bluuebunny/crossref_metadata_2025_split huggingface dataset:
Problematika Peraturan Pemerintah Pengganti Undang-Undang (PERPPU) No. 02 Tahun 2017 Tentang Organisasi Kemasyarakatan
Authors: Salim Choirus 
Published: January 2019

sebelum Perppu Nomor 2 Tahun 2017 Tentang Organisasi Kemasyarakatan disahkan menjadi UU Nomor 6 Tahun 2017 terjadi pro kontra berkaitan dengan isi muatan Perppu tersebut. Kita ketahui bahwa Perppu Nomer 2 Tahun 2017 disahkan menjadi undang-undang melalui mekanisme voting. Ada tujuh fraksi partai politik yang menerima Perppu Nomor 2 Tahun 2017 Tentang Ormas yang dirapatkan sebagai undang-undang yaitu fraksi PPP, PDI-P, Golkar, PKB,Hanura, Demokrat, dan Nasdem. Namun Fraksi Demokrat, PPP dan PKB menerima secara bersyarat Perppu tersebut, yakni mengharuskan supaya DPR dan Pemerintah segera melakukan revisi Perppu yang baru saja disetujui menjadi Undang-undang itu. Setelah dikeluarkannya Perppu No. 2 Tahun 2017 dan dibubarkannya HTI, terjadi perlawanan hukum dengan mengajukan judial review oleh beberapa Organisasi Masyarakat seperti Front Pembela Islam (FPI), Dewa Dakwah Islamiyah (DDI), Perkumpulan Hidayatullah dan Pemuda Indonesia serta HTI sendiri yang lebih dahulu mengajukan judial review ke Mahkamah Konstitus. Dari beberapa uraian di atas, pro kontra berkenaan dengan Perppu No. 2 Tahun 2017 Tentang Ormas juga terjadi pada Organisasi-Organisasi Islam di Kota Metro.
Industrial cooperation as a vector for further development of the market and support to domestic manufacturers
Authors: Shelgunov A. V. 
Published: January 2019

Subject: the problem of industry cooperation.Objectives: analysis of the main problems and prospects of industrial cooperation.Materials and methods: production cooperation allows you to combine the efforts of individual industrial enterprises to implement large-scale projects that are not feasible with the efforts of one enterprise. With the collapse of the USSR, many plants lost their cooperation ties, which, on the one hand, led to the need for their own production, which meant independence and the possibility of creating additional jobs. The main forms of sectoral cooperation are described. It is indicated that the development of the direction of cooperation as a subcontracting will be the most interesting for small and medium-sized businesses, as it gives small businesses the opportunity to move from the simplest value-added schemes to their own industrial production, and large ones to reduce costs and focus all attention on the production of basic products. Describes the stage of entry into industrial cooperation. It is noted that joint cooperation activities involve the disclosure of certain information that is the property of a party, from which there is a clear requirement in the legal protection of their rights. Attention is drawn to the need to further improve the regulatory framework and mechanisms for the involvement of small and medium-sized manufacturing business in the technological chains of large enterprises. Results: In advanced countries, the production cooperation of small businesses with large enterprises is well developed. In connection with the above, the project of the Chamber of Commerce and Industry of the Russian Federation “Register of reliable partners” is an effective tool that will facilitate the way for small and medium-sized enterprises to enter into partnership programs.Conclusions: the need to support small businesses with their small-scale production. The Association of Power and Energy Equipment Manufacturers should unite representatives of small and large businesses in the field of energy and power equipment and become a guarantor for the state about the reliability of its members.
Pemanfaatan Open Jurnal System (OJS) Untuk Pengelolaan Jurnal Lumbung di Politeknik Pertanian Negeri Payakumbuh
Authors: Amrizal Amrizal 
Published: January 2019

Open Journal System atau OJS adalah sebuah Content Management System berbasis web yang khusus dibuat untuk menangani keseluruhan prosesmanajemen publikasi ilmiah dari proses call for paper, peer review, hingga penerbitan dalam bentuk online. Politeknik Pertanian Negeri Payakumbuh memiliki satu jurnal yaitu LUMBUNG yang dikelola oleh Pusat Penelitian dan Pengabdian Kepada Masyarakat (P3M). Jurnal Lumbung diterbitkan dalam edisi cetak karena belum memiliki system untuk publikasi secara online. Kelemahan dari sistem penerbitan yang masih manual ini bisa diatasi dengan mengimplemtasikan sistem penerbitan secara elektronik menggunakan Open Jurnal System (OJS) yang bisa dikelola dan diakses secara online. Penerbitan jurnal menggunakan OJS mesti mengacu kepada standar operasional prosedur (SOP) pada OJS yang sudah ditetapakan dimana beberapa aktor yang terlibat didalam penernbnitan jurnal pada system OJS diaantaranya adalah Manager Jurnal, Editor, Author dan Reviewer.
ТЕПЛОФІЗИЧНІ ВЛАСТИВОСТІ ГОЛОВОК КАПУСТИ ЦВІТНОЇ ЗАЛЕЖНО ВІД УМОВ ВЕГЕТАЦІЙНОГО ПЕРІОДУ
Authors: Pusik L. M. , Gaevaya L. O. 
Published: January 2019

Мета. Дослідити теплофізичні властивості головок капусти цвітної залежно від умов вегетаційного періоду та від особливостей гібрида. Методи. Загальнонаукові: 1. метод гіпотез – складання схем дослідів; 2. метод експерименту – схеми польових і лабораторних дослідів; 3. метод аналізу та синтезу – формування висновків і узагальнень, розрахунково-аналітичні. Результати. Встановлено, що особливість гібрида капусти цвітної ранньостиглої впливає на теплофізичні властивості маси продукції на 8‑15 %, умови вегетаційного періоду – на 76‑87 %, сумісна дія факторів становить 1‑3 %, інших факторів – 2‑6 %. Особливість гібрида капусти цвітної пізньостиглої впливає на теплофізичні властивості маси продукції на 30–75 %. Більші значення теплообмінних характеристик продукції серед досліджуваних ранньостиглих гібридів капусти цвітної – у Опал F1, пізньостиглих – у Каспер F1. За ентальпією ранньостиглі гібриди капусти цвітної неістотно відрізнялися один від одного. Упродовж років досліджень цей показник був на рівні 89,28–106,74 кДж/кг, в середньому за роки досліджень – 96,48–96,93 кДж/кг залежно від гібрида. Ентальпія головок пізньостиглих гібридів капусти цвітної упродовж 2015–2017 рр. була в межах 53,65–83,09 кДж/кг залежно від гібрида. Різниця між гібридами була істотною. Висновки. Питома теплоємність ранньостиглих гібридів капусти цвітної становила 3,74–3,95 кДж/кг.оС, теплопровідність – 1,75 Вт/м.оС, температуропровідність – 4,38–4,44.10-4 м2/с. Питома теплоємність головок пізньостиглих гібридів капусти цвітної коливалася в межах 3,77–3,95 кДж/кг.оС. Гібриди істотно різнилися між собою за теплопровідністю, у середньому за роки досліджень вона становила 1,74‑1,77 Вт/м.оС. Температуропровідність маси продукції гібрида Скайвокер F1 істотно перевищувала показники інших гібридів і становила 4,48.10-4 м2/с. Більші значення теплообмінних характеристик продукції серед досліджуваних ранньостиглих гібридів капусти цвітної – у Опал F1, пізньостиглих – у Каспер F1
KAJIAN YURIDIS PENETAPAN SANKSI DI BAWAH SANKSI MINIMUM DALAM PENYALAHGUNAAN NARKOTIKA
Authors: Nurdin M. 
Published: January 2019

Tindak pidana narkotika merupakan salah satu pidana khusus dalam bentuk extra ordinary crime. Pengaturan hukum tindak pidana narkotika diatur dalam Undang-Undang No. 35 Tahun 2009 tentang Narkotika, dimana di dalamnya mengatur tentang ancaman pidana minimum. Hal ini dapat dilihat dalam Pasal 114 ayat (1) Undang-Undang No. 35 Tahun 2009 tentang Narkotika. Dalam Pasal tersebut terdapat pertentangan apa yang seharusnya dipertimbangkan oleh hakim dalam mengambil keputusan dalam hal penerapan pidana dengan ancaman pidana minimum tersebut. Adapun permasalahan yang dikaji yaitu bagaimanakah pengaturan sanksi tindak pidana narkotika dikaitkan dengan sanksi di bawah sanksi minimum. Dan, bagaimanakah konsekuensi hukum terhadap putusan hakim yang memutuskan perkara pidana narkotika dengan sanksi di bawah minimum. Metode yang digunakan adalah metode yuridis normatif yaitu metode penelitian kepustakaan dengan mengelusuri data sekunder
استخدام الشبكات العصبية لأغراض التمييز
Authors: دخيل طاهر ريسان 
Published: January 2019

يعد اسلوب التمييز بين المجموعات من الاساليب الشائعة الاستخدام وذلك لكثرة الظواهر التطبيقية التي يمكن ان يتم تحليلها من خلال هذا الاسلوب، وهناك العديد من الطرائق التي يمكن ان تستخدم لهذا الغرض، مثل الدالة التمييزية الخطية، والتربيعية، وفي الفترة الاخيرة برز استخدام الشبكات العصبية Neural Networks كأداة للتمييز بين المجموعات .
وفي بحثنا هذا تم استخدام المحاكاة لغرض المقارنة بين طريقة الشبكات العصبية والطريقة التقليدية لتصنيف المشاهدات الى المجموعة التي تنتمي اليها وذلك في حالة كون بعض المتغيرات تتوزع توزيعاً غير التوزيع الطبيعي وذلك لمعرفة افضلية الطريقتين المستخدمتين . وقد تم استخدام معيار نسبة المشاهدات المصنفة خطئا" الى مجموع المشاهدات الكلي كمعيار للمقارنة بين الطريقتين .
جدلية تنظير العلاقة بين الجماعية والتعاون	في إطار نظرية المنظمة
Authors: حمود العنزي سعد علي , ثابت زياد كاظم 
Published: January 2019

أشارت الجهود المعرفية السابقة إلى وجود اهتمام متزايد بالجماعات (Groups) على أساس أنها اللبنات الأساسية لقيام المنظمات. وقد فرض تعدد المنظمات في المجتمعات المعاصرة وتباينها من حيث أهدافها وطبيعة نشاطها، تجزئة فعالياتها إلى تخصصات عدة على وفق إطار تقسيم العمل، وبما أدى إلى تقسيم الأفراد العاملين إلى جماعات مختلفة في أدائها وأحجامها وشكلها، والتي تعمل جميعها لتحقيق هدف تلك المنظمات الذي قامت من اجله، مما يحقق لها البقاء والتقدم في وسط بيئة تتصف بالتغيير السريع. ولعل ابرز ما يشغل الباحثين والممارسين والدارسين للجماعات، هو تحقيق التناسق والتكامل داخلها، ومن أبرز أشكال التناسق والتناغم بين أفراد الجماعة الواحدة هو التعاون (Cooperation) ولقد عدَ (Barnard 1938) وهو أحد أوائل المنظرين في مجال التنظيم الحديث، التعاون شيئاً مهماً جداً لبقاء الوحدة الاجتماعية مستمرة في تلك الوحدة التي يرفع أعضاؤها بعضهم البعض للسلوك التعاوني. وهنالك منظرون آخرون تأثروا بـ Barnard)) أمثال (March & Simon)و (Thomson)، أدخلوا فيما بعد آراء مماثلة لارائه، وبالنتيجة صار التعاون مفهوماً أساسياًً في علم المنظمة والسلوك التنظيمي (Wagner, 1995). وعلى الرغم من الأهمية الكبيرة للتعاون، إلا أن المرء ينظر من خارج علم المنظمة ليجد سيلاً كبيراً من النظريات والبحوث والدراسات التي تتعلق بالتعاون بين أنواع الجماعات في منظمات الأعمال المعاصرة. فقد قام الباحثون في مجال الاقتصاد، وعلم النفس الاجتماعي بدراسة الأنماط السلوكية التي سميت "بالتطفل"Free–Riding) ) "والتواكل" Loafing Social)) أو الاعتمادية على الغير (Wagner, 1995)، وسعت بدورها إلى تحديد العوامل التي تعيق ميول الأفراد نحو التعاون. وفي مجال آخر من البحوث علقّ عدد من علماء الاجتماع على الميول الفردية للعديد من النظريات الحالية بشأن التعاون الاجتماعي والسلوك الإنساني، وأتجه بعضهم للقول إلى أن وجود الميول المتجهة نحو الجماعية قد تحفز التعاون بطرائق لم يجرِ تصورها في معظم البحوث، ومن هذا المنطلق، يجد الباحثان أنفسهما أمام أهمية دراسة مدخل الجماعية وأثره في تعاون الأفراد والجماعات داخل المنظمات، ومن أبرز ما وجداه مهماً هو هذا المدخل الذي يقود الفرد العامل في جماعة ما إلى تحديد سلوكياته داخلها، ومن ثم فأن اتجاهاته تؤثر في سلوكياته نحو التعاون مع أقرانه في الجماعة، أو عدم التعاون معهم.
Cancer statistics, 2019
Authors: Siegel Rebecca L. , Miller Kimberly D. , Jemal Ahmedin 
Published: January 2019

AbstractEach year, the American Cancer Society estimates the numbers of new cancer cases and deaths that will occur in the United States and compiles the most recent data on cancer incidence, mortality, and survival. Incidence data, available through 2015, were collected by the Surveillance, Epidemiology, and End Results Program; the National Program of Cancer Registries; and the North American Association of Central Cancer Registries. Mortality data, available through 2016, were collected by the National Center for Health Statistics. In 2019, 1,762,450 new cancer cases and 606,880 cancer deaths are projected to occur in the United States. Over the past decade of data, the cancer incidence rate (2006‐2015) was stable in women and declined by approximately 2% per year in men, whereas the cancer death rate (2007‐2016) declined annually by 1.4% and 1.8%, respectively. The overall cancer death rate dropped continuously from 1991 to 2016 by a total of 27%, translating into approximately 2,629,200 fewer cancer deaths than would have been expected if death rates had remained at their peak. Although the racial gap in cancer mortality is slowly narrowing, socioeconomic inequalities are widening, with the most notable gaps for the most preventable cancers. For example, compared with the most affluent counties, mortality rates in the poorest counties were 2‐fold higher for cervical cancer and 40% higher for male lung and liver cancers during 2012‐2016. Some states are home to both the wealthiest and the poorest counties, suggesting the opportunity for more equitable dissemination of effective cancer prevention, early detection, and treatment strategies. A broader application of existing cancer control knowledge with an emphasis on disadvantaged groups would undoubtedly accelerate progress against cancer.
Spectroscopic Redshift of the Gamma-Ray Blazar B2 1215+30 from
Lyα Emission
Authors: Furniss A. , Worseck G. , Fumagalli M. , Johnson C. A. , Williams D. A. , Pontrelli P. , Prochaska J. X. 
Published: January 2019

Abstract
We report on Cosmic Origin Spectrograph observations of the gamma-ray bright
blazar B2 1215+30, collected in 2015 November. These observations allow for
the confirmation of the source redshift from the detection of a
Lyα emission feature at
λ ∼ 1374 Å. The emission feature
places the source at a redshift of
z = 0.1305 ± 0.003,
confirming the source’s ground-based spectral measurement. The gamma-ray
emission of the source is discussed in the context of the source distance,
required for the accurate reconstruction of the intrinsic gamma-ray emission
taking the absorption by the extragalactic background light into account. The
source distance is found to be low enough that the previously reported detection
of an exceptional flaring event from B2 1215+30 in 2014 cannot be used to
investigate opacity-specific spectral and variability characteristics introduced
by possible ultra-high-energy cosmic-ray propagation.
Future Prospects for Ground-based Gravitational-wave Detectors: The Galactic Double Neutron Star Merger Rate Revisited
Authors: Pol Nihan , McLaughlin Maura , Lorimer Duncan R. 
Published: January 2019

Abstract
We present the Galactic merger rate for double neutron star (DNS) binaries using an observed sample of eight DNS systems merging within a Hubble time. This sample includes the recently discovered, highly relativistic DNS systems J1757−1854 and J1946+2052, and is approximately three times the sample size used in previous estimates of the Galactic merger rate by Kim et al. Using this sample, we calculate the vertical scale height for DNS systems in the Galaxy to be z
0 = 0.4 ± 0.1 kpc. We calculate a Galactic DNS merger rate of

Myr−1 at the 90% confidence level. The corresponding DNS merger detection rate for Advanced LIGO (Laser Interferometer Gravitational-wave Observatory) is

, where D
r is the range distance. Using this merger detection rate and the predicted range distance of 120–170 Mpc for the third observing run of LIGO, we predict, accounting for 90% confidence intervals, that LIGO–Virgo will detect anywhere between zero and two DNS mergers. We explore the effects of the underlying pulsar population properties on the merger rate and compare our merger detection rate with those estimated using different formation and evolutionary scenario of DNS systems. As we demonstrate, reconciling the rates is sensitive to assumptions about the DNS population, including its radio pulsar luminosity function. Future constraints from further gravitational wave DNS detections and pulsar surveys anticipated in the near future should permit tighter constraints on these assumptions.
Deep Chandra Observations of ESO 428-G014. IV. The Morphology of the Nuclear Region in the Hard Continuum and Fe Kα Line
Authors: Fabbiano G. , Siemiginowska A. , Paggi A. , Elvis M. , Volonteri M. , Mayer L. , Karovska M. , Maksym W. P. , Risaliti G. , Wang Junfeng 
Published: January 2019

Abstract
We report the results of high-resolution subpixel imaging of the hard continuum and Fe Kα line of the Compton-thick (CT) active galactic nucleus (AGN) ESO 428-G014, observed with Chandra ACIS. While the 3–4 keV emission is dominated by an extended component, a single nuclear point source is prominent in the 4–6 keV range. Instead, two peaks of similar intensity, separated by ∼36 pc in projection on the plane of the sky are detected in the Fe Kα emission. The SE knot could be marginally associated with the heavily obscured hard continuum source. We discuss four possible interpretations of the nuclear morphology. (1) Given the bolometric luminosity and likely black hole mass of ESO 428-G014, we may be imaging two clumps of the CT obscuring torus in the Fe Kα line. (2) The Fe Kα knots may be connected with the fluorescent emission from the dusty bicone, or (3) with the light echo of a nuclear outburst. (4) We also explore the less likely possibility that we may be detecting the rare signature of merging nuclei. Considering the large-scale kiloparsec-size extent of the hard continuum and Fe Kα emission (Papers I and II), we conclude that the AGN in ESO 428-G014 has been active for at least 104 yr. Comparison with the models of Czerny et al. suggests high accretion rates during this activity.
An Unexpectedly Small Emission Region Size Inferred from Strong High-frequency Diffractive Scintillation in GRB 161219B
Authors: Alexander K. D. , Laskar T. , Berger E. , Johnson M. D. , Williams P. K. G. , Dichiara S. , Fong W. , Gomboc A. , Kobayashi S. , Margutti R. , Mundell C. G. 
Published: January 2019

Abstract
We present Karl G. Jansky Very Large Array radio observations of the long gamma-ray burst GRB 161219B (z = 0.147) spanning 1–37 GHz. The data exhibit unusual behavior, including sharp spectral peaks and minutes-timescale large-amplitude variability centered at 20 GHz and spanning the full frequency range. We attribute this behavior to scattering of the radio emission by the turbulent ionized Galactic interstellar medium (ISM), including both diffractive and refractive scintillation. However, the scintillation is much stronger than predicted by a model of the Galactic electron density distribution (NE2001); from the measured variability timescale and decorrelation bandwidth we infer a scattering measure of SM ≈ (8–70) × 10−4 kpc m−20/3 (up to 25 times larger than predicted in NE2001) and a scattering screen distance of d
scr ≈ 0.2–3 kpc. We infer an emission region size of

μas (

cm) at ≈4 days, and find that prior to 8 days the source size is an order of magnitude smaller than model predictions for a uniformly illuminated disk or limb-brightened ring, indicating a slightly off-axis viewing angle or significant substructure in the emission region. Simultaneous multi-hour broadband radio observations of future GRB afterglows will allow us to characterize the scintillation more completely, and hence to probe the observer viewing angle, the evolution of the jet Lorentz factor, the structure of the afterglow emission regions, and ISM turbulence at high Galactic latitudes.
The Number of Dwarf Satellites of Disk Galaxies versus their Bulge Mass in the Standard Model of Cosmology
Authors: Javanmardi B. , Raouf M. , Khosroshahi H. G. , Tavasoli S. , Müller O. , Molaeinezhad A. 
Published: January 2019

Abstract
There is a correlation between the bulge mass of the three main galaxies of the Local Group (LG), i.e., M31, Milky Way (MW), and M33, and the number of their dwarf spheroidal galaxies. A similar correlation has also been reported for spiral galaxies with comparable luminosities outside the LG. These correlations do not appear to be expected in standard hierarchical galaxy formation. In this paper, and for the first time, we present a quantitative investigation of the expectations of the standard model of cosmology for this possible relation using a galaxy catalog based on the Millennium-II simulation. Our main sample consists of disk galaxies at the centers of halos with a range of virial masses similar to M33, MW, and M31. For this sample, we find an average trend (though with very large scatter) similar to that observed in the LG; disk galaxies in heavier halos on average host heavier bulges and a larger number of satellites. In addition, we study sub-samples of disk galaxies with very similar stellar or halo masses (but spanning a range of 2–3 orders of magnitude in bulge mass) and find no obvious trend in the number of satellites versus bulge mass. We conclude that, while for a wide galaxy mass range a relation arises (which seems to be a manifestation of the satellite number–halo mass correlation), for a narrow range there is no relation between number of satellites and bulge mass in the standard model. Further studies are needed to better understand the expectations of the standard model for this possible relation.
A Semi-implicit Particle-in-cell Expanding Box Model Code for Fully Kinetic Simulations of the Expanding Solar Wind Plasma
Authors: Elena Innocenti Maria , Tenerani Anna , Velli Marco 
Published: January 2019

Abstract
We address the challenges that come with fully kinetic Particle-In-Cell (PIC) simulations of the expanding solar wind by introducing a semi-implicit, Expanding Box Model (EBM) approach to the study of solar wind kinetic physics. Plasma propagation and expansion are dealt with via the variable change of the EBM. In this way the large separation between scales of interest and domain size is addressed by including solar wind propagation and expansion as time-dependent coupling terms and coordinate stretching. The semi-implicit discretization, in the widely used Implicit Moment Method (IMM) flavor, promises to increase the simulated domain size and duration with respect to explicit discretization. The EBM IMM equations are derived and tested against expected behavior of expanding plasma.
On the Geometry of Curvature Radiation and Implications for Subpulse Drifting
Authors: McSweeney S. J. , Bhat N. D. R. , Tremblay S. E. , Deshpande A. A. , Wright G. 
Published: January 2019

Abstract
The phenomenon of subpulse drifting offers unique insights into the emission geometry of pulsars, and is commonly interpreted in terms of a rotating carousel of “spark” events near the stellar surface. We develop a detailed geometric model for the emission columns above a carousel of sparks that is entirely calculated in the observer’s inertial frame, and which is consistent with the well-understood rotational effects of aberration and retardation. We explore the observational consequences of the model, including (1) the appearance of the reconstructed beam pattern via the cartographic transform, and (2) the morphology of drift bands and how they might evolve as a function of frequency. The model, which is implemented in the software package PSRGEOM, is applicable to a wide range of viewing geometries, and we illustrate its implications using PSRs B0809+74 and B2034+19 as examples. Some specific predictions are made with respect to the difference between subpulse evolution and microstructure evolution, which provides a way to further test our model.