bluuebunny/crossref_metadata_2025_split huggingface dataset:
Faktor-Faktor yang Berhubungan dengan Pengetahuan Ibu Hamil tentang Prevention Of Mother To Child Transmission
Authors: Anggraini Nofa , Sukmawati  
Published: October 2024

Human Immunodeficiency Virus/Acquired Immune Deficiency Syndrome (HIV/AIDS) merupakan masalah kesehatan di seluruh dunia. World Health Organization (WHO) menyatakan bahwa HIV dan AIDS menjadi ancaman global dan mengakibatkan dampak merugikan di semua sektor. Penyakit HIV dan AIDS merupakan penyakit infeksi penyebab kematian peringkat atas dengan angka kematian dan angka kejadian penyakit yang tinggi serta membutuhkan diagnosis serta terapi yang cukup lama (WHO, 2015). Tujuan dari penelitian ini adalah Untuk mengetahui faktor-faktor yang berhubungan dengan pengetahuan ibu hamil tentang PMTCT di Puskesmas Sriamur Bekasi tahun 2017. Metode penelitian yang digunakan adalah analitik dengan pendekatan cross sectional. Populasi dalam penelitian ini adalah seluruh ibu hamil yang melakukan pemeriksaan kehamilan di Puskesmas Sriamur pada bulan Mei 2017 dengan jumlah sampel sebanyak 60 orang. Dari hasil analisis univariat didapatkan sebagian besar responden dengan pengetahuan cukup 46,7%, umur 20-35 tahun 81,7%, pendidikan menengah 60%, paritas multipara 73,3% dan sumber informasi dari media 61,7%. Analisis bivariat menunjukkan adanya hubungan yang bermakna antara umur, pendidikan, paritas dan sumber informasi dengan pengetahuan ibu hamil tentang PMTCT.
Mengatasi Kecemasan Dengan Intervensi Senam Tera
Authors: Prastyaningrum Fitri Damayanti , Sulistyowati Dwi , Adriani Rita Benya , Tarnoto Koko Wahyu 
Published: October 2024

Lanjut usia merupakan fase terakhir dalam kehidupan seseorang. Bertambahnya usia maka semakin banyak permasalahan kesehatan yang dialami oleh lansia, tidak hanya kesehatan fisik tetapi juga kesehatan mental seperti kecemasan. Kecemasan pada lansia memiliki efek pada penurunan tingkat aktivitas fisik dan status fungsional, bahkan hingga berisiko pada kematian Salah satu cara alternatif untuk mengurangi kecemasan yaitu senam tera. Penelitian ini bertujuan untuk mengetahui pengaruh senam tera terhadap penurunan tingkat kecemasan pada lansia di Wilayah Kerja Puskesmas Manahan. Metode penelitian ini dengan desain pre-experimental yaitu one group pre-test and post-test design. Teknik sampling menggunakan metode purposive sampling berjumlah 36 responden dan instrumen penelitian menggunakan kuesioner Geriatric Anxiety Inventory. Intervensi dilakukan selama 4 minggu dalam 1 minggu 2 kali pertemuan. Data hasil penelitian dianalisis menggunakan uji statistik Paired Sample T-test. Hasil penelitian menunjukkan terdapat pengaruh yang signifikan senam tera pada penurunan tingkat kecemasan lansia karena saat melakukan senam tera dapat meningkatkan sekresi hormon endorfin yang bisa menimbulkan perasaan rileks dan bahagia sehingga dapat mengurangi kecemasan. Keseimpulan penelitian ini terdapat penurunan tingkat kecemasan pada lansia setelah dilakukan intervensi senam tera selama 8 kali.

Kata Kunci: Lansia, Kecemasan, Senam Tera
Faktor-Faktor Yang Mempengaruhi Tingkat Nyeri Tenggorokan Pasca Operasi Dengan Penggunaan Endoracheal Tube Pada Pasien Bedah Saraf
Authors: Amelia Khusnul , Olfah Yustiana , Donsu Jenita Doli Tine 
Published: October 2024

Latar Belakang : Nyeri tenggorokan pasca operasi dapat mempengaruhi beberapa aspek yaitu nyeri, gatal di tenggorokan dan rasa nyeri untuk menelan. Tindakan intubasi dapat menyebabkan komplikasi berupa nyeri tenggorokan. Tujuan : untuk mengetahui faktor-faktor yang mempengaruhi tingkat nyeri tenggorokan pasca operasi terhadap penggunaan endotracheal tube pada pasien bedah saraf di RSUD Prof. Dr. Margono Soekarjo Purwokerto. Metode : Penelitian ini dilakukan pada bulanebruari sampai Maret 2024 dengan pengambilan sampel menggunakan teknik konsekutif sampling sebanyak 80 responden pasien bedah saraf. Nyeri pasien diukur menggunakan NRS. Analisis data menggunakan Chi Square dan Regresi Logistik. Jenis penelitian ini adalah penelitian kuantitatif dengan desain observasional menggunakan desain cross-sectional. Hasil : Hasil penelitian didapatkan bahwa hasil uji Chi Square diperoleh nilai signifikansi pada umur (p=0.027), jenis kelamin (p=0.048), durasi penggunaan ETT (p=0.007), ukuran endotracheal tube (ETTp=0.001), dan tekanan manset (p=0.000). Hasil uji Logistic Reggretion tekanan manset mempunyai OR tertinggi yaitu 6,565 (0,000), disusul variabel lain yaitu usia (OR 0,064; p = 0,027), jenis kelamin (OR 4,021; p = 0,048), durasi ETT. penggunaan (OR 1,956; p = 0,007 ), ukuran ETT dan (OR 2,455; p = 0,001). Kesimpulan dan saran : secara keseluruhan usia, Jenis kelamin, lama penggunaan ETT, ukuran ETT, tekanan cuff dapat mempengaruhi tingkat nyeri tenggorokan pasca operasi pada penggunaan selang endotrakeal pada pasien bedah saraf.

Kata kunci : Sakit Tenggorokan, Intubasi Endotrakea, Pasca Operasi
Hasil Pemeriksaan Tes Cepat Molekuler (Genexpert) Pasien Suspek Tuberkulosis Paru Di RSUD Kabupaten Buleleng
Authors: Rejito Ahmad , Bintari Ni Wayan Desi , Idayani Sri 
Published: October 2024

Tuberkulosis adalah infeksi pada paru-paru yang disebabkan Mycobacterium tuberculosis. Prevalensi tuberculosis di Kabupaten Buleleng pada tahun 2021 masih tinggi dengan lebih dari 700 kasus. Tingginya angka kejadian tersebut mendorong perlunya pemeriksaan tuberculosis yang cepat dan akurat melalui Tes Cepat Molekuler (GeneXpert). Tujuan penelitian ini untuk mengetahui gambaran hasil pemeriksaan TCM pada pasien suspek Tuberkulosis paru di RSUD Kabupaten Buleleng pada Januari – Maret 2024. Penelitian dilakukan di Instalasi Laboratorium Klinik RSUD Kabupaten Buleleng. Sampel ditentukan dengan teknik simple random sampling dan besaran sampel dihitung dengan rumus Krejcie dan Morgan. Spesimen sputum pasien suspek tuberculosis dilakukan pemeriksaan dengan TCM GeneXpert. Hasil penelitian menunjukkan berdasarkan hasil TCM GeneXpert dari 204 pasien ditemukan MTB Rif sensitif Low (7,4%), MTB Rif Medium (2,9%), MTB Rif Sensitif High (5,9%), MTB Rif Resisten Low (0,5%), dan MTB Rif Resisten High (0,5%). Sementara itu sebagian besar sampel terdeteksi MTB not detected (82,8%). Berdasarkan distribusi frekuensi jenis kelamin dapat disimpulkan bahwa kejadian tuberkulosis paru pada pasien suspek di RSUD Kabupaten Buleleng pada Januari – Marey 2024 lebih banyak terjadi pada laki-laki dibandingkan wanita.

Kata Kunci: GeneXpert, Rifampisin, Tes Cepat Molekuler, Tuberkulosis, Mycobacterium tuberculosis
Diseño Preliminar de una Herramienta Digital Colaborativa para Mejorar el Aprendizaje Teórico de las Prácticas Clínicas en Seguridad del Paciente en el Programa Profesional de Enfermería
Authors: Carolina Vergara Diana , Pilar Vivas Diana 
Published: October 2024

De acuerdo con los conocimientos de los estudiantes del programa de enfermería respecto a la seguridad del paciente, surge la necesidad de crear una herramienta la cual los estudiantes puedan consultar en cualquier momento y lugar como lo es el podcast, debido a las extensas jornadas estudiantiles se hace necesario que ellos puedan tener a la mano un recurso el cual les permita reforzar los conocimientos y fomenta el trabajo colaborativo, con base a esto surge la pregunta ¿Cómo se puede mejorar el aprendizaje en el tema de seguridad del paciente en la práctica clínica en los estudiantes de enfermería por medio de herramientas digitales de la web 2.0?, para encontrar respuesta se realizó una encuesta de pre saberes a 10 estudiantes en práctica clínica (lo cual aún está en marcha), con el fin de diagnosticar los conocimientos que tiene respecto al tema de seguridad del paciente, posteriormente se realizó un comparativo de las herramientas de aprendizaje en web 2.0 aplicados en el área de la salud, con lo cual se definió sugerir la herramienta de podcast la cual se diseña para los estudiantes de enfermería de noveno semestre en el programa profesional de enfermería, acerca de la seguridad del paciente en la práctica clínica; posteriormente se describirán los resultados sobre el rendimiento académico de los estudiantes de noveno semestre de una universidad en la ciudad de Medellín, como producto del diseño de un podcast y con esta se hará un comparativo del rendimiento académico de los estudiantes de noveno semestre de enfermería del año 2024 con el estudiante del mismo semestre en años anteriores.
Analysis of Ring Galaxies Detected Using Deep Learning with Real and Simulated Data
Authors: Krishnakumar Harish , Kalmbach J. Bryce 
Published: October 2024

Abstract
Understanding the formation and evolution of ring galaxies, which possess an atypical ring-like structure, is crucial for advancing knowledge of black holes and galaxy dynamics. However, current catalogs of ring galaxies are limited, as manual analysis takes months to accumulate an appreciable sample of rings. This paper presents a convolutional neural network (CNN) to identify ring galaxies from unclassified samples. A CNN was trained on 100,000 simulated galaxies, transfer learned onto a sample of real galaxies, and applied to a previously unclassified data set to generate a catalog of rings, which was then manually verified. Data augmentation with a generative adversarial network to simulate images of galaxies was also employed. The resulting catalog contains 1967 ring galaxies. The properties of these galaxies were then estimated from their photometry and compared to the Galaxy Zoo 2 catalog of rings. However, the model’s precision is currently limited due to a severe imbalance of rings in real data sets, leading to a significant false-positive rate of 41.1%, which poses challenges for large-scale applications in surveys imaging billions of galaxies. This study demonstrates the potential of optimizing machine learning pipelines for low training data in rare morphologies and underscores the need for further refinements to enhance precision for extensive surveys like the Vera Rubin Observatory Legacy Survey of Space and Time.
The OATMEAL Survey. I. Low Stellar Obliquity in the Transiting Brown Dwarf System GPX-1
Authors: Giacalone Steven , Dai Fei , Zanazzi J. J. , Howard Andrew W. , Dressing Courtney D. , Winn Joshua N. , Rubenzahl Ryan A. , Carmichael Theron W. , Vowell Noah , Kesseli Aurora , Halverson Samuel , Isaacson Howard , Brodheim Max , Deich William , Fulton Benjamin J. , Gibson Steven R. , Hill Grant M. , Holden Bradford , Householder Aaron , Kaye Stephen , Laher Russ R. , Lanclos Kyle , Payne Joel , Petigura Erik A. , Roy Arpita , Schwab Christian , Shaum Abby P. , Sirk Martin M. , Smith Chris , Stefánsson Guðmundur , Walawender Josh , Wang Sharon X. , Weiss Lauren M. , Yeh Sherry 
Published: October 2024

Abstract
We introduce the OATMEAL survey, an effort to measure the obliquities of stars with transiting brown dwarf companions. We observed a transit of the close-in (P
orb = 1.74 days) brown dwarf GPX-1 b using the Keck Planet Finder spectrograph to measure the sky-projected angle between its orbital axis and the spin axis of its early F-type host star (λ). We measured λ = 6.°9 ± 10.°0, suggesting an orbit that is prograde and well aligned with the stellar equator. Hot Jupiters around early F stars are frequently found to have highly misaligned orbits, with polar and retrograde orbits being commonplace. It has been theorized that these misalignments stem from dynamical interactions, such as von Zeipel–Kozai–Lidov cycles, and are retained over long timescales due to weak tidal dissipation in stars with radiative envelopes. By comparing GPX-1 to similar systems under the frameworks of different tidal evolution theories, we argued that the rate of tidal dissipation is too slow to have re-aligned the system. This suggests that GPX-1 may have arrived at its close-in orbit via coplanar high-eccentricity migration or migration through an aligned protoplanetary disk. Our result for GPX-1 is one of few measurements of the obliquity of a star with a transiting brown dwarf. By enlarging the number of such measurements and comparing them with hot-Jupiter systems, we will more clearly discern the differences between the mechanisms that dictate the formation and evolution of both classes of objects.
CHIANTI—An Atomic Database for Emission Lines—Paper. XVIII. Version 11, Advanced Ionization Equilibrium Models: Density and Charge Transfer Effects
Authors: Dufresne R. P. , Del Zanna G. , Young P. R. , Dere K. P. , Deliporanidou E. , Barnes W. T. , Landi E. 
Published: October 2024

Abstract
Version 11 of the chianti database and software package is presented. Advanced ionization equilibrium models have been added for low charge states of seven elements (C, N, O, Ne, Mg, Si, and S), and represent a significant improvement especially when modeling the solar transition region. The models include the effects of higher electron density and charge transfer on ionization and recombination rates. As an illustration of the difference these models make, a synthetic spectrum is calculated for an electron pressure of 7 × 1015 cm−3 K and compared with an active region observation from HRTS. Increases are seen in factors of 2–5 in the predicted radiances of the strongest lines in the UV from Si iv, C iv, and N v, compared to the previous modeling using the coronal approximation. Much better agreement (within 20%) with the observations is found for the majority of the lines. The new atomic models better equip both those who are studying the transition region and those who are interpreting the emission from higher-density astrophysical and laboratory plasma. In addition to the advanced models, several ion data sets have been added or updated, and data for the radiative recombination energy loss rate have been updated.
The Dark Energy Camera Magellanic Clouds Emission-line Survey
Authors: Points Sean D. , Long Knox S. , Blair William P. , Williams Rosa , Chu 朱 You-Hua 有花 , Winkler P. Frank , White Richard L. , Rest Armin , Li 李 Chuan-Jui 傳睿 , Valdes Francisco 
Published: October 2024

Abstract
We have used the Dark Energy Camera (DECam) on the CTIO Blanco 4 m telescope to perform a new emission-line survey of the Large Magellanic Cloud (LMC) using narrowband Hα and [S ii] filters in addition to a continuum band to create pure emission-line images. We refer to this new survey as DeMCELS, to distinguish it from the earlier Magellanic Cloud Emission-line Survey (MCELS). DeMCELS covers ∼54 deg2, encompassing most of the bright optical disk of the LMC. With DECam's pixel size of only 0.″27, our DeMCELS survey provides a seeing-limited improvement of 3–5 times over MCELS and is comparable in depth, with surface brightness limits of

3.3
×

10

−
17

erg

cm

−
2

s

−
1

arcsec

−
2

and

2.9
×

10

−
17

erg

cm

−
2

s

−
1

arcsec

−
2

in Hα and [S ii], respectively. DeMCELS provides detailed morphological information on nebulae of all scales, from the largest supershells to individual H ii regions and supernova remnants, to bubbles of emission surrounding individual stars, and even to faint structures in the diffuse ionized gas of the LMC. Many complex regions of emission show significant variations in the ratio of [S ii] to Hα—a sign of a mixture of shocks from stellar winds and/or supernovae with photoionization by embedded hot, young stars. We present the details of the observing strategy and data processing for this survey, and show selected results in comparison with previous data. A companion project for the Small Magellanic Cloud is in progress and will be reported separately. We are making these new data available to the community at large via NOIRLab’s Data Lab site.
Spectropolarimetry of Fraunhofer Lines in Local Upper Solar Atmosphere
Authors: Qu Z. Q. , Chang L. , Dun G. T. , Cheng X. M. , Fang C. , Xu Z. , Yuan D. , Deng L. H. , Zhang X. Y. 
Published: October 2024

Abstract
Spectropolarimetric results of Fraunhofer lines between 516.3 and 532.6 nm are presented in local upper solar chromosphere and inner corona below a height of about 0.04 solar radius above the solar limb. The data were acquired on 2013 November 3 during a total solar eclipse in Gabon by the prototype Fiber Arrayed Solar Optical Telescope. It is found that the linear polarizations of the Fraunhofer lines in these layers depend strongly on specific spectral lines and positions. A Fraunhofer line at Mg i
b
1518.4 nm can have a polarization amplitude up to 0.36% with respect to the continuum polarization level, while polarizations of lines like Fe i/Cr i524.7 nm are often merged in the noise level of 6.0 × 10−4. The polarizations of the Fraunhofer lines, like the emission ones and the continuum, increase with height as a whole trend, and their amplitudes can be close to those of emission ones yielded in close positions, and generally larger than those of the continuum. Rotations of the polarization directions of the Fraunhofer lines are often accompanied by variations in their polarization amplitudes and profile shapes. It is also judged from these polarimetric properties, along with other evidence, that neutral metal atoms exist in these atmospheric layers.
Multiple Emission Regions in Jets of the Low-Luminosity Active Galactic Nucleus in NGC 4278
Authors: Dutta Samik , Gupta Nayantara 
Published: October 2024

Abstract
The Large High Altitude Air Shower Observatory (LHAASO) has detected very-high-energy gamma rays from the low-ionization nuclear emission-line region galaxy NGC 4278, which has a low-luminosity active galactic nucleus (LLAGN) and symmetric, mildly relativistic S-shaped twin jets detected by radio observations. Few LLAGNs have been detected in gamma rays due to their faintness. Earlier, several radio-emitting components were detected in the jets of NGC 4278. We model their radio emission with synchrotron emission of ultra-relativistic electrons to estimate the strength of the magnetic field inside these components within a time-dependent framework after including the ages of the different components. We show that the synchrotron and synchrotron self-Compton emission by these components cannot explain the Swift X-ray data and the LHAASO gamma-ray data from NGC 4278. We suggest that a separate component in one of the jets is responsible for the high-energy emission, whose age, size, magnetic field, and the spectrum of the ultra-relativistic electrons inside it have been estimated after fitting the multiwavelength data of NGC 4278 with the sum of the spectral energy distributions from the radio components and the high-energy component. We note that the radio components of NGC 4278 are larger than the high-energy component, which has also been observed in several high-luminosity active galactic nuclei.
3He and Fe Spectral Properties in 3He-rich Solar Energetic Particle Events
Authors: Mason G. M. , Kouloumvakos A. , Ho G. C. , Allen R. C. , Gómez-Herrero R. , Wimmer-Schweingruber R. F. , Rodríguez-Pacheco J. 
Published: October 2024

Abstract
We have surveyed 3He-rich events on the Solar Orbiter mission from 2020 April to 2024 April, selecting isolated injections whose rollover 3He spectral shape is presumed to represent the initial acceleration state, unprocessed by subsequent activity such as coronal mass ejections or jets. A main goal has been to find relationships between the spectra of 3He and heavy ions C–Fe, in order to explore a common acceleration mechanism in spite of the fact that these events show 3He enrichments of up to ∼104, while the heavy-ion enrichment is rarely larger than ∼10. Selecting 34 3He injections, we find that heavy ions are always present, and arrive at the same time as the 3He signaling a common origin. Concentrating on Fe since it is a minor ion but with higher abundance than many others, we find its spectral shape and intensity is similar to 3He. In ∼two-thirds of the cases, if the 3He spectrum is shifted to lower energy by a factor 3.0 ± 1.3, it nearly coincides with the Fe spectrum, illustrating their close connection. Several plasma wave turbulence models have calculated spectra that also show the ion rollovers around 1 MeV nucleon−1. The unique mass-to-charge ratio of 3He allows it to interact more efficiently with the turbulence, thereby gaining several times more energy per nucleon than the other heavy ions. In the spectral rollover region this can lead to the observed enormous enhancements of 3He. The acceleration appears to be associated with magnetic reconnection in emerging flux regions on the Sun.
The A2Π–X2Σ+ Band System of YO
Authors: Bernath Peter F , Bhusal Manish , Pastorek Adam 
Published: October 2024

Abstract
YO bands are conspicuous in the spectra of S stars. The laboratory spectrum of the A2Π–X2Σ+ electronic transition has been recorded with a Fourier transform spectrometer using a composite-wall hollow cathode lamp source. The A2Π–X2Σ+ transition with

v

′

≤
4

and v″ ≤ 4 has been rotationally analyzed using the modern spectral fitting program PGOPHER. Vibronic band strengths were calculated using an ab initio transition dipole moment function. A line list for the A2Π–X2Σ+ transition is provided and can be utilized in the modeling of S stars.
Temporal Evolution of Electron Accelerations behind the Dipolarization Front in the Earth's Magnetotail
Authors: Deng Xiangxi , Yuan Zhigang , Huang Shiyong , Jiang Kui 
Published: October 2024

Abstract
We report the temporal evolution of electron pitch angle distributions behind the dipolarization front (DF) in the Earth's magnetotail with observations of the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft. Taking advantage of multipoint observations from the THEMIS mission lined up in space, we study pitch angle distributions of energetic electrons behind the DF during two typical events. Pancake, rolling-pin, and cigar distributions are observed sequentially during the acceleration process. Based on Liouville's theorem, it is revealed that pancake distribution is dominantly formed by betatron acceleration in the early stage, and rolling-pin distribution is generated by both dominant Fermi and weak betatron acceleration in the transition stage, while cigar distribution is formed by Fermi acceleration finally. Our results provide comprehensive in situ observational evidence of the temporal evolution of electron acceleration behind the DF during propagation.
A Luminous X-Ray Active Galactic Nucleus in the Dwarf–Dwarf Galaxy Merger RGG 66
Authors: Kimbrell Seth J. , Reines Amy E. 
Published: October 2024

Abstract
We present the discovery of a luminous X-ray active galactic nucleus (AGN) in the dwarf galaxy merger RGG 66. The black hole is predicted to have a mass of M
BH ∼ 105.4
M
⊙ and to be radiating close to its Eddington limit (L
bol/L
Edd ∼ 0.75). The AGN in RGG 66 is notable both for its presence in a late-stage dwarf–dwarf merger and for its luminosity of L
2–10 keV = 1042.2 erg s−1, which is among the most powerful AGNs known in nearby dwarf galaxies. The X-ray spectrum has a best-fit photon index of Γ = 2.4 and an intrinsic absorption of N

H
∼ 1021 cm−2. These results come from a follow-up Chandra X-ray Observatory study of four irregular/disturbed dwarf galaxies with evidence for hosting AGNs based on optical spectroscopy. The remaining three dwarf galaxies do not have detectable X-ray sources with upper limits of L
2–10 keV ≲ 1040 erg s−1. Taken at face value, our results on RGG 66 suggest that mergers may trigger the most luminous of AGNs in the dwarf galaxy regime, just as they are suspected to do in more massive galaxy mergers.