bluuebunny/crossref_metadata_2025_split huggingface dataset:
Doctor Honoris Causa Póstuma para o Irmão Marino Latore Ariño
Authors: Mentges Manuir José 
Published: July 2023

A solenidade para aquela que é a máxima distinção concedida por uma Universidade a uma autoridade acadêmica como reconhecimento de seus méritos, por si só, trata-se de um acontecimento histórico. Porém, este ato se reveste de um sentido ainda maior dada a circunstância: uma homenagem póstuma, em memória do nosso estimado Irmão, Dr. Marino.
Ir. Marino reuniu as qualidades de professor, investigador, grande líder e educador marista, reconhecido por suas competências profissionais e socioemocionais e por sua presença constante em fóruns internacionais no âmbito da Educação Superior. Sem dúvida, foi inspiração para muitas pessoas! Um homem que sempre soube compartilhar o conhecimento; afinal, de que adiantaria o conhecimento acumulado sem que estivesse a serviço do próximo? Eis o fator distintivo do nosso homenageado.
Que o seu legado nos fortaleça, para sermos uma verdadeira comunidade: uma experiência de pertença, pois estamos em comunidade cada vez que nos encontramos num lugar ao qual pertencemos. É aquele sentimento de que fazemos parte de algo que é maior do que nós. É a atitude de estar presente e encontrar o propósito mais profundo em tudo o que fazemos. É a sensação de segurança que surge de um lugar no qual nos sentimos emocionalmente, espiritualmente e psicologicamente inteiros. Foi em torno da comunidade acadêmica que o Ir. Marino construiu sua história e nos deixa um grande e significativo legado.
التأثيرات التآزرية لبعض المستخلصات النباتية والمضادات الحيوية في بكتريا Staphylococcus aureus المعزولة من البلعوم الفمي
Authors: د.الهام سعيد بنّو  
Published: July 2023

اظهرت عزلات بكتريا Staphylococcus aureusحساسية للمضادات الحيوية Trimethoprim, Ciprofloxacin) و Tetracyclin) وبنسبة [(90), (74),(50)]% على التوالي، في حين اظهرت مقاومة للمضادات الحيوية (Ampicillin,Amoxicillin, Penicillin, Oxacillin, Cephalexin, Erythromycin, Vancomycin, Gentamycin) وبنسبة (86)، (100)، (80)، (74)، (60)، (54)، (50)، (80)]% على التوالي.
تم التركيز في هذه الدراسة على المضادات البكتيرية لمجموعة من المستخلصات المائية الحارة وهي: اكليل الجبل، البابونج، البربين، الجرجير، الزعتر، الزنجبيل، القرنفل، قشور الرمان ولسان الثور، وتم التحري عن المركبات الفعالة في المستخلصات وبينت النتائج احتوائها على العديد من المركبات الفعالة مثل ( القلويدات، الكلايكوسيدات، الصابونينات، الراتنجات، الدباغيات والفلافونات).
وتم اختبار التأثيرات التآزرية بين المستخلصات النباتية المستخدمة والمضادات الحيوية Amoxicillin, Cephalexin, Erythromycin, Trimethoprim اتجاه عشرة عزلات من بكتريا S.aureusالمعزولة من منطقة البلعوم الفمي، واعطت المستخلصات تأثيرات تآزرية جيدة مع المضادات الحيوية للعزلات المختارة، كما اوضحت النتائج ان اعلى تأثير تآزري كان لمستخلص القرنفل مع مضاد Trimethoprim، الا ان مستخلص نبات لسان الثور لم يظهر تأثير تآزري مع مضادCephalexin .
New Proof of the recent Baseline Primality Conjecture
Authors: Phatak Dhananjay 
Published: July 2023

<p>I have fixed the errors in the previous version of a theoretic proof of the primality conjecture unveiled recently (see Reference [4] in the list of references in the document.).</p>
<p>The net result is a completely new proof which is correct to the best of the author's knowledge.</p>
Image Classification using Different Machine Learning Techniques
Authors: Alaba Simegnew 
Published: July 2023

<p>Artificial Neural Networks and Convolutional Neural Networks have become common tools for classification and object detection, owing to their ability to learn features without prior knowledge. During training, these networks learn the parameters, weights, and biases. This paper proposes a simple Neural Network and Convolutional Neural Network (CNN) for a classification task. Furthermore, the Bayesian neural network work is reproduced as a baseline for comparing my proposed networks. All experiments were conducted using the MNIST dataset.</p>
<p>While the simple neural networks and the convolutional networks adjust their parameters based on the cost function during training, the Bayesian convolutional neural network updates its parameters based on the backdrop that drives a variational approximation to the true posterior. Hyperparameters such as optimizer, learning rate, regularizers, dropout, epochs, etc., were varied to train the two proposed networks. The proposed networks achieved better classification accuracy, approximately 99\%, than the previously implemented Bayesian convolutional neural network. However, it is difficult to predict the certainty of the predictions made by my proposed networks, unlike Bayesian learning, which makes it easy to do so. \href{https://github.com/Simeon340703/Classification_Networks}{You can find the code for this work at}.</p>
Robot-Aided Training of Propulsion: Effects of Torque Pulses Applied to the Hip and Knee Joint Under User-Driven Treadmill Control
Authors: McGrath Robert L. , Sergi Fabrizio 
Published: July 2023

<p>We sought to establish whether torque pulses applied by an exoskeleton to the hip and knee joint modulate propulsion mechanics and whether changes in propulsion mechanics would be sustained after exposure to torque pulses under user-driven treadmill control. We applied twelve different formulations of torque pulses consecutively over 300 strides to 24 healthy participants, and quantified the evolution of four outcome measures -- gait speed (GS), hip extension (HE), trailing limb angle (TLA), normalized propulsive impulse (NPI) -- before, during, and immediately after training. We tested whether the pulse conditions modulated propulsion mechanics during and after training relative to baseline.</p>
<p>Metrics of propulsion mechanics significantly changed both during and after training. After training, HE, NPI, and GS significantly increased in eleven conditions, three conditions, and four conditions, respectively. </p>
<p>Increases in HE during and after training were observed in conjunction with hip/knee flexion pulses during early stance, or hip/knee extension during late stance. Increases in NPI during training were associated with hip/knee extension during early stance, or knee flexion during late stance. Knee flexion during early stance resulted in positive after-effects in NPI. Increases in GS were associated with the application of hip flexion pulses.</p>
<p>Conditions exhibiting the largest positive changes in HE, and not NPI, during training resulted in increased GS after training. Analysis of the relationship between the effects measured during and after training suggests that, when present, after-effects arise from retention of training effects, and that retention is specific to the component of propulsion mechanics affected by training.</p>
DEVELOPMENT OF A COFFEE DRINK WITH THE ADDITION OF SUPERFOODS
Authors: Клемешов Дмитрий Анатольевич , Назарова Алина Салаватовна , Галкин Станислав Геннадьевич 
Published: July 2023

В публикации рассмотрена разработка рецептуры напитка на основе кофе, заваренного в капельной кофеварке. Для составления купажа используются пюре бергамота и фейхоа, эфирное масло сандалового дерева, порошок мескита, порошки фиолетовой кукурузы и лукумы. Изучены физико-химические и органолептические показатели сырья и готовых напитков. Разработана технологическая схема получения напитков с суперфудами.
The publication discusses the development of a drink formulation based on coffee brewed in a drip coffee maker. To compose the blend, bergamot and feijoa puree, sandalwood essential oil, mesquite powder, purple corn and lucuma powders are used. The physicochemical and organoleptic characteristics of raw materials and finished drinks have been studied. A technological scheme for obtaining drinks with superfoods has been developed.
GLOBAL WARMING
Authors: Элинсон Мария Альбертовна , Хаидаров Раиль Данилович , Зиннатуллин Ильдар Рамилевич 
Published: July 2023

В данной статье говорится о том, что прогресс человечества привел к пренебрежению глобального потепления, которое было вызвано увеличением выбросов CO2. Это разрушает атмосферу, вызывая повышение температуры и суровые погодные условия, влияющие на производство воды и продуктов питания. Ископаемое топливо, вырубка лесов, транспорт и животноводство способствуют выбросам парниковых газов. Глобальное потепление вызывает наводнения, голод, вырубку лесов, лесные пожары и засуху, создавая серьезную угрозу человечеству.
This article says that the progress of mankind has led to the neglect of global warming, which was caused by an increase in CO2 emissions. This destroys the atmosphere, causing a rise in temperature and severe weather conditions affecting the production of water and food. Fossil fuels, deforestation, transportation and animal husbandry contribute to greenhouse gas emissions. Global warming causes floods, famine, deforestation, forest fires and drought, posing a serious threat to humanity.
CREATIVE THINKING AS METHOD AND TECHNIQUE OF FOREIGN LANGUAGE TEACHING IN AGRARIAN UNIVERSITY
Authors: Буковский Станислав Леонидович 
Published: July 2023

Настоящая статья посвящена анализу и разработке креативного способа обучения иностранному языку в аграрном вузе. Целью статьи является разработка методики обучения иностранному языку в аграрном вузе, включающей рассмотрение развития креативного мышления в качестве средства и метода обучения. В статье представлены принципы обучения и комплекс упражнений, а также критерии оценивания выполнения заданий.
The present article is devoted to the analysis and development of the creative thinking method of foreign-language teaching in agrarian higher education institution. The aim of the article is to create a method for foreign-language teaching in agrarian higher education institution, including the consideration of creative thinking development as a means and technology of teaching. The article presents the principles, exercises structure and the criteria for assessing the level of creativity of students.
THE USE OF MUSIC IN PHYSICAL EDUCATION CLASSES
Authors: Терещенко Екатерина Александровна , Лесникова Галина Николаевна 
Published: July 2023

В данной статье автор анализирует связь физической культуры и спорта с музыкой, которую применяют в ходе тренировок или при массовых занятиях физкультурой. Установлено взаимодействие этих компонентов и выявлено их влияние на физическое и психологическое положение индивида. С помощью изучения исследований обоснована необходимость применения музыки для повышения эффективности занятия физкультурой.
In this article, the author analyzes the connection of physical culture and sports with music, which is used during training or during mass physical education classes. The interaction of these components has been established and their influence on the physical and psychological situation of the individual has been revealed. Through the study of research, the necessity of using music to increase the effectiveness of physical education is justified.
ANALYSIS OF THE TRADITIONAL METHOD OF FURNITURE PRODUCTION WITH ENTERPRISES USING SMART FACTORY TECHNOLOGIES
Authors: Дмитриев Ричард Владимирович 
Published: July 2023

В данной статье автор проводит комплексное сравнение процесса производства мебели на классических фабриках с фабриками, использующих технологию smart factory. На основе данного материала выявлены преимущества перехода от классического производства к smart factory.
In this article, the author conducts a comprehensive comparison of the furniture production process in classical factories with factories using smart factory technology. Based on this material, the advantages of the transition from classical production to smart factory are revealed.
A Reexamination of Phosphorus and Chlorine Depletions in the Diffuse Interstellar Medium*
Authors: Ritchey Adam M. , Brown J. M. , Federman S. R. , Sonnentrucker Paule 
Published: July 2023

Abstract
We present a comprehensive examination of interstellar P and Cl abundances based on an analysis of archival spectra acquired with the Space Telescope Imaging Spectrograph of the Hubble Space Telescope and the Far Ultraviolet Spectroscopic Explorer. Column densities of P ii, Cl i, and Cl ii are determined for a combined sample of 107 sight lines probing diffuse atomic and molecular gas in the local Galactic interstellar medium. We reevaluate the nearly linear relationship between the column densities of Cl i and H2, which arises from the rapid conversion of Cl+ to Cl0 in regions where H2 is abundant. Using the observed total gas-phase P and Cl abundances, we derive depletion parameters for these elements, adopting the methodology of Jenkins. We find that both P and Cl are essentially undepleted along sight lines showing the lowest overall depletions. Increasingly severe depletions of P are seen along molecule-rich sight lines. In contrast, gas-phase Cl abundances show no systematic variation with molecular hydrogen fraction. However, enhanced Cl (and P) depletion rates are found for a subset of sight lines showing elevated levels of Cl ionization. An analysis of neutral chlorine fractions yields estimates for the amount of atomic hydrogen associated with the H2-bearing gas in each direction. These results indicate that the molecular fraction in the H2-bearing gas is at least 10% for all sight lines with

log
N
(

H

2

)
≳
18

and that the gas is essentially fully molecular at

log
N
(

H

2

)
≈
21

.
Chandra, HST/STIS, NICER, Swift, and TESS Detail the Flare Evolution of the Repeating Nuclear Transient ASASSN -14ko
Authors: Payne Anna V. , Auchettl Katie , Shappee Benjamin J. , Kochanek Christopher S. , Boyd Patricia T. , Holoien Thomas W.-S. , Fausnaugh Michael M. , Ashall Chris , Hinkle Jason T. , Vallely Patrick J. , Stanek K. Z. , Thompson Todd A. 
Published: July 2023

Abstract
ASASSN-14ko is a nuclear transient at the center of the AGN ESO 253−G003 that undergoes periodic flares. Optical flares were first observed in 2014 by the All-Sky Automated Survey for Supernovae (ASAS-SN) and their peak times are well-modeled with a period of

115.2

−
1.2

+
1.3

days and period derivative of −0.0026 ± 0.0006. Here we present ASAS-SN, Chandra, HST/STIS, NICER, Swift, and TESS data for the flares that occurred on 2020 December, 2021 April, 2021 July, and 2021 November. These four flares represent flares 18–21 of the total number of flares observed by ASAS-SN so far since 2014. The HST/STIS UV spectra evolve from blueshifted broad absorption features to redshifted broad emission features over ∼10 days. The Swift UV/optical light curves peaked as predicted by the timing model, but the peak UV luminosities that varied between flares and the UV flux in Flare 20 were roughly half the brightness of the other peaks. The X-ray luminosities consistently decreased and the spectra became harder during the UV/optical rise, but apparently without changes in absorption. Finally, two high-cadence TESS light curves from Flare 18 and Flare 12 showed that the slopes during the rising and declining phases changed over time, which indicates some stochasticity in the flare’s driving mechanism. Although ASASSN-14ko remains observationally consistent with a repeating partial tidal disruption event, these rich multi-wavelength data are in need of a detailed theoretical model.
Theoretical Light-curve Models of the Symbiotic Nova CN Cha—Optical Flat Peak for 3 Yr
Authors: Kato Mariko , Hachisu Izumi 
Published: July 2023

Abstract
CN Cha is a slow symbiotic nova characterized by a 3 yr long optical flat peak followed by a rapid decline. We present theoretical light curves for CN Cha, based on hydrostatic approximation, and estimate the white-dwarf (WD) mass to be ∼0.6 M
☉ for a low metal abundance of Z = 0.004. These kinds of flat-peak novae are border objects between classical novae having a sharp optical peak and extremely slow novae, the evolutions of which are too slow to be recognized as nova outbursts on a human timescale. Theoretically, there are two types of nova envelope solutions—static and optically thick wind—in low-mass WDs (≲0.7 M
☉). Such a nova outburst begins first in a hydrostatic manner, and later it could change to an optically thick wind evolution, due to perturbation by the companion star in the nova envelope. Multiple peaks are a reflection of the relaxation process of the transition. CN Cha supports our explanation of the difference between long-lasting flat-peak novae like CN Cha and multiple-peak novae like V723 Cas, because the companion star is located far outside, and does not perturb, the nova envelope in CN Cha.
Discovery and Timing Analysis of New Pulsars in Globular Cluster NGC 5024: New Observations from FAST
Authors: Lian Yujie , Pan Zhichen , Zhang Haiyan , Freire P. C. C. , Cao Shuo , Qian Lei 
Published: July 2023

Abstract
The most distant globular cluster (GC) with known pulsars is NGC 5024 (M53). In this paper, we report the discovery of a new binary millisecond pulsar, PSR J1312+1810E (M53E), and present the new timing solutions for M53B–E based on 22 observations from the Five-hundred-meter Aperture Spherical radio Telescope (FAST). These discoveries and timing work benefit from FAST’s high sensitivity. We find that M53C is the only isolated millisecond pulsar known in this distant GC, with a spin period of 12.53 ms and spin period derivative of 5.26 × 10−20 s s−1. Our results reveal orbital periods of 47.7, 5.8, and 2.4 days for M53B, D, and E, respectively. The companions, with masses of 0.25, 0.27, and 0.18 M
⊙, respectively, are likely to be white dwarf stars; if they are extended objects, they do not eclipse the pulsars. We find no X-ray counterparts for these millisecond pulsars in archival Chandra images in the band of 0.3–8 keV. The characteristics of this pulsar population are similar to the population of millisecond pulsars in the Galactic disk, as expected from the low stellar density of M53.
Ryugu’s Anhydrous Ingredients and Their Spectral Link to Primitive Dust from the Outer Solar System
Authors: Brunetto R. , Lantz C. , Fukuda Y. , Aléon-Toppani A. , Nakamura T. , Dionnet Z. , Baklouti D. , Borondics F. , Djouadi Z. , Rubino S. , Amano K. , Matsumoto M. , Fujioka Y. , Morita T. , Kukuiri M. , Kagawa E. , Matsuoka M. , Milliken R. , Yurimoto H. , Noguchi T. , Okazaki R. , Yabuta H. , Naraoka H. , Sakamoto K. , Tachibana S. , Yada T. , Nishimura M. , Nakato A. , Miyazaki A. , Yogata K. , Abe M. , Okada T. , Usui T. , Yoshikawa M. , Saiki T. , Tanaka S. , Terui F. , Nakazawa S. , Watanabe S. , Tsuda Y. 
Published: July 2023

Abstract
Ryugu is a second-generation C-type asteroid formed by the reassembly of fragments of a previous larger body in the main asteroid belt. While the majority of Ryugu samples returned by Hayabusa2 are composed of a lithology dominated by aqueously altered minerals, clasts of pristine olivine and pyroxene remain in the least-altered lithologies. These clasts are objects of great interest for revealing the composition of the dust from which the original building blocks of Ryugu's parent asteroid formed. Here we show that some grains rich in olivine, pyroxene, and amorphous silicates discovered in one millimeter-sized stone of Ryugu have infrared spectra similar to the D-type asteroid Hektor (a Jupiter Trojan), to comet Hale–Bopp, and to some anhydrous interplanetary dust particles of probable cometary origin. This result indicates that Ryugu's primary parent body incorporated anhydrous ingredients similar to the building blocks of asteroids (and possibly some comets) formed in the outer solar system, and that Ryugu retained valuable information on the formation and evolution of planetesimals at different epochs of our solar system's history.
Jetted and Turbulent Stellar Deaths: New LVK-detectable Gravitational-wave Sources
Authors: Gottlieb Ore , Nagakura Hiroki , Tchekhovskoy Alexander , Natarajan Priyamvada , Ramirez-Ruiz Enrico , Banagiri Sharan , Jacquemin-Ide Jonatan , Kaaz Nick , Kalogera Vicky 
Published: July 2023

Abstract
Upcoming LIGO–Virgo–KAGRA (LVK) observing runs are expected to detect a variety of inspiralling gravitational-wave (GW) events that come from black hole and neutron star binary mergers. Detection of noninspiral GW sources is also anticipated. We report the discovery of a new class of noninspiral GW sources—the end states of massive stars—that can produce the brightest simulated stochastic GW burst signal in the LVK bands known to date, and could be detectable in LVK run A+. Some dying massive stars launch bipolar relativistic jets, which inflate a turbulent energetic bubble—cocoon—inside of the star. We simulate such a system using state-of-the-art 3D general relativistic magnetohydrodynamic simulations and show that these cocoons emit quasi-isotropic GW emission in the LVK band, ∼10–100 Hz, over a characteristic jet activity timescale ∼10–100 s. Our first-principles simulations show that jets exhibit a wobbling behavior, in which case cocoon-powered GWs might be detected already in LVK run A+, but it is more likely that these GWs will be detected by the third-generation GW detectors with an estimated rate of ∼10 events yr−1. The detection rate drops to ∼1% of that value if all jets were to feature a traditional axisymmetric structure instead of a wobble. Accompanied by electromagnetic emission from the energetic core-collapse supernova and the cocoon, we predict that collapsars are powerful multimessenger events.
Millimeter Observations of the Type II SN 2023ixf: Constraints on the Proximate Circumstellar Medium
Authors: Berger Edo , Keating Garrett K. , Margutti Raffaella , Maeda Keiichi , Alexander Kate D. , Cendes Yvette , Eftekhari Tarraneh , Gurwell Mark , Hiramatsu Daichi , Ho Anna Y. Q. , Laskar Tanmoy , Rao Ramprasad , Williams Peter K. G. 
Published: July 2023

Abstract
We present 1.3 mm (230 GHz) observations of the recent and nearby Type II supernova, SN 2023ixf, obtained with the Submillimeter Array (SMA) at 2.6–18.6 days after explosion. The observations were obtained as part the SMA Large Program, POETS (Pursuit of Extragalactic Transients with the SMA). We do not detect any emission at the location of SN 2023ixf, with the deepest limits of L

ν
(230 GHz) ≲ 8.6 × 1025 erg s−1 Hz−1 at 2.7 and 7.7 days, and L

ν
(230 GHz) ≲ 3.4 × 1025 erg s−1 Hz−1 at 18.6 days. These limits are about a factor of 2 times dimmer than the millimeter emission from SN 2011dh (IIb), about 1 order of magnitude dimmer compared to SN 1993J (IIb) and SN 2018ivc (IIL), and about 30 times dimmer than the most luminous nonrelativistic SNe in the millimeter band (Type IIb/Ib/Ic). Using these limits in the context of analytical models that include synchrotron self-absorption and free–free absorption, we place constraints on the proximate circumstellar medium around the progenitor star, to a scale of ∼2 × 1015 cm, excluding the range

M

̇

∼
few
×

10

−
6

−

10

−
2

M
⊙ yr−1 (for a wind velocity, v

w
= 115 km s−1, and ejecta velocity, v
ej ∼ (1 − 2) × 104 km s−1). These results are consistent with an inference of the mass-loss rate based on optical spectroscopy (∼2 × 10−2
M
⊙ yr−1 for v

w
= 115 km s−1), but are in tension with the inference from hard X-rays (∼7 × 10−4
M
⊙ yr−1 for v

w
= 115 km s−1). This tension may be alleviated by a nonhomogeneous and confined CSM, consistent with results from high-resolution optical spectroscopy.