bluuebunny/crossref_metadata_2025_split huggingface dataset:
Activity of a Gel Combination of Aloe Vera (Aloe Vera (L) Burm.F.) and Snail Mucus (Achatina fulica (Ferussac, 1821)) on Burn Wounds in Male White Rats (Rattus norvegicus) Wistar Strains
Authors: Sianipar Artha Yuliana , Prayoga Andre , Yolanda Nainggolan Agrecia 
Published: July 2023

Burn injury is produced by thermal stress on the skin tissue. This research aimed to determine the combination of Aloe vera and snail mucus used to treat burns and determine the optimal formula. The research was pure with only a randomized control design, including F1 being given placebo gel, F1 (10%:10%), F2 (10%:15%), F3 (10%:20%), and F4 being given bioplacenton. The gel evaluation and tested for the ability to treat burns on rats for about 21 days. The combination gel made a homogenous formulation with a pH 6 based on pH paper while pH meter results were around 6,27- 6,35 cm, a spread of 5,70-6,60 cm, and a viscosity value of 5.600-7.600 cps that was stable for 3 weeks of storage. This evaluation’s findings are consistent with the provisions of National Standard Indonesia (SNI). The activity optimal combination gel obtained by examining the average diameter and discoloration were 10%:20% (0,5560 cm), 10%:15% (0,8120 cm), 10%:10% (0,9860 cm), bioplacenton (0,4780 cm), and placebo gel (1,5340 cm). On the 21st day, the skin condition of K1, K2, K3, and K4 was normal, however, K0 was not normal. The statistical analysis data is normally distributed (p≥0,05), homogeneous (p≥0,05), and a significant difference in all groups (p0,05). According to the experiment, three gel combination of Aloe vera and snail mucus have an effect on healing burns but 10%:20% (F3) could accelerate the optimal healing process.
Gross and Histopathological Findings of Stomach in Cases of Fatal Poisonings Reported at a Tertiary Care Hospital
Authors: Harish Kumar Poola  , Mahesh Mandala  , Ganja Chandra Deepak  , Kattamreddy Ananth Rupesh  , K. Parvathi  , M. Taqiuddin Khan  
Published: July 2023

Poisoning deaths are a major public health concern in India because of intentional consumption of toxic substancesto commit suicide. Poisoning related mortality is huge compared to the morbidity in our country. This is one ofthe reasons for more number of poisoning cases in our autopsy work. Undoubtedly, autopsy is a very essentialtool in knowing the exact cause of death in all these cases. The gross and histopathological examination of postmortemspecimens is crucial for the accurate identification of the cause of poisoning-related deaths along withchemical analysis. In this autopsy-based study, we investigate the gross and histopathological changes in thestomach associated with poisoning caused by various substances, including pesticides, corrosive substances, andmedications.The study included 118 poisoning fatality cases autopsied at Osmania General Hospital, Hyderabad. The mainobjective of this study was to investigate the effects of different poisonings on the stomach wall by conductinggross and histopathological examination of gastric tissue. In addition, the study aimed to evaluate the potentialuse of stomach pathology findings as a diagnostic criterion for various poisonings and to establish a correlationbetween these findings and the chemical analysis of viscera data. The sociodemographic data, circumstances ofpoisoning and reasons for suicide were also studied.The study revealed that the major gross changes observed in the stomach were congestion, erosion, haemorrhage,and paleness, listed in descending order of occurrence. Similarly, the major histopathological findings identifiedin the stomach were congestion, gastritis, necrotic changes, and submucosal haemorrhages, listed in descendingorder of frequency.
In conclusion, this study provides valuable insights into the effects of different poisonings on the stomach wallthrough gross and histopathological examination of gastric tissue. The findings indicate that while gross and histopathological findings alone may not be sufficient for diagnosis, they can be used in conjunction with other diagnostic tools to accurately identify the cause of poisoning-related deaths. Moreover, the study suggests that the development of gastric mucosa specific immunohistochemistry techniques may offer a promising on-spot diagnostic tool for poisoning cases.
Attention to space and time: Independent or interactive systems? A narrative review
Authors: Capizzi Mariagrazia , Chica Ana B. , Lupiáñez Juan , Charras Pom 
Published: July 2023

AbstractWhile there is ample evidence for the ability to selectively attend to where in space and when in time a relevant event might occur, it remains poorly understood whether spatial and temporal attention operate independently or interactively to optimize behavior. To elucidate this important issue, we provide a narrative review of the literature investigating the relationship between the two. The studies were organized based on the attentional manipulation employed (endogenous vs. exogenous) and the type of task (detection vs. discrimination). Although the reviewed findings depict a complex scenario, three aspects appear particularly important in promoting independent or interactive effects of spatial and temporal attention: task demands, attentional manipulation, and their combination. Overall, the present review provides key insights into the relationship between spatial and temporal attention and identifies some critical gaps that need to be addressed by future research.
Tracking X-Ray Source Movement in a Retracting Flux Tube
Authors: Unverferth John , Reep Jeffrey W. 
Published: July 2023

Abstract
Solar flares produce sources of localized, enhanced X-ray emission, thought to be due to the acceleration of nonthermal electrons and the transport of energy away from the reconnection site. The 2002 November 28 C1.6 limb flare showed clear X-ray source motion in the Reuven Ramaty High Energy Solar Spectroscopic Imager observations at 3–10 keV propagating from the apex of the flaring arcade, down toward the footpoints, and then rising back into the corona. Previous work attempted to model this motion using simulations driven by heating with an electron beam or thermal conduction front, finding reasonable agreement only if there were large initial densities. This work extends the previous model by considering a flux tube that retracts through a current sheet away from a magnetic reconnection site. The retraction model includes drag to slow motion in the current sheet, which allows us to vary the energy released by the retraction. This retraction causes a dense and superhot plug of material to form at the loop apex, naturally causing a thermal X-ray source to form in the corona. We find that the observed X-ray source motion, however, is most likely thermal and a signature of the evaporation fronts after initially filling the flux tube.
Warm Molecular Gas in the Central Parsecs of the Buried Nucleus of NGC 4418 Traced with the Fundamental CO Rovibrational Absorptions
Authors: Ohyama Youichi , Onishi Shusuke , Nakagawa Takao , Matsumoto Kosei , Isobe Naoki , Shirahata Mai , Baba Shunsuke , Sakamoto Kazushi 
Published: July 2023

Abstract
We investigated the inner buried nucleus of a nearby luminous infrared galaxy, NGC 4418, using high-resolution spectroscopy of fundamental carbon monoxide (CO) rovibrational absorptions around 4.67 μm for the first time. This method allowed us to examine the physical and kinematical properties in the hot inner region of this nucleus. We detected a series of both very deep (partly saturated) 12CO and moderately deep (optically thin) 13CO absorption lines and inferred a large column density (N
H2 = (5 ± 3) × 1023 cm−2 in front of the 5 μm photosphere) of warm (T
ex ≃ 170 K) molecular gas by assuming an isothermal plane-parallel slab illuminated by a compact background mid-infrared-emitting source. We modeled that the warm CO absorber almost covers the central heating source and that it is an inner layer around the 5 μm photosphere (at r = several parsecs) of a compact shroud of gas and dust (d ∼ 100 pc). The width of the absorption lines (110 km s−1) and their small deviation from the systemic velocity (<10 km s−1) are consistent with a warm and turbulent layer with little bulk motion in the radial direction.
The Evolution of Population III and Extremely Metal-poor Binary Stars
Authors: Tsai Sung-Han , Chen Ke-Jung , Whalen Daniel , Ou Po-Sheng , Woods Tyrone E. 
Published: July 2023

Abstract
Numerical simulations have now shown that Population III (Pop III) stars can form in binaries and small clusters and that these stars can be in close proximity to each other. If so, they could be subject to binary interactions such as mass exchange that could profoundly alter their evolution, ionizing UV and Lyman–Werner photon emission and explosion yields, with important consequences for early cosmological reionization and chemical enrichment. Here we investigate the evolution of Pop III and extremely metal-poor binary stars with the MESA code. We find that interactions ranging from stable mass transfer to common envelope evolution can occur in these binaries for a wide range of mass ratios and initial separations. Mass transfer can nearly double UV photon yields in some of these binaries with respect to their individual stars by extending the life of the companion star, which in turn can enhance early cosmological reionization but also suppress the formation of later generations of primordial stars. Binary interactions can also have large effects on the nucleosynthetic yields of the stars by promoting or removing them into or out of mass ranges for specific SN types. We provide fits to total photon yields for the binaries in our study for use in cosmological simulations.
Slow Solar Wind Connection Science during Solar Orbiter’s First Close Perihelion Passage
Authors: Yardley Stephanie L. , Owen Christopher J. , Long David M. , Baker Deborah , Brooks David H. , Polito Vanessa , Green Lucie M. , Matthews Sarah , Owens Mathew , Lockwood Mike , Stansby David , James Alexander W. , Valori Gherardo , Giunta Alessandra , Janvier Miho , Ngampoopun Nawin , Mihailescu Teodora , To Andy S. H. , van Driel-Gesztelyi Lidia , Démoulin Pascal , D’Amicis Raffaella , French Ryan J. , Suen Gabriel H. H. , Rouillard Alexis P. , Pinto Rui F. , Réville Victor , Watson Christopher J. , Walsh Andrew P. , De Groof Anik , Williams David R. , Zouganelis Ioannis , Müller Daniel , Berghmans David , Auchère Frédéric , Harra Louise , Schuehle Udo , Barczynski Krysztof , Buchlin Éric , Cuadrado Regina Aznar , Kraaikamp Emil , Mandal Sudip , Parenti Susanna , Peter Hardi , Rodriguez Luciano , Schwanitz Conrad , Smith Phil , Teriaca Luca , Verbeeck Cis , Zhukov Andrei N. , De Pontieu Bart , Horbury Tim , Solanki Sami K. , del Toro Iniesta Jose Carlos , Woch Joachim , Gandorfer Achim , Hirzberger Johann , Súarez David Orozco , Appourchaux Thierry , Calchetti Daniele , Sinjan Jonas , Kahil Fatima , Albert Kinga , Volkmer Reiner , Carlsson Mats , Fludra Andrzej , Hassler Don , Caldwell Martin , Fredvik Terje , Grundy Tim , Guest Steve , Haberreiter Margit , Leeks Sarah , Pelouze Gabriel , Plowman Joseph , Schmutz Werner , Sidher Sunil , Thompson William T. , Louarn Philippe , Federov Andrei 
Published: July 2023

Abstract
The Slow Solar Wind Connection Solar Orbiter Observing Plan (Slow Wind SOOP) was developed to utilize the extensive suite of remote-sensing and in situ instruments on board the ESA/NASA Solar Orbiter mission to answer significant outstanding questions regarding the origin and formation of the slow solar wind. The Slow Wind SOOP was designed to link remote-sensing and in situ measurements of slow wind originating at open–closed magnetic field boundaries. The SOOP ran just prior to Solar Orbiter’s first close perihelion passage during two remote-sensing windows (RSW1 and RSW2) between 2022 March 3–6 and 2022 March 17–22, while Solar Orbiter was at respective heliocentric distances of 0.55–0.51 and 0.38–0.34 au from the Sun. Coordinated observation campaigns were also conducted by Hinode and IRIS. The magnetic connectivity tool was used, along with low-latency in situ data and full-disk remote-sensing observations, to guide the target pointing of Solar Orbiter. Solar Orbiter targeted an active region complex during RSW1, the boundary of a coronal hole, and the periphery of a decayed active region during RSW2. Postobservation analysis using the magnetic connectivity tool, along with in situ measurements from MAG and SWA/PAS, showed that slow solar wind originating from two out of three of the target regions arrived at the spacecraft with velocities between ∼210 and 600 km s−1. The Slow Wind SOOP, despite presenting many challenges, was very successful, providing a blueprint for planning future observation campaigns that rely on the magnetic connectivity of Solar Orbiter.
Ultradiffuse Galaxies (UDGs) with Hyper Suprime-Cam. I. Revised Catalog of Coma Cluster UDGs*
Authors: Bautista Jose Miguel G. , Koda Jin , Yagi Masafumi , Komiyama Yutaka , Yamanoi Hitomi 
Published: July 2023

Abstract
This is the first in a series of papers on the properties of ultradiffuse galaxies (UDGs) in clusters of galaxies. We present an updated catalog of UDGs in the Coma Cluster using g- and r-band images obtained with Hyper Suprime-Cam (HSC) of the Subaru telescope. We develop a method to find UDGs even in the presence of contaminating objects, such as halos and background galaxies. This study expands upon our previous works that covered about half the area of the Coma Cluster. The HSC observations covered the whole Coma Cluster up to the virial radius and beyond (an area twice as large as the previous studies) and doubled the numbers of UDGs (r
eff, r ≥ 1.5 kpc) and sub-UDGs (1.0 ≤ r
eff, r < 1.5 kpc) to 774 and 729, respectively. The new UDGs show internal properties consistent with those of previous studies (e.g., a Sérsic index of approximately 1), and are distributed across the cluster, with a concentration around the cluster center. The whole cluster coverage clearly revealed an excess of their distribution toward the east to southwest direction along the cluster center, where Coma connects to other large-scale structure, and where a known substructure exists (the NGC 4839 subgroup). The alignment of the UDG distribution along the large-scale structure around Coma supports the interpretation that most of them lie at the distance of the Coma Cluster and the NGC 4839 subgroup.
The First AGILE Solar Flare Catalog
Authors: Ursi A. , Parmiggiani N. , Messerotti M. , Pellizzoni A. , Pittori C. , Longo F. , Verrecchia F. , Argan A. , Bulgarelli A. , Tavani M. , Tempesta P. , D’Amico F. 
Published: July 2023

Abstract
We report the Astro-rivelatore Gamma a Immagini LEggero (AGILE) observations of solar flares, detected by the onboard anticoincidence system in the 80–200 keV energy range, from 2007 May 1 to 2022 August 31. In more than 15 yr, AGILE detected 5003 X-ray, minute-lasting transients, compatible with a solar origin. A cross-correlation of these transients with the Geostationary Operational Environmental Satellites (GOES) official solar flare database allowed us to associate an intensity class (i.e., B, C, M, or X) to 3572 of them, for which we investigated the main temporal and intensity parameters. The AGILE data clearly revealed the solar activity covering the last stages of the 23rd cycle, the whole 24th cycle, and the beginning of the current 25th cycle. In order to compare our results with other space missions operating in the high-energy range, we also analyzed the public lists of solar flares reported by RHESSI and Fermi Gamma-ray Burst Monitor. This catalog reports 1424 events not contained in the GOES official data set, which, after statistical comparisons, are compatible with low-intensity, short-duration solar flares. Besides providing a further data set of solar flares detected in the hard X-ray range, this study allowed to point out two main features: a longer persistence of the decay phase in the high-energy regime, with respect to the soft X-rays, and a tendency of the flare maximum to be reached earlier in the soft X-rays with respect to the hard X-rays. Both these aspects support a two-phase acceleration mechanism of electrons in the solar atmosphere.
Biotopes of the intertidal zone in Clarence Island (south of the Strait of Magellan)
Authors: Aldea Cristian , Hernández Cristina , Novoa Leslie , Olivera Francisco , Haeger Christian , Bello Nadja 
Published: July 2023

The characteristics of the Strait of Magellan promote the formation of unique environments, with diverse habitats and marine organisms. This fragmentation of the landscape generates diverse little-explored ecological associations, especially in the zone of sub-Antarctic islands of the Tierra del Fuego archipelago. One way to address this lack of knowledge is through the biotope characterization methodology, with ecological units composed of the habitat and the communities associated with these environments, obtaining data and information on the dominant and incidental taxonomic groups. This is a good research model to conduct baseline studies in coastal benthic marine environments.
A data set in Darwin Core standard is presented of the species that make up the intertidal biotopes of Clarence Island (Tierra del Fuego Archipelago, south of the Strait of Magellan). This includes 50 identified species and the specific coordinates for each sampled location, with a total of 1400 georeferenced records. Mollusks were the most diverse taxon with 21 species, followed by algae (14 species). Sessile organisms such as the barnacles Elminius kingii and Austromegabalanus psittacus predominate in these ecosystems, followed by bivalve mollusks such as Choromytilus chorus and Mytilus chilensis, which together with Nacella magellanica and the alga Hildenbrandia sp. make up more than 50% of the total records. The inclusion of biotope patterns in this study complements the information on benthic marine flora and fauna in the intertidal zone, including new records for the coast in the Clarence Island area, which is within the boundary of the Kawésqar National Park.
Le modèle de la fermentation chimique dans Le Fils naturel de Diderot
Authors: Granger Charline 
Published: July 2023

Le Fils naturel de Diderot est fondé sur le sacrifice de Dorval, qui renonce à sa passion pour Rosalie et fait le choix de la vertu. Or cette conversion n’est pas envisagée comme le fruit d’un mystère transcendant : Diderot la pense au contraire sur le modèle de la fermentation, comme une transformation radicale, mais lente et, surtout, explicable, régie par des lois observables. Le dramaturge nous propose au fond une expérience scientifique : observer cette conversion s’opérer dans les personnages du Fils naturel et tenter de la susciter chez le spectateur.
Le théâtre de Buzzati : regarder l’invisible
Authors: Mazzone Serena 
Published: July 2023

La dramaturgie de Buzzati se caractérise par un réseau d’interconnexions et un multilinguisme qui mobilise des éléments théâtraux d'origines diverses, dont le sens est sans cesse décontextualisé voire redéfini. Les liens avec le théâtre de l’absurde, avec la littérature fantastique, avec l’existentialisme (Albert Camus) filtré par un lyrisme tout proche de Leopardi, créent un théâtre visionnaire et symbolique dans lequel les questions de l’homme prennent forme sur scène, avec le sens du mystère qui les accompagne : l’invisible devient chair, accentuant ainsi sa propre action perturbatrice. L’homme évolue dans un univers qu’il ne peut déchiffrer, à la merci de forces auxquelles il ne peut s’opposer, et le destin, souvent cynique et moqueur, semble écraser toutes ses aspirations. La condition existentielle tragique de l’homme se dilue néanmoins dans la vocation morale qui résulte d’une satire des mœurs particulièrement accentuée, évoluant en équilibre entre nihilisme et aspiration fidéiste ; une perte de sens qui aboutit à une sorte de « fatalisme » philosophique très proche de l’ironie de Jacques le Fataliste de Diderot. Dans un équilibre suspendu entre un mystère sans nom et un mystère qui prend la forme d'une « révélation », l’exploration des zones d’ombre qui entourent l’homme s'enveloppe d’une transcendance où le sens du sacré, perdu dans un monde dominé par la rationalité et la productivité, s’élève à la modalité du « sentir », pour finalement s’incarner dans le rite même du théâtre : la scène récupère le « regard » de l’homme qui pousse à la rencontre avec l’invisible, quelle que soit la conception que l’on en ait.
Un « nouveau » fragment arabe de la version kindienne du De insomniis d’Aristote et sa réception dans une recension des Principes des opinions des habitants de la cité vertueuse d’al‑Fārābī
Authors: Rashed Marwan 
Published: July 2023

Cet article présente un texte conservé dans un manuscrit de Téhéran (Mağlis Šūrā 10055), qui a préservé un fragment de la traduction arabe des Parva naturalia d’Aristote, actuellement connue uniquement par un long extrait conservé à Rampur, en Inde (ms. 1752). Ce texte, dont on ne connaissait jusqu’à présent qu’un seul exemplaire, est constitué d’un titre, d’une citation d’Aristote et d’un commentaire de cette citation d’une quinzaine de lignes. La citation reformule légèrement la définition aristotélicienne du rêve telle qu’elle est donnée à la fin du traité Des rêves (462a29‑31). En se fondant sur le texte édité, l’article montre que des spécificités du commentaire, dont des parallèles étroits avec d’autres textes conservés, permettent de l’attribuer à al‑Kindī lui‑même. Cette conclusion s’étend aux Parva naturalia de Rampur, dont l’article montre que le texte de Téhéran devait, à l’origine, faire partie. On montre enfin que ce texte est au fondement du chapitre 14 des Principes des opinions des habitants de la cité vertueuse d’al‑Fārābī, consacré à la prophétie. Plus précisément, on montre que ce chapitre constitue lui‑même un commentaire précis du nouveau texte, que donc al‑Fārābī, dans ce texte, emprunte à al‑Kindī l’essentiel de son interprétation naturaliste de la prophétie. Cette conclusion éclaire d’un nouveau jour la question si mystérieuse de l’influence d’al‑Kindī sur al‑Fārābī.
La pénibilité au travail dans les professions de l’économie verte
Authors: Havet Nathalie , Bayart Caroline , Penot Alexis 
Published: July 2023

Ces dernières décennies, les politiques publiques mises en place aux niveaux national et européen ont permis une forte croissance des emplois relevant de « l’économie verte  ». Dans ce contexte, il est pertinent de se demander si ces emplois, censés limiter les nuisances environnementales, garantissent également des conditions de travail satisfaisantes et durables. En se basant sur les deux dernières éditions de l’enquête française Surveillance médicale des expositions aux risques professionnels (Sumer) de 2010 et 2017, cet article propose d’étudier l’évolution de l’exposition des salariés aux facteurs de pénibilité sur leur lieu de travail (contraintes physiques marquées, environnement physique agressif, rythmes de travail atypiques). L’objectif est de comparer les professions de l’économie verte et les professions des autres secteurs, et d’étudier l’évolution des indicateurs de pénibilité entre les deux enquêtes. Nous chercherons à savoir si le développement de l’économie verte peut être un levier pour réduire certaines inégalités d’exposition aux risques professionnels ou si, au contraire, il contribue à la dégradation des conditions de travail de groupes de salariés déjà fragilisés.