Treu, T. and Roberts-Borsani, G. and Bradac, M. and Brammer, G. and Fontana, A. and Henry, A. and Mason, C. and Morishita, T. and Pentericci, L. and Wang, X. and Acebron, A. and Bagley, M. and Bergamini, P. and Belfiori, D. and Bonchi, A. and Boyett, K. and Boutsia, K. and Calabró, A. and Caminha, G. B. and Castellano, M. and Dressler, A. and Glazebrook, K. and Grillo, C. and Jacobs, C. and Jones, T. and Kelly, P. L. and Leethochawalit, N. and Malkan, M. A. and Marchesini, D. and Mascia, S. and Mercurio, A. and Merlin, E. and Nanayakkara, T. and Nonino, M. and Paris, D. and Poggianti, B. and Rosati, P. and Santini, P. and Scarlata, C. and Shipley, H. V. and Strait, V. and Trenti, M. and Tubthong, C. and Vanzella, E. and Vulcani, B. and Yang, L. (2022) The GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans. Astrophysical Journal, 935 (2). p. 110. ISSN 0004-637X. doi:10.3847/1538-4357/ac8158. https://resolver.caltech.edu/CaltechAUTHORS:20220829-468372700.780
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Abstract
The GLASS-JWST Early Release Science (hereafter GLASS-JWST-ERS) Program will obtain and make publicly available the deepest extragalactic data of the ERS campaign. It is primarily designed to address two key science questions, namely, “what sources ionized the universe and when?” and “how do baryons cycle through galaxies?”, while also enabling a broad variety of first look scientific investigations. In primary mode, it will obtain NIRISS and NIRSpec spectroscopy of galaxies lensed by the foreground Hubble Frontier Field cluster, Abell 2744. In parallel, it will use NIRCam to observe two fields that are offset from the cluster center, where lensing magnification is negligible, and which can thus be effectively considered blank fields. In order to prepare the community for access to this unprecedented data, we describe the scientific rationale, the survey design (including target selection and observational setups), and present pre-commissioning estimates of the expected sensitivity. In addition, we describe the planned public releases of high-level data products, for use by the wider astronomical community.
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| Additional Information: | Support for program JWST-ERS-1324 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile We are grateful to past members of the GLASS-JWST-ERS team for their contribution during the years (L. Abramson, A. Hoag, H. Kuang, and K. Schmidt). C.A.M. acknowledges support from the VILLUM FONDEN under grant 37459 and the Danish National Research Foundation through grant DNRF140. M.B. acknowledges support from the Slovenian national research agency ARRS through grant N1-0238. We acknowledge financial support through grant PRIN-MIUR 2017WSCC32 “Zooming into dark matter and protogalaxies with massive lensing clusters”. G.B.C. acknowledges the Max Planck Society for financial support through the Max Planck Research Group for S. H. Suyu and the academic support from the German Center for Cosmological Lensing. M.N. acknowledges support from grant INAF1.05.01.86.20. This work utilizes gravitational lensing models produced by PIs Bradac, Natarajan & Kneib (CATS), Merten & Zitrin, Sharon, Williams, Keeton, Bernstein, and Diego, and the GLAFIC group. This lens modeling was partially funded by the HST Frontier Fields program conducted by STScI. STScI is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS 5–26555. The lens models were obtained from the Mikulski Archive for Space Telescopes (MAST). This work was partially supported by the Australian Research Council Centre of Excellence for All-Sky Astrophysics in 3 Dimensions (ASTRO-3D) through award CE170100013. B.M.P. and B.V. acknowledge the funding received from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement No. 833824). K.G., T.N., and C.J. acknowledge support from the Australian Research Council Laureate Fellowship FL180100060. L.Y. acknowledges support by JSPS KAKENHI grant No. JP 21F21325. | ||||||||||||||||||||||||||
| Group: | Infrared Processing and Analysis Center (IPAC) | ||||||||||||||||||||||||||
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| Issue or Number: | 2 | ||||||||||||||||||||||||||
| DOI: | 10.3847/1538-4357/ac8158 | ||||||||||||||||||||||||||
| Record Number: | CaltechAUTHORS:20220829-468372700.780 | ||||||||||||||||||||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20220829-468372700.780 | ||||||||||||||||||||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||||||||||||||||||
| ID Code: | 116630 | ||||||||||||||||||||||||||
| Collection: | CaltechAUTHORS | ||||||||||||||||||||||||||
| Deposited By: | Donna Wrublewski | ||||||||||||||||||||||||||
| Deposited On: | 11 Oct 2022 15:57 | ||||||||||||||||||||||||||
| Last Modified: | 11 Oct 2022 15:57 |
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