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arXiv · 2510.08743

The CEERS Photometric and Physical Parameter Catalog

Abstract

We present the Cosmic Evolution Early Release Science Survey (CEERS) catalog, including space-based photometry, photometric redshifts, and physical parameters for more than 80,000 galaxies. The imaging used for this catalog comes from the CEERS survey, which has NIRCam coverage over ~100 sq. arcmin of the Extended Groth Strip (EGS) in seven filters from 1.15$μ$m to 4.44$μ$m. Alongside these data, we also include ancillary HST imaging in seven filters from 0.435$μ$m to 1.6$μ$m. We used Source Extractor with hot and cold detection settings to extract photometry. We derive photometric redshifts using the spectral energy distribution (SED) modeling code, LePHARE, and estimate their accuracy using spectroscopically confirmed galaxies out to $z\sim10$, with $σ_{NMAD}$ ranging from 0.035-0.073, depending strongly on galaxy magnitude and redshift. We compute stellar masses, star formation rates, and E(B-V) using three different SED fitting codes with different templates and assumptions about the galaxy star formation histories. All of these measurements, as well as the full mosaics in all filters, and redshift probability distribution functions, are made available via the CEERS DR1.0 data release.

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Isa G. Cox, Jeyhan S. Kartaltepe, Micaela B. Bagley, Steven L. Finkelstein, Caitlin Rose, Ali Ahmad Khostovan, Katherine Chworowsky, Olivier Ilbert, Anton M. Koekemoer, Henry C. Ferguson, Pablo Arrabal Haro, Bren E. Backhaus, Mark Dickinson, Adriano Fontana, Yuchen Guo, Andrea Grazian, Norman A. Grogin, Santosh Harish, Nimish P. Hathi, Benne W. Holwerda, Kartheik G. Iyer, Lisa J. Kewley, Allison Kirkpatrick, Dale D. Kocevski, Rebecca L. Larson, Jennifer M. Lotz, Ray A. Lucas, Fabio Pacucci, Casey Papovich, Laura Pentericci, Pablo G. Pérez-González, Nor Pirzkal, Swara Ravindranath, Rachel S. Somerville, Jonathan R. Trump, Stephen M. Wilkins, Guang Yang, L. Y. Aaron Yung. 2025-10-09. The CEERS Photometric and Physical Parameter Catalog. https://arxiv.org/abs/2510.08743

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