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http://dx.doi.org/10.1038/509276a | DOI Listing |
Nature
December 2024
NRC Herzberg, Victoria British Columbia, Canada.
Recent observations have found a large number of supermassive black holes already in place in the first few hundred million years after the Big Bang, many of which seem to be overmassive relative to their host galaxy stellar mass when compared with local relation. Several different models have been proposed to explain these findings, ranging from heavy seeds to light seeds experiencing bursts of high accretion rate. Yet, current datasets are unable to differentiate between these various scenarios.
View Article and Find Full Text PDFPLoS One
November 2024
Center for Plants, People and Culture, New York Botanical Garden, Bronx, NY, United States of America.
Based on original ethnographic and ethnobotanical research, we share how in the cosmology of Tanna, an island in Vanuatu's southernmost province of Tafea, the Sun is viewed as a living, interactive being. Our initial interviews explored knowledge and beliefs concerning individual plant species, then subsequent follow-up interviews further explored topics that emerged therefrom. The results of these interviews are a series of oral narratives of the mytho-historical past involving the Sun, and the description of contemporary practices which are influenced by the Sun.
View Article and Find Full Text PDFPhys Rev Lett
October 2024
CERN, Geneva, Switzerland.
Open Res Eur
June 2024
Institute of Theoretical Astrophysics, University of Oslo, Oslo, N-0315, Norway.
During the most active period of star formation in galaxies, which occurs in the redshift range 1 3, strong bursts of star formation result in significant quantities of dust, which obscures new stars being formed as their UV/optical light is absorbed and then re-emitted in the infrared, which redshifts into the mm/sub-mm bands for these early times. To get a complete picture of the high- galaxy population, we need to survey a large patch of the sky in the sub-mm with sufficient angular resolution to resolve all galaxies, but we also need the depth to fully sample their cosmic evolution, and therefore obtain their redshifts using direct mm spectroscopy with a very wide frequency coverage. This requires a large single-dish sub-mm telescope with fast mapping speeds at high sensitivity and angular resolution, a large bandwidth with good spectral resolution and multiplex spectroscopic capabilities.
View Article and Find Full Text PDFProc Natl Acad Sci U S A
October 2024
Steward Observatory, University of Arizona, Tucson, AZ 85721.
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