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Profil bibliographique

Mengyuan Xiao

Informations fournies par OpenAlex. Research Africa ne déduit ni nationalité, ni poste, ni coordonnées personnelles.

3Publications signalées
0Citations signalées
0Affiliations récentes

Les domaines associés

Galaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysical ResearchAstrophysics and Star Formation StudiesAstrophysical Phenomena and ObservationsSpace Technology and Applications

Les publications récentes

Accès ouvert 2026 preprint OpenAlex

A Census of the 200 Most Massive Galaxies Spectroscopically Observed with JWST at zspec $\sim$3-15

Mengyuan Xiao, Pascal A. Oesch, Longji Bing, Rashmi Gottumukkala et autres

Massive galaxies provide strong tests of galaxy formation models, yet a comprehensive spectroscopic view of their properties and demographics in the early Universe has remained elusive. Here we present a JWST spectroscopic census of the 200 most massive galaxies at zspec~3-15, selected …

0 citations arXiv (Cornell University)
Accès ouvert 2026 preprint OpenAlex

Little Red Dots as Intermediate Mass, Super-Eddington Engines: Insights from Type IIn Supernovae and The 1837-1856 Great Eruption of $η$ Carinae

Rohan P. Naidu, Jorryt Matthee, Anna de Graaff, Alberto Torralba et autres

JWST's Little Red Dots (LRDs) display a unique constellation of features that do not occur simultaneously in any other class of galaxies or AGN. Here we observe that many of these features find parallels in the 19th century Great Eruption (GE) of …

0 citations arXiv (Cornell University)
Accès ouvert 2026 preprint OpenAlex

JWST spectroscopy of galaxies at $z>10$: Damped Ly$α$ absorbers reveal efficient star formation and hidden redshift biases

Kasper E. Heintz, C L Pollock, Joris Witstok, R Bouwens et autres

Recent observations with JWST have revealed a remarkable population of surprisingly luminous galaxies at redshifts $z>10$. Their abundance exceed predictions from simulations and empirical extrapolations from lower redshifts, suggesting a transition in the physical conditions under which the first stars formed. Here …

0 citations arXiv (Cornell University)

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