SJ
Shuowen Jin
astro-ph.GAastro-ph.COastro-ph.IMastro-ph.HE
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
Preprints & journals
118 papers in the corpus · 2014–2026CHAMPS: 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
The NIKA2 Cosmological Legacy Survey in COSMOS: Final 1.2mm and 2mm source catalogs and redshift distribution of dusty star-forming galaxies2605.00659v1 · C. R. Carvajal-Bohorquez, G. Lagache, A. Beelen et al.2026 · 0 citationsarXiv
Chaotic Molecular Gas in Five Dusty Star-forming Galaxies in the Spiderweb Protocluster at 2604.27071v1 · Jaclyn B. Champagne, Helmut Dannerbauer, Jose Manuel Perez-Martinez 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
The role of small-scale environments in the quenching of massive galaxies at 2604.11942v2 · Takumi Kakimoto, Masayuki Tanaka, Makoto Ando 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)
The ionised interstellar medium of DSFGs revealed by JWST/NIRSpec and ALMA: Super-solar metallicity, low ionisation parameters and, typical electron densities2602.18558v2 · Steven Gillman, DTU-Space, Kei Ito 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
Deblending the MIGHTEE-COSMOS survey with XID+: The resolved radio source counts to Jy2512.09290v2 · Eliab D. Malefahlo, Matt J. Jarvis, Mario G. Santos et al.2025 · 1 citationarXiv
JWST reveals extended stellar disks for ALMA-bright dusty star-forming galaxies in the Spiderweb protocluster2512.07050v1 · Y. H. Zhang, H. Dannerbauer, J. M. P'erez-Mart'inez et al.2025 · 4 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
Extended Components of Little Red Dots in the Rest-Frame Optical2510.25830v2 · Yiyang Zhang, Xuheng Ding, Lilan Yang et al.2025 · 3 citationsarXiv
Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.442510.23549v2 · Nikolaj B. Sillassen, Shuowen Jin, Georgios E. Magdis et al.2025 · 3 citationsarXiv
Ly-alpha emission reveals two satellite halos around massive groups at z ~ 3: the puzzling case of a quiescent central galaxy2510.01421v3 · Sicen Guo, Emanuele Daddi, Raphael Gobat et al.2025 · 0 citationsarXiv
Investigating the influence of radio-faint AGN activity on the infrared-radio correlation of massive galaxies2509.17536v2 · Giorgia Peluso, Ivan Delvecchio, Jack Radcliffe 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)
The Bigfoot: A footprint of a Coma cluster progenitor at z=3.982508.21356v2 · Hanwen Sun, Tao Wang, Emanuele Daddi et al.2025 · 6 citationsarXiv
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)
Avoiding (photo-) Catastrophe2507.01251v1 · A. J. Battisti, E. da Cunha, S. Jin et al.2025 · 2 citationsarXiv
COSMOS Web: Morphological quenching and size-mass evolution of brightest group galaxies from z = 3.72506.04031v2 · Ghassem Gozaliasl, Lilan Yang, Jeyhan Kartaltepe et al.2025 · 5 citationsA&A 703, A129 (2025)
COSMOS2025: The COSMOS-Web galaxy catalog of photometry, morphology, redshifts, and physical parameters from JWST, HST, and ground-based imaging2506.03243v1 · Marko Shuntov, Hollis B. Akins, Louise Paquereau et al.2025 · 53 citationsA&A 704, A339 (2025)
COSMOS-Web: Unraveling the Evolution of Galaxy Size and Related Properties at 2504.07185v1 · Lilan Yang, Jeyhan S. Kartaltepe, Maximilien Franco et al.2025 · 29 citationsarXiv
The COSMOS-Web Lens Survey (COWLS) I: Discovery of >100 high redshift strong lenses in contiguous JWST imaging2503.08777v2 · James Nightingale, Guillaume Mahler, Jacqueline McCleary et al.2025 · 13 citationsarXiv
The COSMOS-Web Lens Survey (COWLS) II: depth, resolution, and NIR coverage from JWST reveal 17 spectacular lenses2503.08782v1 · Guillaume Mahler, James W. Nightingale, Natalie B. Hogg et al.2025 · 5 citationsMon Not R Astron Soc Lett (2025) L8-L14
A merging pair of massive quiescent galaxies at in the Cosmic Vine2503.01953v1 · K. Ito, F. Valentino, M. Farcy et al.2025 · 18 citationsA&A 697, A111 (2025)
Gas outflows in two recently quenched galaxies at z = 4 and 72503.01990v3 · F. Valentino, K.E. Heintz, G. Brammer et al.2025 · 36 citationsA&A 699, A358 (2025)
Going deeper into the dark with COSMOS-Web: JWST unveils the total contribution of Radio-Selected NIRfaint galaxies to the cosmic Star Formation Rate Density2503.00112v1 · Fabrizio Gentile, Margherita Talia, Andrea Enia et al.2025 · 6 citationsA&A 697, A46 (2025)
COSMOS Spectroscopic Redshift Compilation (First Data Release): 488k Redshifts Encompassing Two Decades of Spectroscopy2503.00120v2 · Ali Ahmad Khostovan, Jeyhan S. Kartaltepe, Mara Salvato et al.2025 · 3 citationsarXiv
The COSMOS-Web ring: Spectroscopic confirmation of the background source at z = 5.12502.20136v1 · Marko Shuntov, Shuowen Jin, Wilfried Mercier et al.2025 · 8 citationsA&A 696, L14 (2025)
The COSMOS-Web deep galaxy group catalog up to 2501.09060v2 · Greta Toni, Ghassem Gozaliasl, Matteo Maturi et al.2025 · 13 citationsA&A 697, A197 (2025)
Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies2501.05288v2 · Malte Brinch, Shuowen Jin, Raphael Gobat et al.2025 · 6 citationsA&A 694, A218 (2025)
A multi-wavelength investigation of spiral structures in galaxies with JWST2501.03325v1 · Boris S. Kalita, Si-Yue Yu, John D. Silverman et al.2025 · 6 citationsarXiv
Clumps as multiscale structures in cosmic noon galaxies2501.03328v1 · Boris S Kalita, Tomoko L Suzuki, Daichi Kashino et al.2025 · 17 citationsMonthly Notices of the Royal Astronomical Society, Volume 536, Issue 3, January 2025, Pages 3090-3111
Hidden in Pixels. I. Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales2412.14246v3 · Takumi S. Tanaka, John D. Silverman, Kazuhiro Shimasaku et al.2024 · 4 citationsarXiv
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)
COALAS III: The ATCA CO(1-0) look at the growth and death of H emitters in the Spiderweb protocluster at z=2.162411.12138v1 · J. M. P'erez-Mart'inez, H. Dannerbauer, B. H. C. Emonts et al.2024 · 11 citationsA&A 696, A236 (2025)
ASWDF: Census of the obscured star formation in a galaxy cluster in formation at 2410.10169v1 · Y. H. Zhang, H. Dannerbauer, J. M. P'erez-Mart'inez et al.2024 · 12 citationsA&A 692, A22 (2024)
COSMOS-Web: stellar mass assembly in relation to dark matter halos across of cosmic history2410.08290v1 · M. Shuntov, O. Ilbert, S. Toft et al.2024 · 64 citationsA&A 695, A20 (2025)
Crimson Behemoth: a Massive Clumpy Structure Hosting a Dusty AGN at 2410.00104v1 · Takumi S. Tanaka, John D. Silverman, Yurina Nakazato et al.2024 · 7 citationsarXiv
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 in the COSMOS field2407.02973v2 · Nikolaj B. Sillassen, Shuowen Jin, Georgios E. Magdis et al.2024 · 17 citationsA&A 690, A55 (2024)
Quasars with Flare/Eclipse-like Variability Identified in ZTF2404.10245v1 · Zhiyuan Zheng, Yong Shi, Shuowen Jin et al.2024 · 1 citationarXiv
Cosmic evolution of radio-excess AGNs in quiescent and star-forming galaxies across 2401.04924v2 · Yijun Wang, Tao Wang, Daizhong Liu et al.2024 · 12 citationsA&A 685, A79 (2024)
Cosmic Vine: A z=3.44 large-scale structure hosting massive quiescent galaxies2311.04867v3 · Shuowen Jin, Nikolaj B. Sillassen, Georgios E. Magdis et al.2023 · 38 citationsarXiv
Characterisation of Herschel-selected strong lens candidates through HST and sub-mm/mm observations2311.01158v1 · Edoardo Borsato, Lucia Marchetti, Mattia Negrello et al.2023 · 0 citationsarXiv
DEIMOS spectroscopy of protocluster candidate in COSMOS -- A massive protocluster embedded in a large scale structure?2311.00511v3 · Malte Brinch, Thomas R. Greve, David B. Sanders et al.2023 · 19 citationsarXiv
Career total: 221 works. 118 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.