Results 91 to 100 of about 184 (166)
Low-redshift Analogs of Cosmic Noon Galaxies as Laboratories for Clumpy Star Formation
It has been established that a significant fraction of star formation at high redshift occurs in clumpy galaxies. The properties of clumps and their formation mechanisms, however, remain highly debated. In this work we analyze a sample of 18 supercompact
Jorge M. Santos-Junior +5 more
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CANUCS: An Updated Mass and Magnification Model of A370 with JWST
We present an updated mass and magnification model of galaxy cluster A370 using new NIRCam, NIRISS, and NIRSpec data from the Canadian NIRISS Unbiased Cluster Survey (CANUCS).
Rachel Gledhill +11 more
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Testing general relativity with cosmological large scale structure. [PDF]
Durrer R.
europepmc +1 more source
Magnification serves as an independent and complementary gravitational lensing measurement to shear. We develop a novel method to achieve an accurate and robust magnification measurement around BOSS CMASS galaxies across physical scales of 0.016 h ^−1 ...
Kun Xu +4 more
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FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning. [PDF]
Kugel R +19 more
europepmc +1 more source
Spatial variations in survey properties due to selection effects generate substantial systematic errors in large-scale structure measurements in optical galaxy surveys on very large scales.
E.L. Gagnon +4 more
doaj +1 more source
Encoding Collective Knowledge, Instructing Data Reusers: The Collaborative Fixation of a Digital Scientific Data Set. [PDF]
Hoeppe G.
europepmc +1 more source
Supermassive Dark Star candidates seen by JWST. [PDF]
Ilie C, Paulin J, Freese K.
europepmc +1 more source
Detection of early-universe gravitational-wave signatures and fundamental physics. [PDF]
Caldwell R +37 more
europepmc +1 more source
Optimal cosmology from gravitational lensing: utilising the magnification and shear signals
Gravitational lensing studies the distortions of a distant galaxy’s observed size, shape or flux due to the tidal bending of photons by matter between the source and observer. Such distortions can be used to infer knowledge on the mass distribution of the intervening matter, such as the dark matter halos in which clusters of individual galaxies may ...
openaire +1 more source

