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161
Stability of Watch-Based Blood Pressure Measurements Analyzed by Pre-Post Calibration Differences
Published 2024-01-01“…This study uses real-world data from a Samsung Galaxy Watch campaign to assess smartwatch-based BP measurements. …”
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162
Real-Time Pose Prediction and Dynamic Anchor Selection for Ultra-Wideband Tagless Gate
Published 2025-01-01“…DynaPose is implemented on Samsung Galaxy Note20 Ultra and Qorvo UWB board to show the feasibility and applicability. …”
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163
Cosmic Reionization on Computers: The Evolution of the Ionizing Background and Mean Free Path
Published 2025-01-01“…In this study, we utilize the Cosmic Reionization on Computers (CROC) simulations, which have both sufficient spatial resolution to resolve galaxy formation and LLSs alongside a fully coupled radiative transfer, to simulate the reionization processes. …”
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164
Hunting for Cold Exoplanets via Microlensing
Published 2023-08-01“…It has shown that having a planet is the rule for stars in our galaxy and shown that super-Earth and Neptune are more abundant than smaller mass telluric planets. …”
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165
Accuracy of the SWAY Mobile Cognitive Assessment Application
Published 2021-08-01“… # Results ANOVAs reported the SWAY CA application (reaction time, impulse control, inspection time) operated reliably with iPhone 6S, Samsung Galaxy S9, and iPad Pro 5 mobile devices (*p* \> 0.05), respectively. …”
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166
Responses of bimetallic Ag/ZnO alloy nanoparticles and urea on morphological and physiological attributes of wheat
Published 2021-09-01“…Different concentrations of urea and Ag/ZnO alloy NPs were applied exogenously to wheat plants (Pakistan‐13 and Galaxy13). A significant effect of 100 mg/L urea and 75 ppm Ag/ZnO alloy NPs was observed on the morphology of wheat, with a maximum increase of 58% plant length, 85% leaf area, 89% plant fresh weight and 76% plant dried weight. …”
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167
Rates of Stellar Tidal Disruption Events around Intermediate-mass Black Holes
Published 2025-01-01“…In this work, we aim to accurately calculate the IMBH TDE rates based on their black hole (BH) masses and the stellar profiles of their host galaxies obtained from the latest observations. We find that the TDE rate per galaxy for IMBHs in the center of small galaxies is similar to that of SMBH TDEs, while the TDE rate per cluster from IMBHs in globular clusters is much lower. …”
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168
mRNA-lncRNA gene expression signature in HPV-associated neoplasia and cervical cancer
Published 2024-05-01“…Raw data were preprocessed using the Galaxy platform. Batch effect correction, identification of differentially expressed genes, and gene set enrichment analysis (GSEA) were performed using R programming language packages. …”
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169
Identificación de áreas inundables del parque provincial San Cayetano (Corrientes, Argentina)
Published 2024-08-01“…Para concretar este objetivo se realizaron en primera instancia mediciones de Puntos de Apoyo Fotogramétricos (PAF) con un receptor GNSS geodésico South Galaxy G1 para otorgar mayor confiabilidad a los resultados generados en la etapa de postproceso y se sobrevoló el Parque San Cayetano con un Drone modelo Mavic 2 pro de la firma DJI, que cuenta con un sensor CMOS de 1” y resolución de 20 megapíxeles, lo que posibilitó la obtención de fotografías aéreas con características necesarias para la generación de un MDE. …”
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170
A Multiple-detection-heads Machine Learning Algorithm for Detecting White Dwarfs
Published 2025-01-01“…White dwarfs (WDs) are the ultimate stage for approximately 97% of stars in the Milky Way and are crucial for studying stellar evolution and galaxy structure. Due to their small size and low luminosity, WDs are not easily observable. …”
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171
Contribution of Unresolved Sources to Diffuse Gamma-Ray Emission from the Galactic Plane
Published 2025-01-01“…The diffuse gamma-ray emission from the Milky Way serves as a crucial probe for understanding the propagation and interactions of cosmic rays within our Galaxy. The Galactic diffuse gamma-ray emission between 10 TeV and 1 PeV has been recently measured by the square kilometer array (KM2A) of the Large High Altitude Air Shower Observatory (LHAASO). …”
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172
Quantifying Baryonic Feedback on the Warm–Hot Circumgalactic Medium in CAMELS Simulations
Published 2025-01-01“…The baryonic physics shaping galaxy formation and evolution are complex, spanning a vast range of scales and making them challenging to model. …”
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173
GRB 241107A: A Giant Flare from a Close-by Extragalactic Magnetar?
Published 2025-01-01“…The presence of the nearby galaxy PGC 86046 in the 3′ radius error region suggests that GRB 241107A might be a giant flare from a magnetar rather than a canonical short gamma-ray burst. …”
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174
Search for Neutrino Signals Correlated with LHAASO Diffuse Galactic Emission
Published 2025-01-01“…The diffuse Galactic γ -ray emission originates from the interactions between cosmic rays and the interstellar medium or radiation fields within our Galaxy, where the production of neutrinos is also anticipated. …”
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175
GD-1 Stellar Stream and Cocoon in the DESI Early Data Release
Published 2025-01-01“…The progenitor of the GD-1 stream was an accreted globular cluster (GC) and: (a) the cocoon was produced by pre-accretion tidal stripping of the GC while it was still inside its parent dwarf galaxy; (b) the cocoon comprises debris from the parent dwarf galaxy; (c) an initially thin GC tidal stream was heated by impacts from dark subhalos in the Milky Way; (d) an initially thin GC stream was heated by a massive Sagittarius dwarf galaxy; or a combination of some of these. …”
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176
Excess Ultraviolet Emission at High Galactic Latitudes: A New Horizons View
Published 2025-01-01“…The former is the first firm detection of the offset in the range 912–1100 Å while the latter result confirms previous results from the Galaxy Evolution Explorer, showing that there is little emission from the solar system from 1400 to 1800 Å. …”
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177
Forest Fire Clustering: A Novel Tool for Identifying Star Members of Clusters
Published 2025-01-01“…We use a Gaia DR3 catalog comprising 322 random objects with distinct heliocentric distances from approximately 0 to 5 kpc, along with one ultrafaint dwarf galaxy Bootes I (∼63 kpc), as our validation sample. …”
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178
Genomic characterization of Achromobacter genogroup 20 and identification of a potential species-specific marker
Published 2025-01-01“…NGS was conducted using Illumina MiSeq, on the NextSeq500 platform with 150 bp paired-end reads, and de novo assembly was assessed using Unicycler (Galaxy). Coding sequences were predicted and confirmed with RAST and BLAST, and resistance determinants were evaluated using Resfinder and manual curation. …”
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179
COSMIC’s Large-scale Search for Technosignatures during the VLA Sky Survey: Survey Description and First Results
Published 2025-01-01“…Jansky Very Large Array (VLA) in New Mexico in order to search for signals throughout the Galaxy consistent with our understanding of artificial radio emissions. …”
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180
The Sunburst Arc with JWST. III. An Abundance of Direct Chemical Abundances
Published 2025-01-01“…With these temperature and density measurements, we measure gas-phase abundances with similar rigor as studies of local galaxies and H ii regions. We measure a gas-phase metallicity for the LCE of $12+\mathrm{log}({\rm{O}}/{\rm{H}})=7.97\pm 0.05$ , and find an enhanced nitrogen abundance $\mathrm{log}({\rm{N}}/{\rm{O}})=-0.6{5}_{-0.25}^{+0.16}$ . …”
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