bluuebunny/crossref_metadata_2025_split huggingface dataset:
Kajian Semantik Jenis-Jenis Metafora dalam Poster Demonstrasi Tolak RUU 2019 <em>(Semantical Study of Metaphors Types Reflected in RUU 2019 Rejection Demonstration Posters)</em>
Authors: Hasanah Dian Uswatun , Mufti Afrizal , Yulianto Agus 
Published: June 2020

Gelombang demonstrasi penolakan RUU oleh mahasiswa menjadi tragedi demonstrasi terbesar pada 2019. Sebagaimana demonstrasi pada umumnya, penyampaian aspirasi sejumlah mahasiswa menggunakan poster bertuliskan kalimat-kalimat unik, lucu, bahkan aneh. Penelitian ini bertujuan menganalisis dan mengetahui jenis-jenis metafora dalam penulisan poster demonstrasi tolak RUU 2019. Penelitian ini termasuk dalam penelitian deskriptif kualitatif dengan menggunakan metode simak dan teknik catat yang diperoleh dari poster demonstrasi atau melalui media sosial whatsapp dan instagram. Data penelitian ini kemudian dianalisis dengan teknik kualitatif berdasarkan kumpulan kata-kata dari poster para demonstran. Hasil analisis menunjukkan dari enam belas data poster, penulis memperoleh enam jenis metafora, yaitu lima metafora bercitra konkret ke abstrak, dua metafora bercitra sinestesia, dua metafora bercitra predikatif, dua metafora bercitra nominatif, tiga metafora bercitra abstrak ke konkret, dan dua metafora bercitra antropomorfik.Â A wave of student rejection bills became the biggest demonstration tragedy in 2019. As a demonstration in general, the delivery of the aspirations of a number of students using posters bearing unique, funny, even strange sentences. This research aims to analyze and find out the types of metaphors in poster demonstration rejecting the RUU 2019. It was a qualitative descriptive research that used observe and take note methods obtained from demonstration posters or through social media whatsapp and instagram. Then, the research data was analyzed using qualitative techniques based on a collection of words from the demonstrators' posters. The analysis showed that from the sixteen poster data, the writer obtained six types of metaphors, those were five concrete-to-abstract metaphors, two synesthesia-based metaphors, two predicate-imagined metaphors, two nominative-imaging metaphors, three abstract-to-concrete-based metaphors, and two anthropomorphic-imaging metaphors.
Pelaporan Keuangan Akuntansi Infak/Sedekah Sesuai PSAK 109 (Studi Kasus pada Komunitas Badar Batang)
Authors: Ningtyas Jilma Dewi Ayu 
Published: June 2020

Sistem Ekonomi Islam berpijak pada asas keadilan dan kemanusiaan. Unutk mengaplikasikan kepedulian social dan meningkatkan kesejahteraan umat manusia, Islam memberikan sebuah media yang dikenal dengan sebutan zakat. ( (Shahnaz, 2016) Zakat, Infak/sedekah merupakan solusi untuk membantu mensejahterakan masyarakat, kita sebagai sesama muslim hendaknya saling membantu. Sesuai ajaran Alqur’an pada Surah Al-Baqarah Ayat 195
Berdasarkan PSAK Syariah NO. 109 terdapat Lembaga pengelola zakat, infak/ sedekah yang disebut dengan Amil dimana tugasnya adalah mengumpulkan dan menyalurkan zakat, infak/sedekah (IAI, 2008). Pada penelitian ini Lembaga yang saya maksud adalah Komunitas Badar. Komunitas Badar menjadi penyalur infaq, sedekah dan amal Jariyah dari harta donator yang sudah mempercayakan sebagian hartanya diberikan kepada anak yatim piatu dan dhuafa, oleh sebab itu pengurus Komunitas tidak bias seenaknya menggunakan uang donator, sehingga dalam pemasukan dan pengeluaran uangnya dicatat dengan sedemikian rupa. Setelah melakukan wawancara dengan ketua Komunitas Badar Sr. Joko Suprapto menyatakan bahwa manajemen keuangan dan pembukuan sudah dilakukan dengan sederhana, berupa pencatatan kas masuk dan keluar sedangkan hal-hal lain tidak diperhatikan. Oleh sebab itu kami berkesempatan untuk mendampingi Komunitas melaksanakan manajemen keuangan dan pembukuan sesuai dengan peraturan yang berlaku yaitu sesuai dengan PSAK no. 109
Jenis penelitian yan digunakan pada penelitian ini adalah penelitian deskriptif kualitatif yaitu metode yang sifatnya menguraikan, menggambarkan, membandingkan suatu data dan keadaan serta menerangkan suatu keadaan sedemikian rupa sehinga dapat ditarik kesimpulan ( (Shahnaz, 2016). Subyek penelitian adalah Komunitas Badar yaitu komunitas penyantun Anak Yatim Piatu dan Dhuafa yang beralamatkan di Jl. Pasar Manis Ds. Kedungmalang Kec. Wonotunggal Batang Jawa Tengah. Waktu penelitian dari bulan Desember s.d Februari 2020. Metode penelitian dengan menggunakan Survey, DOkumentasi dan Wawancara.
Berdasarkan hasil penelitian dan pembahasan diperoleh kesimpulan bahwa 1) Komunitas Badar tidak memiliki Dana Zakat, Dana Amil, dan Dana Non Halal, karena Komunitas Badar berdiri berdasarkan keikhlasan kelompok orang untuk mensedekahkan sebagian hartanya untuk kaum dhuafa dan yatim piatu. 2) Komunitas Badar tidak memiliki Kas dari aktivitas Investasi dan Arus Kas Pendanaan hanya Aktivitas Operasional saja. 3) Laporan Keuangan yang di laporkan merupakan laporan keuangan tahunan transaksi 2018/2019. 4)Pelaporan Keuangan Komunitas Badar hanya bentuk transaksi keluar dan masuk saja, setelah penelitian ini pelaporan keuangan Komunitas Badar dibuat sederhana disesuaikan dengan PSAK No. 109
Coinages and Slogans as Strategies for Identity Construction in the 2019 General Elections in Nigeria
Authors: Adeola Akinola , Muhyideen Imam 
Published: June 2020

The study investigates how coinages and slogans are political conduits used strategically by individuals in constructing their identities in the 2019 general election political discourse in Nigeria. The study adopted Norman Fairclough and Ruth Wodak‘s Discourse-Historical analysis model of CDA, together with Clusivity theory and Halliday’s Systemic Functional Linguistics. Twenty four comments involving coinages and slogans that cut across popular subject areas of politics relating to the Nigerian 2019 general election between 2018 and 2019 are purposively sampled. Data for the study were retrieved from the Nairaland forum archives. The comments were sampled, scrutinized and analysed using the content analysis method. The use of coinages and slogans can be implicit or explicit. It was revealed that when constructing identity, political actors can employ coinages and slogans to reflect the notion of “positive self-representation” and “negative other-representation” established in Wieczorek’s strategies of Inclusion and Exclusion in Clusivity theory. Coinages and slogans are also used for different discursive strategies such as persuasion, negotiation, sarcasm and rhetorical questions. Political actors used coinages and slogans as political conduits to delineate and negotiate their political affiliations and dissociations and also to achieve, advocate, alter and (re)build their political ideologies and leanings in the 2019 general election in Nigeria.
Spreadable Virus of the 21stCentuary: COVID-19
Authors: Chaudhary Priya , Janmeda Pracheta 
Published: June 2020

The latest outbreak of a respiratory disease, known as coronavirus disease 19 (COVID-19), is the third virus spillover from animals to humans in the last two decades. The disease is caused by coronavirus and has converted into an epidemic in recent days. It spread via direct contact or droplets of nasal-discharge from one human-to-another within the mean-incubation period of 6.5 days. Dyspnea, cough and fever are the most common symptoms in the patients of COVID-19, though along with diarrhea in 3% cases. Bilateral pulmonary with ground-glass opacity and consolidation has been observed in 98% cases of the disease by the help of computed tomography. The treatment process of COVID-19 with chloroquine and remdesivir drug is under the clinical trial worldwide and responding well to cure the disease. Under the prevalent circumstances, the main goal is to control the widespread infection of SARS-CoV-2 across the world and to aware the public regarding the possible preventive measures and treatments. However, the public health authorities should keep a close eye on the circumstances strictly, as the more we know about this novel coronavirus and its outbreak, the better we can respond or control the conditions worldwide.
Impact of aqueous and organic extracts of Rhodobryum roseum on inhibition of fungal and bacterial growth
Authors: Singh Shivom , Srivastava Rathore Kajal , Khanna D.R. 
Published: June 2020

Mosses have been known for millennia and highly esteemed all over the world as the rich source of bioactive compounds. The research targets on evolution of microbicidal potentialities of Rhodobryum roseum (extract) used against selected fungus (X. oryzae pv oryzae, S. enteric, P. multocida and M. plutonius) and bacteria (R. solani, S. rolfsii, F. oxysporum and T. indica) to assay antimicrobial activity. Impact of aqueous and undertaken organic viz., ethanol, acetone, choloform, petroleum ether, methanol extract of R. roseum, at varied concentrations and at different time intervals were examined against the growth of bacteria and fungus. All the aqueous extracts were proved to be infective against all the tested pathogens. The antimicrobial potential of six extracts was screened against undertaken bacteria and fungi using micro broth dilution assay. Out of the six (diverse organic and aqueous) extract of R. roseum in ethanol and acetone showed maximum inhibitory activity in S. rolfsii with the MIC value of 5.00 (µg/ml), along with MFC value of 6.25 (µg/ml) in acetone extract and the value of MBC was recorded utmost in X. oryzae with value 3.00 (µg/ml) extracted in ethanol. Over all, the organic extract of R. roseum has potent antimicrobial activity and could be possible source of lead molecules considered for the future development of microbicidal agent.
Preparation and Application of Garnet Electrolyte Thin Films: Promise and Challenges
Authors: Yan Xufeng , Han Weiqiang 
Published: June 2020

All-solid-state batteries (ASSBs) have attracted much attention in recent years, due to their high energy density, excellent cycling performance, and superior safety property. As the key factor of all-solid-state batteries, solid electrolyte determines the performance of the batteries. Garnet-typed cubic Li7La3Zr2O12(LLZO) has been reported as the most promising solid electrolyte on the way to ASSBs. Thin film electrolyte could contribute to a higher energy density and a lower resistance in a battery. This short review exhibits the latest efforts on LLZO thin film and discusses the different preparation methods, together with their effects on characteristics and electrochemical performances of the solid electrolyte film.
PENGENDALIAN SERANGAN HAMA LALAT BUAH PADA INTENSITAS KERUSAKAN BUAH CABAI RAWIT (Capsicum frutescens L) DENGAN BAHAN PETROGENOL
Authors: Budiyani Ni Komang , Sukasana I Wayan 
Published: June 2020

Abstrack
Cayenne pepper is a horticulture plant (vegetable) where the fruit is used for various food purposes. The decrease of the chilly yields productivity caused by several factors including the use of varieties with low yields and the attack of Plant Pests (OPT). Pests that often attack chili plants are fruit flies. Petrogenol could be used to control this pest.The method used was a randomized block design with 7 treatments and 3 replications by comparing the dose of petrogenol.
The results showed that the D3 treatment showed the best parameters in the use of petrogenol doses in controlling fruit fly pests, in the parameters of healthy fruits, damaged fruit, insect catches, and damage intensity. The use of high doses of petrogenol can influence the trapping of fruit flies and as the control of fruit fly attacks
Keywords : Fruit flies, cayenne pepper and petrogenol
Lyα Observations of Comet C/2013 A1 (Siding Spring) Using MAVEN IUVS Echelle
Authors: Mayyasi Majd , Clarke John , Combi Michael , Fougere Nicolas , Quemerais Eric , Katushkina Olga , Bhattacharyya Dolon , Crismani Matteo , Deighan Justin , Jain Sonal , Schneider Nicholas , Jakosky Bruce 
Published: June 2020

Abstract
The close approach of comet C/2013 A1 (Siding Spring) to Mars in 2014 October provided a unique opportunity to observe a dynamically new Oort cloud comet with potential for interaction with a planet’s atmosphere. The water-originating hydrogen coma of the comet extended to over 20 million km from the nucleus. Determining the properties of this coma contributes to characterizing the comet’s water content and production rate. The present study analyzes a unique data set of high spectral resolution UV observations of comet C/2013 A1 Siding Spring measured by the Mars Atmosphere and Volatile Evolution spacecraft. The Siding Spring observations capture Lyα emissions from the Martian corona, the interplanetary medium, as well as the cometary H and D reservoirs. The isolated cometary spectra are analyzed to reveal a velocity distribution of H atoms that are consistent with model estimates of H2O photodissociated H emissions and of OH photodissociated H emissions, Doppler shifted from the main comet H emission line center by 18 km s−1 and 8 km s−1, respectively. The variations in comet H brightness with distance from the nucleus are used to constrain cometary water production to a rate of 0.5 × 1028 molecules s−1 at a time when Siding Spring was at 1.5 au, pre-perihelion.
Rotationally Driven Ultraviolet Emission of Red Giant Stars
Authors: Dixon Don , Tayar Jamie , Stassun Keivan G. 
Published: June 2020

Abstract
Main-sequence stars exhibit a clear rotation-activity relationship, in which rapidly rotating stars drive strong chromospheric/coronal ultraviolet and X-ray emission. While the vast majority of red giant stars are inactive, a few percent exhibit strong ultraviolet emission. Here we use a sample of 133 red giant stars observed by Sloan Digital Sky Survey APOGEE and Galaxy Evolution Explorer to demonstrate an empirical relationship between near-UV (NUV) excess and rotational velocity (

). Beyond this simple relationship, we find that NUV excess also correlates with rotation period and with Rossby number in a manner that shares broadly similar trends to those found in M dwarfs, including activity saturation among rapid rotators. Our data also suggest that the most extremely rapidly rotating giants may exhibit so-called supersaturation, which could be caused by centrifugal stripping of these stars rotating at a high fraction of breakup speed. As an example application of our empirical rotation-activity relation, we demonstrate that the NUV emission observed from a recently reported system comprising a red giant with a black hole companion is fully consistent with arising from the rapidly rotating red giant in that system. Most fundamentally, our findings suggest a common origin of chromospheric activity in rotation and convection for cool stars from main sequence to red giant stages of evolution.
KR Persei, a Mid-F Eclipsing Binary with a One-day Period
Authors: Sowell James R. , Hollingworth Emily , Fekel Francis C. , Muterspaugh Matthew W. , Dale Horace , Savello Alexander D. , Coughlin Jeffrey L. , Williamon Richard M. 
Published: June 2020

Abstract
KR Per is a partially eclipsing binary with an orbital period of 0.9960798 days, very close to one sidereal day, making it difficult to obtain extensive phase coverage in a reasonable amount of time. We used the Wilson–Devinney program to determine its orbital elements and stellar absolute dimensions from recently acquired radial velocities and differential BVRI observations that were supplemented with previous differential UBV measurements and published times of minima. The two components are each F5 V stars with masses of

and

. The radii are

and

. The orbital period of the eclipsing system is variable and more times of minima observations are needed. A comparison with evolutionary tracks indicates that the system has an age of 2.1 ± 0.1 Gyr.
Seeds of Life in Space (SOLIS). IX. Chemical Segregation of SO2 and SO toward the Low-mass Protostellar Shocked Region of L1157
Authors: Feng S. , Codella C. , Ceccarelli C. , Caselli P. , Lopez-Sepulcre A. , Neri R. , Fontani F. , Podio L. , Lefloch B. , Liu H. B. , Bachiller R. , Viti S. 
Published: June 2020

Abstract
We present observations of SO and SO2 lines toward the shocked regions along the L1157 chemically rich outflow, taken in the context of the Seeds of Life in Space IRAM Northern Extended Millimeter Array Large Program, and supported by data from the Submillimeter Array and IRAM-30 m telescope at 1.1–3.6 mm wavelengths. We simultaneously analyze, for the first time, all of the brightest shocks in the blueshifted lobe, namely, B0, B1, and B2. We found the following. (1) SO and SO2 may trace different gas, given that the large(-scale) velocity gradient analysis indicates for SO2 a volume density (

) denser than that of the gas emitting in SO by a factor up to an order of magnitude. (2) Investigating the 0.1 pc scale field of view, we note a tentative gradient along the path of the precessing jet. More specifically,

decreases from the B0–B1 shocks to the older B2. (3) At a linear resolution of 500–1400 au, a tentative spatial displacement between the two emitting molecules is detected, with the SO peak closer (with respect to SO2) to the position where the recent jet is impinging on the B1 cavity wall. Our astrochemical modeling shows that the SO and SO2 abundances evolve on timescales less than about 1000 years. Furthermore, the modeling requires high abundances (2 × 10−6) of both

and S/H injected in the gas phase due to the shock occurrence, so prefrozen OCS only is not enough to reproduce our new observations.
ALMA Observations of Giant Molecular Clouds in M33. I. Resolving Star Formation Activities in the Giant Molecular Filaments Possibly Formed by a Spiral Shock
Authors: Tokuda Kazuki , Muraoka Kazuyuki , Kondo Hiroshi , Nishimura Atsushi , Tosaki Tomoka , Zahorecz Sarolta , Onodera Sachiko , Miura Rie E. , Torii Kazufumi , Kuno Nario , Fujita Shinji , Sano Hidetoshi , Onishi Toshikazu , Saigo Kazuya , Fukui Yasuo , Kawamura Akiko , Tachihara Kengo 
Published: June 2020

Abstract
We report molecular line and continuum observations toward one of the most massive giant molecular clouds (GMCs), GMC-16, in M33 using ALMA with an angular resolution of 0.″44 × 0.″27 (∼2 pc × 1 pc). We have found that the GMC is composed of several filamentary structures in 12CO and 13CO(J = 2–1). The typical length, width, and total mass are ∼50–70 pc, ∼5–6 pc, and ∼105
M
⊙, respectively, which are consistent with those of giant molecular filaments (GMFs) as seen in the Galactic GMCs. The elongations of the GMFs are roughly perpendicular to the direction of the galaxy’s rotation, and several H ii regions are located at the downstream side relative to the filaments with an offset of ∼10–20 pc. These observational results indicate that the GMFs are considered to be produced by a galactic spiral shock. The 1.3 mm continuum and C18O(J = 2–1) observations detected a dense clump with the size of ∼2 pc at the intersection of several filamentary clouds, which is referred to as the “hub filament,” possibly formed by a cloud–cloud collision. A strong candidate for protostellar outflow in M33 has also been identified at the center of the clump. We have successfully resolved the parsec-scale local star formation activity in which the galactic scale kinematics may induce the formation of the parental filamentary clouds.
A Detailed View of the Circumstellar Environment and Disk of the Forming O-star AFGL 4176
Authors: Johnston Katharine G. , Hoare Melvin G. , Beuther Henrik , Linz Hendrik , Boley Paul , Kuiper Rolf , Kee Nathaniel Dylan , Robitaille Thomas P. 
Published: June 2020

Abstract
We present a detailed analysis of the disk and circumstellar environment of the forming O-type star AFGL 4176 mm1, placing results from the Atacama Large Millimeter/submillimeter Array (ALMA) into context with multiwavelength data. With ALMA, we detect seventeen 1.2 mm continuum sources within 5″ (21,000 au) of AFGL 4176 mm1. We find that mm1 has a spectral index of 3.4 ± 0.2 across the ALMA band, with >87% of its 1.2 mm continuum emission from dust. The source mm2, projected 4200 au from mm1, may be a companion or a blueshifted knot in a jet. We also explore the morphological differences between the molecular lines detected with ALMA, finding 203 lines from 25 molecules, which we categorize into several morphological types. Our results show that AFGL 4176 mm1 provides an example of a forming O-star with a large and chemically complex disk, which is mainly traced by nitrogen-bearing molecules. Lines that show strong emission on the blueshifted side of the disk are predominantly oxygen-bearing, which we suggest are tracing a disk accretion shock. The molecules C34S, H2CS, and CH3CCN trace a slow wide-angle wind or dense structures in the outflow cavity walls. With the Australia Telescope Compact Array (ATCA), we detect a compact continuum source (<2000 × 760 au) at 1.2 cm, associated with mm1, of which >96% is from ionized gas. The ATCA NH3(1, 1) and (2, 2) emission traces a large-scale (r ∼ 0.5 pc) rotating toroid with the disk source mm1 in the blueshifted part of this structure offset to the northwest.
On the Formation of SS433
Authors: Han Qin , Li Xiang-Dong 
Published: June 2020

Abstract
SS433 is an extraordinary X-ray binary that is ejecting bipolar jets at 26% the speed of light. Associated with the supernova-like shell W50, SS433 is also probably one of the youngest X-ray binaries with an age of ≲105 yr. However, the masses of the two components in SS433 and even the nature of the compact object are still under debate. In this work, assuming that the compact object is a black hole, we employ a binary population synthesis method to study the formation of SS433. We use previous estimates of the age of W50 and the duration of the jet activity to constrain the evolutionary history. Our calculations suggest that SS433 likely harbored a Hertzsprung gap star at the beginning of the current Roche-lobe overflow phase. The masses of the black hole and the optical/donor star in SS433 suggested by the simulations are around 8 M
☉ and 24 M
☉, respectively. Future measurement of the donor mass and radius can help infer not only the origin of the binary but also the nature of the nebula W50.
A Rapidly Varying Red Supergiant X-Ray Binary in the Galactic Center
Authors: Gottlieb Amy M. , Eikenberry Stephen S. , Ackley Kendall , DeWitt Curtis , Marco Amparo 
Published: June 2020

Abstract
We analyzed multiwavelength observations of the previously identified Galactic center X-ray binary CXO 174528.79–290942.8 (XID 6592) and determine that the near-infrared counterpart is a red supergiant based on its spectrum and luminosity. Scutum X-1 is the only previously known X-ray binary with a red supergiant donor star and closely resembles XID 6592 in terms of X-ray luminosity (L
X), absolute magnitude, and IR variability (L
IR,var), supporting the conclusion that XID 6592 contains a red supergiant donor star. The XID 6592 infrared counterpart shows variability of ∼0.5 mag in the Wide-field Infrared Survey Explorer-1 band (3.4 μm) on timescales of a few hours. Other infrared data sets also show large-amplitude variability from this source at earlier epochs but do not show significant variability in recent data. We do not expect red supergiants to vary by ∼50% in luminosity over these short timescales, indicating that the variability should be powered by the compact object. However, the X-ray luminosity of this system is typically ∼1000× less than the variable luminosity in the infrared and falls below the Chandra detection limit. While X-ray reprocessing can produce large-amplitude fast infrared variability, it typically requires

L
IR,var to do so, indicating that another process must be at work. We suggest that this system may be a supergiant fast X-ray transient (SFXT), and that a large (∼1038 ergs s−1), fast (102-4 s) X-ray flare could explain the rapid IR variability and lack of a long-lasting X-ray outburst detection. SFXTs are normally associated with blue supergiant companions, so if confirmed, XID 6592 would be the first red supergiant SFXT, as well as the second X-ray red supergiant binary.