Results 1 to 10 of about 16,812 (242)
In this paper, we present the Heavy Metal Survey, which obtained ultradeep medium-resolution spectra of 21 massive quiescent galaxies at 1.3 < z < 2.3 with Keck/LRIS and MOSFIRE.
Mariska Kriek +16 more
doaj +1 more source
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
doaj +1 more source
We build upon FEGA25 , a previously introduced semianalytic model (SAM) for galaxy formation and evolution, by focusing on its enhanced treatment of supernova (SN) and active galactic nucleus (AGN) feedback mechanisms.
Emanuele Contini +4 more
doaj +1 more source
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
Co-evolution of the Milky Way high- and low-α sequences with chemical evolution models
Context. Observational data have revealed a clear dichotomy in the [α/Fe] versus [Fe/H] diagram of the Milky Way thick and thin disc stars. Many recent studies have shown evidence of a co-evolution phase between the high- and low-α disc sequences as well
Grisoni V., Spitoni E., Matteucci F.
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
The Parameter Space of Galaxy Formation
Semi-analytic models are a powerful tool for studying the formation of galaxies. However, these models inevitably involve a significant number of poorly constrained parameters that must be adjusted to provide an acceptable match to the observed Universe. In this paper, we set out to quantify the degree to which observational data sets can constrain the
Bower, R. G. +7 more
openaire +3 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

