bluuebunny/crossref_metadata_2025_split huggingface dataset:
PEMANFAATAN MEDIA SOSIAL TIK TOK SEBAGAI MEDIA KAMPANYE GERAKAN CUCI TANGAN DI INDONESIA UNTUK MENCEGAH COVID-19
Authors: Hasiholan Togi Prima , Pratami Rezki , Wahid Umaimah 
Published: August 2020

Indonesia yang sebanyak 64,8% penduduknya sudah menggunakan Internet dan 160 Juta jiwa merupakan pengguna sosial media, membuat Indonesia merupakan pasar yang menjanjikan oleh para pelaku industry sosial media, seperti aplikasi Tik Tok. Ditahun 2020 aplikasi Tik Tok menjadi budaya populer di Indonesia, karena masyarakat Indonesia pasti mengetahui aplikasi iini dan menjadi penggunanya.Populernya Tik Tok di Indonesia menjadi media yang ideal oleh World Health Organization (WHO) yang mengkampanyekan gerakan cuci tangan yang benar untuk memutus penularan Virus COVID-19 atau yang dikenal dengan nama corona dengan memproduksi video serta hastag #safehands challenge di aplikasi Tik Tok yang selanjutnya para creator memproduksi konten video versi mereka sendiri dan menambahkan hastag #safehands challenge untuk mengikuti challenge ini.Kampanye lewat video dengan hastag #safehands challenge ini banyak disaksikan, namun ada beberapa point yang mendasari video mana yang paling banyak disaksikan,sukai dan share oleh pengguna Tik Tok.
A REVIEW OF STREET GRILLED MEAT (SUYA) IN BENIN CITY, NIGERIA: A POTENTIAL PUBLIC HEALTH RISK
Authors: Okhuebor Shadrach , Izevbuwa Osazee 
Published: August 2020

Suya originated in the northern parts of Nigeria is ready to eat grilled skewered meat products prepared in different forms spiced with locally sourced, commonly produced by the Hausas in Northern Nigeria. It has permeated Nigerian society, being affordable for all and available everywhere. It is produced from boneless meat hung on stick and spiced with peanut cake, salt, vegetable oil and other flavourings followed by roasting around a glowing charcoal fire. It’s generally made with skewered beef, ram, or chicken. Innards such as kidney, liver, and tripe are also used. Suya are of three main forms namely Tsire, Kilishi, and Balangu, and Tsire is the most commonly preferred. In Benin City, which is located in the southern part of Nigeria, Suya has become a very common street food delicacy scattered most major areas and are sold mostly in the evening time, only very few vendors will sell Suya in the day time. Concerns have been raised in many research regarding the public health risk of consuming suya, part of which is food poisoning, as a result microbial contamination such as Bacillus cereus, Staphylococcus aureus, aflatoxigenic molds, Staphylococcus epidermidis, Proteus vulgaris, Klebseilla pneumoniae, Escherichia coli, Candida spp., Salmonella enteritica and Enterobacter spp. Trace metals such as zinc, lead, manganese, iron, and copper have been observed in suya in concentrations exceeding recommended tolerable upper intake levels which can consequently cause serious long term health issues. This study reviews the potential public health risk of consuming street grilled meat (Suya) in Benin City.
Fostering trust, collaboration, and a culture of continuous quality improvement: A call for transparency in medical school accreditation
Authors: Javidan Arshia , Raveendran Lucshman , Rai Yeshith , Tackett Sean , Kulasegaram Kulamakan Mahan , Whitehead Cynthia , Rosenfield Jay , Houston Patricia 
Published: August 2020

Medical schools provide the foundation for a physician’s growth and lifelong learning. They also require a large share of government resources. As such, they should seek opportunities to maintain trust from the public, their students, faculty, universities, regulatory colleges, and each other. The accreditation of medical schools attempts to assure stakeholders that the educational process conforms to appropriate standards and thus can be trusted. However, accreditation processes are poorly understood and the basis for accrediting authorities’ decisions are often opaque.
We propose that increasing transparency in accreditation could enhance trust in the institutions that produce society’s physicians. While public reporting of accreditation results has been established in other jurisdictions, such as Australia and the United Kingdom, North American accrediting bodies have not yet embraced this more transparent approach. Public reporting can enhance public trust and engagement, hold medical schools accountable for continuous quality improvement, and can catalyze a culture of collaboration within the broader medical education ecosystem. Inviting patients and the public to peer into one of the most formative and fundamental parts of their physicians’ professional training is a powerful tool for stakeholder and public engagement that the North American medical education community at large has yet to use.
HAMBATAN PELAKSANAAN TUGAS DAN PERAN PEMBIMBING KEMASYARAKATAN TERHADAP ANAK YANG BERHADAPAN DENGAN HUKUM MENURUT UU NOMOR 11 TAHUN 2012
Authors: Khrisnawati Elizabeth Nanik 
Published: August 2020

Abstrak :
Anak yang berhadapan0dengan0hukum0sesuai yang0diatur0dalam0Undang-undang0Sist em0Peradilan0Pidana0Anak0Nomor 11 tahun 2012 memiliki hak untuk didampingi oleh Pembimbing Kemasyarakatan. Pembimbing Kemasyarakatan tidak saja bertugas untuk melakukan penelitian kemasyarakatan, tetapi juga melakukan pembimbingan, pengawasan, dan juga pen dampingan terhadap0Anak0yang0berhadapan0dengan0hukum. 0Pembimbing0Kemasyarakatan0memiliki0pe ran0besar bagi anak yang0berhadapan hukum untuk dapat melalui semua proses pidana yang dijatuhkan padanya. Adapun beberapa faktor yang dapat menjadi pendukung maupun penghambatbagi Pembimbing Kemasyarakatan dalam melaksanakan tugas dan perannya. Faktor-faktor tersebut dapat dilihat dari faktor internal Pembimbing Kemasyarakatan sendiri ataupun dapat berasal dari sisi anak yang berhadapan dengan hukum yaitu yang dikaitkan dengan jumlah anak, psikis dan pribadi anak serta kesediaan kerja samadari pihak keluarga anak. Faktor-faktor tersebut jika dipenuhi dapat menjadi faktor pendukung dan sebaliknya jika tidak terpenuhi baik keseluruhan maupun sebagian maka akan menjadi penghambat dan membuat pelaksanaan tugas Pembimbing Kemasyarakatan kurang optimal.

Kata Kunci :Faktor pendukung, faktor penghambat, Tugas, Peran, Pembimbing Kemasyarakatan, Anak, Hukum
Aspek Digital Marketing Bagi Kemajuan Disc Jockey
Authors: Dewi Liliana , Tantomo Marco 
Published: August 2020

This study aimed to find out the Evaluation of Marketing Strategies for Shift Paradigm. The method used in this research was a qualitative method. Research subjects involved 7 consumers, Shift Paradigm members, expert marketing, and lecturers EP6. This study found Paradigma Shift’s marketing strategy was not effective. Using digital marketing was recommended to maximize marketing strategies for Shift Paradigm. In addition to a digital marketing, involving event planner and promoter were also recommended to reach the marketing targets of the shift paradigm. The results of this study are expected to serve as review materials for the Evaluation of Marketing Strategies for Shift Paradigm and other Disc Jockey Management.
Penerapan SAK-EMKM Pada Kesenian Jaranan Turonggo Bimo Kertosono Sebagai Simbol Budaya
Authors: Erstiawan Martinus Sony 
Published: August 2020

Art groups that have the soul of art in Indonesia are a group of micro, small, and medium entities (EMKM) that can use financial accounting standards for micro, small, and medium entities (SAK-EMKM). One of them is the art group which is still a symbol of cultural preservation, namely jaranan art. Financial management (recording, presentation, and disclosure) in the art of the networking requires the intention and practice as often as possible, so as to produce a simple financial report following accounting standards in force in Indonesia. This essay has the purpose of using a descriptive study of the application of SAK-EMKM to be applied to arts groups in Indonesia.
Analisis Pengaruh Kebijakan Utang, Kepemilikan Saham Publik, Risiko Kebangkrutan Terhadap Biaya Agency
Authors: Sharasanti Diah Anugrah 
Published: August 2020

Financial management strategic decision that can not be ignored is the decision regarding the dividend policy, investment, and financing, are closely associated with the company's goal is to optimize the value of the company. However, the goals are often not carried out in connection with the separation of the functions of ownership and management functions of the company, which makes the manager to act independently and not in line with company objectives. Conflicts over the source of the problem that causes the cost of the agency (agency cost), ie all costs incurred to carry out surveillance (monitoring) on the performance of managers. The research objective was to determine whether the debt ratio, managerial ownership, and earnings volatility significantly affect the cost of agency. Results showed that the ratio of debt, stock ownership by top managers, and earnings volatility significantly not affect the cost of agency.
Efektifitas Media Pembelajaran IPA Berbasis Masalah Untuk Meningkatkan Kreativitas Mahasiswa Calon Guru SD
Authors: Sum Suriya Ningsyih , Syahriani Yulianci  , Adi Apriadi Adiansha  , Nurjumiati  , Asriyadin  
Published: August 2020

Abstrak : Penelitian ini fokus untuk menguji efektifitas dari media pembelajaran IPA berbasis masalah dalam meningkatkan kreativitas mahasiswa calon guru SD yang bertujuan untuk melatih mahasiswa calon guru meningkatkan krativitas dalam mengajar pembelajaran IPA. Desain penelitian ini menggunakan One Shot Case Study yang dilaksanakan pada mahasiswa calon guru SD STKIP Taman Siswa Bima yang menempuh matakuliah pembelajaran IPA SD kelas lanjut. Hasil karya mahasiswa diobservasi sebagai hasil berpikir kreatif mahasiswa dalam mendasain media pembelajaran IPA berbasis masalah. Instrumen yang dugunakan dalam penelitian ini berupa lembar observasi menggunakan skala Penyekoran Holistik. Hasil Analisis data diperoleh nilai rata-rata persentase sebesar 84 % dengan kategori sangat kreatif. Berdasarkan hasil analisis data, dapat disimpulkan bahwa media pembelajaran IPA berbasis masalah efektif dalam meningkatkan kreativitas mahasiswa calon guru SD.
KELT-25 b and KELT-26 b: A Hot Jupiter and a Substellar Companion Transiting Young A Stars Observed by TESS*
Authors: Martínez Romy Rodríguez , Gaudi B. Scott , Rodriguez Joseph E. , Zhou George , Labadie-Bartz Jonathan , Quinn Samuel N. , Penev Kaloyan , Tan Thiam-Guan , Latham David W. , Paredes Leonardo A. , Kielkopf John F. , Addison Brett , Wright Duncan J. , Teske Johanna , Howell Steve B. , Ciardi David , Ziegler Carl , Stassun Keivan G. , Johnson Marshall C. , Eastman Jason D. , Siverd Robert J. , Beatty Thomas G. , Bouma Luke , Bedding Timothy , Pepper Joshua , Winn Joshua , Lund Michael B. , Villanueva Steven , Stevens Daniel J. , Jensen Eric L. N. , Kilby Coleman , Crane Jeffrey D. , Tokovinin Andrei , Everett Mark E. , Tinney C. G. , Fausnaugh Michael , Cohen David H. , Bayliss Daniel , Bieryla Allyson , Cargile Phillip A. , Collins Karen A. , Conti Dennis M. , Colón Knicole D. , Curtis Ivan A. , Depoy D. L. , Evans Phil , Feliz Dax L. , Gregorio Joao , Rothenberg Jason , James David J. , Joner Michael D. , Kuhn Rudolf B. , Manner Mark , Khakpash Somayeh , Marshall Jennifer L. , McLeod Kim K. , Penny Matthew T. , Reed Phillip A. , Relles Howard M. , Stephens Denise C. , Stockdale Chris , Trueblood Mark , Trueblood Pat , Yao Xinyu , Zambelli Roberto , Vanderspek Roland , Seager Sara , Jenkins Jon M. , Henry Todd J. , James Hodari-Sadiki , Jao Wei-Chun , Wang Sharon Xuesong , Butler Paul , Thompson Ian , Shectman Stephen , Wittenmyer Robert , Bowler Brendan P. , Horner Jonathan , Kane Stephen R. , Mengel Matthew W. , Morton Timothy D. , Okumura Jack , Plavchan Peter , Zhang Hui , Scott Nicholas J. , Matson Rachel A. , Mann Andrew W. , Dragomir Diana , Günther Max , Ting Eric B. , Glidden Ana , Quintana Elisa V. 
Published: August 2020

Abstract
We present the discoveries of KELT-25 b (TIC 65412605, TOI-626.01) and KELT-26 b (TIC 160708862, TOI-1337.01), two transiting companions orbiting relatively bright, early A stars. The transit signals were initially detected by the KELT survey and subsequently confirmed by Transiting Exoplanet Survey Satellite (TESS) photometry. KELT-25 b is on a 4.40 day orbit around the V = 9.66 star CD-24 5016 (

K, M
⋆ =

M
⊙), while KELT-26 b is on a 3.34 day orbit around the V = 9.95 star HD 134004 (

=

K, M
⋆ =

M
⊙), which is likely an Am star. We have confirmed the substellar nature of both companions through detailed characterization of each system using ground-based and TESS photometry, radial velocity measurements, Doppler tomography, and high-resolution imaging. For KELT-25, we determine a companion radius of R
P =

R
J and a 3σ upper limit on the companion’s mass of ∼64 M
J. For KELT-26 b, we infer a planetary mass and radius of M
P =

and R
P =

R
J. From Doppler tomographic observations, we find KELT-26 b to reside in a highly misaligned orbit. This conclusion is weakly corroborated by a subtle asymmetry in the transit light curve from the TESS data. KELT-25 b appears to be in a well-aligned, prograde orbit, and the system is likely a member of the cluster Theia 449.
ARES. III. Unveiling the Two Faces of KELT-7 b with HST WFC3*
Authors: Pluriel William , Whiteford Niall , Edwards Billy , Changeat Quentin , Yip Kai Hou , Baeyens Robin , Al-Refaie Ahmed , Fabienne Bieger Michelle , Blain Dorian , Gressier Amélie , Guilluy Gloria , Yassin Jaziri Adam , Kiefer Flavien , Modirrousta-Galian Darius , Morvan Mario , Mugnai Lorenzo V. , Poveda Mathilde , Skaf Nour , Zingales Tiziano , Wright Sam , Charnay Benjamin , Drossart Pierre , Leconte Jérémy , Tsiaras Angelos , Venot Olivia , Waldmann Ingo , Beaulieu Jean-Philippe 
Published: August 2020

Abstract
We present the analysis of the hot-Jupiter KELT-7 b using transmission and emission spectroscopy from the Hubble Space Telescope, both taken with the Wide Field Camera 3. Our study uncovers a rich transmission spectrum that is consistent with a cloud-free atmosphere and suggests the presence of H2O and H−. In contrast, the extracted emission spectrum does not contain strong absorption features and, although it is not consistent with a simple blackbody, it can be explained by a varying temperature–pressure profile, collision induced absorption, and H−. KELT-7 b had also been studied with other space-based instruments and we explore the effects of introducing these additional data sets. Further observations with Hubble, or the next generation of space-based telescopes, are needed to allow for the optical opacity source in transmission to be confirmed and for molecular features to be disentangled in emission.
The Morphology–Density Relationship in 1 < z < 2 Clusters
Authors: Sazonova Elizaveta , Alatalo Katherine , Lotz Jennifer , Rowlands Kate , Snyder Gregory F. , Boone Kyle , Brodwin Mark , Hayden Brian , Lanz Lauranne , Perlmutter Saul , Rodriguez-Gomez Vicente 
Published: August 2020

Abstract
The morphology–density relationship states that dense cosmic environments such as galaxy clusters have an overabundance of quiescent elliptical galaxies, but it is unclear at which redshift this relationship is first established. We study the morphology of four clusters with 1.2 < z < 1.8 using Hubble Space Telescope imaging and the morphology computation code statmorph. By comparing the median morphology of cluster galaxies to CANDELS field galaxies using Monte Carlo analysis, we find that two out of four clusters (at z = 1.19 and 1.75) have an established morphology–density relationship with more than 3σ significance. Approximately 50% of the galaxies in these clusters are bulge-dominated, compared to ∼30% in the field, and they are significantly more compact. This result is more significant for low-mass galaxies with

, showing that low-mass galaxies are affected the most in clusters. We also find an intriguing system of two z ≈ 1.45 clusters at a unusually small 2D separation of 3′ and 3D separation of ≈73 Mpc that exhibit no morphology–density relationship but have enhanced merger signatures. We conclude that the environmental mechanism responsible for the morphology–density relationship is (1) already active as early as z = 1.75; (2) forms compact, bulge-dominated galaxies; and (3) affects primarily low-mass galaxies. However, there is a significant degree of intracluster variance that may depend on the larger cosmological environment in which the cluster is embedded.
A Catalog of 531 White Dwarf Candidates in the Local Galactic Halo from Gaia Data Release 2
Authors: Kim Bokyoung , Lépine Sebastien , Medan Ilija 
Published: August 2020

Abstract
We present a catalog of 531 white dwarf candidates that have large apparent transverse motions relative to the Sun (

km s−1), thus making them likely members of the local Galactic halo population. The candidates were selected from the Gaia Data Release 2 and are located in a great circle with 20° width running across both Galactic poles and the Galactic center and anticenter, a zone that spans 17.3% of the sky. The selection used a combination of kinematic and photometric properties, derived primarily from Gaia proper motions, G magnitudes, and

color, and including parallax whenever available. Additional validation of the white dwarf candidates is made using PanSTARRS photometric (gri) data. Our final catalog includes not only stars having full kinematic and luminosity estimates from reliable Gaia parallax, but also stars with presently unreliable or no available Gaia parallax measurements. We argue that our method of selecting local halo objects with and without reliable parallax data leads us to round up all possible halo white dwarfs in the Gaia catalog (in that particular section of the sky) with recorded proper motions

mas yr−1 and that pass our

km s−1 threshold requirement. We expect this catalog will be useful for the study of the white dwarf population of the local Galactic halo.
A Detailed Study of Massive Galaxies in a Protocluster at z = 3.13
Authors: Shi Ke , Toshikawa Jun , Cai Zheng , Lee Kyoung-Soo , Fang Taotao 
Published: August 2020

Abstract
We present a detailed study of near-IR selected galaxies in a protocluster field at z = 3.13. Protocluster galaxies are selected using the available mutliwavelength data with the photometric redshifts (photo-z) at 2.9 < z < 3.3, reaching a mass completeness of

. Diverse types of galaxies have been found in the field, including normal star-forming galaxies, quiescent galaxies, and dusty star-forming galaxies. The photo-z galaxies form two large overdense structures in the field, largely overlapping with the previously identified galaxy overdensities traced by Lyα emitters (LAEs) and Lyman break galaxies, respectively. The northern overdensity consists of a large fraction of old and/or dusty galaxy populations, while the southern one is mainly composed of normal star-forming galaxies that are spatially correlated with the LAEs. This agrees with our previous study arguing the spatial offset of different galaxy overdensities may be due to halo assembly bias. Given the large end-to-end sizes of the two overdensities, one possibility is that they will form into a supercluster by the present day. We also find strong evidence that the star formation activities of the galaxies in the overdense protocluster regions are enhanced in comparison to their field counterparts, which suggests an accelerated mass assembly in this protocluster.
Common Envelope Wind Tunnel: Range of Applicability and Self-similarity in Realistic Stellar Envelopes
Authors: Everson Rosa Wallace , MacLeod Morgan , De Soumi , Macias Phillip , Ramirez-Ruiz Enrico 
Published: August 2020

Abstract
Common envelope evolution, the key orbital tightening phase of the traditional formation channel for close binaries, is a multistage process that presents many challenges to the establishment of a fully descriptive, predictive theoretical framework. In an approach complementary to global 3D hydrodynamical modeling, we explore the range of applicability for a simplified drag formalism that incorporates the results of local hydrodynamic “wind tunnel” simulations into a semi-analytical framework in the treatment of the common envelope dynamical inspiral phase using a library of realistic giant branch stellar models across the low, intermediate, and high-mass regimes. In terms of a small number of key dimensionless parameters, we characterize a wide range of common envelope events, revealing the broad range of applicability of the drag formalism as well its self-similar nature across mass regimes and ages. Limitations arising from global binary properties and local structural quantities are discussed together with the opportunity for a general prescriptive application for this formalism.
Citlalmitl: A Laser-based Device for Meteoritical Sample Fabrication with Arbitrary Thermal Histories
Authors: Hernández-Reséndiz Patricia , Cruz-Ramírez Héctor , U’Ren Alfred B. , Cervantes-de la Cruz Karina Elizabeth , Segura Antígona 
Published: August 2020

Abstract
We present Citlalmitl (the word for meteorite in the Nahuatl language), a new experimental device designed and built to simulate high-temperature processes relevant for meteoritics, including chondrule formation and the atmospheric entry of micrometeorites (MMs). The main component of Citlalmitl is a 50 W CO2 laser, used to melt samples that simulate the precursors of meteoritical materials. As examples of the operation of our device, we have irradiated silicate samples controlling the laser duty cycle to reproduce heating profiles predicted by shock-wave simulations. Citlalmitl records the sample temperature during and after irradiation, a unique feature that allows us to directly measure the thermal history of the sample, a key parameter for the characteristics observed in MMs and chondrules. We demonstrate that Citlalmitl can reproduce different heating profiles useful to mimic thermal histories in meteoritical processes.
138175 (2000 EE104) and the Source of Interplanetary Field Enhancements
Authors: Jewitt David 
Published: August 2020

Abstract
We present the first optical observations taken to characterize the near-Earth object 138175 (2000 EE104). This body is associated with interplanetary field enhancements (IFEs), thought to be caused by interactions between the solar wind magnetic field and solid material trailing in the orbit of the parent body. Based on optical photometry, the radius (in meters) and mass (in kilograms) of an equal-area sphere are found to be

and

, respectively, where p

R
is the red geometric albedo and a density of ρ = 1500 kg m−3 is assumed. The measured colors are intermediate between those of C-type (primitive) and S-type (metamorphosed) asteroids but, with correction for the likely effects of phase reddening, are more consistent with a C-type classification than with S-type. No evidence for co-moving companions larger than ∼40(0.1/p

R
) m in radius is found, and no dust particle trail is detected, setting a limit to the trail optical depth of τ ≤ 2 × 10−9. Consideration of the size distribution produced by impact pulverization makes it difficult to generate the mass of nanodust (minimum 105–106 kg) required to account for IFEs, unless the size distribution is unusually steep. Furthermore, impact pulverization timescales for source objects of the required size are much longer than the dynamical timescale. While the new optical data do not definitively refute the hypothesis that boulder pulverization is the source of IFEs, neither do they provide any support for it.