bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGAMBILAN KEPUTUSAN MENJADI PEKERJA MIGRAN INDONESIA PEREMPUAN
Authors: Aeni Nurul 
Published: December 2019

ENGLISHDecision of being woman migrant workers brings both positive and negative consequeces for the woman workers as well as their families live behind. This study aimed: (1) to describe the decision making of being migrant workers among the applicants of woman migrant workers from Pati District; (2) to explain the factors correlate to the migrate decision making, and (3) to explain factors correlate to destination country choosing. It used quantitave approach. The primary data were obtained by spreading questionnaires among women migrant worker applicants at four labour supply companies. Meanwhile the secondary data get through desk review. Then, the data were analysed descriptively using chi square and correspondence analysis. The study resulted: (1) economic was the main factor of decision making for being woman migrant workers; (2) the factors correlated to the decision making for being woman migrant workers were the position in household, previous income, and decision making process; (3) high salary was the main factor on choosing the destination country. The factors correlated to destination country preferences were: the reasons for choosing the destination countries, age, previous job, previous salary, and husband’s age. INDONESIAKeputusan menjadi pekerja migran perempuan dapat berkonsekuensi positif maupun negatif bagi pekerja migran maupun keluarga yang ditinggalkan. Penelitian ini bertujuan: (1) menggambarkan pengambilan keputusan menjadi pekerja migran perempuan pada calon pekerja migran di Kabupaten Pati; (2) mendeskripsikan faktor yang berhubungan dengan pengambilan keputusan; dan (3) mendeskripsikan faktor yang berhubungan dengan pemilihan negara tujuan. Penelitian menggunakan pendekatan kuantitatif. Data primer didapatkan melalui pengisian kuesioner oleh para calon pekerja migran perempuan di empat PPTKIS. Sementara data sekunder didapatkan melalui review penelitian terdahulu dan dokumen yang relevan. Data yang diperoleh dianalisis secara deskriptif menggunakan chi square dan analisis korespondensi. Hasil penelitian adalah: (1) ekonomi adalah faktor utama pengambilan keputusan menjadi pekerja migran perempuan; (2) faktor yang berhubungan dengan pengambilan keputusan menjadi pekerja migran adalah posisi dalam rumah tangga, pendapatan sebelumnya, dan proses pengambilan keputusan; (3) gaji yang tinggi merupakan alasan utama pemilihan negara tujuan migrasi. Adapun faktor yang berhubungan dengan pemilihan negara tujuan migrasi adalah alasan pemilihan negara, usia, pekerjaan sebelumnya, pendapatan sebelumnya, dan usia suami.
PENERAPAN METODE PEMBELAJARAN DAHSYAT “POWER TEACHING”
Authors: Suwirya I Wayan , Astawa I Nengah 
Published: December 2019

This article will discuss the Power Teaching Learning method which is more recently known as the Whole Brain Teaching method, which has the same concept as Brain Based Teaching. Power Teaching, in Indonesian can be said "awesome learning"! While the phrase "whole brain teaching" - learning with the whole brain - implies that this learning optimizes the work of the brain of students, left brain, right brain, brain. In other languages, it might be said that this learning involves the aspects of students with 'high impact': cognitive, affective and psychomotor. How effective is this "whole-brain" learning? The writer has tried to apply this method in Public and Private Junior high schools Schools in Denpasar. The results are very encouraging and satisfactory to be able to increase the efficiency, effectiveness and learning outcomes of students. This method is a learning model that is able to focus students' attention on learning through varied activities by combining visual, verbal and kinesthetic aspects
IMPLEMENTASI MULTIPLE INSIDE-OUTSIDE CIRCLE UNTUK MENINGKATKAN KETERAMPILAN BERBICARA
Authors: Murtini Ni Made Wersi , Krismayani Ni Wayan 
Published: December 2019

This study was designed as a classroom action research (CAR). This study was conducted in some cycles consisted of two sessions in each cycle: Planning, Action, Observation, and Reflection. This study is conducted to the students of Germania Class Airport Handling Management Bali Aviation Training Center Denpasar (BATC) which consisted of 22 students (6 male and 16 female) who had low ability in speaking English. It was proven by the average score of pre-test which was 66,59. To solve the problem, the researcher used Multiple Inside-Outside Circle. The data collected from this research were obtained from pre-test, post-test, and questionnaire. The data were analyzed by analysis statistial desriptive. The first finding of this study was there was a significant improvement on students’ speaking skill after the use of Multiple Inside-Outside Circle which can be seen from the average score of pre-test, cycle I and cycle II. The second finding showed that the subjects showed positive respond to the implementation of the Multiple Inside-Outside Circle.
CHARACTER BUILDING IN THE APPLICATION OF COLABORATIVE STRATEGIC READING IN READING CLASS
Authors: Dharmayanti Putu Ayu Paramita 
Published: December 2019

ABSTRACT
This research used descriptive qualitative design that aimed at describing character education values that were built in the application of Collaborative Strategic Reading. As the focus of this study was third grade university students who took Intermediate Reading lecture in English Education Study Program, Faculty of Teacher Training, Mahasaraswati Denpasar University. The data obtained in this study are qualitative data. The qualitative data were collected by observation, open questionnaire and guided interview. Data were collected by using researcher as the key instrument and some research instruments such as, field note, list of open questionnaire questions, and list of guided interview questions. The result of observation, open questionnaire and guided interview were analyzed descriptively using Interactive Model. The result of the study concluded that directly application of Collaborative Strategic Reading could build some values of character education, such as curiosity, creativity, communicative, responsible, hard work, love reading, discipline, and democratic but indirectly application of Collaborative Strategic Reading could build all values of character education through the moral value inserted in each text read by the reader.
Community engagement in global health education supports equity and advances local priorities: an eight year Ecuador-Canada partnership
Authors: Misra Shivali , Doucet Alison , Morales Juana , Andersson Neil , Macaulay Ann , Evans Andrea 
Published: December 2019

Background: Global health education initiatives inconsistently balance trainee growth and benefits to host communities. This report describes a global health elective for medical trainees that focuses on community engagement and participatory research to provide mutually beneficial outcomes for the communities and trainees.Methods: An eight-year university–community partnership, the Chilcapamba to Montreal Global Health Elective is a two-month shared decision-making research and clinical observership experience in rural Ecuador for medical trainees at McGill University, Canada. Research topics are set by matching community-identified priorities with skillsets and interests of trainees, taking into consideration local potential impact.Results: Community outcomes included development of a Community Health Worker program, new collaborations with local organizations, community identification of health priorities, and generation of health improvement recommendations. Collaborative academic outputs included multiple bursary awards, conference presentations and published manuscripts. Conclusion: This medical global health elective engages communities using participatory research to prioritise socially responsible and locally beneficial outcomes.
Chemical Properties of Two Dense Cores in a Planck Galactic Cold Clump G168.72-15.48
Authors: Tang Mengyao , Ge J. X. , Qin Sheng-Li , Liu Tie , Wu Yuefang , Kim Kee-Tae , Liu Sheng-Yuan , Zhang Chao , He J. H. , Ju Bing-Gang , Fang Xinhe 
Published: December 2019

Abstract
To deepen our understanding of the chemical properties of the Planck Galactic Cold Clump (PGCC) G168.72-15.48, we performed observations of nine molecular species, namely, c-C3H, H2CO, HC5N, HC7N, SO, CCH, N2H+, CH3OH, and CH3CCH, toward two dense cores in PGCC G168.72-15.48 using the Tianma Radio Telescope and Purple Mountain Observatory Telescope. We detected c-C3H, H2CO, HC5N, N2H+, CCH, and CH3OH in both G168-H1 and G168-H2 cores, whereas HC7N and CH3CCH were detected only in G168-H1 and SO was detected only in G168-H2. Mapping observations reveal that the CCH, N2H+, CH3OH, and CH3CCH emissions are well coupled with the dust emission in G168-H1. Additionally, N2H+ exhibits an exceptionally weak emission in the denser and more evolved G168-H2 core, which may be attributed to the N2H+ depletion. We suggest that the N2H+ depletion in G168-H2 is dominated by N2 depletion, rather than the destruction by CO. The local thermodynamic equilibrium calculations indicate that the carbon-chain molecules of CCH, HC5N, HC7N, and CH3CCH are more abundant in the younger G168-H1 core. We found that starless core G168-H1 may have the properties of cold dark clouds based on its abundances of carbon-chain molecules. While, the prestellar core G168-H2 exhibits lower carbon-chain molecular abundances than the general cold dark clouds. With our gas-grain astrochemical model calculations, we attribute the observed chemical differences between G168-H1 and G168-H2 to their different gas densities and different evolutionary stages.
Local Metallicity Distribution Function Derived from Galactic Large-scale Radial Iron Pattern Modeling
Authors: Mishurov Yu. N. , Tkachenko R. V. 
Published: December 2019

Abstract
We develop an approach for fitting the results of modeling a wriggling radial large-scale iron pattern along the Galactic disk, derived over young (high-mass) Cepheids, with the metallicity distribution obtained using low-mass long-living dwarf stars in the close solar vicinity. For this purpose, during the step at which the theoretical abundance distribution over low-mass stars in the solar vicinity is computed, we propose the redefinition of the initial mass function so that the resulting theoretical stellar distribution over masses would be close to the distribution in the observed sample. By means of the above algorithm and subsequent corrections of the theoretical metallicity distribution function (MDF), as described in the literature, we have achieved fairly good agreement between the theoretical and observed MDFs for low-mass stars in the local solar vicinity.
Resolving the Metallicity Distribution of the Stellar Halo with the H3 Survey
Authors: Conroy Charlie , Naidu Rohan P. , Zaritsky Dennis , Bonaca Ana , Cargile Phillip , Johnson Benjamin D. , Caldwell Nelson 
Published: December 2019

Abstract
The Galactic stellar halo is predicted to have formed at least partially from the tidal disruption of accreted dwarf galaxies. This assembly history should be detectable in the orbital and chemical properties of stars. The H3 Survey is obtaining spectra for 200,000 stars and, when combined with Gaia data, is providing detailed orbital and chemical properties of Galactic halo stars. Unlike previous surveys of the halo, the H3 target selection is based solely on magnitude and Gaia parallax; the survey therefore provides a nearly unbiased view of the entire stellar halo at high latitudes. In this paper we present the distribution of stellar metallicities as a function of Galactocentric distance and orbital properties for a sample of 4232 kinematically selected halo giants to 100 kpc. The stellar halo is relatively metal-rich,

, and there is no discernible metallicity gradient over the range 6 < R
gal < 100 kpc. However, the halo metallicity distribution is highly structured, including distinct metal-rich and metal-poor components at R
gal < 10 kpc and R
gal > 30 kpc, respectively. The Sagittarius stream dominates the metallicity distribution at 20–40 kpc for stars on prograde orbits. The Gaia–Enceladus merger remnant dominates the metallicity distribution for radial orbits to ≈30 kpc. Metal-poor stars with [Fe/H] < −2 are a small population of the halo at all distances and orbital categories. We associate the “in situ” stellar halo with stars displaying thick disk chemistry on halo-like orbits; such stars are confined to

. The majority of the stellar halo is resolved into discrete features in chemical–orbital space, suggesting that the bulk of the stellar halo formed from the accretion and tidal disruption of dwarf galaxies. The relatively high metallicity of the halo derived in this work is a consequence of the unbiased selection function of halo stars and, in combination with the recent upward revision of the total stellar halo mass, implies a Galactic halo metallicity that is typical for its mass.
Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS). II. Cold Molecular Gas Evolution out to Redshift 6
Authors: Liu Daizhong , Schinnerer E. , Groves B. , Magnelli B. , Lang P. , Leslie S. , Jiménez-Andrade E. , Riechers D. A. , Popping G. , Magdis Georgios E. , Daddi E. , Sargent M. , Gao Yu , Fudamoto Y. , Oesch P. A. , Bertoldi F. 
Published: December 2019

Abstract
We present new measurements of the cosmic cold molecular gas evolution out to redshift 6 based on systematic mining of the Atacama Large Millimeter/submillimeter Array (ALMA) public archive in the COSMOS deep field (A3COSMOS). Our A3COSMOS data set contains ∼700 galaxies (0.3 ≲ z ≲ 6) with high-confidence ALMA detections in the (sub)millimeter continuum and multiwavelength spectral energy distributions. Multiple gas mass calibration methods are compared, and biases in band conversions (from observed ALMA wavelength to rest-frame Rayleigh–Jeans tail continuum) have been tested. Combining our A3COSMOS sample with ∼1000 CO-observed galaxies at 0 ≲ z ≲ 4 (75% at z < 0.1), we parameterize galaxies’ molecular gas depletion time (

) and molecular gas to stellar mass ratio (

) each as a function of the stellar mass (

), offset from the star-forming main sequence (

) and cosmic age (or redshift). Our proposed functional form provides a statistically better fit to current data (than functional forms in the literature) and implies a “downsizing” effect (i.e., more-massive galaxies evolve earlier than less-massive ones) and “mass quenching” (gas consumption slows down with cosmic time for massive galaxies but speeds up for low-mass ones). Adopting galaxy stellar mass functions and applying our

function for gas mass calculation, we for the first time infer the cosmic cold molecular gas density evolution out to redshift 6 and find agreement with CO blind surveys as well as semianalytic modeling. These together provide a coherent picture of cold molecular gas, star formation rate, and stellar mass evolution in galaxies across cosmic time.
On the Expansion, Age, and Origin of the Puzzling Shell/Pulsar-wind Nebula G310.6–1.6
Authors: Reynolds Stephen P. , Borkowski Kazimierz J. 
Published: December 2019

Abstract
We present a 142 ks Chandra observation of the enigmatic combination supernova remnant G310.6–1.6 consisting of a bright pulsar-wind nebula driven by an energetic pulsar, surrounded by a highly circular, very faint shell with a featureless, probably synchrotron, spectrum. Comparison with an observation 6 yr earlier shows no measurable expansion of the shell, though some features in the pulsar-wind nebula have moved. We find an expansion age of at least 2500 yr, implying a current shock velocity less than about 1000 km s−1. We place severe upper limits on thermal emission from the shell; if the shell locates the blast wave, a Sedov interpretation would require the remnant to be very young, about 1000 yr, and to have resulted from a dramatically sub-energetic supernova, ejecting ≪0.02M
⊙ with energy E ≲ 3 × 1047 erg. Even a merger-induced collapse of a white dwarf to a neutron star, with a low-energy explosion, is unlikely to produce such an event. Other explanations seem equally unlikely.
ROME (Radio Observations of Magnetized Exoplanets). II. HD 189733 Does Not Accrete Significant Material from Its Exoplanet Like a T Tauri Star from a Disk
Authors: Route Matthew , Looney Leslie W. 
Published: December 2019

Abstract
It has been asserted that the primary star in the HD 189733 system steadily accretes evaporated exospheric gases from its “hot Jupiter” companion, rather like a T Tauri star accreting from a disk. We conduct statistical and periodogram analyses of the photometric time series of the primary, as acquired by the automated photoelectric telescope, Microvariability and Oscillations of Stars, and Wise Observatory, to investigate this claim with the goal of revealing the presence of accretion shocks or photospheric accretion hotspots as are found in T Tauri systems such as AA Tau. None of the anticipated features were found. We re-analyze existing radio, optical, ultraviolet, and X-ray data within the framework of accreting T Tauri systems to determine physical quantities such as plasma density and temperature, accretion rate, and flare lengths. We find that with an accretion rate of

–1011 g s−1, the star is more similar to a system that intermittently absorbs gas from sungrazing comets in outburst than classical T Tauri systems, which have accretion rates at least two orders of magnitude larger. If such accretion exists, it would result in undetectably low activity at all wavelengths. Alternatively, all of the emission properties observed thus far are in agreement with stellar activity from a magnetically active star.
Modeling the Thermal Bulge of a Hot Jupiter with the Two-stream Approximation
Authors: Gu Pin-Gao , Peng Da-Kai , Yen Chien-Chang 
Published: December 2019

Abstract
We revisit the problem of the thermal bulge of asynchronous hot Jupiters using HD 209458 b as a fiducial study. We improve upon previous works by using a double-gray atmosphere model and interior structure from MESA as the background state and then solve for the thermal bulge in response to the semidiurnal component of stellar insolation. The atmosphere model is based on the radiative transfer with Eddington’s two-stream approximation. Two opacity cases are considered: the first introduces a greenhouse effect, and the second exhibits a strong temperature inversion. We find that for the predominant thermal bulges excited by g-modes of lower orders, our results are qualitatively similar to the adiabatic results from Arras & Socrates. It arises because the perturbed heating due to self-absorption of thermal emissions can be significant (i.e., greenhouse effect) against Newtonian damping, thereby leading to almost undamped thermal bulges. We also find that the contribution to the thermal bulge from the evanescent waves in the convective zone is not negligible, implying that the thermal bulge is not merely confined in the atmosphere and radiative envelope. Assuming the torque balance between the thermal and gravitational bulges, we estimate the tidal quality factor of the planet for gravitational tides to match the observed radius. The limitations of our model are also briefly discussed.
Elevated Risk of Viral Rebound on ART in Migrants Living in France: Role of Socioeconomic Factors
Authors:   the ANRS CO9-COPANA study, Abgrall Sophie , Raho-Moussa Mariem , Seng Rémonie , Ghislain Mathilde , Matheron Sophie , Pialoux Gilles , Goujard Cécile , Meyer Laurence 
Published: December 2019

Background In Western countries, viral rebound on antiretroviral therapy (ART) appears to occur more frequently in migrants. We aimed to assess the respective roles of socioeconomic factors and migration on viral rebound in people living with HIV (PLHIV) in France. Methods We included PLHIV in France, enrolled from 2004 to 2008 in the French ANRS-COPANA cohort, who started a first ART and achieved undetectability (<50 copies/ml) within 1 year. Determinants of viral rebound were assessed using Cox models including geographical origin, HIV transmission group, and clinicobiological and sociodemographic data. Results Of 499 included individuals, 288 were born in France, 158 in sub-Saharan Africa (SSA) and 53 in another country. Kaplan–Meier probabilities of viral rebound-free survival were similar for men having sex with men (MSM) and heterosexuals born in France, and lower in migrants from SSA or other countries ( P<0.001). The crude hazard ratio (HR) of viral rebound was 2.49 (95% CI, 1.59, 3.90) in migrants from SSA and 1.78 (0.94, 3.88) in migrants from other countries compared with MSM born in France. Educational level, financial difficulties and HIV status disclosure had the biggest impact on the difference between the crude and adjusted HRs for viral rebound in migrants. In multivariable analysis, viral rebound was no longer associated with geographical origin, but with protease inhibitor-containing ART, a VACS index ≥35 as a potential indicator of frailty, poor financial status (difficulties or debts) and non-disclosure to friend(s). Conclusions Socioeconomic factors affect outcomes on ART, even in the context of free access to HIV care and treatment. Patient-centred strategies should be encouraged with the intervention of social workers to address basic needs and promote social support for more socially vulnerable individuals.
Male Sexual Function After Pelvic Fracture
Authors: Ozumba Donald , Starr Adam J , Benedetti Gary E , Whitlock Shelly N , Frawley William H 
Published: December 2019

abstract
Fifty-one male patients with prior pelvic fracture completed a Brief Sexual Function Inventory questionnaire (BSFI) 2 years postinjury. Responses were compared to those of 53 men with ankle fractures. Patients with pelvic fracture scored significantly worse than patients with ankle fracture. Patients with pelvic fracture scored poorly on sex drive, erection, ejaculation, and satisfaction with sex life. Older patients had significantly worse sex function scores than younger patients. Sexual dysfunction is common after pelvic fracture, and many facets of sex life are affected. The BSFI was well accepted, and is a useful screening tool for identifying patients with sexual dysfunction.
Mercury Toxicity: Clinical Presentations in Musculoskeletal Medicine
Authors: Saint-Phard Deborah , Van Dorsten Brent 
Published: December 2019

educational objectives
As a result of reading this article, physicians should be able to:
1. Recognize mercury toxicity as a possible cause of paresthesia and neuropathy in a musculoskeletal practice.
2. Describe the prevalence of mercury in the natural environment.
3. Define the pharmacology of inorganic and organic mercury.
4. Describe the clinical presentation and treatment of mercury toxicity from fish consumption.
5. Provide recommendations for safe consumption of fish.
The Role of Concomitant Biceps Tenodesis in Shoulder Arthroplasty for Primary Osteoarthritis: Results of a Multicentric Study
Authors: Fama Giuseppe , Edwards T Bradley , Boulahia Aziz , Kempf Jean-François , Boileau Pascal , Némoz Chantal , Walch Gilles 
Published: December 2019

abstract
This study evaluated the effects of concomitant biceps tenodesis in patients undergoing shoulder arthroplasty for primary osteoarthritis. Six hundred eighty-eight shoulders that had undergone replacement for primary glenohumeral arthritis were reviewed at a mean 43 months postoperatively. One hundred twenty-one patients had undergone a biceps tenodesis at arthroplasty, while the remaining patients did not. Tenodesis was significantly better than no tenodesis in most outcome parameters. No difference was found between the groups in complication rate. Biceps tenodesis is a useful adjunct to shoulder arthroplasty in the treatment of primary osteoarthritis.