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Roasted and Unroasted Cocoa Nibs: Bioactive Compounds Analysis and Application in Cereal Bars. [PDF]
Souza MSDS +9 more
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Do all sedatives promote biological sleep electroencephalogram patterns? A machine learning framework to identify biological sleep promoting sedatives using electroencephalogram. [PDF]
Ramaswamy SM +5 more
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The Role of ISASS in Evolving the Spine Code Landscape: Lumbar Discogenic Pain Receives Specific ICD-10-CM Code. [PDF]
Lorio MP +4 more
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Diffuse X-Ray Emission in M51: A Hierarchical Bayesian Spatially Resolved Spectral Analysis
Astrophysical JournalX-ray observations can be used to effectively probe the galactic ecosystem, particularly its hot and energetic components. However, existing X-ray studies of nearby star-forming galaxies are limited by insufficient data statistics and a lack of suitable ...
Luan Luan, Q. D. Wang
semanticscholar +1 more source
Astrophysical Journal
With a new joint-deconvolution pipeline, we combine the single-dish and interferometric atomic hydrogen (H i) data of M51 observed by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) (FEASTS program) and the Very Large Array (VLA) (THINGS)
Xuchen 旭辰 Lin 林 +15 more
semanticscholar +1 more source
With a new joint-deconvolution pipeline, we combine the single-dish and interferometric atomic hydrogen (H i) data of M51 observed by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) (FEASTS program) and the Very Large Array (VLA) (THINGS)
Xuchen 旭辰 Lin 林 +15 more
semanticscholar +1 more source
1990
We observed the nearby Sc galaxy M51 (NGC 5194) and its companion NGC 5195 with the VLA in the 21-cm line to study the distribution and kinematics of the HI. M51 is a key object in the study of galaxies: its beautiful spiral structure with the clear separation of the dust lanes and associated radio continuum emission from the bright HII regions and OB ...
A. H. Rots +4 more
openaire +1 more source
We observed the nearby Sc galaxy M51 (NGC 5194) and its companion NGC 5195 with the VLA in the 21-cm line to study the distribution and kinematics of the HI. M51 is a key object in the study of galaxies: its beautiful spiral structure with the clear separation of the dust lanes and associated radio continuum emission from the bright HII regions and OB ...
A. H. Rots +4 more
openaire +1 more source

