{"_id":"18584","citation":{"chicago":"Suess, Katherine A., John R. Weaver, Sedona H. Price, Richard Pan, Bingjie Wang, Rachel Bezanson, Gabriel Brammer, et al. “Medium Bands, Mega Science: A JWST/NIRCam Medium-Band Imaging Survey of A2744.” <i>Astrophysical Journal</i>. IOP Publishing, 2024. <a href=\"https://doi.org/10.3847/1538-4357/ad75fe\">https://doi.org/10.3847/1538-4357/ad75fe</a>.","apa":"Suess, K. A., Weaver, J. R., Price, S. H., Pan, R., Wang, B., Bezanson, R., … Zitrin, A. (2024). Medium bands, mega science: A JWST/NIRCam medium-band imaging survey of A2744. <i>Astrophysical Journal</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/1538-4357/ad75fe\">https://doi.org/10.3847/1538-4357/ad75fe</a>","mla":"Suess, Katherine A., et al. “Medium Bands, Mega Science: A JWST/NIRCam Medium-Band Imaging Survey of A2744.” <i>Astrophysical Journal</i>, vol. 976, no. 1, 101, IOP Publishing, 2024, doi:<a href=\"https://doi.org/10.3847/1538-4357/ad75fe\">10.3847/1538-4357/ad75fe</a>.","ama":"Suess KA, Weaver JR, Price SH, et al. Medium bands, mega science: A JWST/NIRCam medium-band imaging survey of A2744. <i>Astrophysical Journal</i>. 2024;976(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/ad75fe\">10.3847/1538-4357/ad75fe</a>","ieee":"K. A. Suess <i>et al.</i>, “Medium bands, mega science: A JWST/NIRCam medium-band imaging survey of A2744,” <i>Astrophysical Journal</i>, vol. 976, no. 1. IOP Publishing, 2024.","ista":"Suess KA, Weaver JR, Price SH, Pan R, Wang B, Bezanson R, Brammer G, Cutler SE, Labbé I, Leja J, Williams CC, Whitaker KE, Atek H, Dayal P, De Graaff A, Feldmann R, Franx M, Fudamoto Y, Fujimoto S, Furtak LJ, Goulding AD, Greene JE, Khullar G, Kokorev V, Kriek M, Lorenz B, Marchesini D, Maseda MV, Matthee JJ, Miller TB, Mitsuhashi I, Mowla LA, Muzzin A, Naidu RP, Nanayakkara T, Nelson EJ, Oesch PA, Setton DJ, Shipley H, Smit R, Spilker JS, Van Dokkum P, Zitrin A. 2024. Medium bands, mega science: A JWST/NIRCam medium-band imaging survey of A2744. Astrophysical Journal. 976(1), 101.","short":"K.A. Suess, J.R. Weaver, S.H. Price, R. Pan, B. Wang, R. Bezanson, G. Brammer, S.E. Cutler, I. Labbé, J. Leja, C.C. Williams, K.E. Whitaker, H. Atek, P. Dayal, A. De Graaff, R. Feldmann, M. Franx, Y. Fudamoto, S. Fujimoto, L.J. Furtak, A.D. Goulding, J.E. Greene, G. Khullar, V. Kokorev, M. Kriek, B. Lorenz, D. Marchesini, M.V. Maseda, J.J. Matthee, T.B. Miller, I. Mitsuhashi, L.A. Mowla, A. Muzzin, R.P. Naidu, T. Nanayakkara, E.J. Nelson, P.A. Oesch, D.J. Setton, H. Shipley, R. Smit, J.S. Spilker, P. Van Dokkum, A. Zitrin, Astrophysical Journal 976 (2024)."},"issue":"1","article_processing_charge":"Yes","OA_place":"publisher","oa_version":"Published Version","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","file":[{"relation":"main_file","success":1,"content_type":"application/pdf","file_name":"2024_AstrophysicalJournal_Suess.pdf","checksum":"dcd854acee73ce998d70a4ce634ead6d","file_id":"18640","date_updated":"2024-12-10T08:18:53Z","date_created":"2024-12-10T08:18:53Z","creator":"dernst","file_size":13352667,"access_level":"open_access"}],"has_accepted_license":"1","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"author":[{"last_name":"Suess","full_name":"Suess, Katherine A.","first_name":"Katherine A."},{"first_name":"John R.","full_name":"Weaver, John R.","last_name":"Weaver"},{"full_name":"Price, Sedona H.","first_name":"Sedona H.","last_name":"Price"},{"last_name":"Pan","full_name":"Pan, Richard","first_name":"Richard"},{"full_name":"Wang, Bingjie","first_name":"Bingjie","last_name":"Wang"},{"full_name":"Bezanson, Rachel","first_name":"Rachel","last_name":"Bezanson"},{"first_name":"Gabriel","full_name":"Brammer, Gabriel","last_name":"Brammer"},{"last_name":"Cutler","first_name":"Sam E.","full_name":"Cutler, Sam E."},{"last_name":"Labbé","first_name":"Ivo","full_name":"Labbé, Ivo"},{"full_name":"Leja, Joel","first_name":"Joel","last_name":"Leja"},{"last_name":"Williams","full_name":"Williams, Christina C.","first_name":"Christina C."},{"last_name":"Whitaker","first_name":"Katherine E.","full_name":"Whitaker, Katherine E."},{"full_name":"Atek, Hakim","first_name":"Hakim","last_name":"Atek"},{"first_name":"Pratika","full_name":"Dayal, Pratika","last_name":"Dayal"},{"first_name":"Anna","full_name":"De Graaff, Anna","last_name":"De Graaff"},{"last_name":"Feldmann","full_name":"Feldmann, Robert","first_name":"Robert"},{"first_name":"Marijn","full_name":"Franx, Marijn","last_name":"Franx"},{"full_name":"Fudamoto, Yoshinobu","first_name":"Yoshinobu","last_name":"Fudamoto"},{"full_name":"Fujimoto, Seiji","first_name":"Seiji","last_name":"Fujimoto"},{"last_name":"Furtak","full_name":"Furtak, Lukas J.","first_name":"Lukas J."},{"last_name":"Goulding","first_name":"Andy D.","full_name":"Goulding, Andy D."},{"last_name":"Greene","first_name":"Jenny E.","full_name":"Greene, Jenny E."},{"first_name":"Gourav","full_name":"Khullar, Gourav","last_name":"Khullar"},{"first_name":"Vasily","full_name":"Kokorev, Vasily","last_name":"Kokorev"},{"first_name":"Mariska","full_name":"Kriek, Mariska","last_name":"Kriek"},{"last_name":"Lorenz","full_name":"Lorenz, Brian","first_name":"Brian"},{"last_name":"Marchesini","full_name":"Marchesini, Danilo","first_name":"Danilo"},{"last_name":"Maseda","full_name":"Maseda, Michael V.","first_name":"Michael V."},{"last_name":"Matthee","id":"7439a258-f3c0-11ec-9501-9df22fe06720","first_name":"Jorryt J","orcid":"0000-0003-2871-127X","full_name":"Matthee, Jorryt J"},{"full_name":"Miller, Tim B.","first_name":"Tim B.","last_name":"Miller"},{"last_name":"Mitsuhashi","first_name":"Ikki","full_name":"Mitsuhashi, Ikki"},{"first_name":"Lamiya A.","full_name":"Mowla, Lamiya A.","last_name":"Mowla"},{"first_name":"Adam","full_name":"Muzzin, Adam","last_name":"Muzzin"},{"last_name":"Naidu","full_name":"Naidu, Rohan P.","first_name":"Rohan P."},{"first_name":"Themiya","full_name":"Nanayakkara, Themiya","last_name":"Nanayakkara"},{"last_name":"Nelson","full_name":"Nelson, Erica J.","first_name":"Erica J."},{"last_name":"Oesch","full_name":"Oesch, Pascal A.","first_name":"Pascal A."},{"full_name":"Setton, David J.","first_name":"David J.","last_name":"Setton"},{"last_name":"Shipley","full_name":"Shipley, Heath","first_name":"Heath"},{"full_name":"Smit, Renske","first_name":"Renske","last_name":"Smit"},{"last_name":"Spilker","full_name":"Spilker, Justin S.","first_name":"Justin S."},{"last_name":"Van Dokkum","full_name":"Van Dokkum, Pieter","first_name":"Pieter"},{"last_name":"Zitrin","first_name":"Adi","full_name":"Zitrin, Adi"}],"article_type":"original","arxiv":1,"type":"journal_article","date_created":"2024-11-24T23:01:48Z","scopus_import":"1","date_updated":"2024-12-10T08:21:08Z","file_date_updated":"2024-12-10T08:18:53Z","status":"public","day":"14","department":[{"_id":"JoMa"}],"abstract":[{"lang":"eng","text":"In this paper, we describe the \"Medium Bands, Mega Science\" JWST Cycle 2 survey (JWST-GO-4111) and demonstrate the power of these data to reveal both the spatially integrated and spatially resolved properties of galaxies from the local Universe to the era of cosmic dawn. Executed in 2023 November, MegaScience obtained ∼30 arcmin2 of deep multiband NIRCam imaging centered on the z ∼ 0.3 A2744 cluster, including 11 medium-band filters and the two shortest-wavelength broadband filters, F070W and F090W. Together, MegaScience and the UNCOVER Cycle 1 treasury program provide a complete set of deep (∼28–30 magAB) images in all NIRCam medium- and broadband filters. This unique data set allows us to precisely constrain photometric redshifts, map stellar populations and dust attenuation for large samples of distant galaxies, and examine the connection between galaxy structures and formation histories. MegaScience also includes ∼17 arcmin2 of NIRISS parallel imaging in two broadband and four medium-band filters from 0.9 to 4.8 μm, expanding the footprint where robust spectral energy distribution (SED) fitting is possible. We provide example SEDs and multiband cutouts at a variety of redshifts, and use a catalog of JWST spectroscopic redshifts to show that MegaScience improves both the scatter and catastrophic outlier rate of photometric redshifts by factors of 2–3. Additionally, we demonstrate the spatially resolved science enabled by MegaScience by presenting maps of the [O iii] line emission and continuum emission in three spectroscopically confirmed z > 6 galaxies. We show that line emission in reionization-era galaxies can be clumpy, extended, and spatially offset from continuum emission, implying that galaxy assembly histories are complex even at these early epochs. We publicly release fully reduced mosaics and photometric catalogs for both the NIRCam primary and NIRISS parallel fields (jwst-uncover.github.io/megascience)."}],"intvolume":"       976","quality_controlled":"1","title":"Medium bands, mega science: A JWST/NIRCam medium-band imaging survey of A2744","date_published":"2024-11-14T00:00:00Z","publisher":"IOP Publishing","publication":"Astrophysical Journal","DOAJ_listed":"1","publication_status":"published","language":[{"iso":"eng"}],"year":"2024","external_id":{"arxiv":["2404.13132"]},"volume":976,"ddc":["520"],"doi":"10.3847/1538-4357/ad75fe","oa":1,"OA_type":"gold","article_number":"101","acknowledgement":"K.A.S. thanks Shelly Meyett, the MegaScience Program Coordinator, for invaluable assistance designing WOPR 88967 and ensuring that this program was fully observed. This proposal was conceived of and developed at the International Space Science Institute (ISSI) in Bern, through ISSI International Team project #562. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The raw 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 JWST Cycle 2 GO program #4111, and this project has gratefully made use of a large number of public JWST programs in the A2744 field including JWST-GO-2641, JWST-ERS-1324, JWST-DD-2756, JWST-GO-2883, JWST-GO-3538, and JWST-GO-3516. Support for program JWST-GO-4111 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Associations of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555.\r\n\r\nThe Cosmic Dawn Center is funded by the Danish National Research Foundation (DNRF) under grant #140. P.D. acknowledges support from the NWO grant 016.VIDI.189.162 (\"ODIN\") and warmly thanks the European Commission's and University of Groningen's CO-FUND Rosalind Franklin program. This work has received funding from the Swiss State Secretariat for Education, Research and Innovation (SERI) under contract number MB22.00072, as well as from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. The work of C.C.W. is supported by NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. T.B.M. was supported by a CIERA Fellowship. H.A. is supported by CNES, focused on the JWST mission, and by the Programme National Cosmology and Galaxies (PNCG) of CNRS/INSU with INP and IN2P3, co-funded by CEA and CNES. The BGU lensing group acknowledges support by grant No. 2020750 from the United States–Israel Binational Science Foundation (BSF) and grant No. 2109066 from the United States National Science Foundation (NSF); by the Ministry of Science & Technology, Israel; and by the Israel Science Foundation grant No. 864/23. Y.F. acknowledges support from JSPS KAKENHI grant No. JP22K21349 and JP23K13149. R.P. and D.M. acknowledge funding from JWST-GO-02561.013 and JWST-GO-04111.035.","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","short":"CC BY (4.0)"},"month":"11"}