dan illness representation. Kesimpulan: Illness belief dan illness representation yang dimiliki oleh pasien DM memiliki pengaruh besar pasien DM. Tindakan perawat terkait dengan illness belief dan illness representation perlu ditingkatkan lagi sehingga dapat meningkatkan kesejahteraan pasien.

Keywords :
Illness belief, illness representation, diabetes mellitus
HUBUNGAN LAMA PEMAKAIAN KB SUNTIK 3 BULAN DEPO MEDROSIK PROGESTERON ASETAT (DMPA) DENGAN PENINGKATAN BERAT BADAN
Authors: Kunang Analia 
Published: August 2020

Kontrasepsi suntik Depo Medroksi Progesteron Asetat (DMPA) merupakan jenis kontrasepsi keluarga berencana yang banyak digunakan dan efektif dalam menekan jumlah angka kelahiran. Salah satu dampak penggunaan KB suntik DMPA adalah peningkatan berat badan. Penelitian ini bertujuan untuk mengetahui hubungan lama pemakaian KB suntik 3 bulan Depo Medrosik Progesteron Asetat (DMPA) dengan peningkatan berat badan di BPM Selva Tiara Kec Bulok Kab. Tanggamus. Metode : penelitian ini menggunakan pendekatan Cross Sectional. Populasi dalam penelitian ini adalah seluruh Ibu yang memakai KB suntik 3 bulan DMPA di BPM Selva sebanyak 42 responden. Tekhnik sampling yang digunakan adalah Total sampling. Hasil Penelitian : analisa univariat diketahui responden dengan lama penggunaan >4 Tahun yaitu sebanyak 17 responden (40,5%) dan responden yang mengalami peningkatan badan yaitu sebanyak 31 responden (73,8%). Ada hubungan antara lama pemakaian KB suntik 3 bulan Depo Medrosik Progesteron Asetat (DMPA) dengan peningkatan berat badan di BPM Selva Tiara Kec Bulok Kab. Tanggamus Tahun 2019 dengan p-value sebesar 0.011. Bagi pengguna kontrasepsi suntik DMPA untuk dapat melakukan pola hidup sehat seperti mengkonsumsi makanan sehat dan berolahraga sebagai upaya pencegahan peningkatan berat badan akibat efek samping kontrasepsi hormonal DMPA
РЕАЛІЗАЦІЯ НАУКОВО-ПЕДАГОГІЧНОЇ ФУНКЦІЇ ВИКЛАДАЧА В КОНТЕКСТІ СТРАТЕГІЇ РОЗВИТКУ ВИЩОЇ ОСВІТИ В УКРАЇНІ
Authors: ЛУГОВИЙ Володимир Іларіонович 
Published: August 2020

З огляду на дуальну «науково-педагогічну» функцію університетського викладача обґрунтовано умови її ефективної реалізації в конкурентоспроможному закладі вищої освіти. Серед цих умов — зниження навчального навантаження, підвищення конкурентоспроможності заробітної плати, необхідна і достатня навчальна, дослідницька, інформаційна інфраструктура закладу, посилення конкурсності відбору викладачів. У контексті стабілізації обсягів видатків на систему вищої освіти на рівні 1,2 % ВВП для створення зазначених умов насамперед потрібна оптимізація мережі закладів вищої освіти шляхом їх укрупнення, концентрації ресурсів, розвитку фінансової автономії для мотивації ефективної діяльності викладачів.
Audience Concern of Eco-Fashion by Fashion Revolution Indonesia Through Marketing Communication in Jakarta
Authors: Tan Kevin 
Published: August 2020

After Rana Plaza tragedy, Fashion Revolution has came to Indonesia on 2016, deliver the objective is to unite people work together to change the perspective about the clothes are sourced, produced and consumed. However, based on Fashion Revolution Indonesia statement, it is challenging to evoke consumer’s concern about eco-fashion.
The concern problem of sustainable fashion remains until now. Simply, the consumers don’t care, trying to deny, blaming others and refuse to take responsibility. Fashion Revolution Indonesia needs to figure out another way to communicate with audience who originally doesn’t concern about eco-fashion in the first place. The goal of this research is to analyze Fashion Revolution Indonesia marketing communication implementation towards audience concern about eco-fashion.
Using qualitative approach, which the researcher gathers the data. Social marketing is more difficult rather than commercial marketing, which prestige, exclusivity, design options, quality, and pricing are some of the commercial marketing elements cater what consumer likes. In the other hand, social marketing is focused on making attitude change for social cause and give up the addictive behavior.
By conclusion, Fashion Revolution Indonesia must understand how the ecosystem works to do the marketing communication in social context from internal and external, because social change is a complex issue. From the way they communicate, the message, media to promote, the organization, campaigners and partners themselves, every single one of the elements are important to lead an impact of attitude change to the audience.

Keywords: Eco-Fashion, Fast Fashion, Concern, Marketing Communication, Fashion Revolution
Perfil competitivo de los tenderos de Tunja, y las grandes superficies del retail
Authors: Martínez Ricardo Santos , Rojas Rodríguez Carlos Alberto 
Published: August 2020

Este artículo tiene como objetivo caracterizar el perfil competitivo de los tenderos de la ciudad de Tunja, cómo ha sido su evolución y su prospectiva competitiva, frente al fenómeno creciente de las cadenas de supermercados de mayoristas de retail. El cuerpo devela, por una parte, la situación actual del tendero de la ciudad de Tunja, realizando una radiografía ajustada a su quehacer gerencial, en procesos administrativos, contables y tributarios; para esto, se escogió una muestra aleatoria de 220 tenderos, a quienes se les aplicó una encuesta estratificada; en segunda instancia, se analizaron las respuestas, comparando los resultados frente a los estudios de fuentes secundarias correspondientes a las grandes superficies. Los resultados del análisis indican, en primera instancia, que los tenderos de la ciudad de Tunja en materia gerencial no hace uso de las teorías y herramientas administrativas para la dirección de sus negocios, su gestión es en ocasiones empírica, heredada y copiada del comercio de principios del siglo XX. Se concluye que el comercio dentro de las nuevas formas implementadas por el denominado “libre comercio” es altamente competitivo, que el desarrollo del retail con las nuevas tecnologías de la información y la comunicación, ha tomado rumbos de desarrollo descomunal frente a las organizaciones que no las tienen o practican.
Faraday Dispersion Function of Disk Galaxies with Axisymmetric Global Magnetic Fields. I.
Authors: Eguchi Haruya , Suzuki Masaki , Miyashita Yoshimitsu , Ideguchi Shinsuke , Takahashi Keitaro 
Published: August 2020

Abstract
Faraday tomography is a novel method to probe the three-dimensional structure of magnetic fields of polarized radio sources. In this paper, we investigate the intrinsic Faraday dispersion function (FDF) of disk galaxies extending a simple analytic model of galactic magnetic fields developed in Ideguchi et al. The model consists of axisymmetric coherent fields and turbulent fields, and we consider the effects of inclination, the relative amplitude of coherent and turbulent magnetic fields, and the pitch angle of coherent fields. Our simple model makes it easy to obtain a physical interpretation of FDFs and helps us understand observational results. We find that FDFs generally have two peaks when galaxies are observed with nonzero inclination and the gap between the two peaks, their relative heights, and their widths are dependent on the model parameters. In particular, the gap is strongly dependent on the inclination angle and typically varies by a factor of two when we consider the inclination of 10°–60°, while the relative height varies by less than 20%. These findings provide us with the important lesson that the presence of two peaks in intrinsic FDFs does not necessarily imply the presence of two separate radio sources within a beam and they allow us to estimate the galactic parameters.
The Origin of a Distributed Stellar Population in the Star-forming Region W4
Authors: Lim Beomdu , Hong Jongsuk , Yun Hyeong-Sik , Hwang Narae , Kim Jinyoung S. , Lee Jeong-Eun , Park Byeong-Gon , Park Sunkyung 
Published: August 2020

Abstract
Stellar kinematics provides the key to understanding the formation process and dynamical evolution of stellar systems. Here, we present a kinematic study of the massive star-forming region (SFR) W4 in the Cassiopeia OB6 association using the Gaia Data Release 2 and high-resolution optical spectra. This SFR is composed of a core cluster (IC 1805) and a stellar population distributed over 20 pc, which is a typical structural feature found in many OB associations. According to a classical model, this structural feature can be understood in the context of the dynamical evolution of a star cluster. The core-extended structure exhibits internally different kinematic properties. Stars in the core have an almost isotropic motion, and they appear to reach virial equilibrium given their velocity dispersion (0.9 ± 0.3 km s−1) comparable to that in a virial state (∼0.8 km s−1). On the other hand, the distributed population shows a clear pattern of radial expansion. From the N-body simulation for the dynamical evolution of a model cluster in subvirial state, we reproduce the observed structure and kinematics of stars. This model cluster experiences collapse for the first 2 Myr. Some members begin to radially escape from the cluster after the initial collapse, eventually forming a distributed population. The internal structure and kinematics of the model cluster appear similar to those of W4. Our results support the idea that the stellar population distributed over 20 pc in W4 originate from the dynamical evolution of IC 1805.
Updated Spin and Orbital Parameters and Energy Dependent Pulse Behaviors of the Accreting Millisecond X-Ray Pulsar IGR J17591–2342
Authors: Tse Kaho , Chou Yi , Hsieh Hung-En 
Published: August 2020

Abstract
We present our work in updating the spin and orbital parameters for the newly discovered accreting millisecond X-ray pulsar (AMXP) IGR J17591–2342 through pulsar timing and analyzing its energy dependent pulse behaviors. The data being analyzed were collected by Neutron Star Interior Composition ExploreR, which observed this AMXP from 2018 August to October. Using the pulse arrival time delay technique, more accurate spin and orbital parameters were evaluated. From the measured spin frequency derivative, it is estimated that the magnetic field of the neutron star in IGR J17591–2342 is approximately 4 × 108 G. Precise pulse profiles can be made using the updated spin and orbital parameters. The soft phase lag phenomenon that is usually seen in other AMXPs is also observed from ∼4 to 12 keV with a value of 0.06 cycles (1.14 μs). Additionally, the pulsed fractional amplitude increases from 1 to ∼5 keV and then decreases for higher energy bands. We found that these phenomena, as well as the energy spectrum, can be explained by the two-component model with a relatively strong blackbody component and an additional unpulsed disk blackbody component.
Giant Micropulse Emission in the Vela Pulsar at the C Band
Authors: Chen J. L. , Wen Z. G. , Hao L. F. , Yuan J. P. , Li J. , Wang H. G. , Yan W. M. , Lee K. J. , Wang N. , Xu Y. H. , Li Z. X. , Huang Y. X. , Yuen R. , Mijit M. 
Published: August 2020

Abstract
We present here the analysis of giant micropulses from the Vela pulsar. A total of 4187 giant micropulses with peak flux density >2.5 Jy were detected during almost 4 hr of observations carried out with the Yunnan 40 m radio telescope at 6800 MHz. Nine of the giant micropulses arrived approximately 3–4 ms earlier than the peak of average pulse profile, longer than that at lower frequencies. The remaining giant micropulses were clustered into three distributions that correspond to three main emission regions, including four giant micropulses occurring on the trailing edge of the averaged profile. We find that the peak flux density distribution follows a power law with index α ≈ −4. Furthermore, a certain amount of memory is present from the giant micropulse waiting time distribution. Possible emission mechanisms are discussed.
The MOSDEF Survey: The Variation of the Dust Attenuation Curve with Metallicity
Authors: Shivaei Irene , Reddy Naveen , Rieke George , Shapley Alice , Kriek Mariska , Battisti Andrew , Mobasher Bahram , Sanders Ryan , Fetherolf Tara , Azadi Mojegan , Coil Alison L. , Freeman William R. , de Groot Laura , Leung Gene , Price Sedona H. , Siana Brian , Zick Tom 
Published: August 2020

Abstract
We derive a UV-optical stellar dust attenuation curve of galaxies at z = 1.4–2.6 as a function of gas-phase metallicity. We use a sample of 218 star-forming galaxies, excluding those with very young or heavily obscured star formation, from the MOSFIRE Deep Evolution Field survey with Hα, Hβ, and [N ii]λ 6585 spectroscopic measurements. We constrain the shape of the attenuation curve by comparing the average flux densities of galaxies sorted into bins of dust obscuration using Balmer decrements, i.e., Hα-to-Hβ luminosities. The average attenuation curve for the high-metallicity sample (

, corresponding to

) has a shallow slope, identical to that of the Calzetti local starburst curve, and a significant UV 2175 Å extinction bump that is ∼0.5× the strength of the Milky Way bump. On the other hand, the average attenuation curve of the low-metallicity sample (

) has a steeper slope similar to that of the SMC curve, only consistent with the Calzetti slope at the 3σ level. The UV bump is not detected in the low-metallicity curve, indicating the relative lack of the small dust grains causing the bump at low metallicities. Furthermore, we find that on average the nebular reddening (E(B − V)) is a factor of 2 times larger than that of the stellar continuum for galaxies with low metallicities, while the nebular and stellar reddening are similar for galaxies with higher metallicities. The latter is likely due to a high surface density of dusty clouds embedding the star-forming regions but also reddening the continuum in the high-metallicity galaxies.
The Contour Method: a New Approach to Finding Modes of Nonadiabatic Stellar Pulsations
Authors: Goldstein J. , Townsend R. H. D. 
Published: August 2020

Abstract
The contour method is a new approach to calculating the nonadiabatic pulsation frequencies of stars. These frequencies can be found by solving for the complex roots of a characteristic equation constructed from the linear nonadiabatic stellar pulsation equations. A complex-root solver requires an initial trial frequency for each nonadiabatic root. A standard method for obtaining initial trial frequencies is to use a star’s adiabatic pulsation frequencies, but this method can fail to converge to nonadiabatic roots, especially as the growth and/or damping rate of the pulsations becomes large. The contour method provides an alternative way to obtain initial trial frequencies that robustly converges to nonadiabatic roots, even for stellar models with extremely nonadiabatic pulsations and thus high growth/damping rates. We describe the contour method implemented in the gyre stellar pulsation code and use it to calculate the nonadiabatic pulsation frequencies of

and

β Cephei star models, and of a

extreme helium star model.
AGN Feedback and Star Formation of Quasar Host Galaxies: Insights from the Molecular Gas
Authors: Shangguan Jinyi , Ho Luis C. , Bauer Franz E. , Wang Ran , Treister Ezequiel 
Published: August 2020

Abstract
Molecular gas serves as a key probe of the complex interplay between black hole accretion and star formation in the host galaxies of active galactic nuclei (AGNs). We use CO(2–1) observations from a new Atacama Large Millimeter/submillimeter Array survey, in conjunction with literature measurements, to investigate the molecular gas properties of a representative sample of 40 z < 0.3 Palomar–Green quasars, the largest and most sensitive study of molecular gas emission to date for nearby quasars. We find that the AGN luminosity correlates with both the CO luminosity and black hole mass, suggesting that AGN activity is loosely coupled to the cold gas reservoir of the host. The observed strong correlation between host galaxy total infrared luminosity and AGN luminosity arises from their common dependence on the molecular gas. We argue that the total infrared luminosity, at least for low-redshift quasars, can be used to derive reliable star formation rates for the host galaxy. The host galaxies of low-redshift quasars have a molecular gas content similar to that of star-forming galaxies of comparable stellar mass. Moreover, they share similar gas kinematics, as evidenced by their CO Tully–Fisher relation and the absence of detectable molecular outflows down to sensitive limits. There is no sign that AGN feedback quenches star formation for the quasars in our sample. On the contrary, the abundant gas supply forms stars prodigiously, at a rate that places most of them above the star-forming main sequence and with an efficiency that rivals that of starburst systems.
Introduction
Authors: Monier Frédéric 
Published: August 2020

L’introduction à ce dossier thématique sur la rémunération des élus constate que les enquêtes de première main, reposant sur des sources documentaires, font défaut dans la plupart des pays européens. La question, plus complexe que ce que l’on imagine, éclaire le rapport entre politique et argent, entre rémunération et projets démocratiques. Différentes configurations apparaissent. Dans le cas français, l’indemnité parlementaire créée en 1789, souvent caractérisée comme une norme démocratique, mérite une étude attentive, y compris en scrutant la genèse d’avantages matériels liés au mandat. Par contraste, la situation en Espagne est marquée par la prégnance d’une vision libérale et conservatrice de la fonction de député comme honneur. L’évolution amorcée au tout début du XIXe siècle, ensuite battue en brèche, ne put s’affirmer qu’avec la Deuxième République, après 1931. Enfin, l’étude du cas roumain montre une configuration différente : la rémunération des députés, instituée en 1866, n’y visait ni une plus grande ouverture des formes de sélection du personnel politique, ni la professionnalisation des acteurs. Il s’agissait plutôt d’un ressort financier « systémique ».