bluuebunny/crossref_metadata_2025_split huggingface dataset:
Nilai Pendidikan Agama Hindu Dalam Lontar Siwa Sasana
Authors: Eka Suadnyana Ida Bagus Putu , Ariyasa Darmawan I Putu 
Published: June 2020

Hinduism in addition to giving teachings also guides its people to achieve happiness and harmonize their lives physically and spiritually. Efforts to maintain the preservation of Religion can be done through strengthening education in the field of religion. For people in Bali this is the basic capital as a mental and spiritual driving force and is a guide, guide and impetus in humans to achieve a better and perfect quality of life. The teachings of Hinduism are based on the Vedic scriptures, but also in secondary books, one of which is the ancient manuscripts in the form of Lontar. Dealing with this, the author intends to examine in depth in terms of the value of Hindu religious education for a lontar, namely lontar "Shiva Sasana" which is a religious literary work that is currently only in demand by a small portion of the community or less attention from the younger generation of Hindus. Theories used to solve research problems are convergence theory and value theory. This research is in the form of a qualitative design with data collected with literature study techniques and interpretive methods. After the data collected the data were analyzed with descriptive analysis techniques. The teachings contained in the Lontar Shiva Sasana based on the writer's findings include the teachings of Shivaism and the teachings of the Trikaya Parisudha and the values ​​contained in the Lontar Shiva Sasana include the ethical values ​​and devotional values.
PEMANFAATAN DAUN Theprosia vogelii DALAM PENGENDALIAN HAMA Sitophilus zeamays (Coleoptera : Curculionidae)
Authors: Puu Yustina Maria Silvia Wonga 
Published: June 2020

Sitophilus zeamays (Coleoptera: Curculionidae) is one of the pests that damage the corn kernels in storage so that it is damaged into corn powder. Control efforts that can be done is to use plant-based insecticides from Theprosia vogelii plants that contain rotenoid compounds so that they can cause pest mortality. The purpose of this study was to determine the effectiveness of Theprosia vogelli leaves in controlling Sitophilus zeamays in storage. The study was conducted at the Laboratory of the Faculty of Agriculture, University of Flores. The design used was a Completely Randomized Design (CRD) consisting of 5 treatments namely T0 = 0 gram (control), T1 (4 gram T. vogelii leaf powder), T2 (8 gram T. vogelii leaf powder), T3 (12 grams T. vogelii leaf powder) and T4 (16 grams of T. vogelii leaf powder). The observation variable was the mortality of the Sitophilus zeamays pest.
The results showed that a dose of 16 grams of T. vogelii leaf powder caused a mortality of S. zeamays of 96.67%.
KÂSIM-I ENVÂR’IN ENÎSÜ’L-ÂRİFÎN ADLI MESNEVİSİNDE MUM, PERVÂNE VE ATEŞ ARASINDAKİ MÜNAZARA
Authors: KOPUZ ÇETİNKAYA Fatma 
Published: June 2020

Şem‘ ve pervane klasik İran edebiyatının en sık kullanılan
mazmunları arasında yer almaktadır. Söz konusu mazmunlar hem klasik hem çağdaş
İran edebiyatında şair ve yazarlar için uzun yıllar ilham kaynağı olmuştur. Klasik
İran edebiyatı VII/XIV yüzyıl önemli mutasavvıf şairleri arasında yer alan
Kâsım-ı Envâr da külliyatında kısa da olsa şem‘ ve pervâne hikâyesine yer
vermiştir. Bu çalışmada, klasik şem‘ ve pervâne hikâyesinin yapısına yakın
ancak içinde farklılıklar da barındıran bu hikâye ele alınmıştır. Kısaca
yazarın hayatı, etkilendiği kişiler, eseri ve dili hakkında bilgi aktarıldıktan
sonra söz konusu hikâyenin Farsça metni ve Türkçeye çevirisi verilmiştir. Diğer
şem‘ ve pervâne hikâyelerine göre tespit edilen farklılık belirlenip
açıklanmıştır.
Elemental Abundances in M31: Iron and Alpha Element Abundances in M31’s Outer Halo*
Authors: Gilbert Karoline M. , Wojno Jennifer , Kirby Evan N. , Escala Ivanna , Beaton Rachael L. , Guhathakurta Puragra , Majewski Steven R. 
Published: June 2020

Abstract
We present [Fe/H] and [α/Fe] abundances, derived using spectral synthesis techniques, for stars in M31’s outer stellar halo. The 21 [Fe/H] measurements and 7 [α/Fe] measurements are drawn from fields ranging from 43 to 165 kpc in projected distance from M31. We combine our measurements with existing literature measurements, and compare the resulting sample of 23 stars with [Fe/H] and 9 stars with [α/Fe] measurements in M31’s outer halo with [α/Fe] and [Fe/H] measurements, also derived from spectral synthesis, in M31’s inner stellar halo (r < 26 kpc) and dSph galaxies. The stars in M31’s outer halo have [α/Fe] patterns that are consistent with the largest of M31’s dSph satellites (And I and And VII). These abundances provide tentative evidence that the [α/Fe] abundances of stars in M31’s outer halo are more similar to the abundances of Milky Way halo stars than to the abundances of stars in M31’s inner halo. We also compare the spectral synthesis–based [Fe/H] measurements of stars in M31’s halo with previous photometric [Fe/H] estimates, as a function of projected distance from M31. The spectral synthesis–based [Fe/H] measurements are consistent with a large-scale metallicity gradient previously observed in M31’s stellar halo to projected distances as large as 100 kpc.
Two Strengths of Ordinary Chondritic Meteoroids as Derived from Their Atmospheric Fragmentation Modeling
Authors: Borovička Jiří , Spurný Pavel , Shrbený Lukáš 
Published: June 2020

Abstract
The internal structure and strength of small asteroids and large meteoroids is poorly known. Observation of bright fireballs in the Earth’s atmosphere can explore meteoroid structure by studying meteoroid fragmentation during the flight. Earlier evaluations showed that the meteoroid’s strength is significantly lower than that of the recovered meteorites. We present a detailed study of atmospheric fragmentation of seven meteorite falls, all ordinary chondrites, and 14 other fireballs, where meteorite fall was predicted but the meteorites, probably also ordinary chondrites, were not recovered. All observations were made by the autonomous observatories of the European Fireball Network and include detailed radiometric light curves. A model, called the semiempirical fragmentation model, was developed to fit the light curves and decelerations. Videos showing individual fragments were available in some cases. The results demonstrated that meteoroids do not fragment randomly but in two distinct phases. The first phase typically corresponds to low strengths of 0.04–0.12 MPa. In two-thirds of cases, the first phase was catastrophic or nearly catastrophic with at least 40% of mass lost. The second phase corresponds to 0.9–5 MPa for confirmed meteorite falls and somewhat lower strengths, from about 0.5 MPa, for smaller meteoroids. All of these strengths are lower than the tensile strengths of ordinary chondritic meteorites cited in the literature, 20–40 MPa. We interpret the second phase as being due to cracks in meteoroids and the first phase as a separation of weakly cemented fragments, which reaccumulated at the surfaces of asteroids after asteroid collisions.
The Stellar Velocity Distribution Function in the Milky Way Galaxy
Authors: Anguiano Borja , Majewski Steven R. , Hayes Christian R. , Prieto Carlos Allende , Cheng Xinlun , Bidin Christian Moni , Beaton Rachael L. , Beers Timothy C. , Minniti Dante 
Published: June 2020

Abstract
The stellar velocity distribution function in the solar vicinity is reexamined using data from the Sloan Digital Sky Survey Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey’s DR16 and Gaia DR2. By exploiting APOGEE’s ability to chemically discriminate with great reliability the thin-disk, thick-disk, and (accreted) halo populations, we can, for the first time, derive the three-dimensional velocity distribution functions (DFs) for these chemically separated populations. We employ this smaller but more data-rich APOGEE+Gaia sample to build a data-driven model of the local stellar population velocity DFs and use these as basis vectors for assessing the relative density proportions of these populations over the 5 < R < 12 kpc and −1.5 < z < 2.5 kpc range as derived from the larger, more complete (i.e., all-sky, magnitude-limited) Gaia database. We find that 81.9% ± 3.1% of the objects in the selected Gaia data set are thin-disk stars, 16.6% ± 3.2% are thick-disk stars, and 1.5% ± 0.1% belong to the Milky Way stellar halo. We also find the local thick-to-thin-disk density normalization to be ρ

T
(R
⊙)/ρ

t
(R
⊙) = 2.1% ± 0.2%, a result consistent with, but determined in a completely different way from, typical star-count/density analyses. Using the same methodology, the local halo-to-disk-density normalization is found to be ρ

H
(R
⊙)/(ρ

T
(R
⊙) + ρ

t
(R
⊙)) = 1.2% ± 0.6%, a value that may be inflated due to the chemical overlap of halo and metal-weak thick-disk stars.
The Semiforbidden C iii] λ1909 Emission in the Rest-ultraviolet Spectra of Green Pea Galaxies
Authors: Ravindranath Swara , Monroe TalaWanda , Jaskot Anne , Ferguson Henry C. , Tumlinson Jason 
Published: June 2020

Abstract
We used the Space Telescope Imaging Spectrograph on the Hubble Space Telescope (HST) to observe the semiforbidden C iii] λλ1907, 1909 doublet emission in green pea galaxies at 0.13 ≤ z ≤ 0.3. We detect C iii] emission in 7/10 galaxies with C iii] equivalent widths (EWs) that range from 2 to 10 Å, confirming that C iii] emission is almost ubiquitous in low-mass, low-metallicity (12+log(O/H) < 8.4) galaxies that are characterized by strong optical [O iii] λ5007 emission. The composite UV spectrum shows evidence for the He ii
λ1640 emission line and interstellar absorption features (e.g., C iv
λλ1548, 1550, Al iii
λλ1854, 1862). We do not detect the O iii] λλ1661, 1666 emission with >3σ significance. The observed C iii] emission line strengths are consistent with the predictions from photoionization models that incorporate the effects of binary stellar evolution with young stellar ages ≤3–5 Myr and high ionization parameters (log U > −2). The hard ionizing radiation from young massive stars and high nebular temperatures at low metallicities can account for the observed high EWs of C iii] λ1909 and [O iii] λ5007 emission lines. Some of the star-forming galaxies at high redshift and local blue compact dwarf galaxies show offsets from the EW(C iii]) versus EW([O iii]) model grids, indicating an additional contribution to the continuum emission from composite stellar populations or different C/O abundances, nebular temperatures, and electron densities than assumed in the photoionization models. The green pea galaxies do not show a significant correlation between the Lyα and C iii] EWs, and the observed scatter is likely due to the variations in the optical depth of Lyα to the neutral gas. Green pea galaxies are likely to be density-bounded, and we examined the dependence of C iii] emission on the Lyman continuum optical depth. The potential LyC leaker galaxies in our sample have high C iii] EWs that can only be reproduced by starburst ages as young as <3 Myr and harder ionizing spectra than the nonleakers. Among the galaxies with similar metallicities and ionization parameters, the C iii] EW appears to be stronger for those with higher optical depth to LyC, as expected from the photoionization models. There are various factors that affect the C iii] emission line strengths, and further investigation of a larger sample of C iii] emitters is necessary to calibrate the dependence of C iii] emission on the escape of LyC radiation and enable application of the C iii] diagnostics to galaxies in the reionization epoch.
Laboratory Study of Bilateral Supernova Remnants and Continuous MHD Shocks
Authors: Mabey P. , Albertazzi B. , Rigon G. , Marquès J.-R. , Palmer C. A. J. , Topp-Mugglestone J. , Perez-Martin P. , Kroll F. , Brack F.-E. , Cowan T. E. , Schramm U. , Falk K. , Gregori G. , Falize E. , Koenig M. 
Published: June 2020

Abstract
Many supernova remnants (SNRs), such as G296.5+10.0, exhibit an axisymmetric or barrel shape. Such morphologies have previously been linked to the direction of the Galactic magnetic field, although this remains uncertain. These SNRs generate magnetohydrodynamic shocks in the interstellar medium, modifying its physical and chemical properties. The ability to study these shocks through observations is difficult due to the small spatial scales involved. In order to answer these questions, we perform a scaled laboratory experiment in which a laser-generated blast wave expands under the influence of a uniform magnetic field. The blast wave exhibits a spheroidal shape, whose major axis is aligned with the magnetic field, in addition to a more continuous shock front. The implications of our results are discussed in the context of astrophysical systems.
Ca hnk: The Calcium-rich Transient Supernova 2016hnk from a Helium Shell Detonation of a Sub-Chandrasekhar White Dwarf
Authors: Jacobson-Galán Wynn V. , Polin Abigail , Foley Ryan J. , Dimitriadis Georgios , Kilpatrick Charles D. , Margutti Raffaella , Coulter David A. , Jha Saurabh W. , Jones David O. , Kirshner Robert P. , Pan Yen-Chen , Piro Anthony L. , Rest Armin , Rojas-Bravo César 
Published: June 2020

Abstract
We present observations and modeling of SN 2016hnk, a Ca-rich supernova (SN) that is consistent with being the result of a He-shell double-detonation explosion of a C/O white dwarf. We find that SN 2016hnk is intrinsically red relative to typical thermonuclear SNe and has a relatively low peak luminosity ( M

B
= −15.4 mag), setting it apart from low-luminosity SNe Ia. SN 2016hnk has a fast-rising light curve that is consistent with other Ca-rich transients (t

r
= 15 days). We determine that SN 2016hnk produced 0.03 ± 0.01 M
⊙ of 56Ni and 0.9 ± 0.3 M
⊙ of ejecta. The photospheric spectra show strong, high-velocity Ca ii absorption and significant line blanketing at λ < 5000 Å, making it distinct from typical (SN 2005E-like) Ca-rich SNe. SN 2016hnk is remarkably similar to SN 2018byg, which was modeled as a He-shell double-detonation explosion. We demonstrate that the spectra and light curves of SN 2016hnk are well modeled by the detonation of a 0.02

helium shell on the surface of a 0.85

C/O white dwarf. This analysis highlights the second observed case of a He-shell double-detonation and suggests a specific thermonuclear explosion that is physically distinct from SNe that are defined simply by their low luminosities and strong [Ca ii] emission.
Stratospheric Transparency and Color of the Total Lunar Eclipse of 1794 February 14 Observed by Jovellanos from Gijón (Spain)
Authors: Vaquero José M. 
Published: June 2020

Abstract
Gaspar Melchor de Jovellanos is the major figure of the Age of Enlightenment in Spain. He observed the total lunar eclipse of 1794 February 14 from Gijón (north of Spain). Jovellanos described the moon color as “glowing iron.” It indicates that the stratosphere around 1794 seems to have been undisturbed volcanically as previous estimates indicate.
Breakthrough Listen Search for Technosignatures toward the Kepler-160 System
Authors: Perez Karen , Brzycki Bryan , Gajjar Vishal , Isaacson Howard , Siemion Andrew , Croft Steve , DeBoer David , Lebofsky Matt , MacMahon David H. E. , Price Danny C. , Sheikh Sofia , Drew Jamie , Worden S. Pete 
Published: June 2020

Abstract
We have conducted a search for artificial radio emission associated with the Kepler-160 system following the report of the discovery of the Earth-like planet candidate KOI-456.04 on 2020 June 4 (Heller et al. 2020). Our search targeted both narrowband (2.97 Hz) drifting (±4 Hz s−1) and wideband pulsed (5 ms at all bandwidths) artificially dispersed technosignatures using the turboSETI (Enriquez et al. 2017) and SPANDAK (V. Gajjar et al. 2020, in preparation) pipelines, respectively, from 1 to 8 GHz. No candidates were identified above an upper limit Equivalent Isotropic Radiated Power of 5.9 × 1014 W for narrowband emission and 7.3 × 1012 W for wideband emission. Here we briefly describe our observations and data reduction procedure.
The Undercommons : extraits
Authors: Harney Stefano , Moten Fred , Deep L  , Citton Yves 
Published: June 2020

Cet article propose une sélection de bonnes feuilles du livre de 2013 The Undercommons , actuellement en voie de traduction pour une publication française en 2021. Y sont abordés les thèmes de la politique « encerclée » ( surrounded ), de la gouvernance, du planning et de la policy , de la logistique, ainsi que de ce qui fait de l’étude consacrée aux undercommons une philosophie du toucher.
Accompagner l’habitat des personnes en souffrance psychique : quelles organisations pour quelle inclusion ?
Authors: Henckes Nicolas 
Published: June 2020

L’habitat inclusif cherche à répondre à un enjeu fondamental dans les politiques actuelles d’accompagnement de la souffrance psychique, de la maladie mentale et du handicap psychique : favoriser la pleine participation sociale des personnes concernées. Il s’adresse en particulier à une demande nouvelle exprimée par les personnes comme par l’ensemble de la société : satisfaire le droit à un logement personnel. Jusqu’à quel point le dispositif effectivement déployé sur les territoires est-il armé pour cela ? Ce sont quelques éléments de réponse à cette question que voudrait apporter cet article. Il s’appuie pour cela sur une réflexion sur les organisations à l’œuvre pour délivrer les services.
Présentation du programme de formation aux premiers secours en santé mentale (PSSM)
Authors: Marescaux Jacques 
Published: June 2020

Le programme de formation aux PSSM est une adaptation à la France d’un programme créé en Australie au début des années 2000: le Mental Health First Aid (MHFA) par un universitaire, le Pr Tony Jorn et une éducatrice et usagère des services de psychiatrie, Betty Kitchener. Leur objectif : contribuer à la lutte contre la stigmatisation des personnes souffrant de troubles psychiques et de leur entourage, améliorer l’accès aux soins en formant des secouristes en santé mentale - et non des soignants -, sur le modèle général du secourisme qui a fait ses preuves.
Sociologie de la traduction
Authors: Gouanvic Jean-Marc 
Published: June 2020

Cet essai a pour ambition d’édifier une sociologie de la traduction à partir des idées de Pierre Bourdieu sur la sociologie de la culture. Est analysée la science-fiction telle qu’elle s’est implantée en France dans les années 1950 par l’action des agents Boris Vian, Raymond Queneau et Michel Pilotin. Issue du courant américain des années 1920, la science-fiction est en elle-même un phénomène de traduction, ayant émergé sous l’impulsion du Luxembourgeois Hugo Gernsback du terreau de Jules Verne et accessoirement H. G. Wells et Edgar Poe. La réception d’H. G. Wells au Mercure de France et dans la NRF (avant la première guerre mondiale) est d’abord présentée, ainsi que des tentatives sans lendemains avant la Seconde Guerre mondiale. Ensuite, est étudiée dans le détail la grande tradition de la science-fiction qui, par la traduction, a pris racine durablement dans la France de l’après-Guerre : la traduction et ses agents, la traduction au Rayon Fantastique (Hachette-Gallimard), Boris Vian traducteur d’Alfred E. van Vogt, la traduction de l’onomastique dans la revue Galaxie. Enfin, en conclusion, l’auteur procède à un exercice de double réflexivité traductologique. L’essai se clôt sur des annexes qui fournissent des bibliographies de traducteurs (livres traduits).
Peace Building and Conflict Transformation in Nigeria: The Role of De Norsemen Kclub Incorporated in an Environmentally Challenged Society, 1982-2018
Authors: Amiara Solomon Amiara , Odii Peace Udoamaka , Nwobi Obiora I. 
Published: June 2020

This paper examined the role of De Norsemen Kclub Incorporated in peace building and conflict transformation in an environmentally challenged society like Nigeria. Over the years, environmental crisis has become a re-occurring decimal that threatens the sovereignty of Nigeria with the civil societies, religious leaders and nongovernmental organisations seeking to proffer solutions. However, arguments have raged on whether or not De Norsemen has the capacity to ensure peace and resolve conflict in a volatile country like Nigeria. Some are of the opinion that De Norsemen Kclub lacks the legitimate powers to maintain peace because of their inclination to school cult gangs and therefore, they should be proscribed. Other side of the argument opines that De Norsemen Kclub Incorporated are legitimate organization registered under the Corporate Affairs Commission whose motto is “service to humanity” and since conflict is a threat to human security, they therefore have the powers to advocate for peace. Against this background, this paper argued that peace building and conflict transformation are concepts in conflict resolution strategies that are often taken to ensure that conflicts in the society are deescalated and reduced to the barest minimal. The position of the paper is that De Norsemen Kclub is not associated with any form of cultism, they operate under the sovereign constitution of Nigeria and has right like other nongovernmental organisations to make peace and resolve conflict in Nigeria.
Key Words: Peace building, conflict transformation, De Norsemen, environment, society
A Tortuous Trajectory: Nigerian Foreign Policy under Military Rule, 1985 – 1999
Authors: Osayande Emmanuel 
Published: June 2020

This article critically examined the complexities that abound in Nigeria’s Foreign Policy under the final three military administrations of Generals Ibrahim Babangida, Sani Abacha, and Abdulsalami Abubakar, before the transition to democratic rule in 1999. It adopted a novel approach by identifying and intricately examining a distinct pattern of contortion evinced in Nigeria’s foreign policy during this epoch. It contended that although Nigeria’s foreign policy had historically been somewhat knotty at varying points in time, this period in its foreign policy and external relations was especially marked by tortuousness and a somewhat back and forth agenda. This began in 1985 with the Babangida administration, whose foreign policy posture initially seemed commendable, only for political debacles to mar it. An exacerbation of this downslide in foreign policy occurred under the Abacha regime, whereby the country obtained pariah status among the comity of nations. Subsequently, a revitalisation occurred under General Abubakar, who deviated from what had become the status quo, reinventing Nigeria’s external image and foreign policy position through his ‘restoration campaign.’ More so, following David Gray’s behavioural theory of foreign policy, this study examined how the behavioural patterns and aspirations of a minuscule cadre of decision-makers deeply affected Nigeria’s foreign policy formulation and implementation during the period under study. The findings of this study include national interest, the crux of any foreign policy, sometimes misaligned with domestic realities. In this regard, this study demonstrated how successive Nigerian governments replicated a ‘munificent’, ‘Santa Claus’ foreign policy which alienated key local developments such as economic hardship, and contributed to the tortuousness that the country’s foreign policy experienced during an era of military dictatorships in the late twentieth century. Through its findings, the study concluded by proffering recommendations to improve the country’s foreign policy, better advance her national interests– which ought to comprise the crux of her foreign policy objectives, – and help in eschewing a recurrence of past ineptitudes and errors.
Key Words: Foreign policy, military rule, Nigeria, behavioural theory,