bluuebunny/crossref_metadata_2025_split huggingface dataset:
Teresa Mannion and the Emergence of Extreme Weather Culture in Ireland
Authors: Negra Diane 
Published: May 2019

In this article I consider how registers of weather media carry/convey cultural information, specifically how texts about extreme weather articulate with investment in a supposed post-recession restored normality marked by the Irish government's commitment to deregulated transnational capitalism. I maintain that, in a process of cross-cultural remediation, sensationalist codes of US weather media that discursively manage awareness of systemic climate problems are just starting to infiltrate the Irish broadcasting environment. In early December 2015 RTÉ’s Teresa Mannion covered a strong gale, Storm Desmond, amidst inclement conditions in Salthill, Co Galway. Modelling the kind of ‘body at risk’ coverage consummately performed by US Weather Channel personnel, Mannion could barely speak over the lashing rain and strong winds in a dramatic broadcast that quickly became a viral video. This article analyses the fascination with Mannion's piece and its memetic, and attends to the nature of the pleasure taken in her on-camera discomfiture and the breach of gendered territory committed by Mannion at a time when national popular culture in Ireland is under increased obligation to identify and explain climate change-related extreme weather.
Implementation of Distracted Estimation System based on Sensor Fusion through Correlation Analysis with Concentration
Authors: Seo Ji-Yun , Noh Yun-Hong , Jeong Do-Un 
Published: May 2019

Sitting for an extended time may cause a serious chronic disease such as a musculoskeletal disorder, or a cardiovascular disease, diabetes, or obesity. Because a consistently improper posture from early childhood to adolescence can have a number of undesirable effects on the formation of the musculoskeletal structure, learning to maintain a correct posture should be emphasized. A consistently improper posture can not only cause physical problems, it may also lead to emotional issues such as distractions, an attention deficit, and hyperactivity, and the possibility of a low efficiency and performance on assignments is high when the students have a low concentration. The present study implemented a distracted estimation system based on sensor fusion through correlation analysis with concentration that could estimate the level of distraction and prevent musculoskeletal diseases caused by poor sitting posture habits in daily life. The implemented system was designed in the form of a sitting cushion to reflect the ethological movements and characteristics of a sitting position that modern people spend a large amount of time in, and can be easily applied to existing chairs. Both algorithms installed in the system detected the center of gravity of the seated person and displayed positional changes that occurred based on the intensity of the postural changes when moving; thus, simultaneous determination of posture and impulsive behavior was possible. To evaluate the system performance, a posture determination evaluation was conducted, along with distraction estimation according to the rate of changes in posture that occur in everyday life. In addition, to evaluate performance in daily life, a movie-watching scenario was set up, and the distracted-limit estimation and concentration indices according to the rate of changes in posture were comparatively evaluated by reviewing a video of the subjects. The results of the posture determination performance evaluation through 100 posture repetitions on 10 subjects showed a high detection performance of 99.04%. The Pearson’s correlation coefficient results showed a high correlation coefficient (inverse) of r = −0.975076 and a P-VALUE = 1.654 × 10 − 6 . This experiment objectively confirmed the correlation between the DLE Index (based on postural change) and the CI Index (based on EEG).
Perancangan Aplikasi Persediaan Barang dan Bahan Makanan Menggunakan Metode FIFO pada KFC Pematangsiantar
Authors: Fadly Muhammad , Suhendro Dedi , Syahputra Andriyan 
Published: May 2019

Pada PT Fast Food Indonesia Tbk, Cabang Pematangsiantar metode pengolahan barang dan bahan makanan belum terdapat aplikasi yang memadai sehingga untuk memonitoring pengeluaran barang dan bahan makanan Stok Control harus mengecek setiap hari terhadap jumlah barang dan bahan makanan yang keluar. Sedangkan untuk membuat laporan akhir bulan barang dan bahan makanan harus menghitung satu-persatu barang dan bahan makanan sehingga membutuhkan waktu dan tenaga yang cukup besar. Sering kali pencatatan persediaan barang dan bahan makanan mengalami selisih antara stok fisik dan stok opname dikomputer yang mengakibatkan kerugian yang ditanggung oleh karyawan di perusahaan tersebut. Maka dibutuhkan aplikasi di PT Fast Food Indonesia Tbk, Cabang pematangsiantar. Dengan adanya aplikasi diharapkan dapat membantu dalam perhitungan barang dan memonitoring barang tersebut sehingga pada laporan akhir bulan tidak terdapat selisi barang barang antara stok fisik dan stok opname dikomputer.
PERANCANGAN APLIKASI E-LEARNING PADA MTS NEGERI 1 MERANGIN
Authors: SHARIPUDDIN  , EFFIYANDI  , DWI  
Published: May 2019

Proses pembelajaran yang berlangsung di MTS Negeri 1 Merangin masih bersifat konvensional, guru dan murid masih bertatap muka secara langsung untuk melakukan proses belajar-mengajar, sehingga apabila guru berhalangan hadir maka informasi tentang materi pelajaran yang disampaikan kurang maksimal dan keterbatasan waktu yang disediakan menyebabkan lambatnya proses pembelajaran dan kurangnya pemahaman materi pelajaran pada siswa. E-learning adalah proses pembelajaran efektif yang diciptakan dengan cara menggabungkan konten yang disampaikan secara digital dengan jasa dan sarana pendukung pembelajaran. Aplikasi dibangun menggunakan Macromedia Adobe Dreamweaver CS5 dan database MySQL. Hasil dari penelitian ini adalah sebuah aplikasi e-learning yang dapat memberikan kemudahan pada siswa untuk mengakses materi pelajaran meski tidak ada pertemuan di kelas dan sebagai solusi alternatif bagi guru untuk tetap dapat memberikan materi meski tidak bisa hadir saat jam pelajaran.
Defining agricultural cluster’s conceptual framework with Delphi technique
Authors: Micskei Péter 
Published: May 2019

The cluster concept is well defined in the literature, but its agricultural adaptation has not been detailed. A method is needed, which involves experts into the study, who are able to confirm that the modell is correct and help to define the conceptual gaps. The Delphi technique is suitablefor the task. This is a well-structure, iterative future foresight technique, based on experts opinion about the research topic. The method leads to consensus by all means, but it also can have a negative outcome of the researcher's point of view, that's why we have to formulate scenarios.The aim is not statistically significant result, but to build in new ideas into the modell with brainstorming.
OPTIMASI NAÏVE BAYES DENGAN PARTICLE SWARM OPTIMIZATION DAN STRATIFIED UNTUK PREDIKSI KREDIT MACET PADA KOPERASI
Authors: Mardiana Tati 
Published: May 2019

Dalam bisnis, koperasi memiliki peranan penting dalam meningkatkan perekonomian nasional. Ketidakmampuan anggota untuk membayar angsuran kredit merupakan masalah utama yang terjadi pada koperasi. Akibatnya, terjadi kredit macet. Koperasi dapat menghindari kredit macet dengan membuat prediksi dari anggota koperasi yang berpotensi terlambat membayar kredit. Dalam beberapa penelitian telah menggunakan Naive Bayes untuk masalah klasifikasi karena perhitungan yang efisien, dan akurasi tinggi. Tetapi Naive Bayes mengasumsikan bahwa semua atribut kelas tidak tergantung pada atribut lainnya. Naive Bayes sesuai untuk masalah klasifikasi dengan atribut besar. Namun, asumsi ini sering tidak dapat dipertahankan dalam masalah klasifikasi nyata. Dalam beberapa dokumen, kinerja Naive Bayes tidak sempurna. Tujuan dari penelitian ini adalah untuk mengoptimalkan metode Naive Bayes menggunakan Particle Swarm Optimization (PSO) dan untuk meningkatkan akurasi dalam memprediksi kredit macet di koperasi. Penelitian ini menggunakan data dari Pusat Data Koperasi (PUSKOPDIT) DKI Jakarta. Data set kredit yang diperoleh sebanyak 565 record dengan 15 prediktor atribut dan 1 atribut kelas. Hasil pengujian dengan confusion matrix dan kurva ROC diperoleh dari nilai akurasi sebesar 86% dan nilai sebesar 0,867 dengan diagnosis klasifikasi baik. Penelitian ini menunjukkan bahwa penggunaan PSO pada NBC untuk memprediksi kredit macet meningkatkan akurasi 21,03% dan AUC sebesar 0,069. Hasil uji T-Test dan Anova menunjukkan bahwa pada dua metode klasifikasi yang diuji memiliki perbedaan yang nyata (signifikan) dalam nilai AUC.
SISTEM INFORMASI PENGGAJIAN PEGAWAI PADA DINAS TATA KOTA PERTAMANAN DAN KEBERSIHAN LOMBOK BARAT
Authors: - Juahrtini , Suhaimi Muh. , Sriasih - , Nurkholis Lalu Moh. 
Published: May 2019

instansi tergantung pada sistem informasi yang terdapat dalam instansi tersebut. Dinas Tata Kota, Pertamanan dan Kebersihan Lombok Barat merupakan suatu instansi pemerintahan yang bertugas merancang dan melaksanakan pembangunan di bidang tata kota, pertamanan dan kebersihan. Sistem penggajiannya masih menggunakan aplikasi microsoft akan tetapi aplikasi yang digunakan tersebut dalam proses penginputan datanya yang sangatlah rumit sehingga data yang disajikan tidak begitu praktis. Sistem informasi ini dibangun dengan menggunakan metode waterfall dalam pengembangan perangkat lunaknya yang dimulai dari proses perencanaan sampe ke implementasi sistem nya. Hasil dari penelitian ini berupa sebuah sistem infomasi penggajian pegawai pada Dinas Tata Kota, Pertamanan dan Kebersihan Lombok Barat yang diharapkan dapat meningkatkan efektifitas dan produktifitas kerja pegawai dalam mengelola data penggajian. Kata Kunci : Penggajian, Dinas Tata Kota, Pegawai
IMPLEMENTASI POSE TO POSE PADA SIMULASI GERAK PANDA BERJALAN DENGAN TEKNIK FRAME BY FRAME
Authors: Purwanto Ibnu Hadi , Qodarsih Laila , Majid Fatimah Hafizh , Syamrahmarini Khalida Arlinta 
Published: May 2019

Perkembangan animasi saat ini semakin memberi tuntutan bagi para animator untuk menyelesaikan pekerjaannya dengan cepat. Di bab ini akan membahas tentang metode yang mana akan mempermudah animator untuk menyelesaikan produksi animasi tanpa membuang-buang waktu. Membuat simulasi gerakan Panda berjalan dengan membandingkan antara pose to pose dan tanpa pose to pose.Animasi 2D yang dipengaruhi oleh proses animating yang baik pada gerakannya akan menjadikan animasi terlihat lebih hidup. Teknik pose to pose adalah salah satu metode yang digunakan pada proses animating karena pada penerapan metode ini menggunakan perinsip-prinsip dasar animasi. Penggunaaan metode frame by frame biasanya digunakan pada membuatan object yang sangat detail dan halus. Metode ini biasa dikatakan dengan metode animasi tradisional. Dengan penggunaan pose to pose dan tanpa pose to pose akan diketahui perbedaan pergerakan panda berjalan yang dihasilan. Perbandingan yang dilakukan bertujuan untuk mengetahui manakah yang menghasilkan proses lebih cepat dan baik dalam pengerjaannya. Kata kunci: Animasi, metode, frame by frame, pose to pose
IASA Research Grant Report
Authors: Thram Diane 
Published: May 2019

Digital conversion of audio, photographic and film collections in sound and audiovisual archives for purposes of preservation and accessibility has been the norm in archival practice since the 1990s. As a result, analog to digital conversion of many music heritage collections, such as the field recordings of Hugh Tracey at the International Library of African Music (ILAM) in South Africa, has been accomplished. With funding secured from the Mellon Foundation, Rand Merchant Bank Expressions Fund, South African National Heritage Council (NAC) and National Research Foundation (NRF), the recordings, films, photos and documents in the Hugh Tracey Collection (hereafter referred to as the Collection) were catalogued and preserved in digital format from 2006-2008. The audio files and 1,000 images in the Collection have been accessible in compressed form via the Internet since late in 2008. Plus, Tracey’s well-known Sound of Africa and Music of Africa LP series are available as CD compilations and as MP3 files from ILAM and various on-line vendors. Not suprisingly, the many and various opportunities for dissemination digital conversion of field recordings has afforded have brought with them ethical issues for cultural heritage archives which are breifly discussed below.
Compressed Video Quality
Authors: Richardson Iain 
Published: May 2019

The concept of video compression goes hand in hand with the switch from analogue to digital video technology that has taken place over the last 25 years. Video delivered to televisions, computers and smartphones typically arrives in a compressed form. The bandwidth and file size savings that compression provides are a significant benefit for consumer and business applications, making it possible to send and receive high-definition video over limited capacity networks. However, for digital archive applications, compression can be problematic, especially when it introduces loss or distortion into a video signal.
‘Born digital’ often means ‘born compressed’ and it is increasingly likely that newly-created digital video material will have gone through at least some level of lossy compression. For this reason, it is important to understand the effect of video compression on visual quality. In this paper I will introduce the concept of video compression and its relationship to video image quality. I will consider the factors that influence visual quality, including technical factors such as codecs and coding parameters, as well as the complex and only partly-understood factors that govern our perception of moving images. I will introduce methods of measuring and quantifying video quality and show how it is possible to compare the quality and performance of video processing systems, despite the limitations of quality measurement.
The Solar Neighborhood. XLV. The Stellar Multiplicity Rate of M Dwarfs Within 25 pc
Authors: Winters Jennifer G. , Henry Todd J. , Jao Wei-Chun , Subasavage John P. , Chatelain Joseph P. , Slatten Ken , Riedel Adric R. , Silverstein Michele L. , Payne Matthew J. 
Published: May 2019

Abstract
We present results of the largest, most comprehensive study ever done of the stellar multiplicity of the most common stars in the Galaxy, the red dwarfs. We have conducted an all-sky volume-limited survey for stellar companions to 1120 M dwarf primaries known to lie within 25 pc of the Sun via trigonometric parallaxes. In addition to a comprehensive literature search, stars were explored in new surveys for companions at separations of 2″–300″. A reconnaissance of wide companions to separations of 300″ was done via blinking archival images. I-band images were used to search our sample for companions at separations of 2″–180″. Various astrometric and photometric methods were used to probe the inner 2″ to reveal close companions. We report the discovery of 20 new companions and identify 56 candidate multiple systems. We find a stellar multiplicity rate of 26.8 ± 1.4% and a stellar companion rate of 32.4 ± 1.4% for M dwarfs. There is a broad peak in the separation distribution of the companions at 4–20 au, with a weak trend of smaller projected linear separations for lower mass primaries. A hint that M-dwarf multiplicity may be a function of tangential velocity is found, with faster moving, presumably older, stars found to be multiple somewhat less often. We calculate that stellar companions make up at least 17% of mass attributed to M dwarfs in the solar neighborhood, with roughly 11% of M-dwarf mass hidden as unresolved companions. Finally, when considering all M-dwarf primaries and companions, we find that the mass distribution for M dwarfs increases to the end of the stellar main sequence.
OGLE-2018-BLG-0022: A Nearby M-dwarf Binary
Authors: Street R. A. , Bachelet E. , Tsapras Y. , Hundertmark M. P. G. , Bozza V. , Dominik M. ,   ROME/REA and MiNDSTEp Teams,   ROME/REA Team, Bramich D. M. , Cassan A. , Horne K. , Mao S. , Saha A. , Wambsganss J. , Zang Weicheng ,   MiNDSTEp Team, Jørgensen U. G. , Longa-Peña P. , Peixinho N. , Sajadian S. , Burgdorf M. J. , Campbell-White J. , Dib S. , Evans D. F. , Fujii Y. I. , Hinse T. C. , Khalouei E. , Lowry S. , Rahvar S. , Rabus M. , Skottfelt J. , Snodgrass C. , Southworth J. , Tregloan-Reed J. 
Published: May 2019

Abstract
We report observations of the binary microlensing event OGLE-2018-BLG-0022, provided by the Robotic Observations of Microlensing Events (ROME)/Reactive Event Assessment (REA) Survey, which indicate that the lens is a low-mass binary star consisting of M3 (0.375 ± 0.020 M
⊙) and M7 (0.098 ± 0.005 M
⊙) components. The lens is unusually close, at 0.998 ± 0.047 kpc, compared with the majority of microlensing events, and despite its intrinsically low luminosity, it is likely that adaptive optics observations in the near future will be able to provide an independent confirmation of the lens masses.
Detecting Unresolved Binaries in TESS Data with Speckle Imaging
Authors: Matson Rachel A. , Howell Steve B. , Ciardi David R. 
Published: May 2019

Abstract
The Transiting Exoplanet Survey Satellite (TESS) is conducting a two-year wide-field survey searching for transiting exoplanets around nearby bright stars that will be ideal for follow-up characterization. To facilitate studies of planet compositions and atmospheric properties, accurate and precise planetary radii need to be derived from the transit light curves. Since 40%–50% of exoplanet host stars are in multiple star systems, however, the observed transit depth may be diluted by the flux of a companion star, causing the radius of the planet to be underestimated. High angular resolution imaging can detect companion stars that are not resolved in the TESS Input Catalog, or by seeing-limited photometry, to validate exoplanet candidates and derive accurate planetary radii. We examine the population of stellar companions that will be detectable around TESS planet candidate host stars, and those that will remain undetected, by applying the detection limits of speckle imaging to the simulated host star populations of Sullivan et al. and Barclay et al. By detecting companions with contrasts of Δm ≲ 7–9 and separations of ∼0.″02–1.″2, speckle imaging can detect companion stars as faint as early M stars around A–F stars and stars as faint as mid-M around G–M stars, as well as up to 99% of the expected binary star distribution for systems located within a few hundred parsecs.
Measurement of CH3D on Titan at Submillimeter Wavelengths
Authors: Thelen Alexander E. , Nixon Conor A. , Cordiner Martin A. , Charnley Steven B. , Irwin Patrick G. J. , Kisiel Zbigniew 
Published: May 2019

Abstract
We present the first radio/submillimeter detection of monodeuterated methane (CH3D) in Titan’s atmosphere, using archival data from of the Atacama Large Millimeter/submillimeter Array (ALMA). The J

K
= 21−11 and J

K
= 20−10 transitions at 465.235 and 465.250 GHz (∼0.644 mm) were measured at significance levels of 4.6σ and 5.7σ, respectively. These two lines were modeled using the Non-linear optimal Estimator for MultivariatE spectral analySIS (NEMESIS) radiative transfer code to determine the disk-averaged CH3D volume mixing ratio = 6.157 × 10−6 in Titan’s stratosphere (at altitudes >130 km). By comparison with the CH4 vertical abundance profile measured by Cassini–Huygens mass spectrometry, the resulting value for D/H in CH4 is (1.033 ± 0.081) × 10−4. This is consistent with previous ground-based and in situ measurements from the Cassini–Huygens mission, though slightly lower than the average of the previous values. Additional CH3D observations at higher spatial resolution will be required to determine a value truly comparable with the Cassini–Huygens CH4 measurements, by measuring CH3D with ALMA close to Titan’s equator. In the post-Cassini era, spatially resolved observations of CH3D with ALMA will enable the latitudinal distribution of methane to be determined, making this an important molecule for further studies.
Multiple Components in the Broadband γ-Ray Emission of the Short GRB 160709A
Authors: Tak Donggeun , Guiriec Sylvain , Uhm Z. Lucas , Yassine Manal , Omodei Nicola , McEnery Julie 
Published: May 2019

Abstract
GRB 160709A is one of the few bright short gamma-ray bursts detected by both the Gamma-ray Burst Monitor and the Large Area Telescope on board the Fermi Gamma-ray Space Telescope. The γ-ray prompt emission of GRB 160709A is adequately fitted by combinations of three distinct components: (i) a nonthermal component described by a power law (PL) with a high-energy exponential cutoff, (ii) a thermal component modeled with a Planck function, and (iii) a second nonthermal component shaped by an additional PL crossing the whole γ-ray spectrum. While the thermal component dominates during ∼0.12 s of the main emission episode of GRB 160709A with an unusually high temperature of ∼340 keV, the nonthermal components dominate in the early and late time. The thermal component is consistent with the photospheric emission resulting in the following parameters: the size of the central engine,

× 108 cm, the size of the photosphere,

× 1010 cm, and a bulk Lorentz factor,

, assuming a redshift of 1. The slope of the additional PL spectrum stays unchanged throughout the burst duration; however, its flux decreases continuously as a function of time. A standard external shock model has been tested for the additional PL component using the relation between the temporal and spectral indices (the closure relation). Each set of spectral and temporal indices from two energy bands (200 keV–40 MeV and 100 MeV–10 GeV) satisfies a distinct closure relation. From the closure relation test we derived the index for the electron spectral distribution, p = 2.5 ± 0.1. The interaction of the jet with the interstellar environment is preferred over the interaction with the wind medium.
Gemini Imaging of the Host Galaxies of Changing-look Quasars
Authors: Charlton Paul J. L. , Ruan John J. , Haggard Daryl , Anderson Scott F. , Eracleous Michael , MacLeod Chelsea L. , Runnoe Jessie C. 
Published: May 2019

Abstract
Changing-look (CL) quasars are a newly discovered class of luminous active galactic nuclei that undergo rapid (≲10 yr) transitions between Type 1 and Type 1.9/2, with an associated change in their continuum emission. We characterize the host galaxies of four faded CL quasars using broadband optical imaging. We use gri images obtained with the Gemini Multi-Object Spectrograph on Gemini North to characterize the surface brightness profiles of the quasar hosts and search for [O iii] λ4959, λ5007 emission from spatially extended regions, or voorwerpjes, with the goal of using them to examine past luminosity history. Although we do not detect, voorwerpjes surrounding the four quasar host galaxies, we take advantage of the dim nuclear emission to characterize the colors and morphologies of the host galaxies. Three of the four galaxies show morphological evidence of merger activity or tidal features in their residuals. The three galaxies that are not highly distorted are fit with a single Sérsic profile to characterize their overall surface brightness profiles. The single-Sérsic fits give intermediate Sérsic indices between the n = 1 of disk galaxies and the n = 4 of ellipticals. On a color–magnitude diagram, our CL quasar host galaxies reside in the blue cloud, with other active galactic nucleus (AGN) host galaxies and star-forming galaxies. On a color-Sérsic index diagram the CL quasar hosts reside with other AGN hosts in the “green valley.” Our analysis suggests that the hosts of CL quasars are predominantly disrupted or merging galaxies that resemble AGN hosts, rather than inactive galaxies.