bluuebunny/crossref_metadata_2025_split huggingface dataset:
Figurative Language in Tame Impala’s Song Lyrics
Authors: Oktavia Dhea 
Published: May 2024

This study is aimed to identify phrases and clauses containing figurative language in Tame Impala’s song lyrics. The theory of figurative language used in this study is the one proposed by Mezo (metaphor, simile, personification, metonymy, synecdoche, hyperbole, and litotes). A qualitative method through a document analysis strategy was applied to this research. The object of this analysis is based on the lyrics of Tame Impala's songs on the four albums, including Innerspeaker (2010), Lonerism (2012), Currents (2015), and The Slow Rush (2020). The result shows that the most common figurative language found in Tame Impala’s song lyrics is Metaphor (38%), Simile (21%), and Personification (19%). It indicates that most of the song lyrics of Tame Impala visualize comparisons and deepen understanding so that it makes readers increase their critical thinking as well as see old things in new ways.
Overview of self-medication pharmaceutical preparations by the public
Authors: H. Ambo Lau Sulfiyana 
Published: May 2024

Introduction: self-medication is an effort made by an individual to obtain medication and use it without diagnosis, prescription, supervision, or consultation with a doctor to treat certain minor illnesses. Self-medication is self-medication without a doctor's prescription. In disease treatment, risks such as misdiagnosis, use of excessive drug doses, and long-term use can cause adverse effects on patients.
Objective: to determine the description of the public's use of self-medicated pharmaceutical preparations.
Methods: This type of research uses a descriptive method, namely research that includes surveys with data collection in the form of questionnaires with a total of 81 respondents. The sampling method uses Non-Probability Sampling with Purposive Sampling techniques using an open-ended questionnaire format in collecting data and recording reports.
Result: results of research data collection that the description of the use of pharmaceutical preparations by self-medication in the Bung Permai Housing Community is that 81 respondents (100.00%) carry out self-medication, the source of drug information is from print and electronic media, namely 36 respondents (44.45%), the place of purchase of medicine was at the pharmacy/clinic, namely 43 respondents (53.02%), the disease suffered was fever, 23 respondents (28.40%), and the pharmaceutical preparation used was paracetamol, 27 respondents (33.33%).
Conclusion: the description of self-help's use of pharmaceutical preparations in the Permai Community Housing is mostly self-medication. Therefore, there is a need for better education and supervision of using pharmaceutical preparations independently to increase understanding and safety in self-medication. It is hoped that in the future, there will be research on public knowledge and behavior regarding self-medication of pharmaceutical preparations so that changes in respondents' knowledge and behavior can be seen after being given good and correct information.
Metal–semiconductor transition in bilayer graphene by bowl inversion of monofluorosumanene
Authors: Maruyama Mina , Gao Yanlin , Okada Susumu 
Published: May 2024

Abstract
The bowl-shaped hydrocarbon molecule, monofluorosumanene (C21H11F), can act as a molecular switch to control the carrier density of bilayer graphene by flipping its conformation. Our calculations indicate that monofluorosumanene, in which F atom is located outside the curved C–C network (exo-F molecular conformation), induces electron and hole co-doping of 1.5 × 1013 cm−2 in monofluorosumanene-intercalated bilayer graphene because of a large dipole moment normal to the molecular plane of the monofluorosumanene. The intercalated monofluorosumanene does not affect the electronic structure of bilayer graphene when the F atom is located inside the curved C–C network (endo-F conformation) owing to a small out-of-plane dipole moment. The application of an external electric field across the graphene layers promotes bowl inversion between endo-F and exo-F molecular conformations because of the low activation barrier (approximately 800 meV) between these two conformations and the dipole moment normal to the molecular plane of the exo-F conformation.
UPAYA PENINGKATAN KESEHATAN IBU DAN ANAK MELALUI PEMBERDAYAAN PEREMPUAN (PERMAINAN BREASTFEEDING MONOPOLY)
Authors: Hapitria Pepi , Widiyastuti Dyah , Nurlina Neli , Lisnawati  , Widiyanti Rani 
Published: May 2024

Saat ini, pencapaian pemberian ASI eksklusif sebesar 69,7%, memenuhi target tahun 2021 sebesar 45%. Namun, pencapaian ini tidak sama di setiap provinsi di Indonesia. Proses pembelajaran mempengaruhi salah satu penyebabnya. Hasil belajar dapat dipengaruhi oleh media pembelajaran yang menarik dan menyenangkan. Oleh karena itu, sangat penting bagi bidan untuk memberikan edukasi dengan menggunakan media pembelajaran yang tepat. Kegiatan ini merupakan kelas edukasi laktasi, yang diikuti oleh 18 orang ibu hamil. Media edukasi yang digunakan adalah breastfeeding monopoly. Tujuan kegiatan adalah untuk meningkatkan pengetahuan dan sikap ibu hamil tentang manajemen laktasi. Kuesioner yang digunakan sebagai instrument kegiatan adalah meliputi kuesioner pengetahuan dan sikap. Analisis yang dibuat berupa analisis deskriptif, yang ditunjang dengan hasil Focus Group Discussion (FGD). Hasil kegiatan menunjukkan bahwa mayoritas ibu hamil memiliki riwayat pemberian ASI secara ekslusif dan kehamilan lebh dari 2. Hasil pengetahuan dan sikap menunjukkan peningkatan sebelum dan setelah edukasi laktasi melalui permainan monopoly laktasi sebesar 5,6% dan 16,7%
The differential impact of face distractors on visual working memory across encoding and delay stages
Authors: Ye Chaoxiong , Xu Qianru , Pan Zhihu , Nie Qi-Yang , Liu Qiang 
Published: May 2024

AbstractExternal distractions often occur when information must be retained in visual working memory (VWM)—a crucial element in cognitive processing and everyday activities. However, the distraction effects can differ if they occur during the encoding rather than the delay stages. Previous research on these effects used simple stimuli (e.g., color and orientation) rather than considering distractions caused by real-world stimuli on VWM. In the present study, participants performed a facial VWM task under different distraction conditions across the encoding and delay stages to elucidate the mechanisms of distraction resistance in the context of complex real-world stimuli. VWM performance was significantly impaired by delay-stage but not encoding-stage distractors (Experiment 1). In addition, the delay distraction effect arose primarily due to the absence of distractor process at the encoding stage rather than the presence of a distractor during the delay stage (Experiment 2). Finally, the impairment in the delay-distraction condition was not due to the abrupt appearance of distractors (Experiment 3). Taken together, these findings indicate that the processing mechanisms previously established for resisting distractions in VWM using simple stimuli can be extended to more complex real-world stimuli, such as faces.
Status and molecular genetic parameters of papillomavirus infection: individual characteristics and associative links with clinical and morphological factors of cervical cancer
Authors: Mkrtchian L. S. , Kiseleva V. I. , Krikunova L. I. , Boyko B. V. , Gusarova V. R. , Bezyaeva G. P. , Panarina L. V. , Ivanov S. A. , Kaprin A. D. , Zamulaeva I. A. 
Published: May 2024

Purpose of the study. Study of the characteristics of human papillomavirus (HPV) infection, comparison of HPV status, molecular and genetic parameters of HPV high risk (HR) with the clinical and morphological characteristics of cervical cancer.Materials and methods. The study included 240 patients with morphologically verified cervical cancer stages I–III, in whom the presence of HPV DNA of 14 genotypes was examined before treatment; upon detection, viral load (VL), the presence and degree of DNA integration into the genome of the host cell were examined.Results. A number of statistically significant associative relationships have been identified between the molecular and genetic parameters of HPV infection and clinical and morphological indicators of the tumor process, in particular the relationship of HPV-negative CC with age and stage of the disease; HPV infection with several genotypes and HPV genotype – with the histological type of tumor; VL – with age, stage and histological type of tumor. Significant associative connections have been established between the molecular genetic parameters of the virus itself: genotype and level of VL, genotype and integration of HPV DNA into the host genome, as well as a negative linear correlation between VL and the degree of integration.Conclusion. The obtained data on the relationship between the molecular and genetic parameters of HPV infection and traditional prognostic factors can become the basis for further research on the development of prognostic models for the purpose of personalizing multimodal treatment programs.
The Highest-redshift Balmer Breaks as a Test of ΛCDM
Authors: Steinhardt Charles L. , Sneppen Albert , Clausen Thorbjørn , Katz Harley , Rey Martin P. , Stahlschmidt Jonas 
Published: May 2024

Abstract
Recent studies have reported tension between the presence of luminous, high-redshift galaxies and the halo mass functions predicted by standard cosmology. Here, an improved test is proposed using the presence of high-redshift Balmer breaks to probe the formation of early 104–105
M
⊙ baryonic minihalos. Unlike previous tests, this does not depend upon the mass-to-light ratio and has only a slight dependence upon the metallicity, stellar initial mass function, and star formation history, which are all weakly constrained at high redshift. We show that the strongest Balmer breaks allowed at z = 9 using the simplest ΛCDM cosmological model would allow a D
4000 as high as 1.26 under idealized circumstances and D
4000 ≤ 1.14 including realistic feedback models. Since current photometric template fitting to JWST sources infers the existence of stronger Balmer breaks out to z ≳ 11, upcoming spectroscopic follow-up will either demonstrate those templates are invalid at high redshift or imply new physics beyond “vanilla” ΛCDM.
PROJECT-J: JWST Observations of HH46 IRS and Its Outflow. Overview and First Results
Authors: Nisini Brunella , Navarro Maria Gabriela , Giannini Teresa , Antoniucci Simone , Kavanagh Patrick, J. , Hartigan Patrick , Bacciotti Francesca , Caratti o Garatti Alessio , Noriega-Crespo Alberto , van Dishoeck Ewine F. , Whelan Emma T. , Arce Hector G. , Cabrit Sylvie , Coffey Deirdre , Fedele Davide , Eislöffel Jochen , Palumbo Maria Elisabetta , Podio Linda , Ray Tom P. , Schultze Megan , Urso Riccardo G. , Alcalá Juan M. , Bautista Manuel A. , Codella Claudio , Greene Thomas P. , Manara Carlo F. 
Published: May 2024

Abstract
We present the first results of the JWST program PROJECT-J (PROtostellar JEts Cradle Tested with JWST), designed to study the Class I source HH46 IRS and its outflow through NIRSpec and MIRI spectroscopy (1.66–28 μm). The data provide line images (∼6.″6 in length with NIRSpec, and up to ∼20″ with MIRI) revealing unprecedented details within the jet, the molecular outflow, and the cavity. We detect, for the first time, the redshifted jet within ∼90 au from the source. Dozens of shock-excited forbidden lines are observed, including highly ionized species such as [Ne iii] 15.5 μm, suggesting that the gas is excited by high velocity (>80 km s−1) shocks in a relatively high-density medium. Images of H2 lines at different excitations outline a complex molecular flow, where a bright cavity, molecular shells, and a jet-driven bow shock interact with and are shaped by the ambient conditions. Additional NIRCam 2 μm images resolve the HH46 IRS ∼110 au binary system and suggest that the large asymmetries observed between the jet and the H2 wide-angle emission could be due to two separate outflows being driven by the two sources. The spectra of the unresolved binary show deep ice bands and plenty of gaseous lines in absorption, likely originating in a cold envelope or disk. In conclusion, JWST has unraveled for the first time the origin of the HH46 IRS complex outflow demonstrating its capability to investigate embedded regions around young stars, which remain elusive even at near-IR wavelengths.
Fallback Rates in Partial Tidal Disruptions of White Dwarfs by Intermediate-mass Black Holes
Authors: Garain Debojyoti , Sarkar Tapobrata 
Published: May 2024

Abstract
The fallback rate of debris after the partial tidal disruption of a star by an intermediate-mass black hole (IMBH) might provide important signatures of such black holes rather than supermassive ones. Here using smoothed particle hydrodynamics methods, we provide a comprehensive numerical analysis of this phenomenon. We perform numerical simulations of single partial tidal disruptions of solar-mass white dwarfs in parabolic orbits, with a nonspinning 103
M
⊙ IMBH for various values of the impact parameter, and determine the core mass fractions and fallback rates of debris into the IMBH. For supermassive black holes, in full disruption processes, it is known that the late-time fallback rate follows a power law t
−5/3, whereas for partial disruptions, such a rate has recently been conjectured to saturate at a steeper power law t
−9/4, independent of the mass of the remnant core. We show here that for IMBHs, partial disruptions significantly alter this conclusion. That is, the fallback rate at late times does not asymptote to a t
−9/4 power law, and this rate is also a strong function of the core mass. We derive a robust formula for the late-time fallback rate as a function of the core mass fraction, which is independent of the mass of the white dwarf, as we verify numerically by varying it.
Maser Activity of Organic Molecules toward Sgr B2(N)
Authors: Xue Ci , Remijan Anthony , Faure Alexandre , Momjian Emmanuel , Hunter Todd R. , Loomis Ryan A. , Herbst Eric , McGuire Brett 
Published: May 2024

Abstract
At centimeter wavelengths, single-dish observations have suggested that the Sagittarius (Sgr) B2 molecular cloud at the Galactic Center hosts weak maser emission from several organic molecules, including CH2NH, HNCNH, and HCOOCH3. However, the lack of spatial distribution information on these new maser species has prevented us from assessing the excitation conditions of the maser emission as well as their pumping mechanisms. Here, we present a mapping study toward Sgr B2 north (N) to locate the region where the complex maser emission originates. We report the first detection of the Class I methanol (CH3OH) maser at 84 GHz and the first interferometric map of the methanimine (CH2NH) maser at 5.29 GHz toward this region. In addition, we present a tool for modeling and fitting the unsaturated molecular maser signals with non-LTE radiative transfer models and Bayesian analysis using the Markov Chain Monte Carlo approach. These enable us to quantitatively assess the observed spectral profiles. The results suggest a two-chain-clump model for explaining the intense CH3OH Class I maser emission toward a region with low continuum background radiation. By comparing the spatial origin and extent of maser emission from several molecular species, we find that the 5.29 GHz CH2NH maser has a close spatial relationship with the 84 GHz CH3OH Class I masers. This relationship serves as observational evidence to suggest a similar collisional pumping mechanism for these maser transitions.
Light Curves of the Explosion of ONe White Dwarf + CO White Dwarf Merger Remnant and Type Icn Supernovae
Authors: Wu Chengyuan , Zha Shuai , Cai Yongzhi , Zhang Zhengyang , Yang Yi , Xiang Danfeng , Lin Weili , Wang Xiaofeng , Wang Bo 
Published: May 2024

Abstract
Type Icn supernovae (SNe Icn) are a newly detected, rare subtype of interacting stripped-envelope supernovae that show narrow P Cygni lines of highly ionized carbon, oxygen, and neon in their early spectra due to the interactions of the SNe ejecta with dense hydrogen- and helium-deficient circumstellar material (CSM). It has been suggested that SNe Icn may have multiple progenitor channels, such as the explosion of carbon-rich Wolf–Rayet stars or the explosion of stripped-envelope SNe, which undergo binary interactions. Among the SNe Icn, SN 2019jc shows unique properties, and previous work inferred that it may stem from the ultrastripped supernova, but other possibilities still exist. In this work, we aim to simulate the light curves from the explosions of oxygen-neon and carbon-oxygen double white dwarf (WD) merger remnants and to further investigate whether the corresponding explosions can appear as some particular SNe Icn. We generate the light curves from the explosive remnants and analyze the influence of different parameters on the light curves, such as the ejecta mass, explosion energy, mass of 56Ni, and CSM properties. Comparing our results with some SNe Icn, we found that the light curves from the explosions of double WD merger remnants can explain the observable properties of SN 2019jc, from which we infer that this special SN Icn may have a different progenitor. Our results indicate that double WD merger may be an alternative model in producing at least one of the SNe Icn.
Observations of Titan’s Stratosphere during Northern Summer: Temperatures, CH3CN and CH3D Abundances
Authors: Thelen Alexander E. , Nixon Conor A. , Cordiner Martin A. , Lellouch Emmanuel , Vinatier Sandrine , Teanby Nicholas A. , Butler Bryan , Charnley Steven B. , Cosentino Richard G. , de Kleer Katherine , Irwin Patrick G. J. , Gurwell Mark A. , Kisiel Zbigniew , Moreno Raphael 
Published: May 2024

Abstract
Titan’s atmospheric composition and dynamical state have previously been studied over numerous epochs by both ground- and space-based facilities. However, stratospheric measurements remain sparse during Titan’s northern summer and fall. The lack of seasonal symmetry in observations of Titan’s temperature field and chemical abundances raises questions about the nature of the middle atmosphere’s meridional circulation and evolution over Titan’s 29 yr seasonal cycle that can only be answered through long-term monitoring campaigns. Here, we present maps of Titan’s stratospheric temperature, acetonitrile (or methyl cyanide; CH3CN) abundance, and monodeuterated methane (CH3D) abundance following Titan’s northern summer solstice obtained with Band 9 (∼0.43 mm) Atacama Large Millimeter/submillimeter Array observations. We find that increasing temperatures toward high southern latitudes, currently in winter, resemble those observed during Titan’s northern winter by the Cassini mission. Acetonitrile abundances have changed significantly since previous (sub)millimeter observations, and we find that the species is now highly concentrated at high southern latitudes. The stratospheric CH3D content is found to range between 4 and 8 ppm in these observations, and we infer the CH4 abundance to vary between ∼0.9% and 1.6% through conversion with previously measured D/H values. A global value of CH4 = 1.15% was retrieved, lending further evidence to the temporal and spatial variability of Titan’s stratospheric methane when compared with previous measurements. Additional observations are required to determine the cause and magnitude of stratospheric enhancements in methane during these poorly understood seasons on Titan.
Lunar North Polar Cold Traps Based on Diurnally and Seasonally Varying Temperatures
Authors: Schörghofer Norbert , Williams Jean-Pierre , Mazarico Erwan 
Published: May 2024

Abstract
Lunar cold traps are defined by extremely low sublimation rates, such that water ice could have accumulated in them. Here time-averaged sublimation rates are calculated for the north polar region of the Moon based on over 14 years of Diviner surface temperature measurements. Data for each spatial pixel are binned according to subsolar (diurnal) and ecliptic (seasonal) longitude. The cold trap area poleward of 80°N is about 32% larger when defined by a time-average sublimation rate instead of by peak temperature. Apparently sunlit cold traps are identified, e.g., in Lenard Crater, where modeling of direct illumination reveals that the Sun briefly rises above the horizon each Draconic year. The true cold trap area is smaller than what can be determined from Diviner data. Also presented are north polar maps for the potential sublimation rate of relic buried ice and for subsurface cold trapping.
Plasmodium yoelii Infection Enhances the Expansion of Myeloid-Derived Suppressor Cells via JAK/STAT3 Pathway
Authors: Zhu Yiqiang , Zhou Lu , Mo Lengshan , Hong Cansheng , Pan Lingxia , Lin Jie , Qi Yanwei , Tan Simin , Qian Manhongtian , Hu Tengfei , Zhao Yi , Qiu Huaina , Lin Peibin , Ma Xiancai , Yang Quan 
Published: May 2024

Abstract
Myeloid-derived suppressor cells (MDSCs), the negative immune regulators, have been demonstrated to be involved in immune responses to a variety of pathological conditions, such as tumors, chronic inflammation, and infectious diseases. However, the roles and mechanisms underlying the expansion of MDSCs in malaria remain unclear. In this study, the phenotypic and functional characteristics of splenic MDSCs during Plasmodium yoelii NSM infection are described. Furthermore, we provide compelling evidence that the sera from P. yoelii–infected C57BL/6 mice containing excess IL-6 and granulocyte-macrophage colony-stimulating factor promote the accumulation of MDSCs by inducing Bcl2 expression. Serum-induced MDSCs exert more potent suppressive effects on T cell responses than control MDSCs within both in vivo P. yoelii infection and in vitro serum-treated bone marrow cells experiments. Serum treatment increases the MDSC inhibitory effect, which is dependent on Arg1 expression. Moreover, mechanistic studies reveal that the serum effects are mediated by JAK/STAT3 signaling. By inhibiting STAT3 phosphorylation with the JAK inhibitor JSI-124, effects of serum on MDSCs are almost eliminated. In vivo depletion of MDSCs with anti–Gr-1 or 5-fluorouracil significantly reduces the parasitemia and promotes Th1 immune response in P. yoelii–infected C57BL/6 mice by upregulating IFN-γ expression. In summary, this study indicates that P. yoelii infection facilitates the accumulation and function of MDSCs by upregulating the expression of Bcl2 and Arg1 via JAK/STAT3 signaling pathway in vivo and in vitro. Manipulating the JAK/STAT3 signaling pathway or depleting MDSCs could be promising therapeutic interventions to treat malaria.