Extremely Large Telescope: publications

The WISDOM of power spectra: how the galactic gravitational potential impacts a galaxy's central gas reservoir in simulations and observations

(2023)

Authors:

Jindra Gensior, Timothy A Davis, Martin Bureau, JM Diederik Kruijssen, Michele Cappellari, Ilaria Ruffa, Thomas G Williams

Continuous daytime and nighttime forecast of atmospheric optical turbulence from numerical weather prediction models.

Optics Express Optica Publishing Group 31:21 (2023) 33850-33872

Authors:

Florian Quatresooz, Ryan Griffiths, Lisa Bardou, Richard Wilson, James Osborn, Danielle Vanhoenacker-Janvier, Claude Oestges

INFUSE: preflight performance of a rocket-borne FUV integral field spectrograph

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 12678 (2023) 1267808-1267808-12

Authors:

Emily M Witt, Brian T Fleming, James C Green, Kevin France, Alex Haughton, Dana Chafetz, Jack Williams, Takashi Sukegawa, Oswald Siegmund, Matthias Tecza

INSPIRE: INvestigating Stellar Population In RElics V. A catalogue of ultra-compact massive galaxies outside the local Universe and their degree of relicness

(2023)

Authors:

C Spiniello, G D'Ago, L Coccato, J Hartke, C Tortora, A Ferré-Mateu, C Pulsoni, M Cappellari, M Maksymowicz-Maciata, M Arnaboldi, D Bevacqua, A Gallazzi, LK Hunt, F La Barbera, I Martín-Navarro, NR Napolitano, M Radovich, P Saracco, D Scognamiglio, M Spavone, S Zibetti

The JWST Hubble Sequence: The Rest-frame Optical Evolution of Galaxy Structure at 1.5 < z < 6.5

The Astrophysical Journal American Astronomical Society 955:2 (2023) 94-94

Authors:

Leonardo Ferreira, Christopher J Conselice, Elizaveta Sazonova, Fabricio Ferrari, Joseph Caruana, Clár-Bríd Tohill, Geferson Lucatelli, Nathan Adams, Dimitrios Irodotou, Madeline A Marshall, Will J Roper, Christopher C Lovell, Aprajita Verma, Duncan Austin, James Trussler, Stephen M Wilkins

Abstract:

© 2023. The Author(s). Published by the American Astronomical Society. This is an open access article distributed under the Creative Commons Attribution License, to view a copy of the license, see: https://creativecommons.org/licenses/by/4.0/We present results on the morphological and structural evolution of a total of 3956 galaxies observed with JWST at 1.5 109 M ⊙ at z > 3 are not dominated by irregular and peculiar structures, either visually or quantitatively, as previously thought. We find a strong dominance of morphologically selected disk galaxies up to z = 6 in this mass range. We also find that the stellar mass and star formation rate densities are dominated by disk galaxies up to z ∼ 6, demonstrating that most stars in the Universe were likely formed in a disk galaxy. We compare our results to theory to show that the fraction of types we find is predicted by cosmological simulations, and that the Hubble Sequence was already in place as early as one billion years after the Big Bang. Additionally, we make our visual classifications public for the community.Peer reviewe

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