The Astrophysical Journal (Jan 2024)

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

  • Rachel Bezanson,
  • Ivo Labbe,
  • Katherine E. Whitaker,
  • Joel Leja,
  • Sedona H. Price,
  • Marijn Franx,
  • Gabriel Brammer,
  • Danilo Marchesini,
  • Adi Zitrin,
  • Bingjie Wang,
  • John R. Weaver,
  • Lukas J. Furtak,
  • Hakim Atek,
  • Dan Coe,
  • Sam E. Cutler,
  • Pratika Dayal,
  • Pieter van Dokkum,
  • Robert Feldmann,
  • Natascha M. Förster Schreiber,
  • Seiji Fujimoto,
  • Marla Geha,
  • Karl Glazebrook,
  • Anna de Graaff,
  • Jenny E. Greene,
  • Stéphanie Juneau,
  • Susan Kassin,
  • Mariska Kriek,
  • Gourav Khullar,
  • Michael Maseda,
  • Lamiya A. Mowla,
  • Adam Muzzin,
  • Themiya Nanayakkara,
  • Erica J. Nelson,
  • Pascal A. Oesch,
  • Camilla Pacifici,
  • Richard Pan,
  • Casey Papovich,
  • David J. Setton,
  • Alice E. Shapley,
  • Renske Smit,
  • Mauro Stefanon,
  • Edward N. Taylor,
  • Christina C. Williams

DOI
https://doi.org/10.3847/1538-4357/ad66cf
Journal volume & issue
Vol. 974, no. 1
p. 92

Abstract

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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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