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B. Magnelli

0000-0002-6777-6490
astro-ph.GAastro-ph.COastro-ph.IMastro-ph.HEastro-phastro-ph.SRastro-ph.EPcluster galaxiescosmologygalaxy formation

On Valency

published · living versions
W_2b646ueg·v1 · currentpublished
Molecular Gas, Dust and Star Formation in Galaxies: II. Dust properties and scalings in \sim\ 1600 nearby galaxies
with G. Orellana, N. M. Nagar D. Elbaz, P. Calderón-Castillo, R. Leiton +5
1 version
W_tx7xf8wu·v1published
GOODS-Herschel: an infrared main sequence for star-forming galaxies

Preprints & journals

229 papers in the corpus · 2008–2026
Sleeping or Dead? Probing the Quenching Mechanism of JWST Dormant Galaxies at z > 3 with ALMA2610.19926v1 · Mengyuan Xiao, Songnan Qi, Pascal A. Oesch 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
Resolved SED modelling with JWST and ALMA: the role of stellar mass surface density in regulating star formation in cosmic noon galaxies2609.12059v2 · Cheng-Lin Liao, Leindert A. Boogaard, Jacqueline A. Hodge et al.2026 · 0 citationsarXiv
The Atacama Large Aperture Submillimeter Telescope (AtLAST): enabling large-scale sub-mm science beyond 20302607.05022v1 · Claudia Cicone, Tony Mroczkowski, Evanthia Hatziminaoglou et al.2026 · 0 citationsarXiv
A Census of the 200 Most Massive Galaxies Spectroscopically Observed with JWST at zspec $\sim$3-152606.30802v1 · Mengyuan Xiao, Pascal A. Oesch, Longji Bing et al.2026 · 0 citationsarXiv
The quasi-star model for Little Red Dots: potential and challenges2606.06575v2 · Fabrizio Gentile, Mauro Giavalisco, Emanuele Daddi 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
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
A first [CII] view of high-z quiescent galaxies2604.09347v1 · C. D'Eugenio, E. Daddi, R. Gobat et al.2026 · 1 citationarXiv
ULTIMATE-deblending I. A 50-band Ultraviolet to Mid-infrared Photometric Catalog Combining Space- and Ground-based Data in the JWST/PRIMER survey2603.05289v4 · Hanwen Sun, Tao Wang, Ke Xu et al.2026 · 2 citationsApJS 285 1 (2026)
Starbursts hiding in the main sequence: a pathway toward quenching?2602.23445v3 · Florent Renaud, Katarina Kraljic, Jonathan Freundlich 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
Stellar Morphology of Optically Dark or Faint Galaxies at z>3z>3 with JWST2512.15127v2 · Arpita Ganguly, Mengyuan Xiao, Pascal A. Oesch et al.2025 · 0 citationsarXiv
What Builds and Quenches the Most Massive Galaxies in the Early Universe?2512.15836v1 · Mengyuan Xiao, Longji Bing, Guilaine Lagache et al.2025 · 0 citationsarXiv
ECOGAL I. Project design and the first catalogue2511.20751v1 · Minju M. Lee, Georgios Magdis, Gabriel Brammer et al.2025 · 0 citationsarXiv
The observed total star formation rate function up to z \sim 6: complementary UV and IR contributions and comparison with state-of-the-art galaxy formation models2511.13828v1 · A. Traina, C. Gruppioni, I. Delvecchio et al.2025 · 0 citationsarXiv
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)
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
Active galactic nuclei-heated dust revealed in "little red dots"2509.07100v4 · I. Delvecchio, E. Daddi, B. Magnelli et al.2025 · 13 citationsA&A 704, A313 (2025)
A3^3COSMOS: The dust content of massive quiescent galaxies and its evolution with cosmic time2508.18097v2 · Sylvia Adscheid, Benjamin Magnelli, Laure Ciesla et al.2025 · 4 citationsA&A 702, A186 (2025)
Noema formIng Cluster survEy (NICE): A Census of Star Formation and Cold Gas Properties in Massive protoclusters at 1.5<z<42507.09971v3 · Luwenjia Zhou, Tao Wang, Emanuele Daddi et al.2025 · 1 citationA&A 701, A234 (2025)
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
PANORAMIC: Discovery of an Ultra-Massive Grand-Design Spiral Galaxy at z∼5.2z\sim5.22412.13264v2 · Mengyuan Xiao, Christina C. Williams, Pascal A. Oesch et al.2024 · 16 citationsA&A 696, A156 (2025)
Behind the dust veil: A panchromatic view of an optically dark galaxy at z=4.822412.09363v1 · Nikolaj B. Sillassen, Shuowen Jin, Georgios E. Magdis et al.2024 · 5 citationsA&A 693, A309 (2025)
Dust emission from the bulk of galaxies at the Epoch of Reionization2412.02557v1 · L. Ciesla, S. Adscheid, B. Magnelli et al.2024 · 6 citationsA&A 700, A277 (2025)
In situ spheroid formation in distant submillimetre-bright galaxies.39633191 · Tan, Qing-Hua, Daddi, Emanuele, Magnelli, Benjamin et al.2024 · 17 citationsNature. 2024;636(8041):69-74
Compact dust-obscured star-formation and the origin of the galaxy bimodality2411.00279v2 · Maxime Tarrasse, Carlos G'omez-Guijarro, David Elbaz et al.2024 · 2 citationsA&A 697, A181 (2025)
Accelerated formation of ultra-massive galaxies in the first billion years.39537883 · Xiao, Mengyuan, Oesch, Pascal A, Elbaz, David et al.2024 · 93 citationsNature. 2024;635(8038):311-315
[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST II. CO foreground masking based on an external catalog2410.17330v1 · C. Karoumpis, B. Magnelli, E. Romano-D'iaz et al.2024 · 0 citationsarXiv
In-Situ Spheroid Formation in Distant Submillimeter-Bright Galaxies2407.16578v2 · Qing-Hua Tan, Emanuele Daddi, Benjamin Magnelli et al.2024 · 0 citationsarXiv
A3^3COSMOS: the dust mass function and dust mass density at 0.5<z<60.5<z<62407.09607v1 · A. Traina, B. Magnelli, C. Gruppioni et al.2024 · 10 citationsA&A 690, A84 (2024)
A photo-z cautionary tale: Redshift confirmation of COSBO-7 at z=2.6252407.07585v2 · Shuowen Jin, Nikolaj B. Sillassen, Jacqueline Hodge et al.2024 · 21 citationsA&A 690, L16 (2024)
NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at 1.5<z<41.5 < z < 4 in the COSMOS field2407.02973v2 · Nikolaj B. Sillassen, Shuowen Jin, Georgios E. Magdis et al.2024 · 17 citationsA&A 690, A55 (2024)
AtLAST Science Overview Report2407.01413v2 · Mark Booth, Pamela Klaassen, Claudia Cicone et al.2024 · 4 citationsarXiv
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Surveying the distant Universe.39403450 · van Kampen, Eelco, Bakx, Tom, De Breuck, Carlos et al.2026 · 14 citationsOpen research Europe. 2024;4:122
PRIMER: JWST/MIRI reveals the evolution of star-forming structures in galaxies at z<2.52406.11571v2 · Yipeng Lyu, Benjamin Magnelli, David Elbaz et al.2024 · 9 citationsA&A 693, A313 (2025)
A3^3COSMOS: Measuring the cosmic dust-attenuated star formation rate density at 4<z<54 < z < 52405.18086v1 · Benjamin Magnelli, Sylvia Adscheid, Tsan-Ming Wang et al.2024 · 11 citationsA&A 688, A55 (2024)
[CII] luminosity models and large-scale image cubes based on COSMOS 2020 and ALPINE-ALMA [CII] data back to the epoch of reionisation2404.05352v3 · J. Clarke, C. Karoumpis, D. Riechers et al.2024 · 3 citationsA&A 689, A101 (2024)
Strong spectral features from asymptotic giant branch stars in distant quiescent galaxies2403.07414v4 · Shiying Lu, Emanuele Daddi, Claudia Maraston et al.2024 · 15 citations2024, oct
A3^3COSMOS and A3^3GOODSS: Continuum Source Catalogues and Multi-band Number Counts2403.03125v2 · Sylvia Adscheid, Benjamin Magnelli, Daizhong Liu et al.2024 · 28 citationsA&A, 685, A1 (2024)
Fitting pseudo-Seˊ{\rm \acute{e}}rsic(Spergel) light profiles to galaxies in interferometric data: the excellence of the uvuv-plane2312.05425v1 · Qing-Hua Tan, Emanuele Daddi, Victor de Souza Magalhaes et al.2023 · 0 citationsarXiv
Measuring the gas reservoirs in 108<10^{8}< M⋆<1011_\star<10^{11} M⊙_\odot galaxies at 1≤z≤31\leq z\leq32311.16279v2 · Rosa M. M'erida, Carlos G'omez-Guijarro, Pablo G. P'erez-Gonz'alez et al.2023 · 2 citationsA&A 686, A64 (2024)
A3^{3}COSMOS: Dissecting the gas content of star-forming galaxies across the main sequence at 1.2 ≤z\leq z < 1.62311.11832v1 · Tsan-Ming Wang, Benjamin Magnelli, Eva Schinnerer et al.2023 · 0 citationsarXiv
Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z=3.952310.15925v2 · Luwenjia Zhou, Tao Wang, Emanuele Daddi et al.2023 · 17 citationsA&A, 684, A196 (2024)
CEERS: 7.7 μ{\mu}m PAH Star Formation Rate Calibration with JWST MIRI2310.07766v2 · Kaila Ronayne, Casey Papovich, Guang Yang et al.2023 · 14 citationsarXiv
Identification of a transition from stochastic to secular star formation around z=9z=9 with JWST2309.15720v1 · L. Ciesla, D. Elbaz, O. Ilbert et al.2023 · 64 citationsA&A 686, A128 (2024)
A3^3COSMOS: the infrared luminosity function and dust-obscured star formation rate density at 0.5<z<60.5<z<62309.15150v1 · A. Traina, C. Gruppioni, I. Delvecchio et al.2023 · 1 citationarXiv
JWST/CEERS sheds light on dusty star-forming galaxies: forming bulges, lopsidedness and outside-in quenching at cosmic noon2307.07599v3 · Aurelien Le Bail, Emanuele Daddi, David Elbaz et al.2023 · 32 citationsA&A 688, A53 (2024)
CEERS: MIRI deciphers the spatial distribution of dust-obscured star formation in galaxies at 0.1<z<2.50.1<z<2.52305.19331v2 · Benjamin Magnelli, Carlos G'omez-Guijarro, David Elbaz et al.2023 · 27 citationsA&A 678, A83 (2023)
Career total: at least 459 works. 229 are in this corpus.Showing the 50 most recent.

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