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相关论文: Cosmic Evolution Early Release Science (CEERS) sur…

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We present an investigation into the first 500 Myr of galaxy evolution from the Cosmic Evolution Early Release Science (CEERS) survey. CEERS, one of 13 JWST ERS programs, targets galaxy formation from z~0.5 to z>10 using several imaging and…

We present the Cosmic Evolution Early Release Science (CEERS) Survey, a 77.2 hour Director's Discretionary Early Release Science Program. CEERS demonstrates, tests, and validates efficient extragalactic surveys using coordinated,…

星系天体物理 · 物理学 2025-01-09 Steven L. Finkelstein , Micaela B. Bagley , Pablo Arrabal Haro , Mark Dickinson , Henry C. Ferguson , Jeyhan S. Kartaltepe , Dale D. Kocevski , Anton M. Koekemoer , Jennifer M. Lotz , Casey Papovich , Pablo G. Perez-Gonzalez , Nor Pirzkal , Rachel S. Somerville , Jonathan R. Trump , Guang Yang , L. Y. Aaron Yung , Adriano Fontana , Andrea Grazian , Norman A. Grogin , Lisa J. Kewley , Allison Kirkpatrick , Rebecca L. Larson , Laura Pentericci , Swara Ravindranath , Stephen M. Wilkins , Omar Almaini , Ricardo O. Amorin , Guillermo Barro , Rachana Bhatawdekar , Laura Bisigello , Madisyn Brooks , Fernando Buitrago , Antonello Calabro , Marco Castellano , Yingjie Cheng , Nikko J. Cleri , Justin W. Cole , M. C. Cooper , Olivia R. Cooper , Luca Costantin , Isa G. Cox , Darren Croton , Emanuele Daddi , Kelcey Davis , Avishai Dekel , David Elbaz , Vital Fernandez , Seiji Fujimoto , Giovanni Gandolfi , Jonathan P. Gardner , Eric Gawiser , Mauro Giavalisco , Carlos Gomez-Guijarro , Yuchen Guo , Ansh R. Gupta , Nimish P. Hathi , Santosh Harish , Aurelien Henry , Michaela Hirschmann , Weida Hu , Taylor A. Hutchison , Kartheik G. Iyer , Anne E. Jaskot , Saurabh W. Jha , Intae Jung , Vasily Kokorev , Peter Kurczynski , Gene C. K. Leung , Mario Llerena , Arianna S. Long , Ray A. Lucas , Shiying Lu , Elizabeth J. McGrath , Daniel H. McIntosh , Emiliano Merlin , Alexa M. Morales , Lorenzo Napolitano , Fabio Pacucci , Viraj Pandya , Marc Rafelski , Giulia Rodighiero , Caitlin Rose , Paola Santini , Lise-Marie Seille , Raymond C. Simons , Lu Shen , Amber N. Straughn , Sandro Tacchella , Brittany N. Vanderhoof , Jesus Vega-Ferrero , Benjamin J. Weiner , Christopher N. A. Willmer , Peixin Zhu , Eric F. Bell , Stijn Wuyts , Benne W. Holwerda , Xin Wang , Weichen Wang , Jorge A. Zavala

Low mass (sub)stellar objects represent the low end of the initial mass function, the transition to free-floating planets and a prominent interloper population in the search for high-redshift galaxies. Without proper motions or…

Numerous high-$z$ galaxies have recently been observed with JWST, providing new insights into early galaxy evolution. Their physical properties are typically derived through spectral energy distribution (SED) fitting, but the reliability of…

星系天体物理 · 物理学 2026-02-25 Jiyoung Choe , Taysun Kimm , Harley Katz , Maxime Rey , Daniel Han , J. K. Jang , Joki Rosdahl

With its exquisite sensitivity, wavelength coverage, and spatial and spectral resolution, the James Webb Space Telescope is poised to revolutionise our view of the distant, high-redshift ($z>5$) Universe. While Webb's spectroscopic…

JWST observations of high redshift galaxies are used to measure their star formation histories - the buildup of stellar mass in the earliest galaxies. Here we use a novel analysis program, SEDz*, to compare near-IR spectral energy…

We present a catalog of about 25,000 images of massive ($M_{\star} \ge 10^9 M_{\odot}$) galaxies at redshift $3 \leq z \leq 6$ from the TNG50 cosmological simulation, tailored for observations at multiple wavelengths carried out with JWST.…

We analyse the photometric and spectroscopic properties of four galaxies in the epoch of reionisation (EoR) within the SMACS 0723 JWST Early Release Observations field. Given the known spectroscopic redshifts of these sources, we…

JWST/NIRCam provides rest-frame near-IR photometry of galaxies up to $z=2.5$ with exquisite depth and accuracy. This affords an unprecedented view of the evolution of the UV-optical-near-IR color distribution and its interpretation in terms…

Galaxy morphology is one of the most fundamental ways to describe galaxy properties, but the morphology we observe may be affected by wavelength and spatial resolution, which may introduce systematic bias when comparing galaxies at…

星系天体物理 · 物理学 2023-07-27 Yao Yao , Jie Song , Xu Kong , Guanwen Fang , Hong-Xin Zhang , Xinkai Chen
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