Results 111 to 120 of about 26,106 (206)
The James Webb Space Telescope (JWST) has revealed a population of red and compact sources at z ≳ 5 known as “little red dots” (LRDs) that are likely active galactic nuclei (AGNs).
Zijian Zhang +3 more
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Long-period comets, which are often considered to be representative of material in the protoplanetary disk that formed the solar system, are ideal to investigate the question of chemical inheritance in astronomy. Determining the chemistry of comets, both
K. D. Foster +9 more
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The James Webb Space Telescope (JWST) has begun to revolutionize our view of the Cosmos. The discovery of Blue Monsters (i.e., ultra-compact yet very bright high-z galaxies) and the Little Red Dots (i.e., very compact dustless strong Balmer break cosmic ...
Cosmin Ilie +3 more
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This work does not propose a new cosmological model, nor does it claim to reproduce structure formation, recombination microphysics, or the CMB power spectrum. It instead examines limited, testable consequences of a previously established background level redshift framework in which frequency-independent redshift is described by collisionless Liouville
openaire +1 more source
The first billion years according to JWST
review article written by the attendees of the 2024 ISSI breakthrough workshop "The first billion year of the Universe", submitted.
Angela Adamo +48 more
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SCUBADive. I. JWST+ALMA Analysis of 289 Submillimeter Galaxies in COSMOS-web
JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of submillimeter galaxies, revealing detail that was previously inaccessible.
Jed McKinney +38 more
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JWST is opening many avenues for exploration. For cold brown dwarfs and exoplanets, JWST has opened the door to the mid-infrared wavelength region, where such objects emit significant energy.
S. K. Leggett, Pascal Tremblin
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Observations of the first galaxies in the Era of JWST
49 pages, 12 figures; Submitted to Encyclopedia of Astrophysics, November ...
Stark, Daniel P. +3 more
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We present follow-up imaging and spectroscopy and pre-explosion imaging of SN 2025pht located in NGC 1637 at 12 Mpc. Our spectroscopy shows that SN 2025pht is a Type II supernova (SN) with broad lines of hydrogen and with minimal line-of-sight extinction
Charles D. Kilpatrick +9 more
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