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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 5.

Examples of our observed photometry and SED fitting results for two F090W dropouts (purple) and two F115W dropouts (blue). Black open diamonds show the observed photometry in each band with errors, where the uncertainty range on the wavelength axis is determined from the half-power wavelengths of the passband, e.g., the wavelengths at which the transmission falls to 50% of its peak value. The colored curves are the best-fit SEDs from EAZY, while the colored circles indicate the corresponding predicted photometry. The insert panel shows the marginalized redshift posterior distribution, p(z), from the SED fitting. We also show image cutouts for each available filter for the given source, marking the dropout filter with a colored border. The 0﹩\mathop{.}\limits^{{\prime\prime} }﹩16 circular aperture in which fluxes are measured is shown on the F444W cutout.

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