Results 101 to 110 of about 2,186 (186)
JWST observations of galaxies at z ≳ 8 suggest that they are more luminous and clumpier than predicted by most models, prompting several proposals on the physics of star formation and feedback in the first galaxies. In this paper, we focus on the role of
Kazuyuki Sugimura +4 more
doaj +1 more source
Impact of stellar population models on the estimated physical properties of galaxies
Context. Accurate estimates of fundamental physical properties of galaxies, such as star formation rates (SFRs) or stellar masses, are essential for testing and constraining models of galaxy formation and evolution.
Stoyanova Bozhidara +7 more
doaj +1 more source
MAMMOTH-Subaru. III. Lyα Halo Identified by Stacking ∼3300 Lyα Emitters at z = 2.2–2.3
In this paper, we present a Ly α halo (LAH) identified by stacking ∼3300 Ly α emitters (LAEs) at z = 2.2–2.3. We carry out imaging observations and data reduction with Subaru/Hyper Suprime-Cam.
Haibin Zhang +10 more
doaj +1 more source
On the Very Bright Dropouts Selected Using the James Webb Space Telescope NIRCam Instrument
The selection of candidate high-redshift galaxies using the dropout technique targeting the Lyman-break signature sometimes yields very bright objects that are too luminous to be easily explained if they are indeed at the expected redshifts.
Bangzheng Sun, Haojing Yan
doaj +1 more source
Properties of High Redshift Galaxies
I review the characteristics of high redshift galaxies, with particular attention to the effects of dust obscuration on the observed light. Galaxies at redshift z~1 and at z>2 are discussed separately, as the accessible information for each redshift range are different.
openaire +2 more sources
Stellar feedback drives the baryon deficiency in low-mass galaxies. [PDF]
Yu H +10 more
europepmc +1 more source
The era of precision cosmology with voids. [PDF]
Contarini S, Verza G, Pisani A.
europepmc +1 more source
Galaxy Evolution with Manifold Learning. [PDF]
Takeuchi TT, Cooray S, Kano RR.
europepmc +1 more source
Formation time-scales for stellar bars in diverse galactic discs. [PDF]
Frosst M, Obreschkow D, Ludlow A.
europepmc +1 more source
An X-ray-emitting protocluster at z ≈ 5.7 reveals rapid structure growth. [PDF]
Bogdán Á +3 more
europepmc +1 more source

