bluuebunny/crossref_metadata_2025_split huggingface dataset:
Emotional Intelligence in Science
Authors: Yang Yunhan , Zhang Chenwei , Ding Ying 
Published: October 2023

ABSTRACTThis is the first on‐going project presenting a four‐dimension metric to identify scholars' emotional intelligence (EI), which has yet to receive much attention. Current study proposes a data‐driven metric rather than a subjective survey to reflect EI's first dimension, self‐awareness. By employing paired‐T‐tests on the DBLP dataset, we found that highly self‐aware scholars are more likely to strive to improve with higher stability, leading to higher productivity and impact. Meanwhile, they have a more significant number of higher diverse collaborators. This research highlights the importance of one's self‐awareness to his/her scientific performance.
Health Information Use of Older Adults with Diabetes: A Preliminary Analysis
Authors: Zhang Xiaoqian , Bartlett Joan C. 
Published: October 2023

ABSTRACTThis poster presents research investigating the health information use of older adults with diabetes in the context of the COVID‐19 pandemic. Data were collected using semi‐structured interviews and were analyzed using thematic analysis. Results‐to‐date showed self‐reported changes in using health information during the pandemic; that is, some participants endeavored to protect themselves during the pandemic, they carefully made health‐related decisions, and they had a challenging time following their caregivers' suggestions (e.g., taking medicine and exercising) even though they knew they should. However, other participants reported no changes during the pandemic.
Drivers of the Virality of COVID‐19 Misinformation Sharing on Social Media
Authors: Zhao Yuehua , Da Jingwei , Yan Jiaqi , Wang Hao , Deng Sanhong , Chen Ye 
Published: October 2023

ABSTRACTDuring global health crises, identifying the key factors of the misinformation dissemination process on social media can provide decision support for public health management. Drawing on the elaboration likelihood model (ELM), this study characterizes the effects of content types and social capital of social media users on the virality of misinformation related to the COVID‐19 pandemic. We used scale, depth, and width to quantify the extent and structure of the virality of misinformation spreading on social media. The findings reveal that both the social capital of users and the content types have major influences on the dissemination of misinformation. Surprisingly, we discovered that the number of followers a user possesses has a varied influence on the dissemination scale, width, and depth, demonstrating the importance of considering dissemination structure.
A Framework for the Unsupervised and Semi-Supervised Analysis of Visual Frames
Authors: Torres Michelle 
Published: October 2023

AbstractThis article introduces to political science a framework to analyze the content of visual material through unsupervised and semi-supervised methods. It details the implementation of a tool from the computer vision field, the Bag of Visual Words (BoVW), for the definition and extraction of “tokens” that allow researchers to build an Image-Visual Word Matrix which emulates the Document-Term matrix in text analysis. This reduction technique is the basis for several tools familiar to social scientists, such as topic models, that permit exploratory, and semi-supervised analysis of images. The framework has gains in transparency, interpretability, and inclusion of domain knowledge with respect to other deep learning techniques. I illustrate the scope of the BoVW by conducting a novel visual structural topic model which focuses substantively on the identification of visual frames from the pictures of the migrant caravan from Central America.
Biogeography and diversification of the Caribbean clade of Miconia (Melastomataceae): a Cuban origin underlies one of the largest Antillean radiations
Authors: Majure Lucas C , Bacci Lucas F , Bécquer Eldis R , Judd Walter S , Clase Teodoro , Skean J Dan , Michelangeli Fabián A 
Published: October 2023

Abstract
The Greater Antilles are renowned as a biodiversity hotspot and known to be geologically complex, which has led, in part, to the generation of organismal diversity in this area. One of the most species-rich montane groups within the Greater Antilles is the tribe Miconieae (Miconia s.l.) of the Melastomataceae, with ca. 325 species found there. The most diverse clade of Miconia in the Caribbean, the Caribbean clade, composes roughly half of that diversity, with an estimated 160 species, nearly all of which are endemic to the Greater Antilles. It is unclear how that diversity has been generated through time or where it originated, but we now have sufficiently well-sampled and robust datasets to test these patterns. Using a custom-built plastome dataset, we generated a robust phylogenetic hypothesis for 106 of the 160 Caribbean clade members and tested biogeographical patterns among the islands. Our results suggest that the Caribbean clade originated in the mid-Miocene, probably from a South American ancestor, and diversified substantially on the island of Cuba before repeatedly dispersing across other parts of the Greater Antilles, especially into nearby Hispaniola and then, to a lesser extent, into Jamaica, Puerto Rico and, finally, into the Lesser Antilles.
Debt and demand regimes in simplified growth models: a comparison of neo-Kaleckian and Supermultiplier models
Authors: Brochier Lídia , Freitas Fabio 
Published: October 2023

Abstract
The paper compares stock-flow consistent (SFC) versions of extended canonical neo-Kaleckian and Supermultiplier models that deal with either households’ or firms’ debt accumulation. This comparison aim is twofold: (i) to evaluate the differences of a debt accumulation process in these models due to their specific closures; (ii) to provide a pedagogical tool for understanding the basic features of each model when dealing with similar issues. In the short run, we find that the relation of debt ratios, demand and growth is similar for both models. In the long run of the Supemultiplier model, only the Minskyan debt regime is economically viable for the firms’ sector. As for the household sector, the paradox of debt is indeed a feature of the canonical Supermultiplier model, yet there may be episodes of rising debt-toincome ratios. As for the neo-Kaleckian model, firms’ leverage ratio can be either pro- or anti-cyclical; in the household sector, the absence of the paradox of debt seems to be the most likely scenario.
Coronary air embolism during transcatheter patent foramen ovale closure for platypnea-orthodeoxia syndrome in a patient with severe respiratory disorder: a case report
Authors: Tanimura Kosuke , Yamamoto Hiroyuki , Hirata Ken-Ichi , Otake Hiromasa 
Published: October 2023

Abstract

Background
Coronary air embolism (CAE) is a rare and life-threatening complication of endovascular procedures, mostly due to procedure-related causes.

Case summary
A 70-year-old man with severe respiratory disorder presented with patent foramen ovale (PFO)-related platypnea-orthodeoxia syndrome (POS). Transcatheter PFO closure was performed under local anaesthesia and intracardiac echocardiographic guidance. After a 5-Fr catheter was passed through the PFO via a 7-Fr femoral vein sheath, the patient suddenly coughed and breathed deeply. Thereafter, intracardiac echocardiography showed massive microbubbles in all cardiac chambers and the ascending aorta, and an electrocardiogram showed ST-segment elevations in the anterior and inferior leads. Emergency coronary angiography confirmed occlusion of the mid-left anterior descending artery, suggesting CAE. As the intracoronary infusion of saline, nitroglycerine, and nicorandil was ineffective, we performed air aspiration using a thrombectomy device, achieving coronary blood flow improvement and ST-segment resolution. Thereafter, positive pressure support using manual bag-valve-mask ventilation under intravenous sedation supported successful transcatheter PFO closure without further air embolization.

Discussion
In this case with severe respiratory dysfunction, spontaneous deep breathing (spontaneous Valsalva manoeuvre) caused negative intrathoracic pressure and large drops in intravascular pressure. This phenomenon might have induced air contamination during device advancement, either by entrapping or leaving residual air in the gaps between the catheter and the sheath. Additionally, PFO with right-to-left shunts is more likely to cause paradoxical air embolization. Thus, the spontaneous Valsalva manoeuvre should be avoided with appropriate respiratory management to prevent paradoxical air embolization, including CAE, during transcatheter PFO closure under local anaesthesia in severe respiratory dysfunction patients.
A dual-process perspective on the relationship between implicit attitudes and discriminatory behaviour
Authors: Tutić Andreas , Grehl Sascha , Liebe Ulf 
Published: October 2023

Abstract
The dual-process perspective (DPP), which contrasts intuitive and deliberative cognitive processes, has advanced our understanding of the conditions under which cultural orientations, such as implicit attitudes, influence overt behaviour considerably. We test a central tenet of the DPP using a choice experiment on the placement of trust in hypothetical economic transactions. According to the principle of catalyzation, the impact of implicit cultural orientations on overt behaviour should be greater if the behaviour comes about in an intuitive rather than a deliberative manner. In this study, we focus on the implicit attitudes towards class and ethnicity and measure their impact on social behaviour via estimates of the effects of corresponding attributes within the choice experiment. Using a framing technique to experimentally induce intuitive or reflective responses, we find that implicit attitudes affect the placement of trust in the intuitive framing condition but not in the reflective framing condition. Besides providing a strict test of a central tenet of the DPP in a choice-experimental set-up, our study also sheds light on different cognitive mechanisms underlying discriminatory behaviour.
A high-quality genome for the slender anole (Anolis apletophallus): an emerging model for field studies of tropical ecology and evolution
Authors: Pirani Renata M , Arias Carlos F , Charles Kristin , Chung Albert K , Curlis John David , Nicholson Daniel J , Vargas Marta , Cox Christian L , McMillan W Owen , Logan Michael L 
Published: October 2023

Abstract
The slender anole, Anolis apletophallus, is a small arboreal lizard of the rainforest understory of central and eastern Panama. This species has been the subject of numerous ecological and evolutionary studies over the past 60 years as a result of attributes that make it especially amenable to field and laboratory science. Slender anoles are highly abundant, short-lived (nearly 100% annual turnover), easy to manipulate in both the lab and field, and are ubiquitous in the forests surrounding the Smithsonian Tropical Research Institute in Panama, where researchers have access to high-quality laboratory facilities. Here, we present a high-quality genome for the slender anole, which is an important new resource for studying this model species. We assembled and annotated the slender anole genome by combining 3 technologies: Oxford Nanopore, 10× Genomics Linked-Reads, and Dovetail Omni-C. We compared this genome with the recently published brown anole (Anolis sagrei) and the canonical green anole (Anolis carolinensis) genomes. Our genome is the first assembled for an Anolis lizard from mainland Central or South America, the regions that host the majority of diversity in the genus. This new reference genome is one of the most complete genomes of any anole assembled to date and should facilitate deeper studies of slender anole evolution, as well as broader scale comparative genomic studies of both mainland and island species. In turn, such studies will further our understanding of the well-known adaptive radiation of Anolis lizards.
When is surgery indicated in metastatic small intestine neuroendocrine tumor?
Authors: Draskacheva Nadica , Saljamovski Darko , Gošić Violeta , Trajkovski Gjorgji , Ristovski Gligor , Misimi Shqipe , Nikolovski Andrej 
Published: October 2023

Abstract
Small intestine neuroendocrine tumors are predominantly small but with high potential for distant metastases development. Diagnosis establishment in early-stage is often difficult and challenging. Small intestine neuroendocrine tumors often initially present with liver metastases. According to the Consensus Guidelines of the North American Neuroendocrine Tumor Society, in patients with liver metastases from unknown origin of primary neuroendocrine tumor, surgical exploration should be performed in order to identify the primary location, prevent small intestine obstruction, and treat one if already present. We present a case of a 69-year-old male patient diagnosed with liver and peritoneal metastases due to small bowel neuroendocrine tumor treated with surgery due to the presence of small intestine obstruction.
The formation channels of multiphase gas in nearby early-type galaxies
Authors: Eskenasy Ryan , Olivares Valeria , Su Yuanyuan , Li Yuan 
Published: October 2023

ABSTRACT
The processes responsible for the assembly of cold and warm gas in early-type galaxies (ETGs) are not well understood. We report on the multiwavelength properties of 15 non-central, nearby (z ≤ 0.008 89) ETGs primarily through Multi-Unit Spectroscopic Explorer (MUSE) and Chandra X-ray observations, to address the origin of their multiphase gas. The MUSE data reveal that 8/15 sources contain warm ionized gas traced by the H α emission line. The morphology of this gas is found to be filamentary in 3/8 sources: NGC 1266, NGC 4374, and NGC 4684, which is similar to that observed in many group and cluster-centred galaxies. All H α filamentary sources have X-ray luminosities exceeding the expected emission from the stellar population, suggesting the presence of diffuse hot gas, which likely cooled to form the cooler phases. The morphologies of the remaining 5/8 sources are rotating gas discs, not as commonly observed in higher mass systems. Chandra X-ray observations (when available) of the ETGs with rotating H α discs indicate that they are nearly void of hot gas. A mixture of stellar mass-loss and external accretion was likely the dominant channel for the cool gas in NGC 4526 and NGC 4710. These ETGs show full kinematic alignment between their stars and gas, and are fast rotators. The H α features within NGC 4191 (clumpy, potentially star-forming ring), NGC 4643, and NGC 5507 (extended structures) along with loosely overlapping stellar and gas populations allow us to attribute external accretion to be the primary formation channel of their cool gas.
How different is the magnetic field at the core–crust interface from that at the neutron star surface? The range allowed in magnetoelastic equilibrium
Authors: Kojima Yasufumi , Yoshida Shijun 
Published: October 2023

ABSTRACT
This study was focused on the investigation of a magnetic field penetrating from the core of a neutron star to its surface. The range of possible field configurations in the intermediate solid crust is less limited owing to the elastic force acting on the force balance. When the Lorentz force is excessively strong, the magnetoelastic equilibrium does not hold, and thus, the magnetic field becomes constrained. By numerically solving for the magnetoelastic equilibrium in a thin crust, the range of the magnetic field at the core–crust interface was determined, while assuming the exterior to be fixed as a dipole in vacuum. The results revealed that the toroidal component should be smaller than the poloidal component at the core–crust interface for the surface dipole, B0 &gt; 2.1 × 1014 G. Consequently, a strong toroidal field, for example, B ∼ 1016 G, as suggested by free precession of magnetars should be confined to a deep interior core and should be reduced to B ∼ 1014 G at the bottom of the crust. The findings of this study provide insights into the interior field structure of magnetars. Further investigations on more complicated geometries with higher multipoles and exterior magnetosphere are necessary.
Simulated non-thermal emission of the supernova remnant G1.9 + 0.3
Authors: Villagran M A , Gómez D O , Velázquez P F , Meyer D M-A , Chiotellis A , Raga A C , Esquivel A , Toledo-Roy J C , Vargas-Rojas K M , Schneiter E M 
Published: October 2023

ABSTRACT
Supernova remnants are the nebular leftover of defunct stellar environments, resulting from the interaction between a supernova blastwave and the circumstellar medium shaped by the progenitor throughout its life. They display a large variety of non-spherical morphologies such as ears that shine non-thermally. We have modelled the structure and the non-thermal emission of the supernova remnant G1.9 + 0.3 through 3D magnetohydrodynamic numerical simulations. We propose that the peculiar ear-shaped morphology of this supernova remnant results from the interaction of its blast wave with a magnetized circumstellar medium, which was previously asymmetrically shaped by the past stellar wind emanating from the progenitor star or its stellar companion. We created synthetic non-thermal radio and X-ray maps from our simulated remnant structure, which are in qualitative agreement with observations, forming ears on the polar directions. Our synthetic map study explains the discrepancies between the measured non-thermal radio and X-ray surface brightness distributions assuming that the inverse Compton process produces the observed X-ray emission.
Feedback-driven anisotropy in the circumgalactic medium for quenching galaxies in the
simba
simulations
Authors: Yang Tianyi , Davé Romeel , Cui Weiguang , Cai Yan-Chuan , Peacock John A , Sorini Daniele 
Published: October 2023

ABSTRACT
We use the simba galaxy formation simulation suite to explore anisotropies in the properties of circumgalactic gas that result from accretion and feedback processes. We particularly focus on the impact of bipolar active galactic nuclei (AGNs) jet feedback as implemented in simba , which quenches galaxies and has a dramatic effect on large-scale gas properties. We show that jet feedback at low redshifts is most common in the stellar mass range (1–5) × 1010 M⊙, so we focus on galaxies with active jets in this mass range. In comparison to runs without jet feedback, jets cause lower densities and higher temperatures along the galaxy minor axis (simba jet direction) at radii $\gtrsim 0.5r_{200c}-4r_{200c}$ and beyond. This effect is less apparent at higher or lower stellar masses, and is strongest within green valley galaxies. The metallicity also shows strong anisotropy out to large scales, driven by star formation feedback. We find substantially stronger anisotropy at $\lesssim 0.5r_{200c}$, but this also exists in runs with no explicit feedback, suggesting that it is due to anisotropic accretion. Finally, we explore anisotropy in the bulk radial motion of the gas, finding that both star formation and AGN wind feedback contribute to pushing the gas outwards along the minor axis at $\lesssim 1$ Mpc, but AGN jet feedback further causes bulk outflow along the minor axis out to several Mpc, which drives quenching via gas starvation. These results provide observational signatures for the operation of AGN feedback in galaxy quenching.
New black hole spin values for Sagittarius A* obtained with the outflow method
Authors: Daly Ruth A , Donahue Megan , O’Dea Christopher P , Sebastian Biny , Haggard Daryl , Lu Anan 
Published: October 2023

ABSTRACT
Six archival Chandra observations are matched with eight sets of radio data and studied in the context of the outflow method to measure and study the spin properties of $\rm {Sgr ~A^{*}}$. Three radio and X-ray data sets obtained simultaneously, or partially simultaneously, are identified as preferred for the purpose of measuring the spin properties of $\rm {Sgr ~A^{*}}$. Similar results are obtained with other data sets. Results obtained with the preferred data sets are combined and indicate weighted mean values of the spin function of $F = 0.62 \pm 0.10$ and dimensionless spin angular momentum of $a_* = 0.90 \pm 0.06$. The spin function translates into measurements of the black hole rotational mass, Mrot, irreducible mass, Mirr, and spin mass–energy available for extraction, Mspin, relative to the total black hole dynamical mass, Mdyn. Weighted mean values of (Mrot/Mdyn) = (0.53 ± 0.06), (Mirr/Mdyn) = (0.85 ± 0.04), (Mspin/Mdyn) = (0.15 ± 0.04), Mrot = (2.2 ± 0.3) × 106 M⊙, Mirr = (3.5 ± 0.2) × 106 M⊙, and Mspin = (6.2 ± 1.6) × 105 M⊙ are obtained; of course (Mrot/Mirr) = (0.62 ± 0.10) since (Mrot/Mirr) = F. Values obtained for $\rm {Sgr ~A^{*}}$ are compared with those obtained for M87 based on the published spin function, which indicate that M87 carries substantially more rotational energy and spin mass–energy relative to the total (i.e. dynamical) black hole mass, the irreducible black hole mass, and in absolute terms.
Assessment of a new sub-grid model for magnetohydrodynamical turbulence – II. Kelvin–Helmholtz instability
Authors: Miravet-Tenés Miquel , Cerdá-Durán Pablo , Obergaulinger Martin , Font José A 
Published: October 2023

ABSTRACTThe modelling of astrophysical systems such as binary neutron star mergers or the formation of magnetars from the collapse of massive stars involves the numerical evolution of magnetized fluids at extremely large Reynolds numbers. This is a major challenge for (unresolved) direct numerical simulations which may struggle to resolve highly dynamical features as, e.g. turbulence, magnetic field amplification, or the transport of angular momentum. Sub-grid models offer a means to overcome those difficulties. In a recent paper we presented MInIT, an MHD-instability-induced-turbulence mean-field, sub-grid model based on the modelling of the turbulent (Maxwell, Reynolds, and Faraday) stress tensors. While in our previous work MInIT was assessed within the framework of the magnetorotational instability, in this paper we further evaluate the model in the context of the Kelvin–Helmholtz instability (KHI). The main difference with other sub-grid models (as e.g. the alpha-viscosity model or the gradient model) is that in MInIT, we track independently the turbulent energy density at sub-grid scales, which is used, via a simple closure relation, to compute the different turbulent stresses relevant for the dynamics. The free coefficients of the model are calibrated using well-resolved box simulations of magnetic turbulence generated by the KHI. We test the model against these simulations and show that it yields order-of-magnitude accurate predictions for the evolution of the turbulent Reynolds and Maxwell stresses.