Results 41 to 50 of about 15,815 (162)
We present JWST NIRCam nine-band near-infrared imaging of the luminous z = 10.6 galaxy GN-z11 from the JWST Advanced Deep Extragalactic Survey of the GOODS-N field.
Sandro Tacchella +47 more
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We build upon the state-of-the-art semianalytic model FEGA24 for the formation and evolution of galaxies, which integrates the latest prescriptions relevant to galaxy formation and evolution, alongside a comprehensive active galactic nuclei (AGN ...
Emanuele Contini +3 more
doaj +1 more source
We present an analysis of the quenching of star formation in massive galaxies ( M _* > 10 ^9.5 M _⊙ ) within the first 0.5–3 Gyr of the Universe’s history utilizing JWST-CEERS data.
Asa F. L. Bluck +12 more
doaj +1 more source
Suppression of Star Formation in Galaxy Pairs
We investigate the suppression of star formation in galaxy pairs based on the isolated galaxy pair sample derived from the Sloan Digital Sky Survey survey.
Shuai Feng +5 more
doaj +1 more source
Inside‐out Galaxy Formation [PDF]
21 pages including 6 ...
openaire +2 more sources
PAC. V. The Roles of Mass and Environment in the Quenching of Galaxies
The roles that mass and environment play in galaxy quenching are still under debate. Leveraging the Photometric objects Around Cosmic webs method, we analyze the excess surface distribution ${\bar{n}}_{2}{w}_{{\rm{p}}}({r}_{{\rm{p}}})$ of photometric ...
Yun Zheng +8 more
doaj +1 more source
Using JWST observations in CANDELS fields, we measure the half-light radius ( r _e,light ) and half-mass–radius ( r _e,mass ) for 14,333 galaxies with stellar masses M _* > 10 ^9 M _⊙ at redshifts 0.2 1, though a slight decreasing trend is seen between
Mingen Xin +5 more
doaj +1 more source
We present an overview and first results from the Spectroscopic Ultradeep Survey Probing Extragalactic Near-infrared Stellar Emission (SUSPENSE), executed with NIRSpec on JWST.
Martje Slob +21 more
doaj +1 more source
On the Signature of Black Holes on the Quenched Stellar Mass Function
As star-forming galaxies approach or exceed a stellar mass of around 10 ^11 M _⊙ , they are increasingly likely to be quenched in a process generically called mass quenching.
Antonio J. Porras-Valverde +1 more
doaj +1 more source
Star formation quenching in galaxies plays a crucial role in galaxy evolution and is believed to be driven primarily by galaxy mass and environment.
Yun Zheng +6 more
doaj +1 more source

