bluuebunny/crossref_metadata_2025_split huggingface dataset:
Retrospective validation of whole genome sequencing-enhanced surveillance of listeriosis in Europe, 2010 to 2015
Authors: Van Walle Ivo , Björkman Jonas Torgny , Cormican Martin , Dallman Timothy , Mossong Joël , Moura Alexandra , Pietzka Ariane , Ruppitsch Werner , Takkinen Johanna ,   European Listeria WGS typing group
Published: August 2018

Background and aim
The trend in reported case counts of invasive Listeria monocytogenes (Lm), a potentially severe food-borne disease, has been increasing since 2008. In 2015, 2,224 cases were reported in the European Union/European Economic Area (EU/EEA). We aimed to validate the microbiological and epidemiological aspects of an envisaged EU/EEA-wide surveillance system enhanced by routine whole genome sequencing (WGS). Methods: WGS and core genome multilocus sequence typing (cgMLST) were performed on isolates from 2,726 cases from 27 EU/EEA countries from 2010–15. Results: Quality controls for contamination, mixed Lm cultures and sequence quality classified nearly all isolates with a minimum average coverage of the genome of 55x as acceptable for analysis. Assessment of the cgMLST variation between six different pipelines revealed slightly less variation associated with assembly-based analysis compared to reads-based analysis. Epidemiological concordance, based on 152 isolates from 19 confirmed outbreaks and a cluster cutoff of seven allelic differences, was good (sensitivity > 95% for two cgMLST schemes of 1,748 and 1,701 loci each; PPV 58‒68%). The proportion of sporadic cases was slightly below 50%. Of remaining isolates, around one third were in clusters involving more than one country, often spanning several years. Detection of multi-country clusters was on average several months earlier when pooling the data at EU/EEA level, compared with first detection at national level. Conclusions: These findings provide a good basis for comprehensive EU/EEA-wide, WGS-enhanced surveillance of listeriosis. Time limits should not be used for hypothesis generation during outbreak investigations, but should be for analytical studies.
THE EFFECT OF FINANCIAL PERFORMANCE OF COMPANIES ON SHARE RETURN IN MANUFACTURING COMPANIES LISTED IN INDONESIA STOCK EXCHANGE YEAR 2014 -2016
Authors: Paryanto Paryanto , Sumarsono N. Dicky 
Published: August 2018

This study aims to determine the effect of parsiil and simultaneous price book value, price earnings ratio, earnings per share and dividend pay out ratio to stock returns on manufacturing companies listed in Indonesia Stock Exchange 2014-2016. The technique of determining the sample in this research is by using purposive sampling. There are several criteria that must be met by companies listed in Indonesia Stock Exchange to be a sample in this research. This research method uses multiple regression analysis which is used to know the influence of independent variable to dependent variable together and partially. The test t is used to test the influence of each price book value variable, price earning ratio, earnings per share and dividend pay out ratio) to stock return variables. Statistical test F aims to examine the influence of price book value variable, price earning ratio, earnings per share and dividend pay out ratio) together to stock return variables. Test R2 (Coefficient of determination) is done to find out how much influence the variable of price book value, price earning ratio, earnings per share and dividend pay out ratio to stock return variable. From result of t test known that price book value, earnings per share and dividend pay out ratio partially significant effect to stock return. Variable Price Earning Ratio partially no significant effect on stock return variables. From result of F test known that Price Book Value, Price Earning Ratio, Earning Per Share and Dividend Pay Out Ratio simultaneously have an effect on signifikan to variable Return of Shares In Manufacturing Company Listed In Indonesia Stock Exchange Year 2014 -2016.

Keywords	: PBV, PER, EPS, DPR, Stock Return
Educação em saúde – estratégia de cuidado integral e multiprofissional para gestantes
Authors: Araújo Maria Luiza Alves , Medeiros Ariany Paula , Zuculin Sara , Souza Evelin Gonçalves , Barros Paula Ferreira , Boaventura Talita , Mendes Patrícia Helena Costa , Maciel Ana Paula Ferreira , Fagundes Neto Mariano 
Published: August 2018

O Programa de Educação pelo Trabalho para a Saúde (PET-Saúde) objetiva iniciar os estudantes das graduações em saúde no trabalho da Estratégia Saúde da Família, oportunizando a vivência das ações desenvolvidas na atenção básica à saúde. Dentre estas atividades, destaca-se a educação em saúde que integra o saber científico com o popular. Um dos grupos prioritários que deve ser alvo da atividade de educação em saúde na Estratégia Saúde da Família é o grupo de gestantes, por se tratar de um período em que a mulher está mais susceptível a receber informações e modificar o comportamento. O objetivo deste trabalho é expor uma experiência de cuidado integral e multiprofissional, utilizando-se a educação em saúde como ferramenta para a adoção de novos hábitos em saúde por parte de um grupo de gestantes assistidas por uma equipe da Estratégia Saúde da Família. O projeto foi realizado no mês de janeiro de 2011 naEquipe de Saúde da Família Independência III, localizado no município de Montes Claros/MG, tendo como agentes facilitadores os acadêmicos da área da saúde da Universidade Estadual de Montes Claros, participantes do PET-Saúde, bem como os profissionais de saúde, que integram a equipe, sendo também preceptores do programa. O curso foi estruturado emsete oficinas, abordando temas chaves para as gestantes.Esse projeto foi de grande importância tanto para as gestantes, que avaliaram de forma positiva a atividade, quanto para os acadêmicos, que puderam adquirir conhecimentos de forma crítica e multidisciplinar.
PET-Saúde: formando discentes multiplicadores - relato de experiência
Authors: Sales Késsia Nara Andrade , Paula Fabiana Angélica de , Ribeiro Mirtes , Ribeiro Liliane Da Consolação Campos , Canuto Sylvana Mara 
Published: August 2018

A interação dos profissionais da saúde ainda na graduação, torna-se possível por meio de iniciativas como o Programa de Educação pelo Trabalho para a Saúde (PET-Saúde), o qual se constitui em um instrumento que viabiliza a inserção dos estudantes no Sistema Único de Saúde - SUS, visando à iniciação ao trabalho científico, estágios e vivências do cotidiano do serviço, contribuindo para a formação de profissionais mais comprometidos com a realidade de saúdee sua transformação. O presente trabalho trata-se de um relato de experiência de caráter descritivo, com o objetivo de relatar a experiência de uma aluna de graduação em Odontologia da Universidade Federal dos Vales do Jequitinhonha e Mucuri (UFVJM), participante do PET-Saúde/Saúde Mental-Drogas/UFVJM e ex-participante do PET-Saúde/Vigilância em Saúde/UFVJM. O PET-Saúde/Vigilância a Saúde da UFVJM, é composto por dois grupos tutoriais sendoque o grupo do qual a acadêmica participou visava ampliar o acesso á testagem para diagnóstico de contaminação pelo vírus HIV, utilizando testes-rápidos. O PET-Saúde/Saúde Mental-Drogas/UFVJM tem como proposta, dentre outros objetivos, qualificar acadêmicos técnicamente, científicamente e tecnologicamente na área da saúde mental, com abordagem a álcool e outras drogas. Além disso, o programa PET-Saúde/UFVJM estimula o aluno a desenvolveratividades de pesquisa com propostas de mudança efetivas em sua realidade. Desta forma, percebe-se que a integração ensino-serviço-comunidade pode ser utilizada como um instrumento valioso na promoção social e no exercício da cidadania, tornando-se fundamental na diminuição das problemáticas sociais existentes.
Efektifitas Pemanfaatan Fly Ash Batubara Sebagai Adsorben Dalam Menetralisir Air Asam Tambang pada Settling Pond Penambangan Banko PT. Bukit Asam (Persero), Tbk
Authors: Gobel Alieftiyani Paramita 
Published: August 2018

Penanganan AAT yang banyak dilakukan di perusahaan tambang batubara dengan cara pengapuran masih kurang efektif karena penggunaan kapur hanya untuk meningkatkan pH rendah menjadi pH netral, namun tidak dapat menurunkan kandungan logam Fe dan Mn. Aplikasi penggunaan fly ash skala laboratorium dengan volume AAT 250ml menunjukkan bahwa adanya penambahan massa fly ash dan kecepatan pengadukan terjadi peningkatan pH dan penurunan konsentrasi logam Fe dan Mn. Fly ash batubara mengandung senyawa mineral utama yaitu kuarsa (SiO2) dan mullite (Al6Si2O13) yang berperan pada proses adsorpsi antara logam berat dengan adsorben fly ash dalam larutan mengandung air. Berdasarkan hasil analisis, efektifitas massa fly ash terhadap perubahan kadar pH rata-rata sebesar 63,11%. Selanjutnya efektifitas massa fly ash terhadap perubahan konsentrasi logam Fe rata-rata sebesar 85,95%, sedangkan efektifitas massa fly ash terhadap perubahan konsentrasi logam Mn rata-rata sebesar 81,77%. Oleh karena itu, kapasitas adsorpsi logam Fe lebih besar daripada kapasitas adsorpsi logam Mn yaitu kapasitas adsorpsi logam Fe sebesar 4,938 mg/g sedangkan kapasitas adsorpsi logam Mn sebesar 4,296 mg/g mengikuti model adsorpsi isotherm Freundlich.
FAKTOR RESIKO YANG BERHUBUNGAN DENGAN KEJADIAN KANKER SERVIK; STUDI KASUS DI RSUP DR. KARIADI SEMARANG
Authors: Aziyah Aziyah , Sumarni Sri , Ngadiyono Ngadiyono 
Published: August 2018

Kanker serviks uteri merupakan salah satu jenis penyakit kanker tidak menular yang diperkirakan meningkat setiap tahunnya. Di RSUP Dr.Kariadi Semarang, kunjungan kanker servik di poliklinik ginekologi dari ke tahun semakin meningkat. Banyak faktor resiko yang mendukung timbulnya penyakit kanker serviks uteri antara lain riwayat hubungan seksual pertama sebelum umur 20 tahun, multiparitas, riwayat KB oral, faktor perilaku tidak sehat, dan faktor keturunan. Tujuan penelitian ini untuk mengetahui faktor resiko kanker servik pada pasien poliklinik ginekologi RSUP Dr. Kariadi Semarang tahun 2016.Jenis penelitian ini adalah penelitian kuantitatif dengan rancangan penelitian observasional analitik korelatif menggunakan pendekatan cross-sectional. Sampel yang digunakan dalam penelitian ini total sampling dengan teknik aksidental sampling sebanyak 103 responden, terdiri dari 68 responden kanker serviks dan 35 responden bukan kanker servik.Hasil penelitian adalah ada Â hubungan antara umur pertama kali berhubungan seksual (p-value=0.001, OR 4.56), status paritas (p-value=0.000, OR 0.09), kontrasepsi KB hormonal (p-value=0.008, OR 3.36), riwayat keturunan dengan sakit kanker (p-value=0.006, OR 5.1), dan perilaku vaginal hygiene (p-value=0.000, OR 6.5) dengan kejadian kanker servik di RSUP Dr. Kariadi Semarang tahun 2016.Â Â Â Â Â Â Â Â Â Â Â Dari hasil penelitian ini diharapkan Â tenaga kesehatan dapat menginformasikan faktor-faktor yang Â berhubungan dengan kanker servik sehingga masyarakat mengerti dan melakukan tindakan preventif.Â Â Â
ANALISIS FAKTOR RESIKO HIPERTENSI SEKUNDER PADA PENGGUNA KONTRASEPSI AKTIF DI PUSKESMAS TANJUNG AGUNG
Authors: Suryanda Suryanda 
Published: August 2018

Abstrak : Analisis Faktor Resiko Hipertensi Sekunder Pada Pengguna Kontrasepsi Aktif Di UPTD Puskesmas Tanjung Agung. Tujuan penelitian menganalisis faktor resiko hipertensi sekunder pada pengguna kontrasepsi Aktif di UPTD Puskesmas Tanjung Agung. Merupakan penelitian deskriptif analitik dengan metode cross-sectional . Populasi adalah wanita pengguna kontrasepsi aktif yang datang ke Poliklinik KIA dan KB Â tahun 2016. Menggunakan tekhnik accidental sampling, didapatkan 45 orang responden. Data dengan kuisioner berbentuk check list dan pertanyaan terbuka. Usia responden pada kisaran 18 tahun hingga 47 tahun, pengguna kontrasepsi aktif dengan kelompok varitas tertinggi adalahÂ 3 â€“ 4 anak 15 responden (33,3 %), kelompok terendah lebih dari 5 anak 3 responden (6,7%). Kelompok terpapar asap rokok 26 reponden (57,7%), kelompok tidak terpapar 19 responden (42,2%). Responden hipertensi 14 responden (31,1%), Â yang tidak hipertensi 31 responden (68,9%). Penggunaaan Kontrasepsi hormonal lebih banyak, yaitu 23 responden (51,1%) dari pada non hormonal, yaitu 22 responden (48,9%). Terdapat Â hubungan bermakna antara pemakaian kontrasepsi hormonal dengan kejadian hipertensi, dengan nilai p.value 0,001. Tidak terdapat hubungan bermakna antara paparan asap rokok pada pengguna kontrasepi dengan kejadian hipertensi, nilai p.value 0,057. Perlunya edukasi Â PHBS terkait paparan asap rokok dan bahaya hipertensi kepada masyarakat.
Editorial Volumen 1 Nro. 2 (2016)
Authors: Gómez Oscar R. 
Published: August 2018

Les doy la bienvenida a este segundo número. Un excelente equilibrio entre fisiología, política y religión; con artículos atravesados por, o que cuestionan, la visión tántrica de sujeto. Los cuatro trabajos seleccionados sintetizan el espíritu presentado en el primer número: un enfoque multidisciplinario sobre un único objeto de estudio —el Hombre y su relación con el universo en el que se desarrolla—. AbstractWelcome to our second issue, which is an excellent balance between physiology, politics, and religion. All its articles are driven by, or question, the tantric viewpoint of the human subject. The four selected works synthesize the spirit presented in the first issue: a multidisciplinary approach on a single object of study —man and his relationship with the universe where he realizes.
TANTRA O YOGA. ESTUDIOS CLÍNICOS, 2ª PARTE: TANTRA
Authors: Gómez Oscar R. 
Published: August 2018

Varios estudios clínicos realizados muestran cómo las prácticas tántricas así como los ejercicios de las tradiciones védicas, como el yoga, o budistas theravada o mahayana, tienen un impacto psicobiológico significativo. Este estudio busca el correlato neurofisiológico de las prácticas llamadas meditaciones tántricas y no-tántricas mediante una revisión sistemática cualitativa de los datos recolectados. Se evidenció que las prácticas tántricas producen un aumento en la actividad simpática, del estado de «alerta fásica» y en el rendimiento en tareas cognitivo visuales. Promueven una mayor vigilia y menor propensión al sueño, generan un incremento en la actividad cognitiva y modificaciones metabólicas contrarias a las que se verifican de las no-tántricas como consecuencia del relax inducido por esas prácticas. Las prácticas tántricas producen un estado de calma y claridad mental, con la energía y excitación suficiente para funcionar en el entorno con eficacia en el manejo de la irritabilidad, la tensión y la fatiga, al igual que el manejo del miedo y de la ansiedad. La experiencia espiritual «del despertar» y de la «autorrealización» tienen su correspondencia neurofuncional y anatómica, de modificaciones neuroplásticas que desarrollan un nuevo nivel de sensibilidad, percepción y autopercepción. AbstractSeveral clinical studies show how exercises in Vedic traditions, such as Yoga, or Theravada or Mahayana Buddhisms as well as tantric practices have a significant psychobiological impact. This study seeks the neurophysiological correlate of the practices called tantric and non-tantric meditations through a qualitative systematic review of the data collected. Tantric practices were proved to show increased sympathetic activity, «phasic alertness», and better performance at cognitive visual tasks. They promote greater wakefulness and decresead propensity to sleep, increased cognitive activity and metabolic changes as contrasted with those resulting from non-tantric practices due to the relaxation induced by such practices. Tantric practices create calmness and mental clarity, with enough energy and excitement to function in the environment effectively in managing irritability, stress and fatigue, as well as fear and anxiety management. The spiritual experience of "awakening" and "self-realization" has a neurofunctional and anatomical correlate of neuroplastic modifications that create new levels of sensitivity, perception and self-perception.
The Gas Composition and Deep Cloud Structure of Jupiter's Great Red Spot
Authors: Bjoraker G. L. , Wong M. H. , Pater I. de , Hewagama T. , Ádámkovics M. , Orton G. S. 
Published: August 2018

Abstract
We have obtained high-resolution spectra of Jupiter’s Great Red Spot (GRS) between 4.6–5.4 μm using telescopes on Mauna Kea to derive gas abundances and to constrain its cloud structure between 0.5–5 bars. We used line profiles of deuterated methane (CH3D) at 4.66 μm to infer the presence of an opaque cloud at 5 ± 1 bars. From thermochemical models, this is almost certainly a water cloud. We also used the strength of Fraunhofer lines in the GRS to obtain the ratio of reflected sunlight to thermal emission. The level of the reflecting layer was constrained to be at 570 ± 30 mbar based on fitting strong NH3 lines at 5.32 μm. We identify this layer as an ammonia cloud based on the temperature where gaseous NH3 condenses. We found evidence for a strongly absorbing but not totally opaque cloud layer at pressures deeper than 1.3 bars by combining Cassini/CIRS spectra of the GRS at 7.18 μm with ground-based spectra at 5 μm. This is consistent with the predicted level of an NH4SH cloud. We also constrained the vertical profile of H2O and NH3. The GRS spectrum is matched by a saturated H2O profile above an opaque water cloud at 5 bars. The pressure of the water cloud constrains Jupiter’s O/H ratio to be at least 1.1 times solar. The NH3 mole fraction is 200 ± 50 ppm for pressures between 0.7–5 bars. Its abundance is 40 ppm at the estimated pressure of the reflecting layer. We obtained 0.8 ± 0.2 ppm for PH3, which is a factor of 2 higher than in the warm collar surrounding the GRS. We detected all five naturally occurring isotopes of germanium in GeH4 in the GRS. We obtained an average value of 0.35 ± 0.05 ppb for GeH4. Finally, we measured 0.8 ± 0.2 ppb for CO in the deep atmosphere.
Blue Straggler Stars Beyond the Milky Way. III. Detection of Evolved Blue Straggler Candidates in Large Magellanic Cloud Clusters
Authors: Li Chengyuan , Deng Licai , Bekki Kenji , Hong Jongsuk , Grijs Richard de , For Bi-Qing 
Published: August 2018

Abstract
We analyze Hubble Space Telescope observations of nine Large Magellanic Cloud star clusters with ages of 1–2 Gyr to search for evolved counterparts of blue straggler stars. Near the red clump regions in the clusters’ color–magnitude diagrams, we find branches of evolved stars that are much brighter than normal evolved stars. We examine the effects of photometric artifacts, differential reddening, and field contamination. We conclude that these bright evolved stars cannot be explained by any of these effects. Our statistical tests show that the contributions of photometric uncertainties, crowding effects, and differential reddening to these bright evolved stars are insufficient to fully explain their presence. Based on isochrone fitting, we have also ruled out the possibility that these bright evolved stars could be reproduced by an internal chemical abundance spread. The spatial distributions of the bright evolved stars exhibit clear concentrations that cannot be explained by homogeneously distributed field stars. This is further confirmed based on Monte Carlo-based tests. By comparing our observations with stellar evolution models, we find that the masses of most of the bright evolved stars do not exceed twice the average mass of normal evolved stars. We suggest that these bright evolved stars are, in fact, evolved blue straggler stars.
Self-similar Approach for Rotating Magnetohydrodynamic Solar and Astrophysical Structures
Authors: Luna M. , Priest E. , Moreno-Insertis F. 
Published: August 2018

Abstract
Rotating magnetic structures are common in astrophysics, from vortex tubes and tornadoes in the Sun all the way to jets in different astrophysical systems. The physics of these objects often combine inertial, magnetic, gas pressure, and gravitational terms. Also, they often show approximate symmetries that help simplify the otherwise rather intractable equations governing their morphology and evolution. Here we propose a general formulation of the equations assuming axisymmetry and a self-similar form for all variables: in spherical coordinates (r, θ, ϕ), the magnetic field and plasma velocity are taken to be of the form

and

, with corresponding expressions for the scalar variables like pressure and density. Solutions are obtained for potential, force-free, and non-force-free magnetic configurations. Potential field solutions can be found for all values of n. Nonpotential force-free solutions possess an azimuthal component B

ϕ
and exist only for n ≥ 2; the resulting structures are twisted and have closed field lines but are not collimated around the system axis. In the non-force-free case, including gas pressure, the magnetic field lines acquire an additional curvature to compensate for an outward pointing pressure gradient force. We have also considered a pure rotation situation with no gravity, in the zero-β limit: the solution has cylindrical geometry and twisted magnetic field lines. The latter solutions can be helpful in producing a collimated magnetic field structure; but they exist only when n < 0 and m < 0: for applications they must be matched to an external system at a finite distance from the origin.
Long-term Behavior of a Type IIP Supernova SN 2004dj in the Radio Bands
Authors: A. J. Nayana , Chandra Poonam , K. Ray Alak 
Published: August 2018

Abstract
We present radio observations and modeling of one of the nearest and brightest Type IIP supernova SN 2004dj exploded in the galaxy NGC 2403 at a distance of ∼3.5 Mpc. Our observations span a wide frequency and temporal range of 0.24–43 GHz and ∼1 day to 12 years since the discovery. We model the radio light curves and spectra with the synchrotron emission. We estimate the mass-loss rate of the progenitor star to be

∼ 1 × 10−6

for a wind speed of 10 km s−1. We calculate the radio spectral indices using 1.06, 1.40, 5.00, and 8.46 GHz flux density measurements at multiple epochs. We witness steepening in the spectral index values for an extended period predominantly at higher frequencies. We explain this as a signature of electron cooling happening at the supernova shock in the plateau phase of the supernova. We estimate the cooling timescales for inverse Compton cooling and synchrotron cooling and find that inverse Compton cooling is the dominant cooling process.
Predictability of the Solar Cycle Over One Cycle
Authors: Jiang Jie , Wang Jing-Xiu , Jiao Qi-Rong , Cao Jin-Bin 
Published: August 2018

Abstract
The prediction of the strength of future solar cycles is of interest because of its practical significance for space weather and as a test of our theoretical understanding of the solar cycle. The Babcock–Leighton mechanism allows predictions by assimilating the observed magnetic field on the surface. Since the emergence of sunspot groups has random properties, making it impossible to accurately predict the solar cycle and strongly limiting the scope of cycle predictions, we develop a scheme to investigate the predictability of the solar cycle over one cycle. When a cycle has been ongoing for more than three years, the sunspot group emergence can be predicted along with its uncertainty during the rest time of the cycle. The method for this prediction is to start by generating a set of random realizations that obey the statistical relations of the sunspot emergence. We then use a surface flux transport model to calculate the possible axial dipole moment evolutions. The correlation between the axial dipole moment at cycle minimum and the subsequent cycle strength and other empirical properties of solar cycles are used to predict the possible profiles of the subsequent cycle. We apply this scheme to predict the large-scale field evolution from 2018 to the end of cycle 25, whose maximum strength is expected to lie in the range from 93 to 155 with a probability of 95%.