bluuebunny/crossref_metadata_2025_split huggingface dataset:
The Notion of “Court” under the Succession Regulation
Authors: Wilderspin Michael 
Published: November 2020

The article concerns the notion of “court” in the Succession Regulation. This notion is used in the Brussels I and Brussels Ia Regulations, where it does not necessarily have the same scope. The author attempts to interpret the concept in the light of the recitals to the Succession Regulation (in particular Recital 20) and of the case law of the Court of Justice. The very general description of the concept contained in Article 3(2) of the Regulation might potentially embrace other authorities and legal professionals, where they exercise judicial functions by way of delegation of power from the court. In the author’s view, the European Court, especially in Oberle and WB v Notariusz Przemysława Bac correctly navigated its way through the Succession Regulation and ruled in a way which is both coherent as regards the operation of the Regulation and consistent with the intentions of the legislator. The above judgments are analysed also with regard to Poland’s omission to notify notaries as “courts” under Article 79 of the Succession Regulation. The European Court found that the criteria for determining whether an authority or a legal professional, in particular a notary public, constitutes a “court” aredetermined by Article 3(2) and not by Article 79. Consequently, Poland’s omission to notify was not conclusive, but was in any event correct in substance. The author expresses the opinion that the judgment is accurate on this point.
ANALISIS NEED ASSESMENT SISWA SMP GENERASI Z TERHADAP PELAYANAN BK DI SEKOLAH SE-KOTA BANJARMASIN
Authors: Rachmayanie J. Ririanti , Sugianto Akhmad , Andri Setiawan Muhammad , Jariah Ainun 
Published: November 2020

Tujuan penelitian ini adalah mengkaji kebutuhan layanan bimbingan dan konseling bagi siswa SMP yang terkategori generasi Z. Dasar dari penelitian untuk menganalisis kebutuhan layanan bimbingan dan konseling sebagai dasar bagi pengembangan program bimbingan dan konseling yang didasarkan pada empat bidang layanan yakni bidang pribadi, sosial, belajar, dan karir. Populasi dari penelitian ini adalah siswa SMP dari 5 sekolah menengah pertama yang berasal dari 5 kecamatan kota Banjarmasin. Dari direncanakan diambil 35 orang dengan total 175 orang siswa, namun yang mengembalikan instrumen hanya 163 orang siswa dengan teknik pengumpulan data cluster sampling. Hasil penelitian menunjukkan bidang pribadi 93% menduduki urutan pertama, disusul oleh karir 89%, diikuti sosial sebanyak 87%, dan terakhir ditutup belajar sebanyak 78% sebagai bidang yang paling dibutuhkan dalam pelayanan bimbingan dan konseling. Hasil penelitian merekomendasikan agar dapat menjadikan penelitian ini sebagai dasar untuk melakukan pengembangan program bimbingan dan konseling. __________________________________________________________The purpose of this study is to examine the need for guidance and counseling services for junior high school students categorized as Z generation. The basis of the research is to analyze the needs of guidance and counseling services as a basis for developing guidance and counseling programs based on four service areas namely personal, social, learning, and career. The population of this research is junior high school students from 5 junior high schools from 5 districts of Banjarmasin city. Of the planned 35 people taken with a total of 175 students, but only 163 students returned the instrument with cluster sampling data collection techniques. The results showed the private sector 93% ranked first, followed by career 89%, followed by social as much as 87%, and finally closed as much as 78% as the most needed field in guidance and counseling services. The results of the study recommend that this research be used as a basis for developing guidance and counseling programs
El papel de los incentivos fiscales a la inversión I+D+i en España
Authors: Palomares Moralles Pascual , Ripoll Alcón Joan 
Published: November 2020

El propósito de este estudio es analizar el papel de los incentivos fiscales a la inversión en investigación, desarrollo e innovación (I+D+i) en España, y en particular, la relevancia de la figura legal Patent Box basada en la cesión de uso de activos intangibles.
Este artículo ilustra, a partir de un análisis comparativo, cómo el esquema Patent Box supone un ahorro fiscal evidente respecto aquella situación en la que no se hace uso del mismo. Este ahorro acaba erigiéndose en un incentivo fiscal efectivo en la promoción de proyectos de innovación empresarial, a diferencia de las deducciones fiscales, cuyo proceloso procedimiento administrativo y la fijación de un límite máximo de reducción de la cuota íntegra del impuesto de sociedades, que se ha revelado insuficiente, han tendido a minar su protagonismo como instrumento de ayuda indirecta a la financiación de la I+D+i.
HUBUNGAN TINGKAT PENGETAHUAN IBU HAMIL DENGAN KEJADIAN HEPATITIS B DI PUSKESMAS BERINGIN KECAMATAN LUBAI KOTA PALEMBANG
Authors: Zulfian Zulfian , Setiawati Octa Reni , Sapitia Anisa 
Published: November 2020

Hepatitis B merupakan salah satu penyakit menular berbahaya yang menyebabkan Kejadian Luar Biasa (KLB) dan kematian. Pemberian Kelengkapan imunisasi dasar pada anak seperti hepatitis B dipengaruhi oleh banyak faktor seperti tingkat pengetahuan dan dukungan keluarga. Penelitian ini merupakan penelitian bersifat deskriptif analitik dengan pendekatan cross-sectional yang dilakukan terhadap 52 responden. Analisis data menggunakan uji Chi-Square dengan program SPSS 16.0. diperoleh ada hubungan yang bermakna antara tingkat pengetahuan dengan kejadian hepatitis B dengan nilai p-value = 0,021. Ada hubungan yang bermakna antara tingkat pengetahuan dengan kejadian hepatitis B (p-value=0.021).
On the Relationship between Investment Risk and Insurance Solvency Optimum
Authors: Szüle Borbála 
Published: November 2020

Solvency is a key issue in the insurance sector. Investments can have significant risks, and a compelling research question is whether the solvency optimizing investment risk corresponds to the lowest possible risk level. This question is even more topical with some interest rates approaching very low levels in many countries. The paper aims to answer this question. Theoretical results suggest that if insurance risk and investment risk are uncorrelated, solvency optimizing investment portfolios with non-risk-free components may exist, and the level of optimal investment risk may inversely depend on the insurance portfolio size.
Gut Microbiota Status in COVID-19: An Unrecognized Player?
Authors: Donati Zeppa Sabrina , Agostini Deborah , Piccoli Giovanni , Stocchi Vilberto , Sestili Piero 
Published: November 2020

Infection with the SARS-CoV-2 virus causes cardiopulmonary and vascular complications, ranging in severity. Understanding the pathogenic mechanisms of the novel SARS-CoV2 infection and progression can provide potential novel targets for its prevention and/or treatment. Virus microbiota reciprocal interactions have been studied in a variety of viral infections. For example, the integrity of Coronavirus particles can be disrupted by surfactin, a bacterial surface molecule that targets other viruses, including that of influenza A. In this light, intestinal microbiota likely influences COVID-19 virulence, while from its side SARS-CoV-2 may affect the intestinal microbiome promoting dysbiosis and other deleterious consequences. Hence, the microbiota pre-existing health status and its alterations in the course of SARS-CoV-2 infection, are likely to play an important, still underscored role in determining individual susceptibility and resilience to COVID-19. Indeed, the vast majority of COVID-19 worst clinical conditions and fatalities develop in subjects with specific risk factors such as aging and the presence of one or more comorbidities, which are intriguingly characterized also by unhealthy microbiome status. Moreover, these comorbidities require complex pharmacological regimens known as “polypharmacy” that may further affect microbiota integrity and worsen the resilience to viral infections. This complex situation may represent a further and underestimated risk with regard to COVID-19 clinical burden for the elderly and comorbid people. Here, we discuss the possible biological, physiopathological, and clinical implications of gut microbiota in COVID-19 and the strategies to improve/maintain its healthy status as a simple and adjunctive strategy to reduce COVID-19 virulence and socio-sanitary burden.
Chemoradiotherapy Is Inferior to Chemotherapy Alone in Adjuvant Setting for Signet Ring Cell Containing Gastric Cancer
Authors: Zhu Yue-Ting , Chen Xin-Zu , Chen Ye , Zhou Yu-Wen , Tang Lian-Sha , Luo De-Yun , Li Qiu , Qiu Meng , Wang Xin , Cao Dan , Yang Yu , Shen Ya-Li , Li Zhi-Ping , Bi Feng , Liu Ji-Yan , Gou Hong-Feng 
Published: November 2020

BackgroundSignet ring cell containing gastric cancer (SRCGC) is a rare subtype of gastric cancer, and its adjuvant therapy is based on general gastric cancer. However, the effectiveness of radiotherapy for those SRCGC patients remains unknown.PurposeThe purpose of the study was to analyze whether the addition of radiotherapy to adjuvant chemotherapy (CT) can benefit survival in resected SRCGC patients.MethodsPatients with SRCGC, who underwent D2 gastrectomy followed by adjuvant chemotherapy or chemoradiotherapy (CRT), were retrospectively collected. According to the proportion of signet ring cells, patients were histologically classified as pure SRCGC (pSRCGC) containing 100% of signet ring cells, mixed SRCGC (mSRCGC) containing &gt;50% of signet ring cells, and contaminated SRCGC (cSRCGC) containing &lt;50% of signet ring cells. Among the 272 patients, 156 were treated by CT alone and 116 by CRT. The primary endpoint was 3-year overall survival rate (3-year OS rate).ResultsWith a median follow-up of 80.5 months, the 3-year OS rate was significantly higher in the CT group (70.5% vs. 58.6%, HR = 0.633, P = 0.017) compared with CRT group. Three independent characteristics were predictive of a poor overall survival: CRT treatment (P = 0.019), tumor size ≥5 cm (P &lt; 0.001), and the presence of vessel invasion (P = 0.009). Subgroup analyses showed CRT significantly impaired prognosis in SRCGC patients in the cSRCGC subset, as well as lesions located in lower-middle sites, subtotal gastrectomy, male, &lt;60 year, and no vessel invasion. Peritoneal was the most common recurrence site in SRCGC patients. The adverse events leukopenia and neutropenia were more common in the CRT group (P = 0.007).ConclusionsAdjuvant chemoradiotherapy was associated with poor survival compared with adjuvant chemotherapy in SRCGC patients with D2 gastrectomy.
ANALISIS TINGKAT PELAYANAN DERMAGA PELABUHAN TANJUNG WANGI KABUPATEN BANYUWANGI
Authors: Amaliyah Rizka Septy , Hasanuddin Akhmad , Kriswardhana Willy 
Published: November 2020

Peningkatan jumlah kunjungan kapal di setiap tahunnya harus diimbangi dengan kinerja pelayanan yang baik. Kinerja pelayanan dari suatu pelabuhan dapat diukur dari sedikitnya waiting time, cepatnya waktu pelayanan pemanduan dan seefektif kapal berada pada dermaga. Tujuan dari penelitian ini adalah untuk mengkaji mengenai kinerja pelayanan Pelabuhan Tanjung Wangi berdasarkan indikator waiting time, approach time, effectife time berbanding berth time yang dibandingkan dengan standar kinerja operasional pelabuhan dan untuk mencegah peningkatan jumlah kunjungan kapal pada tahun yang akan datang perlu dilakukan proyeksi nilai Berth Occupancy Ratio (BOR) jangka panjang menggunakan regresi linier dan memproyeksikan panjang dermaga rencana. Berdasarkan hasil penelitian, pelabuhan tanjung wangi memiliki kinerja yang masih memenuhi nilai standar operasional pelabuhan yaitu (effektif time : berth time) sebesar 60,39% dan nilai maksimum BOR pada tahun 2030 ialah 87,31% dengan panjang dermaga rencana pada tahun 2030 sepanjang 380 meter.
PERANCANGAN APLIKASI MONITORING PENELITIAN DAN PENGABDIAN MASYARAKAT INTERNAL PERGURUAN TINGGI
Authors: Tantrisna Ellen , Manu Gerlan 
Published: November 2020

Penelitian ini bertujuan untuk menghasilkan sebuah sistem yang dapat memanajemen kegiatan Penelitian dan Pengabdian Masyarakat di Lingkup Internal Perguruan Tinggi dengan studi kasus pada Universitas Citra Bangsa. Untuk menjamin tercapainya target penelitian dan pengabdian masyarakat pada suatu Perguruan Tinggi perlu dilakukan monitoring dan evaluasi secara berkesinambungan oleh Lembaga Penelitian, Pengembangan dan Pengabdian kepada Masyarakat (LP3M) atau sejenisnya. Kegiatan monitoring perlu ditunjang dengan adanya aplikasi atau sistem manajemen pada setiap Perguruan Tinggi. Penelitian ini membahas tentang perancangan arsitektur sistem, rancangan basis data, rancangan sistem, serta proses bisnis penggunaan sistem.
An Asymmetric Eclipse Seen toward the Pre-main-sequence Binary System V928 Tau
Authors: van Dam Dirk M. , Kenworthy Matthew A. , David Trevor J. , Mamajek Eric E. , Hillenbrand Lynne A. , Cody Ann Marie , Howard Andrew W. , Isaacson Howard , Ciardi David R. , Rebull Luisa M. , Stauffer John R. , Patel Rahul , Cameron + WASP Collaborators Andrew Collier , Rodriguez Joseph E. , Pojmański Grzegorz , Gonzales Erica J. , Schlieder Joshua E. , Hambsch Franz-Josef , Dufoer Sjoerd , Vanmunster Tonny , Dubois Franky , Vanaverbeke Siegfried , Logie Ludwig , Rau Steve 
Published: November 2020

Abstract
K2 observations of the weak-lined T Tauri binary V928 Tau A and B show the detection of a single, asymmetric eclipse, which may be due to a previously unknown substellar companion eclipsing one component of the binary with an orbital period >66 days. Over an interval of about 9 hr, one component of the binary dims by around 60%, returning to its normal brightness about 5 hr later. From modeling of the eclipse shape, we find evidence that the eclipsing companion may be surrounded by a disk or a vast ring system. The modeled disk has a radius of 0.9923 ± 0.0005 R
*, with an inclination of 56.°78 ± 0.°03, a tilt of 41.°22 ± 0.°05, an impact parameter of −0.2506 ± 0.0002 R
*, and an opacity of 1.00. The occulting disk must also move at a transverse velocity of 6.637 ± 0.002 R
* day−1, which, depending on whether it orbits V928 Tau A or B, corresponds to approximately 73.53 or 69.26 km s−1. A search in ground-based archival data reveals additional dimming events, some of which suggest periodicity, but no unambiguous period associated with the eclipse observed by K2. We present a new epoch of astrometry that is used to further refine the orbit of the binary, presenting a new lower bound of 67 yr, and constraints on the possible orbital periods of the eclipsing companion. The binary is also separated by 18″ (∼2250 au) from the lower-mass CFHT-BD-Tau 7, which is likely associated with V928 Tau A and B. We also present new high-dispersion optical spectroscopy that we use to characterize the unresolved stellar binary.
Planetary Refractory Composition and Volatile Accretion into Gas Giants in the Protoplanetary Disks of the Sun and WASP-12
Authors: Pekmezci G. S. , Mousis O. , Lunine J. I. 
Published: November 2020

Abstract
We present a detailed theoretical exploration of the refractory compositions and volatile enrichments of planets forming in protoplanetary disks with solar-like conditions. The two cases of the Sun and WASP-12 are studied due to the availability of spectral measurements and their known planets. The distribution throughout their disks of solid compounds with a wide range of volatilities is computed by a comprehensive chemical thermodynamics code. After the calculation of refractory compounds down to the water snowline, the compositional distributions are documented for planets generated in certain locations of protoplanetary disks depending on thermodynamic conditions. These results are referred to proposed bulk compositions for solar terrestrial planets, and for the core of the hot Jupiter WASP-12b. The material left over after the formation of rocky components is collected and treated in calculations to determine the abundances of fundamental volatile molecules in the outer regions of the disks. The distributions of planetesimal volatile composition are then altered for four different cases of the carbon-to-oxygen ratios, and for oxidizing and reducing conditions, in order to adjust the best fit for the accretion zone of Jupiter and WASP-12b. We compare the Jovian results to in situ atmospheric measurements from Jupiter’s atmosphere. Overall, this study proposes a holistic approach to estimate possible planetary interior and envelope compositions from hot toward cold disk zones, along with the mass of planetesimals accreted into the envelopes of gas giants.
Gaps and Rings in Protoplanetary Disks with Realistic Thermodynamics: The Critical Role of In-plane Radiation Transport
Authors: Miranda Ryan , Rafikov Roman R. 
Published: November 2020

Abstract
Many protoplanetary disks exhibit annular gaps in dust emission, which may be produced by planets. Simulations of planet–disk interaction aimed at interpreting these observations often treat the disk thermodynamics in an overly simplified manner, which does not properly capture the dynamics of planet-driven density waves driving gap formation. Here we explore substructure formation in disks using analytical calculations and hydrodynamical simulations that include a physically motivated prescription for radiative effects associated with planet-induced density waves. For the first time, our treatment accounts not only for cooling from the disk surface but also for radiation transport along the disk midplane. We show that this in-plane cooling, with a characteristic timescale typically an order of magnitude shorter than the one due to surface cooling, plays a critical role in density wave propagation and dissipation (we provide a simple estimate of this timescale). We also show that viscosity, at the levels expected in protoplanetary disks (

), has a negligible effect on density wave dynamics. Using synthetic maps of dust continuum emission, we find that the multiplicity and shape of the gaps produced by planets are sensitive to the physical parameters—disk temperature, mass, and opacity—that determine the damping of density waves. Planets orbiting at

produce the most diverse variety of gap/ring structures, although significant variation is also found for planets at

. By improving the treatment of the physics governing planet–disk coupling, our results present new ways of probing the planetary interpretation of annular substructures in disks.
A Stream of Hypervelocity Stars from the Galactic Center
Authors: Generozov Aleksey 
Published: November 2020

Abstract
Recent observations have found a 1700 km s−1 star [S5-HVS1] that was ejected from the Galactic center approximately five million years ago. This star was likely produced by the tidal disruption of a binary. In particular, the Galactic center contains a few million year old stellar disk that could excite binaries to nearly radial orbits via a secular gravitational instability. Such binaries would be disrupted by the central supermassive black hole, and would also explain the observed cluster of B stars ∼0.01 pc from the Galactic center. In this paper we predict S5-HVS1 is part of a larger stream, and use observationally motivated N-body simulations to predict its spatial and velocity distributions.
Inverse Compton Cooling in the Coronae of Simulated Black Hole Accretion Flows
Authors: Kinch Brooks E. , Noble Scott C. , Schnittman Jeremy D. , Krolik Julian H. 
Published: November 2020

Abstract
We present a formulation for a local cooling function to be employed in the diffuse, hot corona region of 3D GRMHD simulations of accreting black holes. This new cooling function calculates the cooling rate due to inverse Compton scattering by considering the relevant microphysics in each cell in the corona and approximating the radiation energy density and Compton temperature thereby integrating over the thermal seed photon flux from the disk surface. The method either assumes the ion and electron temperatures are equal (1T) or calculates them separately (2T) using an instantaneous equilibrium approach predicated on the actual relevant rate equations (Coulomb and Compton). The method is shown to be consistent with a more detailed ray-tracing calculation where the bulk of the cooling occurs, but is substantially less costly to perform. As an example, we apply these methods to a harm3d simulation of a 10M
⊙, non-spinning black hole, accreting at nominally 1% the Eddington value. This new approach leads to radiative efficiency values ≃65% above Novikov–Thorne, with a larger fraction of total cooling in the corona as compared to simulations performed using the original target-temperature cooling function. Time-averaged post-processing reveals that the continuum spectral observations predicted from these simulations are qualitatively similar to actual X-ray binary data, especially so for the 1T approach, which yields a harder power-law component (Γ = 2.25) compared to the 2T version (Γ = 2.53).
Element Abundances in the Unshocked Ejecta of Cassiopeia A
Authors: Laming J. Martin , Temim Tea 
Published: November 2020

Abstract
We analyze and model the infrared spectrum of the Cassiopeia A supernova remnant with the aim of determining the masses of various elements in the unshocked ejecta. In this way, we complement the survey of the X-ray-emitting ejecta to provide a complete census of the elemental composition of the Cas A ejecta. We calculate photoionization–recombination equilibria to determine the ionization balance of various elements in the ejecta as a function of density using the X-ray and UV emission from the forward and reverse shocks as the ionizing radiation. With the assumption that all emission lines are principally excited at the ejecta density that maximizes their emission, we can convert observed line intensities into element masses. We find that the majority of the ∼3 M
⊙ ejecta have already been through the reverse shock and are seen today in X-rays. A minority, ∼0.47 ± 0.05 M
⊙, with uncertainties quoted here coming from the data fitting procedure only, are still expanding inside the reverse shock and emitting in the infrared. This component is comprised mainly of O, Si, and S, with no Fe readily detectable. Incorporating uncertainties estimated to come from our modeling, we quote

M
⊙. We speculate that up to a further 0.07 M
⊙ of Fe may be present in diffuse gas in the inner ejecta, depending on the Fe charge state.
Le droit administratif camerounais « postcolonial » en rupture avec le modèle français inspirateur
Authors: Foumena Gaëtan Thierry 
Published: November 2020

Le Cameroun ancienne colonie allemande, a été placé par le système des Nations unies, sous administration de la France et de la Grande Bretagne. La partie confiée à la France a été, non seulement le cadre d’application du droit administratif d’origine française, mais surtout, le lieu d’éclosion d’un droit administratif « intranéen » ; en raison de l’application, dès le départ, du principe de la spécialité législative. C’est la raison pour laquelle, il existe une dichotomie entre les droits administratifs français et camerounais. Cette dichotomie, depuis l’accession du Cameroun à l’indépendance, est davantage consolidée, et, renforce l’idée de l’autonomie et l’originalité des droits africains par rapport au droit français.