bluuebunny/crossref_metadata_2025_split huggingface dataset:
Avaliação da anticoagulação oral com varfarina em hospital universitário
Authors: Oliveira Ana Carolina Amorim , Barreto Danielle Alves , Ferreira Itana Pinho Oliveira , Carvalho Josefa Camila Menezes Reis , Pires Leila Braga , De Melo Enaldo Vieira , Sousa Antônio Carlos Sobral , Campos Milena dos Santos Barros 
Published: December 2022

Introdução: A varfarina constitui um dos principais fármacos utilizados na prevenção de fenômenos embólicos. Como o seu metabolismo é influenciado por diversos fatores, a sua efetividade terapêutica é avaliada pelo TTR (Time in Terapeutic Range) do INR (Razão Normalizada Internacional) do tempo de protrombina. Todavia, tem sido relatada grande variabilidade do TTR entre os serviços de cardiologia. Objetivos: Avaliar o TTR de um ambulatório de anticoagulação e identificar os fatores impeditivos para se atingir o TTR ≥ 60%. Metodologia: Foram avaliados 130 prontuários de pacientes tratados com varfarina, no Hospital da Universidade Federal de Sergipe (HU-UFS), localizado na cidade de Aracaju/SE, no período de janeiro de 2017 a dezembro de 2019. Foram coletados os principais achados demográficos, clínicos e os INR do período do estudo. As variáveis quantitativas foram descritas como média ± desvio padrão, e a comparação entre os grupos foi realizada por meio do teste t de Student. As variáveis categóricas foram sumarizadas como número absoluto e percentagens e a comparação mediante os testes Qui quadrado (X²) e exato de Fischer, quando apropriado. Para análise das variáveis associadas ao TTR < 60%, foi utilizada a regressão logística, por intermédio do método “forward stepwise” e “backward stepwise”. Resultados: Os pacientes tinham idade média de 57,6 ± 16,2 anos e 88 (67,7%) voluntários exibiam fibrilação atrial. A média do TTR foi de 64,4%. A chance de apresentar TTR ≤ 60% foi: 1,69 vezes nos indivíduos do sexo feminino, 1,92 vezes nos portadores de diabetes mellitus (DM), 1,95 vezes em pacientes com trombofilia e 2,17 vezes naqueles que apresentaram acidente vascular cerebral (AVC). Conclusão: Os pacientes tratados com varfarina no HU-UFS exibiram o excelente TTR de 64%. Por outro lado, as mulheres e os portadores, de DM, AVC e trombofilia, tiveram maior chance de apresentar TTR < 60%.
Características clínicas dos pacientes com Covid-19 em um hospital de campanha
Authors: Barbosa Nayara , Saranholi Taís Lopes 
Published: December 2022

Em dezembro de 2019, o Centro de Controle e Prevenção de Doenças, localizado na China, identificou um surto de doença respiratória em Wuhan, a capital da província de Hubei. Posteriormente a esse ocorrido, identificou-se como causador da doença um novo coronavírus, o vírus pertence à família Coronaviridae, onde provoca uma doença respiratória, denominada de Covid-19. A doença disseminou-se rapidamente e, desde então, atingiu mais de muitos países de todos os continentes. A Organização Mundial da Saúde (OMS) declarou a Covid-19 uma pandemia em 11 de março de 2020. A Covid-19 possui uma grande variabilidade clínica em seu comportamento. O estudo teve como objetivo descrever as características clínicas dos pacientes com infecção confirmada pela SARS-CoV-2 diagnosticados e tratados no Hospital de Campanha de Bauru. Foi realizado um estudo, descritivo, documental, através dos prontuários dos pacientes que foram internados nos meses de junho, julho de 2020. Houve a participação de 56 pacientes que permaneceram internados na instituição durante o período do estudo, com idade média de 62 sendo predominante o sexo feminino que o conhecimento de alguns fatores de risco pode contribuir para intervenção e prevenção de disfunções renais e/ou minimizando complicações desses pacientes.
A importância da identificação precoce do Transtorno do Espectro Autista (TEA) em crianças: uma revisão de literatura
Authors: Dias Sara Maria Carvalho , Souza Kelli Costa , Brito Luciana Modesto de , Feitosa Ankilma do Nascimento Andrade , Braga Kassandra Lins , Cândido Rafaella de Abreu , Quental Maria Letícia Cruz , Sarmento Thaise de Abreu Brasileiro 
Published: December 2022

O transtorno do espectro autista (TEA) ainda não tem etiologia esclarecida, ele acomete o desenvolvimento de crianças em seus primeiros anos de vida. O quadro clínico do autista é bem diversificado, porém, apresenta sinais de dificuldades na comunicação verbal e não verbal e dificuldade no convívio social. O diagnóstico precoce é de extrema importância no TEA uma vez que enseja a intervenção precoce. O objetivo é de esclarecer como a identificação precoce da criança com transtorno do espectro autista pode ajudar no seu desenvolvimento e interação social. A presente proposta de estudo desenvolveu-se por meio de uma pesquisa bibliográfica do tipo revisão integrativa de literatura. A base de dados foi de algumas bibliotecas digitais, tais como, Centro Latino-Americano e do Caribe de Informação em Ciências da Saúde, popularmente chamado de BIREME, biblioteca nacional em saúde (BVS), portal de periódicos Capes e Scientific Electronic Library Online (SciELO), trabalhos escritos em português e inglês, de publicações de no máximo uma década. Embora os artigos selecionados mostrarem a importância da identificação do diagnóstico precoce do transtorno do espectro autista, pode-se verificar a carência de trabalhos relacionados ao tema no Brasil. Foi possível concluir que através da revisão bibliográfica realizada so­bre o tema, ficou evidente que ainda existem muitas brechas a serem preenchidas para atingir um comportamento satisfatório, no qual concilie um diag­nóstico precoce e um tratamento adequado o diagnóstico precoce para um tratamento eficaz continua sendo um desafio, devendo ser cada vez mais ex­plorado.
IMPLEMENTASI PENERIMA BANTUAN PANGAN NON TUNAI (BPNT) DENGAN MEGGUNAKAN METODE GENETIC MODIFIED K-NEAREST NEIGHBORI (GMKNN)
Authors: Ikhsan Nurul , Kurnia Gusti Siska , Yusra  , Insani Fitri , Wulandari Fitri 
Published: December 2022

Bantuan Pangan Non Tunai (BPNT) merupakan program pemerintah berupa bantuan pangan yang diberikan kepada Keluarga Penerima Manfaat (KPM) setiap bulannya, dimana kegiatan ini bertujuan untuk mengurangi beban pengeluaran dan mendukung nutrisi seimbang kepada KPM BPNT menggunakan mekanisme akun elektronik untuk membeli pangan di e-Warung yang telah bekerjasama dengan Bank, namun pada pelaksanaan BPNT di Kota Pekanbaru, penerimaan bantuan masih dianggap kurang efisien, sehingga pada penelitian ini, penulis melakukan pembagian pada masyarakat yang bisa menerima bantuan dan tidak bisa menerima bantuan pangan non tunai dengan menggunakan metode MKNN. Kesimpulan yang didapatkan dari penelitian ini adalah Algen (Algoritma Genetika) bisa diterapkan dengan metode MKNN, dan mendapatkan hasil akurasi 86,89% dengan probabilitas crossover adalah 0,9 dan nilai probabilitas mutasi adalah 0,1 dengan nilai K yaitu 3.
Studi Korelasional antara Minat Pasien dan Sarana Prasarana Terkait Kepuasan Pasien Rawat Inap di Rumah Sakit TNI AU Sam Ratulangi Manado
Authors: Molenaar Emmanuela R. , Karamoy Herman , Wagey Freddy , Surya Welong S. 
Published: December 2022

Abstract: As a health institution, hospitals are required to understand the needs of patients based on quality service that could affect the patients’ satisfaction towards the attitudes of medical and non-medical personnels, the facilities and infrastructure provided, and the environment that makes the patients feel comfortable and safe. This study aimed to determine the relationships between patients’ interest and infrastructure with patients’ satisfaction at Rumah Sakit TNI AU Sam Ratulangi Manado. This was a quantitative study. Samples were 67 inpatients obtained by using the quota sampling technique. Data were analyzed with the chi-square test. The results showed that based on the patients’ satisfaction, 58.2% of respondents were satisfied and 41.8% were dissatis-fied. Based on patients’ interest, 50.7% were interested and 49.3% were not interested. Based on facilities and infrastructure, 50.7% were good and 49.3% were not good. The results of the chi-square test confirmed that there was a relationship between patients’ interest and patients’ satisfaction (p=0.000), and there was a relationship between facilities and infrastructure with patients’ satisfaction (p=0.000). In conclusion, there are positive relationships between the patients’ interest as well as facilities and infrastructure with the patients’ satisfaction at Rumah Sakit TNI AU Sam Ratulangi Manado.
Keywords: patients’ satisfaction; patients’ interest; facilities and infrastructure

Abstrak: Rumah Sakit sebagai institusi kesehatan harus memahami kebutuhan pasien dalam hal kualitas pelayanan yang dapat memengaruhi kepuasan pasien terkait kepuasan terhadap sikap tenaga medis maupun non medis, sarana dan prasarana yang disediakan, serta lingkungan yang membuat pasien merasa nyaman dan aman. Penelitian ini bertujuan untuk mengetahui hubungan antara minat pasien dan sarana prasarana dengan kepuasan pasien rawat inap di Rumah Sakit TNI AU Sam Ratulangi Manado. Jenis penelitian ialah kuantitatif. Sampel penelitian sebanyak 67 responden diperoleh dengan menggunakan teknik quota sampling. Analisis statistik menggunakan uji chi square. Hasil penelitian mendapatkan variabel kepuasan pasien yang puas sebesar 58,2% dan tidak puas 41,8%. Variabel minat pasien yang minat sebesar 50,7% dan tidak minat 49,3%. Variabel sarana prasarana yang baik sebesar 50,7% dan kurang baik 49,3%. Hasil uji chi-square menegaskan adanya hubungan antara minat pasien dengan kepuasan pasien (p=0,000), dan adanya hubungan antara sarana prasarana dengan kepuasan pasien (p=0,000). Simpulan penelitian ini terdapat hubungan bermakna antara minat pasien dan sarana prasarana dengan kepuasan pasien di Rumah Sakit TNI AU Sam Ratulangi Manado.
Kata kunci: kepuasan pasien; minat pasien; sarana prasarana
Penggunaan Ice Breaking dalam Meningkatkan Motivasi Belajar Peserta Didik pada Mata Pelajaran Pendidikan Agama Islam Kelas VIII SMP Muhammadiyah Pinrang
Authors: Muharrir Syahruddin Muharrir , Herdah  , Effendy Rustan 
Published: December 2022

Penelitian ini bertujuan untuk mengetahui Penggunaan Ice Breaking dalam Meningkatkan Motivasi Belajar Peserta Didik pada Mata Pelajaran Pendidikan Agama Islam Kelas VIII SMP Muhammadiyah Pinrang. Penelitian ini merupakan penelitian eksperimental dengan rancangan one group pretest-posttest design dengan sampel 56 orang yang diambil .Lokasi penelitian ini bertempat di SMP Muhammadiyah Pinrang Alat pengumpulan data yang digunakan adalah kuesioner Ice Breaking.Peningkatan motivasi belajar PAI pada peserta didik setelah penerapan Ice Breaking sebesar 55.2% dan sisanya dipengaruhi oleh variabel lain. Dengan demikian hipotesis penelitian ini diterima yaitu Ice Breaking berpengaruh dan signifikan terhadap motivasi belajar PAI peserta didik

Kata Kunci: : Ice Breaking, Motivasi Belajar,Pendidikan Agama Islam
Konsep Masjid Integratif: Studi Kasus Masjid Istiqlal
Authors: Hamid Abdul Rosyid 
Published: December 2022

Penelitian ini bertujuan untuk mendeskripsikan kondisi pendidikan Masjid Istiqlal, menformulasikan konsep pendidikan masjid yang Integratif, menganalisis komponen pendidikan masjid Istiqlal dari segi tujuannya, kurikulumnya, proses belajar mengajarnya, tenaga pengajarnya, manajemennya, sarana prasarananya dan evaluasi pendidikannya. Penelitian ini menggunakan metode kualitatif deskriptif dengan studi kasus di masjid Istiqlal Jakarta. Sumber datanya adalah Ketua Harian Badan Pengelola Masjid Istiqlal, Kepala Sekretariat, Kabid Pendidikan dan Latihan, Wakil Direktur Madrasah Istiqlal. Teknik pengumpulan data melalui observasi, wawancara, dan dokumentasi. Teknik analisis data kualitatif dengan menganalisis data lapangan (field reserch) tidak menguji hipotesis melainkan untuk memaparkan data dan mengelolanya secara deskriptif tentang rumusan masalah. Tempat penelitian dilakukan di Masjid Istiqlal dengan beberapa program pendidikan seperti Majelis Taklim Kaum Ibu, Madrasah Istiqlal, Perpustakaan Istiqlal, Pendidikan Kader Ulama, pengajian Dialog Zhuhur, Pengajian Hawamisy, Pengajian Jum’at, Kajian Sabtu Pagi. Hasil penelitian ditemukan pertama; bahwa Masjid Istiqlal menyelenggarakan berbagai kegiatan pendidikan karena salah satu fungsi masjid sebagai pusat pendidikan, kedua Pengelolaan Masjid Istiqlal sangat profesional terutama kegiatan pendidikan sehingga menjadi pusat pendidikan masjid yang komprehensif dan Ideal. Dengan pendidikan masjid yang intensif ini, penulis berkesimpulan bahwa masjid Istiqlal bisa menjadi model pendidikan masjid integratif, dengan penyempurnaan pada aspek tujuan, metode, dan evaluasi.
Kata kunci: Masjid; Pendidikan Integratif
PENGARUH BAURAN PEMASARAN PARIWISATA DAN KUALITAS PELAYANAN MELALUI KEPUASAN WISATAWAN TERHADAP MINAT BERKUNJUNG KEMBALI (STUDI EMPIRIS PADA OBYEK WISATA BANTIMURUNG KABUPATEN MAROS)
Authors: USMAN AMIRUDDIN , Hidayat Muhammad , Daud Anshar 
Published: December 2022

Penelitian ini bertujuan untuk mengetahui dan menganalisis pengaruh bauran pemasaran pariwisata, kualitas layanan pariwisata terhadap kepuasan, untuk mengetahui dan menganalisis pengaruh bauran pemasaran pariwisata dan kualitas pelayananterhadap minat berkunjung kembali. Untuk mengetahui dan menganalisis pengaruh kepuasan terhadap minat berkunjung kembali, Untuk mengetahui dan menganalisis pengaruh bauran pemasaran pariwisata dan kualitas pelayanan terhadap minat berkunjung kembali melalui kepuasan wisatawan pada obyek wisata Bantimurung Kabupaten Maros. Sampel penelitian ini adalah wisatawan baik mancanegara maupun domestic atau nusantara yang sering berkunjung ke obyek wisata Bantimurung Kabupaten Maros. Hasil penelitian bahwa bauran pemasaran pariwisata berpengaruh positif dan signifikan terhadap kepuasan wisatawan. Kualitas pelayanan memberikan pengaruh positif dan signifikan terhadap kepuasan wisatawan. bauran pemasaran pariwisata memberikan pengaruh yang bermakna dalam meningkatkan minat wisatawan untuk melakukan kunjungan kembali. Kualitas pelayanan berpengaruh positif dan signifikan terhadap minat berkunjung kembali. Kepuasan wisatawan berpengaruh positif dan signifikan terhadap minat berkunjung kembali. Kepuasan wisatawan dapat memediasi secara parsial pengaruh bauran pemasaran pariwisata terhadap minat berkunjung kembali. Kepuasan wisatawan dapat memediasi secara parsial pengaruh kualitas pelayanan terhadap minat berkunjung kembali pada obyek wisata Bantimurung Kabupaten Maros
Discovery of a Radio-loud Narrow-line Seyfert 1 Galaxy at z = 0.9 Reddened with a Strong 2175 Å Bump
Authors: Zhou Yipeng , Hao Lei , Jiang Peng , Pan Xiang , Sun Luming , Jin Chichuan , Dai Xuejie , Liu Wenjuan , Ji Tuo , Zheng Zhenya , Huang Xiangning , Shi Xiheng , Wang Yibo , Xiong Yifei , Yang Chenwei 
Published: December 2022

Abstract
We present a broadband spectrophotometric analysis of an unusual quasar, SDSS J160558.86+474300.1, at z = 0.9, found in a systematic search for reddened radio-loud narrow-line Seyfert 1 galaxies (NLS1s). J1605+4743 qualifies for the conventional definition of an NLS1 in its permitted emission line widths and Hβ/[O iii] flux ratio. It also shows strong Fe ii emissions. J1605+4743 has a steep radio spectrum. With a radio loudness of ∼150 (70) before (after) reddening correction, it is among the most radio-loud NLS1s discovered. In addition, the blueshifted emission lines are also found to be weak, suggesting that it can be an exotic “wind-dominated” Seyfert similar to weak-line quasars, especially the ones with strong reddening. As an extreme hybrid central engine, its environment and host galaxy become rather intriguing. We discover in it a proximate 2175 Å absorber with a bump strength similar to the average value of 2175 Å absorbers in the Milky Way, which we suspect can be intrinsic to the quasar. In addition, the quasar seems to have enhanced instead of suppressed star formation at a rate of ≳94 M
⊙ yr−1. The combination of these unusual properties, i.e., the unique extinction, strong Fe ii and [O ii] lines, weak [O iii], Mg ii, and Balmer lines, and large radio loudness, might hold important clues to accretion physics, the formation/destruction of dust grains in the environment of active galactic nuclei, and possibly also the coevolution of supermassive black holes and their host galaxies in general.
The Impact of Initial–Final Mass Relations on Black Hole Microlensing
Authors: Rose Sam , Lam Casey Y. , Lu Jessica R. , Medford Michael , Hosek Matthew W. , Abrams Natasha S. , Ramey Emily , Vasylyev Sergiy S. 
Published: December 2022

Abstract
Uncertainty in the initial–final mass relation (IFMR) has long been a problem in understanding the final stages of massive star evolution. One of the major challenges of constraining the IFMR is the difficulty of measuring the mass of nonluminous remnant objects (i.e., neutron stars and black holes). Gravitational-wave detectors have opened the possibility of finding large numbers of compact objects in other galaxies, but all in merging binary systems. Gravitational lensing experiments using astrometry and photometry are capable of finding compact objects, both isolated and in binaries, in the Milky Way. In this work we improve the Population Synthesis for Compact object Lensing Events (PopSyCLE) microlensing simulation code in order to explore the possibility of constraining the IFMR using the Milky Way microlensing population. We predict that the Roman Space Telescope’s microlensing survey will likely be able to distinguish different IFMRs based on the differences at the long end of the Einstein crossing time distribution and the small end of the microlensing parallax distribution, assuming the small (π

E
≲ 0.02) microlensing parallaxes characteristic of black hole lenses are able to be measured accurately. We emphasize that future microlensing surveys need to be capable of characterizing events with small microlensing parallaxes in order to place the most meaningful constraints on the IFMR.
The Small Separation A-star Companion Population: First Results with CHARA/MIRC-X
Authors: De Furio Matthew , Gardner Tyler , Monnier John , Meyer Michael R. , Kratter Kaitlin , Schaefer Gail , Anugu Narsireddy , Davies Claire L. , Kraus Stefan , Lanthermann Cyprien , Le Bouquin Jean-Baptiste , Ennis Jacob 
Published: December 2022

Abstract
We present preliminary results from our long-baseline interferometry (LBI) survey to constrain the multiplicity properties of intermediate-mass A-type stars within 80 pc. Previous multiplicity studies of nearby stars exhibit orbital separation distributions well fitted with a lognormal with peaks >15 au, increasing with primary mass. The A-star multiplicity survey of De Rosa et al., sensitive beyond 30 au but incomplete below 100 au, found a lognormal peak around 390 au. Radial velocity surveys of slowly rotating, chemically peculiar Am stars identified a significant number of very close companions with periods ≤5 days, ∼0.1 au, a result similar to surveys of O- and B-type primaries. With the improved performance of LBI techniques, we can probe these close separations for normal A-type stars where other surveys are incomplete. Our initial sample consists of 27 A-type primaries with estimated masses between 1.44 and 2.49 M
⊙ and ages 10–790 Myr, which we observed with the MIRC-X instrument at the CHARA Array. We use the open-source software CANDID to detect five companions, three of which are new, and derive a companion frequency of

0.19

−
0.06

+
0.11

over mass ratios of 0.25–1.0 and projected separations of 0.288–5.481 au. We find a probability of 10−6 that our results are consistent with extrapolations based on previous models of the A-star companion population over the mass ratios and separations sampled. Our results show the need to explore these very close separations to inform our understanding of stellar formation and evolution processes.
A Very Large Array Study of Newly Discovered Southern Latitude Nonthermal Filaments in the Galactic Center: Radio Continuum Total-intensity and Spectral Index Properties
Authors: Paré Dylan M. , Lang Cornelia C. , Morris Mark R. 
Published: December 2022

Abstract
The nonthermal filament (NTF) radio structures clustered within a few hundred parsecs of the Galactic center (GC) are apparently unique to this region of the Galaxy. Recent radio images of the GC using MeerKAT at 1 GHz have revealed a multitude of faint, previously unknown NTF bundles (NTFBs), some of which are comprised of as many as 10 or more individual filaments. In this work we present Very Large Array observations at the C- and X-bands (4–12 GHz) at arcsecond-scale resolutions of three of these newly discovered NTFBs, all located at southern Galactic latitudes. These observations allow us to compare their total-intensity properties with those of the larger NTF population. We find that these targets generally possess properties similar to what is observed in the larger NTF population. However, the larger NTF population generally has steeper spectral indices than what we observe for our chosen targets. The results presented here based on the total-intensity properties of these structures indicate that the NTFs are likely a result of synchrotron emission from relativistic electrons that have been generated either by a nearby compact source or by extended magnetic field structures in which the magnetic field line reconnection has accelerated the electrons. In either scenario, once the relativistic electrons are produced and injected locally into the field they diffuse along the magnetic field lines, producing the filaments.
Dust Hot Spots at 10 au Scales around the Class 0 Binary IRAS 16293–2422 A: A Departure from the Passive Irradiation Model
Authors: Maureira María José , Gong Munan , Pineda Jaime E. , Liu Hauyu Baobab , Silsbee Kedron , Caselli Paola , Zamponi Joaquin , Segura-Cox Dominique M. , Schmiedeke Anika 
Published: December 2022

Abstract
Characterizing the physical conditions at disk scales in class 0 sources is crucial for constraining the protostellar accretion process and the initial conditions for planet formation. We use ALMA 1.3 and 3 mm observations to investigate the physical conditions of the dust around the class 0 binary IRAS 16293–2422 A down to ∼10 au scales. The circumbinary material’s spectral index, α, has a median of 3.1 and a dispersion of ∼0.2, providing no firm evidence of millimeter-sized grains therein. Continuum substructures with brightness temperature peaks of T
b ∼ 60–80 K at 1.3 mm are observed near the disks at both wavelengths. These peaks do not overlap with strong variations of α, indicating that they trace high-temperature spots instead of regions with significant optical depth variations. The lower limits to the inferred dust temperature in the hot spots are 122, 87, and 49 K. Depending on the assumed dust opacity index, these values can be several times higher. They overlap with high gas temperatures and enhanced complex organic molecular emission. This newly resolved dust temperature distribution is in better agreement with the expectations from mechanical instead of the most commonly assumed radiative heating. In particular, we find that the temperatures agree with shock heating predictions. This evidence and recent studies highlighting accretion heating in class 0 disks suggest that mechanical heating (shocks, dissipation powered by accretion, etc.) is important during the early stages and should be considered when modeling and measuring properties of deeply embedded protostars and disks.