bluuebunny/crossref_metadata_2025_split huggingface dataset:
FORMATION OF STUDENTS’ VALUE ORIENTATIONS IN THE PROCESS OF PATRIOTIC EDUCATION IN PRIMARY SCHOOL
Authors: Шиканова А.Н. 
Published: June 2023

В данной статье рассматривается насущная проблема современности – формирование ценностных ориентаций у младших школьников в процессе патриотического воспитания. Актуальность исследования обусловлена целевым ориентиром, который задан ФГОС общего начального образования, а также неразработанностью ценностного компонента содержания патриотического воспитания с точки зрения его научно-практической составляющей. Научная новизна исследования состоит в рассмотрении формирования ценностных ориентаций в начальной школе с позиции патриотического воспитания. Цель статьи – научное обоснование педагогических условий формирования ценностных ориентаций у младших школьников в процессе патриотического воспитания. Ключевым аспектом патриотического воспитания является его ценностная составляющая, направленная на формирование у младших школьников таких черт, как гордость за культуру своей страны, любовь, преданность и готовность встать за защиту своей Родины, своего Отечества, что соотносится с сущностью ценностных ориентаций. Представленные в статье материалы отражают практический опыт формирования ценностных ориентаций обучающихся в современной начальной школе на основе реализации выявленных автором педагогических условий, которые обеспечивают эффективность данного процесса, что доказано результатами исследования. Статья представляет интерес для исследователей в области общей педагогики, работников сферы образования.
This article deals with the actual problem of our time, which is the formation of value orientations among younger pupils in the process of patriotic education. The relevance of the study is due to the goal, which is set by the Federal State Educational Standard of General Primary Education, as well as the lack of development of the value component of the content of patriotic education in terms of its scientific and practical component. Scientific novelty consists in considering the formation of value orientations in primary school from the point of patriotic education. The purpose of the article is a scientific substantiation of the pedagogical conditions for the formation of value orientations among younger schoolchildren in the process of patriotic education. The key aspect of patriotic education is its value component, which guides the formation of such traits in junior schoolchildren as pride in the culture of their country, love, devotion and readiness to stand up for the defense of their Motherland, their Fatherland, which correlates with the essence of value orientations. The presented materials of the article reflect the practical experience in the formation of value orientations of students in a modern primary school based on the implementation of the pedagogical conditions identified by the author, the implementation of which ensures the effectiveness of this process, which is proved by the results of the study. The article is of interest to researchers in the field of general pedagogy and educators.
THE USE OF FREE ASSOCIATIVE EXPERIMENT WHEN WORKING WITH RUSSIAN LEXICAL UNITS (ON THE EXAMPLE OF STUDENTS FROM LATIN AMERICA)
Authors: Яниева К.Д. , Митрофанова И.И. 
Published: June 2023

В настоящее время продолжаются начатые методистами много лет назад поиски действенного и по-настоящему эффективного метода изучения материала. Современные подходы к усвоению лексических единиц требуют не только классических методов запоминания, но и взаимодействия с психологическим аспектом в виде сознательного и бессознательного. Актуальность данной работы обусловлена именно такой необходимостью, поскольку современная педагогика нуждается в соответствующих времени решениях проблем при работе с иностранной аудиторией. Одной из подобных проблем может являться недостаточный словарный запас. Свободный ассоциативный эксперимент призван облегчить восприятие русской лексики представителями другой культуры через призму их особенностей. В статье раскрывается основная идея свободного ассоциативного эксперимента как в общем, так и в лингвистическом аспекте, а также рассматривается его использование в рамках изучения лексики русского языка в испаноязычной аудитории. Кроме того, авторами самостоятельно был проведен свободный ассоциативный эксперимент среди студентов из стран Латинской Америки, который продемонстрировал и доказал не только важность восприятия языкового материала, но и необходимость учета таких аспектов, как возраст, гендер, академические и географическиеособенности учащихся, поскольку именно они формируют особое восприятие языка, который является неотъемлемой частью культуры.
Nowadays, the search for an efficient and truly effective method of studying the material, which was begun by methodologists many years ago, continues up to now. Modern approaches to the assimilation of lexical units require not only classical methods of memorization, but also interaction with the psychological aspect in the form of conscious and unconscious. This work is topical because modern pedagogy needs solutions to problems concerning work with foreign students. One of these difficulties is insufficient vocabulary. The free associative experiment is aimed to help foreigners to understand Russian vocabulary through the prism of their cultural differences. The article reveals the main idea of the free associative experiment, both in general and in its linguistic aspect, and discusses its use in the study of the vocabulary of the Russian language in the Spanish-speaking audience. The authors have also independently carried out a free associative experiment with the students from Latin America, which showed and proved not only the importance of perception of the linguistic material, but also the need to take into account such aspects as age, gender, academic and geographical characteristics of the students, because they form a special perception of language, which is an integral part of culture.
Perancangan dan Implementasi Sistem E-Commerce berbasis Web pada UMKM Al Haadziq di Kabupaten Malang
Authors: Gita Indah Marthasari  , Mahar Faiqurahman  , Luqman Hakim  
Published: June 2023

Pandemi Covid-19 yang melanda Indonesia memberi dampak signifikan terhadap keberlangsungan Usaha Mikro Kecil dan Menengah (UMKM). Namun, pandemi juga mendatangkan peluang kepada pelaku UMKM untuk memanfaatkan teknologi informasi dan komunikasi (TIK) sebagai support sytem bagi usahanya. Al Haadziq Team merupakan UMKM yang bergerak di bidang penjualan produk perawatan kulit. Selama ini, promosi dan transaksi penjualan produknya dilakukan melalui media sosial yaitu aplikasi WhatsApp. Untuk memperluas jangkauan pemasaran, pada kegiatan ini dirancang dan dibangun sebuah sistem e-commerce berbasis web yang diharapkan dapat menjadi media pemasaran yang strategis. Metode pelaksanaan diawali dengan analisis persoalan, pembuatan dan pengujian website. Analisis situasi dilakukan melalui observasi dan wawancara kepada pengguna. Selanjutnya, dilakukan rancang bangun aplikasi web dengan fitur-fitur antara lain manajemen katalog dan pemesanan produk. Berdasarkan hasil pengujian, disimpulkan bahwa web e-commerce telah sesuai dengan pengguna.
A Generalist, Automated ALFALFA Baryonic Tully–Fisher Relation
Authors: Ball Catie J. , Haynes Martha P. , Jones Michael G. , Peng Bo , Durbala Adriana , Koopmann Rebecca A. , Ribaudo Joseph , O’Donoghue Aileen A. 
Published: June 2023

Abstract
The baryonic Tully–Fisher relation (BTFR) has applications in galaxy evolution as a test bed for the galaxy–halo connection and in observational cosmology as a redshift-independent secondary distance indicator. This analysis leverages the 31,000+ galaxy Arecibo Legacy Fast ALFA (Arecibo L-band Feed Array) Survey (ALFALFA) sample—which provides redshifts, velocity widths, and H i content for a large number of gas-bearing galaxies in the local universe—to fit and test an extensive local universe BTFR. The fiducial relation is fit using a 3000-galaxy subsample of ALFALFA, and is shown to be consistent with the full sample. This BTFR is designed to be as inclusive of ALFALFA and comparable samples as possible. Velocity widths measured via an automated method and M

b
proxies extracted from survey data can be uniformly and efficiently measured for other samples, giving this analysis broad applicability. We also investigate the role of sample demographics in determining the best-fit relation. We find that the best-fit relations are changed significantly by changes to the sample mass range and to second order by changes to mass sampling, gas fraction, different stellar mass and velocity width measurements. We use a subset of ALFALFA with demographics that reflect the full sample to measure a robust BTFR slope of 3.30 ± 0.06. We apply this relation and estimate source distances, finding general agreement with flow-model distances as well as average distance uncertainties of ∼0.17 dex for the full ALFALFA sample. We demonstrate the utility of these distance estimates by applying them to a sample of sources in the Virgo vicinity, recovering signatures of infall consistent with previous work.
Improved Tomographic Binning of 3 × 2 pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
Authors: Moskowitz Irene , Gawiser Eric , Bault Abby , Broussard Adam , Newman Jeffrey A. , Zuntz Joe ,   The LSST Dark Energy Science Collaboration
Published: June 2023

Abstract
Large imaging surveys, such as the Legacy Survey of Space and Time, rely on photometric redshifts and tomographic binning for 3 × 2 pt analyses that combine galaxy clustering and weak lensing. In this paper, we propose a method for optimizing the tomographic binning choice for the lens sample of galaxies. We divide the CosmoDC2 and Buzzard simulated galaxy catalogs into a training set and an application set, where the training set is nonrepresentative in a realistic way, and then estimate photometric redshifts for the application sets. The galaxies are sorted into redshift bins covering equal intervals of redshift or comoving distance, or with an equal number of galaxies in each bin, and we consider a generalized extension of these approaches. We find that bins of equal comoving distance produce the highest dark energy figure of merit of the initial binning choices, but that the choice of bin edges can be further optimized. We then train a neural network classifier to identify galaxies that are either highly likely to have accurate photometric redshift estimates or highly likely to be sorted into the correct redshift bin. The neural network classifier is used to remove poor redshift estimates from the sample, and the results are compared to the case when none of the sample is removed. We find that the neural network classifiers are able to improve the figure of merit by ∼13% and are able to recover ∼25% of the loss in the figure of merit that occurs when a nonrepresentative training sample is used.
A Gaia Data Release 3 View on the Tip of the Red Giant Branch Luminosity
Authors: Li Siyang , Casertano Stefano , Riess Adam G. 
Published: June 2023

Abstract
The tip of the red giant branch (TRGB) is a standard candle that can be used to help refine the determination of the Hubble constant. Gaia Data Release 3 (DR3) provides synthetic photometry constructed from low-resolution BP/RP spectra for Milky Way field stars that can be used to directly calibrate the luminosity of the TRGB in the Johnson–Cousins I band, where the TRGB is least sensitive to metallicity. We calibrate the TRGB luminosity using a two-dimensional maximum likelihood algorithm with field stars and Gaia synthetic photometry and parallaxes. For a high-contrast and low-contrast break (characterized by the values of the contrast parameter R or the magnitude of the break β), we find M
TRGB

I
= −4.02 and −3.92 mag respectively, or a midpoint of −3.970

−
0.024

+
0.042

(sys) ± 0.062 (stat) mag. This measurement improves upon the TRGB measurement from Li et al., as the higher precision photometry based on Gaia DR3 allows us to constrain two additional free parameters of the luminosity function. We also investigate the possibility of using Gaia DR3 synthetic photometry to calibrate the TRGB luminosity with ω Centauri, but find evidence of blending within the inner region for cluster member photometry that precludes accurate calibration with Gaia DR3 photometry. We instead provide an updated TRGB measurement of m
TRGB

I
= 9.82 ± 0.04 mag in ω Centauri using ground-based photometry from the most recent version of the database described in Stetson et al., which gives M
TRGB

I
= −3.97 ± 0.04 (stat) ± 0.10 (sys) mag when tied to the Gaia EDR3 parallax distance from the consensus of Vasiliev & Baumgardt, Soltis et al., and Maíz Apellániz.
Using Dark Energy Explorers and Machine Learning to Enhance the Hobby–Eberly Telescope Dark Energy Experiment
Authors: House Lindsay R. , Gebhardt Karl , Finkelstein Keely , Cooper Erin Mentuch , Davis Dustin , Ciardullo Robin , Farrow Daniel J , Finkelstein Steven L. , Gronwall Caryl , Jeong Donghui , Johnson L. Clifton , Liu Chenxu , Thomas Benjamin P. , Zeimann Gregory 
Published: June 2023

Abstract
We present analysis using a citizen science campaign to improve the cosmological measures from the Hobby–Eberly Telescope Dark Energy Experiment (HETDEX). The goal of HETDEX is to measure the Hubble expansion rate, H(z), and angular diameter distance, D
A(z), at z = 2.4, each to percent-level accuracy. This accuracy is determined primarily from the total number of detected Lyα emitters (LAEs), the false positive rate due to noise, and the contamination due to [O ii] emitting galaxies. This paper presents the citizen science project, Dark Energy Explorers (https://www.zooniverse.org/projects/erinmc/dark-energy-explorers), with the goal of increasing the number of LAEs and decreasing the number of false positives due to noise and the [O ii] galaxies. Initial analysis shows that citizen science is an efficient and effective tool for classification most accurately done by the human eye, especially in combination with unsupervised machine learning. Three aspects from the citizen science campaign that have the most impact are (1) identifying individual problems with detections, (2) providing a clean sample with 100% visual identification above a signal-to-noise cut, and (3) providing labels for machine-learning efforts. Since the end of 2022, Dark Energy Explorers has collected over three and a half million classifications by 11,000 volunteers in over 85 different countries around the world. By incorporating the results of the Dark Energy Explorers, we expect to improve the accuracy on the D
A(z) and H(z) parameters at z = 2.″4 by 10%–30%. While the primary goal is to improve on HETDEX, Dark Energy Explorers has already proven to be a uniquely powerful tool for science advancement and increasing accessibility to science worldwide.
Surrogate Forward Models for Population Inference on Compact Binary Mergers
Authors: Riley Jeff , Mandel Ilya 
Published: June 2023

Abstract
Rapidly growing catalogs of compact binary mergers from advanced gravitational wave detectors allow us to explore the astrophysics of massive stellar binaries. Merger observations can constrain the uncertain parameters that describe the underlying processes in the evolution of stars and binary systems in population models. In this paper, we demonstrate that binary black hole populations—in particular, their detection rates, chirp masses, and redshifts—can be used to measure cosmological parameters describing the redshift-dependent star formation rate and metallicity distribution. We present a method that uses artificial neural networks to emulate binary population synthesis computer models, and construct a fast, flexible, parallelizable surrogate model that we use for inference.
Gemini Near Infrared Spectrograph–Distant Quasar Survey: Augmented Spectroscopic Catalog and a Prescription for Correcting UV-based Quasar Redshifts
Authors: Matthews Brandon M. , Dix Cooper , Shemmer Ohad , Brotherton Michael S. , Myers Adam D. , Andruchow I. , Brandt W. N. , Gallagher S. C. , Green Richard , Lira Paulina , McLane Jacob N. , Plotkin Richard M. , Richards Gordon T. , Runnoe Jessie C. , Schneider Donald P. , Strauss Michael A. 
Published: June 2023

Abstract
Quasars at z ≳ 1 most often have redshifts measured from rest-frame ultraviolet emission lines. One of the most common such lines, C iv
λ1549, shows blueshifts up to ≈5000 km s−1 and in rare cases even higher. This blueshifting results in highly uncertain redshifts when compared to redshift determinations from rest-frame optical emission lines, e.g., from the narrow [O iii] λ5007 feature. We present spectroscopic measurements for 260 sources at 1.55 ≲ z ≲ 3.50 having −28.0 ≲ M

i
≲ − 30.0 mag from the Gemini Near Infrared Spectrograph–Distant Quasar Survey (GNIRS-DQS) catalog, augmenting the previous iteration, which contained 226 of the 260 sources whose measurements are improved upon in this work. We obtain reliable systemic redshifts based on [O iii] λ5007 for a subset of 121 sources, which we use to calibrate prescriptions for correcting UV-based redshifts. These prescriptions are based on a regression analysis involving C iv full-width-at-half-maximum intensity and equivalent width, along with the UV continuum luminosity at a rest-frame wavelength of 1350 Å. Applying these corrections can improve the accuracy and the precision in the C iv-based redshift by up to ∼850 km s−1 and ∼150 km s−1, respectively, which correspond to ∼8.5 and ∼1.5 Mpc in comoving distance at z = 2.5. Our prescriptions also improve the accuracy of the best available multifeature redshift determination algorithm by ∼100 km s−1, indicating that the spectroscopic properties of the C iv emission line can provide robust redshift estimates for high-redshift quasars. We discuss the prospects of our prescriptions for cosmological and quasar studies utilizing upcoming large spectroscopic surveys.
CEERS Key Paper. VI. JWST/MIRI Uncovers a Large Population of Obscured AGN at High Redshifts
Authors: Yang 杨 G. 光 , Caputi K. I. , Papovich C. , Arrabal Haro P. , Bagley M. B. , Behroozi P. , Bell E. F. , Bisigello L. , Buat V. , Burgarella D. , Cheng Y. , Cleri N. J. , Davé R. , Dickinson M. , Elbaz D. , Ferguson H. C. , Finkelstein S. L. , Grogin N. A. , Hathi N. P. , Hirschmann M. , Holwerda B. W. , Huertas-Company M. , Hutchison T. A. , Iani E. , Kartaltepe J. S. , Kirkpatrick A. , Kocevski D. D. , Koekemoer A. M. , Kokorev V. , Larson R. L. , Lucas R. A. , Pérez-González P. G. , Rinaldi P. , Shen L. , Trump J. R. , de la Vega A. , Yung L. Y. A. , Zavala J. A. 
Published: June 2023

Abstract
Mid-infrared (mid-IR) observations are powerful in identifying heavily obscured active galactic nuclei (AGN) that have weak emission in other wavelengths. Data from the Mid-Infrared Instrument (MIRI) on board the James Webb Space Telescope provides an excellent opportunity to perform such studies. We take advantage of the MIRI imaging data from the Cosmic Evolution Early Release Science Survey to investigate the AGN population in the distant universe. We estimate the source properties of MIRI-selected objects by utilizing spectral energy distribution (SED) modeling, and classify them into star-forming galaxies (SFs), SF-AGN mixed objects, and AGN. The source numbers of these types are 433, 102, and 25, respectively, from four MIRI pointings covering ∼9 arcmin2. The sample spans a redshift range of ≈0–5. We derive the median SEDs for all three source types, respectively, and publicly release them. The median MIRI SED of AGN is similar to the typical SEDs of hot dust-obscured galaxies and Seyfert 2s, for which the mid-IR SEDs are dominated by emission from AGN-heated hot dust. Based on our SED-fit results, we estimate the black hole accretion density (BHAD; i.e., total BH growth rate per comoving volume) as a function of redshift. At z < 3, the resulting BHAD agrees with the X-ray measurements in general. At z > 3, we identify a total of 27 AGN and SF-AGN mixed objects, leading to that our high-z BHAD is substantially higher than the X-ray results (∼0.5 dex at z ≈ 3–5). This difference indicates MIRI can identify a large population of heavily obscured AGN missed by X-ray surveys at high redshifts.
Le rôle de l’État (de droit)
Authors: Moine André 
Published: June 2023

Un des moyens pour les États de contribuer à la vie de la Convention, c’est-à-dire d’en favoriser l’application effective, est de respecter l’État de droit ou d’être un État de droit ; ceci conformément à « leur attachement sincère à la prééminence du droit » proclamé dans le préambule de la Convention. La résolution des États à instaurer, développer, préserver l’État de droit, notamment pour correspondre aux exigences de la Convention telle qu’interprétée par la Cour ou par les juridictions nationales en amont, est en effet déterminante pour la réalisation de la Convention. L’État de droit formel se matérialise par deux éléments principaux, la primauté du droit et un contrôle juridictionnel effectif et indépendant, deux exigences qui sont des ressources vitales pour la Convention. À ces fins, les États renforcent leur caractère « de droit » en modifiant leur réglementation par des révisions constitutionnelles, par l’adoption de lois, par l’évolution de la jurisprudence ou par la modification de pratiques, notamment dans le domaine des recours internes. Les décisions de la Cour européenne des droits de l’homme constituent un moteur de ces évolutions nationales en faveur du respect de la primauté du droit et de contrôles juridictionnels effectifs et indépendants ; perfectionnements étatiques qui contribuent – cercle vertueux – au respect des dispositions de la Convention européenne des droits de l’homme et maintiennent donc cette dernière « en vie ».
H. L. A. Hart et J. Rawls : langage ordinaire et abstention métaphysique en philosophie politique
Authors: Guillarme Bertrand 
Published: June 2023

Le texte cherche à souligner plusieurs correspondances entre les philosophies pratiques de H. L. A. Hart et de J. Rawls. Il montre comment, sur plusieurs thématiques, leur réflexion cherche à éviter une fondation métaphysique de la normativité, en puisant dans les ressources du langage ordinaire et de sa philosophie. Il commence par évoquer la réflexion commune de Hart et de Rawls sur le concept de règles sociales, avant d’analyser le statut épistémologique des principes normatifs qu’ils avancent. Il s’intéresse ensuite à la manière dont les deux auteurs envisagent l’autonomie des agents, et à l’articulation qu’ils imaginent entre autonomie individuelle et normativité sociale. Il conclut en évoquant la justification philosophique des droits, que Hart et Rawls cherchent tous deux à aborder à partir de lectures non métaphysiques de Kant, en cherchant à s’appuyer sur les différentes manières dont le langage ordinaire rend compte du fait « d’avoir un droit ».