bluuebunny/crossref_metadata_2025_split huggingface dataset:
RANCANG BANGUN ALAT PEMANTAU BERAT MENGGUNAKAN ANDROID BERBASIS MIKROKONTROLER
Authors: Ahmad Nurfauzi  , Agil Candra Ramadhan  , M.Ridwan Arif Cahyono  
Published: August 2023

Digital scales are measuring instruments to measure the mass weight of objects or substances with a digital display. In its use, scales are used in various fields, from trade, industry to service companies. In this case, digital scales have many advantages, including: the mass of the scale itself is lighter than manual scales, the results of measuring the measured load are more accurate, suitable for measuring small objects, in terms of design digital scales seem more modern and in terms of maintenance required it is very easy to do. Measuring instruments are designed and made by prioritizing the ability of measuring instruments such as accuracy, accuracy, and reading ability. There are two category systems in scales, namely Analog Scales and Digital Scales.
Load cell is the core component contained in the Digital Scale which functions as a pressure sensor that will convert the analog signal generated by the Load Cell to the amount of electricity. The reading of the load cell data will be processed by Esp 8266 through the HX711 system to convert the amount of potential that occurs in the load cell into digital data. This method uses the measurement principle carried out by Loadcell using the pressure principle that utilizes the Strain Gauge as a sensor. This is evidenced by the results of testing the condition of the tool in good condition and in accordance with the accuracy when the object is weighed to get a result of 99%.
Perancangan Sistem Informasi Penjualan E-Commerce Rempeyek Ilhamum-Taza Berbasis Web
Authors: Heriyani  , Tuty Ulina Malau  
Published: August 2023

Ilhamum-Taza is a micro, small and medium enterprise (UMKM) which is engaged in the production and sale of tempe chips and peanut brittle which have become souvenirs from Jambi. UMKM manage the sale of goods is still manual so that the sale of goods is not optimal. Sales management to be more optimal so that it must use a web based e-commerce information system. The development of this web based e-commerce information system uses the waterfall model and the data flow model uses DFD (Data Flow Diagrams) . This research and design produces an e-commerce information system that will be implemented in UMKM Ilhamum-Taza.
Makna Penggunaan Repetisi Frase “TUHAN Menyesal” dalam Yeremia 26:1-24
Authors: Josua Rezky Alfero , Sualang Farel Yosua , Sulistya Philipus Pada 
Published: August 2023

The purpose of this article is to show that in Jeremiah 26 there is a ladder repetition of the phrase "the LORD regret." Because if you pay special attention, very few interpreters find repetition that occurs three times in Jeremiah 26 verses 3, 13 and 19 regarding the phrase "the LORD regret". Using the sub-hermeneutic leatherative method: Exegesis, this article finds the meaning of the use of repetition of the phrase "The LORD regret" in Jeremiah 26:3, 13 and 19 mentioned by three different subjects "I regret (the LORD)", "The LORD regrets (Jeremiah)," "The LORD regret (the leaders of the nation)." First, the way the LORD conveyed His prophecy by showing an emotional expression (anthropomorphism) because of the sinfulness of the nation of Judah. Secondly, the prophet Jeremiah showed himself to be a true prophet and gave an affirmation of responsiveness for the LORD to cancel His punishment on the nation of Judah. Thirdly, the leaders of the nation remembered the prophecies of Micah and Uriah, so that they should not ignore His message and thus the LORD changed His mind, so that the nation of Judah received salvation and repented by turning to the true LORD.
Tujuan artikel ini untuk memperlihatkan bahwa dalam Yeremia 26 terdapat repetisi bertangga mengenai frase “TUHAN menyesal.” Karena jika diperhatikan secara khusus, sangat sedikit dari para penafsir menemukan adanya repetisi yang terjadi sebanyak tiga kali dalam Yeremia 26 ayat 3, 13 dan 19 mengenai frase “TUHAN menyesal.” Metode kulitatif sub-hermeneutik: Eksegesis, artikel ini menemukan adanya makna penggunaan repetisi frase “TUHAN Menyesal” dalam Yeremia 26:3, 13 dan 19 yang disebutkan oleh tiga subjek berbeda “Aku menyesal (TUHAN)”, “TUHAN menyesal (Yeremia)”, “TUHAN menyesal (para pemimpin bangsa).” Pertama, cara TUHAN menyampaikan nubuat-Nya dengan menunjukkan sebuah ekspresi emosional (anthropomorfisme) karena keberdosaan bangsa Yehuda. Kedua, nabi Yeremia menunjukkan dirinya adalah nabi sejati dan memberikan penegasan mengenai kedaultan responsif agar TUHAN membatalkan hukuman-Nya kepada bangsa Yehuda. Ketiga, para pemimpin bangsa yang teringat nubuat Mikha dan Uria, sehingga mereka tidak boleh mengabaikan pesan-Nya dan dengan itu TUHAN berubah pikiran, supaya bangsa Yehuda menerima keselamatan serta bertobat dengan berbalik kepada TUHAN yang benar.
Pendampingan Konselor Menangani Krisis Keluarga: Kasus Sonduk Hela di Suku Batak
Authors: Manullang Priska , Sihombing Sempurna , Halawa Via Epiphanis , Sagala Joyis 
Published: August 2023

This research aims to be a provision or guide for counselors in accompanying the son-in-law experiencing a family crisis the sonduk hela case the Batak tribe. The focus of the research abaut in accompanying the son-in-law experiencing family crisis the sonduk hela case the Batak tribe in village of Pegagan Julu IV. This research used qualitative methods with literature research (library research), data collection through interviews, observation of data sources, documentation and data analysis using case studies. The results of the research are first by a cross-cultural approach, as a son-in-law becomes aware of the cultural rules Toba Batak, the heir is male and has the courage to make decisions, secondly by the Pastoral Case study metode approach, the son-in-law makes events that occur around him as objective or realistic inspiration, and aware of his identity when he is with his in-laws' family. Third, by cultural counselor approach (klb), pastoral case study method (mskp), and theological approach will help the son-in-law deal with the family crisis of the sonduk hela case the Batak tribe.
Penelitian ini bertujuan menjadi bekal atau pegangan konselor dalam mendampingi menantu yang mengalami krisis keluarga kasus sonduk hela suku Batak. Fokus penelitian ialah menantu laki-laki yang mengalami krisis keluarga kasus sonduk hela suku Batak di desa Pegagan Julu IV. Penelitian ini menggunakan metode kualitatif dengan literature risearch (penelitian perpustakaan), pengumpulan data melalui Interview, Observasi sumber data, dokumentasi dan menganalisa data dengan Case study. Hasil penelitian ialah pertama melalui pendekatan lintas budaya, sebagai menantu laki-laki menjadi sadar dengan aturan budaya Batak Toba yaitu ahli waris adalah laki-laki dan berani menentukan keputusan, kedua melalui pendekatan Metode Studi Kasus Pastoral, menantu laki-laki menjadikan peristiwa yang terjadi disekitar sebagai inspirasi yang objektif atau realistis, serta menyadari jati dirinya saat bersama keluarga mertua. Ketiga, pendekatan konselor lintas budaya (klb), metode studi kasus pastoral (mskp), dan pendekatan teologi akan membatu menantu menangani krisis keluarga kasus sonduk hela di suku Batak.
Aspectos sociológicos de los videojuegos en la cultura de la niñez
Authors: Loayza Jerjes 
Published: August 2023

En la vida del niño son numerosas las influencias que se proyectan en él, tanto en su socialización primaria como en la secundaria. En efecto, los roles y funciones que va adquiriendo poco a poco en la familia y, posteriormente, en la escuela y en el barrio, juegan una importancia fundamental en la estructuración de su subjetividad y en la de su intersubjetividad para con su entorno. Se trata de una recíproca relación entre él y su contexto, en donde deberá fortalecer su seguridad para la constitución del yo, a la vez que aportará con su creatividad y compromiso al espacio social en donde se sumerge con plena intención, abocándose a su identificación y constante integración.
La niñez se ve atravesada por una performatividad que repetirá un proceso dicotómico en torno a la diferenciación social de los sexos que tanto el niño como la niña irán interiorizando bajo el rótulo de lo normal, llegando a perennizarse hasta llegar a la adultez, en donde el individuo se amalgama a una serie de rituales y convergencias de diversa índole. Vale destacar que, de acuerdo con el contexto y sociedad a la cual nos vayamos a referir, esta suerte de performatividad tendrá diversos caminos y resultados en la persona. El caso latinoamericano, por ejemplo, y con mayor particularidad el peruano, refleja el modo en que se inhiben una serie de comportamientos bajo la dicotomía de los sexos aplicados a la identidad de género, la cual resultará acaso la primera aproximación hacia lo que entendemos como socialización.
Meningkatkan hasil belajar matematika melalui implementasi model pembelajaran Jigsaw dengan memperbantukan LKPD
Authors: Nuary Rusdi Hamdany , Triyono Ageng 
Published: August 2023

Tujuan yang hendak dicapai dalam penelitian ini adalah meningkatkan persentase hasil belajar matematika siswa melalui implementasi pembelajaran kooperatif tipe jigsaw dengan memperbantukan LKPD. Penelitian ini menggunakan metode penelitian tindakan kelas (PTK) yang dilakukan dalam dua siklus. Objek penelitian dalam penelitian ini adalah hasil belajar matematika siswa siswa kelas VIII-I SMP Negeri Jakarta. Subjek penelitian terdiri dari 36 siswa, satu orang observer, dan peneliti sendiri yang bertindak sebagai guru. Data penelitian didapatkan dari lembar observasi keaktifan siswa dan instrumen soal tes. Data keaktifan siswa dianalisis menggunakan rumus persentase rerata. Data hasil tes dianalisis menggunakan rumus perhitungan ketuntasan hasil belajar, rumus rerata, dan perhitungan persentase peningkatan hasil belajar. Hasil analisis data menyimpulkan adanya peningkatan persentase pada beberapa aspek pembelajaran, yaitu; (1) keaktifan siswa dari siklus I ke siklus II meningkat sebesar 16,87%; (2) ketuntasan hasil belajar dari kondisi awal ke siklus I meningkat sebesar 66,68%, dan dari siklus I ke siklus II meningkat lagi sebesar 3,51%; (3) nilai rerata kelas dari kondisi awal ke siklus I meningkat sebesar 20,8, dan dari siklus I ke siklus II meningkat lagi sebesar 3,84. Peningkatan hasil belajar dari masing-masing siklus tersebut menunjukkan bahwa implementasi model pembelajaran kooperatif tipe jigsaw dengan memperbantukan LKPD telah berhasil dilaksanakan sesuai tujuan penelitian.
exoMMR: A New Python Package to Confirm and Characterize Mean Motion Resonances
Authors: MacDonald Mariah G. , Polania Vivas Michael S. , D’Angiolillo Skylar , Fernandez Ashley N. , Quinn Tyler 
Published: August 2023

Abstract
The study of orbital resonances allows for the constraint of planetary properties of compact systems. We can predict a system’s resonances by observing the orbital periods of the planets, as planets in or near mean motion resonance (MMR) have period ratios that reduce to a ratio of small numbers. However, a period ratio near commensurability does not guarantee a resonance; we must study the system’s dynamics and resonant angles to confirm resonance. Because resonances require in-depth study to confirm, and because two-body resonances require a measurement of the eccentricity vector which is quite challenging, very few resonant pairs or chains have been confirmed. We thus remain in the era of small-number statistics, not yet able to perform large population synthesis or informatics studies. To address this problem, we build a python package to find, confirm, and analyze MMRs, primarily through N-body simulations. We then analyze all near-resonant planets in the Kepler/K2 and TESS catalogs, confirming over 60 new resonant pairs and various new resonant chains. We additionally demonstrate the package’s functionality and potential by characterizing the mass–eccentricity degeneracy of Kepler-80g, exploring the likelihood of an exterior giant planet in Kepler-80, and constraining the masses of planets in Kepler-305. We find that our methods overestimate the libration amplitudes of the resonant angles and struggle to confirm resonances in systems with more than three planets. We identify various systems that are likely resonant chains but that we are unable to confirm, and highlight next steps for exoplanetary resonances.
Quantifying the Impact of the Dust Torque on the Migration of Low-mass Planets
Authors: Guilera Octavio M. , Benitez-Llambay Pablo , Miller Bertolami Marcelo M. , Pessah Martin E. 
Published: August 2023

Abstract
Disk solids are critical in many planet formation processes; however, their effect on planet migration remains largely unexplored. Here we assess this important issue for the first time by building on the systematic measurements of dust torques on an embedded planet by Benitez-Llambay & Pessah. Adopting standard models for the gaseous disk and its solid content, we quantify the impact of the dust torque for a wide range of conditions describing the disk/planet system. We show that the total torque can be positive and reverse inward planet migration for planetary cores with M
p ≲ 10 M
⊕. We compute formation tracks for low-mass embryos for conditions usually invoked when modeling planet formation processes. Our most important conclusion is that dust torques can have a significant impact on the migration and formation history of planetary embryos. The most important implications of our findings are as follows. (i) For nominal dust-to-gas mass ratios ϵ ≃ 0.01, low-mass planets migrate outwards beyond the water ice-line if most of the mass in the solids is in particles with Stokes numbers St ≃0.1. (ii) For ϵ ≳ 0.02–0.05, solids with small Stokes numbers, St ≃ 0.01, can play a dominant role if most of the mass is in those particles. (iii) Dust torques have the potential to enable low-mass planetary cores formed in the inner disk to migrate outwards and act as the seed for massive planets at distances of tens of au.
Observed Polarized Scattered Light Phase Functions of Planet-forming Disks
Authors: Ginski Christian , Tazaki Ryo , Dominik Carsten , Stolker Tomas 
Published: August 2023

Abstract
Dust particles are the building blocks from which planetary bodies are made. A major goal of studies of planet-forming disks is to constrain the properties of dust particles and aggregates in order to trace their origin, structure, and the associated growth and mixing processes in the disk. Observations of the scattering and/or emission of dust in a location of the disk often lead to degenerate information about the kinds of particles involved, such as the size, porosity, or fractal dimensions of aggregates. Progress can be made by deriving the full (polarizing) scattering phase function of such particles at multiple wavelengths. This has now become possible by careful extraction from scattered light images. Such an extraction requires knowledge about the shape of the scattering surface in the disk, and we discuss how to obtain such knowledge as well as the associated uncertainties. We use a sample of disk images from observations with the Very Large Telescope/SPHERE to, for the first time, extract the phase functions of a whole sample of disks with broad phase-angle coverage. We find that polarized phase functions come in two categories. Comparing the extracted functions with theoretical predictions from rigorous T-Matrix computations of aggregates, we show that one category can be linked back to fractal, porous aggregates, while the other is consistent with more compact, less porous aggregates. We speculate that the more compact particles become visible in disks where embedded planets trigger enhanced vertical mixing.
Excited Hydroxyl Outflow in the High-mass Star-forming Region G34.26 + 0.15
Authors: Tan Wei Siang , Araya Esteban D. , Rigg Cade , Hofner Peter , Kurtz Stan , Linz Hendrik , Rosero Viviana 
Published: August 2023

Abstract
G34.26 + 0.15 is a region of high-mass star formation that contains a broad range of young stellar objects in different stages of evolution, including a hot molecular core, hypercompact H ii regions, and a prototypical cometary ultracompact H ii region. Previous high-sensitivity single-dish observations by our group resulted in the detection of broad 6035 MHz OH absorption in this region; the line showed a significant blueshifted asymmetry indicative of molecular gas expansion. We present high-sensitivity Karl G. Jansky Very Large Array (VLA) observations of the 6035 MHz OH line conducted to image the absorption and investigate its origin with respect to the different star formation sites in the region. In addition, we report detection of 6030 MHz OH absorption with the VLA and further observations of 4.7 GHz and 6.0 GHz OH lines obtained with the Arecibo Telescope. The 6030 MHz OH line shows a very similar absorption profile as the 6035 MHz OH line. We found that the 6035 MHz OH line absorption region is spatially unresolved at ∼2″ scales, and it is coincident with one of the bright ionized cores of the cometary H ii region that shows broad radio recombination line emission. We discuss a scenario where the OH absorption is tracing the remnants of a pole-on molecular outflow that is being ionized inside-out by the ultracompact H ii region.
Constraining the Evolution of the Unstable Accretion Disk in SMC X-1 with NICER
Authors: Brumback McKinley C. , Vasilopoulos Georgios , Coley Joel B. , Dage Kristen , Miller Jon M. 
Published: August 2023

Abstract
Neutron star high-mass X-ray binaries with superorbital modulations in luminosity host warped inner accretion disks that occult the neutron star during precession. In SMC X-1, the instability in the warped disk geometry causes superorbital period “excursions”: times of instability when the superorbital period decreases from its typical value of 55 to ∼40 days. Disk instability makes SMC X-1 an ideal system in which to investigate the effects of variable disk geometry on the inner accretion flow. Using the high-resolution spectral and timing capabilities of the Neutron Star Interior Composition Explorer, we examined the high state of four different superorbital cycles of SMC X-1 to search for changes in spectral shape and connections to the unstable disk geometry. We performed pulse phase-averaged and phase-resolved spectroscopy to closely compare the changes in spectral shape and any cycle-to-cycle variations. While some parameters, including the photon index and absorbing column density, show slight variations with superorbital phase, these changes are most evident during the intermediate state of the superorbital cycle. Few spectral changes are observed within the high state of the superorbital cycle, possibly indicating the disk instability does not significantly change SMC X-1's accretion process.
Fermi-LAT Detection of a New Starburst Galaxy Candidate: IRAS 13052-5711
Authors: Xiang Yunchuan , Jiang Qingquan , Lan Xiaofei 
Published: August 2023

AbstractA likely starburst galaxy (SBG), IRAS 13052–5711, which is the most distant SBG candidates discovered to date, was found by analyzing 14.4 yr of data from the Fermi large-area telescope. This SBG’s significance level is approximately 6.55σin the 0.1–500 GeV band. Its spatial position is close to that of 4FGL J1308.9–5730, determined from the Fermi large telescope fourth-source Catalog (4FGL). Its power-law spectral index is approximately 2.1, and its light curve for 14.4 yr has no significant variability. These characteristics are highly similar to those of SBGs found in the past. We calculate the SBG’s star formation rate (SFR) to be 29.38M⊙yr−1, which is within the SFR range of SBGs found to date. Therefore, IRAS 13052-5711 is considered to be a likely SBG. In addition, its 0.1–500 GeV luminosity is (3.28 ± 0.67) × 1042erg s−1, which deviates from the empirical relationship of theγ-ray luminosity and the total infrared luminosity. We considered a hadronic model to explain the GeV spectrum of IRAS 13052-5711.
No Small-scale Radio Jets Here: Multiepoch Observations of Radio Continuum Structures in NGC 1068 with the VLBA
Authors: Fischer Travis C. , Johnson Megan C. , Secrest Nathan J. , Crenshaw D. Michael , Kraemer Steven B. 
Published: August 2023

Abstract
We present recent Very Long Baseline Array (VLBA) 5 GHz radio observations of the nearby, luminous Seyfert 2 galaxy NGC 1068 for comparison to similar VLBA observations made on 1997 April 26. By cross-correlating the positions of emitting regions across both epochs, we find that spatially resolved extranuclear radio knots in this system have subrelativistic transverse speeds (v ≲0.1c). We discuss sources of the observed knots and how the radio emission relates to additional phases of gas in the central ∼150 pc of this system. We suggest that the most likely explanation for the observed emission is synchrotron radiation formed by shocked host media via interactions between active galactic nucleus winds and the host environment.
Proteolipid Protein–Induced Mouse Model of Multiple Sclerosis Requires B Cell–Mediated Antigen Presentation
Authors: Wilhelm Connor R , Upadhye Mohit A , Eschbacher Kathryn L , Karandikar Nitin J , Boyden Alexander W 
Published: August 2023

Abstract
The pathogenic role B cells play in multiple sclerosis is underscored by the success of B cell depletion therapies. Yet, it remains unclear how B cells contribute to disease, although it is increasingly accepted that mechanisms beyond Ab production are involved. Better understanding of pathogenic interactions between B cells and autoreactive CD4 T cells will be critical for novel therapeutics. To focus the investigation on B cell:CD4 T cell interactions in vivo and in vitro, we previously developed a B cell–dependent, Ab-independent experimental autoimmune encephalomyelitis (EAE) mouse model driven by a peptide encompassing the extracellular domains of myelin proteolipid protein (PLPECD). In this study, we demonstrate that B cell depletion significantly inhibited PLPECD-induced EAE disease, blunted PLPECD-elicited delayed-type hypersensitivity reactions in vivo, and reduced CD4 T cell activation, proliferation, and proinflammatory cytokine production. Further, PLPECD-reactive CD4 T cells sourced from B cell–depleted donor mice failed to transfer EAE to naive recipients. Importantly, we identified B cell–mediated Ag presentation as the critical mechanism explaining B cell dependence in PLPECD-induced EAE, where bone marrow chimeric mice harboring a B cell–restricted MHC class II deficiency failed to develop EAE. B cells were ultimately observed to restimulate significantly higher Ag-specific proliferation from PLP178–191–reactive CD4 T cells compared with dendritic cells when provided PLPECD peptide in head-to-head cultures. We therefore conclude that PLPECD-induced EAE features a required pathogenic B cell–mediated Ag presentation function, providing for investigable B cell:CD4 T cell interactions in the context of autoimmune demyelinating disease.
Sporadic form of Glomerulocystic Kidney Disease in a Child: A Case Report
Authors: Kaur Navpreet , Pradeep D , Nada Ritambhra , Bhatia Anmol , Dawman Lesa , Tiewsoh Karalanglin 
Published: August 2023

Abstract
Glomerulocystic kidney disease (GCKD) is a rare form of cystic renal disease. We report a four-week-old baby girl born to non-consanguineous parents; their antenatal third-trimester ultrasound showed severe oligohydramnios that required amnioinfusion. Post-natal ultrasound examination showed few tiny cysts (2-3mm) involving the cortices in bilateral kidneys. Kidney biopsy showed dilatation of Bowman’s space and cystically dilated glomeruli, suggestive of GCKD. Whole exome sequencing revealed no pathogenic or likely pathogenic variant.