bluuebunny/crossref_metadata_2025_split huggingface dataset:
Kontakty Antoniego Patka ze zmartwychwstańcami
Authors: Czapla Beniamin 
Published: February 2024

Antoni Patek przyszedł na świat w 1812 r. na Lubelszczyźnie. Jako żołnierz wziął udział w powstaniu listopadowym. Po jego upadku udał się na emigrację. W 1835 r. osiadł w Szwajcarii Versoix koło Genewy. Tam też poznał innego polistopadowego emigranta – zegarmistrza Franciszka Czapka. W 1839 r. Patek i Czapek zawiązali spółkę produkującą zegarki Patek, Czapek et Cie. Firma skupiała się głównie na zaopatrywaniu polskiej klienteli. Dlatego też ich zegarki były zdobione wizerunkami polskich królów, książąt, portretami bohaterów narodowych i motywami religijnymi. W 1845 r. Patek zerwał współpracę z Czapkiem. Niedługo później podjął współpracę z innym zegarmistrzem – Adrienem Philippem, jednym z wynalazców systemu nastawczo-naciągowego, oraz dysponującym znacznymi środkami finansowymi rodakiem Wincentym Gostkowskim. Z biegiem czasu grono klientów wytwórni poszerzało się. Prócz zaangażowanych w działalność patriotyczną Polaków, zegarki kupowali też politycy, przywódcy państw, ówcześni artyści i przedsiębiorcy.
Jeden z wyrobów Patka przechowywany jest w zbiorach muzealnych Zgromadzenia Zmartwychwstania Pańskiego. Jak wynika z zachowanych materiałów, należał do ks. Piotra Semenenki.
Patek nawiązał kontakty ze zmartwychwstańcami w latach trzydziestych XIX w., za sprawą Walerego Wielogłowskiego, sekretarza i jednego z najbliższych towarzyszy założyciela zgromadzenia – ks. Bogdana Jańskiego. W 1839 r. Wielogłowski udał się do Genewy, by namówić kuzyna – Ludwika Popiela, do wsparcia popadającego w coraz większe kłopoty finansowe przedsięwzięcia ks. Jańskiego. Tam też poznał Patka, który jako gorliwy katolik szybko uległ jego wpływom ewangelizacyjnym.
Antoni Patek z miejsca stał się wiernym dobroczyńcą i przyjacielem ojców założycieli zgromadzenia. Potwierdzenie zażyłości można znaleźć w zachowanym do dziś zbiorze ich korespondencji. Z jednej strony jest to ciekawe świadectwo wiary Patka, z drugiej zaś – potwierdzenie ich zaangażowania w niesienie pomocy potrzebującym rodakom.
Kapłani, artyści i kacerze, czyli spotkania zmartwychwstańców z Wojciechem Kornelim Stattlerem i Adamem Mickiewiczem w Rzymie i Paryżu
Authors: Nitka Maria 
Published: February 2024

Artykuł rozważa różne postawy ideowe wśród Wielkiej Emigracji, reprezentowanej przez grono przyjaciół Adama Mickiewicza – malarza Wojciecha Kornelego Stattlera oraz Zgromadzenia Zmartwychwstańców, zwłaszcza o. Hieronima Kajsiewicza i o. Piotra Semenenkę. Punktem wyjścia dla prezentacji postaw jest odkryty podczas inwentaryzacji i dokumentacji kolekcji sztuki Zakonu Zmartwychwstańców w Rzymie obraz ukazujący Chrzest Chrystusa w Jordanie, w którym Jan Chrzciciel ma rysy Adama Mickiewicza. Obraz został przypisany Stattlerowi, w wyniku analizy oeuvre i prześledzenia kontaktów malarza z Mickiewiczem. Takie wyobrażenie chrztu Chrystusa zostaje powiązane z mesjanizem, a później również towianizem Mickiewicza i jego oddziaływaniem na emigrację. W tym kontekście zostały ukazane postawy zmartwychwstańców, którzy zaangażowali się w zwalczanie towianizmu. Nie rezygnowali jednak z próby „odzyskania” poety dla sprawy polskiej i przechowywali pamięć o poecie.
The BRICS in Southern Africa
Authors: Chagas de Assis Caroline 
Published: February 2024

The BRICS were created at the beginning of the 21st century to reorganize the international world order to represent their weight in international politics, economics, and geopolitics. Although they are entirely different, the BRICS saw a strategic space to reach these goals in the African continent. Thus, these countries started to broaden their presence in the African continent. As a result, BRICs started their relations with Africa differently, but they acted in similar sectors. The fellow paper pursues to analyze the Brazilian, Russian, Indian and Chinese (called here as BRICs) insertion in Southern Africa, highlighting the main convergence sectors and divergences between them. The methodology will be based on historical analyses, connecting their historical insertion in Southern Africa in a broad perspective of foreign policy objectives in the 21 st century. In the first session, we will approach the economic presence of BRIC in Southern Africa in 21 st century. Latter, we will abstract each one's foreign policy for the region (highlighting the main economic sectors and diplomatic presence).
Moreover, it will be possible to compare their presences, highlighting the convergence and divergence between them. The Chinese and Indian weight in Africa's economy is more perceptive than Brazilian's and Russian's. Nonetheless, all BRICs have been widening their trade and diplomatic relations with Southern Africa in the 21st century due to their perspective of the importance of Africa in international world politics.
Rodent tests of depression and anxiety: Construct validity and translational relevance
Authors: Gencturk Sinem , Unal Gunes 
Published: February 2024

AbstractBehavioral testing constitutes the primary method to measure the emotional states of nonhuman animals in preclinical research. Emerging as the characteristic tool of the behaviorist school of psychology, behavioral testing of animals, particularly rodents, is employed to understand the complex cognitive and affective symptoms of neuropsychiatric disorders. Following the symptom-based diagnosis model of the DSM, rodent models and tests of depression and anxiety focus on behavioral patterns that resemble the superficial symptoms of these disorders. While these practices provided researchers with a platform to screen novel antidepressant and anxiolytic drug candidates, their construct validity—involving relevant underlying mechanisms—has been questioned. In this review, we present the laboratory procedures used to assess depressive- and anxiety-like behaviors in rats and mice. These include constructs that rely on stress-triggered responses, such as behavioral despair, and those that emerge with nonaversive training, such as cognitive bias. We describe the specific behavioral tests that are used to assess these constructs and discuss the criticisms on their theoretical background. We review specific concerns about the construct validity and translational relevance of individual behavioral tests, outline the limitations of the traditional, symptom-based interpretation, and introduce novel, ethologically relevant frameworks that emphasize simple behavioral patterns. Finally, we explore behavioral monitoring and morphological analysis methods that can be integrated into behavioral testing and discuss how they can enhance the construct validity of these tests.
Metodologías de Enseñanza y Aprendizaje en Modalidad a Distancia y en Línea en Educación Superior
Authors: Hidalgo Apolo Gladys Angélica , Torres Díaz Silvia Eugenia , Espinoza Rojas Stalin Jeovanny 
Published: February 2024

En las instituciones de educación superior se enfrentan nuevos desafíos, en un entorno cambiante que pone en evidencia la necesidad de responder a las demandas sociales, culturales y políticas de esta era, y la imperiosa tarea de entender los procesos de enseñanza aprendizaje como dinámicos, cambiantes, poco convencionales y heterogéneos. En este contexto, la investigación tiene el propósito de identificar las metodologías que se van integrando en el proceso de enseñanza aprendizaje en educación a distancia y en línea, y su aporte a la construcción de procesos didácticos innovadores que redefinen la educación superior. La investigación es de diseño descriptivo, con una muestra de 500 estudiantes de las modalidades a distancia y en línea de la Universidad Nacional de Loja; la recolección de la información se realizó mediante una escala Likert. Se concluye que las principales metodologías que se integran al proceso de enseñanza y aprendizaje son activas, enfocadas al desarrollo del pensamiento crítico, principalmente el aprendizaje por descubrimiento, aprendizaje basado en retos, y estudio de caso; y que estas se incorporan de la mano de las tecnologías de la información y comunicación, especialmente plataformas digitales que permiten la presentación de contenidos y de trabajo colaborativo.
Pemodelan Kadar Hemoglobin pada Pasien Demam Berdarah di Kota Samarinda Menggunakan Regresi Semiparametrik Spline Truncated
Authors: Dani Andrea Tri Rian , Putra Fachrian Bimantoro , Zen Muhammad Aldani , Sifriyani Sifriyani , Fauziyah Meirinda , Ratnasari Vita , Adrianingsih Narita Yuri 
Published: February 2024

This article discusses the innovation of statistical modeling in regression analysis with a semiparametric approach applied to health data. Regression analysis is a method in statistics that takes a lot of roles in statistical modeling. Regression analysis is used to model the relationship between the independent variable (x) and the dependent variable (y). There are three approaches to regression analysis, namely parametric, nonparametric, and a combination of the two, namely semiparametric. Semiparametric regression is used when the dependent variable has a known relationship with some of the independent variables and has an unknown pattern of a relationship with some of the other independent variables. The purpose of this study was to model hemoglobin levels in dengue fever patients, with the independent variables used being the number of hematocrits (x1) and the number of leukocytes (x2). The method used is spline truncated semiparametric regression. The truncated spline estimator was chosen for the nonparametric component because it has many advantages in modeling, one of which is being able to model patterns where the form of the relationship is unknown. The parameter estimation used is the maximum estimation. Selection of the optimal knot point using Generalized Cross-Validation (GCV). Based on the results of the analysis, the truncated spline semiparametric regression model was obtained which was applied to the hemoglobin level data in a model with three knots which have a coefficient of determination of 89.074%. Based on the results of testing the hypothesis simultaneously, it can be concluded that simultaneously the independent variable has a significant effect on the dependent variable. In the partial test, it is concluded that the variables x1 and x2 have a significant influence on the dependent variable y .
Peramalan Jumlah Sampah di Kabupaten Lombok Timur dengan Metode ARIMA dan Dekomposisi
Authors: Nurmayanti Wiwit Pura , Kertanah Kertanah , Hasanah Siti Hadijah , Rahim Abdul , Hendrayani Hendrayani 
Published: February 2024

AbstractForecasting is the science of predicting events that will occur using historical data and projecting them into the future with some form of mathematical model that aims to handle and policy in the future. In forecasting there are several methods, two of which are Autoregeressive Integrated Moving Average (ARIMA) and Decomposition. ARIMA is a method developed by George Box and Gwilym Jenkins in 1970. The Decomposition Method is a method that decomposes (breaks) time series data into several patterns, namely trend, cyclical and seasonal, and identifies each of these components separately. Both of these methods can be applied in various fields, one of which is in the field of environmental health, especially data on the amount of waste. Problems related to the amount of waste in East Lombok are still a concern of the government because as the population increases and the needs of the community each year have the potential to cause waste problems. The final disposal site (TPA) in East Lombok is located in Ijo Balit, this TPA is the only one in East Lombok. The purpose of this research is to see which method is the best between ARIMA and Decomposition, and to see the forecasting results of the amount of waste entering TPA Ijo Balit from the best method. Based on the results of the analysis carried out by the Decomposition model, it gives the best performance in terms of the smallest error value so that it can be used for Forecasting and produces an RMSE value of 5201.694, a MAPE of 0.955827 and a MASE of 0.0129691. The results of forecasting using the Decomposition method are that the highest forecast occurs in December, while the lowest occurs in January with a total of 1,439,439 (tons) and 1,117,000 (tons). Keywords: Forecasting, ARIMA, Decomposition, Waste
IMPACTO DEL COVID-19 EN LA COMUNIDAD ESTUDIANTIL DEL I.T.S.T.R.
Authors: Sánchez Luis Ángel Morales , Ramos Rosalina Lezama , Olmos Claudia Domínguez , Y Tovar Edgardo Roldan , Regules Behetzaida Martínez , Pérez Lizbeth Mazariego 
Published: February 2024

El coronavirus SARS-Cov-2 es un virus que apareció en China, después se extendió a todos los continentes del mundo provocando una pandemia. Para que el ritmo de vida pudiera continuar se tuvieron que implementar estrategias para reducir las interacciones sociales. El porcentaje de población que no concluyo el ciclo escolar en educación superior fue de 44.6 %, de los cuales el 25.1% fue por falta de recursos o porque tenían que trabajar. (INEGI 2021). El Instituto Tecnológico Superior de Tepexi de Rodríguez (I.T.S.T.R.) es un organismo público descentralizado del estado Puebla, que pertenece al sistema del Tecnológico Nacional de México. El estudio tuvo como objetivo identificar cuál fue el impacto del COVID-19 en la comunidad estudiantil del Instituto en el año 2021, teniendo un alcancé de tipo exploratorio-descriptivo, para el cual se tomó una muestra de 264 estudiantes, a los cuales se les aplico una encuesta a través de un formulario digital que conto con 21 preguntas divididas en cuatro factores: aprendizaje, accesibilidad en los medios, económico y salud. De acuerdo al estudio realizado se pudo concluir que el impacto del COVID-19 en la comunidad estudiantil fue significativo en el tema de la salud ya que se identificó que el 31% de los estudiantes se contagió del virus del SARS-Cov-2 mientras estaban inscritos en esta institución durante el año 2021, también se pudo identificar que durante el aislamiento experimentaron un sentimiento de incomunicación, estrés y ansiedad, el cual fue un impacto en la salud mental; la pandemia también tuvo un efecto económico en los estudiantes ya que provocó que un 39% de los alumnos inscritos faltará a clases debido a la carencia de recursos económicos y que un 62% tuviera la necesidad de buscar un trabajo para poder continuar con sus estudios y apoyar en los gastos familiares.
The DECam Ecliptic Exploration Project (DEEP). II. Observational Strategy and Design
Authors: Trujillo Chadwick A. , Fuentes Cesar , Gerdes David W. , Markwardt Larissa , Sheppard Scott S. , Strauss Ryder , Chandler Colin Orion , Oldroyd William J. , Trilling David E. , Lin 林 Hsing Wen 省文 , Adams Fred C. , Bernardinelli Pedro H. , Holman Matthew J. , Jurić Mario , McNeill Andrew , Mommert Michael , Napier Kevin J. , Payne Matthew J. , Ragozzine Darin , Rivkin Andrew S. , Schlichting Hilke , Smotherman Hayden 
Published: February 2024

Abstract
We present the DECam Ecliptic Exploration Project (DEEP) survey strategy, including observing cadence for orbit determination, exposure times, field pointings and filter choices. The overall goal of the survey is to discover and characterize the orbits of a few thousand Trans-Neptunian objects (TNOs) using the Dark Energy Camera (DECam) on the Cerro Tololo Inter-American Observatory Blanco 4 m telescope. The experiment is designed to collect a very deep series of exposures totaling a few hours on sky for each of several 2.7 square degree DECam fields-of-view to achieve approximate depths of magnitude 26.2 using a wide V
R filter that encompasses both the V and R bandpasses. In the first year, several nights were combined to achieve a sky area of about 34 square degrees. In subsequent years, the fields have been re-visited to allow TNOs to be tracked for orbit determination. When complete, DEEP will be the largest survey of the outer solar system ever undertaken in terms of newly discovered object numbers, and the most prolific at producing multiyear orbital information for the population of minor planets beyond Neptune at 30 au.
Deconstructing Photospheric Spectral Lines in Solar and Stellar Flares
Authors: Monson Aaron J. , Mathioudakis Mihalis , Kowalski Adam F. 
Published: February 2024

Abstract
During solar flares, spectral lines formed in the photosphere have been shown to exhibit changes to their profiles despite the challenges of energy transfer to these depths. Recent work has shown that deep-forming spectral lines are subject to significant contributions from regions above the photosphere throughout the flaring period, resulting in a composite emergent intensity profile from multiple layers of the atmosphere. We employ radiative–hydrodynamic and radiative transfer calculations to simulate the response of the solar/stellar atmosphere to electron beam heating and synthesize spectral lines of Fe i to investigate the line-of-sight velocity fields information available from Doppler shifts of the emergent intensity profile. By utilizing the contribution function to deconstruct the line profile shape into its constituent sources, we show that variations in the line profiles are primarily caused by changes in the chromosphere. Up-flows in this region were found to create blueshifts or false redshifts in the line core dependent on the relative contribution of the chromosphere compared to the photosphere. In extreme solar and stellar flare scenarios featuring explosive chromospheric condensations, redshifted transient components can dominate the temporal evolution of the profile shape, requiring a tertiary component consideration to fully characterize. We conclude that deep-forming lines require a multicomponent understanding and treatment, with different regions of the spectral line being useful for probing individual regions of the atmosphere’s velocity flows.
Zero Metallicity with Zero CPU Hours: Masses of the First Stars on the Laptop
Authors: Gurian James , Jeong Donghui , Liu Boyuan 
Published: February 2024

Abstract
We develop an analytic model for the mass of the first stars forming in the centers of primordial gas clouds as a function of host halo mass, redshift, and degree of rotation. The model is based on the estimation of key timescales determining the following three processes: the collapse of the gas cloud, the accretion onto the protostellar core, and the radiative feedback of the protostellar core. The final stellar mass is determined by the total mass accreted until the radiative feedback halts the accretion. The analytic estimation, motivated by the result of the full numerical simulations, leads to algebraic expressions allowing an extremely fast execution. Despite its simplicity, the model reproduces the stellar mass scale and its parameter dependencies observed in state-of-the-art cosmological zoom-in simulations. This work clarifies the basic physical principles undergirding such numerical treatments and provides a path to efficiently calibrating numerical predictions against eventual observations of the first stars.
A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Impact of Galaxies on the Circumgalactic Medium Metal Enrichment at z > 6 Using the JWST and VLT
Authors: Zou Siwei , Cai Zheng , Wang Feige , Fan Xiaohui , Champagne Jaclyn B. , Hennawi Joseph F. , Schindler Jan-Torge , Farina Emanuele Paolo , Yang Jinyi , Inayoshi Kohei , Bañados Eduardo , Bosman Sarah E. I. , Li Zihao , Lin Xiaojing , Wu Yunjing , Sun Fengwu , Guo Ziyi , Kulkuarni Girish , Habouzit Mélanie , Charlot Stephane , Chevallard Jacopo , Connor Thomas , Eilers Anna-Christina , Jiang Linhua , Jin Xiangyu , Kakiichi Koki , Li Mingyu , Meyer Romain A. , Walter Fabian , Zhang Huanian 
Published: February 2024

Abstract
We characterize the multiphase circumgalactic medium (CGM) and galaxy properties at z = 6.0–6.5 in four quasar fields from the James Webb Space Telescope A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE) program. We use the Very Large Telescope/X-shooter spectra of quasar J0305–3150 to identify one new metal absorber at z = 6.2713 with multiple transitions (O i, Mg ii, Fe ii, and C ii). They are combined with the published absorbing systems in Davies et al. at the same redshift range to form a sample of nine metal absorbers at z = 6.03–6.49. We identify eight galaxies within 1000 km s−1 and 350 kpc around the absorbing gas from the ASPIRE spectroscopic data, with their redshifts secured by [O iii] (λ
λ4959, 5007) doublets and Hβ emission lines. Our spectral energy distribution fitting indicates that the absorbing galaxies have stellar masses ranging from 107.2 to 108.8
M
⊙ and metallicity between 0.02 and 0.4 solar. Notably, the z = 6.2713 system in the J0305–3150 field resides in a galaxy overdensity region, which contains two (tentatively) merging galaxies within 350 kpc and seven galaxies within 1 Mpc. We measure the relative abundances of α elements to iron ([α/Fe]) and find that the CGM gas in the most overdense region exhibits a lower [α/Fe] ratio. Our modeling of the galaxy’s chemical abundance favors a top-heavy stellar initial mass function and hints that we may be witnessing the contribution of the first generation of Population III stars to the CGM at the end of the reionization epoch.
Optical Appearance of Eccentric Tidal Disruption Events
Authors: Hu Fangyi (Fitz) , Price Daniel J. , Mandel Ilya 
Published: February 2024

Abstract
Stars approaching supermassive black holes can be tidally disrupted. Despite being expected to emit X-rays, tidal disruption events (TDEs) have been largely observed in optical bands, which is poorly understood. In this Letter, we simulate the tidal disruption of a 1 M
⊙ main-sequence star on an eccentric (e = 0.95) orbit with a periapsis distance 1 or 5 times smaller than the tidal radius (β = 1 or 5) using general relativistic smoothed particle hydrodynamics. We follow the simulation for up to 1 yr postdisruption. We show that accretion disks in eccentric TDEs are masked by unbound material outflowing at ∼10,000 km s −1. Assuming electron scattering opacity, this material would be visible as a ∼100 au photosphere at ∼104 K, in line with observations of candidate TDEs.
Computable Species Descriptions and Nanopublications: Applying Ontology-based Technologies to Dung Beetles (Coleoptera: Scarabaeinae)
Authors: Montanaro Giulio , Balhoff James , Girón Jennifer , Söderholm Max , Tarasov Sergei 
Published: February 2024

Taxonomy has long struggled with analyzing vast amounts of phenotypic data due to computational and accessibility challenges. Ontology-based technologies provide a framework for modeling semantic phenotypes that are understandable by computers and compliant with FAIR principles. In this paper, we explore the use of Phenoscript, an emerging language designed for creating semantic phenotypes, to produce computable species descriptions. Our case study centers on the application of this approach to dung beetles (Coleoptera: Scarabaeinae).
We illustrate the effectiveness of Phenoscript for creating semantic phenotypes. We also demonstrate the ability of the Phenospy python package to automatically translate Phenoscript descriptions into natural language (NL), which eliminates the need for writing traditional NL descriptions. We introduce a computational pipeline that streamlines the generation of semantic descriptions and their conversion to NL. To demonstrate the power of the semantic approach, we apply simple semantic queries to the generated phenotypic descriptions. This paper addresses the current challenges in crafting semantic species descriptions and outlines the path towards future improvements. Furthermore, we discuss the promising integration of semantic phenotypes and nanopublications, as emerging methods for sharing scientific information. Overall, our study highlights the pivotal role of ontology-based technologies in modernizing taxonomy and aligning it with the evolving landscape of big data analysis and FAIR principles.