Journal article
ASTRODEEP-JWST: NIRCam-HST multi-band photometry and redshifts for half a million sources in six extragalactic deep fields
E Merlin, P Santini, D Paris, M Castellano, A Fontana, T Treu, SL Finkelstein, JS Dunlop, P Arrabal Haro, M Bagley, K Boyett, A Calabrò, M Correnti, K Davis, M Dickinson, CT Donnan, HC Ferguson, F Fortuni, M Giavalisco, K Glazebrook Show all
Astronomy and Astrophysics | EDP SCIENCES S A | Published : 2024
Abstract
Aims. We present a set of photometric catalogues primarily aimed at providing the community with a comprehensive database for the study of galaxy populations in the high-redshift Universe. The set gathers data from eight JWST NIRCam observational programs, targeting the Abell 2744 (GLASS-JWST, UNCOVER, DDT2756, and GO3990), EGS (CEERS), COSMOS and UDS (PRIMER), and the GOODS North and South (JADES and NGDEEP) deep fields. This dataset covers a total area of ≃ 0.2 sq. degrees. Methods. We obtained photometric estimates by means of well-established techniques, including tailored improvements designed to enhance the performance on the specific dataset. We also included new measurements from HST..
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Grants
Awarded by Ministerio de Ciencia, Innovación y Universidades
Funding Acknowledgements
This work is based in part on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program JWST-ERS-1342. This research is also based in part on observations made with the NASA/ESA Hubble Space Telescope obtained from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program HST-GO-17321. This research is also supported in part by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. We also acknowledge support from the INAF Theory Grant 2022 "Forward modeling of theoretical models for upcoming surveys" (PI Merlin), Large Grant 2022 "Extragalactic Surveys with JWST" (PI Pentericci), Mini Grant 2022 "The evolution of passive galaxies through cosmic time" (PI Santini) and Mini Grant 2022 "Reionization and Fundamental Cosmology with High-Redshift Galaxies" (PI Castellano). B.V. is supported by the European Union - NextGenerationEU RFF M4C2 1.1 PRIN 2022 project 2022ZSL4BL INSIGHT. P.G.P.-G. acknowledges support from grant PID2022-139567NB-I00 funded by Spanish Ministerio de Ciencia, Innovacion y Universidades MCIU/AEI/10.13039/501100011033, and the European Union through FEDER Una manera de hacer Europa.