bluuebunny/crossref_metadata_2025_split huggingface dataset:
A 71-Year-Old Man Presenting with Anemia and a Solitary Skin Lesion Associated with Primary Cutaneous Marginal Zone Lymphoma
Authors: Khudyakova Mariya 
Published: April 2021

A 71-year-old man with a solitary red lesion on his left arm, which initially thought to be a hematoma, was admitted for inpatient evaluation of anemia, which after a positive direct Coombs test was qualified as autoimmune hemolytic anemia. The patient also presented with hoarseness and biopsies from the swelled nasopharynx and an enlarged right tonsil were obtained. Due to uncertain diagnosis and the patient’s previous history of malignancy, (low grade lymphoproliferative lymphoma) skin and bone marrow biopsies were performed. Unfortunately, the patient’s status rapidly deteriorated as a result of septic shock. The obtained skin, nasopharynx, and tonsil biopsies became available after the patient died and showed marginal zone lymphoma with no evidence of lymphoproliferative neoplasm in the bone marrow.
This case demonstrates the diagnostic complexity of nodal marginal zone lymphoma complicated by severe life-threatening autoimmune hemolytic anemia in an elderly patient with multimorbidity, which presents management challenges for health care providers.
Mesotelioma Pleural Maligno
Authors: Palma Maynor , De-León Juan , Arreola José 
Published: April 2021

El Mesotelioma Pleural Maligno (MPM) es un cáncer agresivo y raro de la superficie pleural asociado a exposición de asbesto. La incidencia y prevalencia a nivel mundial son desconocidas. Los datos clínicos son progresivos e incluyen disnea, tos y dolor torácico intenso, asociado o no a derrame pleural. Se diagnostica mediante histología, aunque en la actualidad existen marcadores séricos de ayuda. Las estrategias terapéuticas incluyen cirugía asociada a quimio y radioterapia, sin embargo la sobrevida es de aproximadamente 8-14 meses. Presentamos el caso de un hombre de 61 años diagnosticado con MPM.
Metodologias e estratégias pedagógicas para o ensino das lutas, artes marciais e esportes de combate: uma revisão integrativa
Authors: Terluk Maria Gorete , Ruppel da Rocha Ricelli Endrigo 
Published: April 2021

OBJETIVO: O objetivo foi sintetizar as evidências na literatura sobre as estratégias de ensino das lutas e dos esportes de combate. MÉTODOS: Foi realizada uma busca nas bases de dados da Biblioteca Virtual de Saúde (BVS) que inclui LILACS, MEDLINE, MEDCARIB, OPAS/OMS, PAHO e WHOLIS; SciELO, EBSCO e Periódicos da CAPES no período entre 2010 e 2020. Para a busca utilizou-se a combinação dos seguintes termos: “Artes Marciais” OR “Esportes de Combate”; “Martial Arts” OR “Combat Sports”. RESULTADOS: Os resultados mostraram que 89% dos estudos apontam para estratégias de ensino centradas no aluno, levando em conta os interesses e contextualizando as práticas, de forma lúdica e livre para criar novos movimentos. CONCLUSÃO: As lutas e os esportes de combate através de metodologias e estratégias de ensino centradas nos alunos beneficiam o desenvolvimento integral de seus praticantes.Pedagogical methodologies and strategies for teaching fights, martial arts and fighting sports: an integrative reviewABSTRACTOBJECTIVE: This integrative review aimed at synthetizing the evidence in the literature on strategies for teaching fighting and combat sports. METHODS: A search on the databases of the Virtual Health Library (VHL) was carried out, which included LILACS, MEDLINE, MEDCARIB, OPAS/WHO, PAHO and WHOLIS, ScIELO, EBSCO, in addition to the Journals of CAPES from 2010 to 2020. For the search we used the combination of the following terms: “Martial Arts” OR “Combat Sports”. RESULTS: The results showed that 89% of the studies point to student-centered teaching methods that consider interests and contextualized practices in a playful and free manner to create new movements. CONCLUSION: In conclusion, fights and combat sports through methodologies and teaching strategies centered on students benefit the integral development of their practitioners.
Analisis Kepuasan dalam Meningkatkan Loyalitas melalui Kepercayaan
Authors: Cahyati Peni 
Published: April 2021

Penelitian ini bertujuan untuk mengetahui dan menganalisis pengaruh kepuasan terhadap kepercayaan dan implikasinya terhadap loyalitas (studi pada pasien peserta BPJS di UPT Puskesmas Cimaragas Kabupaten Ciamis). Hasil penelitian ini diharapkan dapat menjadi bahan masukan bagi UPT Puskesmas Cimaragas Kabupaten Ciamis, yang berguna untuk meningkatkan kepuasan sehingga tercapai kepercayaan pasien dan loyalitas pasien. Metode penelitian yang digunakan adalah analisis deskriptif dan verifikatif. Pengumpulan data yang digunakan adalah wawancara dengan menggunakan kuesioner disertai dengan teknik observasi dan kepustakaan, teknik pengambilan p sampel dilakukan secara consecutive sampling dengan menggunakan kriteria inklusi dan eksklusi. Pengumpulan data di lapangan dilaksanakan pada tahun 2019. Teknik analisis data menggunakan Analisis Jalur. Hasil penelitian menunjukkan bahwa secara umum kepuasan, kepercayaan, loyalitas pasien di UPT Puskesmas Cimaragas Kabupaten Ciamis termasuk kategori kurang baik. Terdapat pengaruh kepuasan terhadap kepercayaan serta implikasinya pada loyalitas pasien. Semakin baik kepuasan yang diterima pasien, semakin baik pula kepercayaan pasien terhadap Puskesmas yang pada akhirnya akan berdampak terhadap peningkatan loyalitas pasien di UPT Puskesmas Cimaragas.
Perceptual restoration of locally time-reversed speech: Non-native listeners’ performance in their L2 vs. L1
Authors: Ishida Mako 
Published: April 2021

AbstractNonnative listeners are generally not as good as native listeners in perceptually restoring degraded speech and understand what was being said. The current study investigates how nonnative listeners of English (namely, native Japanese speakers who learned English as a second language) perceptually restore temporally distorted speech in their L2 English as compared with native English listeners (L1 English) reported in Ishida et al. (Cognition, 151,68–75, 2016), and as compared with the listeners’ native tongue (L1 Japanese). In the experiment, listeners listened to locally time-reversed words and pseudowords in their L2 English and L1 Japanese where every 10, 30, 50, 70, 90, or 110 ms of speech signal was flipped in time—these stimuli contained either many fricatives or stops. The results suggested that the intelligibility of locally time-reversed words and pseudowords deteriorated as the length of reversed segments increased in both listeners’ L2 English and L1 Japanese, while listeners understood locally time-reversed speech more in their L1 Japanese. In addition, lexical context supported perceptual restoration in both listeners’ L1 Japanese and L2 English, while phonemic constituents affected perceptual restoration significantly only in listeners’ L1. On the other hand, locally time-reversed words and pseudowords in L1 Japanese were much more intelligible than those in L1 English reported in Ishida et al. It is possible that the intelligibility of temporally distorted lexical items depends on the structure of basic linguistic units in each language, and the Japanese language might have a unique characteristic because of its CV and V structure.
Alfabetización Digital como Puente de Exclusión Social Poscovid-19
Authors: Sandoval-Bravo Carlos Henry 
Published: April 2021

Se inicia una nueva ventana del siglo XXI y con ella una época de profundos retos sociales y es cómo seguir integrando las Tecnologías de la Información y la Comunicación (TIC) y las múltiples innovaciones tecnológicas a las actividades cotidianas. El mundo tiene hoy un gran desafío a causa del impacto del COVID-19, surgen nuevas oportunidades en el campo de las competencias tecnológicas, dando origen a nuevas desigualdades y brechas sociales lo que motiva a crear nuevas estrategias útiles para poderlas abordar. El presente estudio tuvo como objetivo el fortaleciendo de las habilidades y destrezas tecnológicas-digitales en los entornos infocomunicativos para el desarrollo de trabajo colaborativo. En el desarrollo de la investigación se utilizó el enfoque mixto y en el proceso de la recolección de información se utilizó el cuestionario y encuesta. La población objeto de estudio fue conformada por 130 Agentes Educativas Comunitarias, entre 25 y 68 años, pertenecientes a la Cooperativa de Multiactiva de Agentes Educativas de Girón COOMUDAEG, ubicada en Girón Santander, Colombia. Los hallazgos concluyen que en tiempo de posCOVID-19 las Agentes Educativas tienen oportunidad de seguir fortaleciendo sus habilidades y destrezas tecnológicas en los entornos infocomunicativos, para afianzar el trabajo colaborativo, la resolución de problemas en su vida cotidiana y profesional disminuyendo así el riesgo de exclusión social.
The Hubble Constant from Infrared Surface Brightness Fluctuation Distances*
Authors: Blakeslee John P. , Jensen Joseph B. , Ma Chung-Pei , Milne Peter A. , Greene Jenny E. 
Published: April 2021

Abstract
We present a measurement of the Hubble constant H
0 from surface brightness fluctuation (SBF) distances for 63 bright, mainly early-type galaxies out to 100 Mpc observed with the WFC3/IR on the Hubble Space Telescope (HST). The sample is drawn from several independent HST imaging programs using the F110W bandpass, with the majority of the galaxies being selected from the MASSIVE survey. The distances reach the Hubble flow with a median statistical uncertainty per measurement of 4%. We construct the Hubble diagram with these IR SBF distances and constrain H
0 using four different treatments of the galaxy velocities. For the SBF zero-point calibration, we use both the existing tie to Cepheid variables, updated for consistency with the latest determination of the distance to the Large Magellanic Cloud from detached eclipsing binaries, and a new tie to the tip of the red giant branch (TRGB) calibrated from the maser distance to NGC 4258. These two SBF calibrations are consistent with each other and with theoretical predictions from stellar population models. From a weighted average of the Cepheid and TRGB calibrations, we derive H
0 = 73.3 ± 0.7 ± 2.4 km s−1 Mpc−1, where the error bars reflect the statistical and systematic uncertainties. This result accords well with recent measurements of H
0 from Type Ia supernovae, time delays in multiply lensed quasars, and water masers. The systematic uncertainty could be reduced to below 2% by calibrating the SBF method with precision TRGB distances for a statistical sample of massive early-type galaxies out to the Virgo cluster measured with the James Webb Space Telescope.
Gaia EDR3 Parallax Zero-point Offset Based on W Ursae Majoris-type Eclipsing Binaries
Authors: Ren Fangzhou , Chen Xiaodian , Zhang Huawei , de Grijs Richard , Deng Licai , Huang Yang 
Published: April 2021

Abstract
We independently determine the zero-point offset of the Gaia early Data Release-3 (EDR3) parallaxes based on ∼110,000 W Ursae Majoris (EW)-type eclipsing binary systems. EWs cover almost the entire sky and are characterized by a relatively complete coverage in magnitude and color. They are an excellent proxy for Galactic main-sequence stars. We derive a W1-band period–luminosity relation with a distance accuracy of 7.4%, which we use to anchor the Gaia parallax zero-point. The final, global parallax offsets are −28.6 ± 0.6 μas and −25.4 ± 4.0 μas (before correction) and 4.2 ± 0.5 μas and 4.6 ± 3.7 μas (after correction) for the five- and six-parameter solutions, respectively. The total systematic uncertainty is 1.8 μas. The spatial distribution of the parallax offsets shows that the bias in the corrected Gaia EDR3 parallaxes is less than 10 μas across 40% of the sky. Only 15% of the sky is characterized by a parallax offset greater than 30 μas. Thus, we have provided independent evidence that the parallax zero-point correction provided by the Gaia team significantly reduces the prevailing bias. Combined with literature data, we find that the overall Gaia EDR3 parallax offsets for Galactic stars are [−20, −30] μas and 4–10 μas, respectively, before and after correction. For specific regions, an additional deviation of about 10 μas is found.
Evidence for Multiple Accretion Events in the Gaia-Sausage/Enceladus Structures
Authors: Kwang Kim Young , Sun Lee Young , Beers Timothy C. , Koo Jae-Rim 
Published: April 2021

Abstract
We present evidence that multiple accretion events are required to explain the origin of the Gaia-Sausage and Enceladus (GSE) structures, based on an analysis of dynamical properties of main-sequence stars from the Sloan Digital Sky Survey Data Release 12 and Gaia Data Release 2. GSE members are selected to have eccentricity (e) > 0.7 and [Fe/H] < −1.0, and separated into low and high orbital-inclination (LOI/HOI) groups. We find that the LOI stars mainly have e < 0.9 and are clearly separable into two groups with prograde and retrograde motions. The LOI stars exhibit prograde motions in the inner-halo region and strong retrograde motions in the outer-halo region (OHR). We interpret the LOI stars in these regions to be stars accreted from two massive dwarf galaxies with low-inclination prograde and retrograde orbits, affected to different extents by dynamical friction due to their different orbital directions. In contrast, the majority of the HOI stars have e > 0.9, and exhibit a globally symmetric distribution of rotational velocities (V

ϕ
) near zero, although there is evidence for a small retrograde motion for these stars (V

ϕ
∼ −15 km s−1) in the OHR. We consider these stars to be stripped from a massive dwarf galaxy on a high-inclination orbit. We also find that the LOI and HOI stars on highly eccentric and tangential orbits with clear retrograde motions exhibit different metallicity peaks at [Fe/H] = −1.7 and −1.9, respectively, and argue that they are associated with two low-mass dwarf galaxies accreted in the OHR of the Galaxy.
Linemake: An Atomic and Molecular Line List Generator
Authors: Placco Vinicius M. , Sneden Christopher , Roederer Ian U. , Lawler James E. , Den Hartog Elizabeth A. , Hejazi Neda , Maas Zachary , Bernath Peter 
Published: April 2021

Abstract
In this research note, we present linemake, an open-source atomic and molecular line list generator. Rather than a replacement for a number of well-established atomic and molecular spectral databases, linemake aims to be a lightweight, easy-to-use tool to generate formatted and curated lists suitable for spectral synthesis work. We encourage users of linemake to understand the sources of their transition data and cite them as appropriate in published work. We provide the code, line database, and an extensive list of literature references in a GitHub repository (https://github.com/vmplacco/linemake), which will be updated regularly as new data become available.
Fourteen E+A Galaxy Candidates Involved in Interactions
Authors: Greenfield Spencer , Joyce Maya L. , Liu Charles T. 
Published: April 2021

Abstract
Galaxy mergers are a mechanism for rapid quenching of star formation. We are studying E+A galaxies (a type of post-starburst galaxy) and how they are impacted by merging. Examining E+A galaxies with companions offers insight into the evolution of E+As and the quenching process. The Y/Dim Collaboration collected a sample of E+A candidate galaxies from the SDSS DR16. Among the E+A candidates that were visually identified as interacting, 14 were spectroscopically confirmed to have companions. Our sample contained 11 pairs of galaxies and two groups of three galaxies. In one of these groups of three, there are two E+A candidates. Nine of these E+A candidates are involved in minor interactions with their companions.
Optical Constants of a Solar System Organic Analog and the Allende Meteorite in the Near- and Mid-infrared (1.5–13 μm)
Authors: Arnold Jessica A. , Weinberger Alycia J. , Cody George , Videen Gorden , Muñoz Olga 
Published: April 2021

Abstract
Measurements of visible and near-infrared reflection (0.38–5 μm) and mid-to-far-infrared emission (5–200 μm) from telescope and satellite remote-sensing instruments make it possible to investigate the composition of planetary surfaces via electronic transitions and vibrational modes of chemical bonds. Red spectral slopes at visible and near-infrared wavelengths and absorption features at 3.3 and 3.4 μm observed in circumstellar disks, in the interstellar medium (ISM), and on the surfaces of solar system bodies are interpreted to be due to the presence of organic material and other carbon compounds. Identifying the origin of these features requires measurements of the optical properties of a variety of relevant analog and planetary materials. Spectroscopic models of dust within circumstellar disks and the ISM, as well as planetary regoliths, often incorporate just one such laboratory measurement despite the wide variation in absorption and extinction properties of organic and other carbon-bearing materials. Here we present laboratory measurements of transmission spectra in the 1.5–13 μm region and use these to derive real and imaginary indices of refraction for two samples: (1) an analog to meteoritic insoluble organic matter and (2) a powdered Allende meteorite sample. We also test our refractive index retrieval method on a previously published transmission spectrum of an Mg-rich olivine. We compare optical measurements of the insoluble organic matter analog to those of other solar system and extrasolar organic analogs, such as amorphous carbon and tholins, and find that the indices of refraction of the newly characterized material differ significantly from other carbonaceous samples.
Modeling Saturn’s D68 Clumps as a Co-orbital Satellite System
Authors: A’Hearn Joseph A. , Hedman Matthew M. , Hamilton Douglas P. 
Published: April 2021

Abstract
The D68 ringlet is the innermost feature in Saturn’s rings. Four clumps that appeared in D68 around 2014 remained evenly spaced about 30° apart and moved very slowly relative to each other from 2014 up until the last measurements were taken in 2017. D68's narrowness and the distribution of clumps could either indicate that we have a collection of source bodies in a co-orbital configuration or imply that an outside force confines the observed dust and any source bodies. In this paper we explore the possibility that these four clumps arose from four source bodies in a co-orbital configuration. We find that there are no solutions with four masses that produce the observed spacings. We therefore consider whether an unseen fifth co-orbital object could account for the discrepancies in the angular separations and approach a stable stationary configuration. We find a range of solutions for five co-orbital objects where their mass ratios depend on the assumed location of the fifth mass. Numerical simulations of five co-orbitals are highly sensitive to initial conditions, especially for the range of masses we would expect the D68 clumps to have. The fragility of our D68 co-orbital system model implies that there is probably some outside force confining the material in this ringlet.
Décrire la bibliothèque d’André Schwarz-Bart : enjeux et méthodes
Authors: Villeminoz Jérôme 
Published: April 2021

Le fonds Simone et André Schwarz-Bart a été créé en 2017 au département des Manuscrits de la Bibliothèque nationale de France. Il est depuis régulièrement enrichi. À l’été 2018, ce sont environ 1 500 livres annotés de la bibliothèque d’André Schwarz-Bart, ainsi qu’un mètre linéaire de coupures de presse, elles aussi annotées, qui sont arrivés de Guadeloupe. Et avec eux, dans un département pourtant rompu à la gestion de fonds d’archives d’auteurs, un ensemble de questions inhabituelles, aussi stimulantes que le contenu des documents qu’elles concernent.Cet article présente le travail accompli à la BnF sur cette bibliothèque, en le déclinant, sans surprise, selon les grandes missions de l’établissement : collecter, conserver, signaler, communiquer. Il s’agit d’un travail en cours. La phase de description des livres, en particulier, est loin d’être achevée : quelques 350 livres ont été à ce jour examinés et décrits. On se garde donc de donner des informations précises et définitives, comme des dates extrêmes ou même le nombre exact de livres, et l’on doit se contenter souvent d’hypothèses. Pour autant, exposer ce travail est aussi l’occasion de donner une idée juste de la richesse des contenus de cette bibliothèque, et d’esquisser quelques axes de recherche ou pistes d’étude.
Qualité et différenciation des biens informationnels. Une étude exploratoire sur l’information d’actualité
Authors: Lyubareva Inna , Rochelandet Fabrice , Haralambous Yannis 
Published: April 2021

Le numérique, que ce soit à travers les innovations de service ou l’usage massif des médias sociaux, influence la qualité des biens informationnels. C’est le cas notamment des biens culturels et de l’information journalistique. Or, la notion et la mesure de la qualité s’avèrent non consensuelles et renvoient à des conceptions et des attentes sociales très différentes. Dans cet article, nous proposons d’analyser la qualité de l’information journalistique à partir d’un modèle de différenciation verticale et horizontale. Nous nous basons sur les méthodes d’analyse de discours en linguistique pour caractériser les choix éditoriaux des producteurs d’informations. En comparant 93K articles de presse portant sur 31 évènements entre 2015 et 2019 et publiés par 55 médias de presse représentatifs en France, nous proposons une cartographie des médias français selon leurs choix de différenciation et évaluons, sur cette base, la qualité de l’information journalistique offerte aux consommateurs.Classification JEL : L1 Market Structure, Firm Strategy, and Market Performance, O33 Technological Change: Choices and Consequences; Diffusion Processes.
IL-27/IL-27R Mediates Protective Immunity against Chlamydial Infection by Suppressing Excessive Th17 Responses and Reducing Neutrophil Inflammation
Authors: Zha Xiaoyu , Yang Shuaini , Niu Wenhao , Tan Lu , Xu Yueyue , Zeng Jiajia , Tang Yingying , Sun Lida , Pang Gaoju , Qiao Sai , Zhang Hong , Liu Tengli , Zhao Huili , Zheng Ningbo , Zhang Yongci , Bai Hong 
Published: April 2021

Abstract
IL-27, a heterodimeric cytokine of the IL-12 family, has diverse influences on the development of multiple inflammatory diseases. In this study, we identified the protective role of IL-27/IL-27R in host defense against Chlamydia muridarum respiratory infection and further investigated the immunological mechanism. Our results showed that IL-27 was involved in C. muridarum infection and that IL-27R knockout mice (WSX-1–/– mice) suffered more severe disease, with greater body weight loss, higher chlamydial loads, and more severe inflammatory reactions in the lungs than C57BL/6 wild-type mice. There were excessive IL-17–producing CD4+ T cells and many more neutrophils, neutrophil-related proteins, cytokines, and chemokines in the lungs of WSX-1–/– mice than in wild-type mice following C. muridarum infection. In addition, IL-17/IL-17A–blocking Ab treatment improved disease after C. muridarum infection in WSX-1–/– mice. Overall, we conclude that IL-27/IL-27R mediates protective immunity during chlamydial respiratory infection in mice by suppressing excessive Th17 responses and reducing neutrophil inflammation.