Results 71 to 80 of about 306,857 (215)
Abstract Dust, sea salt, and anthropogenic and biogenic particles in total atmospheric deposition are sources of essential elements that can significantly impact biogeochemical cycles in the Atlantic Ocean and in islands of the Caribbean region. This unique 41‐month data set records direct sampling of total atmospheric deposition from March 2015 to ...
Yangjunjie Xu‐Yang +6 more
wiley +1 more source
The architecture of the crust in the French Massif Central (FMC) is described as a nappe stack composed, from top to bottom, of the Upper Gneiss Unit (UGU), the Lower Gneiss Unit (LGU), and the Para-Autochthonous Unit (PAU), which are intruded by ...
Passos do Carmo Caliméria +6 more
doaj +1 more source
YOLO-CIANNA: Galaxy detection with deep learning in radio data
Context. As the scientific exploitation of the Square Kilometre Array (SKA) approaches, there is a need for new advanced data analysis and visualization tools capable of processing large high-dimensional datasets. Aims.
Cornu D. +10 more
doaj +1 more source
Observatoire de Paris. In: Bulletin administratif de l'instruction publique. Tome 46 n°867, 1889.
core +2 more sources
Observatoire de Meudon. In: Bulletin administratif de l'instruction publique. Tome 29 n°534, 1883.
core +2 more sources
Observatoire de Bordeaux. In: Bulletin administratif de l'instruction publique. Tome 44 n°826, 1888.
core +1 more source
Discovery of new N-emitters over a wide redshift range
Context. Recent James Webb Space Telescope (JWST) observations have revealed a small number of galaxies with UV spectra exhibiting intense nitrogen emission lines, which are not typically detected in galaxy spectra.
Morel I. +7 more
doaj +1 more source
Most of phytoplankton influence is barely understood at the sub meso scale and daily scale because of the lack of means to simultaneously assess phytoplankton functionality, dynamics and community structure.
Melilotus eThyssen +14 more
doaj +1 more source
The K-dwarf TOI-4504 hosts two giant planets in a 2:1 mean-motion resonance (MMR) with orbital periods of 41.3 days (planet d) and 82.8 days (planet c). They exhibit among the largest known absolute transit-timing variations, with respective peak-to-node
Almenara J. M. +17 more
doaj +1 more source
Observatoire de Paris. In: Bulletin administratif de l'instruction publique. Tome 42 n°776, 1887.
core +2 more sources

