bluuebunny/crossref_metadata_2025_split huggingface dataset:
eNeuron Project – Facilitating the Energy Transition in a Military Campus by optimizing a Local Energy Community
Authors: Cardoso Carlos , Oliveira Rodrigues Rafael , Cunha Gomes Francisco , Piedade João Lourenço , Mendes Gisela , Figueiredo Raquel , Martins Rui , Cabral Diogo 
Published: October 2023

<p>The eNeuron project is an ongoing Horizon 2020 EU-funded project with the main objective of setting out a practical framework for optimising the design and operation of local energy communities (LECs), acting as multi-carrier energy hubs (EH) and micro-energy hubs (mEH). LECs are key in the transition towards green, decarbonised power from local and renewable sources. The consortium is developing and applying pioneering software and hardware solutions, putting them to the test in real energy communities and introducing new governance models.</p>
<p>There are four demonstration Pilots in the eNeuron Project: The Polish City of Bydgoszcz, the Skagerak Energilab in Norway, the Lisbon Naval Base (LNB) in Portugal, and the UNIVPM University Campus in Italy. </p>
<p>This paper focuses on presenting the Portuguese demo pilot: the Lisbon Naval Base, namely the development of the demonstration activities so far, roughly half of the duration of the project, as well as a balance of all supporting activities, such as Use Case definition, technical activities (asset definition and installation) and social activities (stakeholder engagement). This paper presents a description and conclusion of these activities so far, at the time that the eNeuron preliminary toolbox concept is ready to be shared and implemented in the Pilots.</p>
ASPECTOS E INTERFACES ECONÔMICAS E SOCIOCULTURAIS NA PREVENÇÃO DO CÂNCER DE PRÓSTATA E PÊNIS
Authors: Machado Gabriel Rodrigues de Souza , Ribeiro Wanderson Alves , Santiago Osvaldo Domingues , Costa Sidney Silvino da , Batista Paula Leite , Azeredo Daniel Reymol , Reis Elcio Gomes dos , Costa Thamires Vaz , Miranda Meg Belo , Neves Felippe Gomes de Oliveira , Fassarella Bruna Porath Azevedo , Neves Keila do Carmo 
Published: October 2023

Introdução: O câncer pode surgir quando ocorre uma alteração no DNA de uma célula que começa a se multiplicar de forma desorganizada na qual é denominada como carcinogênese ou oncogênese, que dá origem aos diversos tipos de carcinoma. Essas questões sociais e culturais dificultam o acesso dos homens a medidas de detecção e tratamento precoce, resultando em um maior risco de complicações e até mesmo de óbitos relacionados a doenças evitáveis. Objetivo: Analisar e Revisar artigos e manuais sobre a influência e os aspectos socioculturais correlacionando a medidas preventivas do câncer de próstata e pênis. Metodologia: revisão bibliográfica de caráter descritivo e abordagem qualitativa, com análise de literaturas científicas que nos remetam ao objeto de pesquisa, selecionanda da literatura, artigos completos, publicados em português, no período de 2017-2022, e os critérios de exclusão os artigos repetidos, publicações com textos indisponíveis, fora da língua vernácula e estudos com mais de 5 anos de publicação, fora do recorte temporal. Análise e discussão dos resultados: Culturalmente o homem é visto como o símbolo de força, virilidade e resistência, criando a ideia de que o ser masculino não fica doente e não pode demonstrar fragilidade, devido a essa criação e educação familiar e cultural, imposta e cobrada pela sociedade, o homem é desleixado com sua saúde só procurando a assistência médica quando há um agravamento de seu estado físico Conclusão: os aspectos socioculturais desempenham um papel crucial na prevenção do câncer de próstata e pênis.
Агрохімічні властивості лісових ґрунтів Жеребківського лісництва філії "Ананьївське лісове господарство" ДП "Ліси України"
Authors: Шлапак В. П. , Савченко О. М. , Адаменко С. А. 
Published: October 2023

Досліджено ґрунти у 50-річних культурах дуба звичайного, ясена звичайного, дуба скельного, сосни кримської та гледичії триколючкової, які ростуть у дібровах Жеребківського лісництва філії "Ананьївське лісове господарство" ДП "Ліси України". Встановлено, що ґрунти належать до важкосуглинистих чорноземів, де частка мулуватих частинок у фракції за діаметром менше 0,01 мм є найбільшою і становить в межах від 50,89 до 64,92 %. У культурах дуба звичайного і ясена звичайного запас лісової підстилки майже однаковий (14,07 і 14,67 т/га), що в 1,48 раза більше, ніж у культурах гледичії й у 2,01 раза, ніж у культурах дуба скельного. У культурах сосни кримської запас лісової підстилки є максимальним – 19,04 т/га. Частка повністю розкладеної лісової підстилки змінюється від 16,95 до 44,28 %. У культурах сосни частка її найменша – 16,95 % від загальної маси підстилки. У культурах гледичії, дуба звичайного, ясена звичайного її частка не перевищує 42,61-44,28 %, а дуба скельного – 34,84 %. Вміст амонійного (NН4-N) азоту впродовж вегетаційного періоду майже незмінний, тоді як нітратного азоту (NО3-N) у ґрунтах утримується мало, а в жовтні – ще менше. Встановлено проникнення гумусу майже до материнської породи на глибину до 150-160 см у профілі. У типових чорноземах це пов'язано із впливом на них за попередні роки степової трав'яної рослинності. У горизонті А0 вміст гумусу становить в межах 5,48-8,80 %, у горизонті А1 – 3,29-5,54 %, а у шарі ґрунту (А2) і до материнської породи (В) його вміст значно нижчий. Однак ці горизонти достатньо забезпечені поживними речовинами. Ступінь кислотності ґрунтів за всіма генетичними горизонтами є нейтральним. Гідролітична кислотність дуже низька – змінюється від 1,9 до 6,4 мг-екв. на 100 г ґрунту і до материнської породи зменшується. Найбільш доступним для рослини є калій, оскільки фосфор практично недоступний. Азот накопичується у ґрунті завдяки гумусу, він є основним його джерелом. Також для чорноземів характерна середня та підвищена забезпеченість фосфором.
Аналіз наявних методів і засобів удосконалення навігації БПЛА з використанням штучного інтелекту
Authors: Стасенко Д. В. , Яковина В. С. 
Published: October 2023

Проаналізовано літературні джерела, в яких досліджено методи та засоби на основі нейромереж для удосконалення навігації БПЛА. Встановлено, що навігація на базі GPS є особливо вразливою до радіоелектронної боротьби та залежить від зовнішніх чинників. Охарактеризовано основні методи та засоби навчання і застосування нейромереж для навігації БПЛА. Описано загальні методи удосконалення навігації БПЛА, що дають змогу проводити експерименти та визначати якість тренованої моделі. Визначено використовувані індикатори якості навчання, зокрема: складність навчання, швидкість навчання, алгоритмічна складність обчислень, кількість необхідних кроків для досягнення поставленої цілі. Досліджено основні стратегії навчання з винагородою – DQN, PPO та SAC. Виокремлено основні чинники, що впливають на ефективність процесу навчання: способи та методи навчання, якість даних, навчальне середовище. Встановлено, що згідно з результатами попередніх досліджень, ефективними алгоритмами машинного навчання для навігації БПЛА є методи навчання з підкріпленням, SLAM, 3D-моделювання, візуальна одометрія, Computer Vision та інші. Проаналізовано наявні дослідження, методи та засоби для навчання нейромереж для вдосконалення навігації БПЛА. З'ясовано, що для забезпечення навігації БПЛА існують засоби як на рівні вбудованого бортового комп'ютера БПЛА, так і окремі системи для виконання складних обчислень. Встановлено, що ключовим засобом для удосконалення навігації БПЛА є використання алгоритмів з нечіткою логікою, зокрема необхідність розроблення методів й засобів для вдосконалення навігації БПЛА. Обґрунтовано актуальність використання методів на основі нейромереж для вдосконалення навігації БПЛА. Визначено напрями майбутніх досліджень, зокрема: визначення ефективних факторів й індикаторів для оцінювання результатів навчання; підвищення процесу навчання, покращення якості навчальних даних, збільшення енергоефективності БПЛА; покращення загальної продуктивності; побудова нових моделей навчання; оптимізація наявних алгоритмів; розроблення методів і засобів для вдосконалення навігації БПЛА.
Análise da diversidade e caracterização das síndromes de dispersão de diásporos em um gradiente sucessional de caatinga hiperxerófila
Authors: Alves de Lavôr Iara , De Lavôr Daniela Tábita , Silva de Lavôr Camila , Vieira Braga Dan Vitor 
Published: October 2023

A dispersão de sementes refere-se Ã retirada ou liberação dos diásporos da planta de origem e permite que frutos e/ou sementes escapem de serem depositados nas proximidades desse vegetal, onde as taxas de mortalidade são altas. Com isso o objetivo deste estudo é analisar o comportamento do processo de dispersão de diásporos na comunidade vegetal ao longo de uma cronossequência sucessional em áreas de Caatinga Hiperxerófila. A metodologia constituiu-se na divisão de três áreas de Caatinga selecionadas conforme seu estágio de sucessão, onde foi utilizado o método de parcelas, demarcando-se dois transectos de 30 m x 10 m, em cada condição; estes subdivididos em duas parcelas quadradas de 10 mÂ², estando cada uma separada 10 m entre si. Avaliaram-se todos os indivíduos vegetais de fanerógamas, com hábito arbustivo-arbóreo, â‰¥ 30 cm de altura. Em seguida, realizou-se também a tipificação e classificação dos frutos e síndromesde dispersão. De acordo com os resultados obtidos, observou-se que a síndrome de dispersão por blastocoria destacou-se nos três estágios sucessionais com 46% no inicial, 40% no intermediário, seguido de anemocoria 27% no tardio. Verificou-se ainda uma redução no número de frutos secos Ã medida que a sucessão ecológica avançou, ocorrendo o inverso com os frutos carnosos. Desse modo observou-se que o processo de dispersão de propágulos em área de Caatinga Hiperxerófila varia de acordo com as alterações ambientais presentes em cada estágio sucessional analisado. Assim, no último estágio, a flora local utiliza-se de frutos carnosos como atrativos mais eficientes de dispersores; já nos estágios iniciais da sucessão, houve predominância de estratégias de dispersão por vetores abióticos, como a anemocoria e blastocoria.
Pentingnya Pengetahuan tentang Kenakalan Remaja pada Siswa
Authors: Mintawati Hesri , Albert Jhoni 
Published: October 2023

Perilaku kenakalan remaja mengalami peningkatan yang cukup signifikan dalam beberapa tahun terakhir, sehingga penting untuk membekali siswa-siswi sekolah menengah atas, khususnya SMK PGRI Kota Sukabumi tentang pengetahuan seputar kenakalan remaja. Penelitian ini bertujuan untuk mengetahui bagaimana pengetahuan siswa SMK PGRI Kota Sukabumi terhadap kenakalan remaja. Metode yang digunakan dalam penelitian ini adalah metode kualitatif yang menggunakan pendekatan deskriptif. Dengan diadakannya kegiatan sosialiasi seputar kenaklaan remaja ini, kini siswa-siswa SMK PGRI Kota Sukabumi sudah mengetahui secara lengkap tentang perilaku kenakalan remaja.
Mental association of time and valence
Authors: Ulrich Rolf , de la Vega Irmgard , Eikmeier Verena , Günther Fritz , Kaup Barbara 
Published: October 2023

AbstractFive experiments investigated the association between time and valence. In the first experiment, participants classified temporal expressions (e.g., past, future) and positively or negatively connotated words (e.g., glorious, nasty) based on temporal reference or valence. They responded slower and made more errors in the mismatched condition (positive/past mapped to one hand, negative/future to the other) compared with the matched condition (positive/future to one hand, negative/past to the other hand). Experiment 2 confirmed the generalization of the match effect to nonspatial responses, while Experiment 3 found no reversal of this effect for left-handers. Overall, the results of the three experiments indicate a robust match effect, associating the past with negative valence and the future with positive valence. Experiment 4 involved rating the valence of time-related words, showing higher ratings for future-related words. Additionally, Experiment 5 employed latent semantic analysis and revealed that linguistic experiences are unlikely to be the source of this time–valence association. An interactive activation model offers a quantitative explanation of the match effect, potentially arising from a favorable perception of the future over the past.
Social and non-social feedback stimuli lead to comparable levels of reward learning and reward responsiveness in an online probabilistic reward task
Authors: Sailer Uta , Wurm Franz , Pfabigan Daniela M. 
Published: October 2023

AbstractSocial stimuli seem to be processed more easily and efficiently than non-social stimuli. The current study tested whether social feedback stimuli improve reward learning in a probabilistic reward task (PRT), in which one response option is usually rewarded more often than the other via presentation of non-social reward stimuli. In a pre-registered online study with 305 participants, 75 participants were presented with a non-social feedback stimulus (a star) and information about gains, which is typically used in published PRT studies. Three other groups (with 73–82 participants each) were presented with one of three social feedback stimuli: verbal praise, an attractive happy face, or a “thumbs up”-picture. The data were analysed based on classical signal detection theory, drift diffusion modelling, and Bayesian analyses of null effects. All PRT variants yielded the expected behavioural preference for the more frequently rewarded response. There was no processing advantage of social over non-social feedback stimuli. Bayesian analyses further supported the observation that social feedback stimuli neither increased nor decreased behavioural preferences in the PRT. The current findings suggest that the PRT is a robust experimental paradigm independent of the applied feedback stimuli. They also suggest that the occurrence of a processing advantage for social feedback stimuli is dependent on the experimental task and design.
The High-energy Spectrum of the Young Planet Host V1298 Tau
Authors: Duvvuri Girish M. , Cauley P. Wilson , Aguirre Fernando Cruz , Kilgard Roy , France Kevin , Berta-Thompson Zachory K. , Pineda J. Sebastian 
Published: October 2023

Abstract
V1298 Tau is a young pre-main-sequence star hosting four known exoplanets that are prime targets for transmission spectroscopy with current-generation instruments. This work pieces together observations from the NICER X-ray telescope, the Space Telescope Imaging Spectrograph and Cosmic Origins Spectrograph instruments aboard Hubble Space Telescope, and empirically informed models to create a panchromatic spectral energy distribution for V1298 Tau spanning 1–105 Å. We describe the methods and assumptions used to assemble the panchromatic spectrum and show that despite this star’s brightness, its high-energy spectrum is near the limit of present X-ray and ultraviolet observatories’ abilities to characterize. We conclude by using the V1298 Tau spectrum as a benchmark for the activity saturation stage of high-energy radiation from solar-mass stars to compare the lifetime cumulative high-energy irradiation of the V1298 Tau planets to other planets orbiting similarly massive stars.
Two Warm Super-Earths Transiting the Nearby M Dwarf TOI-2095
Authors: Quintana Elisa V. , Gilbert Emily A. , Barclay Thomas , Silverstein Michele L. , Schlieder Joshua E. , Cloutier Ryan , Quinn Samuel N. , Rodriguez Joseph E. , Vanderburg Andrew , Hord Benjamin J. , Louie Dana R. , Ostberg Colby , Kane Stephen R. , Hoffman Kelsey , Rowe Jason F. , Arney Giada N. , Saxena Prabal , Richardson Taran , Clement Matthew S. , Kartvedt Nicholas M. , Adams Fred C. , Alfred Marcus , Berger Travis , Bieryla Allyson , Bonney Paul , Boyd Patricia , Cadieux Charles , Caldwell Douglas , Ciardi David R. , Charbonneau David , Collins Karen A. , Colón Knicole D. , Conti Dennis M. , Di Sora Mario , Domagal-Goldman Shawn , Dotson Jessie , Fauchez Thomas , Gonzales Erica J. , Günther Maximilian N. , Hedges Christina , Isopi Giovanni , Kohler Erika , Kopparapu Ravi , Kostov Veselin B. , Larsen Jeffrey A. , Lopez Eric , Mallia Franco , Mandell Avi , Mullally Susan E. , Paudel Rishi R. , Powell Brian P. , Ricker George R. , Safonov Boris S. , Schwarz Richard P. , Sefako Ramotholo , Stassun Keivan G. , Wilson Robert , Winn Joshua N. , Vanderspek Roland K. 
Published: October 2023

Abstract
We report the detection and validation of two planets orbiting TOI-2095 (TIC 235678745). The host star is a 3700 K M1V dwarf with a high proper motion. The star lies at a distance of 42 pc in a sparsely populated portion of the sky and is bright in the infrared (K = 9). With data from 24 sectors of observation during Cycles 2 and 4 of the Transiting Exoplanet Survey Satellite, TOI-2095 exhibits two sets of transits associated with super-Earth-sized planets. The planets have orbital periods of 17.7 days and 28.2 days and radii of 1.30 R
⊕ and 1.39 R
⊕, respectively. Archival data, preliminary follow-up observations, and vetting analyses support the planetary interpretation of the detected transit signals. The pair of planets have estimated equilibrium temperatures of approximately 400 K, with stellar insolations of 3.23 and 1.73 S
⊕, placing them in the Venus zone. The planets also lie in a radius regime signaling the transition between rock-dominated and volatile-rich compositions. They are thus prime targets for follow-up mass measurements to better understand the properties of warm, transition-radius planets. The relatively long orbital periods of these two planets provide crucial data that can help shed light on the processes that shape the composition of small planets orbiting M dwarfs.
The Disk Reverberation Mapping of X-Ray Weak Quasars: A Case Study of SDSS J153913.47+395423.4
Authors: Marculewicz Marcin , Sun Mouyuan , Wu Jianfeng , Zhang Zhixiang 
Published: October 2023

Abstract
The widely adopted “lamppost” thermal reprocessing model, in which the variable UV/optical emission is a result of the accretion-disk reprocessing of the highly fluctuating X-ray emission, can be tested by measuring interband time lags in quasars spanning a range of X-ray power. This work reports the interband time lag in an apparent X-ray-weak quasar, SDSS J153913.47+395423.4. A significant cross correlation with a time delay of ∼33 days (observed frame) is detected in the Zwicky Transient Facility g and r light curves of SDSS J153913.47+395423.4. The observed X-ray power seems to be too weak to account for the observed interband cross correlation with time delay. Hence the X-ray-weak quasar SDSS J153913.47+395423.4 is either intrinsically X-ray normal (but observationally X-ray weak), or the X-ray emission is not the only mechanism to drive UV/optical variability. In the former case, the required X-ray power is at least 19 times stronger than observed, which requires either an exceptionally anisotropic corona or Compton-thick obscuration. Alternatively, the corona-heated accretion-disk reprocessing or the EUV torus models may account for the observed time lags.
Fast-rotating Blue Straggler Stars in the Globular Cluster NGC 3201*
Authors: Billi Alex , Ferraro Francesco R. , Mucciarelli Alessio , Lanzoni Barbara , Cadelano Mario , Monaco Lorenzo , Mateo Mario , Bailey John I. , Reiter Megan , Olszewski Edward W. 
Published: October 2023

Abstract
We used high-resolution spectra acquired with the Magellan Telescope to measure radial and rotational velocities of approximately 200 stars in the Galactic globular cluster NGC 3201. The surveyed sample includes blue straggler stars (BSSs) and reference stars in different evolutionary stages (main-sequence turnoff, subgiant, red giant, and asymptotic giant branches). The average radial velocity value (〈V

r
〉 = 494.5 ± 0.5 km s−1) confirms a large systemic velocity for this cluster and was used to distinguish 33 residual field interlopers. The final sample of member stars has 67 BSSs and 114 reference stars. Similarly to what is found in other clusters, the totality of the reference stars has negligible rotation (< 20 km s−1), while the BSS rotational velocity distribution shows a long tail extending up to ∼200 km s−1, with 19 BSSs (out of 67) spinning faster than 40 km s−1. This sets the percentage of fast-rotating BSSs to ∼28%. Such a percentage is roughly comparable to that measured in other loose systems (ω Centauri, M4, and M55) and significantly larger than that measured in high-density clusters (as 47 Tucanae, NGC 6397, NGC 6752, and M30). This evidence supports a scenario where recent BSS formation (mainly from the evolution of binary systems) is occurring in low-density environments. We also find that the BSS rotational velocity tends to decrease for decreasing luminosity and surface temperature, similarly to what is observed in main-sequence stars. Hence, further investigations are needed to understand the impact of BSS internal structure on the observed rotational velocities.
On the Encounter between the GASP Galaxy JO36 and the Radio Plume of GIN 049
Authors: Ignesti Alessandro , Brienza Marisa , Vulcani Benedetta , Poggianti Bianca M. , Marasco Antonino , Smith Rory , Hardcastle Martin J. , Botteon Andrea , Roberts Ian D. , Fritz Jacopo , Paladino Rosita , Gitti Myriam , Wolter Anna , Tomičić Neven , McGee Sean , Moretti Alessia , Gullieuszik Marco , Drabent Alexander 
Published: October 2023

Abstract
We report the serendipitous discovery of an unprecedented interaction between the radio lobe of a radio galaxy and a spiral galaxy. The discovery was made thanks to LOFAR observations at 144 MHz of the galaxy cluster A160 (z = 0.04317) provided by the LOFAR Two-metre Sky Survey. The new low-frequency observations revealed that one of the radio plumes of the central galaxy GIN 049 overlaps the spiral galaxy JO36. Previous studies carried out with MUSE revealed that the warm ionized gas in the disk of JO36, traced by the Hα emission, is severely truncated with respect to the stellar disk. We further explore this unique system by including new uGMRT observations at 675 MHz to map the spectral index. The emerging scenario is that JO36 has interacted with the radio plume in the past 200–500 Myr. The encounter resulted in a positive feedback event for JO36 in the form of a star formation rate burst of ∼14 M
⊙ yr−1. In turn, the galaxy passage left a trace in the radio-old plasma by reshaping the old relativistic plasma via magnetic draping.
Statistical Analysis of Long GRBs’ Prompt Emission and X-Ray Flares: Multivariate Clustering and Correlations
Authors: Saji Joseph , Iyyani Shabnam , Mazde Kratika 
Published: October 2023

Abstract
The extensive observations done by the X-ray Telescope on board Neil Gehrels Swift Observatory have revealed the presence of late-time flares concurrent with the decaying afterglow emission. However, the origins of these flares are elusive. In this work, we make use of the large database of Swift observations (2005–2020) of long gamma-ray bursts (GRBs) to conduct a systematic statistical study between the prompt gamma-ray emission and X-ray flares by characterizing their temporal and spectral properties of duration, quiescent period, peak flux, fluence, minimum variability timescale, and spectral power-law index. The multidimensional database of parameters thereby generated was investigated by principal component analysis, which revealed there is no evident correlation between the different parameters of the prompt emission and X-ray flares. Furthermore, the correlation studies revealed that while there is a trend of positive correlation between the minimum variability timescale of the flare and its duration, and of strong negative correlation with its peak flux, there are no such correlations observed in the prompt emission. Similarly, we find a positive correlation between the quiescent period and the flare duration, and a negative correlation with the flare peak flux, while no such correlations are observed for the prompt emission of the GRBs. Finally, among the X-ray flares, we find two dominant classes, whose variations are driven by the minimum variability timescale, peak flux, and fluence of the flares. A catalog of these different parameters characterizing the prompt and flare emissions is presented.