14,030 results on '"E, Da"'
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2. Effectiveness of TAF in Reducing Clinical Events in CHB Patients Beyond Treatment Indications by Current Guidelines (ATTENTION)
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Samsung Medical Center, Kyunghee University Medical Center, Chung-Ang University Hosptial, Chung-Ang University College of Medicine, Seoul National University Hospital, Ulsan University Hospital, Konkuk University Medical Center, Kyungpook National University Hospital, Korea University Guro Hospital, Seoul St. Mary's Hospital, Kaohsiung Medical University, Chang Gung Memorial Hospital, E-DA Hospital, Taitung Mackay Memorial Hospital, National Cheng-Kung University Hospital, Chi Mei Medical Hospital, Chiayi Christian Hospital, St. Martin De Porress Hospital, Dalin Tzu Chi General Hospital, Taichung Veterans General Hospital, China Medical University Hospital, Seoul National University Bundang Hospital, and Young-Suk Lim, Professor
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- 2024
3. Short Course Regimen in Low Risk Active Tuberculosis- a Multicenter, Randomized, Active-controlled, Trial
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Taipei Veterans General Hospital, Taiwan, National Taiwan University Hospital, Chang Gung Memorial Hospital, Far Eastern Memorial Hospital, E-DA Hospital, Kaohsiung Medical University, and Susan Shin-Jung Lee, Attending physician
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- 2024
4. Statin for Preventing Hepatocellular Carcinoma Recurrence After Curative Treatment (SHOT)
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E-DA Hospital, National Taiwan University Hospital, Taichung Veterans General Hospital, Mackay Memorial Hospital, Tainan Municipal Hospital, National Cheng-Kung University Hospital, and Chi Mei Medical Hospital
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- 2024
5. Water Exchange and CO2 Insufflation with Abdominal Compression Device to Reduce Manual Assistance
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E-Da Dachange Hospital, Kaohsiung, Taiwan and The Sepulveda Ambulatory Care Center, VAGLAHS, UCLA in the USA
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- 2024
6. Can Overall Adenoma Detection Rate Replace Screening Adenoma Detection Rate ? Multicenter Study
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E-DA Hospital, E-Da Dachang Hospital, Chang Gung Memorial Hospital, and Sepulveda Ambulatory Care Center, Veterans Affairs Greater Los Angeles Healthcare System
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- 2024
7. Real-world Clinical Benefit Evaluation in Breast Cancer Patients With Pharmaceutical Interventions for Cancer-related Fatigue
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Taichung Veterans General Hospital, E-Da Cancer Hospital, Chang Gung Memorial Hospital, Taipei, Chang Gung Memorial Hospital, Tri-Service General Hospital, China Medical University Hospital, Kaohsiung Medical University Chung-Ho Memorial Hospital, Mackay Memorial Hospital, Chang Gung Memorial Hospital, Keelung, and Ming-Shen Dai, Chief of Department of Oncology
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- 2024
8. Taiwan Interstitial Lung Disease Multi-center Investigation and Registry (TAILI)
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Tri-Service General Hospital, E-DA Hospital, Chang Gung Memorial Hospital, and Pin-Kuei Fu, MD, PhD, Principal Investigator
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- 2024
9. Clinical Outcomes Of Mega-dosage Supplementations Of Cholecalciferol In Critically Ill Patients With Sepsis (MDC-S)
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E-DA Hospital and Chin-Ming Chen, M.D., Professor
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- 2024
10. Taiwan Severe Asthma Biologic Registry (TARGET)
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E-DA Hospital, National Cheng-Kung University Hospital, National Yang Ming Chiao Tung University Hospital, Chang Gung Memorial Hospital, and Pin-Kuei Fu, MD, PhD, Director of Clinical Trail Center
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- 2024
11. The DairyPrint model: A decision support model to help dairy farmers and other stakeholders toward improved sustainability
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Tadeu E. da Silva and Victor E. Cabrera
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decision support system ,greenhouse gases ,modeling ,simulation ,Dairy processing. Dairy products ,SF250.5-275 ,Dairying ,SF221-250 - Abstract
ABSTRACT: Dairy farmers face increasing pressure to reduce GHG emissions (i.e., carbon dioxide, CO2; methane, CH4; and nitrous oxide, N2O), but measuring on-farm GHG emissions directly is costly or impractical. Therefore, the dairy industry has relied upon mathematical models to estimate these emissions. However, current models tend to be not user-friendly, difficult to access, or sometimes very research-focused, limiting their practical use. To address this, we introduce the DairyPrint model, a user-friendly tool designed to estimate GHG emissions from dairy farming. The model integrates herd dynamics, manure management, crop, and feed costs considerations, simplifying the estimation process while providing comprehensive insights. The herd module simulates monthly herd dynamics based on inputs as total cows, calving interval, and culling rate, outputting average annual demographics and estimating various animal-related variables (i.e., DMI, milk yield, manure excretion, and enteric CH4 emissions). These outputs feed into other modules, such as the manure module, which calculates emissions based on manure, weather data, and facility type. The manure module processes manure according to farm practices, and the crop module accounts for GHG emissions from manure, fertilizers, and limestone application, also estimating nutrient balances. The DairyPrint model was developed using the Shiny framework and the Golem package for robust production-grade Shiny applications in the R programming language. We evaluated the model across 32 simulation scenarios by combining various factors and considering a standard freestall system with 1,000 dairy cows averaging 40 kg/d of milk production. These factors included 2 NDF-ADF levels in the diet (28%–22.8% and 24%–19.5%), the presence or absence of 3-nitrooxypropanol (3-NOP) dietary addition (yes or no) at an average dose of 70 mg/kg DM per cow daily, the type of bedding used (sawdust or sand), the frequency of manure pond emptying (once yearly, only in fall; or twice a year, in fall and spring), and the use or nonuse of a biodigester plus solid-liquid separator (Biod + SL). In our results across the 32 scenarios simulated, the average GHG emission was 0.811 kg CO2 eq/kg of milk, corrected for fat and protein contents (4% and 3.3%, respectively), ranging from 0.644 to 1.082. Notably, the scenario yielding the lowest GHG emission (i.e., 0.644 kg CO2 eq/kg) involved a combination of factors, including a lower NDF-ADF level in the diet in addition to incorporation of 3-NOP, use of sand as bedding, application of Biod + SL, and strategic manure pond emptying in both fall and spring. Conversely, the scenario that resulted in the highest GHG emission (i.e., 1.082 kg CO2 eq/kg) involved a combination of a higher NDF-ADF level in the diet and excluded incorporation of 3-NOP, use of sawdust as bedding, no application of Biod + SL, and manure pond emptying only in fall. All these scenarios can easily be simulated in the DairyPrint model, with results obtained immediately for user evaluation. Therefore, the DairyPrint model can help farmers move toward improved sustainability, providing a user-friendly and intuitive graphical user interface allowing the user to ask what-if questions.
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- 2024
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12. Physiology and production of colored bell pepper cultivars in a semi-hydroponic system/Fisiologia e producao de cultivares de pimentao colorido em cultivo semi-hidroponico
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Leal, Marcia P. da S., Dias, Tiago J., Sousa, Valeria F. de O., da Silva, Toshik I., Ribeiro, Joao E. da S., Pereira, Walter E., Souza, Aline das G., Smiderle, Oscar J., and Alves, Edna U.
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- 2024
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13. Effects of Jing Si Herbal Tea on Quality of Life and Sleep in Dementia and Their Caregivers
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Buddhist Tzu Chi General Hospital, Tzu Chi University, E-DA Hospital, and Chung-Ying Lin, Associate Professor
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- 2024
14. Mapping the nonequilibrium order parameter of a quasi-two dimensional charge density wave system
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C. J. Sayers, Y. Zhang, C. E. Sanders, R. T. Chapman, A. S. Wyatt, G. Chatterjee, E. Springate, G. Cerullo, D. Wolverson, E. Da Como, and E. Carpene
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Astrophysics ,QB460-466 ,Physics ,QC1-999 - Abstract
Abstract The driving force of a charge density wave (CDW) transition in quasi-two dimensional systems is still debated, while being crucial in understanding electronic correlation in such materials. Here we use femtosecond time- and angle-resolved photoemission spectroscopy combined with computational methods to investigate the coherent lattice dynamics of a prototypical CDW system. The photo-induced temporal evolution of the periodic lattice distortion associated with the amplitude mode reveals the dynamics of the free energy functional governing the order parameter. Our approach establishes that optically-induced screening rather than CDW melting at the electronic level leads to a transiently modified potential which explains the anharmonic behaviour of the amplitude mode and discloses the structural origin of the symmetry-breaking phase transition.
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- 2024
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15. Dry mass grassland estimation using UAV ultra-wide RGB images
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R. C. E. da Silva, A. M. G. Tommaselli, N. N. Imai, R. P. Martins-Neto, D. D. S. da Silveira, and E. Moro
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Technology ,Engineering (General). Civil engineering (General) ,TA1-2040 ,Applied optics. Photonics ,TA1501-1820 - Abstract
Dry mass is an important parameter to optimise grassland management. Traditionally, dry mass values are estimated manually by cutting, drying, and weighing vegetation samples. In large areas of cultivation, this becomes a time-consuming and costly activity. In recent years, many researchers have studied different sensors embedded in Unmanned Aerial Vehicles (UAV) to collect spatial data and estimate biomass using machine learning algorithms for forest and agricultural applications. However, there needs to be more research dealing with estimating production indices for pasture, especially in Brazil, as stated. This study evaluates the feasibility of using the GoPro wide-angle RGB camera on UAVs (Unmanned Aerial Vehicles) to estimate the dry mass of pastures. Different data analysis methods were compared, including the combination of vegetation indices (VIs) values and three-dimensional metrics (3D) extracted from the Canopy Height Model (CHM): all metrics (ALL), three VIs plus four 3D metrics (VI3 + CHM4) and only 3D metrics. Random Forest (RF) machine learning algorithm was used to estimate dry mass. The best results were obtained when merging all the variables from the two flight campaigns, with a coefficient of determination (R2) of 0.80 for the model and a Pearson Correlation Coefficient (PCC) of 0.85 for validation, with a Root Mean Square Error (RMSE%) of 20.5%. In summary, using RGB sensors embedded in UAVs is a promising technique for estimating farm grazing parameters.
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- 2024
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16. Whiteness and Damage in the Education Classroom
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Alexandre E. Da Costa
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This paper analyses relationships between whiteness and damage in the university classroom through a focus on two contemporary areas of critical education in Canada: raising white racial consciousness and truth and reconciliation between Indigenous and non-Indigenous people. First, whiteness is damage-producing -- it orients anti-racist education towards white students and their needs, there by harming the well-being and constraining the education of non-white students. Second, whiteness gravitates towards what Unangax scholar Eve Tuck calls "damage-centred approaches," which objectify non-white suffering, pathologising Indigenous peoples whilst obfuscating the ongoing reproduction of racism and colonialism. As such, white educators must remain assiduously vigilant about a key tension regarding whiteness and damage: that our pedagogical focus on racial and colonial oppression can simultaneously raise critical consciousness and divert attention away from more fundamental interrogations of whiteness, agency, and relationality within a systemically racist social order. The article closes with some considerations for educators in terms of addressing complicity in their institutions.
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- 2024
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17. DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys
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Survey, Dark Energy, Collaboration, Kilo-Degree Survey, Abbott, T. M. C., Aguena, M., Alarcon, A., Alves, O., Amon, A., Andrade-Oliveira, F., Asgari, M., Avila, S., Bacon, D., Bechtol, K., Becker, M. R., Bernstein, G. M., Bertin, E., Bilicki, M., Blazek, J., Bocquet, S., Brooks, D., Burger, P., Burke, D. L., Camacho, H., Campos, A., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Cawthon, R., Chang, C., Chen, R., Choi, A., Conselice, C., Cordero, J., Crocce, M., da Costa, L. N., Pereira, M. E. da Silva, Dalal, R., Davis, C., de Jong, J. T. A., DeRose, J., Desai, S., Diehl, H. T., Dodelson, S., Doel, P., Doux, C., Drlica-Wagner, A., Dvornik, A., Eckert, K., Eifler, T. F., Elvin-Poole, J., Everett, S., Fang, X., Ferrero, I., Ferté, A., Flaugher, B., Friedrich, O., Frieman, J., García-Bellido, J., Gatti, M., Giannini, G., Giblin, B., Gruen, D., Gruendl, R. A., Gutierrez, G., Harrison, I., Hartley, W. G., Herner, K., Heymans, C., Hildebrandt, H., Hinton, S. R., Hoekstra, H., Hollowood, D. L., Honscheid, K., Huang, H., Huff, E. M., Huterer, D., James, D. J., Jarvis, M., Jeffrey, N., Jeltema, T., Joachimi, B., Joudaki, S., Kannawadi, A., Krause, E., Kuehn, K., Kuijken, K., Kuropatkin, N., Lahav, O., Leget, P. -F., Lemos, P., Li, S. -S., Li, X., Liddle, A. R., Lima, M., Lin, C. -A, Lin, H., MacCrann, N., Mahony, C., Marshall, J. L., McCullough, J., Mena-Fernández, J., Menanteau, F., Miquel, R., Mohr, J. J., Muir, J., Myles, J., Napolitano, N., Navarro-Alsina, A., Ogando, R. L. C., Palmese, A., Pandey, S., Park, Y., Paterno, M., Peacock, J. A., Petravick, D., Pieres, A., Malagón, A. A. Plazas, Porredon, A., Prat, J., Radovich, M., Raveri, M., Reischke, R., Robertson, N. C., Rollins, R. P., Romer, A. K., Roodman, A., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Sanchez, J., Schneider, P., Secco, L. F., Sevilla-Noarbe, I., Shan, H. -Y., Sheldon, E., Shin, T., Sifón, C., Smith, M., Soares-Santos, M., Stölzner, B., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Troxel, M. A., Tröster, T., Tutusaus, I., Busch, J. L. van den, Varga, T. N., Walker, A. R., Weaverdyck, N., Wechsler, R. H., Weller, J., Wiseman, P., Wright, A. H., Yanny, B., Yin, B., Yoon, M., Zhang, Y., and Zuntz, J.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present a joint cosmic shear analysis of the Dark Energy Survey (DES Y3) and the Kilo-Degree Survey (KiDS-1000) in a collaborative effort between the two survey teams. We find consistent cosmological parameter constraints between DES Y3 and KiDS-1000 which, when combined in a joint-survey analysis, constrain the parameter $S_8 = \sigma_8 \sqrt{\Omega_{\rm m}/0.3}$ with a mean value of $0.790^{+0.018}_{-0.014}$. The mean marginal is lower than the maximum a posteriori estimate, $S_8=0.801$, owing to skewness in the marginal distribution and projection effects in the multi-dimensional parameter space. Our results are consistent with $S_8$ constraints from observations of the cosmic microwave background by Planck, with agreement at the $1.7\sigma$ level. We use a Hybrid analysis pipeline, defined from a mock survey study quantifying the impact of the different analysis choices originally adopted by each survey team. We review intrinsic alignment models, baryon feedback mitigation strategies, priors, samplers and models of the non-linear matter power spectrum., Comment: 40 pages, 21 figures, 15 tables, accepted Open Journal of Astrophysics. Download the chains from https://des.ncsa.illinois.edu/releases/y3a2/Y3key-joint-des-kids or create your own chains with CosmoSIS using https://github.com/joezuntz/cosmosis-standard-library/blob/main/examples/des-y3_and_kids-1000.ini Watch the core team discuss this analysis at https://cosmologytalks.com/2023/05/26/des-kids
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- 2023
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18. Electronic and valleytronic properties of crystalline boron-arsenide tuned by strain and disorder
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Craco, L., Carara, S. S., Barboza, E. da Silva, Pereira, T. A. S., and Milosevic, M. V.
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Condensed Matter - Materials Science ,Condensed Matter - Other Condensed Matter - Abstract
Ab initio density functional theory (DFT) and DFT plus coherent potential approximation (DFT+CPA) are employed to reveal, respectively, the effect of in-plane strain and site-diagonal disorder on the electronic structure of cubic boron arsenide (BAs). It is demonstrated that tensile strain and static diagonal disorder both reduce the semiconducting one-particle band gap of BAs, and a V-shaped p-band electronic state emerges -- enabling advanced valleytronics based on strained and disordered semiconducting bulk crystals. At biaxial tensile strains close to 15% the valence band lineshape relevant for optoelectronics is shown to coincide with one reported for GaAs at low energies. The role played by static disorder on the As sites is to promote p-type conductivity in the unstrained BAs bulk crystal, consistent with experimental observations. These findings illuminate the intricate and interdependent changes in crystal structure and lattice disorder on the electronic degrees of freedom of semiconductors and semimetals., Comment: 7 pages, 6 figures; regular paper
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- 2022
19. Pro-neuroinflammatory and neurotoxic potential of extracellular histones H1 and H3
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Seamus A. McRae, Christy M. Richards, Dylan E. Da Silva, Ishvin Riar, Sijie (Shirley) Yang, Noah E. Zurfluh, Julien Gibon, and Andis Klegeris
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Cytokines ,DAMPs ,Microglia ,Neurodegenerative diseases ,Neuroinflammation ,Neurotoxicity ,Neurosciences. Biological psychiatry. Neuropsychiatry ,RC321-571 - Abstract
Histones organize DNA within cellular nuclei, but they can be released from damaged cells. In peripheral tissues extracellular histones act as damage-associated molecular patterns (DAMPs) inducing pro-inflammatory activation of immune cells. Limited studies have considered DAMP-like activity of histones in the central nervous system (CNS); therefore, we studied the effects of extracellular histones on microglia, the CNS immunocytes, and on neuronal cells. Both the linker histone H1 and the core histone H3 induced pro-inflammatory activation of microglia-like cells by upregulating their secretion of NO and cytokines, including interferon-γ-inducible protein 10 (IP-10) and tumor necrosis factor-α (TNF). The selective inhibitors MMG-11 and TAK-242 were used to demonstrate involvement of toll-like receptors (TLR) 2 and 4, respectively, in H1-induced NO secretion by BV-2 microglia. H1, but not H3, downregulated the phagocytic activity of BV-2 microglia. H1 was also directly toxic to all neuronal cell types studied. We conclude that H1, and to a lesser extent H3, when released extracellularly, have the potential to act as a CNS DAMPs. Inhibition of the DAMP-like effects of extracellular histones on microglia and their neurotoxic activity represents a potential strategy for combating neurodegenerative diseases that are characterized by the adverse activation of microglia and neuronal death.
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- 2024
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20. INFANT HEALTH- Promoting Mental Health and Healthy Weight in Infancy Through Sensitive Parenting
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Danish Council for Independent Research, The Novo Nordic Foundation, University of Glasgow, and ISPA - Instituto Universitario de Ciencias Psicologicas, Sociais e da Vida
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- 2023
21. Chemical quality and bioactive compounds of sweet potatoes under phosphate fertilization /Qualidade quimica e compostos bioativos de batata-doce sob adubacao fosfatada
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Oliveira, Pablo H. de A., de Oliveira, Anna K.S., Coelho, Ester dos S., e Silva, Valecia N.S., Lopes, Welder de A.R., dos Santos, Gisele L., Ribeiro, Joao E. da S., da Silva, Antonio G.C., dos Santos, Jose T., Jr., Barros, Aurelio P., Jr., and da Silveira, Lindomar M.
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- 2024
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22. Effects of supplementation frequency on nutritional performance and metabolism of cattle fed low-quality tropical forage
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Silva, Tadeu E. da, de Oliveira, Cristhiane V.R., Rodrigues, Aline N., Palma, Málber N.N., Camacho, Larissa F., Rennó, Luciana N., Franco, Marcia O., and Detmann, Edenio
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- 2024
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23. Morphophysiology and gas exchange of pomegranate under salt stress and foliar application of nitrogen/Morfofisiologia e trocas gasosas da romãzeira sob estresse salino e aplicação foliar de nitrogênio
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Figueiredo, Francisco R.A., de Fátima, Reynaldo T., Nvbrega, Jackson S., da Silva, Toshik I., Ferreira, Jean T.A., Ribeiro, João E. Da S., Leal, Márcia P. Da S., Soares, Lauriane A. Dos A., and Dias, Hiago J.
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- 2023
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24. Comparison of behavior, thermoregulation, and growth of pair-housed versus individually housed calves in outdoor hutches during continental wintertime
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Kimberly J. Reuscher, Rekia S. Salter, Tadeu E. da Silva, and Jennifer M.C. Van Os
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social housing ,thermal comfort ,cold stress ,Dairy processing. Dairy products ,SF250.5-275 ,Dairying ,SF221-250 - Abstract
ABSTRACT: Cold stress negatively affects the welfare of calves in outdoor hutches. No studies have examined the potential benefits of pair housing calves to buffer against cold stress. Our study evaluated the effects of pair versus individual housing on thermoregulatory, behavioral, and growth performance responses of calves in outdoor hutches during a Wisconsin continental winter. Forty-eight Holstein-Friesian heifer calves were enrolled into 1 of 2 housing treatments: individually (n = 16 calves) or pair housed (n = 16 pairs; 32 calves). Calves were fed milk twice daily, with ad libitum access to starter and water. Step-down weaning began on d 42 of life, and all milk was removed on d 54. Data collection continued through d 59. Calves were restricted inside a hutch (pair-housed calves in the same hutch) for 1 h during wk 4, 6, and 9 of life; internal hutch air temperature (T) was recorded with data loggers, and rectal temperature (RT) was recorded outside the hutch before and after restriction. On the subsequent 3 d in those weeks, calves' locations (outside or inside a hutch) were recorded at 15-min intervals using time-lapse cameras. Linear mixed models (change in T and RT after 1 h) and generalized linear mixed models with a β distribution (proportion of time spent inside hutches) were used to evaluate the fixed effects of housing treatment, week of life, and their interaction. For pair-housed calves, preference to be together was evaluated using one-sample t-tests comparing the proportion of time they were observed in the same location against 50% (chance, no preference), separately for each week of life. Predicted dry matter intake (DMI) of starter and body weight (BW) were standardized by day of life using regression models and used to calculate average daily gain (ADG) and feed conversion ratio (FCR; DMI of starter/ADG). Linear mixed models were constructed for each measure, separately for the preweaning, weaning, and postweaning periods, with a fixed effect of housing treatment; the models for BW included birth weight as a covariate. All mixed models included a random term for housing unit (individual or pair of calves) nested within treatment. Hutch T increased more after 1 h with pair-housed calves inside than with those housed individually (+2.3 vs. 1.4°C, respectively; standard error of the mean = 0.26°C). However, no treatment differences were detected in RT. Individually housed calves spent more time inside the hutches than pair-housed ones (93.9 vs. 90.7% of total time, respectively; standard error of the mean = 0.8%), and the latter chose to be together most of the time, regardless of location (90.0 ± 1.3%, 88.6 ± 1.2%, and 79.4 ± 4.2% in wk 4, 6, and 9 of life, respectively). After weaning, there was some evidence suggesting that pair-housed calves had greater starter DMI than those housed individually. No effects of housing type were found on FCR, BW, or ADG. Our study is the first to explicitly examine the potential benefits of pair housing for alleviating cold stress in outdoor-housed dairy calves, and we found limited evidence in support of our hypotheses.
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- 2024
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25. Micro-Scale Abrasive Wear Resistance of a Nanoceramic Sealant Applied on Galvanized Low Carbon Steel
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Anael P. Krelling, Jefferson L. Jeronimo, Ivandro Bonetti, Gabriela Rabethge, Heitor F. Pensky, Raíssa R.S. Bibow, Bruna F. Zappelino, Julio C.G. Milan, and Cesar E. da Costa
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surface engineering ,adhesion ,abrasive wear ,tribology ,corrosion ,Mechanical engineering and machinery ,TJ1-1570 - Abstract
The idea for this work came from a market need to obtain coatings or sealants that would extend the useful life of metallic materials in applications that involve exposure to corrosive environments. The main objective of the nanoceramic sealant studied in this work is to extend the life of metallic fasteners. To evaluate the performance of the sealant from other perspectives, microstructural analysis, adhesion test, micro-scale abrasive wear tests and corrosion test were carried out. These tests were performed on samples coated only with white zinc, which is commonly used in the fastener industry, and on samples coated with white zinc followed by application of the nanoceramic sealant. The application of the nanoceramic sealant contributed to the improvement of corrosion resistance and reduction of the corrosion rate. The corrosion rate of the sample coated with the sealant reduced by 62.2% when compared to the sample that only went through the white zinc coating process. The coating showed low adhesion to the substrate with the presence of severe delamination and microcracks. This feature contributed to the low wear resistance presented by the coating under the conditions studied in this work. Less attention, compared to studies involving corrosion resistance, has been given to wear resistance in the fastener industry. The results obtained in this paper show that the study of tribological behavior is an important factor in increasing the efficiency of fasteners applied in harsh environments.
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- 2024
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26. ALESS-JWST: Joint (Sub)kiloparsec JWST and ALMA Imaging of z ~ 3 Submillimeter Galaxies Reveals Heavily Obscured Bulge Formation Events
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J. A. Hodge, E. da Cunha, S. Kendrew, J. Li, I. Smail, B. A. Westoby, O. Nayak, A. M. Swinbank, C.-C. Chen, F. Walter, P. van der Werf, M. Cracraft, A. Battisti, W. N. Brandt, G. Calistro Rivera, S. C. Chapman, P. Cox, H. Dannerbauer, R. Decarli, M. Frias Castillo, T. R. Greve, K. K. Knudsen, S. Leslie, K. M. Menten, M. Rybak, E. Schinnerer, J. L. Wardlow, and A. Weiss
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High-redshift galaxies ,Astrophysics ,QB460-466 - Abstract
We present JWST NIRCam imaging targeting 13 z ~ 3 infrared-luminous ( L _IR ∼ 5 × 10 ^12 L _⊙ ) galaxies from the ALESS survey with uniquely deep, high-resolution (0 $\mathop{.}\limits^{\unicode{x02033}}$ 08–0 $\mathop{.}\limits^{^{\prime\prime} }$ 16) Atacama Large Millimeter/submillimeter Array 870 μ m imaging. The 2.0–4.4 μ m (observed frame) NIRCam imaging reveals the rest-frame near-infrared stellar emission in these submillimeter-selected galaxies at the same (sub)kiloparsec resolution as the 870 μ m dust continuum. The newly revealed stellar morphologies show striking similarities with the dust continuum morphologies at 870 μ m, with the centers and position angles agreeing for most sources, clearly illustrating that the spatial offsets reported previously between the 870 μ m and Hubble Space Telescope morphologies were due to strong differential dust obscuration. The F444W sizes are 78% ± 21% larger than those measured at 870 μ m, in contrast to recent results from hydrodynamical simulations that predict larger 870 μ m sizes. We report evidence for significant dust obscuration in F444W for the highest-redshift sources, emphasizing the importance of longer-wavelength MIRI imaging. The majority of the sources show evidence that they are undergoing mergers/interactions, including tidal tails/plumes—some of which are also detected at 870 μ m. We find a clear correlation between NIRCam colors and 870 μ m surface brightness on ∼1 kpc scales, indicating that the galaxies are primarily red due to dust—not stellar age—and we show that the dust structure on ∼kpc scales is broadly similar to that in nearby galaxies. Finally, we find no strong stellar bars in the rest-frame near-infrared, suggesting the extended bar-like features seen at 870 μ m are highly obscured and/or gas-dominated structures that are likely early precursors to significant bulge growth.
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- 2025
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27. Ent-Kaurane Diterpenoids from Coffea Genus: An Update of Chemical Diversity and Biological Aspects
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Víctor de C. Martins, Maria Alice E. da Silva, Valdir F. da Veiga, Henrique M. G. Pereira, and Claudia M. de Rezende
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coffea ,green and roasted coffee ,ent-kaurane ,new compounds ,antidiabetic potential ,Organic chemistry ,QD241-441 - Abstract
Coffee is one of the most important beverages in the world and is produced from Coffea spp. beans. Diterpenes with ent-kaurane backbones have been described in this genus, and substances such as cafestol and kahweol have been widely investigated, along with their derivatives and biological properties. Other coffee ent-kaurane diterpenoids have been reported with new perspectives on their biological activities. The aim of this review is to update the chemical diversity of ent-kaurane diterpenoids in green and roasted coffee, detailing each new compound and reporting its biological potential. A systematic review was performed using the bibliographic databases (SciFinder, Web of Science, ScienceDirect) and specific keywords such as “coffea diterpenes”, “coffee diterpenes”, “coffee ent-kaurane diterpenes” and “coffee diterpenoids”. Only articles related to the isolation of coffee ent-kaurane compounds were considered. A total of 146 compounds were related to Coffea spp. since the first report in 1932. Different chemical skeletons were observed, and these compounds were grouped as furan-type, oxidation-type, rearrangement-type, lacton-type, and lactam-type, among others. In general, the new coffee diterpenoids showed potential as antidiabetic, antidiapogenic, α-glucosidade inhibition, antiplatelet activity, and Cav.3 inhibitors agents, revealing the possibilities for the design, discovery, and development of new drugs.
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- 2024
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28. Numerical Calculations of Adiabatic Invariants From MHD‐Driven Magnetic Fields
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D. E. da Silva, S. R. Elkington, X. Li, J. Murphy, M. K. Hudson, M. J. Wiltberger, and A. A. Chan
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- 2024
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29. Virtual Reality System Controlled by Embedded Artificial Intelligence for Supporting Phobia Treatment.
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Claudio Henrique Medaber Jambo, Vera Maria Benjamim Werneck, and Rosa Maria E. da M. da Costa
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- 2024
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30. PROGNOSE DA ESTRUTURA DIAMÉTRICA DE ESCHWEILERA GRANDIFLORA (AUBL.) SANDWITH, SOB O EFEITO DE EXPLORAÇÃO DE IMPACTO REDUZIDO, PARAGOMINAS, PARÁ
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NASCIMENTO, A. E. da S., primary, SIQUEIRA, C. O., additional, FRANCEZ, L. M. de B., additional, BATISTA, F. de, additional, and RUSCHEL, A. R., additional
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- 2024
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31. Catálogo Taxonômico da Fauna do Brasil: Setting the baseline knowledge on the animal diversity in Brazil
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Walter A. Boeger, Michel P. Valim, Hussam Zaher, José A. Rafael, Rafaela C. Forzza, Alexandre R. Percequillo, Cristiana S. Serejo, André R.S. Garraffoni, Adalberto J. Santos, Adam Slipinski, Adelita M. Linzmeier, Adolfo R. Calor, Adrian A. Garda, Adriano B. Kury, Agatha C.S. Fernandes, Aisur I. Agudo-Padrón, Alberto Akama, Alberto M. da Silva Neto, Alejandro L. Burbano, Aleksandra Menezes, Alessandre Pereira-Colavite, Alexander Anichtchenko, Alexander C. Lees, Alexandra M.R. Bezerra, Alexandre C. Domahovski, Alexandre D. Pimenta, Alexandre L.P. Aleixo, Alexandre P. Marceniuk, Alexandre S. de Paula, Alexandre Somavilla, Alexandre Specht, Alexssandro Camargo, Alfred F. Newton, Aline A.S. da Silva, Aline B. dos Santos, Aline D. Tassi, Allan C. Aragão, Allan P.M. Santos, Alvaro E. Migotto, Amanda C. Mendes, Amanda Cunha, Amazonas Chagas Júnior, Ana A.T. de Sousa, Ana C. Pavan, Ana C.S. Almeida, Ana L.B.G. Peronti, Ana L. Henriques-Oliveira, Ana L. Prudente, Ana L. Tourinho, Ana M.O. Pes, Ana P. Carmignotto, Ana P.G. da Silva Wengrat, Ana P.S. Dornellas, Anamaria Dal Molin, Anderson Puker, André C. Morandini, André da S. Ferreira, André L. Martins, André M. Esteves, André S. Fernandes, André S. Roza, Andreas Köhler, Andressa Paladini, Andrey J. de Andrade, Ângelo P. Pinto, Anna C. de A. Salles, Anne I. Gondim, Antonia C.Z. Amaral, Antonio A.A. Rondón, Antonio Brescovit, Antônio C. Lofego, Antonio C. Marques, Antonio Macedo, Artur Andriolo, Augusto L. Henriques, Augusto L. Ferreira Júnior, Aurino F. de Lima, Ávyla R. de A. Barros, Ayrton do R. Brito, Bárbara L.V. Romera, Beatriz M.C. de Vasconcelos, Benjamin W. Frable, Bernardo F. Santos, Bernardo R. Ferraz, Brunno B. Rosa, Brunno H.L. Sampaio, Bruno C. Bellini, Bruno Clarkson, Bruno G. de Oliveira, Caio C.D. Corrêa, Caleb C. Martins, Camila F. de Castro-Guedes, Camilla Souto, Carla de L. Bicho, Carlo M. Cunha, Carlos A. de M. Barboza, Carlos A.S. de Lucena, Carlos Barreto, Carlos D.C.M. de Santana, Carlos E.Q. Agne, Carlos G.C. Mielke, Carlos H.S. Caetano, Carlos H.W. Flechtmann, Carlos J.E. Lamas, Carlos Rocha, Carolina S. Mascarenhas, Cecilia B. Margaría, Cecilia Waichert, Celina Digiani, Célio F.B. Haddad, Celso O. Azevedo, Cesar J. Benetti, Charles M.D. dos Santos, Charles R. Bartlett, Cibele Bonvicino, Cibele S. Ribeiro-Costa, Cinthya S.G. Santos, Cíntia E.L. Justino, Clarissa Canedo, Claudia C. Bonecker, Cláudia P. Santos, Claudio J.B. de Carvalho, Clayton C. Gonçalves, Cleber Galvão, Cleide Costa, Cléo D.C. de Oliveira, Cristiano F. Schwertner, Cristiano L. Andrade, Cristiano M. Pereira, Cristiano Sampaio, Cristina de O. Dias, Daercio A. de A. Lucena, Daiara Manfio, Dalton de S. Amorim, Dalva L. de Queiroz, Daniara Colpani, Daniel Abbate, Daniel A. Aquino, Daniel Burckhardt, Daniel C. Cavallari, Daniel de C. Schelesky Prado, Daniel L. Praciano, Daniel S. Basílio, Daniela de C. Bená, Daniela G.P. de Toledo, Daniela M. Takiya, Daniell R.R. Fernandes, Danilo C. Ament, Danilo P. Cordeiro, Darliane E. Silva, Darren A. Pollock, David B. Muniz, David I. Gibson, David S. Nogueira, Dayse W.A. Marques, Débora Lucatelli, Deivys M.A. Garcia, Délio Baêta, Denise N.M. Ferreira, Diana Rueda-Ramírez, Diego A. Fachin, Diego de S. Souza, Diego F. Rodrigues, Diego G. de Pádua, Diego N. Barbosa, Diego R. Dolibaina, Diogo C. Amaral, Donald S. Chandler, Douglas H.B. Maccagnan, Edilson Caron, Edrielly Carvalho, Edson A. Adriano, Edson F. de Abreu Júnior, Edson H.L. Pereira, Eduarda F.G. Viegas, Eduardo Carneiro, Eduardo Colley, Eduardo Eizirik, Eduardo F. dos Santos, Eduardo M. Shimbori, Eduardo Suárez-Morales, Eliane P. de Arruda, Elisandra A. Chiquito, Élison F.B. Lima, Elizeu B. de Castro, Elton Orlandin, Elynton A. do Nascimento, Emanuel Razzolini, Emanuel R.R. Gama, Enilma M. de Araujo, Eric Y. Nishiyama, Erich L. Spiessberger, Érika C.L. dos Santos, Eugenia F. Contreras, Eunice A.B. Galati, Evaldo C. de Oliveira Junior, Fabiana Gallardo, Fabio A. Hernandes, Fábio A. Lansac-Tôha, Fabio B. Pitombo, Fabio Di Dario, Fábio L. dos Santos, Fabio Mauro, Fabio O. do Nascimento, Fabio Olmos, Fabio R. Amaral, Fabio Schunck, Fábio S. P. de Godoi, Fabrizio M. Machado, Fausto E. Barbo, Federico A. Agrain, Felipe B. Ribeiro, Felipe F.F. Moreira, Felipe F. Barbosa, Fenanda S. Silva, Fernanda F. Cavalcanti, Fernando C. Straube, Fernando Carbayo, Fernando Carvalho Filho, Fernando C.V. Zanella, Fernando de C. Jacinavicius, Fernando H.A. Farache, Fernando Leivas, Fernando M.S. Dias, Fernando Mantellato, Fernando Z. Vaz-de-Mello, Filipe M. Gudin, Flávio Albuquerque, Flavio B. Molina, Flávio D. Passos, Floyd W. Shockley, Francielly F. Pinheiro, Francisco de A.G. de Mello, Francisco E. de L. Nascimento, Francisco L. Franco, Francisco L. de Oliveira, Francisco T. de V. Melo, Freddy R.B. Quijano, Frederico F. Salles, Gabriel Biffi, Gabriel C. Queiroz, Gabriel L. Bizarro, Gabriela Hrycyna, Gabriela Leviski, Gareth S. Powell, Geane B. dos Santos, Geoffrey E. Morse, George Brown, George M.T. Mattox, Geraldo Zimbrão, Gervásio S. Carvalho, Gil F.G. Miranda, Gilberto J. de Moraes, Gilcélia M. Lourido, Gilmar P. Neves, Gilson R.P. Moreira, Giovanna G. Montingelli, Giovanni N. Maurício, Gláucia Marconato, Guilherme E.L. Lopez, Guilherme L. da Silva, Guilherme Muricy, Guilherme R.R. Brito, Guilherme S.T. Garbino, Gustavo E. Flores, Gustavo Graciolli, Gustavo S. Libardi, Heather C. Proctor, Helcio R. Gil-Santana, Henrique R. Varella, Hermes E. Escalona, Hermes J. Schmitz, Higor D.D. Rodrigues, Hilton de C. Galvão Filho, Hingrid Y.S. Quintino, Hudson A. Pinto, Hugo L. Rainho, Igor C. Miyahira, Igor de S. Gonçalves, Inês X. Martins, Irene A. Cardoso, Ismael B. de Oliveira, Ismael Franz, Itanna O. Fernandes, Ivan F. Golfetti, Ivanklin S. Campos-Filho, Ivo de S. Oliveira, Jacques H.C. Delabie, Jader de Oliveira, Jadila S. Prando, James L. Patton, Jamille de A. Bitencourt, Janaina M. Silva, Jandir C. Santos, Janine O. Arruda, Jefferson S. Valderrama, Jeronymo Dalapicolla, Jéssica P. Oliveira, Jiri Hájek, João P. Morselli, João P. Narita, João P.I. Martin, Jocélia Grazia, Joe McHugh, Jorge J. Cherem, José A.S. Farias Júnior, Jose A.M. Fernandes, José F. Pacheco, José L.O. Birindelli, José M. Rezende, Jose M. Avendaño, José M. Barbanti Duarte, José R. Inácio Ribeiro, José R.M. Mermudes, José R. Pujol-Luz, Josenilson R. dos Santos, Josenir T. Câmara, Joyce A. Teixeira, Joyce R. do Prado, Juan P. Botero, Julia C. Almeida, Julia Kohler, Julia P. Gonçalves, Julia S. Beneti, Julian P. Donahue, Juliana Alvim, Juliana C. Almeida, Juliana L. Segadilha, Juliana M. Wingert, Julianna F. Barbosa, Juliano Ferrer, Juliano F. dos Santos, Kamila M.D. Kuabara, Karine B. Nascimento, Karine Schoeninger, Karla M. Campião, Karla Soares, Kássia Zilch, Kim R. Barão, Larissa Teixeira, Laura D. do N.M. de Sousa, Leandro L. Dumas, Leandro M. Vieira, Leonardo H.G. Azevedo, Leonardo S. Carvalho, Leonardo S. de Souza, Leonardo S.G. Rocha, Leopoldo F.O. Bernardi, Letícia M. Vieira, Liana Johann, Lidianne Salvatierra, Livia de M. Oliveira, Lourdes M.A. El-moor Loureiro, Luana B. Barreto, Luana M. Barros, Lucas Lecci, Lucas M. de Camargos, Lucas R.C. Lima, Lucia M. Almeida, Luciana R. Martins, Luciane Marinoni, Luciano de A. Moura, Luciano Lima, Luciano N. Naka, Lucília S. Miranda, Lucy M. Salik, Luis E.A. Bezerra, Luis F. Silveira, Luiz A. Campos, Luiz A.S. de Castro, Luiz C. Pinho, Luiz F.L. Silveira, Luiz F.M. Iniesta, Luiz F.C. Tencatt, Luiz R.L. Simone, Luiz R. Malabarba, Luiza S. da Cruz, Lukas Sekerka, Lurdiana D. Barros, Luziany Q. Santos, Maciej Skoracki, Maira A. Correia, Manoel A. Uchoa, Manuella F.G. Andrade, Marcel G. Hermes, Marcel S. Miranda, Marcel S. de Araújo, Marcela L. Monné, Marcelo B. Labruna, Marcelo D. de Santis, Marcelo Duarte, Marcelo Knoff, Marcelo Nogueira, Marcelo R. de Britto, Marcelo R.S. de Melo, Marcelo R. de Carvalho, Marcelo T. Tavares, Marcelo V. Kitahara, Marcia C.N. Justo, Marcia J.C. Botelho, Márcia S. Couri, Márcio Borges-Martins, Márcio Felix, Marcio L. de Oliveira, Marco A. Bologna, Marco S. Gottschalk, Marcos D.S. Tavares, Marcos G. Lhano, Marcus Bevilaqua, Marcus T.T. Santos, Marcus V. Domingues, Maria A.M. Sallum, María C. Digiani, Maria C.A. Santarém, Maria C. do Nascimento, María de los A.M. Becerril, Maria E.A. dos Santos, Maria I. da S. dos Passos, Maria L. Felippe-Bauer, Mariana A. Cherman, Mariana Terossi, Marie L.C. Bartz, Marina F. de C. Barbosa, Marina V. Loeb, Mario Cohn-Haft, Mario Cupello, Marlúcia B. Martins, Martin L. Christofersen, Matheus Bento, Matheus dos S. Rocha, Maurício L. Martins, Melissa O. Segura, Melissa Q. Cardenas, Mércia E. Duarte, Michael A. Ivie, Michael M. Mincarone, Michela Borges, Miguel A. Monné, Mirna M. Casagrande, Monica A. Fernandez, Mônica Piovesan, Naércio A. Menezes, Natalia P. Benaim, Natália S. Reategui, Natan C. Pedro, Nathalia H. Pecly, Nelson Ferreira Júnior, Nelson J. da Silva Júnior, Nelson W. Perioto, Neusa Hamada, Nicolas Degallier, Ning L. Chao, Noeli J. Ferla, Olaf H.H. Mielke, Olivia Evangelista, Oscar A. Shibatta, Otto M.P. Oliveira, Pablo C.L. Albornoz, Pablo M. Dellapé, Pablo R. Gonçalves, Paloma H.F. Shimabukuro, Paschoal Grossi, Patrícia E. da S. Rodrigues, Patricia O.V. Lima, Paul Velazco, Paula B. dos Santos, Paula B. Araújo, Paula K.R. Silva, Paula R. Riccardi, Paulo C. de A. Garcia, Paulo G.H. Passos, Paulo H.C. Corgosinho, Paulo Lucinda, Paulo M.S. Costa, Paulo P. Alves, Paulo R. de O. Roth, Paulo R.S. Coelho, Paulo R.M. Duarte, Pedro F. de Carvalho, Pedro Gnaspini, Pedro G.B. Souza-Dias, Pedro M. Linardi, Pedro R. Bartholomay, Peterson R. Demite, Petr Bulirsch, Piter K. Boll, Rachel M.M. Pereira, Rafael A.P.F. Silva, Rafael B. de Moura, Rafael Boldrini, Rafaela A. da Silva, Rafaela L. Falaschi, Ralf T.S. Cordeiro, Ramon J.C.L. Mello, Randal A. Singer, Ranyse B. Querino, Raphael A. Heleodoro, Raphael de C. Castilho, Reginaldo Constantino, Reinaldo C. Guedes, Renan Carrenho, Renata S. Gomes, Renato Gregorin, Renato J.P. Machado, Renato S. Bérnils, Renato S. Capellari, Ricardo B. Silva, Ricardo Kawada, Ricardo M. Dias, Ricardo Siewert, Ricaro Brugnera, Richard A.B. Leschen, Robert Constantin, Robert Robbins, Roberta R. Pinto, Roberto E. dos Reis, Robson T. da C. Ramos, Rodney R. Cavichioli, Rodolfo C. de Barros, Rodrigo A. Caires, Rodrigo B. Salvador, Rodrigo C. Marques, Rodrigo C. Araújo, Rodrigo de O. Araujo, Rodrigo de V.P. Dios, Rodrigo Johnsson, Rodrigo M. Feitosa, Roger W. Hutchings, Rogéria I.R. Lara, Rogério V. Rossi, Roland Gerstmeier, Ronald Ochoa, Rosa S.G. Hutchings, Rosaly Ale-Rocha, Rosana M. da Rocha, Rosana Tidon, Rosangela Brito, Roseli Pellens, Sabrina R. dos Santos, Sandra D. dos Santos, Sandra V. Paiva, Sandro Santos, Sarah S. de Oliveira, Sávio C. Costa, Scott L. Gardner, Sebastián A. Muñoz Leal, Sergio Aloquio, Sergio L.C. Bonecker, Sergio L. de S. Bueno, Sérgio M. de Almeida, Sérgio N. Stampar, Sérgio R. Andena, Sergio R. Posso, Sheila P. Lima, Sian de S. Gadelha, Silvana C. Thiengo, Simone C. Cohen, Simone N. Brandão, Simone P. Rosa, Síria L.B. Ribeiro, Sócrates D. Letana, Sonia B. dos Santos, Sonia C.S. Andrade, Stephane Dávila, Stéphanie Vaz, Stewart B. Peck, Susete W. Christo, Suzan B.Z. Cunha, Suzete R. Gomes, Tácio Duarte, Taís Madeira-Ott, Taísa Marques, Talita Roell, Tarcilla C. de Lima, Tatiana A. Sepulveda, Tatiana F. Maria, Tatiana P. Ruschel, Thaiana Rodrigues, Thais A. Marinho, Thaís M. de Almeida, Thaís P. Miranda, Thales R.O. Freitas, Thalles P.L. Pereira, Thamara Zacca, Thaynara L. Pacheco, Thiago F. Martins, Thiago M. Alvarenga, Thiago R. de Carvalho, Thiago T.S. Polizei, Thomas C. McElrath, Thomas Henry, Tiago G. Pikart, Tiago J. Porto, Tiago K. Krolow, Tiago P. Carvalho, Tito M. da C. Lotufo, Ulisses Caramaschi, Ulisses dos S. Pinheiro, Ulyses F.J. Pardiñas, Valéria C. Maia, Valeria Tavares, Valmir A. Costa, Vanessa S. do Amaral, Vera C. Silva, Vera R. dos S. Wolff, Verônica Slobodian, Vinícius B. da Silva, Vinicius C. Espíndola, Vinicius da Costa-Silva, Vinicius de A. Bertaco, Vinícius Padula, Vinicius S. Ferreira, Vitor C.P. da Silva, Vítor de Q. Piacentini, Vivian E. Sandoval-Gómez, Vivian Trevine, Viviane R. Sousa, Vivianne B. de Sant’Anna, Wayne N. Mathis, Wesley de O. Souza, Wesley D. Colombo, Wioletta Tomaszewska, Wolmar B. Wosiacki, Ximena M.C. Ovando, and Yuri L.R. Leite
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Biodiversity ,knowledge management ,taxonomy ,web services ,zoology ,Zoology ,QL1-991 - Abstract
ABSTRACT The limited temporal completeness and taxonomic accuracy of species lists, made available in a traditional manner in scientific publications, has always represented a problem. These lists are invariably limited to a few taxonomic groups and do not represent up-to-date knowledge of all species and classifications. In this context, the Brazilian megadiverse fauna is no exception, and the Catálogo Taxonômico da Fauna do Brasil (CTFB) (http://fauna.jbrj.gov.br/), made public in 2015, represents a database on biodiversity anchored on a list of valid and expertly recognized scientific names of animals in Brazil. The CTFB is updated in near real time by a team of more than 800 specialists. By January 1, 2024, the CTFB compiled 133,691 nominal species, with 125,138 that were considered valid. Most of the valid species were arthropods (82.3%, with more than 102,000 species) and chordates (7.69%, with over 11,000 species). These taxa were followed by a cluster composed of Mollusca (3,567 species), Platyhelminthes (2,292 species), Annelida (1,833 species), and Nematoda (1,447 species). All remaining groups had less than 1,000 species reported in Brazil, with Cnidaria (831 species), Porifera (628 species), Rotifera (606 species), and Bryozoa (520 species) representing those with more than 500 species. Analysis of the CTFB database can facilitate and direct efforts towards the discovery of new species in Brazil, but it is also fundamental in providing the best available list of valid nominal species to users, including those in science, health, conservation efforts, and any initiative involving animals. The importance of the CTFB is evidenced by the elevated number of citations in the scientific literature in diverse areas of biology, law, anthropology, education, forensic science, and veterinary science, among others.
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- 2024
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32. Immunosuppression-induced Zika virus reactivation causes brain inflammation and behavioral deficits in mice
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Clara de O. Nogueira, Mariana Oliveira Lopes da Silva, Emanuelle V. de Lima, Raíssa Rilo Christoff, Daniel Gavino-Leopoldino, Felipe S. Lemos, Nicolas E. da Silva, Andrea T. Da Poian, Iranaia Assunção-Miranda, Claudia P. Figueiredo, and Julia R. Clarke
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Neuroscience ,Immunology ,Virology ,Science - Abstract
Summary: Zika virus (ZIKV) is a neurotropic flavivirus that can persist in several tissues. The late consequences of ZIKV persistence and whether new rounds of active replication can occur, remain unaddressed. Here, we investigated whether neonatally ZIKV-infected mice are susceptible to viral reactivation in adulthood. We found that when ZIKV-infected mice are treated with immunosuppressant drugs, they present increased susceptibility to chemically induced seizures. Levels of subgenomic flavivirus RNAs (sfRNAs) were increased, relative to the amounts of genomic RNAs, in the brains of mice following immunosuppression and were associated with changes in cytokine expression. We investigated the impact of immunosuppression on the testicles and found that ZIKV genomic RNA levels are increased in mice following immunosuppression, which also caused significant testicular damage. These findings suggest that ZIKV can establish new rounds of active replication long after acute stages of disease, so exposed patients should be monitored to ensure complete viral eradication.
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- 2024
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33. Radiation belt phase space density: calculation analysis and model dependence
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D. E. da Silva, S. R. Elkington, X. Li, M. K. Hudson, A. J. Boyd, A. N. Jaynes, and M. Wiltberger
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radiation belts ,phase space density ,adiabatic invariants ,geomagnetic storms ,magnetospherc physics ,Astronomy ,QB1-991 ,Geophysics. Cosmic physics ,QC801-809 - Abstract
The reprocessing of radiation belt electron flux measurements into phase space density (PSD) as a function of the adiabatic invariants is a widely-used method to address major questions regarding electron energization and loss in the outer radiation belt. In this reprocessing, flux measurements j (α, E) at local pitch angles α, energies E, and optionally magnetometer measurements B, are combined with a global magnetic field model to express the phase space density f (L*) in terms of the third invariant Φ ∝ 1/L* at fixed first and second invariants M and K. While the general framework of the calculation is agreed upon, implementation details vary amongst the literature, and the issue of magnetic field model dependence is rarely addressed. This work reviews the steps of the calculation with lists of commonly used implementation options. For the first time, analysis is presented to display the effect of doing the calculation with different implementation options and with different backing models (including both empirical and MHD-driven models). The results are summarized to inform evaluation of existing results and future efforts calculating and analyzing radiation belt electron phase space density. Three events are analyzed, and while differences are found, the primary structural interpretations of the phase space density analysis exhibit model independence.
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- 2024
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34. Tribological and Corrosion Behavior of AISI 1045 Coated with AISI 316 Film Produced By Triode Magnetron Sputtering
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Silviane C. F. Gorski, Bruno Nunes, Abel A. C. Recco, Cesar E. da Costa, Marcus V. F. Schroeder, and Julio C. Giubilei Milan
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Sliding Wear ,Thin films ,Magnetron Sputtering ,Corrosion Resistance ,Triode Magnetron Sputtering ,Stainless Steel Films ,Materials of engineering and construction. Mechanics of materials ,TA401-492 - Abstract
Recent studies have demonstrated mechanical, tribological and corrosion improvements properties on raw materials coated with stainless steel films produced by magnetron sputtering. However, few studies have reported the tribological behavior of thin austenitic stainless-steel films applied to the surface of carbon steels. The present study investigated the tribological behavior of AISI 1045 carbon steel coated with AISI 316 stainless steel film. Pin-on-disc dry sliding wear test was performed. The wear tracks were analyzed using a scanning electron and confocal microscopes. The corrosion resistance of coated and uncoated AISI 1045 were also assessed through an electrochemical test. Samples which presented a mixture of α-Ferrite and γ-iron, with predominant austenite parts, demonstrated lower friction coefficient, lower wear rates, and better corrosion resistance compared to substrate material. The results were also influenced by the variables used in the deposition process, as observed, heating the substrate and submitting to a higher powder density could improve the results. The results found corroborate to the academic and industrial research which looks for coating alternatives to AISI 1045 tools.
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- 2024
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35. Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
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Zürcher, D., Fluri, J., Sgier, R., Kacprzak, T., Gatti, M., Doux, C., Whiteway, L., Refregier, A., Chang, C., Jeffrey, N., Jain, B., Lemos, P., Bacon, D., Alarcon, A., Amon, A., Bechtol, K., Becker, M., Bernstein, G., Campos, A., Chen, R., Choi, A., Davis, C., Derose, J., Dodelson, S., Elsner, F., Elvin-Poole, J., Everett, S., Ferte, A., Gruen, D., Harrison, I., Huterer, D., Jarvis, M., Leget, P. F., Maccrann, N., Mccullough, J., Muir, J., Myles, J., Alsina, A. Navarro, Pandey, S., Prat, J., Raveri, M., Rollins, R. P., Roodman, A., Sanchez, C., Secco, L. F., Sheldon, E., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bertin, E., Brooks, D., Burke, D., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F., Cawthon, R., Conselice, C., Costanzi, M., da Costa, L., Pereira, M. E. da Silva, Davis, T., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J., Doel, P., Eckert, K., Evrard, A., Ferrero, I., Flaugher, B., Fosalba, P., Friedel, D., Frieman, J., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D., Giannantonio, T., Gruendl, R., Gschwend, J., Gutierrez, G., Hinton, S., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Lima, M., Maia, M., Marshall, J., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchon, F., Pieres, A., Malagón, A. Plazas, Reil, K., Monroy, M. Rodriguez, Romer, K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla, I., Smith, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., and Wilkinson, R.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We constrain the matter density $\Omega_{\mathrm{m}}$ and the amplitude of density fluctuations $\sigma_8$ within the $\Lambda$CDM cosmological model with shear peak statistics and angular convergence power spectra using mass maps constructed from the first three years of data of the Dark Energy Survey (DES Y3). We use tomographic shear peak statistics, including cross-peaks: peak counts calculated on maps created by taking a harmonic space product of the convergence of two tomographic redshift bins. Our analysis follows a forward-modelling scheme to create a likelihood of these statistics using N-body simulations, using a Gaussian process emulator. We include the following lensing systematics: multiplicative shear bias, photometric redshift uncertainty, and galaxy intrinsic alignment. Stringent scale cuts are applied to avoid biases from unmodelled baryonic physics. We find that the additional non-Gaussian information leads to a tightening of the constraints on the structure growth parameter yielding $S_8~\equiv~\sigma_8\sqrt{\Omega_{\mathrm{m}}/0.3}~=~0.797_{-0.013}^{+0.015}$ (68% confidence limits), with a precision of 1.8%, an improvement of ~38% compared to the angular power spectra only case. The results obtained with the angular power spectra and peak counts are found to be in agreement with each other and no significant difference in $S_8$ is recorded. We find a mild tension of $1.5 \thinspace \sigma$ between our study and the results from Planck 2018, with our analysis yielding a lower $S_8$. Furthermore, we observe that the combination of angular power spectra and tomographic peak counts breaks the degeneracy between galaxy intrinsic alignment $A_{\mathrm{IA}}$ and $S_8$, improving cosmological constraints. We run a suite of tests concluding that our results are robust and consistent with the results from other studies using DES Y3 data.
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- 2021
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36. Dark Energy Survey Year 3 results: Marginalisation over redshift distribution uncertainties using ranking of discrete realisations
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Cordero, Juan P., Harrison, Ian, Rollins, Richard P., Bernstein, G. M., Bridle, S. L., Alarcon, A., Alves, O., Amon, A., Andrade-Oliveira, F., Camacho, H., Campos, A., Choi, A., DeRose, J., Dodelson, S., Eckert, K., Eifler, T. F., Everett, S., Fang, X., Friedrich, O., Gruen, D., Gruendl, R. A., Hartley, W. G., Huff, E. M., Krause, E., Kuropatkin, N., MacCrann, N., McCullough, J., Myles, J., Pandey, S., Raveri, M., Rosenfeld, R., Rykoff, E. S., Sánchez, C., Sánchez, J., Sevilla-Noarbe, I., Sheldon, E., Troxel, M., Wechsler, R., Yanny, B., Yin, B., Zhang, Y., Aguena, M., Allam, S., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Cawthon, R., Costanzi, M., da Costa, L., Pereira, M. E. da Silva, De Vicente, J., Diehl, H. T., Dietrich, J., Doel, P., Elvin-Poole, J., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., Garcia-Bellido, J., Gerdes, D., Gschwend, J., Gutierrez, G., Hinton, S., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D., Kuehn, K., Lahav, O., Maia, M. A. G., March, M., Menanteau, F., Miquel, R., Morgan, R., Muir, J., Palmese, A., Paz-Chinchon, F., Pieres, A., Malagón, A. Plazas, Sánchez, E., Scarpine, V., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M., Tarle, G., Thomas, D., To, C., and Varga, T. N.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Cosmological information from weak lensing surveys is maximised by dividing source galaxies into tomographic sub-samples for which the redshift distributions are estimated. Uncertainties on these redshift distributions must be correctly propagated into the cosmological results. We present hyperrank, a new method for marginalising over redshift distribution uncertainties in cosmological analyses, using discrete samples from the space of all possible redshift distributions. This is demonstrated in contrast to previous highly simplified parametric models of the redshift distribution uncertainty. In hyperrank the set of proposed redshift distributions is ranked according to a small (in this work between one and four) number of summary values, which are then sampled along with other nuisance parameters and cosmological parameters in the Monte Carlo chain used for inference. This can be regarded as a general method for marginalising over discrete realisations of data vector variation with nuisance parameters, which can consequently be sampled separately to the main parameters of interest, allowing for increased computational efficiency. We focus on the case of weak lensing cosmic shear analyses and demonstrate our method using simulations made for the Dark Energy Survey (DES). We show the method can correctly and efficiently marginalise over a range of models for the redshift distribution uncertainty. Finally, we compare hyperrank to the common mean-shifting method of marginalising over redshift uncertainty, validating that this simpler model is sufficient for use in the DES Year 3 cosmology results presented in companion papers., Comment: Accepted for publication in MNRAS. 17 pages, 12 figures, comments welcome Replacement: Added small comments suggested by referee
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- 2021
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37. Inoculation methods of Azospirillum brasilense in lettuce and arugula in the hydroponic system (1) /Métodos de inoculação de Azospirillum brasilense em alface e rúcula em sistema hidropônico
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Oliveira, Carlos E. da S., Gato, Isabela M.B., Moreira, Vitoria de A., Jalal, Arshad, Oliveira, Thaissa J.S.S., Oliveira, Julia R., Fernandes, Guilherme C., and Filho, Marcelo C.M. Teixeira
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- 2023
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38. Effect of different air speeds at cow resting height in freestalls on heat stress responses and resting behavior in lactating cows in Wisconsin
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Kimberly J. Reuscher, Nigel B. Cook, Tadeu E. da Silva, Mario R. Mondaca, Karen M. Lutcherhand, and Jennifer M.C. Van Os
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animal welfare ,cow comfort ,ventilation ,heat abatement ,Dairy processing. Dairy products ,SF250.5-275 ,Dairying ,SF221-250 - Abstract
ABSTRACT: Heat abatement (e.g., soakers, fans) effectively reduces the negative physiological and production effects of heat stress, but no previous studies have documented effective interventions for the reduced lying times observed in response to hot weather. Although likely adaptive for heat dissipation, the reduction in motivated lying behavior may be an animal welfare concern. We evaluated the effect of air speed from fans with variable frequency drives on the heat stress responses of cows in a naturally ventilated freestall barn. Eight groups of lactating Holsteins (16 cows/group) were exposed to 3 treatments in a replicated crossover design: control (fans off, 0.4 ± 0.2 m/s, measured 0.5 m above the stall surface to represent cow resting height) versus 60% (1.7 ± 0.5 m/s; ≥1 m/s in all stalls) and 100% (2.4 ± 0.8 m/s) fan power. Each treatment was applied for 3 d of acclimation and 4 d of data collection. The effects of treatment on daily maximum vaginal temperature (VT) and lying time (LT; both measured with data loggers), respiration rate (RR; recorded from video), unshaved scapular skin temperature (ST), milk yield (MY), and dry matter intake (DMI) were analyzed using linear mixed models. All models included the fixed effect of treatment and a repeated term for treatment day within group of cows, with group as the subject. The models for LT, VT, and RR also included a fixed effect for same-day temperature-humidity index (THI; recorded in the pens with data loggers) and the THI × treatment interaction. The models for DMI and MY, using data from the latter 3 d of each treatment period, also included a fixed effect for the previous day's THI and the −1 d THI × treatment interaction. Lying time differed among treatments (100% vs. 60% fan power vs. control: 14.2 vs. 13.9 vs. 13.2 h/d, respectively, SEM = 0.15 h/d), but both fan treatments prevented the reduction in LT observed in the control treatment as THI increased. Relative to the control, both fan treatments effectively reduced ST, RR, and VT and increased DMI and MY. In the control, average values were elevated for both RR (68.7 ± 1.5 breaths/min, mean ± SEM, greater than a common benchmark of 60 breaths/min) and VT (39.3 ± 0.05°C) but remained in the normal range in both fan treatments (54.2 vs. 50.7 breaths/min in the 60% vs. 100% fan power treatments; 39.0°C in both fan treatments). Both fan treatments resulted in greater overall MY (42.6 vs. 43.0 ± 0.4 kg/d in the 60% vs. 100% fan power treatments) relative to the control (41.0 kg/d) and similarly avoided the reduction in MY when −1 d THI increased. Compared with natural ventilation alone, fans delivering air speeds of at least 1 m/s at cow resting height were effective not only for reducing thermoregulatory responses, but also for maintaining lying time, DMI, and MY in heat stress conditions. This is the first study to demonstrate an intervention to improve animal welfare by maintaining lying times during periods of heat stress.
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- 2023
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39. Cross-correlation of DES Y3 lensing and ACT/${\it Planck}$ thermal Sunyaev Zel'dovich Effect I: Measurements, systematics tests, and feedback model constraints
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Gatti, M., Pandey, S., Baxter, E., Hill, J. C., Moser, E., Raveri, M., Fang, X., DeRose, J., Giannini, G., Doux, C., Huang, H., Battaglia, N., Alarcon, A., Amon, A., Becker, M., Campos, A., Chang, C., Chen, R., Choi, A., Eckert, K., Elvin-Poole, J., Everett, S., Ferte, A., Harrison, I., Maccrann, N., Mccullough, J., Myles, J., Alsina, A. Navarro, Prat, J., Rollins, R. P., Sanchez, C., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Abbott, T., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bernstein, G., Bertin, E., Bolliet, B., Bond, J. R., Brooks, D., Burke, D. L., Calabrese, E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cawthon, R., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. da Silva, DeVicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Dunkley, J., Evrard, A. E., Ferraro, S., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., Garcıa-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Herner, K., Hincks, A. D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hughes, J. P., Huterer, D., Jain, B., James, D. J., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Lima, M., Lokken, M., Madhavacheril, M. S., Maia, M. A. G., Marshall, J. L., Mcmahon, J. J., Melchior, P., Moodley, K., Mohr, J. J., Morgan, R., Nati, F., Niemack, M. D., Page, L., Palmese, A., Paz-Chinchon, F., Pieres, A., Malagon, A. A. Plazas, Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Schaan, E., Secco, L. F., Serrano, S., Sheldon, E., Sherwin, B. D., Sifon, C., Smith, M., Soares-Santos, M., Spergel, D., Suchyta, E., Tarle, G., Thomas, D., To, C., Tucker, D. L., Varga, T. N., Weller, J., Wilkinson, R. D., Wollack, E. J., and Xu, Z.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present a tomographic measurement of the cross-correlation between thermal Sunyaev-Zeldovich (tSZ) maps from ${\it Planck}$ and the Atacama Cosmology Telescope (ACT) and weak galaxy lensing shears measured during the first three years of observations of the Dark Energy Survey (DES Y3). This correlation is sensitive to the thermal energy in baryons over a wide redshift range, and is therefore a powerful probe of astrophysical feedback. We detect the correlation at a statistical significance of $21\sigma$, the highest significance to date. We examine the tSZ maps for potential contaminants, including cosmic infrared background (CIB) and radio sources, finding that CIB has a substantial impact on our measurements and must be taken into account in our analysis. We use the cross-correlation measurements to test different feedback models. In particular, we model the tSZ using several different pressure profile models calibrated against hydrodynamical simulations. Our analysis marginalises over redshift uncertainties, shear calibration biases, and intrinsic alignment effects. We also marginalise over $\Omega_{\rm m}$ and $\sigma_8$ using ${\it Planck}$ or DES priors. We find that the data prefers the model with a low amplitude of the pressure profile at small scales, compatible with a scenario with strong AGN feedback and ejection of gas from the inner part of the halos. When using a more flexible model for the shear profile, constraints are weaker, and the data cannot discriminate between different baryonic prescriptions., Comment: submitted to PRD
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- 2021
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40. Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: I. Evidence for thermal energy anisotropy using oriented stacking
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Lokken, M., Hložek, R., van Engelen, A., Madhavacheril, M., Baxter, E., DeRose, J., Doux, C., Pandey, S., Rykoff, E. S., Stein, G., To, C., Abbott, T. M. C., Adhikari, S., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Battaglia, N., Bernstein, G. M., Bertin, E., Bond, J. R., Brooks, D., Calabrese, E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cawthon, R., Choi, A., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. da Silva, De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Dunkley, J., Everett, S., Evrard, A. E., Ferraro, S., Flaugher, B., Fosalba, P., Frieman, J., Gallardo, P. A., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hill, J. C., Hilton, M., Hincks, A. D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., Huang, Z., Hughes, J. P., Huterer, D., Jain, B., James, D. J., Jeltema, T., Kuehn, K., Lima, M., Maia, M. A. G., Marshall, J. L., McMahon, J., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Moodley, K., Morgan, R., Nati, F., Page, L., Ogando, R. L. C., Palmese, A., Chinchón, F. Paz, Malagón, A. A. Plazas, Pieres, A., Romer, A. K., Rozo, E., Sanchez, E., Scarpine, V., Schillaci, A., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Sifón, C., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Tucker, D. L., Varga, T. N., Weller, J., Wechsler, R. H., Wilkinson, R. D., Wollack, E. J., and Xu, Z.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
The cosmic web contains filamentary structure on a wide range of scales. On the largest scales, superclustering aligns multiple galaxy clusters along inter-cluster bridges, visible through their thermal Sunyaev-Zel'dovich signal in the Cosmic Microwave Background. We demonstrate a new, flexible method to analyze the hot gas signal from multi-scale extended structures. We use a Compton-$y$ map from the Atacama Cosmology Telescope (ACT) stacked on redMaPPer cluster positions from the optical Dark Energy Survey (DES). Cutout images from the $y$ map are oriented with large-scale structure information from DES galaxy data such that the superclustering signal is aligned before being overlaid. We find evidence for an extended quadrupole moment of the stacked $y$ signal at the 3.5$\sigma$ level, demonstrating that the large-scale thermal energy surrounding galaxy clusters is anisotropically distributed. We compare our ACT$\times$DES results with the Buzzard simulations, finding broad agreement. Using simulations, we highlight the promise of this novel technique for constraining the evolution of anisotropic, non-Gaussian structure using future combinations of microwave and optical surveys., Comment: 37 pages, 23 figures, 4 tables. Added explanatory figure, table, covariance matrix equations, discussion of CIB impact. Matches the version published in ApJ
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- 2021
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41. Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement
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Rosell, A. Carnero, Rodriguez-Monroy, M., Crocce, M., Elvin-Poole, J., Porredon, A., Ferrero, I., Mena-Fernandez, J., Cawthon, R., De Vicente, J., Gaztanaga, E., Ross, A. J., Sanchez, E., Sevilla-Noarbe, I., Alves, O., Andrade-Oliveira, F., Asorey, J., Avila, S., Brandao-Souza, A., Camacho, H., Chan, K. C., Ferte, A., Muir, J., Riquelme, W., Rosenfeld, R., Cid, D. Sanchez, Hartley, W. G., Weaverdyck, N., Abbott, T., Aguena, M., Sahar, A., Annis, J., Bertin, E., Brooks, D., Buckley-Geer, E., Burke, D., Calcino, J., Carollo, D., Kind, M. Carrasco, Carretero, J., Castander, F., Choi, A., Conselice, C., Costanzi, M., da Costa, L., Pereira, M. E. da Silva, Davis, T., Desai, S., Diehl, H. T., Doel, P., Drlica-Wagner, A., Eckert, K., Everett, S., Evrard, A., Flaugher, B., Fosalba, P., Frieman, J., Garcia-Bellido, J., Gerdes, D., Giannantonio, T., Glazebrook, K., Gruen, D., Gruendl, R., Gschwend, J., Gutierrez, G., Hinton, S., Hollowood, D., Honscheid, K., Hoyle, B., Huterer, D., James, D., Kim, A., Krause, E., Kuehn, K., Lahav, O., Lewis, G., Lidman, C., Lima, M., Maia, M., Malik, U., Marshall, J., Menanteau, F., Miquel, R., Mohr, J., Moller, A., Morgan, R., Ogando, R., Palmese, A., Paz-Chinchon, F., Percival, W., Pieres, A., Malagon, A. Plazas, Roodman, A., Scarpine, V., Schubnell, M., Serrano, S., Sharp, R., Sheldon, E., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M., Tarle, G., Thomas, D., To, C., Tucker, B., Tucker, D., Uddin, S., Varga, T. N., and Collaboration, DES
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
In this paper we present and validate the galaxy sample used for the analysis of the Baryon Acoustic Oscillation signal (BAO) in the Dark Energy Survey (DES) Y3 data. The definition is based on a colour and redshift-dependent magnitude cut optimized to select galaxies at redshifts higher than 0.5, while ensuring a high quality photometric redshift determination. The sample covers $\approx 4100$ square degrees to a depth of $i = 22.3 \ (AB)$ at $10\sigma$. It contains 7,031,993 galaxies in the redshift range from $z$= 0.6 to 1.1, with a mean effective redshift of 0.835. Photometric redshifts are estimated with the machine learning algorithm DNF, and are validated using the VIPERS PDR2 sample. We find a mean redshift bias of $z_{\mathrm{bias}} \approx 0.01$ and a mean uncertainty, in units of $1+z$, of $\sigma_{68} \approx 0.03$. We evaluate the galaxy population of the sample, showing it is mostly built upon Elliptical to Sbc types. Furthermore, we find a low level of stellar contamination of $\lesssim 4\%$. We present the method used to mitigate the effect of spurious clustering coming from observing conditions and other large-scale systematics. We apply it to the DES Y3 BAO sample and calculate sample weights that are used to get a robust estimate of the galaxy clustering signal. This paper is one of a series dedicated to the analysis of the BAO signal in the DES Y3 data. In the companion papers, Ferrero et al. (2021) and DES Collaboration (2021), we present the galaxy mock catalogues used to calibrate the analysis and the angular diameter distance constraints obtained through the fitting to the BAO scale, respectively. The galaxy sample, masks and additional material will be released in the public DES data repository upon acceptance., Comment: Accepted for publication in MNRAS. 24 pages, 24 figures
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- 2021
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42. Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
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DES Collaboration, Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., Avila, S., Bacon, D., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Bhargava, S., Birrer, S., Blazek, J., Brandao-Souza, A., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Camacho, H., Campos, A., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Cawthon, R., Chang, C., Chen, A., Chen, R., Choi, A., Conselice, C., Cordero, J., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. da Silva, Davis, C., Davis, T. M., De Vicente, J., DeRose, J., Desai, S., Di Valentino, E., Diehl, H. T., Dietrich, J. P., Dodelson, S., Doel, P., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Evrard, A. E., Fang, X., Farahi, A., Fernandez, E., Ferrero, I., Ferté, A., Fosalba, P., Friedrich, O., Frieman, J., García-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Giannini, G., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Harrison, I., Hartley, W. G., Herner, K., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., Huff, E. M., Huterer, D., Jain, B., James, D. J., Jarvis, M., Jeffrey, N., Jeltema, T., Kovacs, A., Krause, E., Kron, R., Kuehn, K., Kuropatkin, N., Lahav, O., Leget, P. -F., Lemos, P., Liddle, A. R., Lidman, C., Lima, M., Lin, H., MacCrann, N., Maia, M. A. G., Marshall, J. L., Martini, P., McCullough, J., Melchior, P., Mena-Fernández, J., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Muir, J., Myles, J., Nadathur, S., Navarro-Alsina, A., Nichol, R. C., Ogando, R. L. C., Omori, Y., Palmese, A., Pandey, S., Park, Y., Paz-Chinchón, F., Petravick, D., Pieres, A., Malagón, A. A. Plazas, Porredon, A., Prat, J., Raveri, M., Rodriguez-Monroy, M., Rollins, R. P., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Sanchez, J., Cid, D. Sanchez, Scarpine, V., Schubnell, M., Scolnic, D., Secco, L. F., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tabbutt, M., Tarle, G., Thomas, D., To, C., Troja, A., Troxel, M. A., Tucker, D. L., Tutusaus, I., Varga, T. N., Walker, A. R., Weaverdyck, N., Wechsler, R., Weller, J., Yanny, B., Yin, B., Zhang, Y., and Zuntz, J.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present the first cosmology results from large-scale structure in the Dark Energy Survey (DES) spanning 5000 deg$^2$. We perform an analysis combining three two-point correlation functions (3$\times$2pt): (i) cosmic shear using 100 million source galaxies, (ii) galaxy clustering, and (iii) the cross-correlation of source galaxy shear with lens galaxy positions. The analysis was designed to mitigate confirmation or observer bias; we describe specific changes made to the lens galaxy sample following unblinding of the results. We model the data within the flat $\Lambda$CDM and $w$CDM cosmological models. We find consistent cosmological results between the three two-point correlation functions; their combination yields clustering amplitude $S_8=0.776^{+0.017}_{-0.017}$ and matter density $\Omega_{\mathrm{m}} = 0.339^{+0.032}_{-0.031}$ in $\Lambda$CDM, mean with 68% confidence limits; $S_8=0.775^{+0.026}_{-0.024}$, $\Omega_{\mathrm{m}} = 0.352^{+0.035}_{-0.041}$, and dark energy equation-of-state parameter $w=-0.98^{+0.32}_{-0.20}$ in $w$CDM. This combination of DES data is consistent with the prediction of the model favored by the Planck 2018 cosmic microwave background (CMB) primary anisotropy data, which is quantified with a probability-to-exceed $p=0.13$ to $0.48$. When combining DES 3$\times$2pt data with available baryon acoustic oscillation, redshift-space distortion, and type Ia supernovae data, we find $p=0.34$. Combining all of these data sets with Planck CMB lensing yields joint parameter constraints of $S_8 = 0.812^{+0.008}_{-0.008}$, $\Omega_{\mathrm{m}} = 0.306^{+0.004}_{-0.005}$, $h=0.680^{+0.004}_{-0.003}$, and $\sum m_{\nu}<0.13 \;\mathrm{eV\; (95\% \;CL)}$ in $\Lambda$CDM; $S_8 = 0.812^{+0.008}_{-0.008}$, $\Omega_{\mathrm{m}} = 0.302^{+0.006}_{-0.006}$, $h=0.687^{+0.006}_{-0.007}$, and $w=-1.031^{+0.030}_{-0.027}$ in $w$CDM. (abridged), Comment: See https://www.darkenergysurvey.org/des-year-3-cosmology-results-papers/ for the full DES Y3 3x2pt cosmology release. Matches version accepted in PRD
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- 2021
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43. Active Displacement of a Unique Diatom–Ciliate Symbiotic Association
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Yonara Garcia, Felipe M. Neves, Flavio R. Rusch, Leandro T. De La Cruz, Marina E. Wosniack, J. Rudi Strickler, Marcos G. E. da Luz, and Rubens M. Lopes
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diatom–ciliate symbiosis ,mutualism ,co-evolution ,displacement behavior ,movement ecology ,Thermodynamics ,QC310.15-319 ,Descriptive and experimental mechanics ,QC120-168.85 - Abstract
Adaptive movement in response to individual interactions represents a fundamental evolutionary solution found by both unicellular organisms and metazoans to avoid predators, search for resources or conspecifics for mating, and engage in other collaborative endeavors. Displacement processes are known to affect interspecific relationships, especially when linked to foraging strategies. Various displacement phenomena occur in marine plankton, ranging from the large-scale diel vertical migration of zooplankton to microscale interactions around microalgal cells. Among these symbiotic interactions, collaboration between the centric diatom Chaetoceros coarctatus and the peritrich ciliate Vorticella oceanica is widely known and has been recorded in several studies. Here, using 2D and 3D tracking records, we describe the movement patterns of the non-motile, chain-forming diatoms (C. coarctatus) carried by epibiotic ciliates (V. oceanica). The reported data on the Chaetoceros–Vorticella association illustrated the consortium’s ability to generate distinct motility patterns. We established that the currents generated by the attached ciliates, along with the variability in the contraction and relaxation of ciliate stalks in response to food concentration, resulted in three types of trajectories for the consortium. The characteristics of these distinct paths were determined using robust statistical methods, indicating that the different displacement behaviors allowed the consortium to adequately explore distributed resources and remain within the food-rich layers provided in the experimental containers. A simple mechanical–stochastic model was successfully applied to simulate the observed displacement patterns, further supporting the proposed mechanisms of collective response to the environment.
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- 2024
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44. Basic Cells Special Features and Their Influence on Global Transport Properties of Long Periodic Structures
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Luna R. N. Oliveira and Marcos G. E. da Luz
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transmission properties ,localized potentials ,scattering amplitudes ,band structure ,Science ,Astrophysics ,QB460-466 ,Physics ,QC1-999 - Abstract
In this contribution, we address quantum transport in long periodic arrays whose basic cells, localized potentials U(x), display certain particular features. We investigate under which conditions these “local” special characteristics can influence the tunneling behavior through the full structure. As the building blocks, we consider two types of U(x)s: combinations of either Pöschl–Teller, U0/cosh2[αx], potentials (for which the reflection and transmission coefficients are known analytically) or Gaussian-shaped potentials. For the latter, we employ an improved potential slicing procedure using basic barriers, like rectangular, triangular and trapezoidal, to approximate U(x) and thus obtain its scattering amplitudes. By means of a recently derived method, we discuss scattering along lattices composed of a number, N, of these U(x)s. We find that near-resonance energies of an isolated U(x) do impact the corresponding energy bands in the limit of very large Ns, but only when the cell is spatially asymmetric. Then, there is a very narrow opening (defect or rip) in the system conduction quasi-band, corresponding to the energy of the U(x) quasi-state. Also, for specific U0’s of a single Pöschl–Teller well, one has 100% transmission for any incident E>0. For the U(x) parameters rather close to such a condition, the associated array leads to a kind of “reflection comb” for large Ns; |TN(k)|2 is not close to one only at very specific values of k, when |TN|2≈0. Finally, the examples here—illustrating how the anomalous transport comportment in finite but long lattices can be inherited from certain singular aspects of the U(x)s—are briefly discussed in the context of known effects in the literature, notably for lattices with asymmetric cells.
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- 2024
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45. A Simplified Daily Fit Model to Reduce Costs and Nutrient Intake in Growing-Finishing Pigs
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Yann M. Ferreira, Rayna S. V. Amaral, Blandina G. V. Silva, Leila C. S. Moura, Diana A. Oliveira, Tadeu E. da Silva, Luciano Hauschild, Ines Andretta, and Luan S. Santos
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feed cost reduction ,nutrient management ,precision feeding ,sustainable pig farming ,swine nutrition ,Veterinary medicine ,SF600-1100 ,Zoology ,QL1-991 - Abstract
Precision feeding is an excellent alternative to conventional phase feeding systems for growing-finishing pigs, especially with increasing feeding costs and environmental sustainability concerns. However, precision feeding strategies sometimes require advanced technologies such as electronic devices and the modernization of pig facilities. In addition to hardware implementation, precision feeding is frequently related to mathematical difficulties due to a lack of professionals trained in decision making. Therefore, this study compares a conventional phase feeding model (CON) and a daily fit model (DFM) with a simplified approach to the conscious use of nutrients for pig production. A simulation study was conducted using growth curves of barrow pigs, following three nutritional recommendations for conventional phase feeding. Once the nutrient requirements for CON were determined, these diets were used for the DFM by anticipating a proportional percentage of the next phase diet in the current diet. This simple adjustment does not impair the growth performance of pigs. However, in this study, the DFM showed promise during the growing-finishing phases to reduce pigs’ costs and nutrient intakes, such as crude protein, lysine, and digestible phosphorus, up to 5.58, 7.11 and 9.13%, respectively. In conclusion, the DFM can effectively reduce costs, minimize environmental impact, and promote sustainable practices. Also, this industry-wide adoption of this simplified precision feeding strategy could play a vital role in swine farmers’ challenges, fostering broader environmental benefits and improved resource efficiency.
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- 2024
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46. Foliar nitrogen fertilization attenuating harmful effects of salt stress on purple basil/A adubacao foliar com nitrogenio alivia os efeitos nocivos do estresse salino no manjericao roxo
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Nobrega, Jackson S., Silva, Toshik I. da, Lopes, Adriano S., Costa, Raimundo N. M., Ribeiro, Joao E. da S., Silva, Edcarlos C. da, Bezerra, Ana C., xSilva, Antonio V. da, and Dias, Thiago J.
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- 2023
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47. Legal boundaries and conservation: The case of Seasonally Dry Forests of the Serra da Bodoquena National Park, Brazil
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Geraldo A. Damasceno Junior, Maxwell R. Oliveira, Flávio M. Alves, Rosa Helena da Silva, Vali J. Pott, Adriano A. Spielmann, André Aptroot, Sandro R. S. Pereira, Suziele G. Batista, Lucas E. da Silva, Vivian A. Nakamura, and Arnildo Pott
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Atlantic Forest ,environmental policy ,environmental law ,Neotropical forest ,Protected Area ,Seasonal Forest ,Botany ,QK1-989 - Abstract
ABSTRACT The Serra da Bodoquena National Park is an important protected area that promotes the conservation of a threatened ecosystem, the Dry Forest. It comprises two major fragments of predominantly Seasonally Dry Forest vegetation. The two fragments are under different protection schemes because they are considered different biomes. The southern fragment is considered part of the Atlantic Forest biome, and is thus protected by the Atlantic Forest Law, while the northern one is considered part of the Cerrado biome and is protected by the Native Vegetation Protection Law of Brazil (2012). This difference affects management and threatens the conservation of the National Park. The Native Vegetation Protection Law is more permissive, thus increasing the conflicts between the park and surroundings in the northern fragment. We used floristic composition to provide a more accurate definition for the two fragments with regard to their phytogeographical domain. Our results identified high floristic similarity between the fragments, indicating the same vegetation type for both. Among the 202 plant species identified in this study, 76% belong to the Atlantic Forest biome. This relatively high proportion indicates that the predominant vegetation and species composition of the National Park is typical of the Atlantic Forest. The occurrence of fragments of the Atlantic Forest, with a representative number of species of its flora outside the area of application of the law of the Atlantic Forest, defined by Decree No. 6.660 / 2008, indicates the need to elaborate or adapt the law to protect these fragments.
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- 2024
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48. Quantifying adiabatic motion in the outer radiation belt and ring current with invariant matching
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D. E. da Silva, S. R. Elkington, X. Li, and M. K. Hudson
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radiation belts ,ring current ,adiabatic motion ,adiabatic invariants ,magnetospheric currents ,Astronomy ,QB1-991 ,Geophysics. Cosmic physics ,QC801-809 - Abstract
Adiabatic motion is a fundamental reversible process for geomagnetically trapped particle populations, including particles comprising the ring current and radiation belts. During adiabatic motion, a particle’s trajectory in configuration space responds to sufficiently slow changes in the magnetospheric magnetic field. Previous research has highlighted expected patterns in adiabatic motion, such as radial motion or the Dst effect. In this work, we introduce a method we call Invariant Matching for quantifying adiabatic motion between a pair of magnetospheres. This method can be applied to both simulation and semi-empirical magnetic field models, is computationally efficient, and in particular does not require tracing the particle trajectories. In this work, we use the Tsyganenko et al., Journal of Geophysical Research: Space Physics, 2005, 110 (TS05) magnetic field model, and present adiabatic motion between a storm commencement, the time of the storm’s Dst minimum, and a nominal recovery time. We also analyze adiabatic motion which occurs in response to enhancements of individual major current systems (including the ring current, Chapman-Ferraro current, Birkeland current, and tail current). Our methodology yields vector fields quantifying the displacement of mirror points throughout the magnetosphere, prepared in a way appropriate for application to both outer radiation belt and ring current populations.
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- 2024
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49. Monitoring the micellar packing of photo-crosslinkable Pluronic F127 dimethacrylate during 3D printing
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Mateus P. Bomediano, Laura C. E. da Silva, Pablo Mota-Santiago, Marcelo G. de Oliveira, and Tomás S. Plivelic
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in operando 3D printing ,time-resolved SAXS ,Pluronic ,micellar inks ,hydrogels ,photo-crosslinking ,Chemistry ,QD1-999 ,Medical physics. Medical radiology. Nuclear medicine ,R895-920 ,Polymers and polymer manufacture ,TP1080-1185 - Abstract
Pluronic F127 dimethacrylate (F127-DM) inks exhibit potential for 3D printing biomaterials due to their combined gelation and photo-crosslinking capabilities. Previous studies have explored their application in extrusion 3D printing of medical devices, relying on their long-range micellar ordering to impart mechanical stability, stretchability, and control over drug delivery. However, there is a lack of information regarding the impact of the extrusion and photo-crosslinking processes on the micellar ordering of F127-DM. Herein, we employed in operando 3D printing synchrotron small-angle X-ray scattering (SAXS) to analyze the influence of various printing parameters, including nozzle shape, nozzle size, extrusion rate, ink composition, and photo-crosslinking, on the micellar ordering of F127-DM. Our findings from 2D SAXS patterns indicate orientation of the micellar packing clusters along the flow direction. The nozzle diameter and shape emerged as crucial parameters, leading to increased disruption of long-range ordering. Furthermore, 1D SAXS curves during UV-Vis light exposure and photo-crosslinking revealed a partial preservation of the micellar packing structure, with cluster size reduction, and coexisting with randomly distributed micelles and unimers. These results underscore the importance of in operando synchrotron experiments for the systematic study of 3D printing parameters from a nanostructure perspective.
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- 2024
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50. Molecular structure determination of Nickel(II) isomers bearing bis(thiosemicarbazone) ligands: X-ray, DFT calculations and kinetic groundwork
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Lima, Raíza F. X., Oliveira, Danilo A., do Prado, Cássio R. A., Siqueira Jr., José R., Deflon, Victor M., Hagenbach, Adelhaid, Abram, Ulrich, Machado, Antonio E. da Hora, Bogado, André L., and Maia, Pedro I. S.
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- 2024
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