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Evolution and Mass Dependence of UV-to-near-IR Color Gradients up to z=2.5 from HST+JWST
Marco Martorano, Arjen van der Wel, Andrea Gebek +7
We present the redshift evolution of radial color gradients (in rest-frame and ) for galaxies in the range z $<2.5…
Episodic Star Formation -- I. Overview and Scatter of the Star-Forming Main Sequence
Yuqian Gui, Dandan Xu, Haoyi Wang +4
Episodic star formation cycles in both high- and low-redshift galaxies have gained more and more evidence. This paper aims to understand the detailed physical processes behind such…
SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars
Steven Ramnichal, Junkai Zhang, Stijn Wuyts +1
We present a framework for analysing panchromatic and spatially resolved galaxy observations, dubbed SE3D. SE3D simultaneously and self-consistently models a galaxy's spectral ener…
SE3D: Testing the recovery of stellar population, dust and structural properties on mock-observed toy model and simulated galaxies
Junkai Zhang, Steven Ramnichal, Stijn Wuyts +1
The translation from direct observables to physical properties of galaxies is a key step in reconstructing their evolutionary histories. Star-dust geometry and inhomogeneous stella…
Resolving stellar populations, star formation, and interstellar medium conditions with JWST in a large spiral galaxy at
Eleonora Parlanti, Giulia Tozzi, Natascha M. Förster Schreiber +30
Cosmic noon represents the prime epoch of galaxy assembly, and a sweet spot for observations with the James Webb Telescope (JWST) and ground-based near-IR integral-field unit (IFU)…
The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings
Alberto Torralba, Jorryt Matthee, Gabriele Pezzulli +22
The population of the Little Red Dots (LRDs) may represent a key phase of supermassive black hole (SMBH) growth. A cocoon of dense excited gas is emerging as key component to expla…