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ODIN: Clustering Properties of Lyα Blobs at z ∼ 2.4 and 3.1

  • Authors: Byeongha Moon, Yujin Yang, Eric Gawiser, Kyoung-Soo Lee, Danisbel Herrera, Vandana Ramakrishnan, Nelson Padilla, Nicole M. Firestone, Seongjae Kim, Robin Ciardullo, Caryl Gronwall, Lucia Guaita, Ho Seong Hwang, Sang Hyeok Im, Woong-Seob Jeong, Ankit Kumar, Jaehyun Lee, Seong-Kook Lee, Julie B. Nantais, Changbom Park, Hyunmi Song

Byeongha Moon et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 2.

Observed ACFs of LABs at z ∼ 2.4 and 3.1 [ωobs = (ω − IC)/(1 + IC)]. Open markers are not used for fitting the correlation functions, because they could be the one-halo term. The black dashed–dotted lines represent the best-fit power-law function (Equation (3), β = 0.8), while the red solid lines are the best fit with Equation (6). The best-fit parameters are summarized in Table 1.

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