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
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
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
Origins and lifetimes of secular and tidal bars in simulated disc galaxies. [PDF]
Frosst M +3 more
europepmc +1 more source
A rising tide: intrinsic alignments since the turn of the millennium. [PDF]
Chisari NE.
europepmc +1 more source
Unsupervised multimodal deep learning for galaxy morphology taxonomy: integrating ConvNeXtEmbeddings and morphological parameters for scalable survey science. [PDF]
Selim IM +3 more
europepmc +1 more source
The emergence of globular clusters and globular-cluster-like dwarfs. [PDF]
Taylor ED +9 more
europepmc +1 more source

