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Unveiling the Cosmic Gems Arc at z ∼ 10 with JWST NIRCam

  • Authors: Larry D. Bradley, Angela Adamo, Eros Vanzella, Keren Sharon, Gabriel Brammer, Dan Coe, Jose M. Diego, Vasily Kokorev, Guillaume Mahler, Masamune Oguri, Abdurro'uf, Rachana Bhatawdekar, Lise Christensen, Seiji Fujimoto, Takuya Hashimoto, Tiger Y.-Y Hsiao, Akio K. Inoue, Yolanda Jiménez-Teja, Matteo Messa, Colin Norman, Massimo Ricotti, Yoichi Tamura, Rogier A. Windhorst, Xinfeng Xu, Adi Zitrin

Larry D. Bradley et al 2025 The Astrophysical Journal 991 .

  • Provider: AAS Journals

Caption: Figure 7.

Best-fit EAZYPY photometric redshifts for the Cosmic Gems Arc using the photometry measured in both elliptical Kron apertures and isophotal source segments. The top plots show results using the non-PSF-matched photometry, while the bottom plots are for the PSF-matched photometry. The measured fluxes are shown as blue data points or triangle upper limits. Nondetections are plotted as upper limits at the 2σ level. The best-fit EAZYPY SED model is shown in orange, with squares indicating the expected photometry in a given band. The best-fit EAZYPY SED for the low-redshift (z < 7) solution is shown in green. To the right of each SED, we also plot the P(z) posterior redshift probability distributions. The Cosmic Gems Arc has a best-fit photometric redshift of zphot = 10.2, with low-redshift solutions ruled out at high significance.

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