bluuebunny/crossref_metadata_2025_split huggingface dataset:
Perceptions of Spirituality of Yoga in Minnesota
Authors: Ness Anne , Briles Karen , Mellang Patricia 
Published: February 2020

The purpose of this study was to describe the perception of Yoga spirituality in Minnesota. In this phenomenological study, in-depth semi-structured interviews were conducted with eleven Yoga instructors about the traditional spirituality of Yoga. Although they all perceived that Yoga is traditionally spiritual, many said the spiritual aspect was not well presented in most classes, if at all. Most perceived that spiritual opening occurs with asana practice, and that many benefits were experienced when traditional spiritual Yoga was practiced. Barriers to teaching and learning the traditional spirituality of Yoga were: the fear of being exploited by a guru, the fear of non-Christian spirituality, prohibitions against spiritual talk in public institutions, lack of understanding because of insufficient training, and cultural colonization of Yoga. The implications of these findings are that, although non-spiritual yoga can be a bridge to yoga’s benefits, more training for instructors and respect for Indian culture are needed. More awareness of the spiritual aspect of Yoga and more study of its practice are needed.
El americanismo de Rafael Altamira como puente de una revolución intelectual
Authors: Alfaro-Mancera Ricardo Andrés 
Published: February 2020

Este artículo explora los aportes del historiador alicantino Rafael Altamira y Crevea, quien en 1909 fue comisionado por la Universidad de Oviedo, institución en la que era catedrático, para realizar un viaje por instituciones educativas de Argentina, Chile, México, Perú, Cuba, Uruguay y Estados Unidos con el claro objetivo de restablecer las relaciones académicas e intelectuales entre América y España. Se hace hincapiéen la trascendencia de esta visita, que se reflejó en la buena aceptación de las ideas del intelectual por parte de la opinión pública, la implementación de mecanismos para el intercambio de recursos humanos y materiales entre ambos continentes y su influencia en la construcción del proyecto de la Universidad Nacional de México.
PERAN MODERASI DISIPLIN KERJA PADA PENGARUH KEPEMIMPINAN TERHADAP PRODUKTIVITAS KERJA KARYAWAN PERBANKAN SYARIAH DI MAKASSAR
Authors: Jumady Edy 
Published: February 2020

This study aims to examine the influence of leadership on employees work activity moderated work discipline at Islamic banking in Makassar. Data collection uses the primary data obtained from questionnaires using technitk proportionated random sampling. The population is all 162 permanent employees from 11 Islamic banks in Makassar City, while the sample taken is 62 respondents. The results of the questionnaire have been tested for validity and reliability. Methoddata analysis using SEM technique (Sturctural equation modeling) assisted with WarphPLS Ver.5.0.
The results of this study indicate that the hypothesis of leadership is accepted in part because it shows the result of hypothesis test that negative and significant. This means that influential negative leadership and significant to employees work activity. then result research on work discipline shows that the hypothesis is accepted because it shows results a positive and significant hypothesis. this means that positive discipline work is positive and significant to employees work activity. While the results of research on discipline work as the strengthening variable indicates that the hypothesis is accepted as it shows the results a positive and significant hypothesis. This means that the work discipline variable can strengthen variable leadership on employees work activity.

Keywords: Leadership, Work Discipline, Employee Performance, Islamic Banking
PELAKSANAAN PENDAFTARAN TANAH SISTEMATIS LENGKAP (PTSL) BERDASARKAN PERATURAN MENTERI AGRARIA DAN TATA RUANG/KEPALA BADAN PERTANAHAN NASIONAL NOMOR 6 TAHUN 2018 DI BPN KOTA YOGYAKARTA
Authors: Suyikati Suyikati 
Published: February 2020

Penelitian ini bertujuan untuk mengetahui bagaimana Pelaksanaan Pendaftaran Tanah Sistematis Lengkap (PTSL) dilaksanakan berdasarkan Peraturan Menteri Agraria dan Tata Ruang/Kepala Badan Pertanahan Nasional Nomor 6 Tahun 2018 di BPN Kota Yogyakarta. Penelitian Tentang Pelaksanaan Pendaftaran Tanah Sistematis Lengkap (PTSL) berdasarkan Peraturan Menteri Agraria dan Tata Ruang/ Kepala Badan Pertanahan Nasional Nomor 6 Tahun 2018 di BPN Kota Yogyakarta merupakan penelitian Yuridis Empiris yaitu penelitian yang pada awalnya meneliti data sekunder untuk kemudian dilanjutkan dengan penelitian terhadap data primer di lapangan atau terhadap masyarakat, selanjutnya data yang telah diperoleh dianalisis oleh Peneliti dengan Metode Deskriptif Analitis.Hasil penelitian menunjukkan bahwa Pelaksanaan Pendaftaran Tanah Sistematis Lengkap (PTSL) yang dilaksanakan di BPN Kota Yogyakarta sudah sesuai dengan ketentuan yang terdapat dalam Peraturan Menteri Agraria dan Tata Ruang/Kepala Badan Pertanahan Nasional Nomor 6 Tahun 2018 dengan realisai fisik sebanyak 11,959 bidang tanah dan yang berhasil di terbitkan sertifikat sebanyak 856 bidang tanah, selain itu terdapat produk PTSL tahun 2017 yang naik Kluster dari Kluster 3 ke Kluster 1 sebanyak 94 bidang.
Confirmation of WASP-107b’s Extended Helium Atmosphere with Keck II/NIRSPEC
Authors: Kirk James , Alam Munazza K. , López-Morales Mercedes , Zeng Li 
Published: February 2020

Abstract
We present the detection of helium in the extended atmosphere of the sub-Saturn WASP-107b using high-resolution (R ≈ 25,000) near-infrared spectra from Keck II/Near Infrared Echelle Spectrograph (NIRSPEC). We find peak excess absorption of 7.26% ± 0.24% (30σ) centered on the He i triplet at 10833 Å. The amplitude and shape of the helium absorption profile is in excellent agreement with previous observations of escaping helium from this planet made by CARMENES and the Hubble Space Telescope. This suggests there is no significant temporal variation in the signature of escaping helium from the planet over a two year baseline. This result demonstrates Keck II/NIRSPEC’s ability to detect atmospheric escape in exoplanets, making it a useful instrument to further our understanding of the evaporation of exoplanetary atmospheres via ground-based observations of He i.
OGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf?
Authors: Zhang Xiangyu , Zang Weicheng , Udalski Andrzej , Gould Andrew , Ryu Yoon-Hyun , Wang Tianshu , Yang Hongjing , Mao Shude ,   (Leading Authors), Mróz Przemek , Skowron Jan , Poleski Radoslaw , Szymański Michał K. , Soszyński Igor , Pietrukowicz Paweł , Kozłowski Szymon , Ulaczyk Krzysztof ,   (THE OGLE COLLABORATION), Albrow Michael D. , Chung Sun-Ju , Han Cheongho , Hwang Kyu-Ha , Jung Youn Kil , Shin In-Gu , Shvartzvald Yossi , Yee Jennifer C. , Zhu Wei , Cha Sang-Mok , Kim Dong-Jin , Kim Hyoun-Woo , Kim Seung-Lee , Lee Chung-Uk , Lee Dong-Joo , Lee Yongseok , Park Byeong-Gon , Pogge Richard W. ,   (The KMTNet Collaboration)
Published: February 2020

Abstract
We report the discovery and the analysis of the short (

days) planetary microlensing event, OGLE-2015-BLG-1771. The event was discovered by the Optical Gravitational Lensing Experiment, and the planetary anomaly (at I ∼ 19) was captured by The Korea Microlensing Telescope Network. The event has three surviving planetary models that explain the observed light curves, with planet-host mass ratio q ∼ 5.4 × 10−3, 4.5 × 10−3 and 4.5 × 10−2, respectively. The first model is the best-fit model, while the second model is disfavored by Δχ
2 ∼ 3. The last model is strongly disfavored by Δχ
2 ∼ 15 but not ruled out. A Bayesian analysis using a Galactic model indicates that the first two models are probably composed of a Saturn-mass planet orbiting a late M dwarf, while the third one could consist of a super-Jovian planet and a mid-mass brown dwarf. The source-lens relative proper motion is μ
rel ∼ 9 mas yr−1, so the source and lens could be resolved by current adaptive-optics instruments in 2020 if the lens is luminous.
Role of Intervening Mg ii Absorbers on the Rotation Measure and Fractional Polarization of the Background Quasars
Authors: Malik Sunil , Chand Hum , Seshadri T. R. 
Published: February 2020

Abstract
We probed the magnetic fields in high-redshift galaxies using excess extragalactic contribution to residual rotation measure (RRM) for quasar sightlines with intervening Mg ii absorbers. Based on a large sample of 1132 quasars, we have computed RRM distributions broadening using median absolute deviation from the mean (

), and found it to be 17.1 ± 0.7 rad m−2 for 352 sightlines having Mg ii intervening absorbers in comparison to its value of 15.1 ± 0.6 rad m−2 for 780 sightlines without such absorbers, resulting in an excess broadening (

) of 8.0 ± 1.9 rad m−2 among these two subsamples. This value of

, has allowed us to constrain the average strength of magnetic field (rest frame) in high-redshift galaxies responsible for these Mg ii absorbers, to be ∼1.3 ± 0.3 μG at a median redshift of 0.92. This estimate of magnetic field is consistent with the reported estimate in earlier studies based on radio-infrared correlation and energy equipartition for galaxies in the local universe. A similar analysis on subsample split based on the radio spectral index, α (with F

ν
∝ ν

α
), for flat (α ≥ −0.3; 315 sources) and steep (α ≤ −0.7; 476 sources) spectrum sources shows a significant

(at 3.5σ level) for the former and absent in the latter. An anticorrelation found between the

and percentage polarization (p) with a similar Pearson correlation of −0.62 and −0.87 for subsamples with and without Mg ii, respectively, suggests the main contribution for decrements in the p value to be intrinsic to the local environment of quasars.
Stellar Characterization of M Dwarfs from the APOGEE Survey: A Calibrator Sample for M-dwarf Metallicities
Authors: Souto Diogo , Cunha Katia , Smith Verne V. , Allende Prieto C. , Burgasser Adam , Covey Kevin , García-Hernández D. A. , Holtzman Jon A. , Johnson Jennifer A. , Jönsson Henrik , Mahadevan Suvrath , Majewski Steven R. , Masseron Thomas , Shetrone Matthew , Rojas-Ayala Bárbara , Sobeck Jennifer , Stassun Keivan G. , Terrien Ryan , Teske Johanna , Wanderley Fábio , Zamora Olga 
Published: February 2020

Abstract
We present spectroscopic determinations of the effective temperatures, surface gravities, and metallicities for 21 M dwarfs observed at high resolution (R ∼ 22,500) in the H band as part of the Sloan Digital Sky Survey (SDSS)-IV Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey. The atmospheric parameters and metallicities are derived from spectral syntheses with 1D LTE plane-parallel MARCS models and the APOGEE atomic/molecular line list, together with up-to-date H2O and FeH molecular line lists. Our sample range in T
eff from ∼3200 to 3800 K, where 11 stars are in binary systems with a warmer (FGK) primary, while the other 10 M dwarfs have interferometric radii in the literature. We define an

M

K

S

–radius calibration based on our M-dwarf radii derived from the detailed analysis of APOGEE spectra and Gaia DR2 distances, as well as a mass–radius relation using the spectroscopically derived surface gravities. A comparison of the derived radii with interferometric values from the literature finds that the spectroscopic radii are slightly offset toward smaller values, with Δ = −0.01 ± 0.02 R⋆/R
⊙. In addition, the derived M-dwarf masses based upon the radii and surface gravities tend to be slightly smaller (by ∼5%–10%) than masses derived for M-dwarf members of eclipsing binary systems for a given stellar radius. The metallicities derived for the 11 M dwarfs in binary systems, compared to metallicities obtained for their hotter FGK main-sequence primary stars from the literature, show excellent agreement, with a mean difference of [Fe/H](M dwarf – FGK primary) = +0.04 ± 0.18 dex, confirming the APOGEE metallicity scale derived here for M dwarfs.
The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. II. A Statistical Characterization of Class 0 and Class I Protostellar Disks
Authors: Tobin John J. , Sheehan Patrick D. , Megeath S. Thomas , Díaz-Rodríguez Ana Karla , Offner Stella S. R. , Murillo Nadia M. , van ’t Hoff Merel L. R. , van Dishoeck Ewine F. , Osorio Mayra , Anglada Guillem , Furlan Elise , Stutz Amelia M. , Reynolds Nickalas , Karnath Nicole , Fischer William J. , Persson Magnus , Looney Leslie W. , Li Zhi-Yun , Stephens Ian , Chandler Claire J. , Cox Erin , Dunham Michael M. , Tychoniec Łukasz , Kama Mihkel , Kratter Kaitlin , Kounkel Marina , Mazur Brian , Maud Luke , Patel Lisa , Perez Laura , Sadavoy Sarah I. , Segura-Cox Dominique , Sharma Rajeeb , Stephenson Brian , Watson Dan M. , Wyrowski Friedrich 
Published: February 2020

Abstract
We have conducted a survey of 328 protostars in the Orion molecular clouds with the Atacama Large Millimeter/submillimeter Array at 0.87 mm at a resolution of ∼0.″1 (40 au), including observations with the Very Large Array at 9 mm toward 148 protostars at a resolution of ∼0.″08 (32 au). This is the largest multiwavelength survey of protostars at this resolution by an order of magnitude. We use the dust continuum emission at 0.87 and 9 mm to measure the dust disk radii and masses toward the Class 0, Class I, and flat-spectrum protostars, characterizing the evolution of these disk properties in the protostellar phase. The mean dust disk radii for the Class 0, Class I, and flat-spectrum protostars are

,

, and

au, respectively, and the mean protostellar dust disk masses are 25.9

,

,

, respectively. The decrease in dust disk masses is expected from disk evolution and accretion, but the decrease in disk radii may point to the initial conditions of star formation not leading to the systematic growth of disk radii or that radial drift is keeping the dust disk sizes small. At least 146 protostellar disks (35% of 379 detected 0.87 mm continuum sources plus 42 nondetections) have disk radii greater than 50 au in our sample. These properties are not found to vary significantly between different regions within Orion. The protostellar dust disk mass distributions are systematically larger than those of Class II disks by a factor of >4, providing evidence that the cores of giant planets may need to at least begin their formation during the protostellar phase.
Investigating Taxonomic Diversity within Asteroid Families through ATLAS Dual-band Photometry
Authors: Erasmus N. , Navarro-Meza S. , McNeill A. , Trilling D. E. , Sickafoose A. A. , Denneau L. , Flewelling H. , Heinze A. , Tonry J. L. 
Published: February 2020

Abstract
We present here the c–o colors for identified Flora, Vesta, Nysa–Polana, Themis, and Koronis family members within the historic data set (2015–2018) of the Asteroid Terrestrial-impact Last Alert System (ATLAS). The Themis and Koronis families are known to be relatively pure C- and S-type Bus-DeMeo taxonomic families, respectively, and the extracted color data from the ATLAS broadband c- and o-filters of these two families are used to demonstrate that the ATLAS c–o color is a sufficient parameter to distinguish between the C- and S-type taxonomies. The Vesta and Nysa–Polana families are known to display a mixture of taxonomies possibly due to Vesta’s differentiated parent body origin and Nysa–Polana actually consisting of two nested families with differing taxonomies. Our data show that the Flora family also displays a large degree of taxonomic mixing and the data reveal a substantial H-magnitude dependence on color. We propose and exclude several interpretations for the observed taxonomic mix. Additionally, we extract rotation periods of all of the targets reported here and find good agreement with targets that have previously reported periods.
Maintenir une décision contestée : le cas du stockage des déchets radioactifs
Authors: Blanck Julie 
Published: February 2020

Depuis sa création, la politique française de gestion des déchets radioactifs a reposé sur une décision initiale : réaliser un stockage géologique pour les déchets les plus dangereux. Il s’agit d’une décision prise par les dirigeants scientifiques et techniques du secteur nucléaire, pour apporter une solution à ce problème. Pourtant cette décision a été régulièrement critiquée par des acteurs internes et externes au secteur nucléaire. Pour répondre à ces contestations, les dirigeants du secteur ont enrôlé successivement des acteurs critiques de plus en plus nombreux afin de les faire participer au maintien de cette décision, dont le principe n’est jamais rediscuté. Cet article propose d’étudier cette stratégie d’assimilation de la critique, en suivant la multitude d’acteurs et de dispositifs qui ont permis de maintenir cette décision depuis les années 1970.
Gueroult on Spinoza and the Ethics
Authors: Schmaltz Tad M. 
Published: February 2020

Cet article concerne l’application de la méthode « dianoématique », ou « étude des doctrines », dans le commentaire important de Martial Gueroult aux deux premières parties de l’ Éthique de Spinoza. Gueroult met l’accent sur deux affirmations distinctes dans les deux volumes de ce commentaire. La première affirmation, tirée du premier volume, est que Spinoza adopte une version du monisme dans la première partie de l’ Éthique selon laquelle Dieu, en tant que substance infinie, consiste en une union d’une infinité de substances distinctes constituées chacune d’un attribut unique. La deuxième affirmation, tirée du deuxième volume, est que Spinoza est contraint, du fait de ce qu’il écrit dans la deuxième partie de l’ Éthique , d’accepter la conclusion qu’il existe deux types de «parallélisme» différents entre les attributs divins.
Aux sources de l’empirisme transcendantal. Deleuze avec et au-delà de Gueroult
Authors: Krtolica Igor 
Published: February 2020

La relation de Deleuze à Gueroult est paradoxale. Car sur un plan strictement philosophique, Gueroult professait un rationalisme qui n’avait pas grand-chose à envier à celui d’Alquié ou d’Hyppolite que Deleuze ne manquera pas de critiquer sévèrement. Simplement, non seulement Deleuze n’a pas critiqué les positions de Gueroult, mais il les a même constamment reprises à son compte. Comment l’expliquer ? La raison nous semble la suivante : c’est que Gueroult n’a cessé d’accompagner et de porter l’exigence d’un « ordre synthétique » ou d’un « dynamisme génétique » en philosophie ; or, avant d’être une méthode pour l’historien de la philosophie, cette exigence exprime une certaine conception de la philosophie, dont découlent et la pratique et la philosophie de l’histoire de la philosophie ; et si Deleuze a repris à son compte les positions de Gueroult, c’est qu’il n’a cessé d’alimenter son propre travail philosophique à l’exigence portée par Gueroult, et à la conception de la philosophie qu’elle exprimait. Dans l’œuvre de Deleuze, cette exigence a même rendu possible un geste décisif, au-delà de l’ambition de Gueroult : la critique du rationalisme au nom d’un empirisme transcendantal. Avec Gueroult, au-delà de Gueroult. Le disciple s’est fait créateur. C’est peut-être en ce sens qu’il faut entendre la remarque d’Olivier Revault d’Allonnes : « J’ai toujours trouvé que Gilles [Deleuze] a été un grand élève de Gueroult ».
Leçon inédite sur les deux versions de la déduction kantienne des catégories
Authors: Gueroult Martial , Pelletier Arnaud 
Published: February 2020

Martial Gueroult donna un cours au Collège de France sur la Critique de la raison pure de Kant lors de l’année 1957-1958, qui est à ce jour inédit. Le texte qui est présenté ici est l’édition d’une des leçons portant sur la différence entre les deux versions de la déduction transcendantale des catégories. Gueroult y aborde une question classique du commentaire, celle de savoir si la deuxième édition de la Critique a renié la doctrine de la première version. Contre l’interprétation de Herman Jan de Vleeschauwer, Gueroult défend que l’effort de clarification de la déduction, non moins que le souci d’écarter une lecture psychologisante des facultés, ont conduit Kant à emprunter un unique chemin de la déduction des catégories : de haut en bas.
État des lieux sur les mesures en variables latentes : le cas du sentiment d’employabilité des cadres séniors du secteur privé français
Authors: Deacken Nadia , Jaotombo Franck 
Published: February 2020

Cet article fait le point sur l’évolution des différents modèles de mesure à variables latentes utilisés en Sciences de Gestion. On commence par rappeler les modèles traditionnels utilisés depuis les années 1980, puis on présente les avancées les plus récentes de cette dernière décennie, notamment la redécouverte des modèles bifactoriels et le développement des modèles en équations structurelles exploratoires (ESEM). Ces deux derniers modèles représentent une généralisation du modèle traditionnel d’analyse factorielle confirmatoire (ICM CFA) et démontrent à la fois un meilleur ajustement aux données et une meilleure validité de construit (convergente, discriminante, prédictive). Ces méthodes sont ensuite illustrées par l’opérationnalisation du construit de « sentiment d’employabilité ». Le modèle traditionnel de CFA s’avère significativement être moins ajusté aux données que les modèles ESEM et présente des qualités de validité et de fiabilité bien moindres. Le résultat final donne lieu à un modèle bifactoriel ESEM comportant un facteur général intégrateur de sentiment d’employabilité et dix facteurs spécifiques, lesquels prédisent qu’un cadre sénior demandeur d’emploi a plus de chance de se sentir employable qu’un cadre sénior actif, à l’exception des facteurs de sentiment d’efficacité professionnelle et de compétences. Quelques biais théoriques et empiriques du modèle de CFA traditionnel sont ensuite évoqués, puis des implications managériales et académiques indiquées pour de futures recherches.
Strategic sourcing: Developing a progressive framework for make-or-buy decisions
Authors: Medina-Serrano Rubén , González-Ramírez Reyes , Gasco-Gasco Jose , Llopis-Taverner Juan 
Published: February 2020

Purpose: Make-or-buy decisions represent a critical dilemma faced by many firms. The appropriate decision between designing and manufacturing parts or services in-house, buying them from external providers or combining both is a fundamental firm process. This paper seeks to address this question by updating the traditional make-or-buy literature with new academic insights, developing a make-or-buy framework with a tool for its operationalisation to help managers evaluate sourcing decisions.Design/methodology/approach: First, a literature review of the principal theories and approaches about make-or-buy decisions is discussed. Second, the development of the make-or-buy framework is described and explained based on the results of qualitative interviews with practitioners and a set of interviews of an in-firm case study. Third, the results and the implementation of the framework are outlined.Findings: Our study not only validates the proposed framework through a set of in-firm make-or-buy decisions, but also provides a structure for its implementation and design a decision matrix with a pairwise comparison tool for helping practitioners to put the framework into practice.Research limitations/implications: This paper aims to contribute to the study of the make-or-buy literature in supply chain management through the graphical representation of why and how make-or-buy decisions are made. Interestingly, the paper presents relevant dimensions and factors to be studied and evaluates possible outcomes when approaching make-or-buy decisions.Originality/value: Our results suggest that practitioners should combine this framework with a pairwise comparison matrix and a multi-criteria decision analysis based on the TOPSIS methodology to assess strategic sourcing decisions.