302 citations · 6.5k across the 129 of their papers we have counts for
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Blue Monsters at . Where has all their dust gone?
A. Ferrara, A. Pallottini, L. Sommovigo
The properties of luminous, blue (a.k.a. Blue Monsters), super-early galaxies at redshift have been successfully explained by the attenuation-free model (AFM) in which dust…
Accurate Simultaneous Constraints on the Dust Mass, Temperature and Emissivity Index of a Galaxy at Redshift 7.31
Hiddo Algera, Hanae Inami, Ilse De Looze +21
We present new multi-frequency ALMA continuum observations of the massive [], UV-luminous [] $z=7.31…
The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
A. Pallottini, A. Ferrara, S. Gallerani +5
Galaxy evolution emerges from the balance between cosmic gas accretion, fueling star formation, and supernova (SN) feedback, regulating the metal enrichment. Hence, the stellar mas…
Investigating the ultraviolet and infrared radiation through the turbulent life of molecular clouds
Fabio Di Mascia, Andrea Pallottini, Laura Sommovigo +1
Context. Molecular Clouds (MCs) are the place where stars are formed and their feedback starts to take place, regulating the evolution of galaxies. Therefore, MCs represent the cri…
REBELS-25: Discovery of a dynamically cold disc galaxy at z = 7.31
Lucie E. Rowland, Jacqueline Hodge, Rychard Bouwens +21
We present high resolution (" = 710 pc) ALMA [CII] 158m and dust continuum follow-up observations of REBELS-25, a [CII]-luminous ($L_{\mathrm{[CII]}}=(1.7\pm0.2)\times…
An optically-dark merging system at z~6 detected by JWST
Giulia Rodighiero, Andrea Enia, Laura Bisigello +16
Near- to mid-Infrared observations (from Spitzer and JWST) have revealed a hidden population of galaxies at redshift z=3-6, called optically-dark objects, which are believed to be…
Gas-phase metallicity gradients in galaxies at
G. Venturi, S. Carniani, E. Parlanti +18
The study of gas-phase metallicity and its spatial distribution at high redshift is crucial to understand the processes that shaped the growth and evolution of galaxies in the earl…
Unveiling [CII] clumps in a lensed star-forming galaxy at z ~ 3.4
A. Zanella, E. Iani, M. Dessauges-Zavadsky +15
Observations at UV and optical wavelengths have revealed that galaxies at z~1-4 host star-forming regions, dubbed "clumps", which are believed to form due to the fragmentation of g…
Time evolution of the galactic relation: the impact of the magnetic field morphology
A. Konstantinou, E. Ntormousi, K. Tassis +1
One of the most frequently used indicators to characterize the magnetic field's influence on star formation is the relation between magnetic field strength and gas density ( r…
Primordial Rotating Disk Composed of 15 Dense Star-Forming Clumps at Cosmic Dawn
S. Fujimoto, M. Ouchi, K. Kohno +43
Early galaxy formation, initiated by the dark matter and gas assembly, evolves through frequent mergers and feedback processes into dynamically hot, chaotic structures. In contrast…
Dust attenuation evolution in - JWST galaxies
V. Markov, S. Gallerani, A. Ferrara +5
A sizable fraction of the heavy elements synthesized by stars in galaxies condenses into sub-micron-sized solid-state particles, known as dust grains. Dust produces a wavelength-de…