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| Format: | Preprint |
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2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2506.03243 |
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| _version_ | 1866914252875366400 |
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| author | Shuntov, Marko Akins, Hollis B. Paquereau, Louise Casey, Caitlin M. Ilbert, Olivier Arango-Toro, Rafael C. McCracken, Henry Joy Franco, Maximilien Harish, Santosh Kartaltepe, Jeyhan S. Koekemoer, Anton M. Yang, Lilan Huertas-Company, Marc Berman, Edward M. McCleary, Jacqueline E. Toft, Sune Gavazzi, Raphaël Achenbach, Mark J. Bertin, Emmanuel Brinch, Malte Champagne, Jackie Chartab, Nima Drakos, Nicole E. Egami, Eiichi Endsley, Ryan Faisst, Andreas L. Fan, Xiaohui Flayhart, Carter Hartley, William G. Hatamnia, Hossein Gozaliasl, Ghassem Gentile, Fabrizio Jermann, Iris Jin, Shuowen Kakiichi, Koki Khostovan, Ali Ahmad Kümmel, Martin Laigle, Clotilde Laishram, Ronaldo Lambrides, Erini Liu, Daizhong Lyu, Jianwei Magdis, Georgios Mobasher, Bahram Moutard, Thibaud Renzini, Alvio Robertson, Brant E. Schefer, Marc Scognamiglio, Diana Scoville, Nick Sattari, Zahra Sanders, David B. Taamoli, Sina Trakhtenbrot, Benny Valentino, Francesco Wang, Feige Weaver, John R. Yang, Jinyl |
| author_facet | Shuntov, Marko Akins, Hollis B. Paquereau, Louise Casey, Caitlin M. Ilbert, Olivier Arango-Toro, Rafael C. McCracken, Henry Joy Franco, Maximilien Harish, Santosh Kartaltepe, Jeyhan S. Koekemoer, Anton M. Yang, Lilan Huertas-Company, Marc Berman, Edward M. McCleary, Jacqueline E. Toft, Sune Gavazzi, Raphaël Achenbach, Mark J. Bertin, Emmanuel Brinch, Malte Champagne, Jackie Chartab, Nima Drakos, Nicole E. Egami, Eiichi Endsley, Ryan Faisst, Andreas L. Fan, Xiaohui Flayhart, Carter Hartley, William G. Hatamnia, Hossein Gozaliasl, Ghassem Gentile, Fabrizio Jermann, Iris Jin, Shuowen Kakiichi, Koki Khostovan, Ali Ahmad Kümmel, Martin Laigle, Clotilde Laishram, Ronaldo Lambrides, Erini Liu, Daizhong Lyu, Jianwei Magdis, Georgios Mobasher, Bahram Moutard, Thibaud Renzini, Alvio Robertson, Brant E. Schefer, Marc Scognamiglio, Diana Scoville, Nick Sattari, Zahra Sanders, David B. Taamoli, Sina Trakhtenbrot, Benny Valentino, Francesco Wang, Feige Weaver, John R. Yang, Jinyl |
| contents | We present COSMOS2025, the COSMOS-Web catalog of photometry, morphology, photometric redshifts and physical parameters for more than 700,000 galaxies in the Cosmic Evolution Survey (COSMOS) field. This catalog is based on our \textit{James Webb Space Telescope} 255\,h COSMOS-Web program, which provides deep near-infrared imaging in four NIRCam (F115W, F150W, F277W, F444W) and one MIRI (F770W) filter over the central $\sim 0.54 {\, \rm deg}^2$ ($\sim 0.2 {\, \rm deg}^2$ for MIRI) in COSMOS. These data are combined with ground- and space-based data to derive photometric measurements of NIRCam-detected sources using both fixed-aperture photometry (on the space-based bands) and a profile-fitting technique on all 37 bands spanning 0.3-8 micron. We provide morphology for all sources from complementary techniques including profile fitting and machine-learning classification. We derive photometric redshifts, physical parameters and non-parametric star formation histories from spectral energy distribution (SED) fitting. The catalog has been extensively validated against previous COSMOS catalogs and other surveys. Photometric redshift accuracy measured using spectroscopically confirmed galaxies out to $z\sim9$ reaches $σ_{\rm MAD} = 0.012$ at $m_{\rm F444W}<28$ and remains at $σ_{\rm MAD} \lesssim 0.03$ as a function of magnitude, color, and galaxy type. This represents a factor of $\sim 2$ improvement at 26 AB mag compared to COSMOS2020. The catalog is approximately 80\% complete at $\log(M_{\star}/{\rm M}_{\odot}) \sim 9$ at $z \sim 10$ and at $\log(M_{\star}/{\rm M}_{\odot}) \sim 7$ at $z \sim 0.2$, representing a gain of 1\,dex compared to COSMOS2020. COSMOS2025 represents the definitive COSMOS-Web catalog. It is provided with complete documentation, together with redshift probability distributions, and it is ready for scientific exploitation today. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2506_03243 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | COSMOS2025: The COSMOS-Web galaxy catalog of photometry, morphology, redshifts, and physical parameters from JWST, HST, and ground-based imaging Shuntov, Marko Akins, Hollis B. Paquereau, Louise Casey, Caitlin M. Ilbert, Olivier Arango-Toro, Rafael C. McCracken, Henry Joy Franco, Maximilien Harish, Santosh Kartaltepe, Jeyhan S. Koekemoer, Anton M. Yang, Lilan Huertas-Company, Marc Berman, Edward M. McCleary, Jacqueline E. Toft, Sune Gavazzi, Raphaël Achenbach, Mark J. Bertin, Emmanuel Brinch, Malte Champagne, Jackie Chartab, Nima Drakos, Nicole E. Egami, Eiichi Endsley, Ryan Faisst, Andreas L. Fan, Xiaohui Flayhart, Carter Hartley, William G. Hatamnia, Hossein Gozaliasl, Ghassem Gentile, Fabrizio Jermann, Iris Jin, Shuowen Kakiichi, Koki Khostovan, Ali Ahmad Kümmel, Martin Laigle, Clotilde Laishram, Ronaldo Lambrides, Erini Liu, Daizhong Lyu, Jianwei Magdis, Georgios Mobasher, Bahram Moutard, Thibaud Renzini, Alvio Robertson, Brant E. Schefer, Marc Scognamiglio, Diana Scoville, Nick Sattari, Zahra Sanders, David B. Taamoli, Sina Trakhtenbrot, Benny Valentino, Francesco Wang, Feige Weaver, John R. Yang, Jinyl Astrophysics of Galaxies We present COSMOS2025, the COSMOS-Web catalog of photometry, morphology, photometric redshifts and physical parameters for more than 700,000 galaxies in the Cosmic Evolution Survey (COSMOS) field. This catalog is based on our \textit{James Webb Space Telescope} 255\,h COSMOS-Web program, which provides deep near-infrared imaging in four NIRCam (F115W, F150W, F277W, F444W) and one MIRI (F770W) filter over the central $\sim 0.54 {\, \rm deg}^2$ ($\sim 0.2 {\, \rm deg}^2$ for MIRI) in COSMOS. These data are combined with ground- and space-based data to derive photometric measurements of NIRCam-detected sources using both fixed-aperture photometry (on the space-based bands) and a profile-fitting technique on all 37 bands spanning 0.3-8 micron. We provide morphology for all sources from complementary techniques including profile fitting and machine-learning classification. We derive photometric redshifts, physical parameters and non-parametric star formation histories from spectral energy distribution (SED) fitting. The catalog has been extensively validated against previous COSMOS catalogs and other surveys. Photometric redshift accuracy measured using spectroscopically confirmed galaxies out to $z\sim9$ reaches $σ_{\rm MAD} = 0.012$ at $m_{\rm F444W}<28$ and remains at $σ_{\rm MAD} \lesssim 0.03$ as a function of magnitude, color, and galaxy type. This represents a factor of $\sim 2$ improvement at 26 AB mag compared to COSMOS2020. The catalog is approximately 80\% complete at $\log(M_{\star}/{\rm M}_{\odot}) \sim 9$ at $z \sim 10$ and at $\log(M_{\star}/{\rm M}_{\odot}) \sim 7$ at $z \sim 0.2$, representing a gain of 1\,dex compared to COSMOS2020. COSMOS2025 represents the definitive COSMOS-Web catalog. It is provided with complete documentation, together with redshift probability distributions, and it is ready for scientific exploitation today. |
| title | COSMOS2025: The COSMOS-Web galaxy catalog of photometry, morphology, redshifts, and physical parameters from JWST, HST, and ground-based imaging |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2506.03243 |