bluuebunny/crossref_metadata_2025_split huggingface dataset:
Islamic Consumption Behavior In Realizing Family Welfare
Authors: Januari Anas Tania , Rofiq Aunur , Khusnudin Khusnudin 
Published: August 2024

Consumption in a country's economy, with higher levels of consumption causing increased economic activity and changes in a country's national income. The impact of consumption on household financial stability, with excessive spending relative to income causing personal financial problems. material and spiritual well-being in the household, is very important in balancing worldly and spiritual needs for overall well-being. This research is qualitative research with a normative approach. Obtaining secondary data in the form of data on welfare indicators which refer to the consumption behavior of Indonesian people obtained from the Central Statistics Agency in a certain period. This data is used as a reference in the importance of discussing consumption behavior, especially in the context of sharia. Meanwhile, the behavioral theory approach is used for the purposes of analyzing the goals of consumption behavior by adhering to Islamic principles to realize prioritized welfare among households. Research shows that consumption behavior in realizing the welfare of Muslim families can be seen from several indicators listed in data processed by the Central Statistics Agency. Consumption pattern indicators are influenced by income levels which reflect people's purchasing power and abilities. Meanwhile, other indicators can be seen from the quality of health and nutrition, education, housing and other social issues, such as a lifestyle that follows the times
A Time Trend and Persistence Analysis of Sunflower Oil and Olive Oil Prices in the Context of the Russia-Ukraine War
Authors: Monge Manuel 
Published: August 2024

The imbalances between sunflower oil production (Ukraine) and olive oil production (Europe) due to the substitution effects caused by the Russian invasion of Ukraine on 24 February 2022 affected the prices. Given that Ukraine is the largest producer of global sunflower oil and Europe is the largest territory that produces olive oil, this scientific article tries to analyze the global prices of both vegetable oils and understand how the war between Russia and Ukraine has affected them. Advanced statistical and econometric methods to carry out this analysis have been used. It is found that the prices of both variables separately have similar behavior and that the shock caused by the war will be transitory, with the original price trend recovering in the long term using fractional integration methods. In a multivariate analysis, using a causality test in the frequency domain we observe that both variables are related to each other, and the effects of war will have an impact in the long term, with olive oil being the cause. A negative relationship between both variables measured with a wavelet analysis is also observed. Furthermore, if this trend continues, the price of olive oil would prevail over the price of sunflower in the war between Russia and Ukraine. Finally, a 12-month prediction is presented using artificial neural networks, where the price of olive oil will be high for at least 11 more months. The price of sunflower oil is predicted to last for only 5 more months.
Avaliação do risco de extinção do veado-campeiro Ozotoceros bezoarticus Linnaeus, 1758, no Brasil
Authors: Barbanti Duarte José Maurício , Vogliotti Alexandre , Dos Santos Zanetti Eveline , Leite de Oliveira Márcio , Tiepolo Liliani Marília , Figueiredo Rodrigues Lilian , Bonjorne de Almeida Lilian , Gass Braga Fernanda 
Published: August 2024

O estado de conservação no Brasil, das duas subespécies do veado-campeiro, Ozotoceros bezoarticus (Linnaeus, 1758), que ocorrem no país, foi avaliado de acordo com os critérios da IUCN (2001), com base nos dados disponíveis até 2010. Síntese do processo de avaliação pode ser encontrada em Peres et al. (2011) e em Beisiegel et al. (2012). A subespécie Ozotoceros bezoarticus leucogaster, que ocorre no Pantanal, foi considerada Vulnerável (VU), sob os critérios A3ce, ou seja, em função de provável redução populacional no futuro. A subespécie Ozotoceros bezoarticus bezoarticus, que ocorre no Cerrado, foi considerada Vulnerável (VU) sob os critérios A4cde, C1, ou seja, em função de redução populacional passada, bem como redução projetada para o futuro, além de possuir pequeno tamanho populacional. A mudança de status da espécie na presente avaliação deve-se tanto ao aumento de conhecimento sobre as ameaças distintas que colocam em risco as duas subespécies, gerando a necessidade de avaliações separadas para as duas, quanto Ã intensificação destas ameaças. A avaliação de cada subespécie e a justificativa de categorização são apresentadas separadamente para cada subespécie e as demais informações, conjuntamente.

Justificativa - Ozotoceros bezoarticus estava incluída na lista oficial de espécies ameaçadas da em 1989 e foi retirada da lista da em 2003 (MMA 2003) devido a um aumento do conhecimento sobre a espécie, que revelou novas populações. A mudança de status da espécie na presente avaliação deve-se tanto a novo aumento de conhecimento sobre as ameaças distintas que colocam em risco as duas subespécies, causando a necessidade de avaliações separadas para as duas, quanto Ã intensificação destas ameaças.
Avaliação do risco de extinção do veado-catingueiro Mazama gouazoubira G. Fischer [von Waldhein], 1814, no Brasil
Authors: Barbanti Duarte José Maurício , Vogliotti Alexandre , Dos Santos Zanetti Eveline , Leite de Oliveira Márcio , Tiepolo Liliani Marília , Figueiredo Rodrigues Lilian , Bonjorne de Almeida Lilian 
Published: August 2024

O estado de conservação do veado-catingueiro, Mazama gouazoubira (G. Fischer [von Waldheim], 1814) foi avaliado de acordo com os critérios da IUCN (2001), com base nos dados disponíveis até 2010. Síntese do processo de avaliação pode ser encontrada em Peres et al. (2011) e Beisiegel et al. (2012). A categoria proposta para o táxon é Menos preocupante (Least concern - LC), com base em informações sobre ecologia, distribuição geográfica, populações e ameaças. Justificativa - O veado-catingueiro é uma espécie de pequeno porte, que ocorre em todo o Brasil, apesar de estudos recentes indicarem sua substituição por Mazama nemorivaga na região amazônica. Trata-se de uma espécie com extrema plasticidade ecológica, adaptando-se a ambientes modificados. Estima-se que as populações estejam em equilíbrio ou crescimento devido Ã capacidade de ocupar áreas antropizadas. A espécie apresenta tendência de ampliação de área de ocorrência e da área de ocupação e uma população total de indivíduos maduros maior que 10.000 indivíduos. Não existem evidências de emigração ou imigração diferencial de indivíduos desta espécie entre o Brasil e os países vizinhos, portanto a categoria da espécie não é alterada quando se aplica a avaliação regional. A classificação não mudou em relação Ã lista oficial anterior de fauna ameaçada (MMA 2003).
Avaliação do risco de extinção do jacaré-do-pantanal Caiman yacare (Daudin, 1802) no Brasil
Authors: Farias Izeni Pires , Marioni Boris , Verdade Luciano M. , Bassetti Luís , Coutinho Marcos E. , Mendonça Sônia H. S. T. de , Vieira Tiago , Magnusson William E. , Campos Zilca 
Published: August 2024

O risco de extinção de Caiman yacare foi avaliado de acordo com os critérios da União Internacional para a Conservação da Natureza (IUCN 2001, 2003), com base nos dados disponíveis até 2011. A espécie é encontrada nas regiões alagadas do nordeste e leste da Bolívia, no Pantanal brasileiro e afluentes do rio Madeira, no Paraguai e no nordeste da Argentina. Sua extensão de ocorrência (EOO) em território brasileiro é de 195.160,3 km2, podendo ser bem maior, caso as investigações sobre o status taxonômico da espécie confirmarem a sua distribuição nas bacias dos rios Madeira, Mamoré e Guaporé. Acredita-se que sua área de ocupação (AOO) seja maior que 20.000 km2. Os levantamentos populacionais confirmam que, no Pantanal brasileiro, Caiman yacare apresenta uma das mais vigorosas populações naturais de crocodilianos no mundo, com densidades superiores a 100 ind/km2, distribuídos por toda planície Pantaneira. O tamanho populacional em toda essa região está na ordem dos milhões de indivíduos. Aparentemente, Caiman yacare e C. crocodilus apresentam maior resiliência Ã s alterações ambientais e Ã caça do que as demais espécies de crocodilianos brasileiros e ocorre em várias Unidades de Conservação. Portanto, a espécie foi categorizada como Menos Preocupante (LC). Há conectividade com populações dos países vizinhos, porém não se sabe se há trocas significativas e, tendo em vista a grande distribuição da espécie no território brasileiro, o estado de conservação nos países vizinhos não altera a classificação da avaliação no Brasil. Embora a caça ilegal no Pantanal para o comércio de peles tenha sido reduzido, o comércio para carne tem sido documentado, o que representa um aspecto preocupante para a conservação da espécie aliado a outras ameaças no seu ambiente.
TEKNIK TIME TOKEN: ALTERNATIF MENINGKATKAN KEMAMPUAN SISWA DALAM MENYAMPAIKAN PENDAPAT
Authors: Romiaty  , Bryan Tiovanno Richard 
Published: August 2024

Penelitian ini bertujuan untuk mengetahui penerapan teknik Time Token dalam meningkatkan kemampuan menyampaikan pendapat pada siswa. Ruang lingkup penelitian hanya pada siswa kelas VIII SMP Kristen Palangka Raya yang berjumlah 10 siswa. Metodologi penelitian yang digunakan dalam penelitian ini adalah Pre-Eksperimental dengan jenis penelitian one group pretest-posttest design. Alat pengumpul data utama adalah kuesioner, dan alat pengumpul data pendukung berupa observasi, wawancara dan dokumentasi. Kuesioner disusun berdasarkan indikator yaitu kemampuan dalam bertanya, menjawab pertanyaan, menyampaikan pendapat, dan menjelaskan ide. Uji analisis data penelitian menggunakan Uji paired T-test untuk melihat peningkatan kemampuan menyampaikan pendapat pada siswa sebelum dan sesudah diberikan perlakuan berupa teknik Time Token. Berdasarkan hasil pretest dan post test terdapat peningkatan pada setiap indikator. Indikator kemampuan dalam bertanya terdapat peningkatan sebanyak 57, indikator Kemampuan dalam menjawab pertanyaan mengalami peningkatan sebanyak 41, indikator Kemampuan dalam menyampaikan pendapat mengalami peningkatan sebanyak 48, dan indikator Kemampuan dalam menjelaskan ide mengalami peningkatan sebanyak 55. Hasil yang didapat bahwa tingkat signifikansi adalah 0,05, sehingga kriteria keputusannya adalah jika t_(hitung)> t_(tabel), maka Ha diterima dan Ho ditolak. Hasil uji t menunjukkan bahwa t_(hitung)= 13.622, sementara t dari 10 sampel dengan tingkat signifikansi 0,05 = t_(tabel) (2,262). Dengan demikian, t_(hitung)> t_(tabel). Hal ini menunjukkan bahwa Ha diterima yaitu teknik Time Token dapat meningkatkan kemampuan siswa dalam menyampaikan pendapat
Interactions between latent variables in count regression models
Authors: Kiefer Christoph , Wilker Sarah , Mayer Axel 
Published: August 2024

AbstractIn psychology and the social sciences, researchers often model count outcome variables accounting for latent predictors and their interactions. Even though neglecting measurement error in such count regression models (e.g., Poisson or negative binomial regression) can have unfavorable consequences like attenuation bias, such analyses are often carried out in the generalized linear model (GLM) framework using fallible covariates such as sum scores. An alternative is count regression models based on structural equation modeling, which allow to specify latent covariates and thereby account for measurement error. However, the issue of how and when to include interactions between latent covariates or between latent and manifest covariates is rarely discussed for count regression models. In this paper, we present a latent variable count regression model (LV-CRM) allowing for latent covariates as well as interactions among both latent and manifest covariates. We conducted three simulation studies, investigating the estimation accuracy of the LV-CRM and comparing it to GLM-based count regression models. Interestingly, we found that even in scenarios with high reliabilities, the regression coefficients from a GLM-based model can be severely biased. In contrast, even for moderate sample sizes, the LV-CRM provided virtually unbiased regression coefficients. Additionally, statistical inferences yielded mixed results for the GLM-based models (i.e., low coverage rates, but acceptable empirical detection rates), but were generally acceptable using the LV-CRM. We provide an applied example from clinical psychology illustrating how the LV-CRM framework can be used to model count regressions with latent interactions.
Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z = 4–8 from CEERS
Authors: Chworowsky Katherine , Finkelstein Steven L. , Boylan-Kolchin Michael , McGrath Elizabeth J. , Iyer Kartheik G. , Papovich Casey , Dickinson Mark , Taylor Anthony J. , Yung L. Y. Aaron , Arrabal Haro Pablo , Bagley Micaela B. , Backhaus Bren E. , Bhatawdekar Rachana , Cheng Yingjie , Cleri Nikko J. , Cole Justin W. , Cooper M. C. , Costantin Luca , Dekel Avishai , Franco Maximilien , Fujimoto Seiji , Hayward Christopher C. , Holwerda Benne W. , Huertas-Company Marc , Hirschmann Michaela , Hutchison Taylor A. , Koekemoer Anton M. , Larson Rebecca L. , Li Zhaozhou , Long Arianna S. , Lucas Ray A. , Pirzkal Nor , Rodighiero Giulia , Somerville Rachel S. , Vanderhoof Brittany N. , de la Vega Alexander , Wilkins Stephen M. , Yang Guang , Zavala Jorge A. 
Published: August 2024

Abstract
We analyze the evolution of massive (log10[M
⋆/M
⊙] > 10) galaxies at z ∼ 1–4 selected from JWST Cosmic Evolution Early Release Survey (CEERS). We infer the physical properties of all galaxies in the CEERS NIRCam imaging through spectral energy distribution (SED) fitting with dense basis to select a sample of high-redshift massive galaxies. Where available we include constraints from additional CEERS observing modes, including 18 sources with MIRI photometric coverage, and 28 sources with spectroscopic confirmations from NIRSpec or NIRCam WFSS. We sample the recovered posteriors in stellar mass from SED fitting to infer the volume densities of massive galaxies across cosmic time, taking into consideration the potential for sample contamination by active galactic nuclei. We find that the evolving abundance of massive galaxies tracks expectations based on a constant baryon conversion efficiency in dark matter halos for z ∼ 1–4. At higher redshifts, we observe an excess abundance of massive galaxies relative to this simple model, resulting in a shallower decline of observed volume densities of massive galaxies. These higher abundances can be explained by modest changes to star formation physics and/or the efficiencies with which star formation occurs in massive dark matter halos, and are not in tension with modern cosmology.
Formation of Galactic Disks. II. The Physical Drivers of Disk Spin-up
Authors: Semenov Vadim A. , Conroy Charlie , Chandra Vedant , Hernquist Lars , Nelson Dylan 
Published: August 2024

Abstract
Using a representative sample of Milky Way (MW)–like galaxies from the TNG50 cosmological simulation, we investigate physical processes driving the formation of galactic disks. A disk forms as a result of the interplay between inflow and outflow carrying angular momentum in and out of the galaxy. Interestingly, the inflow and outflow have remarkably similar distributions of angular momentum, suggesting an exchange of angular momentum and/or outflow recycling, leading to continuous feeding of prealigned material from the corotating circumgalactic medium. We show that the disk formation in TNG50 is correlated with stellar bulge formation, in qualitative agreement with a recent theoretical model of disk formation facilitated by steep gravitational potentials. Disk formation is also correlated with the formation of a hot circumgalactic halo with around half of the inflow occurring at subsonic and transonic velocities corresponding to Mach numbers of ≲2. In the context of recent theoretical works connecting disk settling and hot halo formation, our results imply that the subsonic part of the inflow may settle into a disk while the remaining supersonic inflow will perturb this disk via the chaotic cold accretion. We find that disks tend to form when the host halos become more massive than ∼(1–2) × 1011
M
⊙, consistent with previous theoretical findings and observational estimates of the predisk protogalaxy remnant in the MW. Our results do not prove that either corotating outflow recycling, gravitational potential steepening, or hot halo formation cause disk formation, but they show that all these processes occur concurrently and may play an important role in disk growth.
Apparently Ultralong Period Radio Signals from Self-lensed Pulsar–Black Hole Binaries
Authors: Xiao 肖 Xinxu 欣旭 , Shen 申 Rong-Feng 荣锋 
Published: August 2024

Abstract
Pulsar–black hole (BH) close binary systems, which have not been found yet, are unique laboratories for testing theories of gravity and understanding the formation channels of gravitational-wave sources. We study the self-gravitational lensing effect in a pulsar–BH system on the pulsar’s emission. Because this effect occurs once per orbital period for almost edge-on binaries, we find that it could generate apparently ultralong period (minutes to hours) radio signals when the intrinsic pulsar signal is too weak to detect. Each of such lensed signals, or “pulse,” is composed of a number of amplified intrinsic pulsar pulses. We estimate that a radio telescope with a sensitivity of 10 mJy could detect a few systems that emit such signals in our Galaxy. The model is applied to three recently found puzzling long-period radio sources: GLEAM-X J1627, PSR J0901-4046, and GPM J1839-10. To explain their observed signal durations and periods, the masses of their lensing components are estimated as ∼104
M
⊙, ∼4 M
⊙, and 103−6
M
⊙, respectively, with their binary coalescence times ranging from a few tens to thousands of years. However, the implied merger rates (as high as ∼103−4 Myr−1 per galaxy) and the large period decay rates (>10−8 s s−1) tend to disfavor this self-lensing scenario for these three sources. Despite this, our work still provides observational characteristics for self-lensed pulsar–BH binaries, which could help the detection of related sources in the future. Finally, for a binary containing a millisecond pulsar and a stellar-mass BH, the Shapiro delay effect would cause a ≥10% variation of the profile width for the subpulses in such lensed signals.
On the (Higher Multipoles) Variance Asymmetry in the Cosmic Microwave Background
Authors: Jamshidi MohammadHossein , Banihashemi Abdolali , Khosravi Nima 
Published: August 2024

Abstract
We have studied the cosmic microwave background (CMB) map looking for features beyond cosmological isotropy. We began by tiling the CMB variance maps (which are produced by different smoothing scales) with stripes of different sizes along the most prominent dipole direction. We were able to confirm previous findings regarding the significance of the dipole. Furthermore, we discovered that some of the higher multipoles exhibit significance comparable to the dipole that naturally depends on the smoothing scales. In the end, we discussed this result having an eye on the look-elsewhere-effect. We believe our results may indicate an anomalous patch in the CMB sky that warrants further investigation.
Ancient Nova Shells of RX Pup Indicate Evolution of Mass Transfer Rate
Authors: Iłkiewicz Krystian , Mikołajewska Joanna , Shara Michael M. , Faherty Jacqueline K. , Scaringi Simone 
Published: August 2024

Abstract
RX Pup is a symbiotic binary that experienced a nova outburst in the 1970s. Here we report a discovery of a ∼1300 yr old nova shell around the system and a possible detection of a ∼7000 yr old nova shell. Together with the nova shell ejected in the 1970s, this makes RX Pup the first system with three nova shells observed. This triad of eruptions suggests a change in the nova recurrence time. The most likely explanation is an alteration in the mass transfer rate attributed to evolutionary changes of the mass donor in the system. Notably, comparative analyses with theoretical models indicate an increase in the average mass transfer rate by a factor of 3 over the past 10,000 yr. This makes RX Pup a unique system, which allows us to probe millennium-scale evolution of mass transfer rates in binary systems.
Mild Primary or Breakthrough SARS-CoV-2 Infection Promotes Autoantibody Production in Individuals with and without Neuro-PASC
Authors: Visvabharathy Lavanya , Dalil Neda , Leonor Lucia , Zhu Chengsong , Orban Zachary S , Jimenez Millenia , Lim Patrick H , Penaloza-MacMaster Pablo , Koralnik Igor J 
Published: August 2024

Abstract
Patients with long COVID can develop humoral autoimmunity after severe acute SARS-CoV-2 infection. However, whether similar increases in autoantibody responses occur after mild infection and whether vaccination prior to SARS-CoV-2 breakthrough infection can limit autoantibody responses is unknown. In this study, we demonstrate that mild SARS-CoV-2 infection increases autoantibodies associated with rheumatic autoimmune diseases and diabetes in most individuals, regardless of vaccination status prior to infection. However, patients with long COVID and persistent neurologic and fatigue symptoms (neuro-PASC) have substantially higher autoantibody responses than convalescent control subjects at an average of 8 mo postinfection. Furthermore, high titers of systemic lupus erythematosus– and CNS-associated autoantibodies in patients with neuro-PASC are associated with impaired cognitive performance and greater symptom severity. In summary, we found that mild SARS-CoV-2 primary and breakthrough infections can induce persistent humoral autoimmunity in both patients with neuro-PASC and healthy COVID convalescents, suggesting that a reappraisal of mitigation strategies against SARS-CoV-2 is warranted to prevent transmission and potential development of autoimmunity.