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BEACON: JWST NIRCam Pure-parallel Imaging Survey. III. Constraints on the Ultraviolet Luminosity Function and the Clustering of z ∼ 7–14 Galaxies

  • Authors: Kimi C. Kreilgaard, Charlotte A. Mason, Takahiro Morishita, Yechi Zhang, Viola Gelli, Nicha Leethochawalit, Tommaso Treu, Michele Trenti, Abdurro'uf, Hakim Atek, Maruša Bradac, Larry D. Bradley, Andrew J. Bunker, Novan Saputra Haryana, Matthew J. Hayes, Zhaoran Liu, Vihang Mehta, Marc Rafelski, Guido Roberts-Borsani, Claudia Scarlata, Massimo Stiavelli, Ryo A. Sutanto, Kosuke Takahashi, Benedetta Vulcani

Kimi C. Kreilgaard et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 1.

Sky distribution of the 36 fields included in BEACON DR2 (orange circles), overlaid on a temperature map from the Wilkinson Microwave Anisotropy Probe 7 yr data (N. Jarosik et al. 2011). We also show some JWST legacy fields (gray squares): COSMOS-Web (C. M. Casey et al. 2023), PRIMER-UDS (J. S. Dunlop et al. 2021), CEERS-EGS (S. L. Finkelstein et al. 2025), JADES-GOODS-South, and JADES-GOODS-North (D. J. Eisenstein et al. 2026). The symbol sizes do not represent the true sky size, but they are roughly scaled to the corresponding survey area.

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