bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH INTELLECTUAL CAPITAL TERHADAP KINERJA KEUANGAN DAN NILAI PASAR PERUSAHAAN YANG LISTED DI JAKARTA ISLAMIC INDEX
Authors: Usman Halim , Mustafa Sri Wahyuni 
Published: February 2020

This study aims to examine the effect of intellectual capital on financial performance and market value of the company. The intellectual capital variable uses three proxies, namely employed capital efficiency, human capital efficiency and structural capital efficiency, while the company's financial performance variable uses return on equity proxy and market to book ratio to proxy the company's market value. The object of this research is companies included in the Jakarta Islamic Index 2011-2017 period. Sampling is done by purposive sampling. The data analysis used is regression analysis to examine the effect of intellectual capital on financial performance and market value of the company. The results showed that intellectual capital had no effect on financial performance so that it affected the company's market value.

Penelitian ini bertujuan untuk menguji pengaruh intellectual capital terhadap kinerja keuangan dan nilai pasar perusahaan. Variabel intellectual capital menggunakan tiga proksi, yakni capital employed efficiency, human capital efficiency dan structural capital efficiency sedangkan untuk variabel kinerja keuangan perusahaan menggunakan proksi return on equity dan market to book ratio untuk proksi nilai pasar perusahaan. Objek dari penelitian ini adalah perusahaan yang masuk dalam Jakarta Islamic Index periode 2011-2017. Pengambilan sampel dilakukan dengan purposive sampling. Adapun analisis data yang digunakan adalah analsis regresi untuk menguji pengaruh intellectual capital terhadap kinerja keuangan dan nilai pasar perusahaan. Hasil penelitian menunjukkan bahwa intellectual capital tidak berpengaruh terhadap kinerja keuangan sehingga namun berpengaruh terhadap nilai pasar perusahaan
Benzyne in V4334 Sqr: A Quest for the Ring with SOFIA/EXES
Authors: Woodward C. E. , Evans A. , Richter M. , DeWitt C. N. , Montiel E. , Banerjee D. P. K. , Clayton G. C. , Eyres S. P. S. , Gehrz R. D. , Hinkle K. H. , Joyce R. R. , Liimets T. , Starrfield S. , Wagner R. M. , Worters H. 
Published: February 2020

Abstract
Large aromatic molecules are ubiquitous in both circumstellar and interstellar environments. Detection of small aromatic molecules, such as benzene (C6H6) and benzyne (C6H4), are rare in astrophysical environments. Detection of such species will have major implications for our understanding of the astrochemistry involved in the formation of the molecules necessary for life, including modeling the chemical pathways to the formation of larger hydrocarbon molecules. We conducted a search for the infrared 18 μm spectral signature of benzyne in V4334 Sgr with the Stratospheric Observatory for Infrared Astronomy (SOFIA)/Echelon-Cross-Echelle Spectrograph (EXES) finding no evidence for a feature at the sensitivity of our observations.
The Role of Environment in Galaxy Evolution in the SERVS Survey. I. Density Maps and Cluster Candidates
Authors: Krefting Nick , Sajina Anna , Lacy Mark , Nyland Kristina , Farrah Duncan , Darvish Behnam , Duivenvoorden Steven , Duncan Ken , Gonzalez-Perez Violeta , del P. Lagos Claudia , Oliver Seb , Shirley Raphael , Vaccari Mattia 
Published: February 2020

Abstract
We use photometric redshifts derived from new u-band through 4.5 μm Spitzer IRAC photometry in the 4.8 deg2 of the XMM-LSS field to construct surface density maps in the redshift range of 0.1–1.5. Our density maps show evidence for large-scale structure in the form of filaments spanning several tens of megaparsecs. Using these maps, we identify 339 overdensities that our simulated light-cone analysis suggests are likely associated with dark matter halos with masses, M
halo, log(M
halo/M
⊙) > 13.7. From this list of overdensities we recover 43 of 70 known X-ray-detected and spectroscopically confirmed clusters. The missing X-ray clusters are largely at lower redshifts and lower masses than our target log(M
halo/M
⊙) > 13.7. The bulk of the overdensities are compact, but a quarter show extended morphologies that include likely projection effects, clusters embedded in apparent filaments, and at least one potential cluster merger (at z ∼ 1.28). The strongest overdensity in our highest-redshift slice (at z ∼ 1.5) shows a compact red galaxy core, potentially implying a massive evolved cluster.
Statistical Study of Hard X-Ray Emitting Electrons Associated with Flare-related Coronal Jets
Authors: Musset Sophie , Jeunon Mariana , Glesener Lindsay 
Published: February 2020

Abstract
We present the statistical analysis of 33 flare-related coronal jets, and discuss the link between the jet and the flare properties in these events. We selected jets that were observed between 2010 and 2016 by the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) that are temporally and spatially associated with flares observed by the Reuven Ramaty High Energy Solar Spectrometric Imager (RHESSI). For each jet, we calculated the jet duration and projected velocity in the plane of sky. The jet duration distribution has a median of 18.8 minutes. The projected velocities are between 31 and 456 km s−1 , with a median at 210 km s−1. For each associated flare, we performed X-ray imaging and spectroscopy and identify nonthermal emission. Nonthermal emission was detected in only 1/4 of the events considered. We did not find a clear correlation between the flare thermal energy or soft X-ray (SXR) peak flux and the jet velocity or jet duration. There is no preferential time delay between the flare and the jet. The X-ray emission is generally located at the base of the jet. The analysis presented in this paper suggests that the flare and jet are part of the same explosive event, that the jet is driven by the propagation of an Alfvénic perturbation, and that the energy partition between flare and jets varies substantially from one event to another.
Optical Transmission Spectra of Hot Jupiters: Effects of Scattering
Authors: Sengupta Sujan , Chakrabarty Aritra , Tinetti Giovanna 
Published: February 2020

Abstract
We present new grids of transmission spectra for hot Jupiters by solving the multiple-scattering radiative transfer equations with non-zero scattering albedo instead of using the Beer–Bouguer–Lambert law for the change in the transmitted stellar intensity. The diffused reflection and transmission due to scattering increase the transmitted stellar flux resulting, in a decrease in the transmission depth. Thus, we demonstrate that scattering plays a double role in determining the optical transmission spectra—increasing the total optical depth of the medium and adding the diffused radiation due to scattering to the transmitted stellar radiation. The resulting effects yield an increase in the transmitted flux and hence a reduction in the transmission depth. For a cloudless planetary atmosphere, Rayleigh scattering albedo alters the transmission depth up to about 0.6 μm, but the change in the transmission depth due to forward scattering by cloud or haze is significant throughout the optical and near-infrared regions. However, at wavelengths longer than about 1.2 μm, the scattering albedo becomes negligible, hence the transmission spectra match with that calculated without solving the radiative transfer equations. We compare our model spectra with existing theoretical models and find significant differences at wavelengths shorter than one micron. We also compare our models with observational data for a few hot Jupiters, which may help with constructing better retrieval models in the future.
Reconstructing the Observed Ionizing Photon Production Efficiency at z ∼ 2 Using Stellar Population Models
Authors: Nanayakkara Themiya , Brinchmann Jarle , Glazebrook Karl , Bouwens Rychard , Kewley Lisa , Tran Kim-Vy , Cowley Michael , Fisher Deanne , Kacprzak Glenn G. , Labbe Ivo , Straatman Caroline 
Published: February 2020

Abstract
The ionizing photon production efficiency, ξ
ion, is a critical parameter that provides a number of physical constraints to the nature of the early universe, including the contribution of galaxies to the timely completion of the reionization of the universe. Here, we use KECK/MOSFIRE and ZFOURGE multiband photometric data to explore the ξ
ion of a population of galaxies at z ∼ 2 with

. Our 130 Hα detections show a median

of 24.8 ± 0.5 when dust corrected using a Calzetti et al. dust prescription. Our values are typical of mass/magnitude selected ξ
ion values observed in the z ∼ 2 universe. Using BPASSv2.2.1 and Starburst99 stellar population models with simple parametric star formation histories (SFH), we find that even with models that account for effects of stellar evolution with binaries/stellar rotation, model galaxies at

have low Hα equivalent widths (EWs) and redder colors compared to our z ∼ 2 observed sample. We find that introducing starbursts to the SFHs resolve the tension with the models; however, due to the rapid time evolution of ξ
ion, Hα EWs, and rest-frame optical colors, our Monte Carlo simulations of starbursts show that random distributions of starbursts in evolutionary time of galaxies are unlikely to explain the observed distribution. Thus, either our observed sample is specially selected based on their past SFH, or stellar models require additional mechanisms to reproduce the observed high UV luminosity of galaxies for a given production rate of hydrogen ionizing photons.
An Extremely Massive Quiescent Galaxy at z = 3.493: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models*
Authors: Forrest Ben , Annunziatella Marianna , Wilson Gillian , Marchesini Danilo , Muzzin Adam , Cooper M. C. , Marsan Z. Cemile , McConachie Ian , Chan Jeffrey C. C. , Gomez Percy , Kado-Fong Erin , Barbera Francesco La , Labbé Ivo , Lange-Vagle Daniel , Nantais Julie , Nonino Mario , Peña Theodore , Saracco Paolo , Stefanon Mauro , van der Burg Remco F. J. 
Published: February 2020

Abstract
We present spectra of the most massive quiescent galaxy yet spectroscopically confirmed at z > 3, verified via the detection of Balmer absorption features in the H- and K-bands of Keck/MOSFIRE. The spectra confirm a galaxy with no significant ongoing star formation, consistent with the lack of rest-frame UV flux and overall photometric spectral energy distribution. With a stellar mass of

at z = 3.493, this galaxy is nearly three times more massive than the highest redshift spectroscopically confirmed absorption-line-identified galaxy known. The star formation history of this quiescent galaxy implies that it formed >1000 M
⊙ yr−1 for almost 0.5 Gyr beginning at z ∼ 7.2, strongly suggestive that it is the descendant of massive dusty star-forming galaxies at 5 < z < 7 recently observed with ALMA. While galaxies with similarly extreme stellar masses are reproduced in some simulations at early times, such a lack of ongoing star formation is not seen there. This suggests the need for a quenching process that either starts earlier or is more rapid than that currently prescribed, challenging our current understanding of how ultra-massive galaxies form and evolve in the early universe.
Orphelines ou sœurs ?
Authors: Hobson Faure Laura 
Published: February 2020

Peu d’attention historique a été accordée aux frères et sœurs en tant qu’unités familiales, pendant et après la Shoah. Les historiens ont tendance à considérer les « orphelins de la Shoah » comme des cas individuels. Cet article, établi à partir d’entretiens d’histoire orale, de dossiers sociaux, de papiers privés et d’archives organisationnelles françaises et américaines, utilise une approche microhistorique. À partir de l’expérience de deux sœurs ayant survécu à la Shoah en France et ayant ensuite immigré aux États-Unis, il questionne leur capacité à rester ensemble. L’article affirme que les orphelins ne sont pas aussi seuls que nous le pensions mais qu’il existe d’importantes différences dans la façon dont les frères et sœurs abordent et interagissent avec leur passé. Ainsi une interaction soutenue avec nos sujets de recherche peut-elle enrichir les résultats historiques.
Les relations franco-polonaises face aux événements de mars 1968 en Pologne
Authors: Weber Pierre-Frédéric 
Published: February 2020

L’année 1968, marquée par une révolte générationnelle dans plusieurs sociétés occidentales, connut aussi des soubresauts dans certains pays socialistes où ils étaient partiellement motivés par d’autres aspirations – essentiellement à plus de liberté. Ainsi, en Pologne, les événements de « mars 68 » constituèrent une césure dans l’histoire de l’après-guerre. Au moment où la diplomatie française cherchait l’ouverture à l’Est en réactivant notamment ses liens traditionnels avec la Pologne, ces troubles du régime polonais mirent à l’épreuve les rapports franco-polonais, mais des facteurs tant intérieurs à la France que dus au contexte international absorbèrent ces turbulences, finalement sans effet majeur sur la suite des relations bilatérales.
Libération homosexuelle et socialisme réel à Berlin-Est
Authors: Kiani Sarah 
Published: February 2020

L’article interroge le concept de « révolution sexuelle » en observant le cadre discursif du premier mouvement homosexuel du bloc de l’Est dans une dynamique comparative avec le mouvement de Berlin-Ouest au cours des années 1970. Si le mouvement de libération homosexuelle apparaît à l’Ouest dans la continuité d’autres luttes sociales, il cherche en RDA à inscrire son projet émancipateur dans celui du « socialisme réel ». Malgré cette différence de cadres sociaux et politiques dans lesquels les deux mouvements évoluent, ils cherchent tous deux à imposer une discussion sur les homosexualités dans un espace public dont ils se sentent exclus. Cet article souligne l’importance des circulations entre les deux côtés du Mur, et plaide pour une analyse de l’histoire de la RDA qui prenne en compte les pratiques des acteurs.
Bromodomain and Extra-Terminal (BET) Domain Protein Inhibitors for Solid Tumor Cancers
Authors: Nguyen Martin V. , Loof Lydia , Falchook Gerald S. 
Published: February 2020

Abstract
The bromodomain and extraterminal (BET) domain protein family is involved in the process of transcription of genetic information. The BET protein family includes BRD2, BRD3, BRD4, and bromodomain testis-specific protein. BET protein alterations are associated with some solid tumor cancers, including nuclear protein in testis midline carcinoma. BET protein has a role in carcinogenesis and in the regulation of the cell cycle. A number of BET inhibitors have entered clinical trials. This review discusses the results of BET inhibitor clinical trials in solid tumor cancers.
Classification of anatomical variants of maxillary sinus shapes and symmetry using computerized tomographic imaging
Authors: Aliu Abdulhameed , Mohammad Ma’aji S. , Sirajo Bello S. , Ibrahim Ahmad M. , Abdullahi Zagga D. 
Published: February 2020

Background:
The maxillary sinus is characterized by a considerable variation in sizes and shapes and between the right and left sides. Due to easy access to all its walls and surfaces, imaging via computerized tomography (CT) has enhanced the quality and quantity of information obtainable from the assessment of the maxillary sinus.

Aim:
To determine normal variations in shapes and symmetry of the maxillary sinus using CT.

Methods:
A total of 130 subjects comprising 79 males and 51 females, between the ages of 20 and 80 years, with normal maxillary sinus CT anatomy, who had head CT scans carried out at the Radiology Department of the Usmanu Danfodiyo University Teaching Hospital (UDUTH) Sokoto, over a period of five years, were used for this study. Images were taken with a GE Bright Speed Multidetector Helical CT (GE Healthcare, USA, 2005) Scanner, while films were viewed on the computer monitor. Variations in shapes of the maxillary sinus were identified on axial images and classified based on their resemblance to known shapes of solids. Data were analyzed using Minitab 16.0 statistical package (Minitab inc. USA).

Results:
Five distinct shapes of the maxillary sinus were identified. These were: irregular in two subjects (0.77%) (right = 1 and left = 1); oval in three subjects (1.15%) (right = 2 and left = 1); quadrangular in three subjects (1.15%) (right = 2 and left = 1); spherical in 61 subjects (23.46%) (right = 30 and left = 31); and triangular 191 (73.46%) (right = 95 and left = 96). Shapes were symmetrical in 85.38% and asymmetrical in 14.62% of subjects.

Conclusion:
Five normal but distinct shapes of the maxillary sinus were identified, with the predominant shape, being the triangular type, and sinuses of individuals were frequently symmetrical in shape.
ENTEROPARASITES, DEMOGRAPHIC PROFILE, SOCIOECONOMIC STATUS AND EDUCATION LEVEL IN THE RURAL POPULATION OF THE RECÔNCAVO OF BAHIA, BRAZIL
Authors: Bispo Reis Leonardo , Da Silva Santos Raíssa , Henrique Silva Mota Luiz , De Souza Almeida Jamille , Merces Oliveira e Oliveira Juliana , Dos Santos Andrade Raoni , Andrade dos Santos Glauber , Lucia Moreno Amor Ana 
Published: February 2020

Demographic and social studies, as well as economic and cultural factors in a community are important regarding public health. This study identified demographic, socioeconomic and cultural aspects correlated with intestinal parasites in the population of Santo Antônio de Jesus, Bahia-Brazil, from July to October 2015. 53 semi-structured questionnaires were applied to the rural population of the municipality with previous clarification on the purpose of the study. There were questions related to the individual’s gender, family income and parental level of education. Laboratory parasitological analyzes were performed to investigate enteroparasites and produced the following results: 53.7% (n=58) were female; 62.8% (n=66) with monthly family income lower or equal to the minimum wage and 48% (n=48) of adults with incomplete basic education. The main enteroparasites found in this population were: Iodamoeba butschlii, Entamoeba histolytica/Entamoeba dispar complex, Giardia intestinalis, Entamoeba coli and Endolimax nana in addition to some geohelminths, such as hookworms and Enterobius vermicularis. The profile visualized can be understood as a risk factor for the development of certain parasitic infections that are intrinsically associated to the social and economic aspects of vulnerable populations.KEY WORDS: Teenager; adult; child; parasitic diseases.
A randomized, controlled trial of transcutaneous tibial nerve stimulation to treat overactive bladder and neurogenic bladder patients
Authors: Welk Blayne , McKibbon Mary 
Published: February 2020

Introduction: We aimed to determine if transcutaneous tibial nerve stimulation (TTNS) is effective at treating overactive bladder (OAB) symptoms among neurogenic and non-neurogenic patients.
Methods: We conducted a randomized, double-blind, sham-controlled study. Adult patients were recruited from one of two groups: 1) women with OAB; and 2) patients with neurogenic disease and bladder symptoms. The intervention was stimulation of the posterior tibial nerve, for 30 minutes, three times per week for 12 weeks at home using transcutaneous patch electrodes. The primary outcome was improvement of the patient perception of bladder condition (PPBC). We used ANCOVA (with adjustment for baseline values) and followed the intention-to-treat principle; we reported marginal means (MM) and a p<0.05 was considered significant.
Results: We recruited 50 patients (OAB n=20, neurogenic bladder n=30); 24 were allocated to the sham group and 26 to the active TTNS group. Baseline characteristics in both groups were similar. At the end of the study, there was no significant difference in the PPBC between sham or active groups: 13% (3/24) of sham patients and 15% (4/26) of active TTNS patients were responders (p=0.77), and the marginal mean of the end-of-study PPBC score was 3.3 (95% confidence interval [CI] 2.8–3.7) vs. 2.9 (95% CI 2.5–3.4), respectively (p=0.30). Similarly, there were no significant differences in secondary outcomes (24-hour pad weight, voiding diary parameters, or condition-specific patient-reported outcomes). The results were similar within the OAB and neurogenic bladder subgroups.
Conclusions: TTNS does not appear to be effective for treating urinary symptoms of people with OAB or neurogenic bladder dysfunction.
Psychosociale aspecten van crisismanagement: taken en uitdagingen voor bestuur en beleid
Authors: Dückers Michel , van Hoof Wera , Holsappel Jorien 
Published: February 2020

Psychosocial aspects of crisis management: Tasks and challenges for public leadership and policy
Crises and disasters can seriously affect the health, well-being and functioning of the people involved. From a governance perspective, it is important that public leaders and crisis managers are aware of what the psychosocial dimension of crisis management entails. The objective of the current contribution is to analyse dilemmas and challenges described in evaluations of crises that occurred in the Netherlands between 2012 and 2016. Thirty-six evaluations were analysed against the background of a theoretical framework combining crisis leadership tasks and psychosocial support principles along the crisis life cycle. Public leaders and crisis managers had to deal with classical crisis problems concerning coordination, collaboration and communication. Other recurring themes were linked to social media, and the tension between tasks such as meaning making (social recognition), account giving and learning. Moreover, the analysis illustrates how difficult it is to gain insight into the needs, problems and vulnerabilities of the individuals and groups affected.
‘Gelukkig is geen ramp ontstaan’
Authors: Blommers Michael 
Published: February 2020

‘Fortunately no disaster has occurred’ – meeting the needs of victims after big fires
Based on a retrospective analysis of six large scale and fatal fires in the Netherlands, an improvement in terms of meeting the needs of victims can be seen. A comparison of the legal settlement of these fires shows mayor differences in the fulfilling of different aspects of social justice that are identified in social psychology. Two victim needs commonly associated with retributive justice – financial compensation and a thorough, neutral investigation into the causes of the disaster – were fulfilled to a higher degree after the most recent fires than after those that occurred decades ago. The legal settlement after the New Year’s fire in Volendam (2001) appears – at least on paper – to have been more just from the victim’s point of view than the ones after the other incidents. Empirical research into the experienced social justice after the New Year’s fire can be valuable to assess the factors that can lead to a just settlement after disasters.