bluuebunny/crossref_metadata_2025_split huggingface dataset:
Distractor similarity and category variability effects in search
Authors: Robbins Arryn , Evdokimov Anatolii 
Published: July 2024

AbstractCategorical search involves looking for objects based on category information from long-term memory. Previous research has shown that search efficiency in categorical search is influenced by target/distractor similarity and category variability (i.e., heterogeneity). However, the interaction between these factors and their impact on different subprocesses of search remains unclear. This study examined the effects of target/distractor similarity and category variability on processes of categorical search. Using multidimensional scaling, we manipulated target/distractor similarity and measured category variability for target categories that participants searched for. Eye-tracking data were collected to examine attentional guidance and target verification. The results demonstrated that the effect of category variability on response times (RTs) was dependent on the level of target/distractor similarity. Specifically, when distractors were highly similar to target categories, there was a negative relation between RTs and variability, with low variability categories producing longer RTs than higher variability categories. Surprisingly, this trend was only present in the eye-tracking measures of target verification but not attentional guidance. Our results suggest that searchers more effectively guide attention to low-variability categories compared to high-variability categories, regardless of the degree of similarity between targets and distractors. However, low category variability interferes with target match decisions when distractors are highly similar to the category, thus the advantage that low category variability provides to searchers is not equal across processes of search.
Halk Oyunları Çalışmalarının Ritim Yeteneği ve Çeviklik Üzerine Etkisi
Authors: Taşkın Ali Kemal 
Published: July 2024

Bu kitap, halk oyunları çalışmalarının ritim yeteneği ve çeviklik üzerine etkisini ele almaktadır. Yazar, halk oyunlarının tanımını, doğuşunu ve genel niteliklerini açıklamaktadır. Ayrıca, Türkiye'deki halk oyunlarının gelişimini ve çeşitlerini de incelenmektedir. Halk oyunlarına teşvik edici faktörler, boş zaman, kitle iletişim araçlarının etkinliği, aile, kıyafet, müzik ve yöresel özellikler, okul ve eğitim gibi konular da ele alınmaktadır. Kitapta ayrıca halk oyunlarının işlevleri, iletişim, sosyalleşme, sağlık ve spor üzerindeki etkileri de tartışılmaktadır. Bu çalışma, halk oyunlarının ritim yeteneği ve çeviklik üzerindeki olumlu etkilerini vurgulamaktadır.

This book examines the impact of folk dance studies on rhythm and agility. The author explains the definition, origin, and general characteristics of folk dances. Additionally, the development and varieties of folk dances in Turkey are also examined. Factors that encourage folk dances, such as leisure time, the effectiveness of mass media, family, clothing, music, regional characteristics, school, and education, are also discussed. The book also discusses the functions of folk dances and their effects on communication, socialization, health, and sports. This study emphasizes the positive effects of folk dances on rhythm and agility.
The Values of Islamic Education in the Traditional Wedding Ceremony of the Karo Tribe
Authors: Barus Ari Pramaji , Budianti Yusnaili , Arsyad Junaidi 
Published: July 2024

This study aims to analyze what processions are relevant to Islamic education's values and the values of Islamic education in traditional ceremonies of the Karo tribe in Aji Baho Village, Biru-Biru District, Deli Serdang Regency. This research is qualitative with a phenomenological approach. The source of the data used is primary data collected directly by researchers, namely data obtained from informants, namely the Head of Aibaho Village, Community Leaders of Ajibaho Village, Several People of Ajibaho Village, Biru-Biru District, Deli Serdang Regency. The secondary data are village archives, records of observations, and several other documents related to research in Ajibaho village, Biru-Biru District, Deli Serdang Regency. The results of the study were. First, the procession was divided into 2, namely pre-marriage (the stage of nungkuni kata, ngembah belo selembar, nganting manuk) and the wedding procession (process rose, reconnaissance pedah-pedah / luah, prayer congratulations, traditional work perjabun singuda, belo selembar, man bersama and man sepiring) and second, the value of education in ceremonies that contain the value of tawhid, worship, morals, ukhuwah. According to the researchers' analysis, the procession and the value of education at the ceremony contain prayers, hopes for happiness, health, cheap sustenance, active effort, and obedience to worship. The value of Islamic education in the Karo tribal wedding ceremony can be seen in two processes: the premarital and when the wedding occurs.
Resultados de la Aplicación de un Programa de Ejercicio en Trabajadores de una Institución de Educación Superior
Authors: Díaz-Cevallos MsC. Ana Cristina , Obando Mazón Dra. Luz Alexandra , Pozo Pozo Dra. Lidia Tatiana , Hermoza Ruiz Dr. Harold Hernando 
Published: July 2024

El presente estudio se realizó por 6 en los meses, a 40 personas de 30 a 58 años de edad, en la ciudad de Quito, con los objetivo de promover la práctica de ejercicio físico en trabajadores sedentarios, y también determinar la modificación de peso corporal y peso graso después de la aplicación de una rutina de entrenamiento físico durante tres veces a la semana. La investigación ejecutada fue de tipo aplicativa, prospectiva y longitudinal. El estudio consistió en realizar mediciones antropométricas antes de la aplicación de la rutina de ejercicio físico, para comparar los resultados iniciales y los finales en cuanto a peso corporal, y peso grasa. Se concluyó que si existe un cambio significativamente estadístico p<0.05 en el peso corporal y en el peso graso, al finalizar la rutina de entrenamiento físico.
Pemberdayaan Siswa Sekolah Dasar Dalam Pelatihan Dan Edukasi Apoteker Cilik Dalam Rangka Pencapaian Desa Peduli Kesehatan Di Kecamatan Pagimana
Authors: Abdulkadir Widy Susanti , Akuba Juliyanty 
Published: July 2024

Apoteker merupakan tenaga kesehatan yang memiliki keahlian di bidang obat-obatan. Banyaknya masyarakat yang belum mengenal profesi apoteker. Melalui apoteker cilik ini kita berusaha untuk mengenalkan profesi apoteker sebagai salah satuvtenaga kesehatan yang memiliki keahlian dibidang penggunaan obat kepada masyarakat. Penting untuk bisa memberikan pengenalan terhadap dunia kesehatan pada anak-anak sejak mereka kecil, salah satunya melalui program apoteker cilik. Saat ini, pemberdayaan program pendidikan kesehatan serta pelayanan kesehatan di usia dini terutama di level sekolah dasar (SD) telah mulai berkembang. Tujuan kegiatan pengabdian kepada masyarakat ini adalah memperkenalkan profesi apoteker sebagai salah satu tenaga kesehatan dan sumber informasi obat serta memberikan pelatihan keterampilan dan edukasi tentang penggunaan obat yang tepat Pelaksanaan pengabdian kepada masyarakat di Sekolah Dasar desa Taloyon dan desa Sepa Kecamatan Pagimana.Pengenalan kepada anak usia dini dalam memperkenalkan profesi Apoteker kepada siswa SD dapat meningkatkan pengetahuan masyarakat atas profesi Apoteker, serta memperkenalkan istilah Apoteker Cilik akan meningkatkan popularitas profesi Apoteker. Edukasi obat kepada anak usia dini harus terus ditingkatkan supaya membawa perubahan mindset mengenai pengetahuan dan kesadaran tentang penggunaan obat secara tepat.
Peningkatkan Pembangunan Desa Melalui Program KKN Tematik Dalam Membangun Desa Bina Jaya, Kecamatan Tolangohula
Authors: Latief Mukhlisulfatih , Olii Salahuddin , Suleman Adriansyah R 
Published: July 2024

Program yang dibuat oleh mahasiswa KKN Universitas Negeri Gorontalo ditargetkan kepada masyarakat yang ada di Desa Bina Jaya Kecamatan Tolangohula Kabupaten Gorontalo, yang bertujuan untuk meningkatkan pembangunan desa yang menyesuaikan potnesi dari RPJM desa. Metode yang digunakan dalam program ini yaitu observasi dan pengkajian RPJM desa. Dengan alur kegiatan yaitu persiapan dan pembekalan mahasiswa KKN, kemudian dilanjutkan dengan pelaksanaan program diawali dengan observasi desa, mengkaji RPJM dalam melihat kembali program apa yang belum dijalankan dan dilanjutkan dengan menentukan proritas masalah, menentukan prioritas dari program yang akan dilaksanakan
Gerakan Masyarakat Sadar Stunting di Desa Helumo Kecamatan Anggrek Kabupaten Gorontalo Utara
Authors: Kobi Wiwin , Nurfaika Nurfaika 
Published: July 2024

Stunting atau kondisi gagal tumbuh merupakan masalah gizi utama di Indonesia. Permasalahan stunting pada balita berhubungan dengan kemiskinan masyarakat. Prevalensi stunting balita Indoensia pada tahun 2015 sebesar 36,4%. Hal ini menjelaskan bahwa sekitar 8,8 juta balita mengalami masalah tinggi badan dibawah standar sesuai usianya. Organisasi Kesehatan dunia menyatakan sekitar 20% kejadian stunting terjadi pada saat bayi berada dalam kandungan. penyebabnya antara lain asupan makanan ibu selama hamil yang kurang bergizi sehingga nutrisi janin sedikit yang erat kaitannya dengan kemiskinan. Factor penyebab lainnya yaitu MPASI ( Makanan Pendamping Asi) bayi usia dibawah 2 tahun yang kurang berkualitas, akses pelayanan Kesehatan yang terbatas, serta kurangnya pengetahuan ibu mengenai makanan bergizi. Sosialisasi mengenai Stunting di Desa Helumo merupakan salah satu kegiatan pelaksanaan program kerja Mahasiswa KKNT Periode II. Adapun Tujuan dari diadakan sosialisasi Stunting ini sebagai upaya peningkatan pengetahuan masyarakat terutama ibu hamil terhadap pencegahan stunting pada balita.
Pelatihan Pemanfaatan Aplikasi Media Sosial Untuk Layanan Stunting
Authors: Tuloli Mohamad Syafri , Novian Dian , Kadim Ahmad Azhar 
Published: July 2024

Media sosial adalah suatu platform dengan fasilitas yang membuat penggunanya dalam hal ini masyarakat dapat melakukan aktivitas sosial. Aktivitas sosial ini bisa seperti komunikasi sebagai interaksi sosial dengan mengirim atau memberi informasi. Pada dasarnya, media sosial merupakan bagian dari pengembangan akibat kemajuan teknologi dalam hal ini internet. Internet yang muncul beberapa dekade lalu berhasil membuat media sosial berkembang dengan cepat, bahkan bertumbuh dengan segala fasilitas atau manfaat baru yang diberikan kepada penggunanya. Dengan adanya internet yang terjangkau di Desa Tunggulo maka dapat mempermudah masyarakat untuk mendapatkan layanan informasi mengenai stunting menggunakan aplikasi media sosial. Di era moderen ini masyarakat lebih cenderung menggunakan media sosial untuk medapatkan atau memberikan informasi kepada orang lain, tidakterkecuali Masyarakat Desa Tunggulo. Maka dari itu kami memanfaatkan aplikasi media sosial yang sering atau sebagian besar masyarakat Desa Tunggulo gunakan yaitu Facebook untuk mendapatkan layanan informasi stunting. Stunting atau kondisi gagaltumbuh merupakan masala gizi utama pada desa Tunggulo. Permasalahan stunting pada balita berhubungan dengan kurangnyapengetahuan dan informasi yang berkaitan dengan stunting. Maka dari itu Kami membuat forum dan merekrut masyarakat untukbergabung guna untuk mendapatkan informasi-informasi mengenai stunting seperti pencegahan, penanagan dan asupan-asupan giziyang baik untuk menghindari penyebab stunting.
Colaboração da terapia cognitivo-comportamental no tratamento de Transtorno Afetivo Bipolar
Authors: Silva Uanderson Pereira da , Silveira Francis Moreira da , Azevedo Luiza Moura de Souza , Farias Wanderson , Rodrigues Michele Aparecida Cerqueira , Lopes Gabriel César Dias 
Published: July 2024

Introdução: A Terapia Cognitivo-Comportamental (TCC) tem se destacado como uma abordagem eficaz no tratamento do Transtorno Afetivo Bipolar (TAB). Este transtorno, caracterizado por oscilações extremas de humor entre episódios de mania e depressão, apresenta desafios significativos no seu manejo, e a TCC oferece uma série de estratégias que visam melhorar a qualidade de vida e estabilizar os sintomas dos pacientes. Objetivo: Analisar a contribuição da Terapia Cognitiva Comportamental no tratamento de pessoas afetadas pelo Transtorno Afetivo Bipolar. Método: Para isso foi usada uma abordagem qualitativa do tipo revisão de literatura, a pesquisa usou descritores para consulta em sites de busca, esses foram retirados dos Descritores em Ciências da Saúde (DeCS). As buscas das fontes foram na Biblioteca Virtual de Saúde (BVS) e na Scielo Scientific Electronic Library Online. Os descritores usados foram: Saúde mental AND Terapia Cognitiva Comportamental AND Transtorno de Humor AND Transtorno Bipolar, com uso de critérios de inclusão e exclusão. Resultados: A TCC no tratamento do TAB oferece uma abordagem ampla e eficaz para ajudar os pacientes a gerenciarem seus sintomas, prevenir recaídas e melhorar sua qualidade de vida. Ao combinar técnicas cognitivas, comportamentais e interpessoais, a TCC oferece aos pacientes ferramentas importantes para enfrentar os desafios únicos do TAB e alcançar uma recuperação sustentável. Conclusões: Concluiu-se que a TCC atua na gestão dos sintomas, prevenção de recaídas e melhora na qualidade de vida dos pacientes com TAB, proporcionando uma recuperação mais sustentável para os indivíduos afetados.
Climbing the Cliffs: Classifying Young Stellar Objects in the Cosmic Cliffs JWST Data Using a Probabilistic Random Forest
Authors: Crompvoets B. L. , Di Francesco J. , Teimoorinia H. , Preibisch T. 
Published: July 2024

Abstract
Among the first observations released to the public from the JWST was a section of the star-forming region NGC 3324 known colloquially as the “Cosmic Cliffs.” We build a photometric catalog of the region and test the ability of using the probabilistic random forest machine-learning method to identify its young stellar objects (YSOs). We find 450 candidate YSOs (cYSOs) out of 19,497 total objects within the field, 413 of which are cYSOs not found in previous works. These classifications are verified with several different metrics, including recall and precision. Using the obtained probabilities of objects being YSOs, we employ a Monte Carlo approach to determine the surface density of cYSOs in the Cosmic Cliffs, which we find to be largely coincident with column densities derived from Herschel data, up to a column density of 1.37 × 1022 cm−2. The newly determined number and spatial distribution of YSOs in the Cosmic Cliffs demonstrate that JWST is far more capable of detecting YSOs in dusty regions than Spitzer. Comparisons of the observed colors and brightness of faint cYSOs with those of pre-main-sequence models suggest JWST has detected a significant population of substellar YSOs in the Cosmic Cliffs. The size of this population further suggests previous estimates of star formation efficiencies in molecular clouds have been systematically low.
Exoplanet Aeronomy: A Case Study of WASP-69 b’s Variable Thermosphere
Authors: Levine W. Garrett , Vissapragada Shreyas , Feinstein Adina D. , King George W. , Hernandez Aleck , Corrales Lía , Greklek-McKeon Michael , Knutson Heather A. 
Published: July 2024

Abstract
Aeronomy, the study of Earth’s upper atmosphere and its interaction with the local space environment, has long traced changes in the thermospheres of Earth and other solar system planets to solar variability in the X-ray and extreme-ultraviolet (collectively, XUV) bands. Extending comparative aeronomy to the short-period extrasolar planets may illuminate whether stellar XUV irradiation powers atmospheric outflows that change planetary radii on astronomical timescales. In recent years, near-IR transit spectroscopy of metastable Hei has been a prolific tracer of high-altitude planetary gas. We present a case study of exoplanet aeronomy using metastable Hei transit observations from Palomar Observatory's Wide Field InfraRed Camera and follow-up high-energy data from the Neil Gehrels Swift Observatory that were taken within 1 month of the WASP-69 system, a K-type main-sequence star with a well-studied hot Jupiter companion. Supplemented by archival data, we find that WASP-69's X-ray flux in 2023 was less than 50% of what was recorded in 2016 and that the metastable Hei absorption from WASP-69 b was lower in 2023 versus past epochs from 2017 to 2019. Via atmospheric modeling, we show that this time-variable metastable Hei signal is in the expected direction given the observed change in stellar XUV, possibly stemming from WASP-69's magnetic activity cycle. Our results underscore the ability of multiepoch, multiwavelength observations to paint a cohesive picture of the interaction between an exoplanet’s atmosphere and its host star.
Breaking Giant Chains: Early-stage Instabilities in Long-period Giant Planet Systems
Authors: Nagpal Vighnesh , Goldberg Max , Batygin Konstantin 
Published: July 2024

Abstract
Orbital evolution is a critical process that sculpts planetary systems, particularly during their early stages where planet–disk interactions are expected to lead to the formation of resonant chains. Despite the theoretically expected prominence of such configurations, they are scarcely observed among long-period giant exoplanets. This disparity suggests an evolutionary sequence wherein giant planet systems originate in compact multiresonant configurations, but subsequently become unstable, eventually relaxing to wider orbits—a phenomenon mirrored in our own solar system’s early history. In this work, we present a suite of N-body simulations that model the instability-driven evolution of giant planet systems, originating from resonant initial conditions, through phases of disk dispersal and beyond. By comparing the period ratio and normalized angular momentum distributions of our synthetic aggregate of systems with the observational census of long-period Jovian planets, we derive constraints on the expected rate of orbital migration, the efficiency of gas-driven eccentricity damping, and typical initial multiplicity. Our findings reveal a distinct inclination toward densely packed initial conditions, weak damping, and high giant planet multiplicities. Furthermore, our models indicate that resonant chain origins do not facilitate the formation of Hot Jupiters via the coplanar high-eccentricity pathway at rates high enough to explain their observed prevalence.
GAINN: The Galaxy Assembly and Interaction Neural Networks for High-redshift JWST Observations
Authors: Santos-Olmsted Lillian , Barrow Kirk S. S. , Hartwig Tilman 
Published: July 2024

Abstract
We present the Galaxy Assembly and Interaction Neural Networks (Gainn), a series of artificial neural networks for predicting the redshift, stellar mass, halo mass, and mass-weighted age of simulated galaxies based on James Webb Space Telescope (JWST) photometry. Our goal is to determine the best neural network for predicting these variables at 11 < z < 15. The parameters of the optimal neural network can then be used to estimate these variables for real, observed galaxies. The inputs of the neural networks are JWST filter magnitudes of a subset of five broadband filters (F150W, F200W, F277W, F356W, and F444W) and two medium-band filters (F162M and F182M). We compare the performance of the neural networks using different combinations of these filters, as well as different activation functions and numbers of layers. The best neural network predicted redshift with a normalized rms error of

0.010

−
0.001

+
0.003

, stellar mass with rms =

0.089

−
0.022

+
0.044

, halo mass with a mean-squared error of

0.022

−
0.008

+
0.014

, and mass-weighted age with rms =

12.466

−
2.408

+
5.065

. We also test the performance of Gainn on real data from MACS0647JD, an object observed by JWST. Predictions from Gainn for the first projection of the object (JD1) have normalized bias 〈Δz〉 < 0.00228, which is significantly smaller than found with template-fitting methods. We find that the optimal filter combination is F277W, F356W, F162M, and F200W when considering both theoretical accuracy and observational resources from JWST.
The Dynamic Response of Jovian Magnetotail Reconnection to Enhanced Solar Wind Ram Pressure
Authors: Chen Junjie , Zhang Binzheng , Delamere Peter A. , Yao Zhonghua , Brambles Oliver 
Published: July 2024

Abstract
In this study, we employ the Grid Agnostic Magnetohydrodynamic (MHD) for Extended Research Applications (GAMERA), a high-resolving-power, three-dimensional global MHD model, to simulate magnetotail reconnection in Jupiter's magnetosphere. While previous satellite observations have provided initial statistics on magnetotail reconnection properties at Jupiter, they have been limited in spacetime coverage, leaving the dynamic process of Jovian magnetotail reconnection and its response to the solar wind (SW) poorly understood. Using MHD simulations, we quantitatively analyze the temporal evolution and spatial dependence of nightside reconnection in Jupiter's magnetotail under ideal quiet and enhanced SW conditions. Our results demonstrate that magnetotail reconnection tends to occur in the midnight and postmidnight sectors, with a low occurrence in the premidnight sector, consistent with both Galileo and Juno observations and predictions by Delamere & Bagenal. The magnetic local time (MLT)–radial distribution of magnetotail reconnection is broad, indicating that Jovian magnetotail reconnection is always dynamic rather than steady state. Enhanced SW ram pressure can decrease the MLT coverage of magnetotail reconnection by compressing Jupiter's magnetosphere. However, the occurrence of magnetotail reconnection near the midnight and postmidnight sectors is enhanced by SW compression beyond 60 R
J, but is not significantly impacted by SW compression within 60 R
J. Conversely, SW compression suppresses reconnection in the premidnight sector, leading to a stronger dawn–dusk asymmetry in the occurrence and location of magnetotail reconnection. This study validates the applicability of the GAMERA code for simulating Jupiter’s magnetosphere and provides complementary insights into the dynamic structure and the SW response of Jupiter’s magnetosphere.
ALMA Reveals Spatially Resolved Properties of Molecular Gas in the Host Galaxy of FRB 20191001A at z = 0.2340
Authors: Yamanaka Itsuki , Hatsukade Bunyo , Egusa Fumi , Hashimoto Tetsuya , Niino Yuu , Hsu Tzu-Yin , Kaneko Hiroyuki , Kohno Kotaro 
Published: July 2024

Abstract
We report the detection of the CO(2–1) emission line with a spatial resolution of 0.″9 (3.5 kpc) from the host galaxy of the fast radio burst (FRB), FRB 20191001A at z = 0.2340, using the Atacama Large Millimeter/submillimeter Array. This is the first detection of spatially resolved CO emission from the host galaxy of an FRB at a cosmological distance. The inferred molecular gas mass of the host galaxy is (2.3 ± 0.4) × 1010
M
⊙, indicating that it is gas-rich, as evidenced by the measured molecular gas fraction μ
gas = 0.50 ± 0.22. This molecular gas mass and the star formation rate of the host, SFR = (8.06 ± 2.42) M
⊙ yr−1, differ from those observed in the other FRB host galaxies with the average M
gas = 9.6 × 108
M
⊙ and SFR = 0.90M
⊙ yr−1. This lends further credibility to the hypothesis that FRBs may originate from single or multiple progenitors across a diverse range of galaxy environments. Based on the observed velocity field modeling, we find that the molecular gas disk is dominated by an ordered circular rotation, despite the fact that the host galaxy has a gas-rich companion galaxy with a projected separation of ∼25 kpc. The formation of the FRB’s progenitor might not have been triggered by this interaction. We derive the 3σ upper limit of the molecular gas column density at the FRB detection site to be <2.1 × 1021 cm−2 with a 3σ upper limit.