Publicación:
JADES Data Release 3: NIRSpec/Microshutter Assembly Spectroscopy for 4000 Galaxies in the GOODS Fields

dc.contributor.authorD'Eugenio, Francesco
dc.contributor.authorCameron, Alex J.
dc.contributor.authorScholtz, Jan
dc.contributor.authorCarniani, Stefano
dc.contributor.authorWillott, Chris J.
dc.contributor.authorCurtis-Lake, Emma
dc.contributor.authorBunker, Andrew J.
dc.contributor.authorParlanti, Eleonora
dc.contributor.authorMaiolino, Roberto
dc.contributor.authorWillmer, Christopher N. A.
dc.contributor.authorJakobsen, Peter
dc.contributor.authorRobertson, Brant
dc.contributor.authorJohnson, Benjamin D.
dc.contributor.authorTacchella, Sandro
dc.contributor.authorCargile, Phillip
dc.contributor.authorRawle, T. D.
dc.contributor.authorArribas, Santiago
dc.contributor.authorChevallard, Jacopo
dc.contributor.authorCurti, Mirko
dc.contributor.authorEgami, E.
dc.contributor.authorEisenstein, Daniel
dc.contributor.authorKumari, Nimisha
dc.contributor.authorLooser, Tobias J.
dc.contributor.authorRieke, Marcia
dc.contributor.authorRodriguez Del Pino, Bruno
dc.contributor.authorSaxena, Aayush
dc.contributor.authorÜbler, Hannah
dc.contributor.authorVenturi, Giacomo
dc.contributor.authorWitstok, Joris
dc.contributor.authorBaker, William M.
dc.contributor.authorBhatawdekar, Rachana
dc.contributor.authorBonaventura, Nina
dc.contributor.authorBoyett, Kristan
dc.contributor.authorCharlot, Stephane
dc.contributor.authorDanhaive, Angelica Lola
dc.contributor.authorHainline, Kevin N.
dc.contributor.authorHausen, Ryan
dc.contributor.authorHelton, Jakob M.
dc.contributor.authorJi, Xihan
dc.contributor.authorJi, Zhiyuan
dc.contributor.authorJones, Gareth C.
dc.contributor.authorJuodžbalis, Ignas
dc.contributor.authorMaseda, Michael
dc.contributor.authorPérez-González, Pablo G.
dc.contributor.authorPerna, Michele
dc.contributor.authorPuskás, Dávid
dc.contributor.authorShivaei, Irene
dc.contributor.authorSilcock, Maddie
dc.contributor.authorSimmonds, Charlotte
dc.contributor.authorSmit, Renske
dc.contributor.authorSun, Fengwu
dc.contributor.authorVillanueva, Natalia C.
dc.contributor.authorWilliams, Christina C.
dc.contributor.authorZhu, Yongda
dc.contributor.funderScience and Technology Facilities Council (STFC)
dc.contributor.funderEuropean Research Council (ERC)
dc.contributor.funderAgencia Estatal de Investigación (AEI)
dc.contributor.funderComunidad de Madrid
dc.contributor.funderUniversity of Arizona (UA)
dc.contributor.funderDanish National Research Foundation (DNRF)
dc.contributor.funderAustralian Research Council (ARC)
dc.date.accessioned2026-06-01T10:24:35Z
dc.date.available2026-06-01T10:24:35Z
dc.date.issued2025-02-14
dc.description.abstractWe present the third data release of the JWST Advanced Deep Extragalactic Survey (JADES), providing both imaging and spectroscopy in the two GOODS fields. Spectroscopy consists of medium-depth and deep NIRSpec/microshutter assembly spectra of 4000 targets, covering the spectral range 0.6-5.3 μm and observed with both the low-dispersion prism (R = 30-300) and all three medium-resolution gratings (R = 500-1500). We describe the observations, data reduction, sample selection, and target allocation. We measured 2375 redshifts (2053 from multiple emission lines); our targets span the range from z = 0.5 up to z = 13, including 404 at z > 5. The data release includes 2D and 1D fully reduced spectra, with slit-loss corrections and background subtraction optimized for point sources. We also provide redshifts and signal-to-noise ratio > 5 emission-line flux catalogs for the prism and grating spectra, and concise guidelines on how to use these data products. Alongside spectroscopy, we are also publishing fully calibrated NIRCam imaging, which enables studying the JADES sample with the combined power of imaging and spectroscopy. Together, these data provide the largest statistical sample to date to characterize the properties of galaxy populations in the first billion years after the Big Bang.
dc.description.peerreviewedPeerreview
dc.description.sponsorshipF.D.E., J.S., R.M., T.J.L., J.W., W.M.B., X.J., I.J., and C.S. acknowledge support by the Science and Technology Facilities Council (STFC), by the ERC through Advanced Grant 695671 “QUENCH,” and by the UKRI Frontier Research grant RISEandFALL. R.M. also acknowledges funding from a research professorship from the Royal Society. A.J.C., A.J.B., J.C., A.S., and G.C.J. acknowledge funding from the “FirstGalaxies” Advanced Grant from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement No. 789056) S.C., E.P., and G.V. acknowledge support by the European Union’s HE ERC Starting grant No. 101040227 - WINGS. E.C.L. acknowledges support of an STFC Webb Fellowship (ST/W001438/1). S.A., B.R.P., and M.P. acknowledge support from grant PID2021-127718NB-I00 funded by the Spanish Ministry of Science and Innovation/State Agency of Research (MICIN/AEI/ 10.13039/501100011033). M.P. also acknowledges support from the Programa Atracción de Talento de la Comunidad de Madrid via grant 2018-T2/TIC-11715. C.N.A.W., B.E.R., B.D.J., D.J.E., P.A.C., E.E., M.J.R., and F.S. acknowledge JWST/NIRCam contract to the University of Arizona NAS5-02015. B.E.R. also acknowledges support from the JWST Program 3215. D.J.E. is supported as a Simons Investigator. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant DNRF140. S.T. acknowledges support by the Royal Society Research grant G125142. H.Ü. gratefully acknowledges support by the Isaac Newton Trust and by the Kavli Foundation through a Newton-Kavli Junior Fellowship. 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 No. CE170100013. A.L.D. thanks the University of Cambridge Harding Distinguished Postgraduate Scholars Program and Technology Facilities Council (STFC) Center for Doctoral Training (CDT) in Data intensive science at the University of Cambridge (STFC grant number 2742605) for a PhD studentship. Funding for this research was provided by the Johns Hopkins University, Institute for Data Intensive Engineering and Science (IDIES). P.G.P.-G. acknowledges support from grant PID2022-139567NB-I00 funded by Spanish Ministerio de Ciencia e Innovación MCIN/AEI/10.13039/501100011033, FEDER, UE. D.P. acknowledges support by the Huo Family Foundation through a P.C. Ho PhD Studentship. M.S.S. acknowledges support by the Science and Technology Facilities Council (STFC) grant ST/V506709/1. R.S. acknowledges support from a STFC Ernest Rutherford Fellowship (ST/S004831/1). N.C.V. acknowledges support from the Charles and Julia Henry Fund through the Henry Fellowship. The research 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. This work was performed using resources provided by the Cambridge Service for Data Driven Discovery (CSD3) operated by the University of Cambridge Research Computing Service (http://www.csd3.cam.ac.uk), provided by Dell EMC and Intel using Tier-2 funding from the Engineering and Physical Sciences Research Council (capital grant EP/T022159/1), and DiRAC funding from the Science and Technology Facilities Council (http://www.dirac.ac.uk). The authors acknowledge use of the lux supercomputer at UC Santa Cruz, funded by NSF MRI grant AST 1828315. This study made use of the Prospero high-performance computing facility at Liverpool John Moores University. Facility: JWST (NIRCam), JWST (NIRSpec/MSA), HST (ACS), HST (WFC3) -
dc.identifier.citationAstronomy & Astrophysics 277 (4): 34pp (2025)
dc.identifier.doi0.3847/1538-4365/ada148
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000271
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000781
dc.identifier.funderhttp://dx.doi.org/10.13039/501100011033
dc.identifier.funderhttp://dx.doi.org/10.13039/100012818
dc.identifier.funderhttp://dx.doi.org/10.13039/100007899
dc.identifier.funderhttp://dx.doi.org/10.13039/501100001732
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000923
dc.identifier.issn0067-0049
dc.identifier.otherhttps://iopscience.iop.org/article/10.3847/1538-4365/ada148
dc.identifier.urihttps://hdl.handle.net/20.500.12666/1862
dc.language.isoeng
dc.publisherAmerican Astronomical Society
dc.relationStar formation quenching and feedback in galaxies throughout the cosmic epochs
dc.relationFinding the most distant galaxies with NIRSpec guaranteed time on the James Webb Space Telescope
dc.relationWinds in galaxies
dc.relationPARTICIPACION ESPAÑOLA EN EL TELESCOPIO ESPACIAL JAMES WEBB: ACTIVIDADES TECNICAS POSTERIORES AL LANZAMIENTO Y PROGRAMAS CIENTIFICOS DE TIEMPO GARANTIZADO
dc.relationDISECCION DE LA HISTORIA DEL ENSAMBLAJE DE LAS GALAXIAS MASIVAS CON JWST
dc.rightsAttribution 4.0 Internationalen
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.rights.license© 2025. The Author(s). Published by the American Astronomical Society.
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.titleJADES Data Release 3: NIRSpec/Microshutter Assembly Spectroscopy for 4000 Galaxies in the GOODS Fields
dc.typeinfo:eu-repo/semantics/article
dc.type.coarhttp://purl.org/coar/resource_type/c_6501
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion
dspace.entity.typePublication
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oaire.awardNumberPID2022-139567NB-I00
oaire.awardTitleStar formation quenching and feedback in galaxies throughout the cosmic epochs
oaire.awardTitleFinding the most distant galaxies with NIRSpec guaranteed time on the James Webb Space Telescope
oaire.awardTitleWinds in galaxies
oaire.awardTitlePARTICIPACION ESPAÑOLA EN EL TELESCOPIO ESPACIAL JAMES WEBB: ACTIVIDADES TECNICAS POSTERIORES AL LANZAMIENTO Y PROGRAMAS CIENTIFICOS DE TIEMPO GARANTIZADO
oaire.awardTitleDISECCION DE LA HISTORIA DEL ENSAMBLAJE DE LAS GALAXIAS MASIVAS CON JWST
oaire.awardURIhttps://digital.inta.es/handle/123456789/1221
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