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Early Results from GLASS-JWST. II. NIRCam Extragalactic Imaging and Photometric Catalog

Merlin, Emiliano and Bonchi, Andrea and Paris, Diego and Belfiori, Davide and Fontana, Adriano and Castellano, Marco and Nonino, Mario and Polenta, Gianluca and Santini, Paola and Yang, Lilan and Glazebrook, Karl and Treu, Tommaso and Roberts-Borsani, Guido and Trenti, Michele and Birrer, Simon and Brammer, Gabriel and Grillo, Claudio and Calabrò, Antonello and Marchesini, Danilo and Mason, Charlotte and Mercurio, Amata and Morishita, Takahiro and Strait, Victoria and Boyett, Kristan and Leethochawalit, Nicha and Nanayakkara, Themiya and Vulcani, Benedetta and Bradac, Marusa and Wang, Xin (2022) Early Results from GLASS-JWST. II. NIRCam Extragalactic Imaging and Photometric Catalog. Astrophysical Journal Letters, 938 (2). Art. No. L14. ISSN 2041-8205. doi:10.3847/2041-8213/ac8f93. https://resolver.caltech.edu/CaltechAUTHORS:20221031-575177800.27

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Abstract

We present the reduced images and multiwavelength catalog of the first JWST NIRCam extragalactic observations from the GLASS Early Release Science Program, obtained as coordinated parallels of the NIRISS observations of the Abell 2744 cluster. Images in seven bands (F090W, F115W, F150W, F200W, F277W, F356W, and F444W) have been reduced using an augmented version of the official JWST pipeline; we discuss the procedures adopted to remove or mitigate defects in the raw images. We obtain a multiband catalog by means of forced aperture photometry on point-spread function (PSF)-matched images at the position of F444W-detected sources. The catalog is intended to enable early scientific investigations, and it is optimized for faint galaxies; it contains 6368 sources, with limiting magnitude 29.7 at 5σ in F444W. We release both images and catalog in order to allow the community to become familiar with the JWST NIRCam data and evaluate their merit and limitations given the current level of knowledge of the instrument.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/2041-8213/ac8f93DOIArticle
ORCID:
AuthorORCID
Merlin, Emiliano0000-0001-6870-8900
Bonchi, Andrea0000-0002-2667-5482
Paris, Diego0000-0002-7409-8114
Fontana, Adriano0000-0003-3820-2823
Castellano, Marco0000-0001-9875-8263
Nonino, Mario0000-0001-6342-9662
Polenta, Gianluca0000-0003-4067-9196
Santini, Paola0000-0002-9334-8705
Yang, Lilan0000-0002-8434-880X
Glazebrook, Karl0000-0002-3254-9044
Treu, Tommaso0000-0002-8460-0390
Roberts-Borsani, Guido0000-0002-4140-1367
Trenti, Michele0000-0001-9391-305X
Birrer, Simon0000-0003-3195-5507
Brammer, Gabriel0000-0003-2680-005X
Grillo, Claudio0000-0002-5926-7143
Calabrò, Antonello0000-0003-2536-1614
Marchesini, Danilo0000-0001-9002-3502
Mason, Charlotte0000-0002-3407-1785
Mercurio, Amata0000-0001-9261-7849
Morishita, Takahiro0000-0002-8512-1404
Strait, Victoria0000-0002-6338-7295
Boyett, Kristan0000-0003-4109-304X
Leethochawalit, Nicha0000-0003-4570-3159
Nanayakkara, Themiya0000-0003-2804-0648
Vulcani, Benedetta0000-0003-0980-1499
Bradac, Marusa0000-0001-5984-0395
Wang, Xin0000-0002-9373-3865
Additional Information:This work is based 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-1324. We acknowledge financial support from NASA through grant JWST-ERS-1324. This research is supported in part by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. K.G. and T.N. acknowledge support from Australian Research Council Laureate Fellowship FL180100060. M.B. acknowledges support from the Slovenian national research agency ARRS through grant N1-0238. We acknowledge financial support through grants PRIN-MIUR 2017WSCC32 and 2020SKSTHZ. C.M. acknowledges support by the VILLUM FONDEN under grant 37459. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant DNRF140. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. The authors thank Paola Marrese and Silvia Marinoni (Space Science Data Center, Italian Space Agency) for their contribution to the work.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASAJWST-ERS-1324
Australian Research CouncilCE170100013
Australian Research CouncilFL180100060
ARRSN1-0238
Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR)2017WSCC32
Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR)2020SKSTHZ
Villum Foundation37459
Danish National Research FoundationDNRF140
NASANAS 5-03127
Gaia Multilateral AgreementUNSPECIFIED
Issue or Number:2
DOI:10.3847/2041-8213/ac8f93
Record Number:CaltechAUTHORS:20221031-575177800.27
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20221031-575177800.27
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:117664
Collection:CaltechAUTHORS
Deposited By: Research Services Depository
Deposited On:09 Nov 2022 19:53
Last Modified:11 Nov 2022 18:07

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