bluuebunny/crossref_metadata_2025_split huggingface dataset:
The concentration of interleukin-17 in the blood and urine of patients with chronic glomerulonephritis with nephrotic syndrome
Authors: Chemodanova D. A. , Vinogradov A. A. , Сao V. , Krasnova T. N. , Chebotareva N. V. 
Published: June 2023

BACKGROUND. In the mechanisms of immune inflammation in chronic glomerulonephritis (CGN), activation of T-cells plays an important role. The role of Th1 and Th2 cells in the pathogenesis of some forms of CGN has been well studied, while the activation of Th17 cells in CGN has been only evaluated in isolated studies. THE AIM: to evaluate the value of determining the level of IL-17 in urine and blood serum in chronic glomerulonephritis.PATIENTS AND METHODS. Adult patients with active CGN (N=40) were recruited aged from 18 to 75 years. Ten patients had focal segmental glomerulosclerosis, 6 had membranoproliferative glomerulonephritis, 15 had IgA nephropathy, and 9 had membranous nephropathy at histological examination. The control group included 10 healthy subjects. The IL-17A levels in the urine and blood serum were determined by enzyme-linked immunosorbent assay (ELISA). The IL17A levels in the urine were calculated as the ratio to urinary creatinine. The levels of IL-17 in urine and blood serum were compared with the indicators of proteinuria, albumin, creatinine, serum sodium, also the severity of hypertension, edema and daily sodium excretion.RESULTS. The results of our study showed a significantly higher concentration of IL-17 in urine in patients with a marked decrease in renal function. Also, the levels of IL-17 in urine directly correlated with serum sodium and inversely correlated with eGFR. We also found an association between increase levels of IL-17 in urine with arterial hypertension and the severity of edema. There were no significant correlations of IL-17 in blood serum and other laboratory indicators of nephritis activity.CONCLUSION. Patients with CGN have increase levels of IL-17 in the urine compared to healthy subjects. A more significant increase of IL-17 in urine is observed in patients with high clinical activity of HCG. IL-17A may participate in the mechanisms of sodium retention, the development of hypertension and edema in patients with nephrotic syndrome.
Hubungan Teknik Relaksasi Benson Terhadap Kadar Gula Darah Pasien Penderita Diabetes Militus Tipe 2
Authors: Zega Beni Wijaya , Sembiring Lora Pati Adelina Br , Laoli Delvin Sri Ariani , Silaban Helen Taruli T. , Ginting Chrismis Novalinda 
Published: June 2023

Pasien diabetes militus sekelompok yang mengalami metabolisme yang dikenali dengan gula darah tinggi. Pasien yang memiliki diabetes mempunyai resiko dua kali lipat yang mengakibatkan terkena penyakit kardiovaskuler dan terdapat sekitar 75% diabetes akan mengakibatkan kematian. Maksud dari penelitian ini ialah untuk memahami adakah pengaruh korelasi relaksasi benson dengan derajat kadar gula darah pada pasien DM. Metode riset menggunakan metode Quasy experiment menggunakan desain pre test-post test design. Populasi digunakan pada riset ini yaitu seluruh pasien yang mengalami penyakit gula darah yang tinggi pada DM tipe 2 di puskesmas Darussalam dari bulan Juni-Desember 2022 dengan jumlah 56 responden. Penarikan sampel yang kami gunakan yaitu sampel random untuk menentukan banyak sampel yang akan diambil. Media ukur yang digunakan yaitu lembaran observasi. Dalam penelitian ini ada dua analisa data yang digunakan yaitu analisa univariat yang dimana hasilnya dimasukan dalam tabel distribusi frekuensi dan analisa bivariat dengan menghubungkan dua variabel dengan uji t berpasangan. Hasil penelitian Karakteristik pada penderita DM tipe 2 mayoritas pada jenis kelamin laki-laki, usia >66, pendidikan terakhir SMP dan status pekerjaan tidak bekerja. Kadar gula darah yang penderita DM terdapat tipe 2 sebelum dilakukan dan sesudah dilakukan relaksasi benson terhadap perbedaan.Ada hubungan teknik relaksasi benson terhadap gula darah pada penderita DM tipe 2.
ANALYSIS OF MORAL VALUES IN THE ENOLA HOLMES MOVIE
Authors: Kurniati Natalia Sri , Bunau Eusabinus , Rezeki Yanti Sri 
Published: June 2023

The purpose of this research was to examine the kinds of moral values and describe how they are presented in the Enola Holmes movie directed by Harry Bradbeer. The research design was a descriptive qualitative study and the Enola Holmes movie script was the primary data source. The SPEAKING Model (setting, participants, ends, act sequence, key, instrumentalities, norms, genre) by Dell Hymes is used as the framework to assess the conversation in the movie. The results showed that the movie contained some moral values defined by Haidt such as care, fairness or proportionality, liberty, authority or respect, and loyalty or in group, also moral values defined by Barrow, such as fairness, respect for persons, freedom, and well-being. The most dominant moral values in this movie were liberty or freedom. The moral values are stated mostly by the characters in the movie directly, while some are stated indirectly. The moral values described in this research have important implications for teachers and other researchers, which encourage the use of various tools in analyzing discourse in literary works and able to apply the moral values in daily life.Keywords: moral value, literature, SPEAKING model, descriptive.
Analisis Strategi Pengembangan Usaha Menggunakan SWOT dan Business Model Canvas Pada Produk Air Minum Dalam Kemasan PT. Abutama
Authors: Arifin Moh Mawan , Agustin Meilan 
Published: June 2023

Industri Air Minum Dalam Kemasan (AMDK) di Indonesia saat ini memiliki peluang bisnis yang baik, dikarenakan tingkat konsumsi masyarakat akan air mineral terus mengalami peningkatan. PT. Abutama merupakan produsen air minum telah mulai diproduksi sejak tahun 2019. Penjualan produk AMDK “Aisy” yang dilakukan selama tahun 2019 belum mencapai target penjualan. Target penjualan yang masih belum tercapai disebabkan karena perusahaan masih melakukan tahap pengenalan produk dan jumlah agen penjual yang masih sedikit. Tujuan penelitian ini untuk membuat perencanaan strategi bagi perusahaan AMDK dalam mengembangkan usahanya sehingga dapat bersaing di pasar global. Metode yang digunakan adalah analisis Strenght, Weakness, Opportunity, Threatment (SWOT) dan Business Model Canvas. Hasil penelitian menunjukkan PT. Abutama berada dalam posisi bertahan. Perusahaan memiliki sisi kelemahan dan ancaman yang banyak. Perusahaan harus melakukan strategi perbaikan pada bagian internal dengan meminimalkan permasalahan yang ada dan situasi di eksernal dengan melakukan beberapa perbaikan agar bisa mendapatkan peluang yang lebih baik. Hasil analisis dengan Business Model Canvas yaitu value proposition menciptakan produk yang berkualitas, variasi produk, harga terjangkau dan menjalin komunikasi dengan beberapa perusahaan. Komunikasi dengan pelanggan melalui telepon, website, revenue stream dengan peningkatan penjualan produk dan key resources dengan memperbaiki fasilitas produksi.
Praktik Media Relations pada Pemerintahan Kota Bandung
Authors: Apriliyanti  
Published: June 2023

ABSTRACT
The government as an institution that represents the public interest requires media channels to maintain its reputation. The purpose of writing this article is to determine the practice of media relations carried out by the city government of Bandung. In conducting this research the writer used a qualitative descriptive research method using investigative interview techniques and in-depth interviews so that they were able to describe the results of observations and analyze the data obtained in the field. After analyzing and discussing the problem, the authors conclude that the media relations practices that occur in Bandung city government tend to be too "intimate". This has led to the practice of giving "envelopes". The forms of "envelopes" given by government agencies to journalists include transportation money, news money, THR and Eid gifts and souvenirs, souvenirs, wedding gifts or birthday gifts, and press trips. However, most of the journalists who covered considered what they received was not an “envelope” category. They think it is their right, and must be accepted because of pamali if they have to refuse fortune. Meanwhile, for the public relations staff, the gift is considered normal only as a form of appreciation and gratitude.
Keywords: public relations, media relations, government public relations.
ABSTRAK
Pemerintah sebagai Lembaga yang merepresentasikan kepentingan publik membutkan saluran media untuk menjaga reputasinya. Tujuan penulisan artikel ini adalah untuk mengetahui praktik media relations yang dilakukan oleh pemerintah kota Bandung. Dalam melakukan penelitian ini penulis menggunakan metode penelitian deskripsi kualitatif dengan menggunakan teknik wawancara investigasi dan in-depth interview sehingga mampu menggambarkan hasil observasi dan menganalisa data-data yang diperoleh dilapangan. Setelah melakukan analisis dan pembahasan masalah, penulis memperoleh kesimpulan bahwa praktik media relations yang terjadi di pemerintahan kota Bandung cenderung terlalu “mesra”. Hal tersebut menimbulkan adanya praktik pemberian “amplop”. Bentuk-bentuk “amplop” yang diberikan oleh dinas pemerintahan kepada wartawan diantaranya berupa uang transportasi, uang berita, THR dan bingkisan lebaran dan souvenir, souvenir, kado pernikahan atau kado ulang tahun, dan press trip. Namun, sebagian besar wartawan yang meliput menganggap apa yang mereka terima bukan termasuk dalam kategori “amplop”. Mereka beranggapan itu sudah merupakan hak mereka, dan harus diterima karena pamali kalau harus menolak rejeki. Sedangkan bagi staf humas sendiri, pemberian tersebut dianggap wajar hanya sebagai bentuk penghargaan dan bentuk rasa terimakasih.
Kata Kunci: public relations, media relations, Humas Pemerintah
Perbandingan Penerimaan Pembayaran E-wallet DANA dan OVO Menggunakan TAM Pada Generasi Z
Authors: Setiyani Lila , Vina Maulidina  , Femmy  
Published: June 2023

Perkembangan teknologi informasi mengakibatkan perubahan dalam hal transaksi pembayaran. Transaksi pembayaran yang awalnya secara tunai kini beralih menjadi non tunai atau cashless yaitu dengan menggunakan e-wallet. Banyaknya aplikasi e-wallet dapat mempermudah dalam hal pembayaran. Tujuan dari penelitian ini adalah untuk melakukan perbandingan penerimaan pembayaran e-wallet DANA dan OVO pada generasi Z. Prosedur dari penelitian ini dengan pengumpulan data melalui kuesioner dengan menggunakan skala likert, populasi dalam penelitian ini yaitu generasi Z dikota karawang, teknik sampel yang digunakan non-probability sampling dengan metode purpose sampling. Sampel yang diperoleh yakni, 200 responden. Bedasarkan hasil penelitian menunjukan bahwa generasi Z di kota karawang paling banyak menggunakan e-wallet DANA dibandingkan dengan OVO, dilihat dari jumlah responden DANA sebesar 124 responden dan OVO sebesar 76 responden.
Pengembangan Aplikasi E-UKM Berbasis Android Untuk Mendukung Era Digitalisasi Badan Eksekutif Mahasiswa Universitas Bina Insani
Authors: Arifin Rita Wahyuni , Apriani Rika , Wicaksono Harjunadi , Prameswara Andhika , Nabila SO Khairunisah , Romlah Siti 
Published: June 2023

Abstract
Student Activity Units (UKM) are student organizations where students with similar interests, hobbies, creativity, and orientations for extracurricular activities on campus gather. In the recruitment process of UKM members, it is currently conducted manually, where biodata forms are distributed to prospective members and collected by the UKM committee. The function of E-UKM BIU is to assist students and UKM committee members in facilitating the recruitment process of new members by utilizing E-UKM BIU. As it evolves, data from each UKM in Universitas Bina Insani is required. Additionally, there is also student data involved in the registration process, where the input data will be stored in a database and retrieved for the registration process conducted by the students. The software used in developing BIU E-UKM is Android Studio and Java, while the database utilizes SQLITE.
Keywords: Android, Digitalization, Student Activity Unit (UKM), Prototype
Abstrak
Unit Kegiatan Mahasiswa (UKM) adalah organisasi kemahasiswaan tempat para mahasiswa yang memiliki minat, hobi, kreativitas, dan orientasi yang sama untuk kegiatan ekstrakurikuler di kampus berkumpul. UKM dalam proses rekrutmen anggota masih dilakukan secara manual dimana dengan menggunakan biodata yang dibagikan kepada calon anggota dan dikumpulkan kepada pengurus UKM. Fungsi E-UKM BIU adalah untuk membantu mahasiswa dan pengurus UKM dalam memfasilitasi proses rekrutmen anggota baru dengan memanfaatkan E-UKM BIU. Dalam perkembangannya dibutuhkan data dari setiap UKM yang ada di Universitas Bina Insani, selain itu juga terdapat data mahasiswa dalam proses pendaftaran dimana data input akan disimpan dalam database dan data tersebut akan diambil untuk proses pendaftaran yang dilakukan oleh mahasiswa. Perangkat lunak yang digunakan dalam pengembangan BIU E-UKM adalah Android Studio dan Java, sedangkan database menggunakan SQLITE.
Kata Kunci : Android, Digitalisasi, Unit Kegiatan Mahasiswa, Prototipe
Unraveling Twisty Linear Polarization Morphologies in Black Hole Images
Authors: Emami Razieh , Ricarte Angelo , Wong George N. , Palumbo Daniel , Chang Dominic , Doeleman Sheperd S. , Broderick Avery E. , Narayan Ramesh , Wielgus Maciek , Blackburn Lindy , Prather Ben S. , Chael Andrew A. , Anantua Richard , Chatterjee Koushik , Marti-Vidal Ivan , Gómez Jose L. , Akiyama Kazunori , Liska Matthew , Hernquist Lars , Tremblay Grant , Vogelsberger Mark , Alcock Charles , Smith Randall , Steiner James , Tiede Paul , Roelofs Freek 
Published: June 2023

Abstract
We investigate general relativistic magnetohydrodynamic simulations to determine the physical origin of the twisty patterns of linear polarization seen in spatially resolved black hole images and explain their morphological dependence on black hole spin. By characterizing the observed emission with a simple analytic ring model, we find that the twisty morphology is determined by the magnetic field structure in the emitting region. Moreover, the dependence of this twisty pattern on spin can be attributed to changes in the magnetic field geometry that occur due to the frame dragging. By studying an analytic ring model, we find that the roles of Doppler boosting and lensing are subdominant. Faraday rotation may cause a systematic shift in the linear polarization pattern, but we find that its impact is subdominant for models with strong magnetic fields and modest ion-to-electron temperature ratios. Models with weaker magnetic fields are much more strongly affected by Faraday rotation and have more complicated emission geometries than can be captured by a ring model. However, these models are currently disfavoured by the recent EHT observations of M87*. Our results suggest that linear polarization maps can provide a probe of the underlying magnetic field structure around a black hole, which may then be usable to indirectly infer black hole spins. The generality of these results should be tested with alternative codes, initial conditions, and plasma physics prescriptions.
Tracer Particles for Core-collapse Supernova Nucleosynthesis: The Advantages of Moving Backward
Authors: Sieverding Andre , Waldrop Preston G. , Harris J. Austin , Hix W. Raphael , Lentz Eric J. , Bruenn Stephen W. , Messer O. E. Bronson 
Published: June 2023

Abstract
After decades, the theoretical study of core-collapse supernova explosions is moving from parameterized, spherically symmetric models to increasingly realistic multidimensional simulations. However, obtaining nucleosynthesis yields based on such multidimensional core-collapse supernova simulations is not straightforward. Frequently, tracer particles are employed. Tracer particles may be tracked in situ during the simulation, but often they are reconstructed in a post-processing step based on the information saved during the hydrodynamic simulation. Reconstruction can be done in a number of ways, and here we compare the approaches of backward and forward integration of the equations of motion to the results based on inline particle trajectories. We find that both methods agree reasonably well with the inline results for isotopes for which a large number of particles contribute. However, for rarer isotopes that are produced only by a small number of particle trajectories, deviations can be large. For our setup, we find that backward integration leads to better agreement with the inline particles by more accurately reproducing the conditions following freeze-out from nuclear statistical equilibrium, because the establishment of nuclear statistical equilibrium erases the need for detailed trajectories at earlier times. Based on our results, if inline tracers are unavailable, we recommend backward reconstruction to the point when nuclear statistical equilibrium was last applied, with an interval between simulation snapshots of at most 1 ms for nucleosynthesis post-processing.
LIMFAST. II. Line Intensity Mapping as a Probe of High-redshift Galaxy Formation
Authors: Sun Guochao , Mas-Ribas Lluís , Chang Tzu-Ching , Furlanetto Steven R. , Mebane Richard H. , Gonzalez Michael O. , Parsons Jasmine , Trapp A. C. 
Published: June 2023

Abstract
The epoch of reionization (EoR) offers a unique window into the dawn of galaxy formation, through which high-redshift galaxies can be studied by observations of both themselves and their impact on the intergalactic medium. Line intensity mapping (LIM) promises to explore cosmic reionization and its driving sources by measuring intensity fluctuations of emission lines tracing the cosmic gas in varying phases. Using LIMFAST, a novel seminumerical tool designed to self-consistently simulate LIM signals of multiple EoR probes, we investigate how building blocks of galaxy formation and evolution theory, such as feedback-regulated star formation and chemical enrichment, might be studied with multitracer LIM during the EoR. On galaxy scales, we show that the star formation law and the feedback associated with star formation can be indicated by both the shape and redshift evolution of LIM power spectra. For a baseline model of metal production that traces star formation, we find that lines highly sensitive to metallicity are generally better probes of galaxy formation models. On larger scales, we demonstrate that inferring ionized bubble sizes from cross-correlations between tracers of ionized and neutral gas requires a detailed understanding of the astrophysics that shape the line luminosity–halo mass relation. Despite various modeling and observational challenges, wide-area, multitracer LIM surveys will provide important high-redshift tests for the fundamentals of galaxy formation theory, especially the interplay between star formation and feedback by accessing statistically the entire low-mass population of galaxies as ideal laboratories, complementary to upcoming surveys of individual sources by new-generation telescopes.
Detection of X-Ray Polarized Emission and Accretion-disk Winds with IXPE and NICER in the Black Hole X-Ray Binary 4U 1630−47
Authors: Rawat Divya , Garg Akash , Méndez Mariano 
Published: June 2023

Abstract
We detect a high level of polarization in the X-ray emission of the black hole binary 4U 1630–47 in an observation with the Imaging X-ray Polarimetry Explorer. The 2–8 keV polarization degree is 8% at a position angle of 18°, with the polarization degree increasing significantly with energy, from ∼6% at ∼2 keV to ∼11% at ∼8 keV. The continuum emission in the spectrum of simultaneous observations with the Neutron Star Interior Composition Explorer (NICER) is well described with only a thermal disk spectrum, with stringent upper limits to any Comptonized emission from the corona. Together with the lack of significant variability in the Fourier power spectrum, this suggests that the source was in the high soft state at the time of these observations. The NICER spectrum reveals the presence of several absorption lines in the 6–9 keV band that we fit with two ionized absorbers, providing evidence of the presence of a strong disk wind, which supports the idea that the source was in the soft state. Previous measurements of X-ray polarization in other sources in harder states were associated with the corona or the jet in those systems. Given that the corona is significantly absent in this observation of 4U 1630–47, and that the jet in black hole binaries is quenched in the high soft state, we speculate that in this observation of 4U 1630–47, the polarization likely arises from the direct and reflected radiation of the accretion disk in this source.
JWST/NIRSpec Measurements of the Relationships between Nebular Emission-line Ratios and Stellar Mass at z ∼ 3–6
Authors: Shapley Alice E. , Reddy Naveen A. , Sanders Ryan L. , Topping Michael W. , Brammer Gabriel B. 
Published: June 2023

Abstract
We analyze the rest-optical emission-line ratios of star-forming galaxies at 2.7 ≤ z < 6.5 drawn from the Cosmic Evolution Early Release Science (CEERS) Survey and their relationships with stellar mass (M
*). Our analysis includes both line ratios based on the [N ii] λ6583 feature ([N ii] λ6583/Hα, ([O iii] λ5007/Hβ)/([N ii] λ6583/Hα) (O3N2), and [N ii] λ6583/[O ii] λ3727) and those featuring α-elements ([O iii] λ5007/Hβ, [O iii] λ5007/[O ii] λ3727 (O32), ([O iii] λλ4959, 5007 + [O ii] λ3727)/Hβ (R23), and [Ne iii] λ3869/[O ii] λ3727). Given the typical flux levels of [N ii] λ6583 and [Ne iii] λ3869, which are undetected in the majority of individual CEERS galaxies at 2.7 ≤ z < 6.5, we construct composite spectra in bins of M
* and redshift. Using these composite spectra, we compare the relationships between emission-line ratios and M
* at 2.7 ≤ z < 6.5 with those observed at lower redshift. While there is significant evolution toward higher excitation (e.g., higher [O iii] λ5007/Hβ, O32, O3N2) and weaker nitrogen emission (e.g., lower [N ii] λ6583/Hα and [N ii] λ6583/[O ii] λ3727) between z ∼ 0 and z ∼ 3, we find in most cases that there is no significant evolution in the relationship between line ratio and M
* beyond z ∼ 3. The [Ne iii] λ3869/[O ii] λ3727 ratio is anomalous in showing evidence for significant elevation at 4.0 ≤ z < 6.5 at fixed mass, relative to z ∼ 3.3. Collectively, however, our empirical results suggest no significant evolution in the mass–metallicity relationship at 2.7 ≤ z < 6.5. Representative galaxy samples and metallicity calibrations based on existing and upcoming JWST/NIRSpec observations will be required to translate these empirical scaling relations into ones tracing chemical enrichment and gas cycling and to distinguish among descriptions of feedback in galaxy formation simulations at z > 3.