bluuebunny/crossref_metadata_2025_split huggingface dataset:
THE IMPACT OF HONEY ON CHANGE IN NUTRITIONAL STATUS IN CHILDREN WITH POOR NUTRITION
Authors: Harmiyati Harmiyati , Soejoenoes Ariawan , Wahyuni M Sri , Aristiati Kun , Hadisaputro Soeharyo 
Published: February 2019

Background: Toddlers are vulnerable groups to malnutrition. Thus, to maintain their nutritional status is needed. Honey is considered having health benefits that may increase the nutritional status in children. However, little is known about the impact of honey on nutritional change in Sumbawa, Indonesia.
Objectives: The aim of this study is to analyze the effect of honey on changes in nutritional status in children with poor nutrition in the area of the Health Center of Lopok, Sumbawa, Indonesia
Methods: This study employed a quasi-experiment design with pretest-posttest with control group. The total sample in this study were 60 children recruited by simple random sampling, divided into 2 groups, namely 30 children in an intervention group and 30 children in a control group. The sampling technique used a simple random sampling. Data were analyzed using Mann Whitney and linear regression test.
Results: Findings showed that there were significant mean differences between the intervention and control group in term of weight (intervention 1.316; control 0.903), height (intervention 1.586; control 1.030), weight-for-height (W/H) z-score (intervention 0.713; control 0.595), weight-for-age (W/A) z-score (intervention 0.717; control 0.531), and height-for-age (H/A) z-score (intervention 0.847; control 0.423) with p-value < 0.05.
Conclusion: There was a significant effect of honey on changes in nutritional status in children with poor nutrition. It is suggested that health providers may use honey to take care of children under nutrition to increase their appetite and change their nutritional status.
SWEET POTATO (IPMOEA BATATAS L.) LEAF: ITS EFFECT ON PROLACTIN AND PRODUCTION OF BREAST MILK IN POSTPARTUM MOTHERS
Authors: Kusuma Ima Candra , Setiani Onny , Umaroh Umaroh , Pramono Noor , Widyawati Melyana Nurul , Kumorowulan Suryati 
Published: February 2019

Background: Sweet potato leaf is assumed to be one of alternative herbs that can increase breast milk production. However, there were no studies found in the literature that examine the sweet potato leaves to increase the levels of prolactin and milk production.
Objective: To examine the effect of sweet potato (Ipomoea batatas L.) leaf on the level of prolactin and milk production in postpartum mothers.
Methods: This was a quasi-experimental study with pretest-posttest design with control group, conducted on November 2016 to December 2016 in the Health Center (Puskesmas) of Boyolali I. Thirty respondents were selected using consecutive sampling, which were divided to be 15 respondents in intervention group and 15 respondents in control group. Enzyme-linked immunosorbent assay (ELISA) was used to measure prolactin levels, while breast milk production was measured based on the volume of breast milk and baby’s weight. Data were analyzed using Independent t-test and paired t-test.
Results: Finding showed that there was a significant difference in prolactin levels between the intervention (270.43) and control group (156.28) after intervention with p-value 0.000, and a significant difference in breast milk production in terms of breast milk volume (intervention group 136.33; and control group 119) with p-value 0.028; and baby’s weight (intervention group 3030.3; and control group 2787.33) with p-value 0.000.
Conclusion: There was a significant effect of sweet potato (Ipomoea batatas L.) leaf on the levels of prolactin and breast milk production. Thus, it could be suggested that sweet potato leaves should be considered to be one of alternative treatments for health care providers, especially for midwives to help breastfeeding mothers in increasing their breast milk production and prolactin levels. Further research is needed to examine all factors affecting breast milk production.
EFFECT OF MORINGA OLEIFERA ON LEVEL OF PROLACTIN AND BREAST MILK PRODUCTION IN POSTPARTUM MOTHERS
Authors: Sulistiawati Yuni , Suwondo Ari , Hardjanti Triana Sri , Soejoenoes Ariawan , Anwar M. Choiroel , Susiloretni Kun Aristiati 
Published: February 2019

Background: Breastfeeding among postpartum mothers has been a problem due to low milk supply. As a result, mothers often decide to give formula milk or other additional foods, which may affect infant’s growth and development.
Objective: This study aims to investigate the effect of moringa oliefera on the levels of prolactin and breast milk production (baby’s weight and sleep duration) in postpartum mothers.
Methods: Quasi-Experimental study with non-equivalent control group design. There were 30 respondents recruited by purposive sampling, consisted of 15 respondents in intervention group and 15 respondents in the control group. This study was conducted from November until December 2016 in Four Midwives Independent Practice (BPM) in the working area of the Health Center of Tlogosari Wetan Semarang. Data were analyzed using Independent t-test.
Results: Findings showed that there was a mean difference of prolactin level in the intervention group (231.72 ng / ml) and the control group (152.75 ng / ml), and a significant effect on increasing the levels of prolactin (p = 0.002). The mean of baby’s weight in the intervention group was 3783.33 grams and in the control group was 3599.00 grams. However, there was no significant effect of moringa oleifera on baby’s weight (p = 0.313> 0.05), while the mean difference on sleep duration was 128.20 minutes in the intervention group and 108.80 minutes in the control group. There was a significant effect on baby’s sleep duration (p= 0.000).
Conclusion: There were significant effects of moringa oleifera on mother’s prolactin and sleep duration of the baby. However, there was no significant effect on baby’s weight. Thus, it can be suggested that moringa oleifera can be used as an alternative treatment to increase breast milk production and prolactin hormones. Midwives should promote the benefits of moringa leaves as one of alternative supplements.
RELATIONSHIP BETWEEN NURSING AND ELDERLY CARE STUDENTS’ ATTITUDES TOWARDS AGEISM
Authors: Çayir Yilmaz Merve , Ince Fatma Zehra 
Published: February 2019

Background: Perceptions of individuals and society about the elderly are reflected in the services provided to them. These reflections might be revealed in various fields such as health care services and sufficient job opportunities, or they could be revealed in the issue of discrimination against the elderly, which is a problem emerging in advanced ages.
Objective: This study aims to identify the relationship between nursing and elderly care program students’ attitudes towards ageism.
Methods: This study, which is descriptive and relational method, was conducted between November and December, 2016. The participants were 220 students. The data were collected through a questionnaire, and the Ageism Attitude Scale, and were analyzed using t-test, two-way multivariate analysis of variance (MANOVA) and one-way analysis of variance (ANOVA).
Findings: Results show that the students generally had positive attitudes towards ageism. Nursing department students received significantly higher scores in the Limiting the Elderly Person’s Life sub-dimension and Ageism Attitude Scale in comparison to Elderly Care Program students. 3rd year nursing department students had higher scores in the Ageism Attitudes Scale in comparison to 1st and 2nd year nursing department students and students in the Elderly Care Program. “Positive Discrimination towards the Elderly” sub-dimension and the “Ageism Attitudes Scale” total scores were found to be significantly higher in nursing department students according to the variable of desire to work in a geriatric service in the future. (p<0.05).
Conclusion: This study found that students had positive attitudes towards ageism, and nursing students’ Ageism Attitudes Scale mean scores were higher than those of elderly care program students. More comprehensive studies are needed in order to improve students’ attitudes towards elderly people.
EFFECT OF PROGRESSIVE MUSCULAR RELAXATION ON ANXIETY LEVELS IN PATIENTS WITH CHRONIC KIDNEY DISEASE UNDERGOING HEMODIALYSIS IN THE GENERAL HOSPITAL OF TUGUREJO SEMARANG, INDONESIA
Authors: Astuti Ary , Anggorowati Anggorowati , Johan Andrew 
Published: February 2019

Background: Patients with chronic kidney disease undergoing hemodialysis suffer changes in lifestyle, which cause physical and psychosocial problems, particularly anxiety. Progressive muscular relaxation is considered as an intervention to reduce anxiety.
Objective: This study aims to examine the effect of progressive muscular relaxation in in reducing anxiety in patients with chronic kidney disease undergoing hemodialysis.
Methods: This study used a quasi-experimental design involved 78 respondents, with 38 randomly assigned in the intervention and control group. The progressive muscular relaxation was performed on 14 muscle groups for 4-week period. Hamilton anxiety rating scale was used to measure anxiety. Univariate, bivariate and multivariate analyses were performed for data analyses.
Results: The results showed a statistically significant difference in anxiety values between the intervention and control group with p-value 0.000 (<0.05).
Conclusion: There was a significant effect of progressive muscular relaxation in reducing anxiety in patients with chronic kidney disease undergoing hemodialysis. The results of this study is expected to be one reference in making the progressive muscular relaxation as a nursing intervention in reducing anxiety in patients undergoing hemodialysis.
HOME CARE NURSES’ ROLES IN ENHANCING QUALITY OF NURSING CARE FOR PATIENTS AT HOME: A PHENOMENOLOGICAL STUDY
Authors: Ligita Titan 
Published: February 2019

Background: Provision of health care service at home is one of the advanced forms of care for patients being discharged from hospitalization. Little is known about the experience of nurses providing home care services through a nursing home-care model especially in Indonesian context.
Objective: This study aims to explore the experience in order to increase understanding on the form of home care provision, and consequently the nurses may understand the form of home care globally.
Methods: This study employed a phenomenological design and performed interview in the process of data collection. Data were analysed by using content analysis.
Results: The main contexts of home care nurse experiences were generated. There were definition and role of home care nurses, the involvement of family members in the provision of care, the facilitating and hindering factors contributed to home care provision as well as manual on providing home care nursing.
Conclusion: The implication from this study is that nursing care should be given to the patients continuously and consequently the need for family involvement is important. Additionally, in providing the home care, a proper manual is needed by home care nurses as the guidance to give best quality of care to patients.
Принципи сучасного арт-менеджменту у проведенні заходів ІХ Міжнародної Пасхальної асамблеї-2017
Authors: Rozhok Oleksandr 
Published: February 2019

У статті розглянуто програми заходів під час Пасхальних асамблей, наголошено, що, формуючи їх зміст, їх організатори популяризують духовну музику, сучасне музичне виконавство. Згідно з принципами сучасного арт-управління (арт-менеджменту), важливого значення набувають критерії формування програм проведення таких акцій. Так, започаткована 2009 року, Асамблея об’єднала найкращих виконавців України ідеєю духовності під гаслом «Господи, Господи, силою Твоєю!». Від самого початку головною умовою участі в ній було виконання канонічної духовної хорової музики. Її організатори надавали перевагу духовним творам, які звучать під час Пасхальних богослужінь. Щороку ці програми збагачувалися й урізноманітнювалися відповідно до мети і завдань заходу. Програми ІІ Асамблеї-2010 мали свою специфіку – репертуарну і виконавську, боце вже був міжнародний захід. VІ Міжнародна Пасхальна асамблея-2014 відбувалась під новим гаслом – «Духовність єднає Україну» відповідно до особливої соціально-політичної ситуації, яка склалася в Україні наприкінці 2013–початку 2014 років, і це логічно відбилося у змісті програм. Під час VІІ Міжнародної Пасхальної асамблеї-2015 організатори прагнули наголосити на її миротворчій місії, протистояти дестабілізаційним викликам сучасності. Охарактеризовано заходи ІХ Міжнародної Пасхальної асамблеї-2017 – музичні діалоги, тематичні вечори, музичні присвяти, вечори пам’яті, конференції, благодійні концерти, розкрито їх значення у розкритті духовного і творчого потенціалу українського суспільства як основи для налагодження мирних відносин з іншими народами. Формуючи програми заходів, організатори і керівники проекту дбають, щоб під час їх проведення панувало творче піднесення, щоб мистецтво сприяло згуртуванню духовних сил у суспільстві, зміцнювало міжнаціональні відносини, підносило роль культурного діалогу й утверджувало його як єдино мирний і перспективний в сучасному світі.
Ноктюрн ор. 16 І. Я. Падеревського: стильовий та інтерпретаційний аспекти
Authors: Nechepurenko Viktoria 
Published: February 2019

Мета статті. Виявити стильові особливості Ноктюрну ор. 16 №4 І. Я. Падеревського, а також інтерпретаційну варіантність його тексту на прикладі виконавських версій К. Кіннера і Х. Рутковського. Проаналізувати індивідуальні риси композитора на прикладі даного твору. Методологія дослідження передбачає застосування теорії інтерпретації, розробленої В. Г. Москаленко, а також історичного та компаративного аналізу, які слугують підвалинами у даній розвідці. Наукова новизна дослідження полягає у тому, що вперше в українському музикознавстві проаналізовано Ноктюрн І.Я. Падеревського у стильовому та інтерпретаційному аспектах. Висновки. Обраний для аналізу твір І. Падеревського є яскравим зразком пізньоромантичної фортепіанної мініатюри. В ньому, з одного боку проявляється відданість створеній Ф. Шопеном традиції, а з іншого – присутні тенденції музичної мови доби fin de siècle. Прикладом багатогранності музичного тексту Ноктюрну І. Падеревського стають дві виконавські версії створені Х. Рутковським і К. Кіннером.
Spitzer Microlensing Parallax for OGLE-2016-BLG-1067: A Sub-Jupiter Orbiting an M Dwarf in the Disk
Authors: Calchi Novati S. , Suzuki D. , Udalski A. , Gould A. , Shvartzvald Y. , Bozza V. , Bennett D. P. , Beichman C. , Bryden G. , Carey S. , Gaudi B. S. , Henderson C. B. , Yee J. C. , Zhu W. ,   (Spitzer team), Abe F. , Asakura Y. , Barry R. , Bhattacharya A. , Bond I. A. , Donachie M. , Evans P. , Fukui A. , Hirao Y. , Itow Y. , Kawasaki K. , Koshimoto N. , Li M. C. A. , Ling C. H. , Matsubara Y. , Miyazaki S. , Muraki Y. , Nagakane M. , Ohnishi K. , Ranc C. , Rattenbury N. J. , Saito To. , Sharan A. , Sullivan D. J. , Sumi T. , Tristram P. J. , Yamada T. , Yonehara A. ,   (MOA Collaboration), Mróz P. , Poleski R. , Skowron J. , Szymański M. K. , Soszyński I. , Kozłowski S. , Pietrukowicz P. , Ulaczyk K. , Pawlak M. ,   (OGLE Collaboration), Albrow M. D. , Chung S.-J. , Han C. , Hwang K.-H. , Jung Y. K. , Ryu Y.-H. , Shin I.-G. , Zang W. , Cha S.-M. , Kim D.-J. , Kim H.-W. , Kim S.-L. , Lee C.-U. , Lee D.-J. , Lee Y. , Park B.-G. , Pogge R. W. ,   (KMTNet Collaboration)
Published: February 2019

Abstract
We report the discovery of a sub-Jupiter-mass planet orbiting beyond the snow line of an M dwarf most likely in the Galactic disk as part of the joint Spitzer and ground-based monitoring of planetary microlensing anomalies toward the Galactic bulge. Most of the microlensing parameters are strongly constrained by the light-curve modeling, and in particular there is a Spitzer-based measurement of the microlens parallax, π
E. However, there are no caustic crossings, so the angular Einstein radius has only an upper limit based on the light-curve modeling alone. Additionally, the analysis leads us to identify eight degenerate configurations: the fourfold microlensing parallax degeneracy being doubled by a degeneracy in the caustic structure present at the level of the ground-based solutions. To calculate the physical parameters, and at the same time to break the parallax degeneracy, we make use of a series of arguments: the χ
2 hierarchy, the Rich argument (stating that the small-parallax solution is more likely), and a prior Galactic model. The preferred configuration, favored by a likelihood ratio of at least 4000, is for a host at

with mass

, orbited by a Saturn-like planet with

at projected separation

, about 2.1 times beyond the system snow line. Therefore, it adds to the growing population of sub-Jupiter planets orbiting beyond the snow line of M dwarfs discovered by microlensing. Based on the rules of the real-time protocol for the selection of events to be followed up with Spitzer, this planet will not enter the sample for measuring the Galactic distribution of planets.
Forward Modeling of the Kepler Stellar Rotation Period Distribution: Interpreting Periods from Mixed and Biased Stellar Populations
Authors: van Saders Jennifer L. , Pinsonneault Marc H. , Barbieri Mauro 
Published: February 2019

Abstract
Stellar surface rotation carries information about stellar parameters—particularly ages—and thus the large rotational data sets extracted from Kepler time series represent powerful probes of stellar populations. In this article, we address the challenge of interpreting such data sets with a forward-modeling exercise. We combine theoretical models of stellar rotation, a stellar population model for the galaxy, and prescriptions for observational bias to predict the rotation distribution in the Kepler field under standard “vanilla” assumptions. We arrive at two central conclusions: first, that standard braking models fail to reproduce the observed distribution at long periods, and second, that the interpretation of the period distribution is complicated by a mixture of evolutionary states and observational uncertainties. If we assume that the detectability of rotational signatures scales with the Rossby number, we can show that the observed period distribution contains an apparent “Rossby edge” at

, above which long-period, high Rossby number stars are either absent or undetected. This threshold suggests either that weakened magnetic braking is in operation in the full Kepler population or that stars undergo a transition in spottedness and activity. We discuss the observations necessary to disentangle these competing scenarios. Regardless of the physical origin of the edge, it biases the inferred age distributions, affecting stars older than ∼9 Gyr at

, older than

at solar temperatures, and

at 6500 K. Below

, rotation periods should be viable age diagnostics in even the oldest stars in the population.
Search for Gamma-Ray Emission from the Sun during Solar Minimum with the ARGO-YBJ Experiment
Authors: Bartoli B. , Bernardini P. , Bi X. J. , Cao Z. , Catalanotti S. , Chen S. Z. , Chen T. L. , Cui S. W. , Dai B. Z. , D’Amone A. , Danzengluobu  , Mitri I. De , Piazzoli B. D’Ettorre , Girolamo T. Di , Sciascio G. Di , Feng C. F. , Feng Zhaoyang , Feng Zhenyong , Gao W. , Gou Q. B. , Guo Y. Q. , He H. H. , Hu Haibing , Hu Hongbo , Iacovacci M. , Iuppa R. , Jia H. Y. , Labaciren  , Li H. J. , Li Z. , Liu C. , Liu J. , Liu M. Y. , Lu H. , Ma L. L. , Ma X. H. , Mancarella G. , Mari S. M. , Marsella G. , Mastroianni S. , Montini P. , Ning C. C. , Perrone L. , Pistilli P. , Salvini P. , Santonico R. , Shen P. R. , Sheng X. D. , Shi F. , Surdo A. , Tan Y. H. , Vallania P. , Vernetto S. , Vigorito C. , Wang H. , Wu C. Y. , Wu H. R. , Xue L. , Yang Q. Y. , Yang X. C. , Yao Z. G. , Yuan A. F. , Zha M. , Zhang H. M. , Zhang L. , Zhang X. Y. , Zhang Y. , Zhao J. , Zhaxiciren  , Zhaxisangzhu  , Zhou X. X. , Zhu F. R. , Zhu Q. Q. ,   (The ARGO-YBJ Collaboration)
Published: February 2019

Abstract
The hadronic interaction of cosmic rays with solar atmosphere can produce high energy gamma-rays. The gamma-ray luminosity is correlated both with the flux of primary cosmic rays and the intensity of the solar magnetic field. The gamma-rays below 200 GeV have been observed by Fermi without any evident energy cutoff. The bright gamma-ray flux above 100 GeV has been detected only during solar minimum. The only available data in the TeV range come from the HAWC observations, however, outside the solar minimum. The ARGO-YBJ data set has been used to search for sub-TeV/TeV gamma-rays from the Sun during the solar minimum from 2008 to 2010, the same time period covered by the Fermi data. A suitable model containing the Sun shadow, solar disk emission, and inverse-Compton emission has been developed, and the chi-square minimization method was used to quantitatively estimate the disk gamma-ray signal. The result shows that no significant gamma-ray signal is detected and upper limits to the gamma-ray flux at 0.3–7 TeV are set at the 95% confidence level. In the low energy range these limits are consistent with the extrapolation of the Fermi-LAT measurements taken during solar minimum and are compatible with a softening of the gamma-ray spectrum below 1 TeV. They also provide an experimental upper bound to any solar disk emission at TeV energies. Models of dark matter annihilation via long-lived mediators predicting gamma-ray fluxes >10−7 GeV cm−2 s−1 below 1 TeV are ruled out by the ARGO-YBJ limits.
A Long-duration Luminous Type IIn Supernova KISS15s: Strong Recombination Lines from the Inhomogeneous Ejecta–CSM Interaction Region and Hot Dust Emission from Newly Formed Dust*
Authors: Kokubo Mitsuru , Mitsuda Kazuma , Morokuma Tomoki , Tominaga Nozomu , Tanaka Masaomi , Moriya Takashi J. , Yoachim Peter , Ivezić Željko , Sako Shigeyuki , Doi Mamoru 
Published: February 2019

Abstract
We report the discovery of an SN 1988Z–like type IIn supernova KISS15s found in a low-mass star-forming galaxy at redshift z = 0.038 during the course of the Kiso Supernova Survey (KISS). KISS15s shows long-duration optical continuum and emission line light curves, indicating that KISS15s is powered by a continuous interaction between the expanding ejecta and dense circumstellar medium (CSM). The Hα emission line profile can be decomposed into four Gaussians of narrow, intermediate, blueshifted intermediate, and broad velocity width components, with a full width at half maximum of ≲100, ∼2000, and ∼14,000 km s−1 for the narrow, intermediate, and broad components, respectively. The presence of the blueshifted intermediate component, of which the line-of-sight velocity relative to the systemic velocity is about −5000 km s−1, suggests that the ejecta-CSM interaction region has an inhomogeneous morphology and anisotropic expansion velocity. We found that KISS15s shows increasing infrared continuum emission, which can be interpreted as hot dust thermal emission of T ∼ 1200 K from newly formed dust in a cool, dense shell in the ejecta-CSM interaction region. The progenitor mass-loss rate, inferred from bolometric luminosity, is

, where v

w
is the progenitor’s stellar wind velocity. This implies that the progenitor of KISS15s was a red supergiant star or a luminous blue variable that had experienced a large mass loss in the centuries before the explosion.