bluuebunny/crossref_metadata_2025_split huggingface dataset:
Kegiatan Imunisasi Sub Pin Polio Putaran 1 Dalam Rangka Pencegahan Penyakit Polio Di Wilayah Kerja Puskesmas Kota Selatan Kota Kediri
Authors: Puspitasari Betristasia , Darmayanti Rofik , Yunarsih Yunarsih , Santoso Puguh , Sucipto Sucipto , Kristanto Heny , Krisnawati Dyah Ika 
Published: August 2024

Polio adalah penyakit yang disebabkan oleh virus polio dan dapat menyebabkan kelumpuhan. Polio sebenarnya bisa menyerang siapa saja, tapi lebih rentan menyerang anak-anak, terutama usia di bawah 5 tahun. Tujuan Kegiatan Sub PIN polio adalah sebagai pencegahan terjadinya kasus polio. Kegiatan Pengabdian Masyarakat ini dilakukan dengan metode memberikan secara langsung imunisasi Polio kepada anak usia 0-7 tahun. Setelah diberikan imunisasi, setiap anak diberikan tanda tinta pada jari dan kartu imunisasi. Pada orangtua dipesan agar mengikuti kegiatan PIN kedua dengan jarak satu bulan. Dari hasil kegiatan pekan imunisasi Sub PIN Polio Putaran 1 di Puskesmas Kota Selatan Kota Kediri dinyatakan berhasil dengan capaian sebanyak 3470 (98,2%). Masyarakat khususnya orangtua yang mempunyai anak usia 0-7 tahun sangat antusias dalam kegiatan ini, terbukti dengan kehadiran masyarakat yang memenuhi undangan untuk imunisasi. Diharapkan untuk putaran ke 2 antusiasme masyarakat meningkat sehingga berhasil mencapai cakupan 100%.
Perancangan Sistem Isnformasi Manajemen Masjid Jami Al-Fath Berbasis Web
Authors: Setiawan Imam Imam 
Published: August 2024

Masjid merupakan salah satu tempat beribadah umat islam. Di era modern saat ini masjid mengalami perkembangan yang sangat pesat, baik dalam bentuk teknologi maupun informasi. Tetapi perkembangan sistem informasi pada masjid masih belum maksimal, perlunya inovasi yang sesuai dengan perkembang teknologi yang ada untuk memajukan masjid dengan memberikan pembaharuan dalam menajemen sistem masjid. Masjid jami al-fath merupakan salah satu masjid yang beralamat di Jalan Tengku Amir Hamzah, Kelurahan, Jati Karya, Kecamatan, Binjai Utara. Masjid jami al-fath sering sekali mengadakan kegiatan-kegiatan seperti peringatan hari besar islam, dakwah, serta pengajian remaja dan lainnya. Masjid jami al-fath dalam mengelolah informasi kegiatan-kegiatan tersebut masih belum mengunakan sistem informasi berbasis web dalam menyampaikan informasi.
PANORAMA DE CRIANÇAS DIAGNOSTICADAS COM INSUFICIÊNCIA CARDÍACA
Authors: Sanches Emanuella Tannure , Justa Jose William Oliveira Dos Santos , Pacheco Natália Gonçalves , Pinheiro Geanderson Victor Ferreira , Gomes Anna Karynna Barbosa , Nóbrega Francisco Ricardo Resende da , Silva Alyne Leitão , Carvalho Lívia Rodrigues , Rocha Mariana da Costa , Magalhães Leyliane Diógenes , Barbosa Bianca Santana , Silva Camila Meury Albino da , Barros Vitória Sousa 
Published: August 2024

O presente artigo tem como objetivo principal analisar o panorama epidemiológico de crianças acometidas por insuficiência cardíaca. Estudo descritivo, ecológico, através de dados obtidos pelo Departamento de Informática do Sistema Único de Saúde (DATASUS), por meio da plataforma Sistema de Informações Hospitalares (SIH). Foram analisados dados de crianças internadas com diagnóstico de insuficiência cardíaca o recorte temporal de 2018 a 2022, no Brasil, foram analisados variaveis de ano de atendimento, faixa etaria, região e sexo. Houve uma prevalência no ano de 2019, na região Nordeste, menores de 1 ano e crianças do sexo masculino. Diante do exposto, fica evidente que os números de hospitalizações de crianças com diagnóstico de insuficiência cardíaca ainda são alarmantes. Dessa forma, concluiu-se que estratégias públicas de incentivo à saúde e prevenção primária são essenciais para diminuir a frequência da enfermidade e, consequentemente, a necessidade de hospitalização de infantes com IC.
EVALUASI EROSI TANAH BERVEGETASI DENGAN ALAT RAINFALL SIMULATOR (TES EKSPERIMENTAL DI LABORATORIUM)
Authors: Azzahra Iftasya Shafa , Romdania Yuda , Herison Ahmad , Tugiono Subuh , Murda Gung Bagus J 
Published: August 2024

Hujan adalah bagian dari siklus hidrologi yang paling berbahaya karena dapat menyebabkan erosi. Penelitian di Kebun Kolektif TP PKK Kota Bandar Lampung mengindikasikan kekurangan unsur hara akibat erosi yang disebabkan oleh limpasan air hujan, ditambah dengan kondisi lahan yang cukup curam. Tujuan penelitian adalah menganalisis pengaruh variasi kemiringan dan intensitas curah hujan terhadap laju erosi serta upaya pengendaliannya. Metode yang digunakan pada penelitian ini adalah rainfall simulator. Hasil dari penelitian adalah laju erosi terkecil terjadi pada intensitas curah hujan 0,75 liter/menit dan kemiringan lereng 8% terjadi sebesar 0,04 Ton/Ha sedangkan laju erosi paling besar terjadi yaitu pada intensitas curah hujan 1,75 liter/menit dan kemiringan lereng 45% terjadi sebesar 0,59 Ton/Ha, terlihat bahwa intensitas curah hujan dan kemiringan lereng mempunyai pengaruh signifikan terhadap laju erosi tanah, laju erosi semakin meningkat seiring dengan kedua faktor tersebut. Kesimpulannya adalah curah hujan dengan intensitas tinggi dan kemiringan lereng yang curam meningkatkan laju erosi yang dapat merusak struktur tanah, sehingga perlu dilakukan teknik konservasi untuk mengurangi laju erosi dan menjaga kesuburan tanah, seperti pemeliharaan vegetasi penutup tanah dan penyuluhan teknik konservasi tanah bagi petani dan masyarakat.
Kata kunci: Siklus Hidrologi, Vegetasi, Limpasan, Curah Hujan, Kemiringan Lereng
EVALUASI BANGUNAN PENGAMAN LERENG SUNGAI CILIWUNG RUAS KALIBATA DENGAN MENGGUNAKAN ANALISIS BERDASARKAN LOAD RESISTANCE FACTOR DESIGN
Authors: Harjanto Furqaan , Adi Agus Darmawan , Hardiyatmo Hary Christady 
Published: August 2024

ABSTRAK
Dinding penahan tanah merupakan struktur yang biasa digunakan untuk menahan tanah dengan kemiringan lereng yang lebih curam melebihi yang dapat ditahan oleh tanah itu sendiri. Metode tersebut diterapkan pada lereng Sungai Ciliwung Ruas Kalibata yang menggunakan dinding penahan tanah tipe non gravitasi. Namun konstruksi tersebut mengalami longsor saat terjadi banjir, sehingga penelitian ini memiliki tujuan untuk mengetahui jenis konstruksi penahan tanah yang dapat digunakan, serta stabilitas masing – masing jenis konstruksi penahan tanah. Analisis dilakukan pada potongan dengan kode P.07 menggunakan data tanah berupa hasil bor dengan kode BH-24, dan data laboratorium hasil pengujian dari bor tersebut pada tiga kedalaman sampel yang berbeda. Analisis menggunakan metode Load Resistance Factor Design dengan bantuan software GEO5. Hasil analisis pada semua kombinasi beban menunjukkan jenis dinding penahan tanah tipe semi gravitasi kantilever tidak dapat digunakan karena tidak memenuhi stabilitas geser, eksentrisitas dan daya dukung pada semua kombinasi beban. Untuk jenis non gravitasi kantilever tidak memenuhi terhadap kombinasi Layan 1 dikarenakan nilai perpindahan horizontal yang besar, sehingga digunakan perkuatan angkur. Pada kombinasi Kuat 1 dengan angkur, memberikan hasil kedalaman penetrasi sebesar 18.4 meter dengan angkur dipasang pada kedalaman 2.5 meter dari permukaan, dan perpindahan horizontal sebesar 2.7 centimeter
PENGARUH PENAMBAHAN SILICA FUME TERHADAP CAMPURAN BETON MEMADAT SENDIRI (SELF COMPACTING CONCRETE) MUTU TINGGI
Authors: Sundariyati Nadya Putri Astika Ningrum , Pranowo Dadang Dwi , Wari Wahyu Naris , Utanaka Ahmad , Khomari Mohammad Galuh 
Published: August 2024

Self Compacting Concrete (SCC) adalah jenis beton yang memiliki kemampuan untuk mengalir dan memadat sendiri tanpa menggunakan bantuan vibrator. Beton SCC memerlukan pengaturan agregat, proporsi agregat, dan zat admixture superplastiziser agar didapatkan kekentalan yang sesuai tanpa menggunakan bantuan vibrator. Pada kebanyakan kasus bahan pokok campuran beton meliputi agregat kasar, agregat halus, semen, dan air. Namun, dalam beberapa situasi tertentu, sifat campuran beton dapat dipengaruhi oleh admixture dan bahan tambah lainnya, seperti superplasticizer dan bahan tambah lainnya silica fume. Dalam penelitian ini, silica fume digunakan sebagai bahan tambah pada beton SCC yang bertujuan untuk mengetahui pengaruh kuat tekan silica fume terhadap campuran beton SCC. Penelitian ini dilakukan dengan menambah silica fume dengan persentase 0%, 5%, dan 10% dari berat semen serta superplasticizer dengan persentase 0.5% dari berat semen. Metode rancangan campuran menggunakan metode ACI (American Concrete Institute) dengan kuat tekan rencana 41 MPa diuji kuat tekan pada umur 7, 14, dan 28 hari. Hasil menunjukkan bahwa kuat tekan dengan variasi beton normal memiliki kuat tekan rata – rata 39.90 MPa pada umur 28 hari. Tetapi, nilai kuat tekan dengan variasi silica fume 5% mengalami penurunan yang signifikan mencapai 30,72 MPa pada umur 28 hari. Nilai kuat tekan dengan variasi silica fume 10% lebih tinggi dibandingkan dengan variasi sebelumnya, rata – rata 36,185 MPa. Hal ini menunjukkan bahwa penambahan silica fume terhadap beton Self Compacting Concrete dapat menyebabkan nilai kuat tekan beton menurun.
Relasi Fungsi, Bentuk dan Material Pada Arsitektur Rumah Baja Karya Ahmad Djuhara
Authors: Wibowo Danang Harito 
Published: August 2024

ABSTRACT
Steel house by Ir. This Ahmad Djuhara I.A.I, comes with a prominent metal material dominance. In addition to being used in the main structure and the main outer enclosure, all these materials are displayed in a straightforward and naked manner. Making the expression of this building really unusual. Perhaps because of this, as far as is known, since 2002 it has received the most and widest coverage from the media (print, television and online) than any other architect's works. This steel house received an award from the Indonesian Architects Association (IAI Award), such as confirming the existence and presence of this unique steel house. This study aims to examine how the relationship aspects of Form, Function & Material. The method used is qualitative - descriptive. Through the study of the anatomy of the building, then data collection by means of field observations, direct interviews with users. Then, to fulfill its objectivity, interviews were also conducted on 15 residents (chosen randomly) who live around the location (radius not more than 600 m). The results of the study show that the relationship from triangulation aspects of Form, Function and Material does not work as expected, especially regarding materials. This research is expected to be useful for architectural science, practitioners and students. So that in its design, it is necessary to be more careful in determining the dominance of the material.
Key word : Relation, Form, Function, Material, Building Anatomy and Steel house.
Importancia de las Habilidades Emocionales en el Proceso de Enseñanza Aprendizaje en Niños y Adolescentes
Authors: Bauz Ruano Andrea Carolina , Pupiales Mariño Andrea Valeria , Rodríguez Pulupa Cristian Eduardo , Quinata Encarnación Lourdes del Rocío , Catagña Alquinga Bryan Sthevven 
Published: August 2024

La importancia de las habilidades emocionales en el proceso de enseñanza-aprendizaje en niños y adolescentes es fundamental para el desarrollo integral de los estudiantes. Este estudio tiene como objetivo analizar el impacto del desarrollo de habilidades emocionales en el rendimiento académico y bienestar general de los estudiantes. Para alcanzar este objetivo, se utilizó un enfoque metodológico cualitativo y descriptivo, realizando una revisión sistemática de literatura científica y académica siguiendo las directrices del PRISMA-SCR. Los principales hallazgos revelan que los programas que fomentan habilidades emocionales tienen un impacto positivo significativo en la capacidad de los estudiantes para enfrentar desafíos académicos y regular sus emociones. Además, se destacó la importancia de un enfoque emocional en la educación para mejorar el desempeño tanto de estudiantes como de docentes. Se concluye que desarrollar habilidades emocionales desde una edad temprana promueve la resiliencia y mejora la capacidad para manejar el estrés y las presiones académicas.
The Use of Short Stories to Improve Vocabulary: Understanding the Perceptions of EFL Students
Authors: García-Cañarte Alan , Ocaña Mauro 
Published: August 2024

The integration of technologies, such as virtual learning environments, web-based collaborative setups, and gamified applications, tend to promote the positive effects of short stories on vocabulary learning in a foreign language. This study investigates the effectiveness of using short stories as a pedagogical tool for enhancing vocabulary acquisition in English as a Foreign Language (EFL) students. Two cohorts of participants took part simultaneously in a course to improve vocabulary through short stories graded according to their level of proficiency. The highly validated tool MSLQ was applied to gather perceptions of motivation and learning strategies throughout the course. Correlational analyses suggest that short stories, combined with appropriate technological and pedagogical strategies, offer a powerful approach to vocabulary learning in diverse educational contexts. The study also emphasizes the importance of self-regulated learning mechanisms, which promote learner autonomy and self-efficacy, leading to better vocabulary outcomes. This research contributes to the understanding of effective vocabulary learning and provides practical insights for educators seeking to enhance EFL students' language mastery.
Resonant and Ultra-short-period Planet Systems Are at Opposite Ends of the Exoplanet Age Distribution
Authors: Schmidt Stephen P. , Schlaufman Kevin C. , Hamer Jacob H. 
Published: August 2024

Abstract
Exoplanet systems are thought to evolve on secular timescales over billions of years. This evolution is impossible to directly observe on human timescales in most individual systems. While the availability of accurate and precise age inferences for individual exoplanet host stars with ages τ in the interval 1 Gyr ≲ τ ≲ 10 Gyr would constrain this evolution, accurate and precise age inferences are difficult to obtain for isolated field dwarfs like the host stars of most exoplanets. The Galactic velocity dispersion of a thin-disk stellar population monotonically grows with time, and the relationship between age and velocity dispersion in a given Galactic location can be calibrated by a stellar population for which accurate and precise age inferences are possible. Using a sample of subgiants with precise age inferences, we calibrate the age–velocity dispersion relation in the Kepler field. Applying this relation to the Kepler field’s planet populations, we find that Kepler-discovered systems plausibly in second-order mean-motion resonances have 1 Gyr ≲ τ ≲ 2 Gyr. The same is true for systems plausibly in first-order mean-motion resonances, but only for systems likely affected by tidal dissipation inside their innermost planets. These observations suggest that many planetary systems diffuse away from initially resonant configurations on secular timescales. Our calibrated relation also indicates that ultra-short-period (USP) planet systems have typical ages in the interval 5 Gyr ≲ τ ≲ 6 Gyr. We propose that USP planets tidally migrated from initial periods in the range 1 day ≲ P ≲ 2 days to their observed locations at P < 1 day over billions of years and trillions of cycles of secular eccentricity excitation and inside-planet damping.
The Potential for Organic Synthesis in the Ocean of Enceladus
Authors: Liu Can , Xu Weiming , Zhang Zongbin , Robinson Kirt , Lau Maggie , Huang 黄 Fang 放 , Huang 黄 Fang 方 , Glein Christopher R. , Hao Jihua 
Published: August 2024

Abstract
The Cassini spacecraft detected a soup of organics in the plume of Saturn’s moon Enceladus. Those compounds could provide building blocks for the potential emergence or sustenance of microbial life in Enceladus’ subsurface ocean. However, the sources and stabilities of organics in Enceladus’ ocean are still poorly understood. Here, we perform nonequilibrium thermodynamic calculations to assess the energetics of abiotic synthesis for a broad spectrum of small organic molecules under both cold oceanic and hydrothermal conditions on Enceladus. Most of the organics that we studied are thermodynamically favorable to synthesize at micromolal dissolved concentrations over wide ranges of pH (8.5–11) and redox conditions. This suggests that many of the organic compounds detected by Cassini may be derived from reactions of CO2 and H2. However, some widely assumed precursors of biomolecules, such as formaldehyde, hydrogen cyanide, and acetylene, are found to be unstable and therefore unfavorable to be synthesized. We found that higher temperatures also seem to favor the synthesis of organic species under Enceladus hydrothermal conditions. Detection of thermodynamically unstable species in the plume might reflect artifacts introduced during high-speed spacecraft flybys and/or active synthesis via degradation of primordial chondritic organics, or biological activities.
Modeling Blazar Broadband Emission with Convolutional Neural Networks. II. External Compton Model
Authors: Sahakyan N. , Bégué D. , Casotto A. , Dereli-Bégué H. , Giommi P. , Gasparyan S. , Vardanyan V. , Khachatryan M. , Pe’er A. 
Published: August 2024

Abstract
In the context of modeling spectral energy distributions (SEDs) for blazars, we extend the method that uses a convolutional neural network (CNN) to include external inverse Compton processes. The model assumes that relativistic electrons within the emitting region can interact with and up-scatter external photons originating from the accretion disk, the broad-line region, and the torus, to produce the observed high-energy emission. We trained the CNN on a numerical model that accounts for the injection of electrons, their self-consistent cooling, and pair creation-annihilation processes, considering both internal and all external photon fields. Despite the larger number of parameters compared to the synchrotron self-Compton model and the greater diversity in spectral shapes, the CNN enables an accurate computation of the SED for a specified set of parameters. The performance of the CNN is demonstrated by fitting the SED of two flat-spectrum radio quasars, namely 3C 454.3 and CTA 102, and obtaining their parameter posterior distributions. For the first source, the available data in the low-energy band allowed us to constrain the minimum Lorentz factor of the electrons,

γ

min

, while for the second source, due to the lack of these data,

γ

min

=

10

2

was set. We used the obtained parameters to investigate the energetics of the system. The model developed here, along with one from Bégué et al., enables self-consistent, in-depth modeling of blazar broadband emissions within a leptonic scenario.
Effects of Halo Spin on the Formation and Evolution of Bars in Disk Galaxies
Authors: Jang Dajeong , Kim Woong-Tae 
Published: August 2024

Abstract
The spin of dark halos has been shown to significantly affect bar formation and evolution in disk galaxies. To understand the physical role of halo spin in bar formation, we run N-body simulations of isolated, Milky Way–sized galaxies by varying the halo spin parameter in the range −0.16 ≤ λ ≤ 0.16 and the bulge mass. We find that our adopted halo alone is subject to swing amplification of an m = 2 nonaxisymmetric mode rotating in the same sense as the halo, which assists or inhibits the bar formation in a disk depending on its sense of rotation. The m = 2 mode in the disk, growing via swing amplification, interacts constructively (destructively) with the m = 2 mode in the prograde (retrograde) halo, promoting (delaying) bar formation. A bar grows by losing its angular momentum primarily to a halo. Since the halo particles inside (outside) the corotation resonance with the bar can emit (absorb) angular momentum to (from) the bar, the bar pattern speed decays more slowly for larger λ > 0, while it decreases relatively fast almost independent of λ ≤ 0. Models with a strong bar develop a boxy peanut-shaped bulge. In models without a bulge, this occurs rapidly via buckling instability, while bars with a bulge thicken gradually without undergoing buckling instability. Among the models considered in the present work, the bar in the λ = 0.06 model with a bulge of 10% of the disk mass best describes the Milky Way in terms of its length and pattern speed.
Cold Water Emission Cannot Be Used to Infer Depletion of Bulk Elemental Oxygen [O/H] in Disks
Authors: Ruaud Maxime , Gorti Uma 
Published: August 2024

Abstract
We reexamine the constraints provided by Herschel Space Observatory data regarding cold water emission from protoplanetary disks. Previous disk models that were used to interpret observed water emission concluded that oxygen (O/H) is depleted by at least 2 orders of magnitude if a standard, interstellar gas/dust mass ratio is assumed in the disk. In this work, we use model results from a recent disk parameter survey and show that most of the Herschel constraints obtained for cold water (i.e., for transitions with an upper energy level E
up < 200 K, where the bulk of the disk water lies) can be explained with disk models adopting interstellar medium-like oxygen elemental abundance (i.e., O/H = 3.2 × 10−4) and the canonical gas/dust mass ratio of 100. We show that cold water vapor is mainly formed by photodesorption of water ice at the interface between the molecular layer and the midplane, and that its emission is relatively independent of the main disk properties like the disk gas mass and gas/dust mass ratio. We find that the abundance of water vapor in the outer disk is set by photoprocesses and depends on the (constant) vertical column density of water ice needed to attenuate the far-ultraviolet photon flux, resulting in roughly constant emission for the parameters (gas mass, dust mass, disk radius) varied in our survey. Importantly, water line emission is found to be optically thick and hence sensitive to temperature more than abundance, possibly driving previous inferences of large-scale oxygen depletion.
Late-time Radio Flares in Tidal Disruption Events
Authors: Matsumoto Tatsuya , Piran Tsvi 
Published: August 2024

Abstract
Radio monitoring unveiled late (hundreds to a thousand days) radio flares in a significant fraction of tidal disruption events. We propose that these late-time radio flares are a natural outcome if the surrounding density profile flattens outside the Bondi radius. At the Bondi radius, the outflow is optically thin (above a few GHz) to synchrotron self-absorption. As more and more material is swept up, the radio emission rises asymptotically as ∝ t
3 until the outflow begins to decelerate. A detection of such a rise and a late-time maximum constrains the black hole mass and the mass and energy of the radio-emitting outflow. We show that this model can give reasonable fits to some observed light curves, leading to reasonable estimates of the black hole and outflow masses. We also find that the slope of the density profile within the Bondi radius determines whether an early-time (∼102 days) radio peak exists.