bluuebunny/crossref_metadata_2025_split huggingface dataset:
Ksiądz Józef Wilk (1937–2003) – salezjanin, pedagog prewencyjny, mistrz o wielkim sercu
Authors: Miąso Janusz 
Published: February 2024

Artykuł w nurcie biografistyki pedagogicznej prezentuje, analizuje i promuje postać ks. profesora Józefa Wilka, człowieka o wielkim sercu, salezjanina z bardzo mocną identyfikacją i realizacją misji ks. Jana Bosko, pedagoga z pasją i powołaniem, który przez wiele lat służył edukacji i wielowymiarowemu kształtowaniu ludzi młodych i ludzi nauki, aby czynić świat bardziej ludzki. Artykuł to badania poświęcone skutecznej koncepcji pedagogicznej, jaką jest system prewencyjny Jana Bosko, który metodycznie i merytorycznie wprowadzał, uaktualniał i czynił ciągle skutecznym ks. Wilk. W badaniach zwrócono uwagę na Jego wieloaspektową pracę naukową i dydaktyczną – pochylenie się nad dzieckiem, uczniem, młodzieńcem, nauczycielem i rodziną a przede wszystkim kształtującą bogate człowieczeństwo w tych wszystkich obszarach życia bo płynące z relacji mistrz – uczeń. Ks. Wilk całe życie pasjonował się chrześcijaństwem, jako żywą obecnością Mistrza – Chrystusa, mobilizującego wszystkich do realizacji przykazania miłości – sam kochał ludzi i pomagał, aby to przykazanie było realizowane w szkole, w uniwersytecie, w domu i wszędzie, a szczególnie tam, gdzie ludzie tego najbardziej potrzebują.
Stanisława Aleksandra Chmielarczyk – zapomniana artystka teatrów dramatycznych
Authors: Stoch Elżbieta 
Published: February 2024

Celem artykułu jest upowszechnienie nieznanych faktów z biografii Stanisławy Aleksandry Chmielarczyk (1867–1912), zapomnianej artystki teatrów dramatycznych w Warszawie pod zaborem rosyjskim, oraz jej syna, aktora Maksymiliana Chmielarczyka (1891–1953), pseudonim „Cybulski”. Autorka odnalazła w archiwach nieznane dokumenty, w tym m.in. rękopisy metryk, aktów stanu cywilnego. Odkryte dokumenty pozwoliły jej odsłonić nieznane dotąd fakty z życia Stanisławy Aleksandry: daty urodzenia i śmierci oraz biografię aktorki (samotne macierzyństwo, małżeństwo czy ślub jej syna Maksymiliana w 1911 r.). Badaczka odtworzyła drzewo genealogiczne Stanisławy Aleksandry Chmielarczyk oraz jej syna, Maksymiliana, przyszłego aktora, reżysera, dyrektora Teatru Miejskiego w Lublinie (1947–1949), a potem Państwowego Teatru im. Juliusza Osterwy (1949–1952), w czasach socrealizmu w Polsce. W kontekście biografii rodziny aktorskiej Chmielarczyka w artykule znajdują się również cenne odniesienia do nieznanych faktów z życia m.in. artysty Józefa Cybulskiego (1840–1912).
Ludwika z Rzewuskich Chodkiewiczowa (1744-1816) – w kręgu spraw rodzinnych
Authors: Żołądź-Strzelczyk Dorota 
Published: February 2024

Ludwika Maria Róża z Rzewuskich Chodkiewiczowa nie znajduje się w grupie kobiet, o których losach pisali historycy. Funkcjonowała na uboczu wielkiej polityki, jej różnorodna aktywność skupiona była głównie na rodzinie, rodzinnych majętnościach, własnych zainteresowaniach. Celem niniejszych rozważań jest przedstawienie jej aktywności rodzinnej, a posłużą do tego materiały źródłowe zgromadzone w Archiwum Młynowskim, przechowywanym w Archiwum Narodowym w Krakowie.
Artykuł uwzględnia jej życie w domu rodzinnym, w Podhorcach. Omówione zostały relacje z matką oraz szczególna bliskość z ojcem, Wacławem. Podjęta została próba odtworzenia jej edukacji, która wpłynęła na późniejsze zainteresowania panny Rzewuskiej. Kolejny etap życia Ludwiki Marii to czasy jej małżeństwa ze starostą żmudzkim Janem Mikołajem Chodkiewiczem. Ich ślub odbył się w styczniu 1766 r. i byli małżeństwem do śmierci starosty w 1781 r. Powiększająca się rodzina zamieszkała w Czarnobylu., a następnie w wybudowanym po śmierci starosty pałacu w Młynowie. Chodkiewiczowa urodziła siedmioro dzieci, dwójka zmarła we wczesnym dzieciństwie, a pierworodny syn Wacław nie dożył osiemnastych urodzin. Rodzice troszczyli się o odpowiednią edukację dzieci, szczególnie synów, którzy kolejno wysyłani byli do Warszawy, gdzie na pensji Marcina Nikuty pobierali nauki i przygotowywali się do przyszłych obowiązków. Ludwika Maria była matką bardzo troskliwą, wymagającą, nie znosiła sprzeciwu, nie zezwalała dzieciom na samodzielne decyzje. Próbowała wpływać na ich życie nawet kiedy były dorosłe. Wszystko w imię interesów rodziny Chodkiewiczów.
Technological entrepreneurship readiness
Authors: Ndofirepi Takawira , Steyn Renier 
Published: February 2024

Technological entrepreneurship presents opportunities for accelerated growth during the Fourth Industrial Revolution and assessing the readiness for such entrepreneurship would be important to investors (interested in profit) and governments (interested in economic growth). The aim was to assess and rank the BRICS (Brazil, Russia, India, China, and South Africa) countries on their level of technological entrepreneurship readiness, as to direct investor funding or alternatively guide government initiatives. Data which was collected in Brazil, Russia, India, China, and South Africa, for the World Values Survey, was used in the study (N=13 895). Mean and composite scores linked to entrepreneurship as well as the embracement of technology were compared across countries. These were combined to generate a score used to rank the countries. With each of the individual, as well as the composite variables, significant differences were found across the BRICS countries. China was rated the highest on attitudes towards science while South Africa was rated highest on the openness to entrepreneurship. On the composite score, technology entrepreneurship readiness, China scored the highest. China was ranked as the BRICS countries most viable for technology entrepreneurship. Technology investors should thus consider directing their venture capital eastward. The governments of the other countries should take note of their shortcomings and the results could inform policies to enhance readiness. The results, at a theoretical level, provided some insights into the conceptualisation of technology-related entrepreneurship.
Scandinavian Style On Illustration of Flora Marimekko
Authors: Putri Citra Kemala 
Published: February 2024

The Scandinavian style is one of the styles that has big influence on the development of interior design, product and visual in the world. The Scandinavian style is influenced by several things including folk culture, as well as local and international historical events. Marimekko is a Finnish and Scandinavian-style pioneered company that was founded in 1951.By today, Marimekko has produced thousands of illustrations which are used as patterns on dresses, home furnishings, etc. The objects those Marimekko's illustrations usually used such as geometric, abstract and floral objects. This study is analizing the influence of the Scandinavian style on the floral illustrations of Marimekko’s pattern illustrations. The case of this study are several Marimekko illustrations entitled "Unikko (Poppy)" and "Maalaisruusuu (Country Roses)" by Maija Isola in 1964, "Ajusko" by Annika Rimala in 1968, "Kuuma (Hot)" by Fujiwo Ishimoto in 1978, “Kylmankukka (Pasque Flower)” by Aino-Maija Metsoia in 2008, “Oodi (Ode)” by Teija Puranen in 2012, and “Hyma (Frost)” by Aino Maija Metsola in 2019 This study uses qualitative method which is supported by various data sources. The results of this study reveal that the way of depicting the illustrations use Naturalist Perspective Momentopname visual language (NPM) dominantly and they contain Scandinavian illustration characteristics. The illustrations used in the Marimekko patterns show a strong character and identity, not only as a brand, but also as cultural identity whch are geographical and communal folk tradition identity.
Domestic Solid Waste and Health related Challenges among men and women: a case of Kiandutu informal settlement, Kiambu County, Kenya
Authors: Mwangi Willy W. , Waweru Lucy W. 
Published: February 2024

Health is a life component that cannot be ignored. In developing economies, the migration of people, both men and women, from rural areas into urban areas results from multiple factors. The social dynamics that include a search for a better life take the lead. This dire and never-ending relocation has led to an ever-increasing mushrooming of informal settlements in the urban areas. Among the devastating consequences is the increase in domestic solid waste and its poor management. This poor domestic solid waste management health challenges is coupled with gendered socialization and perceptions, some knowledge and practices. Social Context Theory was used to guide this study. The theory assumes that there exists flexibility of gender within a defined context. The study employed exploratory research design whose choice allowed an in-depth view of the generation of both qualitative and quantitative data. Random sampling of the villages and purposive sampling of the respondents were used to identify the study sample. A total number of 264 households was used as the sample size. This was a representation of 10% of all the households in the randomly sampled villages with each village being allocated a number of the respondents in regard to gender. The unit of analysis was the household, with the household heads, male and female being the respondents. Key informants were also considered in the study. They included the village elders, community health workers and the local administration. Tools that were considered for the generation of data included observation checklists, guided questionnaires and interview guides. Qualitative data was thematically coded and analysed using SPSS V24. The study concluded that early gendered socialisation has the capacity to contribute to poor methods household solid waste for both men and women, hence contributing to health challenges. The study also observed that inadequate knowledge among men and women in the management of solid waste was linked to inequitable health challenges experienced by both genders in informal settlements. The social realities plug into the dominant arrangements of gendered social behaviour that have great capacity to affect individuals’ health. The findings suggest that gender-sensitive policies can be used to promote community awareness creation and education to modify the behaviour of men and women in protecting their own lives in terms of health
НАЦІЄТВОРЧІ ЗАСАДИ УКРАЇНОМОВНОЇ ОСВІТИ (про результати проведення щорічного вебінару «Рідномовна і багатомовна освіта у контексті сталого розвитку» до Міжнародного дня рідної мови 2024)
Authors: Vovk Myroslava 
Published: February 2024

У повідомленні представлено результати проведення щорічного вебінару «Рідномовна і багатомовна освіта у контексті сталого розвитку суспільства», присвяченого Міжнародному дню рідної мови (15 лютого 2024 р.). Ініціатори заходу — Інститут педагогічної освіти і освіти дорослих імені Івана Зязюна НАПН України, Кафедра ЮНЕСКО «Неперервна професійна освіта ХХІ століття». Співорганізаторами вебінару виступили Секретаріат уповноваженого із захисту рідної мови, Інститут української мови НАН України, Інститут літератури імені Тараса Шевченка НАН України, Всеукраїнське товариство «Просвіта» імені Тараса Шевченка, ГО «Українська асоціація освіти дорослих». Метою вебінару є просвітницька місія партнерства наукових установ, закладів фахової передвищої і вищої освіти, заклади загальної освіти у дієвій реалізації політики україномовного навчання та раціональної підтримки багатомовної освіти; утвердження цінності мови як маркеру української ідентичності в умовах воєнних реалій.Учасники вебінару (понад 180 осіб): громадські діячі, науковці, студенти, магістранти, аспіранти, докторанти, викладачі закладів фахової передвищої і вищої освіти, працівники бібліотек, музейних інституцій (Сумський державний педагогічний університет імені А.С. Макаренка, Уманський державний педагогічний університет імені Павла Тичини, Прикарпатський національний університет імені Василя Стефаника, Ізмаїльський державний гуманітарний університет, Державна науково-педагогічна бібліотека імені В. Сухомлинського НАПН України, Державний ліцей «Міжнародна українська школа» та ін.). Акцентовано увагу на сучасних викликах у контексті утвердження української мови як націєтворчого чинника суспільного поступу.
Bayes Estimator of Exponential Distribution Parameters of Type II Censored Data with Linear Exponential Loss Function Method Based on Jeffrey Priors
Authors: Previan Anggara Teguh , Kurniawan Ardi , Mardianto M. Fariz Fadillah , Sediono Sediono 
Published: February 2024

Survival analysis is often used in the application of analyzing the survival of an object such as living things or objects. This analysis is identical to data censoring which is divided into three, namely: type I, II, and III censored data. Type II censored data is data censoring done by determining the number of objects to be analyzed from the total number of observation objects . Type II censored data is used when the analysis is intended to maximize the results of the analysis. Bayesian Linear Exponential (LINEX) loss function is one method that can be used to estimate parameters in survival analysis by minimizing the expected value of LINEX. The purpose of this study is to determine the Bayesian LINEX loss function parameter estimation on type II censored data using exponential distribution. This method uses the concept of posterior distribution and prior distribution. The prior distribution used is the Jeffrey prior distribution which has objective properties and is based on Fisher information theory The application of the parameter estimation results is carried out on the survival data of lung cancer patients obtained from the North Central Cancer Treatment Group. Based on the results of parameter estimation, it is concluded that the greater the value of the controller (a) can produce a smaller value of parameter estimation results (θ^) . The results of this study can be used as a reference in conducting survival tests using type II censored exponential distribution data using the LINEX loss function method based on Jeffrey priors.
The DECam Ecliptic Exploration Project (DEEP). III. Survey Characterization and Simulation Methods
Authors: Bernardinelli Pedro H. , Smotherman Hayden , Langford Zachary , Portillo Stephen K. N. , Connolly Andrew J. , Kalmbach J. Bryce , Stetzler Steven , Jurić Mario , Oldroyd William J. , Lin 林 Hsing Wen 省文 , Adams Fred C. , Chandler Colin Orion , Fuentes Cesar , Gerdes David W. , Holman Matthew J. , Markwardt Larissa , McNeill Andrew , Mommert Michael , Napier Kevin J. , Payne Matthew J. , Ragozzine Darin , Rivkin Andrew S. , Schlichting Hilke , Sheppard Scott S. , Strauss Ryder , Trilling David E. , Trujillo Chadwick A. 
Published: February 2024

Abstract
We present a detailed study of the observational biases of the DECam Ecliptic Exploration Project’s B1 data release and survey simulation software that enables direct statistical comparisons between models and our data. We inject a synthetic population of objects into the images, and then subsequently recover them in the same processing as our real detections. This enables us to characterize the survey’s completeness as a function of apparent magnitudes and on-sky rates of motion. We study the statistically optimal functional form for the magnitude, and develop a methodology that can estimate the magnitude and rate efficiencies for all survey’s pointing groups simultaneously. We have determined that our peak completeness is on average 80% in each pointing group, and our magnitude drops to 25% of this value at m
25 = 26.22. We describe the freely available survey simulation software and its methodology. We conclude by using it to infer that our effective search area for objects at 40 au is 14.8 deg2, and that our lack of dynamically cold distant objects means that there at most 8 × 103 objects with 60 < a < 80 au and absolute magnitudes H ≤ 8.
The DECam Ecliptic Exploration Project (DEEP). I. Survey Description, Science Questions, and Technical Demonstration
Authors: Trilling David E. , Gerdes David W. , Jurić Mario , Trujillo Chadwick A. , Bernardinelli Pedro H. , Napier Kevin J. , Smotherman Hayden , Strauss Ryder , Fuentes Cesar , Holman Matthew J. , Lin 林 Hsing Wen 省文 , Markwardt Larissa , McNeill Andrew , Mommert Michael , Oldroyd William J. , Payne Matthew J. , Ragozzine Darin , Rivkin Andrew S. , Schlichting Hilke , Sheppard Scott S. , Adams Fred C. , Chandler Colin Orion 
Published: February 2024

Abstract
We present here the DECam Ecliptic Exploration Project (DEEP), a 3 yr NOAO/NOIRLab Survey that was allocated 46.5 nights to discover and measure the properties of thousands of trans-Neptunian objects (TNOs) to magnitudes as faint as VR ∼ 27 mag, corresponding to sizes as small as 20 km diameter. In this paper we present the science goals of this project, the experimental design of our survey, and a technical demonstration of our approach. The core of our project is “digital tracking,” in which all collected images are combined at a range of motion vectors to detect unknown TNOs that are fainter than the single exposure depth of VR ∼ 23 mag. Through this approach, we reach a depth that is approximately 2.5 mag fainter than the standard LSST “wide fast deep” nominal survey depth of 24.5 mag. DEEP will more than double the number of known TNOs with observational arcs of 24 hr or more, and increase by a factor of 10 or more the number of known small (<50 km) TNOs. We also describe our ancillary science goals, including measuring the mean shape distribution of very small main-belt asteroids, and briefly outline a set of forthcoming papers that present further aspects of and preliminary results from the DEEP program.
Chondrule Survivability in the Solar Nebula
Authors: Taki Tetsuo , Wakita Shigeru 
Published: February 2024

Abstract
The lifetime of millimeter-sized dust grains, such as chondrules, in the nominal solar nebula model is limited to ∼105 yr, due to an inward drift driven by gas drag. However, isotopic and petrological studies of primitive meteorites indicate a discrepancy of ≳106 yr between the formation time of chondrules and that of chondritic parent bodies. Therefore, chondrules should survive for ≳106 yr in the solar nebula against the inward drift without subsequent growth (i.e., planetesimal formation). Here, we investigate the conditions of the solar nebula that are suitable for the long lifetime of chondrule-sized dust particles. We take the turbulent strength, the radial pressure gradient force, and the disk metallicity of the solar nebula as free parameters. For 1 mm radius chondrules to survive and keep their size for ≳106 yr, the suitable condition is a weak turbulence (α ∼ 10−6), a flat radial profile (η ≲ 10−3), and a high metallicity (Z ∼ 0.1). This condition is qualitatively consistent with the characteristics of protoplanetary disks suggested by recent observations. We eventually propose that planetesimal formation may be induced by disk evolution, e.g., the inside-out dispersal of the gas component due to the disk wind.
Detection of Asymmetry in the Narrow Fe Kα Emission Line in MCG-5-23-16 with Chandra
Authors: Liu Victor , Zoghbi Abderahmen , Miller Jon M. 
Published: February 2024

Abstract
Iron Kα (Fe Kα) emission is observed ubiquitously in active galactic nuclei (AGN), and it is a powerful probe of their circumnuclear environment. Examinations of the emission line play a pivotal role in understanding the disk geometry surrounding black holes. It has been suggested that the torus and the broad-line region (BLR) are the origins of emission. However, there is no universal location for the emitting region relative to the BLR. Here, we present an analysis of the narrow component of the Fe Kα line in the Seyfert AGN MCG-5-23-16, one of the brightest AGN in X-rays and in Fe Kα emission, to localize the emitting region. Spectra derived from Chandra/HETGS observations show asymmetry in the narrow Fe Kα line, which has only been confirmed before in the AGN NGC 4151. Models including relativistic Doppler broadening and gravitational redshifts are preferred over simple Gaussians and measure radii consistent with R ≃ 200–650 r

g
. These results are consistent with those of NGC 4151 and indicate that the narrow Fe Kα line in MCG-5-23-16 is primarily excited in the innermost part of the optical BLR, or X-ray BLR. Characterizing the properties of the narrow Fe Kα line is essential for studying the disk geometries of the AGN population and mapping their innermost regions.
Clouds and Seasonality on Terrestrial Planets with Varying Rotation Rates
Authors: Williams Daniel A. , Ji 纪 Xuan 璇 , Corlies Paul , Lora Juan M. 
Published: February 2024

Abstract
Using an idealized climate model incorporating seasonal forcing, we investigate the impact of rotation rate on the abundance of clouds on an Earth-like aquaplanet, and the resulting impacts upon albedo and seasonality. We show that the cloud distribution varies significantly with season, depending strongly on the rotation rate, and is well explained by the large-scale circulation and atmospheric state. Planetary albedo displays nonmonotonic behavior with rotation rate, peaking at around 1/2ΩE. Clouds reduce the surface temperature and total precipitation relative to simulations without clouds at all rotation rates, and reduce the dependence of total precipitation on rotation rate, causing nonmonotonic behavior and a local maximum around 1/8ΩE; these effects are related to the impacts of clouds on the net atmospheric and surface radiative energy budgets. Clouds also affect the seasonality. The influence of clouds on the extent of the winter Hadley cell and the intertropical convergence zone is relatively minor at slow rotation rates (<1/8ΩE), but becomes more pronounced at intermediate rotation rates, where clouds decrease their maximum latitudes. The timing of seasonal transitions varies with rotation rate, and the addition of clouds reduces the seasonal phase lag.
IRIS2+: A Comprehensive Database of Stratified Thermodynamic Models in the Low Solar Atmosphere
Authors: Sainz Dalda Alberto , Agrawal Aaryan , De Pontieu Bart , Gošić Milan 
Published: February 2024

Abstract
We present the most comprehensive collection of stratified-in-optical-depth thermodynamic models of the lower solar atmosphere. This database, named IRIS2+, consists of 40,320 synthetic representative profiles (RPs) and their corresponding representative model atmospheres (RMAs). The latter result from inverting the observed RPs, which are the result of clustering multiline spectral profiles observed by the Interface Region Imaging Spectrograph in 126 active regions (ARs). Each AR was clustered in 320 RPs considering five solar features: umbra, pore or pore-like, penumbra, plage, and quiet Sun. The multiline spectral profiles contain 12 lines with encoded physical information from the top of the chromosphere to the midphotosphere. These 12 spectral lines, six chromospheric and six photospheric, were simultaneously inverted with the Stockholm Inversion Code. Therefore, the stratified-in-optical-depth low solar atmosphere models obtained in this study are better constrained than those obtained from the nonsimultaneous inversion of individual lines. Each tuple in the database contains an inverted RP, its corresponding RMA, the solar feature label where the observed RP was clustered, its heliocentric angle, and its date and time of observation. The database may be used as an inversion code for any of the lines present in the RPs, and the RMAs may be used for synthesizing spectral lines in the chromosphere and photosphere or as mean constraints for numerical models of the solar atmosphere.