bluuebunny/crossref_metadata_2025_split huggingface dataset:
Analisis Kinerja Keuangan Menggunakan Analisis Dupont Sistem (Studi Empiris Pada PT Sumber Alfaria Trijaya Tbk Periode 2019-2022)
Authors: Oktaviani Azzahara Rita , Sentosa Nona Abigail , Rostiani Yeny , Rustiadi Rizzky 
Published: November 2023

Penelitian ini bertujuan untuk menganalisis kinerja keuangan menggunakan anailis DuPont pada PT PT Sumber Alfaria Trijaya Tbk, menggunakan laporan auditan tahun 2019 – 2022 yang dipublikasikan di Bursa Efek Indonesia. hasil analisis data diperoleh bahwa tingkat Net Profit Margin (NPM) pada tahun 2022 mengalai peningkatn, Hal ini disebabkan karena adanya peningkatan pada laba bersih dan penjualan. Peningkatan laba bersih disebabkan meningkatnya penjualan, penambahan jumlah gerai, dan pendapatan lainya. Hasil perhitungan otal Asset Turnover hasil perhitungan mengalami peningkatan di tahun 2022 sebesar 3,15 kali (naik 0,05 kali) dari 3,10 kali pada tahun 2021. Hal ini disebabkan karena adanya penurunan penjualan dan total aset. Return on Investment (ROI ) tahun 2022 mengalami peningkatan sebesar 0,094% (naik 0,023%) dari 0,094% pada tahun 2021. Hal ini disebabkan karena Net Profit Margin mengalami penurunan dan Total Asset Turnover mengalami peningkatan. . Hasil perhitungan Return on Equity (ROE) pada tahun 2022 mengalami peningkatan sebesar 0,25% (naik 0,05%) dari 0,20 pada tahun 2021. Hal ini disebabkan oleh Return on Investment mengalami penurunan dan Equity Multiplier mengalami peningkatan.
Decision-making during fires in mountainous areas: a comparative analysis of monitoring methods
Authors: Matveev Aleksandr , Matiev Ruslan 
Published: November 2023

One of the main factors ensuring a reduction in the risk of wild fires or their prompt elimination at the initial stage of a fire is the creation of an effective monitoring system. Obtaining reliable and timely data on natural fires makes it possible to increase the adequacy of management decisions aimed at responding to and minimizing possible damage from fires.
The article discusses various methods of monitoring active wildfires in mountainous areas: space, aviation, ground and using unmanned aerial vehicles. An analysis of the advantages and disadvantages of each method was carried out. It has been shown that traditional methods have limitations related to the frequency of data acquisition, measurement accuracy, safety, cost and other factors. This is especially true when monitoring in mountainous areas.
The use of unmanned aerial vehicles is considered a promising direction, as it allows one to obtain operational information with high detail. The advantages of unmanned aerial vehicles are noted in speed of response, maneuverability, economic efficiency and the absence of risk for direct performers.
An example of a natural fire in a mountainous area that occurred in a specially protected natural area in one of the constituent entities of the Russian Federation, demonstrating the shortcomings of traditional methods, is considered. The feasibility of a combined approach for increasing the efficiency and accuracy of monitoring is shown.
Comparative Analysis of Contrast-Enhanced Ultrasound and Computed Tomography in the Differential Diagnosis of Focal Liver Lesions in Patients with a History of Advanced Cancer
Authors: Козубова Ксения Вячеславовна , Бусько Екатерина Александровна , Багненко Сергей Сергеевич , Кадырлеев Роман Андреевич , Костромина Екатерина Викторовна , Гончарова Анастасия Борисовна , Буровик Илья Александрович , Оконечникова Дарья Викторовна , Любимская Эльвира Сергеевна , Постаногов Роман Анатольевич 
Published: November 2023

Цель. Проанализировать диагностическую эффективность мультипараметрического ультразвукового исследования с контрастным усилением в дифференциальной диагностике очаговых образований печени у онкопациентов и сравнить полученные данные с компьютерной томографией и гистологическим заключением.
Материалы и методы. Проведён ретроспективный анализ результатов исследований 123 пациентов с очаговыми изменения печени, из них 96 женщин (средний возраст 56,1 ±13,6) и 27 мужчин (средний возраст 55,0±14,0). Всем пациентам проводилось мультипараметрическое ультразвуковое исследование и компьютерная томография с контрастированием. При подозрении на злокачественный процесс выполнялась трепан-биопсия печени под ультразвуковым наведением. В случае выявления признаков, характерных для доброкачественных образований, пациент находился на динамическом контроле каждые 3 месяца в первый год наблюдения, отсутствие динамики через 6-12 месяцев свидетельствовало в пользу доброкачественного процесса. При увеличении размеров образования также выполнялась морфологическая верификация.
Результаты. Результаты для серошкального режима составили: чуствительность (Ч)-58,1%, специфичность (С)-68,4%, точность (Т)-60,2%, прогностическая ценность положительного результата (ПЦПР)- 87,8%, прогностическая ценность отрицательного результата (ПЦОР)-29,5%. Эффективность контрастно-усиленного ультразвукового исследования (КУУЗИ) значимо превышала исследование в традиционном серошкальном режиме и составила: Ч-90,5%, С-84,2%, Т-89,2%, ПЦПР-95,7%, ПЦОР-69,6%. Для компьютерной томографии с контрастным усилением (КТ с КУ) результаты были сопоставимы с КУУЗИ и составили: Ч-83,6%, С-78,9%, Т-82,6%, ПЦПР-93,8%, ПЦОР-55,6%.
Полученные нами значения подтверждают высокую информативность КУУЗИ в оценке очагового поражения печени, в связи с чем в ряде случаев (отсутствие технической возможности проведения или наличие противопоказаний к КТ с КУ, а также полученные неоднозначные результаты по другим методика) может выступить в качестве метода выбора.
Заключение. Мультимодальная диагностика превосходит единый метод визуализации по чувствительности скрининга и точности диагностики. КТ с КУ и КУУЗИ дополняют друг друга при дифференциальной диагностике очагов в печени неясного генеза. Использование КТ с КУ в сочетании с КУУЗИ показывает клиническую ценность для пациентов, что особенно важно у лиц с отягощённым онкоанамнезом.
Virgilluethite: A New Mineral and the Natural Analogue of Synthetic β-MoO3·H2O, from Cookes Peak, Luna County, New Mexico, USA
Authors: Yang Hexiong , Gu Xiangping , Gibbs Ronald B. , Downs Robert T. 
Published: November 2023

Abstract
The new mineral virgilluethite, ideally β-MoO3·H2O, was discovered in an unnamed short adit on the Summit group of claims near Cookes Peak, Luna County, New Mexico, USA. All virgilluethite crystals are pseudomorphs after sidwillite and occur as aggregates of sub-parallel platy crystals. Associated minerals include sidwillite, raydemarkite, tianhuixinite, ilsemannite, jordisite, powellite, fluorite, baryte, pyrite, and quartz. Virgilluethite is pale yellow-green in transmitted light, transparent with white streak and vitreous luster. It is flexible with a Mohs hardness of ∼2; cleavage is perfect on {010}. No twinning was observed visually. The measured and calculated densities are 3.71(5) and 3.69 g/cm3, respectively. Virgilluethite is insoluble in water or hydrochloric acid. An electron probe microanalysis yielded an empirical formula (Mo1.00)O3·H2O based on 4 O apfu.
Virgilluethite is the natural analogue of the β-form of MoO3·H2O, which was first synthesized over a century ago (Rosenheim & Davidsohn 1903). It is monoclinic, space group P21/c, with unit-cell parameters a = 7.2834(3), b = 10.6949(6), c = 7.4861(3) Å, β = 112.779(2)°, V = 583.03(5) Å3, and Z = 4. The crystal structure of virgilluethite, which is topologically identical to that of tungstite (WO3·H2O), is characterized by highly distorted and elongated MoO5(H2O) octahedra that share four corners in the equatorial plane with one another to form sheets parallel to (010). These sheets, analogous to those in sidwillite, are held together by H-bonding between the H2O molecule and the O atom in the axial position in the adjacent sheets. Virgilluethite and raydemarkite are dimorphs of MoO3·H2O. Unlike virgilluethite, the MoO6 octahedra in raydemarkite share edges to form isolated double chains, resembling those found in zhenruite, (MoO3)2·H2O.
Structural Controls on the Origin and Emplacement of Lithium-Bearing Pegmatites
Authors: Silva David , Groat Lee , Martins Tânia , Linnen Robert 
Published: November 2023

Abstract
Exploration and mining of lithium pegmatites has increased in recent years to meet the growing demand for critical metals, which are required for electric-powered transportation as well as sustainable energy production and storage. Pegmatite deposits produced approximately 60% of global lithium production in 2018, the vast majority of which was from spodumene pegmatites. However, there is lack of comprehensive models linking mineral system evolution and structural controls of lithium pegmatites. The majority of studies on lithium pegmatites have focused on chemical fractionation and assume that pegmatites have evolved from a parental granitic source, yet problems emerge when the connection between the granitic source and the pegmatite bodies is not obvious. This lack of connection has given rise to an alternative model of pegmatite formation, the anatectic model. In the anatectic model, granitic pegmatites form from granitic melts produced by partial melting of a suitable lithology, typically pelitic metasediments, without forming a large granitic body followed by fractional crystallization.
Here, we first examine the formation of granitic melts related to anatexis, as well as how regional crustal structures influence chemical composition, crustal migration, and melt accumulation within the crust. We next examine the Wekusko Lake pegmatite field located in Manitoba, Canada, in terms of the probable melt source migration, the relationship between crustal-scale strain-zones and spatial pegmatite emplacement, and the chemical fractionation trend that records the formation of lithium-enriched pegmatites.
AuDrA: An automated drawing assessment platform for evaluating creativity
Authors: Patterson John D. , Barbot Baptiste , Lloyd-Cox James , Beaty Roger E. 
Published: November 2023

AbstractThe visual modality is central to both reception and expression of human creativity. Creativity assessment paradigms, such as structured drawing tasks Barbot (2018), seek to characterize this key modality of creative ideation. However, visual creativity assessment paradigms often rely on cohorts of expert or naïve raters to gauge the level of creativity of the outputs. This comes at the cost of substantial human investment in both time and labor. To address these issues, recent work has leveraged the power of machine learning techniques to automatically extract creativity scores in the verbal domain (e.g., SemDis; Beaty & Johnson 2021). Yet, a comparably well-vetted solution for the assessment of visual creativity is missing. Here, we introduce AuDrA – an Automated Drawing Assessment platform to extract visual creativity scores from simple drawing productions. Using a collection of line drawings and human creativity ratings, we trained AuDrA and tested its generalizability to untrained drawing sets, raters, and tasks. Across four datasets, nearly 60 raters, and over 13,000 drawings, we found AuDrA scores to be highly correlated with human creativity ratings for new drawings on the same drawing task (r = .65 to .81; mean = .76). Importantly, correlations between AuDrA scores and human raters surpassed those between drawings’ elaboration (i.e., ink on the page) and human creativity raters, suggesting that AuDrA is sensitive to features of drawings beyond simple degree of complexity. We discuss future directions, limitations, and link the trained AuDrA model and a tutorial (https://osf.io/kqn9v/) to enable researchers to efficiently assess new drawings.
Influence of Crustal Magnetic Fields on Horizontal Plasma Transport and Ion Escape on Mars
Authors: Li Guokan , Lu Haoyu , Li Yun , Cao Jinbin , Zhang Xiaoxin , Li Shibang 
Published: November 2023

Abstract
Owing to its unevenly distributed crustal fields, Mars acts as a unique obstacle to the solar wind. In the presence of the crustal fields, the transport of the planetary ions on the dayside ionosphere exhibits north–south asymmetry. Additionally, the heavy-ion loss in the magnetotail is affected by the crustal fields. In this paper, a three-dimensional multispecies magnetohydrodynamic model is employed to simulate Mars–solar wind interactions. Numerical results indicate that the meridional transport is dominant in most areas on the dayside ionosphere. In the presence of the crustal fields, the meridional transport on the southern hemisphere (southward transport) is reduced by more than 70% above the strong crustal sources, and the zonal velocity shows local changes inside strong and weak crustal field regions. These effects result in an increase or decrease in the number density of the heavy ions reaching the terminator, thereby influencing the thickness of the ionosphere. Decreased southward velocity leads to a reduction in the heavy-ion loss on the southern magnetotail. The radial outward flux is reduced by more than 30% for O2
+ and CO2
+ and by 10% for O+. This study shows that in addition to the zonal transport, the meridional transport is important for the day-to-night transport on the dayside of Mars. Collectively, the horizontal plasma transport, controlled by crustal fields, is associated with the altered ionosphere structure and reduced heavy-ion loss in the magnetotail.
Circumgalactic Medium at High Halo Masses—Signatures of Cold Gas Depletion in Luminous Red Galaxies
Authors: Smailagić Marijana , Prochaska Jason Xavier , Burchett Joseph , Zhu Guangtun 
Published: November 2023

Abstract
We study ultraviolet H i and metal-line transitions in the circumgalactic medium (CGM) of 15 massive, quenched luminous red galaxies (LRGs) at redshift z ∼ 0.5 and with impact parameters up to 400 kpc. We selected eight LRG–CGM systems to study general properties of the CGM around LRGs, while the other seven are already known to contain cool CGM gas from Mg ii optical studies (Mg ii-LRGs). In the general LRG population, we detect H i in four of eight LRGs, in all cases with N
H I < 1016.7cm−2. In contrast, all Mg ii-LRGs show H i; for four LRGs, the H i column density is N
H I ≳ 1018cm−2. The CGM of LRGs also shows low and intermediate ionized lines (such as C iii, C ii, Si iii, and Si ii) and highly ionized lines of O vi (we detect O vi around five of seven Mg ii-LRGs and one of eight in the random sample). Next, we combine our sample with literature LRGs and ≲L
* galaxies, and we find that while for ≲L
* galaxies CGM H i Lyα absorption is stronger as galaxies are more massive, the cool CGM traced by H i Lyα is suppressed above stellar masses of M* ∼ 1011.5
M
☉. While most LRG–CGM systems show weak or nondetectable O vi (equivalent width < 0.2 Å), a few LRG–CGM systems show strong O vi 1031, which in most cases likely originates from groups containing both an LRG and a blue star-forming neighboring galaxy.
Mapping Dust Attenuation and the 2175 Å Bump at Kiloparsec Scales in Nearby Galaxies
Authors: Zhou Shuang , Li Cheng , Li Niu , Mo Houjun , Yan Renbin , Eracleous Michael , Molina Mallory , Gronwall Caryl , Ajgaonkar Nikhil , Cheng Zhuo , Guo Ruonan 
Published: November 2023

Abstract
We develop a novel approach to measure the dust attenuation properties of galaxies, including the dust opacity, the shape of the attenuation curve, and the strength of the 2175 Å absorption feature. From an observed spectrum, the method uses a model-independent approach to derive a relative attenuation curve with an absolute amplitude calibrated using NIR photometry. The dust-corrected spectrum is fitted with stellar population models to derive the dust-free model spectrum, which is compared with the observed SED/spectrum from NUV to NIR to determine the dust attenuation properties. We apply this method to investigate dust attenuation on kiloparsec scales using a sample of 134 galaxies with integral field spectroscopy from MaNGA, NIR imaging from 2MASS, and NUV imaging from Swift/UVOT. We find that the attenuation curve slope and the 2175 Å bump in both the optical and NUV span a wide range at kiloparsec scales. The slope is shallower at higher optical opacity, regardless of the specific star formation rate (sSFR), the minor-to-major axis ratio (b/a) of the galaxies, and the location of spaxels within individual galaxies. The 2175 Å bump presents a strong negative correlation with the sSFR, while the correlations with the optical opacity, b/a, and the locations within individual galaxies are all weak. All of these trends appear to be independent of the stellar mass of the galaxies. Our results support the scenario that the variation of the 2175 Å bump is driven predominantly by processes related to star formation, such as the destruction of small dust grains by UV radiation in star-forming regions.
Integral Field Spectroscopy of 13 Tidal Disruption Event Hosts from the Zwicky Transient Facility Survey
Authors: Hammerstein Erica , Cenko S. Bradley , Gezari Suvi , Veilleux Sylvain , O’Connor Brendan , van Velzen Sjoert , Ward Charlotte , Yao Yuhan , Graham Matthew 
Published: November 2023

Abstract
The host galaxies of tidal disruption events (TDEs) have been shown to possess peculiar properties, including high central light concentrations, unusual star formation histories, and “green” colors. The ubiquity of these large-scale galaxy characteristics among TDE host populations suggests that they may serve to boost the TDE rate in such galaxies by influencing the nuclear stellar dynamics. We present the first population study of integral field spectroscopy for 13 TDE host galaxies across all spectral classes and X-ray brightnesses with the purpose of investigating their large-scale properties. We derive the black hole masses via stellar kinematics (i.e., the M–σ relation) and find masses in the range

5.0
≲
log
(

M

BH

/

M

⊙

)
≲
8.0

, with a distribution dominated by black holes with M
BH ∼ 106
M
⊙. We find one object with M
BH ≳ 108
M
⊙, above the “Hills mass”, which if the disrupted star was of solar type, allows a lower limit of a ≳ 0.16 to be placed on its spin, lending further support to the proposed connection between featureless TDEs and jetted TDEs. We also explore the level of rotational support in the TDE hosts, quantified by (V/σ)
e
, a parameter that has been shown to correlate with the stellar age and may explain the peculiar host-galaxy preferences of TDEs. We find that the TDE hosts exhibit a broad range in (V/σ)
e
following a similar distribution as E + A galaxies, which have been shown to be overrepresented among TDE host populations.
Radial and Local Density Dependence of Star Formation Properties in Galaxy Clusters from the Hyper Suprime-Cam Survey
Authors: Jian Hung-Yu , Lin Lihwai , Hsieh Bau-Ching , Umetsu Keiichi , Lopez-Coba Carlos , Oguri Masamune , Bottrell Connor , Toba Yoshiki , Koyama Yusei , Chang Yu-Yen , Kodama Tadayuki , Komiyama Yutaka , More Surhud , Lin Kai-Yang , Nishizawa Atsushi J. , Tanaka Ichi 
Published: November 2023

Abstract
This study examines the impact of cluster environments on galaxy properties using data from the Hyper Suprime-Cam Subaru Strategic Program and an optically selected CAMIRA cluster sample. Specifically, the study analyzes the fractions of quiescent and green valley galaxies with stellar masses above 108.6
M
⊙ at z ∼ 0.2 and 109.8
M
⊙ at z ∼ 1.1, investigating their trends in radius and density. The results indicate that a slow quenching mechanism is at work, as evidenced by a radially independent specific star formation rate reduction of 0.1 dex for star-forming galaxies in a cluster environment. The study also finds that slow quenching dominates fast quenching only for low-mass galaxies (<109.2
M
⊙) near the cluster edge, based on their contributions to the quiescent fraction. After controlling for M
*, z, and local overdensity, the study still finds a significant radial gradient in the quiescent fraction, indicating active ram pressure stripping in dense environments. That said, analyzing the density trend of the quiescent fraction with other fixed parameters suggests that radial and density-related quenching processes are equally crucial for low-mass cluster galaxies. The study concludes that ram pressure stripping is the primary environmental quenching mechanism for high stellar mass galaxies in clusters. By contrast, ram pressure stripping and density-related quenching processes act comparably for low-mass cluster galaxies around the center. Near the cluster boundary, starvation and harassment become the leading quenching processes for low stellar mass galaxies.
Two Candidate Pulsar TeV Halos Identified from Property-similarity Studies
Authors: Zheng Dong , Wang Zhongxiang 
Published: November 2023

Abstract
Teraelectronvolt halos have been suggested to be a common phenomenon associated with middle-aged pulsars. Based on our recent work on the middle-aged pulsar J0631+1036, which is the only known source positionally coincident with a hard teraelectronvolt γ-ray source and likely powers the latter as a teraelectronvolt halo, we select three candidate teraelectronvolt halos from the first Large High Altitude Air Shower Observatory (LHAASO) catalog of γ-ray sources. The corresponding pulsars, given by the positional coincidences and property similarities, are PSR J1958+2846, PSR J2028+3332, and PSR J1849-0001. We analyze the gigaelectronvolt γ-ray data obtained with the Large Area Telescope on board the Fermi Gamma-ray Space Telescope for the first two pulsars, as the last is γ-ray quiet. We remove the pulsed emissions of the pulsars from the source regions from timing analysis, and determine that there are no residual gigaelectronvolt emissions in the regions as any possible counterparts to the teraelectronvolt sources. Considering the previous observational results for the source regions and comparing the two pulsars to Geminga (and Monogem), the LHAASO-detected teraelectronvolt sources are likely the pulsars’ respective teraelectronvolt halos. We find that the candidate and identified teraelectronvolt halos, including that of PSR J1849-0001, have luminosities at 50 TeV (estimated from the differential fluxes) approximately proportional to the spin-down energy

E

̇

of the pulsars, and the ratios of the former to the latter are ∼6 × 10−4.
« […] plus loin que l’inconscient »
Authors: Askofaré Sidi 
Published: November 2023

Contrairement à ce qui a pu se penser ou se dire, Le Sinthome n’aura pas été le « dernier mot » du « Retour à Freud » de Jacques Lacan. Ce dernier reviendra, avant Le moment de conclure – donc dans son propre temps pour comprendre – sur le maître-mot de la découverte freudienne : l’inconscient. Non seulement pour, cet inconscient, le repenser à nouveaux frais et le renommer, insu, mais pour aller plus loin. Au-delà de l’inconscient : le parlêtre ? Le présent article tente d’établir en quoi, si le parlêtre lacanien n’est pas seulement la condensation de l’être parlant, mais aussi et surtout le terme proposé par Lacan comme substitut à l’inconscient, cette substitution vient parachever tout une série de mises en question, de critiques et de mises en cause, avec des conséquences, encore insoupçonnées – à explorer, donc – sur le corps, l’identification, l’interprétation et la fin de l’analyse