bluuebunny/crossref_metadata_2025_split huggingface dataset:
FAKTOR-FAKTOR YANG MEMPENGARUHI PERENCANAAN SUMBER DAYA MANUSIA: LINGKUNGAN EXTERNAL, KEPUTUSAN-KEPUTUSAN ORGANISASIONAL, PERSEDIAAN KARYAWAN (LITERATURE REVIEW MSDM)
Authors: Salsabilah Firyaal , Fahmi Setiawan Moch , Prasista Whardani Safa 
Published: January 2023

Sumber daya manusia (SDM) yaitu sesuatu faktor penting, bahkan tidak dapat dilepaskan dari sebuah organisasi, baik institusi maupun perusahaan. SDM juga merupakan kunci yang menentukan perkembangan perusahaan. Pada hakikatnya, SDM berupa manusia yang dipekerjakan di sebuah organisasi sebagai penggerak, pemikir serta perencana untuk mencapai sebuah tujuan organisasi. Karyawan bukan sebagai sumber daya saja, melainkan lebih berupa modal atau aset bagi institusi atau organisasi. Karena itu kemudian muncullah istilah baru di luar H.R. (Human Resources), yaitu H.C. atau Human Capital. Di sini SDM dilihat bukan sekadar sebagai aset utama, tetapi aset yang bernilai dan dapat dilipatgandakan, dikembangkan (bandingkan dengan portfolio investasi) dan juga bukan sebaliknya sebagai liability (beban,cost). Di sini perspektif SDM sebagai investasi bagi institusi atau organisasi lebih mengemuka. Maka dari pada itu perencanaan sumber daya manusia harus di jalankan pada perusahaan, agar tidak adanya kerugian dari perusahaan tersebut. Agar dalam pelaksanaan perencanaan SDM bisa berhasil, setidaknya terdapat beberapa aspek perencanaan SDM yang harus diperhatikan yaitu: (1) berapa perkiraan jumlah karyawan yang dibutuhkan (forecasting of employees), (2) identifikasi SDM yang tersedia dalam organisasi (human resource audit), (3) analisis keseimbangan penawaran dan permintaan (demand and suplay analysis), (4) menjalankan program aksi (action program).
PENGARUH HARGA, PROMOSI DAN BRAND IMAGE TERHADAP KEPUTUSAN PEMBELIAN (LITERATURE REVIEW STRATEGI MARKETING MANAJEMENT)
Authors: Nurliyanti Nurliyanti , Anestesia Arnis Susanti  , Baruna Hadibrata  
Published: January 2023

Riset terdahulu atau riset yang relevan sangat penting dalam suatu riset atau artikel ilmiah. Riset terdahulu atau riset yang relevan berfungsi untuk memperkuat teori dan penomena hubungan atau pengaruh antar variable. Artikel ini mereview pengaruh harga, promosi dan brand image terhadap keputusan pembelian, suatu studi literatur Strategic Marketing Management. Tujuan penulisan artikel ini guna membangun hipotesis pengaruh antar variabel untuk digunakan pada riset selanjutnya. Hasil artikel literature review ini adalah: 1) harga berpengaruh terhadap keputusan pembelian; 2) promosi berpengaruh terhadap keputusan pembelian; dan 3) brand image berpengaruh terhadap keputusan pembelian.
Kepler-102: Masses and Compositions for a Super-Earth and Sub-Neptune Orbiting an Active Star
Authors: Brinkman Casey L. , Cadman James , Weiss Lauren , Gaidos Eric , Rice Ken , Huber Daniel , Claytor Zachary R. , Bonomo Aldo S. , Buchhave Lars A. , Cameron Andrew Collier , Cosentino Rosario , Dumusque Xavier , Martinez Fiorenzano Aldo F. , Ghedina Adriano , Harutyunyan Avet , Howard Andrew , Isaacson Howard , Latham David W. , López-Morales Mercedes , Malavolta Luca , Micela Giuseppina , Molinari Emilio , Pepe Francesco , Philips David F. , Poretti Ennio , Sozzetti Alessandro , Udry Stéphane 
Published: January 2023

Abstract
Radial velocity (RV) measurements of transiting multiplanet systems allow us to understand the densities and compositions of planets unlike those in the solar system. Kepler-102, which consists of five tightly packed transiting planets, is a particularly interesting system since it includes a super-Earth (Kepler-102d) and a sub-Neptune-sized planet (Kepler-102e) for which masses can be measured using RVs. Previous work found a high density for Kepler-102d, suggesting a composition similar to that of Mercury, while Kepler-102e was found to have a density typical of sub-Neptune size planets; however, Kepler-102 is an active star, which can interfere with RV mass measurements. To better measure the mass of these two planets, we obtained 111 new RVs using Keck/HIRES and Telescopio Nazionale Galileo/HARPS-N and modeled Kepler-102's activity using quasiperiodic Gaussian process regression. For Kepler-102d, we report a mass upper limit M

d
< 5.3 M
⊕ (95% confidence), a best-fit mass M

d
= 2.5 ± 1.4 M
⊕, and a density ρ

d
= 5.6 ± 3.2 g cm−3, which is consistent with a rocky composition similar in density to the Earth. For Kepler-102e we report a mass M

e
= 4.7 ± 1.7 M
⊕ and a density ρ

e
= 1.8 ± 0.7 g cm−3. These measurements suggest that Kepler-102e has a rocky core with a thick gaseous envelope comprising 2%–4% of the planet mass and 16%–50% of its radius. Our study is yet another demonstration that accounting for stellar activity in stars with clear rotation signals can yield more accurate planet masses, enabling a more realistic interpretation of planet interiors.
Cosmic Evolution of Gas and Star Formation
*
Authors: Scoville Nick , Faisst Andreas , Weaver John , Toft Sune , McCracken Henry J. , Ilbert Olivier , Diaz-Santos Tanio , Staguhn Johannes , Koda Jin , Casey Caitlin , Sanders David , Mobasher Bahram , Chartab Nima , Sattari Zahra , Capak Peter , Vanden Bout Paul , Bongiorno Angela , Vlahakis Catherine , Sheth Kartik , Yun Min , Aussel Herve , Laigle Clotilde , Masters Dan 
Published: January 2023

Abstract
Atacama Large Millimeter/submillimeter Array (ALMA) observations of the long-wavelength dust continuum are used to estimate the gas masses in a sample of 708 star-forming galaxies at z = 0.3−4.5. We determine the dependence of gas masses and star formation efficiencies (SFEs; SFR per unit gas mass) on redshift (z), M
*, and star formation rate (SFR) relative to the main sequence (MS). We find that 70% of the increase in SFRs of the MS is due to the increased gas masses at earlier epochs, while 30% is due to increased efficiency of star formation (SF). For galaxies above the MS this is reversed—with 70% of the increased SFR relative to the MS being due to elevated SFEs. Thus, the major evolution of star formation activity at early epochs is driven by increased gas masses, while the starburst activity taking galaxies above the MS is due to enhanced triggering of star formation (likely due to galactic merging). The interstellar gas peaks at z = 2 and dominates the stellar mass down to z = 1.2. Accretion rates needed to maintain continuity of the MS evolution reach >100 M
⊙ yr−1 at z > 2. The galactic gas contents are likely the driving determinant for both the rise in SF and AGN activity from z = 5 to their peak at z = 2 and subsequent fall at lower z. We suggest that for self-gravitating clouds with supersonic turbulence, cloud collisions and the filamentary structure of the clouds regulate the star formation activity.
Growth of a Massive Black Hole in a Dense Star Cluster Via Tidal Disruption Accretion
Authors: Lee Seungjae , Kim Ji-hoon , Oh Boon Kiat 
Published: January 2023

Abstract
Stars that are tidally disrupted by a massive black hole (MBH) may contribute significantly to the growth of the MBH, especially in dense nuclear star clusters. Yet, this tidal disruption accretion (TDA) of stars onto the MBH has largely been overlooked compared to the gas accretion (GA) channel in most numerical experiments until now. In this work, we implement a black hole growth channel via TDA in the high-resolution adaptive mesh refinement code Enzo to investigate its influence on an MBH seed’s early evolution. We find that an MBH seed grows rapidly from 103 to ≳106
M
⊙ in 200 Myr in some of the tested simulations. Compared to an MBH seed that grows only via GA, TDA can enhance the MBH’s growth rate by more than 1 order of magnitude. However, as predicted, TDA mainly helps the early growth of the MBH (from 103–4 to ≲105
M
⊙) while the later evolution is generally dominated by GA. We also observe that the star formation near the MBH is suppressed when TDA is the most active, sometimes with a visible cavity in gas (of size ∼ a few pc) created in the vicinity of the MBH. It is because the MBH may grow expeditiously with both GA and TDA, and the massive MBH could consume its neighboring gas faster than being replenished by gas inflows. Our study demonstrates the need to consider different channels of black hole accretion that may provide clues for the existence of supermassive black holes at high redshifts.
The Behavior of HgMn Stars in the Far UV—Paper 27: HD 1909
Authors: Monier Richard 
Published: January 2023

Abstract
The analysis of two spectra of the spectroscopic binary B9 Hg star HD 1909 recorded by the SWP camera on board the International Ultraviolet Explorer reveals one instance of variations of the far-ultraviolet flux of this star from 1300 up to 2000 Å. The first TESS lightcurve of HD 1909 on the MAST website is periodic with a period close to 7 days which is very close to an earlier period found for the variations of the Strömgren index u. The FUV variations, which occur over about 5 yr, could be caused by the motion of the lower mass companion.
Impacts of Organic Ice Condensation on the Optical Properties of Haze on Pluto
Authors: Wang Jingyu , Fan Siteng , Liu Chao , Natraj Vijay , Young Leslie A. , Yung Yuk L. 
Published: January 2023

Abstract
The flyby of the New Horizons spacecraft in 2015 July revealed an unexpected cold atmosphere of Pluto and confirmed the existence of its atmospheric haze. The observed and simulated vertical profiles of chemical species and microphysical processes suggest that the haze particles in Pluto’s middle and lower atmosphere may contain organic ice condensation. Such organic ice components can potentially affect Pluto’s haze chemistry and optical properties, as well as its energy budget. This study investigates the influence of the ice components on the scattering properties of Pluto’s haze by comparing New Horizons observations and simulated particle scattering properties. Comprehensive tests are performed for various haze particle parameters, including their size, chemical component, ice content, and morphology. Scattering properties of these ice-bearing haze particles are calculated by a discrete dipole approximation method and compared to multispectral observations obtained by four New Horizons instruments in spectral regions ranging from the ultraviolet to the near-infrared. The results indicate that the inclusion of the organic ice component leads to higher ratios of backscattering in the visible to extinction in the ultraviolet and provides better agreement with observations compared to monodispersed homogeneous aggregates. But it alone is not sufficient to explain the observed forward scattering values in the visible and near-infrared. Therefore, other scattering sources and/or mechanisms are still required to explain the full set of scattering observations. Further observations, as well as laboratory measurements and numerical tests, are anticipated to improve our understanding of the morphology and ice content of Pluto’s haze.
Pluto’s Surface Mapping Using Unsupervised Learning from Near-infrared Observations of LEISA/Ralph
Authors: Emran A. , Dalle Ore C. M. , Ahrens C. J. , Khan M. K. H. , Chevrier V. F. , Cruikshank D. P. 
Published: January 2023

Abstract
We map the surface of Pluto using an unsupervised machine-learning technique using the near-infrared observations of the LEISA/Ralph instrument on board NASA’s New Horizons spacecraft. The principal-component-reduced Gaussian mixture model was implemented to investigate the geographic distribution of the surface units across the dwarf planet. We also present the likelihood of each surface unit at the image pixel level. Average I/F spectra of each unit were analyzed—in terms of the position and strengths of absorption bands of abundant volatiles such as N2, CH4, and CO and nonvolatile H2O—to connect the unit to surface composition, geology, and geographic location. The distribution of surface units shows a latitudinal pattern with distinct surface compositions of volatiles—consistent with the existing literature. However, previous mapping efforts were based primarily on compositional analysis using spectral indices (indicators) or implementation of complex radiative transfer models, which need (prior) expert knowledge, label data, or optical constants of representative end-members. We prove that an application of unsupervised learning in this instance renders a satisfactory result in mapping the spatial distribution of ice compositions without any prior information or label data. Thus, such an application is specifically advantageous for a planetary surface mapping when label data are poorly constrained or completely unknown, because an understanding of surface material distribution is vital for volatile transport modeling at the planetary scale. We emphasize that the unsupervised learning used in this study has wide applicability and can be expanded to other planetary bodies of the solar system for mapping surface material distribution.
Corrigendum: Salvi D, Al-Kandari M, Oliver PG, Berrilli E, Garzia M (2022) Cryptic marine diversity in the northern Arabian Gulf: an integrative approach uncovers a new species of oyster (Bivalvia: Ostreidae), Ostrea oleomargarita. Journal of Zoological Systematics and Evolutionary Research 2022: 7058975. https://doi.org/10.1155/2022/7058975
Authors: Salvi Daniele , Al-Kandari Manal , Oliver P. Graham , Berrilli Emanuele , Garzia Matteo 
Published: January 2023

Here we provide a Code-compliant description of Ostrea oleomargarita Oliver, Salvi, and Al-Kandari, sp. nov as reported in Salvi et al. (2022) and complemented with the ZooBank registration numbers of the publication and of the new species name.
Results of phylogenetic, species delimitation, and morphological analyses on which the systematic assessment of this new species is based can be found in Salvi et al. (2022).
Mejores prácticas y excelencia empresarial. Análisis de una PYME exportadora mexicana
Authors: Arredondo Hidalgo María Guadalupe , Caldera González Diana del Consuelo , Ortega Carrillo Miguel Agustín 
Published: January 2023

L’excellence entrepreneuriale d’une petite entreprise exportatrice mexicaine du secteur de la chaussure, qui existe depuis plus de huit décennies, est analysée. La méthodologie est mixte. Dans la phase quantitative, une enquête basée sur le modèle européen d’excellence (EFQM) a été appliquée. La phase qualitative a consisté en des entretiens semi-structurés. Les résultats montrent que l’entreprise a obtenu 855 points sur l’échelle EFQM (1 000 points). Les critères les mieux évalués sont: la performance des personnes (92,78 %), les partenariats-ressources (92,64 %), la politique et la stratégie (90,33 %). Les critères les moins bien évalués sont: la performance de la société (74,42 %) et les personnes (74,83 %). Nous concluons que cette entreprise est excellente et que le cas est pertinent pour évaluer de meilleures pratiques entrepreneuriales, en reproduisant la méthodologie dans des PME similaires d’Amérique latine.
Recherche en histoire de l’acoustique moderne
Authors: Tkaczyk Viktoria , Ribac François 
Published: January 2023

Dans cet entretien, Viktoria Tkaczyk, directrice de l’équipe « Epistemes of Modern Acoustics » au Max Planck Institute de Berlin traite des travaux en cours, des perspectives de recherche et du tournant sonore dans l’histoire des sciences. Elle présente son groupe de travail et leurs objets de recherche, une série de travaux sur la place du son et de la musique dans les sciences depuis la Révolution scientifique. Elle rend compte de la façon dont émergent une conception et une autre histoire des sciences en donnant à certains acteurs une place qu’ils/elles n’avaient pas et en montrant comment le son a été utilisé, par exemple par Mach, comme un outil de connaissance pour explorer des terrains non soniques, édifier des laboratoires, produire des objets, etc. Elle résume un panorama de travaux, peu connus en France, qui croisent histoire des sciences, sound studies et savoirs de la musique. Musique et son sont abordés sous l’angle de l’histoire des sciences, des mesures et des standardisations ; en même temps, l’histoire des sciences est en quelque sorte « resonorisée ».
Recombinant Human Thrombomodulin Reduces Mortality and Acute Lung Injury Caused by Septic Peritonitis in Rats
Authors: Kono Hiroshi , Hosomura Naohiro , Amemiya Hidetake , Kawaida Hiromichi , Furuya Shinji , Shoda Katsutoshi , Akaike Hidenori , Kawaguchi Yoshihiko , Ichikawa Daisuke 
Published: January 2023

Abstract
This study aimed to investigate the therapeutic effects of recombinant human thrombomodulin (rhTM) on acute lung injury (ALI) caused by sepsis in rats. Rats that underwent cecal ligation and puncture (CLP) were treated with or without rhTM, and then mortality was analyzed. In another set of experiments, ALI was assessed. Furthermore, microthrombosis in the lungs was investigated by immunohistochemistry. Moreover, plasma inflammatory and anti-inflammatory cytokines, such as TNF-α, high-mobility group box chromosomal protein 1 (HMGB-1), and IL-10, were evaluated by ELISA. Production of TNF-α and HMGB-1 by isolated tissue macrophages (Mφs) was assessed in vitro. Mortality after CLP was significantly improved by rhTM treatment. In addition, rhTM treatment improved the wet/dry weight ratio of the lungs, the pulmonary microvascular permeability, and the lung injury scores in animals that underwent CLP. Microthrombosis was detected in the lungs after CLP. These pathophysiological changes were blunted by rhTM treatment. Increased plasma TNF-α and HMGB-1 levels were blunted by rhTM treatment; however, the anti-inflammatory cytokine IL-10 was significantly greater in the rhTM(+) group than in the rhTM(−) group. Increased TNF-α and HMGB-1 production by the tissue Mφs stimulated with LPS were significantly blunted by rhTM treatment in vitro, but the production of IL-10 by the tissue Mφs was not changed in the cells incubated with rhTM. Overall, rhTM improved the mortality caused by septic peritonitis. The possible mechanisms are most likely anti-inflammatory and anticoagulant effects, which lead to the prevention of ALI.
Long Noncoding RNA U90926 Is Induced in Activated Macrophages, Is Protective in Endotoxic Shock, and Encodes a Novel Secreted Protein
Authors: Sabikunnahar Bristy , Caldwell Sydney , Varnum Stella , Hogan Tyler , Cooper Alexei , Lahue Karolyn G , Bivona Joseph J , Cousens Phoebe M , Symeonides Menelaos , Ballif Bryan A , Poynter Matthew E , Krementsov Dimitry N 
Published: January 2023

Abstract
Thousands of long noncoding RNAs are encoded in mammalian genomes, yet most remain uncharacterized. In this study, we functionally characterized a mouse long noncoding RNA named U90926. Analysis of U90926 RNA levels revealed minimal expression across multiple tissues at steady state. However, the expression of this gene was highly induced in macrophages and dendritic cells by TLR activation, in a p38 MAPK- and MyD88-dependent manner. To study the function of U90926, we generated U90926-deficient (U9-KO) mice. Surprisingly, we found minimal effects of U90926 deficiency in cultured macrophages. Given the lack of macrophage-intrinsic effect, we investigated the subcellular localization of U90926 transcript and its protein-coding potential. We found that U90926 RNA localizes to the cytosol, associates with ribosomes, and contains an open reading frame that encodes a novel glycosylated protein (termed U9-ORF), which is secreted from the cell. An in vivo model of endotoxic shock revealed that, in comparison with wild type mice, U9-KO mice exhibited increased sickness responses and mortality. Mechanistically, serum levels of IL-6 were elevated in U9-KO mice, and IL-6 neutralization improved endotoxemia outcomes in U9-KO mice. Taken together, these results suggest that U90926 expression is protective during endotoxic shock, potentially mediated by the paracrine and/or endocrine actions of the novel U9-ORF protein secreted by activated myeloid cells.
Single-Cell Analysis in Blood Reveals Distinct Immune Cell Profiles in Gouty Arthritis
Authors: Wang Maojie , Chen Wenying , Zhang Xiaolin , Mei Liyan , Wu Xiaodong , Chen Xiumin , Yang Zhihua , Gao Kaixin , Huang Huanjie , Huang Runyue 
Published: January 2023

Abstract
Gout is a chronic disease caused by monosodium urate crystal deposition. Previous studies have focused on the resident macrophage, infiltrating monocyte, and neutrophil responses to monosodium urate crystal, yet the mechanisms of the potential involvement of other immune cells remain largely unknown. In this study, we enrolled seven gout patients and five age-matched healthy individuals and applied single-cell mass cytometry to study the distribution of immune cell subsets in peripheral blood. To our knowledge, our study reveals the immune cell profiles of gout at different stages for the first time. We identified many immune cell subsets that are dysregulated in gout and promote gouty inflammation, especially those highly expressing CCR4 and OX40 (TNFR superfamily member 4), including CCR4+OX40+ monocytes, CCR4+OX40+CD56high NK cells, CCR4+OX40+CD4+ NK T cells, and CCR4+CD38+CD4+ naïve T cells. Notably, the plasma levels of CCL17 and CCL22, measured by ELISA, increased in the acute phase of gout and declined in the interval. We also found a clue that Th2-type immune responses may participate in gout pathology. Moreover, the subset of granzyme B+ (GZMB+) CD38+ NK cells is positively correlated with serum urea acid level, and another two γδT subsets, GZMB+CD161+ γδT cells and GZMB+CCR5+ γδT cells, are negatively correlated with erythrocyte sedimentation rate. In sum, gouty arthritis is not a disease simply mediated by macrophages; multiple types of immune cell may be involved in the pathogenesis of the disease. Future research needs to shift attention to other immune cell subsets, such as NK cells and T cells, which will facilitate the identification of novel therapeutic targets.
Algebra Tiles as Physical Manipulatives to Support Students’ Understanding of Linear Equations in One Variable
Authors: Rini Dyah Sinto 
Published: January 2023

To help students in solving the linear equations in one variable, teacher can use a learning media such as algebra tiles. Algebra tiles are square and rectangle-shaped tiles that represent numbers and variables. Algebra tiles consist of three different-size pieces. The smallest tile is square shape and represents ± 1, the other tile is rectangular shape and represents ± x and the largest tile is large square shape that represents ± x2. The pieces are usually colour-coded so that one colour represents positive values and another color represents negative values. This research is a best practice that was conducted at class VII.7 SMPN 18 Tangerang. The aim of this research is to describe how the algebra tiles supports students’ understanding in solving linear equations in one variable. The competence achievement indicators are: modelling algebraic expressions using algebra tiles; solving linear equations in one variable using algebra tiles; solving linear equations in one variable without use algebra tiles. Data collection through photos, videos, worksheet and students’ work. Students did reducing and balancing ways to find the simple form of algebra tiles. The purpose of reducing or balancing of both sides of linear equations in one variable is to get how many square tiles that equals to one rectangular tile. Algebra tiles made students to be easier in solving linear equations in one variable. Students were very happy to learn mathematics using algebra tiles. The algebra tiles supports students’ understanding in solving linear equations in one variable.