bluuebunny/crossref_metadata_2025_split huggingface dataset:
FEN BİLİMLERİ ÖĞRETMEN ADAYLARI KİMYA BİLGİLERİNİ GÜNLÜK YAŞAMLARIYLA NE KADAR İLİŞKİLENDİREBİLİYOR?
Authors: CANPOLAT Erdal , ATEŞ Hasan , AYYILDIZ Kübra 
Published: July 2019

Bu çalışmada, üniversite 1.
,2. ,3. ve 4. sınıf fen bilgisi öğrencilerinin kimya bilgilerini günlük
yaşamlarıyla ilişkilendirebilme düzeyleri açısından hazır bulunuşlukları ve
günlük yaşam kimyasına karşı tutumları tespit edilmeye çalışılmıştır.
Araştırmanın örneklemini 2017-2018 eğitim-öğretim yılında Fırat Üniversitesi ve
Siirt Üniversitesi Fen Bilgisi Öğretmenliği 1. ,2. ,3. ve 4. sınıflarında okuyan
öğretmen adayları oluşturmaktadır. Çalışma Fırat Üniversitesi’nden 208, Siirt
Üniversitesi’nden 171 öğretmen adayı ile yürütülmüştür. Araştırmada 14 açık
uçlu sorudan oluşan “Günlük Olayları Açıklama Testi” (GOAT) ve 25 soruluk 5
likert tipi bir ölçekten oluşan “Günlük Yaşam Kimyası Tutum Ölçeği” (GYKTÖ)
kullanılmıştır. Parametrik testler (t-testi, ANOVA) ve parametrik olmayan
testler (Kruskal Wallis ve Mann-Whitney U Testi) ile analiz edilmiştir. Sonuç
olarak, fen bilgisi öğretmen adaylarının günlük yaşam olaylarıyla olan
ilişkileri ve günlük yaşam kimyasına karşı tutumları arasında anlamlı bir
ilişki olduğu bulunmuştur. Ancak günlük hayatta karşılaşılan olayları
açıklamada yetersiz oldukları ve konular ile ilgili kavram yanılgılarına sahip
oldukları gözlenmiştir. Extended abstract: İngilizce uzun özet bölümüdür. Makalenin kaynaklar bölümünden sonra “Extended Abstract” başlığı altında geniş bir İngilizce özet bulunmalıdır. “Extended Abstract” 750-1000 sözcükten oluşmalı, Purpose, Method, Results, Discussion, Conclusion bölümlerini içermeli ve atıf içermemelidir. İngilizce özet dergiye gönderilmeden önce dil bilgisi hatası içermemesi için alanda uzman biri tarafından kontrol edilmelidir.
Recensión de Libros: La psicoterapia dei processi di significato personale dei disturbi psicopatologici. Manuale teorico-pratico
Authors: Ugarte Pérez Carla 
Published: July 2019

Recensión del libro " La psicoterapia dei processi di significato personale dei disturbi psicopatologici. Manuale teorico-pratico". EDITORES: Quiñones, A., Cimbolli, P. y Pascale, A.Editorial Casa Alpes, RomaAño de publicación 2014ISBN-10: 8865312076
Entrenamiento en “Open Mindfuness: Un Estudio Piloto
Authors: Miró Barrachina María Teresa , Ibáñez Ignacio , Felipe Isaura , García Nieves M. 
Published: July 2019

The purpose of this study is to explore the effects of a mindfulness training program, "The Open Mindfulness Fundamental Training" (OMFT), on a non-clinical sample of 27 persons. On the one hand, it was intended to study pre-post intervention changes and, on the other hand, whether previous experience was modulating these changes. Results showed significant differences in several dimensions of interoceptive awareness: the ability to control attention regarding body sensations, the ability to regulate body tensions paying attention to embodied sensations, and the ability to trust that the body is safe and reliable. In addition, decentering skills improve significantly after training, as well as perception of the awareness level and attention to the present experience during a specific time in a given context. Previous experience in meditation was not related to participants improvement after the intervention, so all of them were equally benefited.
Measuring adherence to therapy in apparent treatment-resistant hypertension: a feasibility study in Irish primary care
Authors: Hayes Peter , Casey Monica , Glynn Liam G , Molloy Gerard J , Durand Hannah , O’Brien Eoin , Dolan Eamon , Das Kishor , Newell John , Finn David , Harhen Brendan , Conneely Ann , Murphy Andrew W 
Published: July 2019

BackgroundApparent treatment-resistant hypertension (aTRH) is defined as uncontrolled blood pressure (BP) in patients taking three or more antihypertensive medications. Some patients will have true treatment-resistant hypertension, some undiagnosed secondary hypertension, while others have pseudo-resistance. Pseudo-resistance occurs when non-adherence to medication, white-coat hypertension (WCH), lifestyle, and inadequate drug dosing are responsible for the poorly controlled BP.AimTo examine the feasibility of establishing non-adherence to medication, for the first time in primary care, using mass spectrometry urine analysis. Operationalisation would be established by at least 50% of patients participating and 95% of samples being suitable for analysis. Clinical importance would be confirmed by >10% of patients being non-adherent.Design and settingEligible patients with aTRH (n = 453) in 15 university research-affiliated Irish general practices were invited to participate.MethodParticipants underwent mass spectrometry urine analysis to test adherence and ambulatory BP monitoring (ABPM) to examine WCH.ResultsOf the eligible patients invited, 52% (n = 235) participated. All 235 urine samples (100%) were suitable for analysis: 174 (74%) patients were fully adherent, 56 (24%) partially adherent, and five (2%) fully non-adherent to therapy. A total of 206 patients also had ABPM, and in total 92 (45%) were categorised as pseudo-resistant. No significant associations were found between adherence status and patient characteristics or drug class.ConclusionIn patients with aTRH, the authors have established that it is feasible to examine non-adherence to medications using mass spectrometry urine analysis. One in four patients were found to be partially or fully non-adherent. Further research on how to incorporate this approach into individual patient consultations and its associated cost-effectiveness is now appropriate.
ANALISIS POLA DISTRIBUSI USAHA TELUR IKAN TERBANG DI KECAMATAN GALESONG KABUPATEN TAKALAR
Authors: HERDIANA HERDIANA 
Published: July 2019

This study aims to (1) Identify the distribution patterns of flying fish eggs in Takalar District, (2) Analyze the profit and marketing margins of flying fish egg marketing institutions, (3) Analyze and identify distribution problems in the flying fish egg marketing agency. This research was conducted in the village of Palalakan, Galesong District, Takalar District. Data was collected through observation and structured and in-depth interviews with the samples selected by purposive sampling on 43 respondents consisting of 30 patriotic fishermen, 10 Papalele, 2 collecting traders and 1 exporter using qualitative and quantitative descriptive analysis (margin formula, profit) and Fishbone analysis. The results of the study show that (1) The distribution pattern of flying fish eggs is one-way in accordance with co-workers where fishermen market to papalele, papalele to collectors, and collector traders to exporters (2) Exporters have greater margins and profits than other institutions which are Rp.50,000 per kilogram, (3) The results of the fishbon analysis show that the distribution pattern of flying fish eggs shows that patoranist fishermen are people who do not have big profits because they do not have full power in determining prices due to the inability of fishermen to finance their own business capital loans from other institutions especially to papalele, so there needs to be a change in the pattern of distribution and the involvement of the government to help patoranist fishermen so they can have their own capital so that they do not depend on other business institutions
ANALISIS FAKTOR-FAKTOR YANG MEMPENGARUHI PENDAPATAN UMKM DI KABUPATEN TABANAN
Authors: ARTINI NI RAI 
Published: July 2019

This study aims to determine the effect of variables of capital and labor on MSME income in Tabanan Regency. This study uses 95 respondents spread across 10 Districts of Tabanan Regency, then the data are analyzed using multiple linear regression. The results of the analysis simultaneously show that the variables of capital and labor have a significant effect on MSME income in Tabanan Regency. While the results of the partial analysis of the variables of capital and labor have a real influence on the income of MSMEs in Tabanan Regency. Capital is the dominant variable that affects income, the higher the capital will increase the amount of additional production so as to increase income. Likewise with labor, the more labor, the production will also increase
Enseñanza de la Bioética en la Educación Universitaria
Authors: Llacsa Soto León 
Published: July 2019

Se revisa el tema, considerado al inicio como ética, y su realidad académica en la Universidad Se fundamenta la necesidad de la enseñanza de la bioética, su desarrollo, en todas las profesiones y no sólo en salud. Que su objetivo, es generar conocimientos, aprendizajes, reflexiones, actitudes y comportamiento ético sociales. En su metodología resalta el aprendizaje basado en problemas, por favorecer el razonamiento ético, cambio de actitudes y trabajo en equipo; los Seminarios y los estudios de caso como más usados. Se concluye que en la universidad es imprescindible la formación en bioética para mejorar la calidad educativa, promover comportamientos éticos con sentido, personal, profesional y social; que el aprendizaje basado en problemas, seminarios, estudio de casos, entre otros, permiten aprendizajes que respetan, valores, derechos, democracia y ambiente. Así mismo que la responsabilidad social de la calidad educativa es función de la gestión institucional y de sus actores.
Kajian sifat fsik dan serat pangan pada gѐblek substitusi daun kelor (Moringa oleifera L.)
Authors: Meiyana Klara Tri , Dewi Devillya Puspita , Kadaryati Sri 
Published: July 2019

Latar Belakang : Penyakit degeneratif menduduki urutan utama sebagai penyebab kematian di Kulon Progo. Salah satu upaya pencegahan penyakit degeneratif dilakukan melalui pemberian makanan tinggi serat. Tepung daun kelor memiliki kandungan serat pangan yang tinggi. Pencampuran tepung daun kelor dalam pembuatan geblek diharapkan meningkatkan kadar serat pangan pada geblek. Namun hal ini juga dapat mempengaruhi sifat fisik geblek, sehingga perlu diketahui vasiasi substitusi yang sesuai. Tujuan: Mengetahui pengaruh variasi substitusi tepung daun kelor terhadap sifat fisik dan kadar serat pangan geblek. Metode Penelitian : Jenis penelitian ini adalah observasional. Geblek dibuat dengan empat variasi, yaitu pencampuran tepung daun kelor sebanyak 0% (A), 5% (B), 7,5% (C), 10% (D). Penelitian ini dilaksanakan pada bulan Januari-Februari 2017. Pembuatan geblek dan uji sifat fisik dilakukan di Laboratorium Dietetik/Gizi Universitas Respati Yogyakarta. Sifat fisik geblek diamati secara subjektif pada warna, aroma, rasa dan tekstur. Pengujian kadar serat pangan menggunakan metode enzimatis di Laboratorium Chem-mix Pratama Yogyakarta. Data disajikan secara deskriptif. Hasil : Semakin banyak pencampuran tepung daun kelor pada geblek menyebabkan warna geblek semakin hijau, aroma semakin khas daun kelor (langu), rasa semakin khas daun kelor (sepat), dan tekstur semakin kehilangan kekenyalannya. Semakin banyak tepung daun kelor menyebabkan kadar serat geblek semakin tinggi. Serat pangan tertinggi pada geblek D yaitu 14,02%. Kesimpulan : Substitusi tepung daun kelor berpegaruh sifat fisik dan meningkatkan serat pangan geblek.
Dealing With δ-Scuti Variables: Transit Light Curve Analysis of Planets Orbiting Rapidly Rotating, Seismically Active A/F Stars
Authors: Ahlers John P. , Barnes Jason W. , Myers Samuel A. 
Published: July 2019

Abstract
We measure the bulk system parameters of the seismically active, rapidly rotating δ-Scuti KOI-976 and constrain the orbit geometry of its transiting binary companion using a combined approach of asteroseismology and gravity-darkening light curve analysis. KOI-976 is a 1.62 ± 0.2 M
⊙ star with a measured v sin(i) of 120 ± 2 km s−1 and seismically induced variable signal that varies by ∼0.6% of the star’s total photometric brightness. We take advantage of the star’s oblate shape and seismic activity to perform three measurements of its obliquity angle relative to the plane of the sky. We first apply a rotational splitting theory to the star’s variable signal observed in short-cadence Kepler photometry to constrain KOI-976's obliquity angle, and then subtract off variability from that data set using the linear algorithm for significance reduction software LASR. We perform gravity-darkened fits to Kepler variability-subtracted short-cadence photometry and to Kepler’s phase-folded long-cadence photometry to obtain two more measurements of the star’s obliquity. We find that the binary system transits in a grazing configuration with measured obliquity values of 36° ± 17°, 46° ± 16°, and 43° ± 20°, respectively, for the three measurements. We perform these analyses as a way to demonstrate overcoming the challenges high-mass stars can present to transit light curve fitting and to prepare for the large number of exoplanets that the Transiting Exoplanet Survey Satellite will discover orbiting A/F stars.
Characterizing K2 Candidate Planetary Systems Orbiting Low-mass Stars. IV. Updated Properties for 86 Cool Dwarfs Observed during Campaigns 1–17
Authors: Dressing Courtney D. , Hardegree-Ullman Kevin , Schlieder Joshua E. , Newton Elisabeth R. , Vanderburg Andrew , Feinstein Adina D. , Duvvuri Girish M. , Arnold Lauren , Bristow Makennah , Thackeray Beverly , Abrahams Ellianna Schwab , Ciardi David R. , Crossfield Ian J. M. , Yu Liang , Martinez Arturo O. , Christiansen Jessie L. , Crepp Justin R. , Isaacson Howard 
Published: July 2019

Abstract
We present revised stellar properties for 172 K2 target stars that were identified as possible hosts of transiting planets during Campaigns 1–17. Using medium-resolution near-infrared spectra acquired with the NASA Infrared Telescope Facility/SpeX and Palomar/TripleSpec, we found that 86 of our targets were bona fide cool dwarfs, 74 were hotter dwarfs, and 12 were giants. Combining our spectroscopic metallicities with Gaia parallaxes and archival photometry, we derived photometric stellar parameters and compared them to our spectroscopic estimates. Although our spectroscopic and photometric radius and temperature estimates are consistent, our photometric mass estimates are systematically ΔM
⋆ = 0.11 M
⊙ (34%) higher than our spectroscopic mass estimates for the least massive stars (M
⋆,phot < 0.4 M
⊙). Adopting the photometric parameters and comparing our results to parameters reported in the Ecliptic Plane Input Catalog, our revised stellar radii are ΔR
⋆ = 0.15 R
⊙ (40%) larger, and our revised stellar effective temperatures are roughly ΔT
eff = 65 K cooler. Correctly determining the properties of K2 target stars is essential for characterizing any associated planet candidates, estimating the planet search sensitivity, and calculating planet occurrence rates. Even though Gaia parallaxes have increased the power of photometric surveys, spectroscopic characterization remains essential for determining stellar metallicities and investigating correlations between stellar metallicity and planetary properties.
Toward a Full MHD Jet Model of Spinning Black Holes. I. Framework and a Split Monopole Example
Authors: Huang Lei , Pan Zhen , Yu Cong 
Published: July 2019

Abstract
In this paper, we construct a framework for investigating the magnetohydrodynamical jet structure of spinning black holes (BHs), where electromagnetic fields and fluid motion are governed by the Grad–Shafranov equation and the Bernoulli equation, respectively. Assuming steady and axisymmetric jet structure, we can self-consistently obtain electromagnetic fields, fluid energy density, and velocity within the jet, given proper plasma loading and boundary conditions. Specifically, we structure the two coupled governing equations as two eigenvalue problems, and develop full numerical techniques for solving them. As an example, we explicitly solve the governing equations for the split monopole magnetic field configuration and simplified plasma loading on the stagnation surface where the poloidal fluid velocity vanishes. As expected, we find the rotation of magnetic field lines is dragged down by fluid inertia, and the fluid as a whole does not contribute to energy extraction from the central BH, i.e., the magnetic Penrose process is not working. However, if we decompose the charged fluid as two oppositely charged components, we find the magnetic Penrose process does work for one of the two components when the plasma loading is low enough.
Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star-forming Galaxies at z ∼ 3
Authors: Jarugula Sreevani , Vieira Joaquin D. , Spilker Justin S. , Apostolovski Yordanka , Aravena Manuel , Béthermin Matthieu , Breuck Carlos de , Chen Chian-Chou , Cunningham Daniel J. M. , Dong Chenxing , Greve Thomas , Hayward Christopher C. , Hezaveh Yashar , Litke Katrina C. , Mangian Amelia C , Narayanan Desika , Phadke Kedar , Reuter Cassie A. , Werf Paul Van der , Weiss Axel 
Published: July 2019

Abstract
Water (H2O), one of the most ubiquitous molecules in the universe, has bright millimeter-wave emission lines that are easily observed at high redshift with the current generation of instruments. The low-excitation transition of H2O,

(ν
rest = 987.927 GHz), is known to trace the far-infrared (FIR) radiation field independent of the presence of active galactic nuclei (AGNs) over many orders of magnitude in FIR luminosity (

). This indicates that this transition arises mainly due to star formation. In this paper, we present spatially (∼0.″5 corresponding to ∼1 kiloparsec) and spectrally resolved (∼100 kms−1) observations of

in a sample of four strong gravitationally lensed high-redshift galaxies with the Atacama Large Millimeter/submillimeter Array. In addition to increasing the sample of luminous (>1012
L
⊙) galaxies observed with H2O, this paper examines the

relation on resolved scales for the first time at high redshift. We find that

is correlated with

on both global and resolved kiloparsec scales within the galaxy in starbursts and AGN with average

. We find that the scatter in the observed

relation does not obviously correlate with the effective temperature of the dust spectral energy distribution or the molecular gas surface density. This is a first step in developing

as a resolved star formation rate calibrator.
The Escape of the Hydrogen-rich Atmosphere of Exoplanets: Mass-loss Rates and the Absorption of Stellar Lyα
Authors: Yan Dongdong , Guo Jianheng 
Published: July 2019

Abstract
Because mass-loss rates are the function of the mean density of a planet and the stellar irradiation, we calculated about 450 models covering planets with different densities and stellar irradiation. Our results show that the mass-loss rates are dependent on the stellar irradiation and the mean density. However, the mass-loss rates predicted by the energy-limited equation are higher than those predicted by the hydrodynamic model when the integrated extreme ultraviolet flux is higher than ∼2 × 104 erg cm−2 s−1. The overestimation can be revised if the kinetic and thermal energies of the escaping atmosphere is included in the energy-limited equation. We found that the heating efficiencies are proportional to the product of the gravitational potential of the planet and the stellar irradiation. The mean absorption radii of stellar irradiation are 1.1–1.2 R

p
for Jupiter-like planets, while they vary in the range of 1.1–1.7 R

p
for planets with smaller sizes. We evaluated the absorption of stellar Lyα by the planetary atmosphere and found that the deeper Lyα absorptions tend to be located in the high stellar irradiation and low planetary mean density regions, and vice versa. Moreover, planets with mass-loss rates higher than 1011 g s−1 are likely to exhibit obvious absorptions. Finally, we suggest that the absorption levels are related to the inherent properties of exoplanets. The planets with larger sizes (or lower mean density) show strong Lyα absorptions. Neptune-like and Earth-like planets tend to have weak Lyα absorptions because of their small sizes (or high densities).
CO (J = 1–0) Observations toward Filamentary Molecular Clouds in the Galactic Region with l = [169.°75, 174.°75], b = [−0.°75, 0.°5]
Authors: Xiong Fang , Chen Xuepeng , Zhang Qizhou , Yang Ji , Fang Min , Zhang Miaomiao , Guo Weihua , Sun Li 
Published: July 2019

Abstract
We present observations of the CO isotopologues (12CO, 13CO, and C18O) toward the Galactic region with 169.°75 ≤ l ≤ 174.°75 and −0.°75 ≤ b ≤ 0.°5 using the Purple Mountain Observatory 13.7 m millimeter-wavelength telescope. Based on the 13CO (J = 1 − 0) data, we find five molecular clouds within the velocity range between −25 and 8 km s−1 that are all characterized by conspicuous filamentary structures. We have identified eight filaments with a length of 6.38–28.45 pc, a mean H2 column density of 0.70 × 1021–6.53 × 1021 cm−2, and a line mass of 20.24–161.91 M
☉ pc−1, assuming a distance of ∼1.7 kpc. Gaussian fittings to the inner parts of the radial density profiles lead to a mean FWHM width of 1.13 ± 0.01 pc. The velocity structures of most filaments present continuous distributions with slight velocity gradients. We find that turbulence is the dominant internal pressure to support the fragmentation of filaments instead of thermal pressure. Most filaments have virial parameters smaller than 2; thus, they are gravitationally bound. Four filaments have an LTE line mass close to the virial line mass. We further extract dense clumps using the 13CO data and find that 64% of the clumps are associated with the filaments. According to the complementary IR data, most filaments have associated Class II young stellar objects. Class I objects are mainly found to be located in the filaments with a virial parameter close to 1. Within two virialized filaments, 12CO outflows have been detected, indicating ongoing star-forming activity therein.
An Adaptive Scheduling Tool to Optimize Measurements to Reach a Scientific Objective: Methodology and Application to Measurements of Stellar Orbits in the Galactic Center
Authors: Hees A. , Dehghanfar A. , Do T. , Ghez A. M. , Martinez G. D. , Campbell R. , Lu J. R. 
Published: July 2019

Abstract
In various fields of physics and astronomy, access to experimental facilities or to telescopes is becoming more and more competitive and limited. It therefore becomes important to optimize the type of measurements and their scheduling to reach a given scientific objective and to increase the chances of success of a scientific project. In this communication, extending the work of Ford and of Loredo et al., we present an efficient adaptive scheduling tool aimed at prioritizing measurements in order to reach a scientific goal. The algorithm, based on the Fisher matrix, can be applied to a wide class of measurements. We present this algorithm in detail and discuss some practicalities such as systematic errors or measurement losses due to contingencies (such as weather, experimental failure, ...). As an illustration, we consider measurements of the short-period star S0-2 in our Galactic Center (GC). We show that the radial velocity measurements at the two turning points of the radial velocity curve are more powerful for detecting the gravitational redshift than measurements at the maximal relativistic signal. We also explicitly present the methodology that was used to plan measurements in order to detect the relativistic redshift considering systematics and possible measurement losses. For the future, we identify the astrometric turning points to be highly sensitive to the relativistic advance of the periastron. Finally, we also identify measurements particularly sensitive to the distance to our GC: the radial velocities around periastron and the astrometric measurements just before closest approach and at the maximal R.A. astrometric turning point.