bluuebunny/crossref_metadata_2025_split huggingface dataset:
PNEUMONIA ADQUIRIDA NA COMUNIDADE: utilização do CURB-65 para avaliação de gravidade e direcionamento ao tratamento clínico
Authors: SOUSA COELHO LARA BEATRIZ DE , Francisco Héricles Moreira de Carvalho  , Aleksandra Szezepanowski Lopes  , Vinicius Mendes Farias  , Rodrigo dos Santos Carneiro de Andrade  , João Lucas Santana Spindola  , Cláudio Nunes Soares Neto  , George Moreira de Vasconcelos Filho  , Marina Batista Cipriano  , Luiza Eduarda Lebre Góes  , Linda Rachel Akashi Oliveira  , Álvaro Henrique Silva Varão  
Published: July 2024

Introdução: A Pneumonia Adquirida na Comunidade (PAC) constitui uma das principais causas de mortalidade e hospitalizações a nível mundial. A PAC consiste em uma infecção aguda de caráter respiratório que atinge diretamente os pulmões, podendo ser de origem bacteriana ou viral e acomete os alvéolos. Os princiais agentes são os vírus, apesar de que o patógeno Streptococcus pneumoniae, até os dias atuais, representa um significativo número de casos. A doença representa uma importante causa de internação hospitalar. Portanto, cabe a necessidade de investigação de recursos que fundamentem a tomada de decisão, como o uso da ferramenta CURB-65, criado em 2003 pela British Thoracic Society. Objetivo: Evidenciar utilização do CURB-65 para avaliação de gravidade e direcionamento ao tratamento clínico da Pneumonia Adquirida na Comunidade. Método: Trata-se de uma revisão integrativa de literatura, um instrumento da prática baseada em evidências. Inicialmente, foi formulada a seguinte questão de pesquisa: “Quais as evidências da utilização do CURB-65 para avaliação de gravidade e direcionamento ao tratamento clínico da Pneumonia Adquirida na Comunidade?”. A análise de dados foi proveniente da Biblioteca Virtual em Saúde nas bases de dados da Literatura Latino-Americana e do Caribe em Ciências da Saúde (LILACS) e Medical Literature Analysis and Retrievel System Online (MEDLINE). A partir da busca inicial, ocorrida de junho a julho de 2024, oito (8) foram condizentes com a questão de pesquisa. Resultados e Discussão: O CURB-65 torna possível a avaliação precoce da gravidade clínica, uma vez que atribuiu-se valores ao quadro de saúde apresentado pelo paciente. Verifica-se que os modelos preditivos, como o CURB-65, são ferramentas fundamentais à Saúde Pública, uma vez que auxiliam na tomada de decisão. Em vista do exposto, as decisões são fundamentais à segurança do paciente e ao uso racional de recursos. Isso porque a admissão no período tardio na Unidade de Terapia Intensiva apontam para a elevação nas taxas de mortalidade. Conclusão: Compreendeu-se, ao final da pesquisa, que o escore constitui uma ferramenta essencial à prática clínica e o manejo adequado constitui uma atribuição indispensável ao profissional de saúde. Desse modo, objetiva-se, primordialmente, a ocorrência de desfechos assertivos ao tempo em que há a redução da mortalidade.
Pengaruh Pengemasan Terhadap Lama Simpan Produk Hortikultura
Authors: Ariefin Muhammad Noor , Mita Karmelita Gresiana , Haim Kristina , Anatolana Kalista Setia , Dir Imaculata Safitri , Walong Lugerio Ferino Putra 
Published: July 2024

Pasca panen merupakan sebagai berbagai tindakan atau perlakuan yang diberikan pada hasil pertanian setelah panen sampai komoditas berada di tangan konsumen. Penanganan pasca panen (postharvest) sering disebut juga sebagai pengolahan primer (primary processing) merupakan istilah yang digunakan untuk semua perlakuan dari mulai panen sampai komoditas dapat dikonsumsi “segar” atau untuk persiapan pengolahan berikutnya. Tujuan penelitian ini mengenai lama simpan produk hortikulturan terhadap berbagai perlakuan pengemasan. Penelitian ini telah dilaksanakan pada bulan Juli di Laboratorium pasca panen Universitas Katolik Indonesia, dengan metode penelitian deskriptif. Bahan yang digunakan dalam penelitian ini antara lain: Tomat, cabe merah besar, wortel, kangkung dan pisang kepok. Alat yang digunakan antara lain: Plastik, Aluminium foil, timbangan analitik, koran, guntung, penggaris dan camera. Parameter penelitian ini meliputi berat akhir, kekerasan, aroma dan warna. Berdasarkan hasil dari penelitian yang telah dilakukan dapat disimpulkan bahwa pengemasan berpengaruh terhadap mutu produk hortikultura. Beberapa perlakuan yang diuji ditemukan bahwa pengemasan dengan aluminium foil dan pengemasan plastik berpengaruh terhadap susut bobot, tekstur, warna dan aroma. Perlakuan kemasan kertas koran tidak berpengaruh dengan perlakuan palstik dan aluminium foil. Dari beberapa perlakuan tersebut tidak memberi pengaruh pada buah tomat untuk parameter warna, kekerasan dan aroma. Hal serupa terjadi pada buah cabai merah besar yang tidak mengalami pengaruh terhadap warna, kekerasan dan aroma.
Untangling the threads of motivated memory: Independent influences of reward and emotion
Authors: Bowen Holly J. , Madan Christopher R. 
Published: July 2024

Abstract
Motivational and emotional influences on memory have been studied extensively; however, despite the link between these constructs, they have been studied in separate lines of research, with very little work examining their effects concurrently. The current study takes a novel approach to manipulate motivational and emotional influences orthogonally, and within the same task, to test their interplay on intentional memory formation. If emotion and reward motivation are tightly linked, they may rely on overlapping cognitive mechanisms, thus we would not expect emotion and reward to interact in memory. Alternatively, they could be distinct constructs and therefore would boost memory when both are included in the same experimental trial, above and beyond additive effects. To test these competing predictions, in Experiment 1, participants (n = 180) completed an old/new recognition memory task with emotional (negative, positive) and neutral words intentionally encoded with high or low reward anticipation cues. In Experiment 2, participants (n = 159) encoded emotional and neutral words with a high or low reward cue, but memory was tested with free recall using study–test blocks. The findings from both experiments converged. There were main effects of emotion and reward in generally hypothesized directions, but no evidence of an interaction between these factors. This is in line with the prediction that emotion and reward motivation are similar constructs. Their combination within a trial does not boost memory above and beyond either of these factors alone perhaps indicating these constructs have similar cognitive mechanisms.
oMEGACat. II. Photometry and Proper Motions for 1.4 Million Stars in Omega Centauri and Its Rotation in the Plane of the Sky
Authors: Häberle Maximilian , Neumayer N. , Bellini A. , Libralato M. , Clontz C. , Seth A. C. , Nitschai M. S. , Kamann S. , Alfaro-Cuello M. , Anderson J. , Dreizler S. , Feldmeier-Krause A. , Kacharov N. , Latour M. , Milone A. P. , Pechetti R. , van de Ven G. , Voggel K. 
Published: July 2024

Abstract
Omega Centauri (ω Cen) is the most massive globular cluster of the Milky Way. It is thought to be the nucleus of an accreted dwarf galaxy because of its high mass and its complex stellar populations. To decipher its formation history and study its dynamics, we created the most comprehensive kinematic catalog for its inner region, by analyzing both archival and new Hubble Space Telescope (HST) data. Our catalog contains 1,395,781 proper-motion measurements out to the half-light radius of the cluster (

∼
5.0
′

) and down to m
F625W ≈ 25 mag. The typical baseline for our proper-motion measurements is 20 yr, leading to a median 1D proper motion precision of ∼11 μas yr−1 for stars with m
F625W ≈ 18 mag, with even better precision (∼6.6 μas yr−1) achieved in the extensively observed centermost (

r
<
1.5
′

) region. In addition to our astrometric measurements, we also obtained precise HST photometry in seven filters spanning from the ultraviolet to the near-infrared. This allows detailed color–magnitude diagram studies and separation of the multiple stellar populations of the cluster. In this work, we describe the data reduction used to obtain both the photometric and the proper-motion measurements. We also illustrate the creation and the content of our catalog, which is made publicly available. Finally, we present measurements of the plane-of-sky rotation of ω Cen in the previously unprobed inner few arcminutes and a precise measurement of the inclination, i = 43.°9 ± 1.°3.
symfind
: Addressing the Fragility of Subhalo Finders and Revealing the Durability of Subhalos
Authors: Mansfield Philip , Darragh-Ford Elise , Wang Yunchong , Nadler Ethan O. , Diemer Benedikt , Wechsler Risa H. 
Published: July 2024

Abstract
A major question in ΛCDM is what this theory actually predicts for the properties of subhalo populations. Subhalos are difficult to accurately simulate and to find within simulations, and this propagates into uncertainty in theoretical predictions for satellite galaxies. We present Symfind, a new particle-tracking-based subhalo finder, and demonstrate that it can track subhalos to orders-of-magnitude lower masses than commonly used halo-finding tools, with a focus on Rockstar and consistent-trees. These longer survival times mean that at a fixed peak subhalo mass, we find ≈ 15%–40% more subhalos within the virial radius, R
vir, and ≈35%–120% more subhalos within R
vir/4 in the Symphony dark-matter-only simulation suite. More subhalos are found as the resolution is increased, in contrast to the Rockstar halo finder, which appears to be converged at smaller subhalo counts. We perform extensive numerical testing. In agreement with idealized simulations, we show that the

v
max

, the maximum circular velocity, is systematically biased low until high resolutions (n
peak ≳ 3 × 104) are achieved, but that mass loss itself can be resolved at much more modest resolutions (n
peak ≳ 4 × 103). We show that Rockstar converges to false solutions for the mass function, radial distribution, and disruption masses of subhalos. We argue that our new method can trace resolved subhalos until the point of typical galaxy disruption without invoking post hoc orphan modeling. We outline a concrete set of steps for determining whether other subhalo finders meet the same criteria. We publicly release Symfind catalogs and particle data for the Symphony simulation suite at http://web.stanford.edu/group/gfc/symphony.
UVCANDELS: The Role of Dust on the Stellar Mass–Size Relation of Disk Galaxies at 0.5 ≤ z ≤ 3.0
Authors: Nedkova Kalina V. , Rafelski Marc , Teplitz Harry I. , Mehta Vihang , DeGroot Laura , Ravindranath Swara , Alavi Anahita , Beckett Alexander , Grogin Norman A. , Häußler Boris , Koekemoer Anton M. , Oyarzún Grecco A. , Prichard Laura , Revalski Mitchell , Snyder Gregory F. , Sunnquist Ben , Wang Xin , Windhorst Rogier A. , Chartab Nima , Conselice Christopher J. , Guo Yicheng , Hathi Nimish , Hayes Matthew J. , Ji Zhiyuan , Kim Keunho J. , Lucas Ray A. , Mobasher Bahram , O’Connell Robert W. , Sattari Zahra , Smith Brent M. , Taamoli Sina , Yung L. Y. Aaron ,   the UVCANDELS Team
Published: July 2024

Abstract
We use the Ultraviolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey fields (UVCANDELS) to measure half-light radii in the rest-frame far-UV for ∼16,000 disk-like galaxies over 0.5 ≤ z ≤ 3. We compare these results to rest-frame optical sizes that we measure in a self-consistent way and find that the stellar mass–size relation of disk galaxies is steeper in the rest-frame UV than in the optical across our entire redshift range. We show that this is mainly driven by massive galaxies (≳1010
M
⊙), which we find to also be among the most dusty. Our results are consistent with the literature and have commonly been interpreted as evidence of inside-out growth wherein galaxies form their central structures first. However, they could also suggest that the centers of massive galaxies are more heavily attenuated than their outskirts. We distinguish between these scenarios by modeling and selecting galaxies at z = 2 from the VELA simulation suite in a way that is consistent with UVCANDELS. We show that the effects of dust alone can account for the size differences we measure at z = 2. This indicates that, at different wavelengths, size differences and the different slopes of the stellar mass–size relation do not constitute evidence for inside-out growth.
On the Response of the Transition Region and the Corona to Rapid Excursions in the Chromosphere
Authors: Chaurasiya Ravi , Bayanna A. Raja , Louis R. E. , Pereira T. M. D. , Mathew S. K. 
Published: July 2024

Abstract
Spicules are the thin hair/grass-like structures that are prominently observed at the chromospheric solar limb. It is believed that fibrils and rapid blueshifted and redshifted excursions (RBEs and RREs; collectively referred to as REs) correspond to on-disk counterparts of type I spicules and type II spicules, respectively. Our investigation focuses on observing the response of these REs alongside similar spectral features in the chromosphere, transition region (TR), and corona, utilizing space–time plots derived from coordinated observations from the Swedish 1 m Solar Telescope/Hα, Interface Region Imaging Spectrograph (IRIS), and Solar Dynamics Observatory. Our analysis reveals upflowing REs, promptly reaching temperatures characteristic of the TR and corona, indicating a multithermal nature. Similarly, downflowing features exhibiting similar spectral signatures over the disk display plasma motion from the corona to chromospheric temperatures, demonstrating a multithermal nature. In addition to distinct upflows and downflows, we observe sequential upflow and downflow along the same path, depicting a distinctive parabolic trajectory in space–time plots of observations sampling TR and various coronal passbands. Similar to isolated upflows and downflows, these REs also exhibit a multithermal nature throughout their trajectory. Furthermore, our results reveal a more intricate motion of the REs in which both upflow and downflow coexist at the same spatial location. On a different note, our analysis, utilizing coordinated IRIS spectral observations, shows spatiotemporal redshifts/downflows in both the TR and chromosphere, suggesting that at least subsets of the strong redshifts/downflows observed in TR temperature spectra result from the return from the upper atmosphere flow of plasma in the form of bundles of spicules or features exhibiting similar spectra.
WIYN Open Cluster Study. XC. Barium Surface Abundances of Blue Straggler Stars in the Open Clusters NGC 7789 and M67
Authors: Nine Andrew C. , Mathieu Robert D. , Schuler Simon C. , Milliman Katelyn E. 
Published: July 2024

Abstract
We investigate barium (Ba) abundances in blue straggler stars (BSSs) in two open clusters, NGC 7789 (1.6 Gyr) and M67 (4 Gyr), as signatures of asymptotic-giant-branch (AGB) mass transfer. We combine our findings with previous Ba abundance analyses of NGC 6819 (2.5 Gyr) and NGC 188 (7 Gyr). Out of 35 BSSs studied in NGC 7789, NGC 6819, and M67, 15 (43% ± 11%) are Ba enriched; no BSSs in NGC 188 are Ba enriched. The Ba abundances of enriched BSSs show an anticorrelation with cluster age, ranging from an enrichment of [Ba/Fe] ∼ +1.5 dex in NGC 7789 to [Ba/Fe] ∼ +1.0 dex in M67. The Ba-enriched BSSs all lie in the same region of the H-R diagram, irrespective of cluster age or distance from the main-sequence turnoff. Our data suggest a link between AGB donor mass and mass-transfer efficiency in BSSs, in that less massive AGB donors tend to undergo more conservative mass transfer. We find that 40% ± 16% of the Ba-enriched BSSs are in longer-period spectroscopic binaries with orbital periods less than 5000 days. Those Ba-enriched BSSs that do not exhibit radial-velocity variability suggest AGB mass transfer in wide binaries by either wind mass transfer or wind Roche-lobe overflow. Given the preponderance of long orbital periods in the BSSs of M67 and NGC 188 and the frequency of Ba enrichment in NGC 7789, NGC 6819, and M67, it may be that AGB mass transfer is the dominant mechanism of BSS formation in open clusters older than 1 Gyr.
Time-dependent Hinode/EIS Atlas of a Coronal Mass Ejection Containing Cool Material
Authors: Wraback E. M. , Landi E. , Manchester W. B. 
Published: July 2024

Abstract
We report the first time-dependent spectral atlas of a coronal mass ejection (CME) observed by the Hinode/Extreme Ultraviolet Imaging Spectrometer (EIS). EIS observed the Cartwheel CME on 2008 April 9 at 09:30–10:00 UT in its full wavelength range and captured the bright core containing prominence material as it passed across the slit field of view. The measurement of the differential emission measure (DEM) showed that the observation captured two plasma components, a coronal component at Log T ≈ 6.05 K and a cold component at Log T ≈ 5.30 K, which we interpret as the prominence material in the CME core. We used this DEM to develop a spectral atlas for the four EIS spectra containing the CME material and the pre- and postevent spectra. These observations provide the basis for studying CME plasma evolution in the low solar corona, as well as guide observations from the current and upcoming spectrometers, including Solar Orbiter/SPICE, Solar-C/EUVST, and MUSE, which will advance our understanding of CME plasma evolution.
On the Interpretation of Mid-infrared Absorption Lines of Gas-phase H2O as Observed by JWST/MIRI
Authors: Li 李 Jialu 佳璐 , Boogert Adwin , Tielens Alexander G. G. M. 
Published: July 2024

Abstract
Rovibrational absorption lines of H2O in the 5–8 μm wavelength range selectively probe gas against the mid-infrared continuum-emitting background of the inner regions of young stellar objects and active galactic nuclei and deliver important information about these warm, dust-obscured environments. JWST/Mid-Infrared Instrument (MIRI) detects these lines in many lines of sight at a moderate spectral resolving power of R ∼ 3500 (full width at half-maximum of 85 km s−1). Based on our analysis of high-resolution SOFIA/EXES observations, we find that the interpretation of JWST/MIRI absorption spectra can be severely hampered by the blending of individual transitions and the lost information on the intrinsic line width or the partial coverage of the background continuum source. In this paper, we point out problems such as degeneracy that arise in deriving physical properties from an insufficiently resolved spectrum. This can lead to differences in the column density by 2 orders of magnitude. We emphasize the importance of weighting optically thin and weak lines in spectral analyses and provide recipes for breaking down the coupled parameters. We also provide an online tool to generate the H2O absorption line spectra that can be compared to observations.
Considérations épistémologiques sur la vérité judiciaire
Authors: Vorms Marion 
Published: July 2024

Dans cet article, j’examine deux ensembles d’arguments venant à l’appui de l’idée largement partagée selon laquelle la vérité judiciaire relèverait d’un régime à part. Selon un premier ensemble d’arguments, que je qualifie de « modestes », les contraintes qui s’imposent au juge le conduisent à devoir se contenter d’une vérité imparfaite – de « second rang » si on la compare à la vérité dite « scientifique ». Je montre que ces arguments reposent sur une vision erronée et naïve de cette dernière et que rien ne distingue, de ce point de vue, les conclusions factuelles sur lesquelles les juges doivent appuyer leurs décisions de celles que tout décideur en situation d’incertitude doit admettre. Selon un second ensemble d’arguments, que j’appelle « présomptueux », l’impératif d’autorité des décisions de justice oblige à considérer que ce qui sort de la bouche du juge est la vérité ; pour en préserver le caractère incontestable, on affirme, à nouveau, qu’elle ne correspond pas à la vérité « tout court » – ou encore à la vérité « absolue ». Je montre que, si l’on entend par « vérité judiciaire » ce qu’expriment les conclusions du juge qui comportent des qualifications juridiques, alors il est clair que cette vérité judiciaire n’est pas du même ordre que la vérité factuelle, mais je suggère que l’on peut se passer, dans ce cas, de la notion de vérité au profit de celle de décision ; en outre, pour que ces décisions soient justes, il convient de s’assurer que leur fondement factuel soit le plus exact possible – comme pour tout autre décision que l’on doit prendre en situation d’incertitude.
Le droit comparé, refuge de l’empirie juridique
Authors: Bordere Camille 
Published: July 2024

Alors que la pensée juridique française se (re)cherche face aux transformations de l’univers juridique dans lequel elle baigne, la voie de l’empirie apparaît comme l’une des options possibles pour se saisir de la complexité moderne du droit. Si les manifestations scientifiques, les publications collectives et les programmes de recherche se multiplient et s’aventurent toujours plus loin dans l’exercice empirique, l’on ne peut s’empêcher de remarquer le vide laissé par l’éternel grand absent : le comparatiste. Historiquement versé dans les différentes démarches empiriques, le comparatiste aurait, à ce stade encore précoce du (potentiel) développement d’une empirie juridique à la française , des choses à dire et des pratiques à exposer à ceux qui la promeuvent. Il en aurait d’autant plus que cette appétence particulière lui a déjà permis d’aborder les écueils, difficultés et obstacles sur lesquels cette dernière bute aujourd’hui. Sans avoir toutes les réponses à toutes les questions, le refuge créé par les comparatistes à l’empirie juridique apparaît comme l’une des multiples voix à entendre si la pensée juridique française devait, finalement, faire une place à cette voie alternative.
Les voies du polylogue
Authors: Vanoosthuyse François 
Published: July 2024

Le polylogue est une structure dont la fréquence, la complexité et la portée sémantique sont particulièrement remarquables dans le roman français du xix e siècle. La linguistique conversationnelle a élaboré une description d’ensemble des structures polylogales, en différenciant des types de dynamique interactionnelle, des types de locuteurs et d’auditeurs, des manières de gérer les tours de parole. Cette étude s’intéresse au polylogue dans la perspective d’une poétique et d’une histoire du roman. On y distingue deux structures principales (elles-mêmes susceptibles d’être déclinées) : le dialogue à plus de deux personnages et le collage-montage de dialogues, plus caractéristique des productions de la seconde moitié du siècle. On réfléchit aux enjeux sémantiques (notamment politiques) de la structure polylogale dans le contexte post-révolutionnaire, et aux enjeux de son ironisation par le montage.
Le dialogue médical dans les romans réalistes et naturalistes du second XIX e siècle
Authors: Tron-Ymonet Laure-Hélène 
Published: July 2024

Le xix e siècle permet le développement de la clinique. Le médecin apprend à lire sur les corps les indices de la maladie. Cette enquête visuelle est renforcée par le dialogue que le médecin instaure avec son patient : tandis que l’interrogatoire auquel il le soumet permet de construire l’histoire de la maladie, le discours qu’il propose est supposé donner un sens aux symptômes du patient. Alors qu’ils sont pressentis comme le lieu de représentation par excellence de ce dialogue d’enquête, les romans réalistes et naturalistes du second xix e siècle, pourtant désireux de relayer les nouveaux discours médicaux et de participer à la construction des savoirs de leur temps, semblent toujours l’escamoter ou le dévoyer. Cet article entend étudier ces modalités de transformation du discours médical et faire émerger, ainsi, les fonctions qu’il prend au sein de la diégèse.