bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH KARAKTERISTIK PERUSAHAAN, STRUKTUR KEPEMILIKAN DAN KUALITAS AUDIT TERHADAP MANAJEMEN LABA
Authors: FELICYA CINDY , SUTRISNO PAULINA 
Published: June 2020

Tujuan dilakukannya penelitian ini adalah untuk mengetahui hubungan antara karakteristik perusahaan yang meliputi pertumbuhan perusahaan, kinerja perusahaan, ukuran perusahaan, umur perusahaan, ukuran dewan komisaris, serta struktur kepemilikan berupa kepemilikan manajerial, kepemilikan institusional dan kualitas audit terhadap manajemen laba pada perusahaan non keuangan yang terdaftar di Bursa Efek Indonesia. Penelitian ini menggunakan sampel sebanyak 139 perusahaan non keuangan yang terdaftar di Bursa Efek Indonesia yang dipilih dengan menggunakan metode purposive sampling selama periode 2016 sampai 2018 dengan total observasi sebanyak 417 data. Penelitian ini menggunakan analisis regresi linear berganda. Hasil dari penelitian ini menunjukan bahwa karakteristik perusahaan seperti pertumbuhan perusahaan dan kinerja perusahaan memiliki pengaruh terhadap manajemen laba, sedangkan variabel independen lainnya seperti ukuran perusahaan, umur perusahaan, ukuran dewan komisaris, kepemilikan manajerial, kepemilikan institusional dan kualitas audit tidak memiliki pengaruh terhadap manajemen laba perusahaan.
Çocuklarla Felsefe Programının Çocukların İnsani Değerlere Yönelik Tutumları Üzerindeki Etkililiği
Authors: MEHDİYEV Gülsüm , TOZDUMAN YARALI Kevser 
Published: June 2020

Bu araştırmanın amacı; çocuklarla felsefe programının yedinci sınıfa devam eden çocukların insani değerlere yönelik tutumları üzerindeki etkisini incelemektir. Araştırmada karma model kullanılmıştır. Araştırmanın nicel boyutunda deneysel desen oluşturulmuş ve veri toplama aracı olarak “İnsani Değerler Ölçeği” kullanılmıştır. Nitel boyuttaki verilerin toplanmasında doküman incelemesi ve odak grup görüşmesinden yararlanılmıştır. Araştırmanın çalışma grubu 20 çocuktan oluşmuştur. Deney grubundaki çocuklarla 10 hafta süren felsefe eğitim programı uygulanmıştır. Nicel verilerin analizinde, Mann Whitney U testi ve Wilcoxon testi uygulanmıştır. Nitel verilerin analizinde doküman incelemesi için betimsel analiz, odak grup görüşmesi için içerik analizi yapılmıştır. Çalışmanın sonucunda felsefe eğitiminin çocukların insani değerlere yönelik tutumlarını olumlu etkilediği bulunmuştur.
TENDÊNCIAS DE MORTALIDADE POR DOENÇAS RESPIRATÓRIAS E DOENÇAS CARDIOVASCULARES EM TERESINA-PI
Authors: Da Silva Gleison Vitor Ferreira de Castro , Nogueira Luciana Tolstenko , Araujo Izael Francisco de Brito , De Souza Daiane Ribeiro , De Sousa Geovanna Arnaldo , Da Silva Allan Dellon 
Published: June 2020

Este estudo teve por objetivo analisar as tendências de mortalidade por doenças respiratórias e cardiovasculares e comparar o comportamento dessas tendências entre si no período entre 2009 a 2016, em Teresina, Piauí. Trata-se de um estudo descritivo, de análise quantitativa, realizado na capital do Piauí. A pesquisa teve como base fundamental os dados do Sistema de Informação sobre Mortalidade (SIM) e do Núcleo de Informação em Serviços de Saúde (NUINSA). O aumento proporcional das mortes por Doenças do Aparelho Circulatório (DAC) foi um pouco maior que o das mortes por Doenças Respiratórias (DR) (40,6% versus 38,6%), com destaque no grupo de Doenças do Aparelho Circulatório para as doenças isquêmicas do coração e doenças cerebrovasculares e no grupo de Doenças Respiratórias para influenza e pneumonia. O incremento nos óbitos por doenças do aparelho circulatório e doenças respiratórias entre 2009 e 2016, discretamente maior entre as primeiras, aponta para a necessidade de comprometimento local com o plano de ações nacional para enfrentamento das Doenças Crônicas Não Transmissíveis e também para a fragilidade nos processos de saúde que visam a prevenção e cuidado
EFESIENSI PEMUPUKAN NITROGEN TERHADAP SIFAT FISIK TANAH SERTA HASIL TANAMAN KANGKUNG DARAT MELALUI APLIKASI PUPUK ORGANIK CAIR KRINYU (Ipomea reptans poir)
Authors: Stefan Stefan Jaghu Renggi , Mutiara Charly 
Published: June 2020

The problems faced are the use of inorganic fertilizers that damage the level of soil organic matter decreases, soil structure is damaged, and environmental pollution. This research utilizes liquid organic fertilizer, kirinyu because it has N elements which are high enough to provide yield of ground water spinach plants and soil physical properties.
This study aims to determine the effect of nitrogen fertilizer efficiency on soil physical properties and the effect of nitrogen fertilizer efficiency on land kale yield. The study was arranged based on 2 factors: the outcome variable using a randomized block design (RBD) and the variable saving of Soil Physical Properties.
The results of statistical analysis show that the efficiency of nitrogen fertilization on the yield of ground water spinach plants has a very significant influence on yield variables which include fresh weight of land spinach tan-1 (g) and fresh weight of water spinach ha-1 (ton). The efficiency of nitrogen fertilization on the yield of ground water spinach plants has a very significant effect with an average increase in each treatment for fresh water spinach per plant by 27.97% and the fresh weight of water spinach per hekatar by 27.97%. The efficiency of nitrogen fertilization on the physical properties of the soil in kangkung cultivation in Lokoboko village has sandy clay soil texture, has a density value of contents ranging from 1.33 g / cm - 1.37 g / cm and soil porosity 45.46% - 50.22 %. The soil color is dominated by 10 YR 2/1 Black and 10 YR 2/2 Very Dark Brown, having soil temperatures ranging from 25,250C - 26,750C.
Electrochemical evaluation of the patina of the weathering steel sculpture Once Módulo
Authors: Crespo Ibañez Ana , Ramírez Barat Blanca , Díaz Ocaña Iván , Cano Emilio 
Published: June 2020

Weathering steels (WS) have been widely used due to the protective rust formed on the surface of the bare metal exposed to the atmosphere. They have been studied attending to specifications and characteristics in engineering, but in cultural heritage the use of this material does not follow the same criteria and has different needs which must be addressed. Among them, the design and the location of the sculpture may have an impact on the rust formed and may not be as protective as it was supposed to be.
This work presents the study of the weathering steel sculpture Once Módulo which shows areas with different exposure to rainwater and different surface heterogeneities. The results obtained by Electrochemical Impedance Spectroscopy (EIS) have shown that the protective ability of the rust depends on the previous differences and that design and location of the artwork play an important role for its conservation.
Refining the Census of the Upper Scorpius Association with Gaia*
Authors: Luhman K. L. , Esplin T. L. 
Published: June 2020

Abstract
We have refined the census of stars and brown dwarfs in the Upper Sco association (∼10 Myr, ∼145 pc) by (1) updating the selection of candidate members from our previous survey to include the high-precision astrometry from the second data release of Gaia, (2) obtaining spectra of a few hundred candidate members to measure their spectral types and verify their youth, and (3) assessing the membership (largely with Gaia astrometry) of 2020 stars toward Upper Sco that show evidence of youth in this work and previous studies. We arrive at a catalog of 1761 objects that are adopted as members of Upper Sco. The distribution of spectral types among the adopted members is similar to those in other nearby star-forming regions, indicating a similar initial mass function. In previous studies, we have compiled mid-infrared photometry from the Wide-field Infrared Survey Explorer and the Spitzer Space Telescope for members of Upper Sco and used those data to identify the stars that show evidence of circumstellar disks; we present the same analysis for our new catalog of members. As in earlier work, we find that the fraction of members with disks increases with lower stellar masses, ranging from ≲10% for >1 M
⊙ to ∼22% for 0.01–0.3 M
⊙. Finally, we have estimated the relative ages of Upper Sco and other young associations using their sequences of low-mass stars in

versus G
BP − G
RP. This comparison indicates that Upper Sco is a factor of two younger than the β Pic association (21–24 Myr) according to both nonmagnetic and magnetic evolutionary models.
OSSOS XX: The Meaning of Kuiper Belt Colors
Authors: Nesvorný David , Vokrouhlický David , Alexandersen Mike , Bannister Michele T. , Buchanan Laura E. , Chen Ying-Tung , Gladman Brett J. , Gwyn Stephen D. J. , Kavelaars J. J. , Petit Jean-Marc , Schwamb Megan E. , Volk Kathryn 
Published: June 2020

Abstract
Observations show that 100 km class Kuiper Belt objects (KBOs) can be divided into (at least) two color groups, red (R; g − i < 1.2) and very red (VR; g − i > 1.2), reflecting a difference in their surface composition. This is thought to imply that KBOs formed over a relatively wide range of radial distance, r. The cold classicals at 42 au < r < 47 au are predominantly VR, and known Neptune Trojans at r ≃ 30 au are mostly R. Intriguingly, however, the dynamically hot KBOs show a mix of R and VR colors and no correlation of color with r. Here we perform migration/instability simulations where the Kuiper Belt is populated from an extended planetesimal disk. We find that the color observations can be best understood if R objects formed at r < r* and VR objects at r > r*, with 30 au < r* < 40 au. The proposed transition at 30 au < r* < 40 au would explain why the VR objects in the dynamically hot population have smaller orbital inclinations than the R objects, because the orbital excitation from Neptune weakens for orbits starting beyond 30 au. Possible causes of the R–VR color bimodality are discussed.
Gravitational-wave Memory from a Propagating Relativistic Jet: A Probe of the Interior of Gamma-Ray Burst Progenitors
Authors: Yu Yun-Wei 
Published: June 2020

Abstract
It is believed that the relativistic jets of gamma-ray bursts (GRBs) should initially propagate through a heavy envelope of the massive progenitor stars or through merger ejecta formed from compact binary mergers. The interaction of a jet with a stellar envelope or merger ejecta can lead to the deceleration of the head material of the jet and simultaneously the formation of a hot cocoon. However, this jet-envelope/ejecta interaction is actually undetectable with electromagnetic radiation and can only be inferred indirectly by the structure of the breakout jet. Therefore, as a solution to this phenomenon, we suggest the jet-envelope/ejecta interaction can produce a gravitational-wave (GW) memory of an amplitude of

, which could be detected with some future GW detectors sensitive in the frequency range from sub-Hertz to several tens of Hertz. This provides a potential direct way to probe the jet propagation and then the interior of the GRB progenitors.
Cosmological Information from the Small-scale Redshift-space Distortion
Authors: Tonegawa Motonari , Park Changbom , Zheng Yi , Park 박현 Hyunbae 배 , Hong 홍성 Sungwook E. 욱 , Hwang Ho Seong , Kim 김주 Juhan 한 
Published: June 2020

Abstract
The redshift-space distortion (RSD) in the observed distribution of galaxies is known as a powerful probe of cosmology. Observations of large-scale RSD, caused by the coherent gravitational infall of galaxies, have given tight constraints on the linear growth rate of the large-scale structures in the universe. On the other hand, the small-scale RSD, caused by galaxy–random motions inside clusters, has not been much used in cosmology, but it also has cosmological information because universes with different cosmological parameters have different halo mass functions and virialized velocities. We focus on the projected correlation function w(r

p
) and the multipole moments ξ

l
on small scales (1.4–30 h
−1 Mpc). Using simulated galaxy samples generated from a physically motivated most bound particle (MBP)–galaxy correspondence scheme in the Multiverse Simulation, we examine the dependence of the small-scale RSD on the cosmological matter density parameter Ω
m
; the satellite velocity bias with respect to MBPs,

; and the merger timescale parameter α. We find that α = 1.5 gives an excellent fit to the w(r

p
) and ξ

l
measured from the Sloan Digital Sky Survey–Korea Institute for Advanced Study value-added galaxy catalog. We also define the “strength” of the Fingers of God as the ratio of the parallel and perpendicular size of the contour in the two-point correlation function set by a specific threshold value and show that the strength parameter helps constrain

by breaking the degeneracy among them. The resulting parameter values from all measurements are

, indicating a slight reduction of satellite galaxy velocity relative to the MBP. However, considering that the average MBP speed inside halos is 0.94 times the dark matter velocity dispersion, the main drivers behind the galaxy velocity bias are gravitational interactions, rather than baryonic effects.
Neutral Cr and V in the Atmosphere of Ultra-hot Jupiter WASP-121 b
Authors: Ben-Yami Maya , Madhusudhan Nikku , Cabot Samuel H. C. , Constantinou Savvas , Piette Anjali , Gandhi Siddharth , Welbanks Luis 
Published: June 2020

Abstract
Ultra-hot Jupiters (UHJs), giant exoplanets with equilibrium temperatures above 2000 K, are ideal laboratories for studying metal compositions of planetary atmospheres. At these temperatures the thermal dissociation of metal-rich molecules into their constituent elements makes these atmospheres conducive for elemental characterization. Several elements, mostly ionized metals, have been detected in UHJs recently using high-resolution transit spectroscopy. Even though a number of neutral transition metals (e.g., Fe, Ti, V, Cr) are expected to be strong sources of optical/near-ultraviolet (NUV) opacity and, hence, influence radiative processes in the lower atmospheres of UHJs, only Fe i has been detected to date. We conduct a systematic search for atomic species in the UHJ WASP-121 b. Using theoretical models we present a metric to predict the atomic species likely to be detectable in such planets with high-resolution transmission spectroscopy. We search for the predicted species in observations of WASP-121 b and report the first detections of neutral transition metals Cr i and V i in an exoplanet at 3.6σ and 4.5σ significance, respectively. We confirm previous detections of Fe i and Fe ii. Whereas Fe ii was detected previously in the NUV, we detect it in the optical. We infer that the neutral elements Fe i, V i, and Cr i are present in the lower atmosphere, as predicted by thermochemical equilibrium, while Fe ii is a result of photoionization in the upper atmosphere. Our study highlights the rich chemical diversity of UHJs.
Being Careful with the Field Formation Interpretation of GW190412
Authors: Safarzadeh Mohammadtaher , Hotokezaka Kenta 
Published: June 2020

Abstract
The LIGO/Virgo Scientific Collaboration recently announced the detection of a compact object binary merger, GW190412, as the first asymmetric binary black hole (BBH) merger with mass ratio q ≈ 0.25. Other than the mass ratio, this BBH has been shown to have a positive effective spin of around χ
eff ≈ 0.28. Assuming a field formation channel, associating this effective spin to either the primary or the secondary black hole (BH) each have implications: if the spin of the BBH comes from the primary BH, it has consequences for the efficiency of angular momentum transport in the formation of the BH. If, on the other hand, the spin is due to the secondary BH through tidal spin-up processes, it should be noted that (i) such processes have very short delay times, and (ii) subsequently, their local merger rate is determined by local star formation rate at the assumed formation metallicity of the BBH. We show that the predicted merger rate density from this channel is

, and is in tension with the rather high local merger rate of such systems, which we estimate from this single event to be

(90% confidence interval, and assuming 50 days of observing time). Large natal kicks (v ≳ 500 km s−1) would be required to get such an BBHs with an in-plane spin component to account for the marginal detection of precession in GW190412. However, this would only exacerbate the tension as the estimated local merger rate would be further decreased. Similarly, the formation of such systems through the dynamical assembly is exceedingly rare; consequently, it is difficult to account for this system with the currently accepted paradigms of BBH formation.
Comparison of Enhanced Absorption in He i 10830 Å in Observations and Modeling during the Early Phase of a Solar Flare
Authors: Huang Nengyi , Sadykov Viacheslav M. , Xu Yan , Jing Ju , Wang Haimin 
Published: June 2020

Abstract
The He i 10830 Å triplet is a very informative indicator of chromospheric activities as the helium is the second most abundant element in the solar atmosphere. Taking advantage of the high resolution of the 1.6 m Goode Solar Telescope at Big Bear Solar Observatory, previous observations have shown clear evidence of the enhanced absorption, instead of typically observed emission, for two M-class flares. In this study, we analyze the evolution of the He i 10830 Å emission in numerical models and compare it with observations. The models represent the RADYN simulation results obtained from the F-CHROMA database. We consider the models with the injected electron spectra parameters close to observational estimates for the 2013 August 17 flare event (δ = 8,

,

) in detail, as well as other available models. The modeling results agree well with observations, in the sense of both the maximum intensity decrease (−17.1%, compared with the observed value of −13.7%) and the trend of temporal variation (initial absorption phase followed by the emission). All models demonstrate the increased number densities and decreased ratio of the upper and lower level populations of the He i 10830 Å transition in the initial phase, which enhances the opacity and forms an absorption feature. Models suggest that the temperatures and free electron densities at heights of 1.3–1.5 Mm should be larger than ∼104 K and 6 × 1011 cm−3 thresholds for the line to start being in emission.
La validation des acquis de l’expérience en psychologie : des enjeux aux propositions
Authors: Jeoffrion Christine , Clarys David , Voisin Dimitri , Abrivat Elisabeth , Ernd Aline 
Published: June 2020

Cet article rend compte du symposium organisé par la commission pédagogique de l’Association des enseignants-chercheurs en psychologie des universités (AEPU), lors des « Deuxièmes entretiens » organisés par la Fédération française des psychologues et de psychologie (FFPP), en novembre 2006. Il traite de la mise en place de la validation des acquis de l’expérience (VAE) en psychologie. La première partie en présente le cadre général et les enjeux particuliers en psychologie. La deuxième partie expose quelques difficultés concrètes à partir d’une illustration à l’université de Tours. La troisième partie présente un résumé du rapport sur la VAE en psychologie, co-signé par l’AEPU, la FFPP, la Société française de psychologie et le Syndicat national des psychologues, ainsi que les travaux en cours sur le Master. On retiendra la nécessité d’une harmonisation des pratiques et des décisions, au sein des universités, pour éviter une dévalorisation des diplômes de psychologie.
Réglementation du titre de psychothérapeute : analyse d’une imposture
Authors: Grosbois Philippe 
Published: June 2020

À partir d’une proposition de loi du député Bernard Accoyer en 1999, après de nombreux débats, les parlementaires ont finalement adopté un article de loi relatif à l’usage du titre de psychothérapeute. Plusieurs réunions de concertation, au ministère de la Santé, ont eu lieu à propos du contenu du futur décret d’application de cette loi, sans aboutir, pour autant, à un consensus, car les intérêts en jeu au niveau des acteurs concernés sont contradictoires : d’une part, deux professions réglementées, les psychologues et les médecins, d’autre part, deux types d’activité non réglementées, les psychanalystes et les « psychothérapeutes » non-médecins et non-psychologues. Ces derniers revendiquent la création d’une nouvelle profession indépendante de « psychothérapeute », et contestent la nécessité d’une formation universitaire de base, soutenus par une minorité des sociétés de psychanalyse. Les divergences portent donc, essentiellement, sur la différence d’appréciation des critères de formation en psychopathologie exigés par la loi, certaines organisations contestant que cette formation soit le monopole des universités. Une autre ambiguïté porte sur le fait que la loi fait l’impasse sur la formation à la psychothérapie proprement dite, le Sénat ayant opté pour l’exigence minimale d’une formation en psychopathologie. Le présent article a pour objet de revenir sur les stratégies des acteurs qui se sont mobilisés lors des versions successives de cette proposition de loi, et de proposer quelques repères quant aux positions idéologiques soustendues par ces stratégies.
Découvrir la dynamique de l’expérience vécue
Authors: Petitmengin Claire 
Published: June 2020

Contrairement à une croyance largement répandue, l’accès à la conscience de sa propre expérience subjective n’est ni immédiat ni facile, mais suppose une véritable expertise qui s’apprend. Un tel entraînement permet de découvrir que l’expérience vécue, associée à la réalisation d’un processus cognitif donné, loin d’être un brouillon, possède une structure dynamique très précise : elle est constituée d’une succession déterminée de sensations et d’opérations, qui restent habituellement pré-réfléchies. Par les possibilités de transformation qu’elle ouvre, la prise de conscience de cette micro-dynamique crée des perspectives inattendues dans les domaines médical, thérapeutique et existentiel. Mais surtout, parce qu’elle permet de guider et d’affiner les analyses neurophysiologiques, cette prise de conscience annonce la levée d’un interdit : celui qui excluait jusqu’à présent l’expérience vécue du champ de l’investigation scientifique.
Temps, famille, discriminations professionnelles
Authors: Grésy Brigitte 
Published: June 2020

La prise en compte de l’exercice de la parentalité n’est toujours pas à l’agenda dans les entreprises. Les pères en sont dissuadés tandis que les mères sont sanctionnées. Et le double déplacement n’a pas eu lieu : les femmes sont allées en masse dans le monde du travail mais les hommes n’ont pas investi la sphère privée, et la norme est encore une priorisation professionnelle masculine. Les chiffres sont là pour montrer cet inégal partage des responsabilités familiales et domestiques. Or c’est là la cause essentielle des inégalités structurelles entre les femmes et les hommes, et du sexisme qui leur est associé. Pour remédier à ces problèmes, il faut jouer sur le temps et sur l’implication des pères dans la parentalité tout au long de la vie, en allongeant le congé de paternité et en créant un nouveau droit individuel à la parentalité, pour prendre en compte non seulement les enfants mais aussi les proches avec lesquels les salarié.e.s sont en relation d’interdépendance.
Imbroglio institutionnel – isomorphisme ; prendre le temps de les chercher
Authors: Maisin Antoine , Denis Jennifer , Meynckens-Fourez Muriel 
Published: June 2020

Au travers d’une situation clinique prise en charge par une « équipe mobile » qui fut mise en place en Belgique par décision politique, comme alternative à l’hospitalisation psychiatrique de longue durée, l’article met en évidence l’isomorphisme entre la situation institutionnelle et la situation familiale. Les auteurs décrivent comment, sans le vouloir, des enjeux relationnels entre deux équipes peuvent reproduire des impasses et de la souffrance chez le patient. Ils indiquent aussi comment ces impasses s’apparentent aux « jeux psychotiques dans les familles », comme M. Selvini-Palazzoli et ses collaborateurs l’ont si bien décrit.