bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGEMBANGAN TEKNOLOGI PENGENALAN WAJAH PADA SISTEM TIKET KAPAL SEBAGAI SOLUSI OPTIMAL UNTUK MENGURANGI ANTRIAN BOARDING PASS
Authors: Muhammad Abdul Haris , Mandar Gamaria , Irwan Risman 
Published: October 2024

Dua metode utama yang digunakan dalam penelitian ini adalah Local Binary Pattern Histogram (LBPH) dan Haar Cascade. Total data yang digunakan adalah 1.500 citra wajah, dengan 1.000 data latih dan 500 data uji. Setiap citra memiliki ukuran dimensi 200 x 200 piksel, dan diambil pada jarak 30 cm dari subjek. Metode LBPH digunakan untuk mengekstraksi ciri dari setiap citra wajah, di mana metode ini sangat efisien dalam mendeteksi pola tekstur lokal pada citra wajah. Sementara itu, metode Haar Cascade digunakan untuk melakukan deteksi wajah dengan cepat berdasarkan pemrosesan tingkat awal, yang memungkinkan sistem untuk memetakan fitur penting pada wajah. Pengujian dilakukan dengan menggunakan algoritma gabungan ini menggunakan bahasa pemrograman python, jupyter noteboo untuk meningkatkan efisiensi dan akurasi dalam proses pengenalan. Hasil penelitian menunjukkan bahwa sistem ini mampu mengidentifikasi penumpang hanya dalam rentang waktu antara 6 detik hingga 1 menit saat proses boarding pass. Tingkat akurasi yang dicapai adalah 97%, yang membuktikan bahwa sistem pengenalan wajah ini sangat efektif dalam mempersingkat waktu antrean penumpang di pelabuhan. Berdasarkan hasil tersebut, dapat disimpulkan bahwa teknologi pengenalan wajah menggunakan kombinasi metode LBPH dan Haar Cascade merupakan solusi yang efisien dan akurat untuk mengurangi antrian proses boarding pass.Kata Kunci: Pengenalan Wajah, E-Tiket, Pulau Bacan, Pelabuhan Babang
Ambliopia em crianças: Classificação, triagem e avaliação
Authors: Antônio Ramos dos Santos João , Silva Fasciani Júlia , Almeida Viana Evelise , Da Silva Rocha Ana Carolina 
Published: October 2024

Introdução: Ambliopia é uma redução funcional na acuidade visual causada por desenvolvimento visual anormal no início da vida. É uma consequência secundária de distúrbio visual precoce por estrabismo ou outras condições indutoras de ambliopia durante o período crítico para o desenvolvimento visual. Objetivos: discutir a ambliopia em crianças e sua classificação, triagem e avaliação. Metodologia: Revisão de literatura integrativa a partir de bases científicas de dados da Scielo, da PubMed e da BVS, no período de janeiro a abril de 2024, com os descritores "Amblyopia", "Child", AND "Classification". Incluíram-se artigos de 2019-2024 (total 34), com exclusão de outros critérios e escolha de 05 artigos na íntegra. Resultados e Discussão: A ambliopia é classificada em três tipos principais com base na condição subjacente que induz a ambliopia: estrabismo, causado pelo alinhamento anormal dos olhos; refrativa, causada por foco desigual entre os olhos ou erro refrativo grave não corrigido em ambos os olhos; ; privação, causada por anormalidades estruturais do olho que obscurecem as imagens recebidas. Todas as crianças <5 anos devem passar por uma triagem da visão de rotina para detectar ambliopia. A detecção precoce e o tratamento da ambliopia melhoram o prognóstico para o desenvolvimento normal da visão. A triagem inclui avaliação do risco de visão em todas as visitas de manutenção da saúde e triagem da visão aos três, quatro e cinco anos de idade. Deve-se suspeitar de ambliopia se a visão nos dois olhos for desigual ou se a criança tiver uma condição indutora de ambliopia (por exemplo, estrabismo, erro refrativo assimétrico, catarata, ptose). O teste usado para diagnosticar ambliopia depende da idade da criança. Em crianças pré-verbais, a assimetria da visão pode ser indicada por um reflexo de fixação anormal ou teste de objeção de oclusão. Em crianças mais velhas, a visão assimétrica é detectada por meio de testes formais de acuidade visual. Crianças com suspeita de ambliopia devem ser encaminhadas a um oftalmologista ou optometrista que seja adequadamente treinado e experiente no tratamento de crianças. Os critérios para encaminhamento incluem: acuidade visual pior que 20/40 em uma criança de 3 a 5 anos de idade ou pior que 20/30 em uma criança ≥6 anos, diferença de acuidade visual de ≥2 linhas entre os olhos em um gráfico de visão padrão (por exemplo, 20/30 no olho esquerdo e 20/40 no direito); alinhamento ocular anormal (ou seja, estrabismo); reflexo vermelho anormal; assimetria da visão (preferência ocular;) ptose unilateral ou outras lesões que ameaçam o eixo visual (por exemplo, hemangioma palpebral. Conclusão: Ambliopia é a redução funcional na acuidade visual causada por desenvolvimento visual anormal no início da vida. É uma consequência secundária de distúrbio visual precoce durante o período crítico para o desenvolvimento visual.
Justification of the design and technological scheme of a new type of machine for applying mineral fertilizers
Authors:   INSTITUTE of MECHANICS and AUTOMATICS of AGROINDUSTRIAL PRODUCTION of the NATIONAL ACADEMY of AGRARIAN SCIENCES of UKRAINE, Adamchuk V. , Vitruh P. ,   INSTITUTE of MECHANICS and AUTOMATICS of AGROINDUSTRIAL PRODUCTION of the NATIONAL ACADEMY of AGRARIAN SCIENCES of UKRAINE, Adamchuk О. ,   INSTITUTE of MECHANICS and AUTOMATICS of AGROINDUSTRIAL PRODUCTION of the NATIONAL ACADEMY of AGRARIAN SCIENCES of UKRAINE
Published: October 2024

Annotation Purpose. Rationale for the structural and technological scheme of the transport-technological machine for the application of solid mineral fertilizers, which will ensure the improvement of the quality of the application of mineral fertilizers by stabilizing the dose of their application as the body of the machine is emptied and its annual load increases. Methods. Analysis of known designs of machines for applying solid mineral fertilizers, theoretical based on the laws of mechanics and experimental using standard methods. Results. The structural and technological scheme of a new type of machine for applying mineral fertilizers and dependencies for determining the main parameters and modes of operation of its working bodies are substantiated. Its experimental sample was created, the results of which in the process of laboratory and field studies confirmed the independence of the dose of mineral fertilizers from the filling (emptying) of the car body with mineral fertilizers. In addition, the possibility of using the machine in the operations of transporting loose technological materials and transshipping them to other technical means and stationary capacities, as well as unloading to the site, was confirmed, which ensured an increase in its annual loading by more than 4 times. Conclusions. The creation of body-type machines for applying solid mineral fertilizers according to the principle of transport-technological machines, which include a body equipped with a feeder, a screw conveyor, a hopper with a dispenser and sorting working bodies, ensures: -	exclusion of the influence of the degree of filling (emptying) of the body machines with mineral fertilizers for the dose of their introduction; -	expansion of the scope of application of the machine thanks to its additional use in transportation operations of loose technological materials and their transshipment into other technical means and stationary capacities, as well as unloading at the site, which in general leads to an increase in its annual loading more than 4 times.
1-жасқа дейінгі балалардағы сарғаю синдромының диагностикасын алғашқы медико-санитарлық көмек деңгейінде оңтайландыру: әдебиетке шолу
Authors: Исаева Г.А. , Сейсебаева Р.Ж. , Нургалиева Ж.Ж. 
Published: October 2024

Өзектілігі: Жаңа туған нәрестелер мен жаңа туған нәрестелер өмірінің алғашқы тәуліктерінде кездесетін сарғыштық синдромын зерттеу өте маңызды. 1-жасқа дейінгі балалардағы сарғаю синдромын уақытылы диагностикалау көптеген асқынулардың алдын алады. Жаңа туған нәрестелер мен жалпы нәрестелердің алғашқы айларында сарғаю синдромы табиғи физиологиялық (толық туған нәрестелерде 2 аптаға дейін және шала туылған нәрестелерде 3 аптаға дейін) және патологиялық (туған кезден бастап алғашқы екі күннен бір айдан астам уақытқа дейін). Сарғаюды дер кезінде диагностикалап, емдеу өскелең ұрпақтың дені сау болып өсуінің кепілі.
Зерттеудің мақсаты – ерте балалық шақтағы сарғаю синдромының қауіп факторлары мен диагностикалық маңыздылығы туралы ағымдағы деректерді жинақтау.
Материалдар мен әдістері: NCBI (PubMed), Scopus, Medline, Google Scholar, CyberLeninka және eLibrary дерекқорларындағы 2014-2024 жылдар аралығындағы отандық және шетелдік басылымдарға шолу жүргізілді. Ғылыми зерттеу нәтижелерін іздеуде мындай түйінді сөздер қолданылды: «сарғаю», «неонатальді сарғаю», «гипербилирубинемия», «холестаз», «гепатит», «жаңа туған нәресте». Іздеу кілт сөздерді қолдана отырып, MESH іздеу құралы арқылы жүргізілді.
Нәтижелері: Кішкентай балалардағы сарғаю ауыр асқынулардың алдын алу үшін ерте анықтауды және тиісті емдеуді қажет етеді. Жалпы біздің ғылыми әдебиеттерден жинақтағанымыз жаңа туған нәрестелер мен ерте жастағы балалар арасындағы сарғаю синдромының қауіп факторлеріне: жүкті әйелдің жүктілік кезеңіндегі қосалқы аурулары (ЖРВИ, гестационды диабет, қаназдық), босану барысында жүргізілген эпизиотомия,сусыз кезеңнің ұзаққа созылуы,баланың ана сүтінің сары уызымен алғашқы тәуліктерде жеткілікті дәрежеде қоректенуі сияқты себептер тікелей әсер етеді. Жаңа туған нәрестелер мен нәресте өмірінің алғашқы айларында кездесетін сарғаюдың Ерте жастағы балалардағы сарғаюдың себеп-салдарын, диагностикасын дер кезінде емдеу әдістерін қолдану медицина мамандары соның ішінде участкілік дәрігерлер мен медбикелердің жұмысын едәуір оңтайландырады.
Қорытынды: Соңғы зерттеулер сарғаю синдромы бір жасқа дейінгі балаларда, әсіресе жаңа туған нәрестелерде жиі кездесетінін көрсетеді. Сарғаюды ерте анықтау ықтимал ұзақ мерзімді асқынулардың алдын алады. Сары ауруды диагностикалау мен емдеуді жақсарту және зардап шеккен балаларда ұзақ мерзімді асқынулардың жиілігін азайту үшін қосымша зерттеулер қажет.
Gender en asiel: "zelfstandige" mannen en "afhankelijke" vrouwen
Authors: Peter Mascini , Marjolein Van Bochove 
Published: October 2024

Terwijl de aandacht voor de achterstelling van vrouwen in de asielprocedure de afgelopen decennia groeit, blijkt dat juist mannen hierin een kleinere slaag?kans hebben. Dit blijkt te maken te hebben met het traditionele gendermigratie patroon en de hieraan gekoppelde typering van mannen als calculerende gelukszoekers en van vrouwen als slachtoffers van patriarchale overheersing.
High-latitude Observations of Dissipation-range Turbulence by the Ulysses Spacecraft during the Solar Minimum of 1993–96: The Spectral Break and Anisotropy
Authors: Watson Abigale S. , Smith Charles W. , Marchuk Anastasia V. , Argall Matthew R. , Joyce Colin J. , Isenberg Philip A. , Vasquez Bernard J. , Schwadron Nathan A. , Murphy Neil 
Published: October 2024

Abstract
We examine Ulysses magnetic field observations from 1993 to 1996 as the spacecraft made its first fast-latitude scan from the southern to the northern hemisphere. Most of the observations we use are representative of high-latitude solar minimum conditions. We examine magnetic field power spectra characteristics of interplanetary turbulence at high frequencies, where the spectrum breaks from an inertial range into the ion dissipation range. The onset and spectral index of the dissipation spectrum are consistent with low-latitude observations at 1 au. Both ranges have a ratio of power in perpendicular magnetic field components to parallel components near 3. The power spectrum ratio test developed by Bieber et al. for single-spacecraft analyses that determines the underlying anisotropy of the wave vectors yields only marginally more energy associated with field-aligned wave vectors than perpendicular wave vectors when comparing the inertial and dissipation-range spectra. The lack of significant change in the anisotropies between the inertial and dissipation ranges contrasts strongly with the turbulence found typically for 1 au near-ecliptic observations, where significant differences in both anisotropies are observed.
The JWST UNCOVER Treasury Survey: Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization
Authors: Bezanson Rachel , Labbe Ivo , Whitaker Katherine E. , Leja Joel , Price Sedona H. , Franx Marijn , Brammer Gabriel , Marchesini Danilo , Zitrin Adi , Wang 王 Bingjie 冰洁 , Weaver John R. , Furtak Lukas J. , Atek Hakim , Coe Dan , Cutler Sam E. , Dayal Pratika , van Dokkum Pieter , Feldmann Robert , Förster Schreiber Natascha M. , Fujimoto Seiji , Geha Marla , Glazebrook Karl , de Graaff Anna , Greene Jenny E. , Juneau Stéphanie , Kassin Susan , Kriek Mariska , Khullar Gourav , Maseda Michael , Mowla Lamiya A. , Muzzin Adam , Nanayakkara Themiya , Nelson Erica J. , Oesch Pascal A. , Pacifici Camilla , Pan Richard , Papovich Casey , Setton David J. , Shapley Alice E. , Smit Renske , Stefanon Mauro , Taylor Edward N. , Williams Christina C. 
Published: October 2024

Abstract
In this paper we describe the survey design for the Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization (UNCOVER) Cycle 1 JWST Treasury program, which executed its early imaging component in 2022 November. The UNCOVER survey includes ultradeep (∼29–30AB) imaging of ∼45 arcmin2 on and around the well-studied A2744 galaxy cluster at z = 0.308 and will follow up ∼500 galaxies with extremely deep low-resolution spectroscopy with the NIRSpec/PRISM during the summer of 2023, with repeat visits in summer 2024. We describe the science goals, survey design, target selection, and planned data releases. We also present and characterize the depths of the first NIRCam imaging mosaic, highlighting previously unparalleled resolved and ultradeep 2–4 μm imaging of known objects in the field. The UNCOVER primary NIRCam mosaic spans 28.8 arcmin2 in seven filters (F115W, F150W, F200W, F277W, F356W, F410M, and F444W) and 16.8 arcmin2 in our NIRISS parallel (F115W, F150W, F200W, F356W, and F444W). To maximize early community use of the Treasury data set, we publicly release the full reduced mosaics of public JWST imaging including 45 arcmin2 NIRCam and 17 arcmin2 NIRISS mosaics on and around the A2744 cluster, including the Hubble Frontier Field primary and parallel footprints.
Multipolar Electromagnetic Emission of Newborn Magnetars
Authors: Wang Yu , Moradi Rahim , Li Liang 
Published: October 2024

Abstract
It is generally recognized that the electromagnetic multipolar emission from magnetars can be used to explain radiation from soft gamma repeaters or anomalous X-ray pulsars, but they have little impact on the spin-down of magnetars. We here present an analytical solution for the neutron star multipolar electromagnetic fields and their associated expected luminosities. We find that for newborn millisecond magnetars, the spin-down luminosity from higher multipolar components can match or even exceed that from the dipole component. Such high-intensity radiation will undoubtedly affect related astrophysical phenomena at the birth of a magnetar. We show that the spin-down luminosity from multipoles can well explain the majority of gamma-ray burst (GRB) afterglows, from the plateau starting at several hundred seconds until the normal decay phase lasting for many years. The fitted magnetar parameters for GRB afterglows are all typical values, with spins in the millisecond range and magnetic field strengths on the order of 1014–1015 G. Our results, in turn, provide support for the hypothesis that GRBs originate from the birth of magnetars with a period of a few milliseconds, thus deepening our understanding of the complex magnetic field structure and the equation of state of magnetars.
Determining the Interstellar Wind Longitudinal Inflow Evolution Using Pickup Ions in the Helium Focusing Cone
Authors: Spitzer Sarah A. , Lepri Susan T. , Raines Jim M. , Gilbert Jason A. , Bower Jonathan , Dewey Ryan M. , Möbius Eberhard 
Published: October 2024

Abstract
The size, shape, and composition of the heliosphere are affected by its interaction with the local interstellar medium. A means of quantifying this interaction is by measuring the relative motion of the two media. We determine the flow direction,

λ
ISN

, of the interstellar wind through the heliosphere and its trend over an 11 yr solar cycle using Advanced Composition Explorer/Solar Wind Ion Composition Spectrometer He+ double-coincidence pickup ion (PUI) measurements from a data set spanning 13 full orbits, with focusing cone crossings occurring between the years 1998 and 2010. We measure the flow direction by fitting a kappa function to the focusing cone signature in the count rates of He+ at the PUI cutoff measured as a function of ecliptic longitude. We determine

λ
ISN

for each three-orbit boxcar centered on the years 1999 through 2009 and find the trend of the resulting linear fit. We account for solar transients by removing measurements associated with CMEs. However, there still may be effects from compression regions, such as stream–stream and corotating interaction regions. We additionally make considerations to ensure the PUI torus is in view, to account for varying interplanetary magnetic field angles, to ensure that we analyze newly injected interstellar PUIs largely unaffected by transport effects, and to account for general solar activity. We measure a slope in the flow direction to be 0.00° ± 0.51°​​​​ yr−1, indicating that we do not measure a varying trend over this period. We repeat the focusing cone analysis for the combined data set and determine an overall flow direction of 75.37° ± 0.43°.
What Are the Pillars of Reionization? Revising the AGN Luminosity Function at z ∼ 5
Authors: Grazian Andrea , Giallongo Emanuele , Boutsia Konstantina , Cristiani Stefano , Fontanot Fabio , Bischetti Manuela , Bisigello Laura , Bongiorno Angela , Calderone Giorgio , Chiti Tegli Francesco , Cupani Guido , De Lucia Gabriella , D’Odorico Valentina , Feruglio Chiara , Fiore Fabrizio , Gandolfi Giovanni , Girardi Giorgia , Guarneri Francesco , Hirschmann Michaela , Porru Matteo , Rodighiero Giulia , Saccheo Ivano , Simioni Matteo , Trost Andrea , Viitanen Akke 
Published: October 2024

Abstract
In the past, high-z active galactic nuclei (AGNs) were given a minor role as possible drivers of reionization, despite initial evidence in favor of their large space densities at low luminosities by Chandra and the Hubble Space Telescope. Recent observations from JWST are finding relatively large numbers of faint AGNs at z > 4, convincingly confirming these early results. We present a sample of z ∼ 5 AGNs, both from wide, shallow ground-based surveys and from deep, pencil-beam observations from JWST, allowing us to estimate their space densities with unprecedented accuracy. The bright end (M
1450 < −26) of the z ∼ 5 AGN luminosity function is well constrained, with a rather steep slope. The faint end (M
1450 ≥ −22) indicates a high space density, the scatter is significant, and the knee (M
1450 ∼ −24) is mostly undetermined. Comparisons with state-of-the-art models find reasonable agreement with the observed AGN luminosity function at z = 5, while the predicted space density evolution at higher redshifts appears to be too fast with respect to observational constraints. Given the large variance at the faint end, we consider different options in fitting the luminosity functions and deriving the ionizing emissivity. Even in the most conservative scenario, the photoionization rate produced by z ∼ 5 AGNs is consistent with the ultraviolet background measurements. A slow evolution of the space density of faint AGNs is observed, indicating that active SMBHs are probably producing large amounts of ionizing photons at z > 6, well into the Epoch of Reionization. This is an important indication that high-z AGNs could be major contributors to the reionization of the Universe.
Detection of Dimethyl Ether in the Central Region of the MWC 480 Protoplanetary Disk
Authors: Yamato Yoshihide , Aikawa Yuri , Guzmán Viviana V. , Furuya Kenji , Notsu Shota , Cataldi Gianni , Öberg Karin I. , Qi Chunhua , Law Charles J. , Huang Jane , Teague Richard , Le Gal Romane 
Published: October 2024

Abstract
Characterizing the chemistry of complex organic molecules (COMs) at the epoch of planet formation provides insights into the chemical evolution of the interstellar medium (ISM) and the origin of organic materials in our solar system. We report a detection of dimethyl ether (CH3OCH3) in the disk around the Herbig Ae star MWC 480 with sensitive Atacama Large Millimeter/submillimeter Array observations. This is the first detection of CH3OCH3 in a nontransitional Class II disk. The spatially unresolved, compact (≲25 au in radius) nature, broad line width (∼30 km s−1), and high excitation temperature (∼200 K) indicate the sublimation of COMs in the warm inner disk. Despite the detection of CH3OCH3, methanol (CH3OH), the most abundant COM in the ISM, has not been detected, from which we constrain the column density ratio of CH3OCH3/CH3OH ≳ 7. This high ratio may indicate the reprocessing of COMs during the disk phase, as well as the effect of the physical structure in the inner disk. We also find that this ratio is higher than in COM-rich transition disks recently discovered. This may indicate that in the full disk of MWC 480, COMs have experienced substantial chemical reprocessing in the innermost region, while the COM emission in the transition disks predominantly traces the inherited ice sublimating at the dust cavity edge located at larger radii (≳20 au).
Repeating Nuclear Transients from Repeating Partial Tidal Disruption Events: Reproducing ASASSN-14ko and AT2020vdq
Authors: Bandopadhyay Ananya , Coughlin Eric R. , Nixon C. J. , Pasham Dheeraj R. 
Published: October 2024

Abstract
Some electromagnetic outbursts from the nuclei of distant galaxies have been found to repeat on months-to-years timescales, and each of these sources can putatively arise from the accretion flares generated through the repeated tidal stripping of a star on a bound orbit about a supermassive black hole (SMBH), i.e., a repeating partial tidal disruption event (rpTDE). Here, we test the rpTDE model through analytical estimates and hydrodynamical simulations of the interaction between a range of stars, which differ from one another in mass and age, and an SMBH. We show that higher-mass (≳1M
⊙), evolved stars can survive many (≳10−100) encounters with an SMBH while simultaneously losing few × 0.01M
⊙, resulting in accretion flares that are approximately evenly spaced in time with nearly the same amplitude, quantitatively reproducing ASASSN-14ko. We also show that the energy imparted to the star via tides can lead to a change in its orbital period that is comparable to the observed decay in the recurrence time of ASASSN-14ko’s flares,

P

̇

≃
−
0.0026

. Contrarily, lower-mass and less-evolved stars lose progressively more mass and produce brighter accretion flares on subsequent encounters for the same pericenter distances, leading to the rapid destruction of the star and cessation of flares. Such systems cannot reproduce ASASSN-14ko-like transients, but are promising candidates for recreating events such as AT2020vdq, which displayed a second and much brighter outburst compared to the first. Our results imply that the lightcurves of repeating transients are tightly coupled with stellar type.