bluuebunny/crossref_metadata_2025_split huggingface dataset:
Kecemasan Ibu Hamil Pada Masa Covid19 Di RSUD B Jakarta
Authors: Aini Nur , Yocki Yuanti  , Daniah  
Published: August 2023

Virus corona yang tengah merebak di Indonesia dan seluruh dunia sangat cepat Penularannya, terutama bagi kelompok rentan seperti ibu hamil. Hal ini menyebabkan timbul kecemasan yang dapat berdampak terhadap pertumbuhan janin. Tujuan penelitian ini menganalisis faktor kecemasan ibu hamil di RSUD B. Metode menggunakan kualitatif dalam pengembangan instrumen dan kuantitatif untuk analisis faktor. Responden sebanyak 75 orang bumil dengan pengumpulan data menggunakan kuisioner secara accidental sampling. Hasil : Berdasarkan uji statistik diketahui bahwa terdapat perbedaan usia ibu (p value 0,000) dan pengetahuan (p value 0,048) serta tidak terdapat perbedaan pada usia kehamilan (p value 0,137), status vaksinasi ( p value 0,511)
Virus corona yang tengah merebak di Indonesia dan seluruh dunia sangat cepat Penularannya, terutama bagi kelompok rentan seperti ibu hamil. Hal ini menyebabkan timbul kecemasan yang dapat berdampak terhadap pertumbuhan janin. Tujuan penelitian ini menganalisis faktor kecemasan ibu hamil di RSUD B. Metode menggunakan kualitatif dalam pengembangan instrumen dan kuantitatif untuk analisis faktor. Responden sebanyak 75 orang bumil dengan pengumpulan data menggunakan kuisioner secara accidental sampling. Hasil : Berdasarkan uji statistik diketahui bahwa terdapat perbedaan usia ibu (p value 0,000) dan pengetahuan (p value 0,048) serta tidak terdapat perbedaan pada usia kehamilan (p value 0,137), status vaksinasi ( p value 0,511)
Pola Komunikasi yang digunakan Ibu terhadap Keberhasilan Anak dalam Melakukan Toilet Training
Authors: Ramadhani Dina , Oswati Hasanah  , Rismadefi Woferst  
Published: August 2023

Pendahuluan: Toilet training merupakan cara untuk melatih kemampuan dalam mengendalikan diri, khususnya mengontrol buang air kecil dan buang air besar. Toilet training adalah salah satu tugas perkembangan saat anak memasuki usia toddler, sedangkan kemandirian dalam melakukan toilet training dicapai saat anak di usia pre school. Tercapainya toilet training dipengaruhi oleh beberapa faktor salah satunya adalah pola komunikasi. Pola komunikasi terdiri dari pola komunikasi fungsional dan pola komunikasi disfungsional. Penelitian ini bertujuan untuk mengetahui hubungan dari pola komunikasi yang digunakan ibu terhadap keberhasilan anak dalam melakukan toilet training. Metode: Penelitian ini menggunakan desain deskriptif korelatif dengan pendekatan cross sectional. Sampel penelitian adalah 97 responden menggunakan teknik purposive sampling. Penelitian ini menggunakan kuesioner yang telah di uji validitas dan reliabilitasnya. Analisis yang digunakan adalah analisis univariat dan analisis bivariat. Hasil: hasil analisis univariat menunjukkan mayoritas anak berada pada usia preschool (37-48) bulan (61,9%), jenis kelamin perempuan (50,5%), pendidikan orang tua adalah perguruan tinggi (47,4%), Pekerjaan orang tua adalah ibu rumah tangga (49,5%). Responden berhasil melakukan toilet training sebanyak 55 responden (56,7%), Hasil penelitian ini juga menunjukkan bahwa lebih dari setengah responden memiliki pola komunikasi yang baik/ fungsional (58,8%). Hasil analisis bivariat menunjukkan bahwa ada hubungan antara pola komunikasi ibu dengan keberhasilan anak dalam melakukan toilet training pada anak toddler dan preschool (p value 0,000; alpha 0,05%). Kesimpulan: Pola komunikasi yang baik/ fungsional mempengaruhi keberhasilan anak dalam melakukan toilet training.
Kata kunci: Pola komunikasi, pre school, toddler, toilet training
faktor-faktor yang mempengaruhi kejadian postpartum blues di BPM Elizabet wilayah kerja puskesmas payung sekaki
Authors: Purwati Anjeli indah , Nurhidaya Fitria  , Wira Ekdeni Aifa  
Published: August 2023

Postpartum blues yang juga disebut sebagai kemurungan masa nifas merupakan suatu fenomena perubahan psikologis yang dialami oleh ibu nifas. Postpartum blues terjadi pada hari ketiga sampai hari ke lima dan dalam rentang 14 hari. Faktor – faktor yang menyebabkan Postpartum blues yaitu usia, pekerjaan, dukungan keluarga, penghasilan. Tujuan penelitian ini untuk mengetahui ada kah hubungan antara faktor tersebut dengan kejadian Postpartum blues di BPM Elizabeth wilayah kerja Puskesmas Payung Sekaki Tahun 2022. Jenis penelitian ini merupakan penelitian kuantitatif dengan metode observasional-analitik menggunakan Desain penelitian cross-sectional. Teknik pengambilan sampel dengan teknik random sampling. Pengambilan data dengan menggunakan kuesioner EPDS dan PDPI. Analisis data menggunakan Chi Square. Hasil penelitian yang di peroleh terdapat hubungan yang signifikan pada semua variabel dengan kejadian Postpartum Blues. Variabel usia, dukungan keluarga, penghasilan dengan nilai p-value 0.000 dan variabel pekerjaan dengan p-value 0.001 yang berarti ada hubungan antara variabel terhadap kejadian Postpartum Blues. Disarankan bidan untuk meningkatkan pelayanan kesehatan untuk memberikan fasilitas yang menunjang seperti penyuluhan masa nifas, pendkes bahaya nifas, dan kelainan yang terjadi pada masa nifas untuk menurunkan angka kejadian Postpartum Blues.
Correlation between Uric Acid Levels and the Severity of Psoriasis Vulgaris Patients
Authors: Monica Pristia Widya , Nurrachmat Mulianto  
Published: August 2023

Introduction: Psoriasis vulgaris (PV) is a recurrent chronic inflammatory skin disease characterized by erythematous, scaly, well-defined plaques with the greatest predilection, generally in the areas of the elbows, knees, scalp, and lower back. The psoriasis area and severity index (PASI) is one of the most widely used evaluation tools to determine the development of psoriasis vulgaris in a patient. Hyperuricemia is the dominant risk factor for PV when compared to other known risk factors, such as obesity or metabolic syndrome. This study aimed to determine whether there is a relationship between serum uric acid levels and the severity of PV based on the PASI score.
Methods: Cross-sectional study with one-time sampling conducted from December 2021 to February 2022 in psoriasis vulgaris patients who came to the Dermatology and Venereology clinic at Dr. Moewardi General Hospital, Surakarta, Indonesia. All data were statistically analyzed using SPSS 26. Variables, including age, gender, disease duration, body mass index, and uric acid levels, were subjected to univariate analysis. Bivariate analysis was then followed by a parametric test. The p-value <0.05 was considered significant.
Results: There were 36 patients during the study period. The average uric acid level was 6.0135, with an average PASI score of 10.6388. The relationship between uric acid levels and the severity of psoriasis vulgaris was found to be significant, with a value of p = 0.025.
Conclusion: There is a significant relationship between uric acid levels and the severity of psoriasis vulgaris, where the higher the uric acid level, the more severe the severity of psoriasis vulgaris.
PEMERINTAHAN DESA DALAM PENGUNDANGAN RANCANGAN PERATURAN DESA KENAKALAN REMAJA BERDASARKAN PERATURAN BUPATI SAMBAS NOMOR 7 TAHUN 2018 TENTANG PEDOMAN TEKNIS PERATURAN DESA (Studi Kasus Di Desa Tengguli Kecamatan Sajad)
Authors: Hanapi  , Hasiah  
Published: August 2023

Pembentukan peraturan desa memiliki tahapan-tahapan yang telah diatur oleh pemerintah yang secara spesifiknya diatur oleh peraturan daerah masing-masing. Tahapan-tahapan tersebut diawali dengan musyawah pemerintah Desa bersama BPD hingga ke tahapan akhir yaitu pengundangan peraturan Desa. Namun, dalam hal pengundangan desa, terdapat Desa yang belum memahami proses pengundangannya seperti di Desa Tengguli Kecamatan Sajad terkait membentuk peraturan tentang kenakalan remaja. Meskipun pemerintahan Desa Tengguli telah mengikuti teknis pembentukan peraturan Desa sesuai Peraturan Bupati Sambas Nomor 7 Tahun 2018 Tentang Tata Cara Penyusunan Peraturan di Desa namun pada fase pengundangan yang tidak dievaluasi oleh Dinas Kabupaten sehingga saat ini peraturan tersebut belum diberlakukan. Oleh sebab itu, pemerintah desa memiliki peran penting dalam mengimplementasikan Perda Nomor 7 Tahun 2018 tentang Teknis Peraturan Desa maka perlu adanya peneltian dari perwujudan peran tersebut.
Adapun jenis penelitian sebagai upaya penguraian jurnal ini, penulis menggunakan jenis penelitian kualitatif dengan pendekatan empiris. Pendekatan empiris yang dimaksud sebagai pengungkap fenomena-fenoma hukum yang berlaku di masyarakat. Adapun, hasil yang diperoleh dapat disimpulkan bahwa dalam proses pembentukan peraturan desa, Pemerintah Desa Tengguli telah berperan aktif dalam tahapan perencanaan, penyusunan dan pembahasan, namun tidak pada tahap pengundangan dan sosialisasi. Pemerintah Desa tidak berupaya mengkonfirmasi ke pihak pemerintah Kabupaten terkait evalusi Perdes yang telah dibuat sehingga dapat menghambat terbitnya produk hukum yang seharusnya bisa dilaksanakan dalam hal menangani isu remaja masyarakat. Disisi lain, dengan pembentukan rancangan Perdes oleh Desa Tengguli dapat dikatakan bentuk peran Pemerintah sebagai penyelenggara pemerintah lokal dalam merespon isu-isu kenakalan remaja yang menjadi permasalahan sosial di masyarakat. Tidak hanya itu, terhambatnya pengundangan rancangan Perdes dikarenakan minimnya referensi masyarakat dan pemerintah desa dalam melakukan pembacaan terhadap regulasi, khususnya pada tahapan pengundangan peraturan di desa. Kurangnya koordinasi dengan lembaga yang berhubungan dengan perkara pengundangan peraturan desa juga membuat peraturan desa yang seharusnya sudah disosialisasikan menjadi terhambat.
Alteration of Gut microbiota during HIV infection
Authors: Altın Kevser Hanne 
Published: August 2023

Gut flora is the community of microbial populations that live in the intestine. Approximately 30% of this population is shared by all humans, but the remaining 70% is unique to each individual, hence gut microbiota serves as an identity card. Gut microbiota play numerous functions in the body's defense against invasion, the synthesis of important vitamins, the regulation of immunological marker production, and others. Researchers observed several data when analyzing bacteria species present in HIV-infected individuals using the 16S rRNA sequencing approach, concluding that HIV-infected people had a high number of Prevotella species, while Lachnospiraceae, Christensenellaceae, Ruminococcaceae, and Bacteroidaceae were all less. Those microbiota shifts may help explain how gut-related disorders interact with HIV. Researchers have discovered various methods for altering the composition of the gut microbiota in order to achieve a healthy gut. This review will focus on and highlight recent discoveries in Gut microbiota shifts during HIV infection and emphasize the immune response and treatment options.
Hemşirelerin Basınç Yaralanmalarını Önlemeye Yönelik Bilgi ve Tutumlarının Değerlendirilmesi
Authors: ÖZYÜREK Pakize , GÜRLEK KISACIK Öznur 
Published: August 2023

Amaç: Bu araştırmada hemşirelerin basınç yaralanmalarını önlemeye yönelik bilgi düzeyi ve tutumlarının değerlendirilmesi amaçlanmıştır.
Gereç ve Yöntem: Tanımlayıcı ve kesitsel tipteki bu araştırma 01.04.2020-01.09.2020 tarih aralığında bir hastanede çalışan toplam 140 hemşire ile yürütülmüştür. Veriler, "Hemşire Bilgi Formu", ''Basınç Ülseri Önlemede Bilgi Değerlendirme Ölçeği Türkçe versiyonu'' (BÜÖBDÖ) ve "Basınç Ülserlerini Önlemeye Yönelik Tutum Ölçeği (BÜÖYTÖ)" ile toplanmıştır.
Bulgular: Katılımcıların yaş ortalaması 26.71±5.55 olup mesleki çalışma süresi ise 6.48±5.09 olarak saptanmıştır. Hemşirelerin, BÜÖBDÖ toplam puanı 26 üzerinden 10.82 puan aldıkları ve sadece %8.5'inin (n=12) doğru cevap yüzdesi ve kabul edilebilir bilgi puanına (≥%60; ≥16) sahip olduğu bulunmuştur. Hemşirelerin BÜÖYTÖ toplam tutum puanı 52 üzerinden 37.10 olarak saptanırken, tutum yüzdesinin %41.6 olduğu belirlenmiştir. Hemşirelerin %42.8'inin (n=60) ortalama tutum puanının ≥%75 (tatmin edici tutum düzeyi) olduğu bulunmuştur. Hemşirelerin yaşları ile tutum puanları arasında pozitif yönde (rs= 0.198; p= 0.019), klinikte çalışma süreleri ile tutum puanları arasında ise negatif yönde zayıf düzeyde bir ilişki olduğu bulunuştur (rs= -0.199; p= 0.018).
Sonuç: Hemşirelerin basınç yaralanmalarını önlemeye yönelik bilgileri kabul edilebilir puan düzeyinde ve tutumlarının ise tatmin edici düzeyde olmadığı belirlenmiştir. Basınç yaralanmalarını önlemeye yönelik uygulamaları iyileştirmek için hemşirelerin bilgilerini arttırmaya ve olumlu tutumlar geliştirmelerine yönelik eğitimsel stratejiler ve müdahaleler geliştirilmelidir.
Optical Studies of Seven Bright Southern Cataclysmic Variable Stars
Authors: Thorstensen John R. , Alvarado-Anderson Chase K. , Burrows Abigail D. , Goebel-Bain Rowan M. , Katz David C. 
Published: August 2023

Abstract
We report spectroscopic observations of seven bright southern cataclysmic variable stars, collected on a single two-week observing run using the 1.9 m Radcliffe telescope at the South African Astronomical Observatory. We used a radial-velocity time series, in some cases in combination with other data, to determine or clarify orbital periods for five of them, namely ATO J061.1478−31.0634, BMAM-V547, MGAB-V202, NSV 4202, and V1147 Cen. For BMAM-V547, we use data from the Transiting Exoplanet Survey Satellite (TESS) to corroborate and sharpen the orbital period; the TESS data also show a photometric period near 3.93 days, likely indicating precession of the accretion disk. Also, we find a periodic modulation in the radial velocities of the SU UMa-type dwarf nova Var Ret2005, but are unable to specify a unique cycle count. Finally, we show a spectrum of ASASSN-V J061528.41−412007.3 that appears typical of a luminous novalike variable.
ALMA as a Redshift Machine: Using [C ii] to Efficiently Confirm Galaxies in the Epoch of Reionization
Authors: Schouws Sander , Bouwens Rychard , Smit Renske , Hodge Jacqueline , Stefanon Mauro , Witstok Joris , Hilhorst Juliëtte , Labbé Ivo , Algera Hiddo , Boogaard Leindert , Maseda Michael , Oesch Pascal , Röttgering Huub , van der Werf Paul 
Published: August 2023

Abstract
The [C ii]158μm line has long been proposed as a promising line to spectroscopically confirm galaxies in the epoch of reionization. In this paper, we present the results of new ALMA observations spectral scanning for [C ii] in six particularly luminous Lyman-break galaxies at z ∼ 7. The six sources were drawn from a sample of bright z ∼ 7 galaxies identified using the wide-area optical, near-IR, and Spitzer/IRAC data over the COSMOS/UltraVISTA field and were targeted on the basis of tight constraints on their redshifts from their IRAC [3.6]–[4.5] colors. We detect significant (>9σ) [C ii] lines in three of our six targets (50%) cospatial with the rest-UV emission from the ground/space-based near-IR imaging. The luminosities of the [C ii] lines lie in the range 5.6–8.8 × 108
L
⊙, consistent with the local [C ii]–SFR relation. Meanwhile, their [C ii]/L
IR ∼ 1–3 × 10−3 ratios are slightly elevated compared to local (U)LIRGS. This could be due to lower dust-to-gas or dust-to-metal ratios. We also find that our sources display a large kinematic diversity, with one source showing signs of rotation, one source a likely major merger, and one dispersion-dominated source that might contain a bright star-forming clump. Our results highlight the effectiveness of spectral scans with ALMA in spectroscopically confirming luminous galaxies in the epoch of reionization, something that is being be applied on a significantly larger sample in the ongoing REBELS large program.
The Temperature, Electron, and Pressure Characteristics of Switchbacks: Parker Solar Probe Observations
Authors: Huang Jia , Kasper Justin C. , Larson Davin E. , McManus Michael D. , Whittlesey Phyllis , Livi Roberto , Rahmati Ali , Romeo Orlando , Liu Mingzhe , Jian Lan K. , Verniero Jaye L. , Velli Marco , Badman Samuel T. , Rivera Yeimy J. , Niembro Tatiana , Paulson Kristoff , Stevens Michael , Case Anthony W. , Bowen Trevor A. , Pulupa Marc , Bale Stuart D. , Halekas Jasper S. 
Published: August 2023

Abstract
Parker Solar Probe observes unexpectedly prevalent switchbacks, which are rapid magnetic field reversals that last from seconds to hours, in the inner heliosphere, posing new challenges to understanding their nature, origin, and evolution. In this work, we investigate the thermal states, electron pitch-angle distributions, and pressure signatures of both inside and outside the switchbacks, separating a switchback into spike, transition region (TR), and quiet period (QP). Based on our analysis, we find that the proton temperature anisotropies in TRs seem to show an intermediate state between spike and QP plasmas. The proton temperatures are more enhanced in the spike than in the TR and QP, but the alpha temperatures and alpha-to-proton temperature ratios show the opposite trend to the proton temperatures, implying that the preferential heating mechanisms of protons and alphas are competing in different regions of switchbacks. Moreover, our results suggest that the electron-integrated intensities are almost the same across the switchbacks, but the electron pitch-angle distributions are more isotropic inside than outside switchbacks, implying switchbacks are intact structures, but strong scattering of electrons happens inside switchbacks. In addition, the examination of pressures reveals that the total pressures are comparable through an individual switchback, confirming switchbacks are pressure-balanced structures. These characteristics could further our understanding of ion heating, electron scattering, and the structure of switchbacks.
As Simple as Possible but No Simpler: Optimizing the Performance of Neural Net Emulators for Galaxy SED Fitting
Authors: Mathews Elijah P. , Leja Joel , Speagle 沈 Joshua S. 佳士 , Johnson Benjamin D. , Gibson Justus , Nelson Erica J. , Suess Katherine A. , Tacchella Sandro , Whitaker Katherine E. , Wang 王 Bingjie 冰洁 
Published: August 2023

Abstract
Artificial neural network emulators have been demonstrated to be a very computationally efficient method to rapidly generate galaxy spectral energy distributions, for parameter inference or otherwise. Using a highly flexible and fast mathematical structure, they can learn the nontrivial relationship between input galaxy parameters and output observables. However, they do so imperfectly, and small errors in flux prediction can yield large differences in recovered parameters. In this work, we investigate the relationship between an emulator’s execution time, uncertainties, correlated errors, and ability to recover accurate posteriors. We show that emulators can recover consistent results to traditional fits, with a precision of 25%–40% in posterior medians for stellar mass, stellar metallicity, star formation rate, and stellar age. We find that emulation uncertainties scale with an emulator’s width N as ∝N
−1, while execution time scales as ∝N
2, resulting in an inherent tradeoff between execution time and emulation uncertainties. We also find that emulators with uncertainties smaller than observational uncertainties are able to recover accurate posteriors for most parameters without a significant increase in catastrophic outliers. Furthermore, we demonstrate that small architectures can produce flux residuals that have significant correlations, which can create dangerous systematic errors in colors. Finally, we show that the distributions chosen for generating training sets can have a large effect on an emulator’s ability to accurately fit rare objects. Selecting the optimal architecture and training set for an emulator will minimize the computational requirements for fitting near-future large-scale galaxy surveys. We release our emulators on GitHub (http://github.com/elijahmathews/MathewsEtAl2023).
Formation Mechanism of Laser-driven Magnetized “Pillars of Creation”
Authors: Lei Zhu , Wang Lifeng , Li Jiwei , Zou Shiyang , Wu Junfeng , Zhao Zhonghai , Sun Wei , Yuan Wenqiang , Li Longxing , Yan Zheng , Li Jun , Ye Wenhua , He Xiantu , Qiao Bin 
Published: August 2023

Abstract
The Pillars of Creation, one of the most recognized objects in the sky, are believed to be associated with the formation of young stars. However, so far, the formation and maintenance mechanism of the pillars are still not fully understood due to the complexity of the nonlinear radiation magnetohydrodynamics (RMHD). Here, assuming laboratory laser-driven conditions, we studied the self-consistent dynamics of pillar structures in magnetic fields by means of two-dimensional and three-dimensional (3D) RMHD simulations, and the results support our proposed experimental scheme. We find that only when the magnetic pressure and ablation pressure are comparable, the magnetic field can significantly alter the plasma hydrodynamics. For medium-magnetized cases (β
initial ≈ 3.5), the initial magnetic fields undergo compression and amplification. This amplification results in the magnetic pressure inside the pillar becoming large enough to support the sides of the pillar against radial collapse due to pressure from the surrounding hot plasma. This effect is particularly pronounced for the parallel component (B

y
), which is consistent with observational results. In contrast, a strong perpendicular (B

x
, B

z
) magnetic field (β
initial < 1) almost retains its initial distribution and significantly suppresses the expansion of blown-off gas plasma, leading to the inability to form pillar-like structures. The 3D simulations suggest that the bending at the head of “Column I” in the Pillars of Creation may be due to nonparallel magnetic fields. After similarity scaling transformation, our results can be applied to explain the formation and maintenance mechanism of the pillars, and can also provide useful information for future experimental designs.
Isolating Dust and Free–Free Emission in ONC Proplyds with ALMA Band 3 Observations
Authors: Ballering Nicholas P. , Cleeves L. Ilsedore , Haworth Thomas J. , Bally John , Eisner Josh A. , Ginsburg Adam , Boyden Ryan D. , Fang Min , Kim Jinyoung Serena 
Published: August 2023

Abstract
The Orion Nebula Cluster (ONC) hosts protoplanetary disks experiencing external photoevaporation by the cluster’s intense UV field. These “proplyds” are comprised of a disk surrounded by an ionization front. We present ALMA Band 3 (3.1 mm) continuum observations of 12 proplyds. Thermal emission from the dust disks and free–free emission from the ionization fronts are both detected, and the high-resolution (0.″057) of the observations allows us to spatially isolate these two components. The morphology is unique compared to images at shorter (sub)millimeter wavelengths, which only detect the disks, and images at longer centimeter wavelengths, which only detect the ionization fronts. The disks are small (r

d
= 6.4–38 au), likely due to truncation by ongoing photoevaporation. They have low spectral indices (α ≲ 2.1) measured between Bands 7 and 3, suggesting the dust emission is optically thick. They harbor tens of Earth masses of dust as computed from the millimeter flux using the standard method although their true masses may be larger due to the high optical depth. We derive their photoevaporative mass-loss rates in two ways: first, by invoking ionization equilibrium and second, by using the brightness of the free–free emission to compute the density of the outflow. We find decent agreement between these measurements and

M

̇

= 0.6–18.4 × 10−7
M
⊙ yr−1. The photoevaporation timescales are generally shorter than the ∼1 Myr age of the ONC, underscoring the known “proplyd lifetime problem.” Disk masses that are underestimated due to being optically thick remains one explanation to ease this discrepancy.