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October 1, 2024The Astrophysical Journal137 citationsOpen Access

The JWST UNCOVER Treasury Survey: Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization

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RBRachel BezansonILIvo LabbéKWKatherine E. Whitaker

Key Points

  • Detail the survey design, science objectives, and early data products of the JWST UNCOVER Treasury program targeting the massive galaxy cluster A2744.
  • Obtained ultradeep NIRCam imaging over 28.8 arcmin² across seven filters and NIRISS parallel imaging over 16.8 arcmin² across five filters around galaxy cluster A2744 (z = 0.308).
  • Designed spectroscopic follow-up targeting approximately 500 galaxies using low-resolution NIRSpec/PRISM observations across multiple visits in 2023 and 2024.
  • Achieved ultradeep imaging reaching ~29–30 AB magnitude across ~45 arcmin², resolving unprecedented 2–4 µm structures of known background sources.
  • Produced and publicly released full reduced mosaics covering 45 arcmin² with NIRCam and 17 arcmin² with NIRISS across primary and parallel cluster fields.

Abstract

Abstract In this paper we describe the survey design for the Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization (UNCOVER) Cycle 1 JWST Treasury program, which executed its early imaging component in 2022 November. The UNCOVER survey includes ultradeep (∼29–30AB) imaging of ∼45 arcmin 2 on and around the well-studied A2744 galaxy cluster at z = 0.308 and will follow up ∼500 galaxies with extremely deep low-resolution spectroscopy with the NIRSpec/PRISM during the summer of 2023, with repeat visits in summer 2024. We describe the science goals, survey design, target selection, and planned data releases. We also present and characterize the depths of the first NIRCam imaging mosaic, highlighting previously unparalleled resolved and ultradeep 2–4 μ m imaging of known objects in the field. The UNCOVER primary NIRCam mosaic spans 28.8 arcmin 2 in seven filters (F115W, F150W, F200W, F277W, F356W, F410M, and F444W) and 16.8 arcmin 2 in our NIRISS parallel (F115W, F150W, F200W, F356W, and F444W). To maximize early community use of the Treasury data set, we publicly release the full reduced mosaics of public JWST imaging including 45 arcmin 2 NIRCam and 17 arcmin 2 NIRISS mosaics on and around the A2744 cluster, including the Hubble Frontier Field primary and parallel footprints.

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Cite This Study

Bezanson et al. (2024) studied this question.

synapsesocial.com/papers/6a108d20d13714ec9600079ahttps://doi.org/10.3847/1538-4357/ad66cf
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Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

  1. 1The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM Spectra for ∼700 Galaxies from $z$ ∼ 0.3–13 in A27442025
  2. 2Medium Bands, Mega Science: a JWST/NIRCam Medium-Band Imaging Survey of Abell 27442024
  3. 3The NIRSpec Wide GTO Survey2024 · 27 citations
  4. 4COSMOS-Web: Comprehensive Data Reduction for Wide-area JWST NIRCam Imaging2026 · 8 citations
  5. 5JADES NIRSpec initial data release for the Hubble Ultra Deep Field. Redshifts and line fluxes of distant galaxies from the deepest JWST Cycle 1 NIRSpec multi-object spectroscopy2024 · 171 citations