MF
Maximilien Franco
astro-ph.GAastro-ph.COastro-ph.IMastro-ph.HEastro-ph.SREarly universeGalaxies and clusters
On Valency
published · living versionsW_unu28bt7·v1 · currentpublished
Why a Multi-Cycle Treasury Program is Essential to Maximize JWST's Scientific Contributions to Galaxy Formation
with Genesis Community, Alice Shapley, Steven L. Finkelstein, Rachel S. Somerville +416
1 version
W_887b9nun·v1published
Preprints & journals
147 papers in the corpus · 2017–2026An Attenuation Bump at z=9.3: Probing Dust Diversity at Cosmic Dawn2610.20722v1 · Giulia Rodighiero, Santiago 'Alvarez-C'ordoba, Michele Catone et al.2026 · 0 citationsarXiv
Prevalence of radio Active Galactic Nuclei in galaxy groups since z=3.5 in the COSMOS-Web field2610.10719v1 · F. Ubertosi, I. Delvecchio, I. Prandoni et al.2026 · 0 citationsarXiv
Do Submillimeter Galaxies Trace Megaparsec Large-scale Structures? -- An Overdensity Analysis of 449 Submillimeter Galaxies in COSMOS2610.01136v1 · Canze Deng, Daizhong Liu, Helmut Dannerbauer et al.2026 · 0 citationsarXiv
X-ray Characterization of Galaxy Groups and Hickson Groups in COSMOS-Web to z~3.8 I. X-ray Luminosity Function Evolution2610.02470v1 · Ghassem Gozaliasl, Gunther Hasinger, Gavin Leroy et al.2026 · 0 citationsarXiv
COSMOS-3D: Diverse Environments and Hot-dust Signatures among Dusty Star-forming Galaxies at = 4.9-7.22609.35987v1 · Siwei Zou, Manuel Aravena, Shaoze Geng et al.2026 · 0 citationsarXiv
CHAMPS: The COSMOS High-Redshift ALMA-MIRI Population Survey - A New Census of the Dusty Early Universe2609.35992v1 · Andreas L. Faisst, Felix Martinez III, Jeyhan S. Kartaltepe et al.2026 · 0 citationsarXiv
CHAMPS: Data Reduction and Detection of ~3300 Dusty Galaxies at 1.2 mm2609.36076v1 · Felix Martinez III, Jeyhan S. Karaltepe, Andreas L. Faisst et al.2026 · 0 citationsarXiv
ALMA Chemical Evolution (ACE) survey: an overview -- extending dust and gas inference to low metallicities at cosmic noon2609.21604v1 · Irene Shivaei, Gergo Popping, Leindert A. Boogaard et al.2026 · 0 citationsarXiv
JWST Spectra Conclusively Show an Excess of Neutral Gas Outflows in Quiescent Galaxies at z=2-52609.09459v1 · Rion Oh, Gourav Khullar, Arianna S. Long et al.2026 · 0 citationsarXiv
JWST Reveals a Candidate Supermassive Black Hole Binary at z=4.3 in the Brightest Sub-millimeter Galaxy in COSMOS-Web2609.01711v1 · Jed McKinney, Ansh Gupta, Julian B. Munoz et al.2026 · 0 citationsarXiv
Resolved Dust in Galaxies with JWST/MIRI MRS: Survey Description and First View on PAHs, Mid-IR Atomic Emission, and Warm H2608.27560v2 · Wuji Wang, Andreas L. Faisst, Thomas S.-Y. Lai et al.2026 · 0 citationsarXiv
COSMOS-Web: From early star-formation enhancement to late suppression in galaxy groups2608.26348v2 · R. C. Arango-Toro, C. Laigle, J. Lewis et al.2026 · 0 citationsarXiv
The Extended Mapping Obscuration to Reionization with ALMA (Ex-MORA) Survey: A Molecular Gas Line Search2608.10165v2 · V. Cat'an, J. Gonz'alez-L'opez, M. Aravena et al.2026 · 0 citationsarXiv
COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies?2606.31978v1 · Louise Paquereau, Clotilde Laigle, Henry Joy McCracken et al.2026 · 0 citationsarXiv
Dust in the Average Galaxy: Attenuation, Emission, and Opacity from 2606.17270v2 · Caitlin M. Casey, Hollis B. Akins, Andrew J. Battisti et al.2026 · 1 citationarXiv
COSMOS-Web: A Multi-wavelength Morphological Catalog of ~780,000 Galaxies2606.14869v1 · Lilan Yang, Jeyhan S. Kartaltepe, Nicole E. Drakos et al.2026 · 0 citationsarXiv
Euclid: Disky titans - surprisingly high star formation activity and gas content in two brightest group galaxies at z~0.752606.02687v2 · F. Gentile, E. Daddi, D. Elbaz et al.2026 · 0 citationsarXiv
COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 m Since 2605.31415v1 · Si-Yue Yu, Andreas L. Faisst, Taotao Fang et al.2026 · 0 citationsarXiv
ODIN: Rest-frame Optical Morphologies and Star Formation Activity of Ly{\alpha} Emitters at z=2.4, 3.1, and 4.52605.29344v2 · Sang Hyeok Im, Ho Seong Hwang, Jeong Hwan Lee et al.2026 · 0 citationsarXiv
Quiescent fractions in high-redshift galaxy groups reflect their hot-or-cold state of gas accretion2604.22401v1 · Guillaume Elias, Emanuele Daddi, Chiara D'Eugenio et al.2026 · 0 citationsarXiv
Do little red dots really form a distinct class of astronomical objects?2604.11677v3 · Jean-Baptiste Billand, David Elbaz, Maximilien Franco et al.2026 · 0 citationsarXiv
Multi-wavelength morphology and dust emission in low-redshift dwarf galaxies in COSMOS-Web with HST and JWST2602.09085v1 · D. Kakkad, I. Lazar, S. Harish et al.2026 · 0 citationsarXiv
From Grism to IFU: Revising the Redshift and Nature of the Massive Dusty Galaxy S1 with JWST and ALMA2602.03030v1 · Mengyuan Xiao, Longji Bing, Gabriel Brammer et al.2026 · 0 citationsarXiv
An ultra-high-resolution map of (dark) matter2601.17239v1 · Diana Scognamiglio, Gavin Leroy, David Harvey et al.2026 · 5 citationsPublished in Nature Astronomy, 2026
Expanding the High-z Supernova Frontier: "Wide-Area" JWST Discoveries from the First Two Years of COSMOS-Web2601.08931v2 · Ori D. Fox (STSc), Armin Rest, JHU et al.2026 · 0 citationsarXiv
Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups2601.06297v1 · Z. Ghaffari (1, G. Gozaliasl (3, A. Biviano (1 et al.2026 · 1 citationarXiv
Through Thick and Thin: The Cosmic Evolution of Disk Scale Height2601.04988v2 · Si-Yue Yu, Luis C. Ho, Takafumi Tsukui et al.2026 · 5 citationsarXiv
The NIRISS PASSAGE Spectroscopic Redshift Catalog in COSMOS2601.02220v2 · Mason S. Huberty, Kalina V. Nedkova, Zahra Sattari et al.2026 · 1 citationarXiv
ALMA and JWST Identification of Faint Dusty Star-Forming Galaxies up to z~82512.16215v1 · Jorge A. Zavala, Andreas L. Faisst, Manuel Aravena et al.2025 · 0 citationsarXiv
From "The Cliff" to "Virgil": Mapping the Spectral Diversity of Little Red Dots with JWST/NIRSpec2512.15853v2 · Guillermo Barro, Pablo G. Perez-Gonzalez, Dale Kocevski et al.2025 · 5 citationsarXiv
Sparse by the River: Diverse Environments of z > 3 Massive Quiescent Galaxies2512.14881v1 · Nguyen Binh, Arianna S. Long, Jacqueline Antwi-Danso et al.2025 · 1 citationarXiv
THRILS -- The High-(Redshift+Ionization) Line Search: Program Description & Redshift Catalog2512.12509v1 · Taylor A. Hutchison, Rebecca L. Larson, Pablo Arrabal Haro et al.2025 · 0 citationsarXiv
Large-Scale Structure in COSMOS-Web: Tracing Galaxy Evolution in the Cosmic Web up to with the Largest JWST Survey2511.10727v1 · Hossein Hatamnia, Bahram Mobasher, Sina Taamoli et al.2025 · 1 citationarXiv
An almost NIRCam-dark dusty star-forming galaxy at z=6.632511.08672v1 · Longji Bing, Seb Oliver, Mengyuan Xiao et al.2025 · 1 citationMon Not R Astron Soc (2026)
The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web2511.05259v1 · Marko Shuntov, Olivier Ilbert, Claudia del P. Lagos et al.2025 · 3 citationsarXiv
Probing the dawn of galaxies: star formation and feedback in the JWST era through the GAEA model2511.03787v1 · Sebastiano Cantarella, Gabriella De Lucia, Fabio Fontanot et al.2025 · 0 citationsarXiv
Euclid Quick Data Release (Q1). Quenching precedes bulge formation in dense environments but follows it in the field2511.02964v2 · F. Gentile, E. Daddi, D. Elbaz et al.2025 · 0 citationsarXiv
Extended Components of Little Red Dots in the Rest-Frame Optical2510.25830v2 · Yiyang Zhang, Xuheng Ding, Lilan Yang et al.2025 · 3 citationsarXiv
Formation of Substructure in Luminous Submillimeter Galaxies (FOSSILS): Evidence of Multiple Pathways to Trigger Starbursts in Luminous Submillimeter Galaxies2510.18006v2 · Ryota Ikeda, Daisuke Iono, Ken-ichi Tadaki et al.2025 · 4 citationsThe Astrophysical Journal, Volume 996, Issue 2, id.121, 17 pp. (2026)
The ALPINE-CRISTAL-JWST Survey: JWST/IFU Optical Observations for 18 Main-Sequence Galaxies at z=4-62510.16111v2 · A. L. Faisst, S. Fujimoto, A. Tsujita et al.2025 · 11 citationsarXiv
The ALPINE-CRISTAL-JWST Survey: NIRSpec IFU Data Processing and Spatially-resolved Views of Chemical Enrichment in Normal Galaxies at z=4-62510.16116v1 · Seiji Fujimoto, Andreas L. Faisst, Akiyoshi Tsujita et al.2025 · 3 citationsarXiv
The Stellar Morphology & Size of X-ray-selected Active Galactic Nuclei Host Galaxies Revealed by JWST2510.13719v2 · Bovornpratch Vijarnwannaluk, Zhen-Kai Gao, Wei-Hao Wang et al.2025 · 0 citationsarXiv
Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot2509.09607v1 · Erini Lambrides, Rebecca Larson, Taylor Hutchison et al.2025 · 0 citationsarXiv
COSMOS-Web galaxy groups: Evolution of red sequence and quiescent galaxy fraction2509.08040v2 · Greta Toni, Matteo Maturi, Gianluca Castignani et al.2025 · 6 citationsA&A 707, A87 (2026)
Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution (PASSAGE): Survey Overview2509.00596v1 · Matthew A. Malkan, Vihang Mehta, Ayan Acharyya et al.2025 · 4 citationsarXiv
JWST+ALMA reveal the ISM kinematics and stellar structure of MAMBO-9, a merging pair of DSFGs in an overdense environment at 2508.06607v1 · Hollis B. Akins, Caitlin M. Casey, Jaclyn B. Champagne et al.2025 · 1 citationarXiv
Physical properties of galaxies and the UV Luminosity Function from to in COSMOS-Web2508.04791v1 · Maximilien Franco, Caitlin M. Casey, Hollis B. Akins et al.2025 · 1 citationarXiv
Discovery of a Little Red Dot candidate at in COSMOS-Web based on MIRI-NIRCam selection2508.00057v2 · Takumi S. Tanaka, Hollis B. Akins, Yuichi Harikane et al.2025 · 1 citationarXiv
Investigating the Growth of Little Red Dot Descendants at z<4 with the JWST2507.04011v2 · Jean-Baptiste Billand, David Elbaz, Fabrizio Gentile et al.2025 · 6 citationsarXiv
Clumpiness of galaxies revealed in the near-infrared with COSMOS-Web2506.13881v1 · Wilfried Mercier, Boris Sindhu Kalita, Marko Shuntov et al.2025 · 3 citationsarXiv
Career total: 252 works. 147 are in this corpus.Showing the 50 most recent.
Profile built from the corpus for this byline.
Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.