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Nāpōwawā‘enakaulua: A Close Quasar Pair at Cosmic Dawn in the Aether Survey

  • Authors: Silvia Onorato, Emanuele Paolo Farina, Roberto Decarli, Klaudia Protušová, Elia Pizzati, Debora Pelliccia, Devin S. Chu, Larry Lindsey Kimura, Leinani Lozi, Emily Peavy, Fabrizio Arrigoni–Battaia, Eduardo Bañados, Aaron J. Barth, Silvia Belladitta, Manuela Bischetti, Sarah E. I. Bosman, Hyunseop Choi, Tiago Costa, Anna-Christina Eilers, Xiaohui Fan, Simona Gallerani, Thomas R. Geballe, Anniek J. Gloudemans, Eunchong Kim, Brian C. Lemaux, Weizhe Liu, 伟哲 刘, Yoshiki Matsuoka, Chiara Mazzucchelli, Atsuko Nitta, Jan-Torge Schindler, Andrew W. Stephens, Hyewon Suh, Fabian Walter, Feige Wang, Jinyi Yang

Silvia Onorato et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 4.

Projected quasar autocorrelation function 〈wp〉( < rp) as a function of the projected radius rp. The solid blue, pink, orange, and green lines represent the power-law fit from A.-C. Eilers et al. (2024), J. Huang et al. (2026b), F. Wang et al. (2026), J. Arita et al. (2023), respectively, with the dashed lines being extrapolations. The black star indicates the clustering amplitude measured for Nāpōwawā‘enakaulua.

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