bluuebunny/crossref_metadata_2025_split huggingface dataset:
Hubungan antara Persepsi terhadap Celebrity Endorser dan Kecenderungan Pembelian Kompulsif Online
Authors: Handayani Winda Citra , Renanita Theda 
Published: January 2023

Penelitian ini bertujuan untuk mengetahui hubungan antara persepsi terhadap celebrity endorser dan kecenderungan pembelian kompulsif online. Hipotesis dalam penelitian ini adalah adanya hubungan positif antara dimensi persepsi terhadap celebrity endorser yaitu expertise, attractiveness, dan trustworthiness dengan kecenderungan pembelian kompulsif online. Subjek penelitian ini berjumlah 172. Penelitian ini menggunakan metode penelitian kuantitatif dengan desain korelasional. Data diperoleh dengan menggunakan skala persepsi terhadap celebrity endorser yang dikembangkan oleh peneliti dan skala kecenderungan pembelian kompulsif online yang diadaptasi dari Valence, d’Astous, & Fortier (1988). Hasil penelitian ini menunjukkan bahwa terdapat hubungan positif antara dimensi expertise dan attractiveness dengan kecenderungan pembelian kompulsif online {(r = 0.110 dengan p= 0.049; r = 0.118 dengan p = 0.038)}, dan tidak ada hubungan antara dimensi trustworthiness dengan kecenderungan pembelian kompulsif online (r = 0.023 dengan p = 0.679).
Hubungan antara Spiritualitas dan Adversity Quotient pada Mahasiswa Perguruan Tinggi Negeri X dan Y di Surabaya
Authors: Prasetyawati Nandia , Virlia Stefani 
Published: January 2023

Penelitian ini bertujuan untuk mengetahui hubungan antara spiritualitas dan adversity quotient pada mahasiswa perguruan tinggi negeri (PTN) X dan Y di Surabaya menggunakan metode penelitian kuantitatif dengan desain korelasional. Hipotesis dalam penelitian ini adalah terdapat korelasi positif antara spiritualitas serta dimensi-dimensinya (belief in God, search for meaning, mindfulness, feeling of security) dan adversity quotient pada mahasiswa PTN X dan Y di Surabaya. Data diperoleh dengan mengadaptasi skala the spirituality questionnaire dan adversity quotient. Subjek penelitian adalah 205 mahasiswa. Hasil penelitian menunjukkan terdapat korelasi positif antara spiritualitas serta dimensi- dimensinya (belief in God, search for meaning, mindfulness, feeling of security) dengan adversity quotient pada mahasiswa PTN X dan Y di Surabaya (r = 0.401; r = 0.332; r = 0.268; r = 0.230; r = 397 dengan p = 0.000). Hal ini menunjukkan semakin tinggi spiritualitas dan dimensi- dimensinya yang diperoleh mahasiswa, maka semakin tinggi pula adversity quotient yang dimilikinya, begitupun sebaliknya.
Family Business Succession Planning at PT. X
Authors: Nourmalasari Raisha Dian 
Published: January 2023

The purpose of this research is to know succession planning from the second generation to the third generation in PT. X. This research is descriptive quantitative, which is research that produces descriptive data in the form of written or spoken words from informants and understands the behavior of individuals and groups that can be observed. The data obtained were collected and analyzed by interview and observation to six informants from PT. X is three of the second generation, and three of the third generation with triangulation analysis techniques. The result of this research the role of succession in the third generation of PT. X which includes pre-succession, succession planning, and succession management is already at the pre-succession stage that can support the sustainability of PT. X so that the company's condition can run well.
Vitamin D Supplementation in Alleviation of Oxidative Stress among Type 2 Diabetics
Authors: Begum Nadia , Kawser Mahbuba , Sadi Sheikh Khalid Saifullah , Tarafdar Monowar Ahmad , Islam Sheikh Nazrul 
Published: January 2023

Globally diabetes mellitus (T2DM) is a burning issue. Prediction of global estimation that the proportion of diabetes with adult will increase 69% for the year 2030. Hans Selye, the Canadian physiologist, was the first scientist to study the effects of psychological stress on the human body in 1936.Diabetic patients are in a state of high oxidative stress which leading to impaired glucose homeostasis, insulin insufficiency, and other complications.: A randomized controlled trial was conducted to see the effect of the vitamin D supplementation on oxidative stress in vitamin D deficientT2DM patients. In this study, a total of 124 T2DM patients were randomly enrolled, among them Treatment group 61 and placebo 63. In treatment group received 20,000IU vitamin D every 5thDay for three months in addition to regular treatment. Analysis of fasting plasma glucose (FPG), Vitamin D 25(OH)2, malondialdehyde (MDA) and superoxide dismutase (SOD) have been estimated both at the time of study recruitment, at 6th weeks and after 12-weeks of vitamin D supplementation (endline). Present study showed after vitamin D supplementation, baseline mean FBG gradually significantly (P<0.001) decreased at the end line in treatment group as compared to placebo. All biochemical indices by P- trend like FBG, vitamin D, MDA and SOD were significantly different (P<0.05). Whenever, consider between groups vitamin D increased (P<0.05) and FBG decreased significantly (P<0.05) in treatment group as compared to placebo. However, no significant impact on socio-demography variables, vitamin D and Stress-related characteristics between treatment and control groups after vitamin D supplementation as those variables are somewhat independent (p>0.05) both at baseline and end line. The results were considered significant at P<0.05. The statistical calculations were done using SPSS version 26 software. A strong positive co-relation between diabetes and oxidative stress were observed in this study and showed beneficial impact of vitamin D supplementation to reduce oxidative stress those who were vitamin D deficient.
ВЛИЯНИЕ КУМАРИНА НА УСТОЙЧИВОСТЬ ДОННИКА И СПОСОБ ЗАГОТОВКИ КОРМА, СНИЖАЮЩИЙ ВЫСОКУЮ КОНЦЕНТРАЦИЮ КУМАРИНА
Authors: Байдалин М.Е. , Сагалбеков У.М. , Байдалина С.Е. , Ахет А.О. , Байкен А.С. 
Published: January 2023

В данной статье представлены результаты научных исследований за 2019-2022 годы по изучению влияния содержания кумарина в доннике на устойчивость к засухе и вредителям и определению способа заготовки донника на корм, снижающего содержание кумарина.
Научные исследования проводились на опытном поле ТОО «Кокшетауское опытно-производственное хозяйство» (Акмолинская область, Зерендинский район, с. Чаглинка), расположенном в степной зоне Северного Казахстана.
Целью данных научных исследований является определение влияния кумарина на устойчивость донника к засухе и вредителям, а также снижение в листостебельной массе высокой концентрации кумарина до безопасных пределов.
При проведении исследований были использованы общепринятые в агрономии методы постановки полевых опытов, лабораторные исследования проводились по установленным методам и стандартам на современных оборудованиях.
Объектом исследований является донник желтый.
Проведенные научно-производственные опыты показали, что возделывание сортов донника желтого с высокой концентрацией кумарина является эффективным приемом защиты растений от засушливых условий и вредителей, а также заготовка сена с различными температурными режимами снижает концентрацию кумарина и повышает питательную ценность корма.
Проведенные результаты исследования позволяют рекомендовать производству высокопродуктивные, засухоустойчивые и устойчивые к вредителям сорта донника желтого с высоким содержанием кумарина с заготовкой на корм с безопасной концентрацией кумарина для животных.
Область использования результатов – кормопроизводство и животноводство Северного Казахстана.
The Target-selection Pipeline for the Dark Energy Spectroscopic Instrument
Authors: Myers Adam D. , Moustakas John , Bailey Stephen , Weaver Benjamin A. , Cooper Andrew P. , Forero-Romero Jaime E. , Abolfathi Bela , Alexander David M. , Brooks David , Chaussidon Edmond , Chuang Chia-Hsun , Dawson Kyle , Dey Arjun , Dey Biprateep , Dhungana Govinda , Doel Peter , Fanning Kevin , Gaztañaga Enrique , A Gontcho Satya Gontcho , Gonzalez-Morales Alma X. , Hahn ChangHoon , Herrera-Alcantar Hiram K. , Honscheid Klaus , Ishak Mustapha , Karim Tanveer , Kirkby David , Kisner Theodore , Koposov Sergey E. , Kremin Anthony , Lan Ting-Wen , Landriau Martin , Lang Dustin , Levi Michael E. , Magneville Christophe , Napolitano Lucas , Martini Paul , Meisner Aaron , Newman Jeffrey A. , Palanque-Delabrouille Nathalie , Percival Will , Poppett Claire , Prada Francisco , Raichoor Anand , Ross Ashley J. , Schlafly Edward F. , Schlegel David , Schubnell Michael , Tan Ting , Tarle Gregory , Wilson Michael J. , Yèche Christophe , Zhou Rongpu , Zhou Zhimin , Zou Hu 
Published: January 2023

Abstract
In 2021 May, the Dark Energy Spectroscopic Instrument (DESI) began a 5 yr survey of approximately 50 million total extragalactic and Galactic targets. The primary DESI dark-time targets are emission line galaxies, luminous red galaxies, and quasars. In bright time, DESI will focus on two surveys known as the Bright Galaxy Survey and the Milky Way Survey. DESI also observes a selection of “secondary” targets for bespoke science goals. This paper gives an overview of the publicly available pipeline (desitarget) used to process targets for DESI observations. Highlights include details of the different DESI survey targeting phases, the targeting ID (TARGETID) used to define unique targets, the bitmasks used to indicate a particular type of target, the data model and structure of DESI targeting files, and examples of how to access and use the desitarget code base. This paper will also describe “supporting” DESI target classes, such as standard stars, sky locations, and random catalogs that mimic the angular selection function of DESI targets. The DESI target-selection pipeline is complex and sizable; this paper attempts to summarize the most salient information required to understand and work with DESI targeting data.
A Low-mass, Pre-main-sequence Eclipsing Binary in the 40 Myr Columba Association—Fundamental Stellar Parameters and Modeling the Effect of Star Spots
Authors: Tofflemire Benjamin M. , Kraus Adam L. , Mann Andrew W. , Newton Elisabeth R. , Gully-Santiago Michael A. , Vanderburg Andrew , Waalkes William C. , Berta-Thompson Zachory K. , Collins Kevin I. , Collins Karen A. , Nielsen Louise D. , Bouchy François , Ziegler Carl , Briceño César , Law Nicholas M. 
Published: January 2023

Abstract
Young eclipsing binaries (EBs) are powerful probes of early stellar evolution. Current models are unable to simultaneously reproduce the measured and derived properties that are accessible for EB systems (e.g., mass, radius, temperature, and luminosity). In this study we add a benchmark EB to the pre-main-sequence population with our characterization of TOI 450 (TIC 77951245). Using Gaia astrometry to identify its comoving, coeval companions, we confirm TOI 450 is a member of the ∼40 Myr Columba association. This eccentric (e = 0.2969), equal-mass (q = 1.000) system provides only one grazing eclipse. Despite this, our analysis achieves the precision of a double-eclipsing system by leveraging information in our high-resolution spectra to place priors on the surface-brightness and radius ratios. We also introduce a framework to include the effect of star spots on the observed eclipse depths. Multicolor eclipse light curves play a critical role in breaking degeneracies between the effects of star spots and limb-darkening. Including star spots reduces the derived radii by ∼2% from a unspotted model (>2σ) and inflates the formal uncertainty in accordance with our lack of knowledge regarding the starspot orientation. We derive masses of 0.1768( ± 0.0004) and 0.1767( ± 0.0003) M
⊙, and radii of 0.345(±0.006) and 0.346(±0.006) R
⊙ for the primary and secondary, respectively. We compare these measurements to multiple stellar evolution isochones, finding good agreement with the association age. The MESA MIST and SPOTS (f
s = 0.17) isochrones perform the best across our comparisons, but detailed agreement depends heavily on the quantities being compared.
Position and Proper Motion of Sagittarius A* in the ICRF3 Frame from VLBI Absolute Astrometry
Authors: Gordon David , de Witt Aletha , Jacobs Christopher S. 
Published: January 2023

Abstract
Sagittarius A* (Sgr A*) is a strong, compact radio source believed to be powered by a supermassive black hole at the galactic center. Extinction by dust and gas in the galactic plane prevents observing it optically, but its position and proper motion have previously been estimated using radio interferometry. We present new VLBI absolute astrometry measurements of its precise position and proper motion in the frame of the third realization of the International Celestial Reference Frame (ICRF3). The observations used were made at 52 epochs on the VLBA at K band (24 GHz) between 2006 June and 2022 August. We find the proper motion of Sgr A* to be −3.128 ± 0.042 mas yr−1 in R.A. and −5.584 ± 0.075 mas yr−1 in decl., or 6.400 ± 0.073 mas yr−1 at a position angle of 209.°26 ± 0.°51. We also find its J2000 ICRF3 coordinates at the 2015.0 proper motion epoch to be 17h45m40.ˢ034047 ± 0.ˢ000018, −29°00′28.″21601 ± 0.″00044. In galactic coordinates, Sgr A* shows proper motion of −6.396 ± 0.071 mas yr−1 in galactic longitude and −0.239 ± 0.045 mas yr−1 in galactic latitude, indicating solar motion of 248.0 ± 2.8 km s−1 in the galactic plane and 9.3 ± 1.9 km s−1 toward the north galactic pole.
Fast Outflowing Warm Absorbers in Narrow-line Seyfert 1 Galaxy PG 1001+054 Revealed by HST/COS Spectra
Authors: Fu Xiao-Dan , Wang Junfeng , Xu 许 Xiaoyu 啸宇 , Zhang Zhi-Xiang 
Published: January 2023

Abstract
Narrow-line Seyfert 1 (NLS1) galaxies are an important type of active galactic nucleus (AGN), generally expected to be accreting at a high Eddington rate. The properties of their outflows and importance of AGN feedback remain intriguing. We report on the discovery of fast outflowing warm absorbers (WAs) in the NLS1 PG 1001+054 with velocities in the range of ∼7000–9000 km s−1. They are identified with blueshifted Lyα, N v, and Si iv lines in the high-resolution ultraviolet (UV) spectra taken with the Cosmic Origins Spectrograph on board the Hubble Space Telescope. We perform photoionization modeling using XSTAR with three WAs. The derived physical properties are typical of WAs in terms of ionization and column density, whereas the outflow velocities are significantly higher. The estimated location of these WAs ranges from 1 to 73 parsecs away from the AGN. Together with previous detection of high ionization absorbers in the X-ray for PG 1001+054, we suggest that fast outflowing UV absorbers are probably part of a multiphase outflow. Such a structure is likely produced by the outflow launched from the AGN at an accretion disk scale, which shocks the ambient interstellar medium (ISM), producing stratified absorbers. Assuming contribution from the three WAs at tens of parsecs, the estimated ratio between the kinetic power of the outflow and AGN Eddington luminosity could reach 1.7%, raising the possibility of sufficient influence on the host galaxy when compared to some theoretical models for efficient AGN feedback.
Sustained Heating of the Chromosphere and Transition Region Over a Sunspot Light Bridge
Authors: Louis Rohan E. , Mathew Shibu K. , Bayanna A. Raja , Beck Christian , Choudhary Debi P. 
Published: January 2023

Abstract
Sunspot light bridges (LBs) exhibit a wide range of short-lived phenomena in the chromosphere and transition region. In contrast, we use here data from the Multi-Application Solar Telescope (MAST), the Interface Region Imaging Spectrograph (IRIS), Hinode, the Atmospheric Imaging Assembly (AIA), and the Helioseismic and Magnetic Imager (HMI) to analyze the sustained heating over days in an LB in a regular sunspot. Chromospheric temperatures were retrieved from the MAST Ca ii and IRIS Mg ii lines by nonlocal thermodynamic equilibrium inversions. Line widths, Doppler shifts, and intensities were derived from the IRIS lines using Gaussian fits. Coronal temperatures were estimated through the differential emission measure, while the coronal magnetic field was obtained from an extrapolation of the HMI vector field. At the photosphere, the LB exhibits a granular morphology with field strengths of about 400 G and no significant electric currents. The sunspot does not fragment, and the LB remains stable for several days. The chromospheric temperature, IRIS line intensities and widths, and AIA 171 and 211 Å intensities are all enhanced in the LB with temperatures from 8000 K to 2.5 MK. Photospheric plasma motions remain small, while the chromosphere and transition region indicate predominantly redshifts of 5–20 km s−1 with occasional supersonic downflows exceeding 100 km s−1. The excess thermal energy over the LB is about 3.2 × 1026 erg and matches the radiative losses. It could be supplied by magnetic flux loss of the sunspot (7.5 × 1027 erg), kinetic energy from the increase in the LB width (4 × 1028 erg), or freefall of mass along the coronal loops (6.3 × 1026 erg).
Rapid Decay of a Penumbral Sector Associated with a Strong Light Bridge in Active Region NOAA 12680
Authors: Li Qiaoling , Zhang Li , Yan Xiaoli , Wang Jingcheng , Yang Liheng , Xue Zhike 
Published: January 2023

Abstract
We present observations of the rapid decay of a penumbral sector associated with a strong light bridge (LB) in the active region NOAA 12680 by analyzing the scattered light-corrected Solar Dynamics Observatory/Helioseismic and Magnetic Imager data. At the beginning of penumbral decay, some dark structures gradually broke away from the umbra to which they were attached. The intensity, vertical field strength, and magnetic inclination of the dark structures are intermediate between those of the umbra and penumbra. And a strong LB formed in the umbra, which originated from the intrusion of neighboring penumbral filaments. With the formation of an LB, the total magnetic flux in the whole penumbra decreased, and a penumbral sector of the sunspot rapidly disappeared on one side of the LB. After performing a partition analysis of the penumbra, it was found that the decay rate in this region of the penumbral sector is significantly accelerated after the appearance of an outward motion of magnetic flux along the LB. The area of this penumbral sector decreased from 21–16 MSH in 4 hr. The reduction in area in this penumbral sector is accompanied by a large decay rate of the magnetic flux, 2.5 × 1019 Mx hr−1. These results suggest that the rapid decay of the penumbral sector is associated with the LB. The appearance of dark structures in the penumbra and the strong LB in the umbra may offer a hint that the origin of massive flux migration from the sunspot umbra may have accelerated the decay of the sunspot.
WISE Green Objects (WGOs): The Massive Star Candidates in the Whole Galactic Plane (∣b∣ < 2°)
Authors: Zhang Chang , Zhang Guo-Yin , Li Jin-Zeng , Yuan Jing-Hua 
Published: January 2023

Abstract
Massive young stellar objects (MYSOs) play a crucial role in star formation. Given that MYSOs were previously identified based on the extended structure and the observational data for them is limited, screening the Wide-field Infrared Survey Explorer (WISE) objects showing green features (for the common coding of the 4.6 μm band as the green channel in three-color composite WISE images) will yield more MYSO candidates. Using WISE images in the whole Galactic plane (0° < l < 360° and ∣b∣ < 2°), we identified sources with strong emissions at the 4.6 μm band, then according to morphological features divided them into three groups. We present a catalog of 2135 WISE Green Objects (WGOs). 264 WGOs have an extended structure. 1366 WGOs show compact green features but without extended structure. 505 WGOs have neither extended structure nor green features, but the intensity at 4.6 μm is numerically at least 4.5 times that of 3.4 μm. According to the analysis of the coordinates of WGOs, we find WGOs are mainly distributed in ∣l∣ < 60°, coincident with the position of the giant molecular clouds in ∣l∣ > 60°. Matching results with various masers show that those three groups of WGOs are at different evolutionary stages. After crossmatching WGOs with published YSO survey catalogs, we infer that ∼50% of WGOs are samples of newly discovered YSOs. In addition, 1260 WGOs are associated with Hi-GAL sources, according to physical parameters estimated by spectral energy distribution fitting, of which 231 are classified as robust MYSOs and 172 as candidate MYSOs.
Le rôle des maréchaux de la Grande Guerre dans la promotion des commandeurs du désastre de juin 1940
Authors: Schiavon Max 
Published: January 2023

Les maréchaux de la Première Guerre mondiale, incarnations de la victoire et objets d’une extraordinaire glorification dans l’entre-deux-guerres, ont soutenu ou poussé vers la haute hiérarchie militaire des « poulains » qui assumeront de hautes responsabilités au cours de la Seconde Guerre mondiale. Qu’en était-il de ce lien ? Cette filiation a-t-elle joué un rôle dans la défaite de 1940 ?
Les phénix
Authors: Yvelin Maxime 
Published: January 2023

S’élever est au cœur de l’expérience du soldat : cela sonne comme une évidence. Mais quels en sont les mécanismes ? À travers le témoignage d’une passation de commandement, le chef d’escadron Maxime Yvelin montre en quoi la vie militaire est une perpétuelle élévation collective.
Notes sur Diderot et les simulacres errants
Authors: Sarrasin Robichaud Philippe 
Published: January 2023

À la fois nécessaire à la pensée humaine et potentiellement illusoire, le simulacre est une entité trouble chez Diderot. Si, comme le « mot », il s’oppose à la « chose », il n’en fait pas moins partie du monde matériel. Proche des écrits d’Épicure et de son disciple Lucrèce, la conception de l’encyclopédiste en fait une sorte de bruissement du réel. Il s’agit d’une voix à écouter, mais avec laquelle il est nécessaire de dialoguer de manière curieuse et critique afin de ne pas en faire une sentence univoque qui mènerait infailliblement à l’idolâtrie.
Suzanne simulacre
Authors: Igalens Jean-Christophe 
Published: January 2023

Cet article s’intéresse aux simulacres à apparence humaine évoqués dans La Religieuse de Diderot pour montrer les relations qui les unissent et interpréter ainsi la signification de ces images : des enjeux essentiels de l’œuvre s’y condensent, le roman militant et pathétique s’y articule avec les paradoxes qui déjouent et complexifient, sans cependant les abolir, ses oppositions structurantes (liberté/aliénation ; innocente passive/persécutrices actives ; naïveté/séduction, etc.). L’image d’une Suzanne-automate est associée à la représentation de l’aliénation, depuis les vœux que le personnage prononce en étant « physiquement aliénée » jusqu’à la répétition machinale des gestes du couvent après son évasion. Le terme de « simulacre » apparaît à propos des images peintes et en particulier des portraits, associé à une opposition cruciale entre les images qui laissent froid et celles qui affectent. L’écriture romanesque de Diderot impose alors de s’interroger non seulement sur la séduction ambivalente d’une Suzanne-tableau, mais bien sur le pouvoir d’une Suzanne-simulatrice, d’une Suzanne-pantomime. Les comparaisons avec une statue concentrent enfin les relations problématiques du personnage et de la narratrice avec le désir. Si la réduction de Suzanne à un simulacre dit la dépossession de soi à laquelle le personnage semble condamné, le réinvestissement du simulacre par Suzanne-tableau et Suzanne-pantomime constitue aussi la manifestation romanesque d’une résistance à cette dépossession.