bluuebunny/crossref_metadata_2025_split huggingface dataset:
"Stylistics of mass media" as an academic discipline in the training process of future journalists
Authors: Bashmanivska Liubov , Bashmanivskyi Valerii 
Published: June 2024

The training process of future journalists is of great importance in higher education institutions. The aim of it is to form creative, competent, innovation-oriented professionals who are good with words, able to express their thoughts and quickly adapt to a multicultural environment, and use knowledge, skills and abilities to succeed. This is due to modern requirements for the journalistic profession, society's demand for professional skills, improving the com­municative and linguistic level of future professionals.
The article examines the issue of studying stylistics of mass media as an academic discipline in the training process of media officers. It also reveals the problem of improving the stylistic skills of journalism students in the process of mastering the course as an important factor in their training. The necessity of work on stylistic dexterity of speech in the context of improving the professional skills of a journalist is substantiated as well.
It points out the importance of stylistics of mass media in the modern teaching process of future media officers as a means of forming a highly educated language personality that a modern journalist should be like.
It is concluded that the stylistics of the media has great communicative potential, which contributes to the communicatively appropriate use of language in the future journalistic profession. Additionally, the study of this educational component will contribute to the assimilation of future journalists of the norms of modern Ukrainian literary language, and the formation of skills to create and edit media texts of different genres and styles. During the study of the educational component "Stylistics of mass media" higher education students master the skills of literate, expressive, clear speech, acquire skills in stylistic editing, use of oral and written forms of all functional styles, following spelling, orthoepic, lexical and grammatical, punctuation, thus improving their communication skills.
IDENTIFIKASI STRATEGI DESTINATION BRANDING KEPULAUAN SERIBU BERBASISKAN WISATA BAHARI
Authors: Rinaldo Edo , Dwihadiah Desideria Lumongga 
Published: June 2024

Penelitian ini bertujuan mengidentifikasikan strategi destination branding Kepulauan Seribu berbasiskan wisata bahari. Strategi destination branding menjadi kunci dalam memperkuat citra destinasi, melibatkan identitas dan keunikan Kepulauan Seribu. Penelitian ini menggunakan konsepsi teori dari identifikasi Kenneth Burke menyoroti peran kunci identitas dalam membentuk persepsi masyarakat terhadap potensi pariwisata. Pendekatan penelitian yang digunakan adalah kualitatif dengan metode deskriptif. Informan penelitian terdiri dari pemerintah yaitu pihak Dinas Pariwisata DKI Jakarta, pelaku usaha yang mengoperasikan jasa pariwisata di Kepulauan Seribu, masyarakat sekaligus penggiat pariwisata di Kepulauan Seribu. Temuan penelitian menunjukkan bahwa, implementasi strategi destination branding Kepulauan Seribu berbasiskan wisata bahari didukung adanya program pariwisata, kearifan lokal, penggunaan media, dan infrastruktur. Hambatan dalam mewujudkan strategi destination branding Kepulauan Seribu berbasiskan wisata bahari terdapat 3 aspek yaitu (1) komunikasi primer (ketidakseimbangan informasi dan keterbatasan akses informasi); (2) komunikasi sekunder (respon negatif dan ketidakjelasan diferensiasi; dan (3) komunikasi tersier (ketidaksesuaian pesan dan medium komunikasi). Peran aktor pariwisata, seperti pemerintah daerah dan pengelola objek wisata, penting dalam menciptakan dan memelihara identitas brand destinasi. Destination marketing organization menjadi upaya pengoordinasian pemangku kepentingan, memastikan kolaborasi harmonis. Konsep identifikasi Kenneth Burke relevan dalam membentuk identitas dan komunikasi dalam konteks destination branding. Dengan keterlibatan terkoordinasi, Kepulauan Seribu dapat membangun citra yang kuat, meningkatkan dampak ekonomi lokal, dan mempromosikan keberlanjutan pariwisata
Kata Kunci: Branding, Kepulauan Seribu, Strategi Destinasi, Wisata bahari
DEVELOPMENT OF SOCIAL MEDIA STRATEGIES IN ONLINE NEWS PUBLISHER INDUSTRY (A Case Study In Kapanlagi Youniverse)
Authors: Husna Nisrin , Pratiwi Sefya Dian 
Published: June 2024

Impact of the COVID-19 pandemic has changed the condition of online news publisher industry both in term of economic and existence. The aim of this research is to find out the condition of social media communication strategy KapanLagi Youniverse as a media group in Indonesia for strengthening brand equity. The theoretical foundation of this research is using the Circular Model of SoMe for Social Communications and Brand Equity’s dimension Theory. The research method that will be used in this research is qualitative research with the design of a study case, which the data collected by interview and observation. The result of this research shows that in the pandemic situation KapanLagi Youniverse (KLY) could rise through strengthening their existence as a media group in Indonesia. Social media communication strategy of KapanLagi Youniverse uses the aspect of share (cross platform social media and type of content), optimize (PESO model), manage (media monitoring and user experience), and engage (interactivity and media community approach) in strengthening brand equity.
Keywords: Social Media Communication Strategy, Online News Publisher Industry, Brand Equity, Pandemic
Crise aiguë thyrotoxique en réanimation
Authors: Bourcier Simon , Coutrot Maxime , Schmidt Matthieu 
Published: June 2024

La crise aigüe thyrotoxique (CAT), ou « orage thyroïdien », est une forme exceptionnelle de thyrotoxicose menaçant le pronostic vital. Le diagnostic de CAT est peu évident à évoquer devant des manifestations cliniques multisystémiques et peu spécifiques. De plus, la pathologie thyroïdienne est méconnue dans 30 à 40% des cas avant la CAT. Elle doit pourtant être rapidement suspectée par le clinicien pour permettre une prise en charge thérapeutique précoce. La CAT est caractérisée par un tableau clinique explosif incluant fréquemment des manifestations cardiaques au premier plan, déterminantes pour le pronostic vital. A l’origine de défaillances d’organe, la CAT nécessite une prise en charge en réanimation en collaboration étroite avec les endocrinologues. Le traitement généralement recommandé est multimodal, visant notamment à diminuer les taux d’hormones circulantes et contrôler les effets tissulaires. Celui-ci doit-être également personnalisé en évitant des choix thérapeutiques potentiellement délétères. En particulier, l’administration des bétabloquants devrait s’accompagner d’une surveillance étroite de la fonction cardiaque en raison de la fréquence du choc cardiogénique. Les échanges plasmatiques et la thyroïdectomie représentent des solutions thérapeutiques de recours pour lesquelles les données publiées ne permettent pas à ce jour de proposer des critères décisionnels ou d’identifier les patients les plus à même d’en bénéficier.
Nephrology nurse practitioner model of care for chronic kidney disease: Lessons learned and informing future healthcare delivery
Authors: Bonner Ann , Stone Cassandra , Purtell Louise , Gillespie Kerri 
Published: June 2024

Background: Chronic kidney disease (CKD) affects more than 10% of the Australian adult population. It is a progressive disease that involves multiple physiological systems and is associated with several comorbid conditions, making it particularly burdensome on patients and the healthcare system. Alternative models of healthcare delivery are required to slow the progression to kidney failure.
Aim: To describe the characteristics, patient profiles, and health outcomes of patients with CKD attending a nephrology nurse practitioner-led clinic.
Design: Longitudinal health-service exploratory design.
Methods: Following ethics approval, data were extracted from a chronic kidney disease registry for all consenting patients who attended a nephrology nurse practitioner-led clinic. Data were analysed descriptively.
Results: Over the study period, 253 patients (122 male and 131 female) attended the clinic. The mean age was 70.27 ± 10.48 years, and at baseline most had either chronic kidney disease grade 3A (32.8%) or 3B (41.5%). For the majority of those who remained in the clinic, kidney function remained stable or slightly improved. A large proportion were within recommended target ranges for systolic (85.6%) and diastolic (98%) blood pressure although many had high BMI (mean 31.99 ± 6.47) and HbA1c (57.1%).
Conclusion: The nephrology nurse practitioner-led clinic demonstrated effectiveness in addressing CKD targets for patients and provides an opportunity to transform traditional primary and specialist healthcare delivery.
What is already known about the topic?

Early intervention in chronic kidney disease (CKD) can slow or halt the progression of the disease, reducing long-term burden and healthcare costs.
An integrated model of care including primary and specialist providers is considered optimal for the early detection and treatment of CKD.
An integrated nephrology nurse practitioner model is an emerging model of care for CKD patients. However, studies investigating the cost-effectiveness, efficacy, and characteristics of this model compared to specialist or primary care in Australia are lacking.

What this paper adds:

This paper describes the characteristics and outcomes of a nephrology nurse practitioner-led outpatient clinic embedded within a multidisciplinary model of care.
The majority of patients who remained in nephrology nurse practitioner care maintained recommended CKD targets.
The findings provide evidence that nephrology nurse practitioners are able to manage patients with less advanced CKD grades who have comorbid conditions and other health risk-factors.
Comparing child word associations to adult associative norms: Evidence for child-specific associations with a strong priming effect in 3-year-olds
Authors: Fitzpatrick Nadine , Floccia Caroline 
Published: June 2024

AbstractInvestigating how infants first establish relationships between words is a necessary step towards understanding how an interconnected network of semantic relationships develops in the adult lexical-semantic system. Stimuli selection for these child studies is critical since words must be both familiar and highly imageable. However, there has been a reliance on adult word association norms to inform stimuli selection in English infant studies to date, as no resource currently exists for child-specific word associations. We present three experiments that explore the strength of word–word relationships in 3-year-olds. Experiment 1 collected children’s word associations (WA) (N = 150; female = 84, L1 = British English) and compared them to adult associative norms (Moss & Older, 1996; Nelson et al., 2004 (Behavior Research Methods, Instruments, & Computers, 36(3), 402–407)). Experiment 2 replicated WAs from Experiment 1 in an online adaptation of the task (N = 24: 13 female, L1 = British English). Both experiments indicated a high proportion of child-specific WAs not represented in adult norms (Moss & Older, 1996; Nelson et al., 2004 (Behavior Research Methods, Instruments, & Computers, 36(3), 402–407)). Experiment 3 tested noun–noun WAs from these responses in an online semantic priming study (N = 40: 19 female, L1 = British English) and found that association type modulated priming (F(2.57, 100.1) = 13.13, p <. 0001, generalized η2 = .19). This research presents a resource of child-specific imageable noun–noun word pair stimuli suitable for testing young children in word recognition and semantic priming studies.
A Self-consistent Treatment of the Line-driving Radiation Force for Active Galactic Nuclei Outflows: New Prescriptions for Simulations
Authors: Lattimer Aylecia S. , Cranmer Steven R. 
Published: June 2024

Abstract
Flows driven by photons have been studied for almost a century, and a quantitative description of the radiative forces on atoms and ions is important for understanding a wide variety of systems with outflows and accretion disks, such as active galactic nuclei (AGN). Quantifying the associated forces is crucial to determining how these outflows enable interactive mechanisms within these environments, such as AGN feedback. The total number of spectral lines in any given ion of the outflow material must be tabulated in order to give a complete characterization of this force. Here, we provide calculations of the dimensionless line force multiplier for AGN environments. For a wide array of representative AGN sources, we explicitly calculate the photoionization balance at the proposed wind-launching region above the accretion disk, compute the strength of the line-driving force on the gas, and revisit and formalize the role of the commonly used ionization parameter ξ in ultimately determining the line-driving force. We perform these computations and analyses for a variety of AGN central source properties, such as black hole mass, initial wind velocity, and number density. We find that, while useful, the ionization parameter provides an incomplete description of the overall ionization state of the outflow material. We use these findings to provide an updated method for calculating the strength of the radiative line-driving using both the X-ray spectral index Γ
X
and the ionization parameter.
Polarization Properties of 128 Nonrepeating Fast Radio Bursts from the First CHIME/FRB Baseband Catalog
Authors: Pandhi Ayush , Pleunis Ziggy , Mckinven Ryan , Gaensler B. M. , Su Jianing , Ng Cherry , Bhardwaj Mohit , Brar Charanjot , Cassanelli Tomas , Cook Amanda , Curtin Alice P. , Kaspi Victoria M. , Lazda Mattias , Leung Calvin , Li Dongzi , Masui Kiyoshi W. , Michilli Daniele , Nimmo Kenzie , Pearlman Aaron B. , Petroff Emily , Rafiei-Ravandi Masoud , Sand Ketan R. , Scholz Paul , Shin Kaitlyn , Smith Kendrick , Stairs Ingrid 
Published: June 2024

Abstract
We present a 400–800 MHz polarimetric analysis of 128 nonrepeating fast radio bursts (FRBs) from the first CHIME/FRB baseband catalog, increasing the total number of FRB sources with polarization properties by a factor of ∼3. A total of 89 FRBs have >6σ linearly polarized detections, 29 FRBs fall below this significance threshold and are deemed linearly unpolarized, and for 10 FRBs, the polarization data are contaminated by instrumental polarization. For the 89 polarized FRBs, we find Faraday rotation measure (RM) amplitudes, after subtracting approximate Milky Way contributions, in the range 0.5–1160 rad m−2 with a median of 53.8 rad m−2. Most nonrepeating FRBs in our sample have RMs consistent with Milky Way–like host galaxies, and their linear polarization fractions range from ≤10% to 100% with a median of 63%. We see marginal evidence that nonrepeating FRBs have more constraining lower limits than repeating FRBs for the host electron-density-weighted line of sight magnetic field strength. We classify the nonrepeating FRB polarization position angle (PA) profiles into four archetypes: (i) single component with constant PA (57% of the sample), (ii) single component with variable PA (10%), (iii) multiple components with a single-constant PA (22%), and (iv) multiple components with different or variable PAs (11%). We see no evidence for population-wide frequency-dependent depolarization, and, therefore, the spread in the distribution of fractional linear polarization is likely intrinsic to the FRB emission mechanism. Finally, we present a novel method to derive redshift lower limits for polarized FRBs without host galaxy identification and test this method on 20 FRBs with independently measured redshifts.
Effects of an Explicit Time-dependent Radiation Pressure Force on Trajectories of Primary Neutral Hydrogen in the Heliosphere
Authors: Dyke Lucas , Müller Hans-Reinhard 
Published: June 2024

Abstract
Radiation pressure exerted by solar photon output is salient to the motion of primary neutral hydrogen atoms streaming into the inner heliosphere directly from the local interstellar medium. The action of a time-dependent radiation pressure force, when coupled with the usual gravitational force, changes the characteristic velocities, and therefore energies, of the atoms when they reach regions in which explorer probes are present. A study is presented that uses a 2D code to backtrace neutral hydrogen trajectories from representative target points located 1 au from the Sun. It makes use of both a radiation pressure function and a function for the photoionization rate at 1 au that both oscillate with time based on measurements over a typical solar cycle, as well as a time-independent charge exchange ionization rate at 1 au. Assuming a Maxwellian distribution in the distant upwind direction, phase space data is calculated at the target points, at different moments in time. The dependence of the force on the radial particle velocity has been omitted in the analysis, such that the emphasis is on the effects of the global solar UV intensity variations through the solar cycle. This process allows for the analysis of direct and indirect Maxwellian components through time and space in the time-dependent force environment. Additionally, pseudo-bound orbits caused by energy losses associated with this force environment are observed, and their properties are evaluated with the aim of determining their effects on potential measurements by explorer probes.
The SDSS-V Black Hole Mapper Reverberation Mapping Project: C iv Broad Absorption Line Acceleration in the Quasar SBS 1408+544
Authors: Wheatley Robert , Grier Catherine J. , Hall Patrick B. , Brandt W. N. , Lotz Jonah , Schneider D. P. , Trump Jonathan R. , Shen Yue , Seaton Lucas M. , Anderson Scott F. , Temple Matthew J. , Assef Roberto , Fries Logan B. , Homayouni Y. , Kakkad Darshan , Koekemoer Anton M. , Martínez-Aldama Mary Loli , Negrete C. Alenka , Ricci Claudio , Bizyaev Dmitry , Brownstein Joel R. , Morrison Sean , Pan Kaike 
Published: June 2024

Abstract
We present the results of an investigation of a highly variable C iv broad absorption line (BAL) feature in spectra of the quasar SBS 1408+544 (z = 2.337) that shows a significant shift in velocity over time. This source was observed as a part of the Sloan Digital Sky Survey (SDSS) Reverberation Mapping project and the SDSS-V Black Hole Mapper Reverberation Mapping project, and has been included in two previous studies, both of which identified significant variability in a high-velocity C iv BAL on timescales of just a few days in the quasar rest frame. Using ∼130 spectra acquired over 8 yr of spectroscopic monitoring with SDSS, we have determined that this BAL is not only varying in strength, but is also systematically shifting to higher velocities. Using cross-correlation methods, we measure the velocity shifts (and corresponding acceleration) of the BAL over a wide range of timescales, measuring an overall velocity shift of

Δ
v
=
−

683

−
84

+
89

km s−1 over the 8 yr monitoring period. This corresponds to an average rest-frame acceleration of a = 1.04

−
0.13

+
0.14

cm s−2, though the magnitude of the acceleration on shorter timescales is not constant throughout. We place our measurements in the context of BAL-acceleration models and examine various possible causes of the observed velocity shift.
Exploring the Properties of Photosphere and Emission Lines for Tidal Disruption Events Based on the Global Solution of Slim Disk and Winds
Authors: Zhang Yuehua , Wu Qingwen , Wu Jiancheng , Cao Xinwu , Lei Weihua 
Published: June 2024

Abstract
The theoretical debris supply rate from a tidal disruption of stars can exceed about 100 times of Eddington accretion rate for a 106−7
M
⊙ supermassive black hole. It is believed that a strong wind will be launched from the disk surface due to the radiation pressure in the case of super-Eddington accretion, which may be one of the mechanisms for the formation of the envelope, as observed in tidal disruption events (TDEs). In this work, we explore the evolution of the envelope that formed from the optical thick winds by solving the global solution of the slim-disk model. Our model can roughly reproduce the typical temperature, luminosity, and size of the photosphere for TDEs. Based on Cloudy modeling, we find that, if only considering the radiation-driven disk wind, the emission line luminosities are normally much lower than the typical observational results, due to the limited atmosphere mass outside the envelope. We propose that the ejection of the outflow from the self-collision of the stellar debris during the circularization may provide enough matter outside the disk-wind photosphere. Our calculated spectra can roughly reproduce the main properties of several typical emission lines (e.g., Hα, Hβ, and He ii), which was applied well to a TDE candidate AT2018dyb.
JWST Reveals a Surprisingly High Fraction of Galaxies Being Spiral-like at 0.5 ≤ z ≤ 4
Authors: Kuhn Vicki , Guo Yicheng , Martin Alec , Bayless Julianna , Gates Ellie , Puleo AJ 
Published: June 2024

Abstract
Spiral arms are one of the most important features used to classify the morphology of local galaxies. The cosmic epoch when spiral arms first appeared contains essential clues to the evolution of disk galaxies. In this Letter, we used James Webb Space Telescope images from the Cosmic Evolution Early Release Science Survey to visually identify spiral galaxies with redshift 0.5 ≤ z ≤ 4 and stellar mass ≥1010
M
⊙. Out of 873 galaxies, 216 were found to have a spiral structure. The spiral galaxies in our sample have higher star formation rates and larger sizes than nonspiral galaxies. We found the observed spiral fraction decreases from 48% at z ∼ 0.75 to 8% at z ∼ 2.75. These fractions are higher than the fractions observed with the Hubble Space Telescope. We even detect possible spiral-like features at redshifts z > 3. We artificially redshifted low-redshift galaxies to high redshifts and reinspected them to evaluate observational effects. By varying the input spiral fraction of the redshifted sample, we found that the input fraction of ∼35% matches the observed fraction at z = 2–3 the best. We are able to rule out spiral fractions being <20% (2σ) and <10% (3σ) for real galaxies at z ∼ 3. This fraction is surprisingly high and implies that the formation of spiral arms, as well as disks, was earlier in the Universe.