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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 3.

Histogram showing the absolute UV magnitudes for galaxy candidates in each of the three dropout selections. The UV magnitudes are measured as the average flux in the rest-frame 1450–1550 Å wavelength range based on a power law fitted to the UV continuum sampled by the available NIRCam photometry for each source. We note that the F150W-dropout candidate is not included in our final sample, as its nondetection in independent overlapping datasets suggests it is likely not a galaxy (see Section 3.2).

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