bluuebunny/crossref_metadata_2025_split huggingface dataset:
HUBUNGAN PENGETAHUAN, SIKAP, DAN HYGIENE PERORANGAN PENJAMAH MAKANAN PADA PENYELENGGARAAN MAKANAN DI KANTIN SMA NEGERI 4 KENDARI
Authors: Gerung Jumartin , Rezki Wulandari Armelia 
Published: January 2022

Penjamah makanan di kantin SMA Negeri 4 Kendari menyatakan bahwa tidak pernah memperoleh penyuluhan tentang penyelenggaraan makanan yang memenuhi syarat kesehatan. Hal ini ditandai dengan sebagian besar penjamah makanan belum memenuhi syarat hygiene perorangan dalam menyelenggarakan makanan yang telah ditetapkan dalam Kemenkes RI. Penelitian ini bertujuan untuk menganalisis hubungan pengetahuan, sikap, dan hygiene perorangan penjamah makanan pada penyelenggaraan makanan di kantin SMA Negeri 4 Kendari. Jenis penelitian ini adalah penelitian observasional dengan desain penelitian cross sectional. Populasi dalam penelitian ini adalah penjamah makanan yang bekerja di kantin SMA Negeri 4 Kendari sebanyak 40 orang. Teknik pengambilan sampel purposive sampling dengan menggunakan rumus Slovin dengan jumlah sampel 36 orang. Metode analisis menggunakan uji statistik yakni uji Chi Square dan Phi. Hasil penelitian ini menunjukkan bahwa ada hubungan sedang antara pengetahuan pada penyelenggaraan makanan. Hubungan kuat antara sikap pada penyelenggaraan makanan. Hubungan sangat kuat antara hygiene perorangan pada penyelenggaraan makanan.
Kesimpulan pada penelitian ini adalah pengetahuan, sikap, dan hygiene perorangan merupakan faktor-faktor yang mempengaruhi penyelenggaraan makanan, penjamah makanan perlu mengikuti pelatihan mengenai penyelenggaraan makanan.
FAKTOR – FAKTOR YANG BERHUBUNGAN DENGAN PENYAKIT DERMATITIS PADA PEKERJA PENGANGKUT SAMPAH DI TPA PUUWATU KOTA KENDARI
Authors: Ulva Sitti Marya 
Published: January 2022

Data dari Dinas Kebersihan Kota Kendari pada tahun 2015 diketahui bahwa volume sampah yang dibuang ke tempat pembuangan akhir Puuwatu mencapai 680,24 m3/hari. Tujuan dari penelitian ini yaitu untuk mengetahui faktor – faktor yang berhubungan dengan penyakit dermatitis pada pekerja pengangkut sampah di tempat pembuangan akhir Puuwatu Kota Kendari. Jenis penelitian ini adalah survey analitik dengan pendekatan/desain Cross Sectional Study. Populasi Dalam penelitian ini sebanyak 70 orang dan jumlah sampel sebanyak 42 orang. Metode analisis menggunakan uji statistik Chi-Square.
Berdasarkan hasil penelitian diperoleh ada hubungan ketersedian air bersih nilai X2hit = 20,673 > X2tab = 3,841, ada hubungan kebiasaan mandi nilai X2hit = 18,497 > X2tab = 3,841 dan ada hubungan kebiasaan cuci tangan nilai X2hit = 11,573 > X2tab = 3,841 dengan penyakit dermatitis pada pekerja pengangkut sampah di tempat pembuangan akhir Puuwatu Kota Kendari.
Kesimpulan dari penelitian ini yaitu ada hubungan kuat ketersediaan air bersih, ada hubungan kuat kebiasaan mandi dan ada hubungan kuat kebiasaan cuci tangan dengan Kejadian Penyakit dermatitis pada pekerja pengangkut sampah di TPA Puuwatu Kota kendari.
FAKTOR-FAKTOR YANG BERHUBUNGAN DENGAN KEJADIAN DIARE PADA ANAK BALITA DI WILAYAH PESISIR KELURAHAN LAPULU KECAMATAN ABELI KOTA KENDARI
Authors: Fitri Rachmillah Fadmi  , Andi Mauliyana  , Zatyani Muthia Mangidi  
Published: January 2022

Diare merupakan gangguan buang air besar yang ditandai buang air besar lebih dari 3 kali sehari dengan konsentrasi tinja cair disertai darah. Berdasarkan data profil Puskesmas Abeli pada tahun 2016 terdapat 286 balita yang menderita diare kemudian pada tahun 2017 terdapat 269 balita yang menderita diare dan pada tahun 2018 terdapat 160 balita yang menderita diare. Tujuan penelitian ini untuk mengetahui faktor-faktor yang berhubungan dengan kejadian penyakit diare pada Balita di wilayah Pesisir Kelurahan Lapulu Kecamatan Abeli Kota Kendari. Jenis penelitian yang digunakan adalah analitik dengan pendekatan observasional yang menggunakan rancangan Cross Sectional Study. Populasi dalam penelitian ini berjumlah 96 balita. Jumlah sampel sebanyak 49 responden, dengan teknik penarikan sampel menggunakan Simple Random Sampling. Metode analisis menggunakan uji Chi-Square dan uji Phi. Hasil penelitian menunjukan bahwa ada hubungan sedang antara pengetahuan ibu p-value (0,012 < α 0,05), ada hubungan sedang antara penyediaan air bersih p-value (0,003< α 0,05), dan ada hubungan sedang antara jamban keluarga p-value (0,004 < α 0,05) dengan kejadian penyakit diare pada Balita di wilayah Pesisir Kelurahan Lapulu Kecamatan Abeli Kota Kendari.
Wychodząc z kina
Authors: Barthes Roland 
Published: January 2022

Esej Rolanda Barthes’a, pierwotnie opublikowany w czasopiśmie „Communications” (1975, nr 23), określa „sytuację kinową” jako „prehipnotyczną”. Autor analizuje warunki specyficzne dla sali kinowej, a także stan psychiczny widza przed wejściem do kina i po wyjściu z niego. Według Barthes’a ciemność sali kinowej w połączeniu z doświadczeniem wspólnotowym, a zarazem indywidualnym stanowi o specyfice kina. Autor artykułuje różnicę między kinem a telewizją, która kojarzy się z życiem rodzinnym i nie wywołuje takiej fascynacji jak kino. Zgodnie z podejściem psychoanalitycznym Barthes zachęca czytelnika do zatracenia się w doświadczeniu kinowym, ale ważny jest dla niego także dystans między widzem a ekranem. Autor zwraca uwagę na ideologiczny wymiar odbioru filmu w kinie, w efekcie czego zaprasza czytelnika do „zakochania się w dystansie”.
Ze względu na ograniczenia praw autorskich artykuł jest dostępny tylko w wydaniu papierowym.
Przemieszczona tożsamość. Kino PRL wobec problemu Ziem Zachodnich
Authors: Copik Ilona 
Published: January 2022

W artykule został podjęty problem „tożsamości przemieszczonej” rozumianej jako odgórny - narodowy i społeczny - projekt dla przestrzeni pojałtańskich. Chociaż celem projektu była homogenizacja narodowa oraz integracja w nowych granicach geograficznych i ustrojowych, faktycznie wywołał on kryzys przynależności i identyfikacji, dziedziczony przez kolejne pokolenia powojennych mieszkańców nowych terenów. Przedmiotem badań autorki są polskie filmy fabularne z lat 1956-1970, które stanowią reprezentację tytułowego zagadnienia, a których udział w recepcji „Ziem Odzyskanych” był znaczący. Twórcy tych filmów podejmowali temat migracji, osadnictwa i zagospodarowywania nowych obszarów, przez co zasadniczo wpływali na kształt zbiorowej wyobraźni. Analizie poszczególnych utworów towarzyszą pytania o to, w jaki sposób kino uczestniczyło w procesach konstrukcji monoetniczności, a także - na ile wyrażało racje polityczne oraz ukazywało życie codzienne, problemy adaptacyjne i konflikty społeczne. Celem podjętych badań jest uzupełnienie dotychczasowej wiedzy z zakresu historii kina polskiego okresu PRL oraz jego kontekstów politycznych i społeczno-kulturowych związanych z tematyką Ziem Zachodnich.
Iron-Deficiency Anemia Related to Ancylostoma duodenale Infection in 67 Years Old Female Patient
Authors: Prasetyo Widodo Adi , Armen Ahmad  
Published: January 2022

Background. Ancylostomiasis is an infection caused by hookworms. It is estimated that hookworms infect 1.2 billion people worldwide and cause higher morbidity than other types, mainly due to iron deficiency anemia. Hookworm infection increases with age. The main clinical manifestations are abdominal pain, features of iron deficiency anemia and hypoproteinemia. Diagnosis is based on the finding of characteristic eggs in the stool.
Case presentation. A 67-year-old female patient had been administered into the Internal Medicine Ward of Dr. M. Djamil Padang Hospital with the main complaint of weakness, fatigue, and lethargy which had increased since 3 days before being admitted to the hospital. The patient also had complaints of pale skin, fever, heartburn, decreased appetite and weight loss. The patient was admitted to the hospital with awareness of compost mentis, cooperative, and his general condition appeared to be moderately ill, blood pressure 130/90 mmHg, pulse rate 104 x/minute, regular pulse, adequate filling, respiratory rate 22 x/minute, temperature 37.8 C. On physical examination, the conjunctiva of the pantient’s eyes were anemic. Laboratory examination revealed Hemoglobin 4 g/dl, Hematocrit 16%, MCV/MCH/MCHC 62fl/15pg/25g/dL, Reticulocytes 0.5%, SI/TIBC 22/315 mg/dL, Ferritin 8.5 ng/mL, and peripheral blood smear showing severe hypochromic microcytic anemia and relative eosinofilia. Ancylostoma duodenale worm eggs were found on routine stool examination. Final diagnosis was Severe microcytic hypochromic anemia caused by an iron deficiency and Ancylostomiasis. Severe microcytic hypochromic anemia caused by iron deficiency and ancylostomiasis was established based on the patient’s history, physical examination and laboratory investigations.
Conclusions. Hookworms infect many people worldwide and cause high morbidity, mainly due to iron deficiency anemia. The highest prevalence is found in the tropics and subtropics, including Indonesia. The main clinical manifestations are abdominal pain, features of iron deficiency anemia and hypoproteinemia. Diagnosis is based on the finding of characteristic eggs in the stool. Albendazole 400 mg single dose resulted in 80% cure and a dose of 200 mg/day for 3 days gave 100% cure. Treatment of anemia is by administering ferrous sulfate or ferrous gluconate orally 200 mg three times a day and continued for up to 3 months after normal hemoglobin levels are achieved to maintain iron stores.
Efecto del confinamiento sobre el estado emocional en una muestra de habitantes panameños
Authors: Romero-Ramos Néstor , Romero-Ramos Óscar , González Suárez Arnoldo , Lobach Yulianna 
Published: January 2022

La pandemia causada por COVID-19 ha llevado a los países a tomar medidas en lo económico, político y social, para garantizar que el número de contagiados pueda ser tratado por los servicios de salud, causando diversos problemas a nivel físico y mental en la población. Esta investigación tiene como propósito conocer el estado emocional de una muestra de habitantes panameños durante los primeros meses de confinamiento obligatorio y evaluar la estructura factorial del test EVEA (escala de valoración del estado de ánimo) en el contexto panameño. Se envió el test EVEA y un cuestionario ad hoc por correo electrónico, a dos grupos de participantes (grupo 1, n = 199, 41% de hombres; grupo 2, n = 123, 41% de hombres). Se aplicaron pruebas de contraste no paramétricas, análisis factorial exploratorio, análisis de correlación bivariado y regresión jerárquica. La emoción que predomina según el test aplicado es la alegría, seguida de la ansiedad. Se obtuvo una estructura factorial de tres factores y un α de Cronbach superior a 0.8 en todas las subescalas. Se encontró una correlación negativa y significativa entre la ansiedad, tristeza e ira y la actividad física (AF); con la relajación/meditación (RM) ocurre lo mismo, pero también se correlacionó positiva y significativamente con la alegría. Después de controlar algunas variables, la AF predice la ansiedad y la tristeza. La RM, después de controlar algunas variables, predice la alegría, la ansiedad, la ira y la depresión. Aunque la emoción predominante es la alegría, se encontraron niveles altos para las subescalas de ansiedad, tristeza e ira, lo cual se atribuye a la situación de la población durante el confinamiento. La AF y la RM tienen un efecto protector sobre el estado emocional de las personas, y se sugiere la implementación de programas que fomenten dichas actividades, durante el confinamiento.
Un acercamiento a la noción de alfabetización en energía
Authors: Dixon-Pineda Manuel 
Published: January 2022

Actualmente estamos en un mundo cambiante debido al cambio climático, lo que obliga a que el uso de los recursos, incluyendo la energía, fundamental para el desarrollo humano deba ser sustentable en el tiempo. Por ende, es importante comprender cómo es el consumo de energía de las personas. En el presente artículo se analiza un concepto de la educación ambiental que puede ayudar a comprender la compleja relación entre el comportamiento humano y el uso de la energía: la alfabetización en energía. Aquí se presenta un primer acercamiento a este concepto que evalúa de dónde surge y cómo nos puede servir en el futuro, utilizando como ejemplo el caso del consumo energético en Panamá.
Study of Video Games as Alternative Teaching Media In Covid-19 Pandemic Era
Authors: Utomo Pandu R 
Published: January 2022

Technology has a direct impact on human’s behaviors and lifestyles in Covid-19 pandemic era. Various sectors such as education and economy adapted technology-based remote work and study. With the existence of remote study, the educational world will still face some issues related to the study effectiveness which requires students’ initiatives in the process. This research’s aim is to explore video game's potential as an alternative education method to solve those issues. Also, it is to study the reason why videogames are considered as a solution for remote study’s challenges during this pandemic. A study method towards related literature was used in this research. Conclusion achieved from this research is that videogames are able to stimulate students’ initiatives in exploring learning materials. Video games gave play-like learning experience and thus, reduced the stress on the students during remote study. However, the result still needs further study to achieve realistic methods that can be applied in the field.
Keywords: Game, Remote Study, Pandemic
La Multidisciplinariedad en la Ingeniería
Authors: Mujica-Sequera Ruth M. 
Published: January 2022

Los nuevos medios interactivos han creado muchos entornos educativos. Donde es llamado al método de enseñanza la " caja de herramientas ", que luego de utilizar este medio se puede obtener los objetivos que tenemos dentro de las limitaciones de un entorno determinado.
High-contrast Imaging with Fizeau Interferometry: the Case of Altair*
Authors: Spalding E. , Morzinski K. M. , Hinz P. , Males J. , Meyer M. , Quanz S. P. , Leisenring J. , Power J. 
Published: January 2022

Abstract
The Large Binocular Telescope (LBT) has two 8.4 m primary mirrors that produce beams that can be combined coherently in a “Fizeau” interferometric mode. In principle, the Fizeau point-spread function (PSF) enables the probing of structure at a resolution up to three times better than that of the adaptive-optics-corrected PSF of a single 8.4 m telescope. In this work, we examined the nearby star Altair (5.13 pc, type A7V, hundreds of Myr to ≈1.4 Gyr) in the Fizeau mode with the LBT at Brα (4.05 μm) and carried out angular differential imaging to search for companions. This work presents the first filled-aperture LBT Fizeau science data set to benefit from a correcting mirror that provides active phase control. In the analysis of the λ/D angular regime, the sensitivity of the data set is down to ≈0.5 M
⊙ at 1″ for a 1.0 Gyr system. This sensitivity remains limited by the small amount of integration time, which is in turn limited by the instability of the Fizeau PSF. However, in the Fizeau fringe regime we attain sensitivities of Δm ≈ 5 at 0.″2 and put constraints on companions of 1.3 M
⊙ down to an inner angle of ≈0.″15, closer than any previously published direct imaging of Altair. This analysis is a pathfinder for future data sets of this type, and represents some of the first steps to unlocking the potential of the first Extremely Large Telescope. Fizeau observations will be able to reach dimmer targets with upgrades to the instrument, in particular the phase detector.
CHILES. VII. Deep Imaging for the CHILES Project, an SKA Prototype
Authors: Dodson R. , Momjian E. , Pisano D. J. , Luber N. , Blue Bird J. , Rozgonyi K. , Smith E. T. , van Gorkom J. H. , Lucero D. , Hess K. M. , Yun M. , Rhee J. , van der Hulst J. M. , Vinsen K. , Meyer M. , Fernandez X. , Gim H. B. , Popping A. , Wilcots E. 
Published: January 2022

Abstract
Radio astronomy is undergoing a renaissance, as the next generation of instruments provides a massive leap forward in collecting area and therefore raw sensitivity. However, to achieve this theoretical level of sensitivity in the science data products, we need to address the much more pernicious systematic effects, which are the true limitation. These become all the more significant when we consider that much of the time used by survey instruments, such as the Square Kilometre Array (SKA), will be dedicated to deep surveys. CHILES is a deep H i survey of the COSMOS field, with 1000 hr of Very Large Array time. We present our approach for creating the image cubes from the first epoch, with discussions of the methods and quantification of the data quality from 946 to 1420 MHz—a redshift range of 0.5−0. We lay out the problems we had to solve and describe how we tackled them. These are important because CHILES is the first deep wide-band multiepoch H i survey and has relevance for ongoing and future surveys. We focus on the accumulated systematic errors in the imaging, as the goal is to deliver a high-fidelity image that is only limited by the random thermal errors. To understand and correct these systematic effects, we ideally manage them in the domain in which they arise, and that is predominately the visibility domain. CHILES is a perfect test bed for many of the issues we can expect for deep imaging with the SKA or ngVLA, and we discuss the lessons we have learned.
The Structure of Multiphase Galactic Winds
Authors: Fielding Drummond B. , Bryan Greg L. 
Published: January 2022

Abstract
We present a novel analytic framework to model the steady-state structure of multiphase galactic winds comprised of a hot, volume-filling component and a cold, clumpy component. We first derive general expressions for the structure of the hot phase for arbitrary mass, momentum, and energy source terms. Next, informed by recent simulations, we parameterize the cloud–wind mass transfer rates, which are set by the competition between turbulent mixing and radiative cooling. This enables us to cast the cloud–wind interaction as a source term for the hot phase and thereby simultaneously solve for the evolution of both phases, fully accounting for their bidirectional influence. With this model, we explore the nature of galactic winds over a broad range of conditions. We find that (i) with realistic parameter choices, we naturally produce a hot, low-density wind that transports energy while entraining a significant flux of cold clouds, (ii) mixing dominates the cold cloud acceleration and decelerates the hot wind, (iii) during mixing thermalization of relative kinetic energy provides significant heating, (iv) systems with low hot phase mass loading factors and/or star formation rates can sustain higher initial cold phase mass loading factors, but the clouds are quickly shredded, and (v) systems with large hot phase mass loading factors and/or high star formation rates cannot sustain large initial cold phase mass loading factors, but the clouds tend to grow with distance from the galaxy. Our results highlight the necessity of accounting for the multiphase structure of galactic winds, both physically and observationally, and have important implications for feedback in galactic systems.
Rebounding Cores to Build Star Cluster Multiple Populations
Authors: Parmentier G. , Pasquali A. 
Published: January 2022

Abstract
We present a novel approach to the riddle of star cluster multiple populations. Stars form from molecular cores. But not all cores form stars. Following their initial compression, such “failed” cores re-expand, rather than collapsing. We propose that their formation and subsequent dispersal regulate the gas density of cluster-forming clumps and, therefore, their core and star formation rates. Clumps for which failed cores are the dominant core type experience star formation histories with peaks and troughs (i.e., discrete star formation episodes). In contrast, too few failed cores results in smoothly decreasing star formation rates. We identify three main parameters shaping the star formation history of a clump: the star and core formation efficiencies per free-fall time, and the timescale on which failed cores return to the clump gas. The clump mass acts as a scaling factor. We use our model to constrain the density and mass of the Orion Nebula Cluster progenitor clump, and to caution that the star formation histories of starburst clusters may contain close-by peaks concealed by stellar age uncertainties. Our model generates a great variety of star formation histories. Intriguingly, the chromosome maps and O–Na anticorrelations of old globular clusters also present diverse morphologies. This prompts us to discuss our model in the context of globular cluster multiple stellar populations. More massive globular clusters exhibit stronger multiple stellar population patterns, which our model can explain if the formation of the polluting stars requires a given stellar mass threshold.
Evolutionary and Observational Consequences of Dyson Sphere Feedback
Authors: Huston Macy , Wright Jason 
Published: January 2022

Abstract
The search for signs of extraterrestrial technology, or technosignatures, includes the search for objects which collect starlight for some technological use, such as those composing a Dyson sphere. These searches typically account for a star’s light and some blackbody temperature for the surrounding structure. However, such a structure inevitably returns some light back to the surface of its star, either from direct reflection or thermal reemission. In this work, we explore how this feedback may affect the structure and evolution of stars, and when such feedback may affect observations. We find that in general this returned light can cause stars to expand and cool. Our MESA models show that this energy is only transported toward a star’s core effectively by convection, so low-mass stars are strongly affected, while higher-mass stars with radiative exteriors are not. Ultimately, the effect only has significant observational consequences for spheres with very high temperatures (much higher than the often assumed ∼300 K) and/or high specular reflectivity. Lastly, we produce color–magnitude diagrams of combined star–Dyson sphere systems for a wide array of possible configurations.
COLDz: Probing Cosmic Star Formation With Radio Free–Free Emission
Authors: Algera Hiddo S. B. , Hodge Jacqueline A. , Riechers Dominik A. , Leslie Sarah K. , Smail Ian , Aravena Manuel , Cunha Elisabete da , Daddi Emanuele , Decarli Roberto , Dickinson Mark , Gim Hansung B. , Guaita Lucia , Magnelli Benjamin , Murphy Eric J. , Pavesi Riccardo , Sargent Mark T. , Sharon Chelsea E. , Wagg Jeff , Walter Fabian , Yun Min 
Published: January 2022

Abstract
Radio free–free emission is considered to be one of the most reliable tracers of star formation in galaxies. However, as it constitutes the faintest part of the radio spectrum—being roughly an order of magnitude less luminous than radio synchrotron emission at the GHz frequencies typically targeted in radio surveys—the usage of free–free emission as a star formation rate tracer has mostly remained limited to the local universe. Here, we perform a multifrequency radio stacking analysis using deep Karl G. Jansky Very Large Array observations at 1.4, 3, 5, 10, and 34 GHz in the COSMOS and GOODS-North fields to probe free–free emission in typical galaxies at the peak of cosmic star formation. We find that z ∼ 0.5–3 star-forming galaxies exhibit radio emission at rest-frame frequencies of ∼65–90 GHz that is ∼1.5–2 times fainter than would be expected from a simple combination of free–free and synchrotron emission, as in the prototypical starburst galaxy M82. We interpret this as a deficit in high-frequency synchrotron emission, while the level of free–free emission is as expected from M82. We additionally provide the first constraints on the cosmic star formation history using free–free emission at 0.5 ≲ z ≲ 3, which are in good agreement with more established tracers at high redshift. In the future, deep multifrequency radio surveys will be crucial in order to accurately determine the shape of the radio spectrum of faint star-forming galaxies, and to further establish radio free–free emission as a tracer of high-redshift star formation.