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ODIN: Confirmation and 3D Reconstruction of Six Massive Protoclusters at Cosmic Noon

  • Authors: Ashley Ortiz, Vandana Ramakrishnan, Kyoung-Soo Lee, Arjun Dey, Yucheng Guo, Ethan Pinarski, Anand Raichoor, Francisco Valdes, J. Aguilar, S. Ahlen, Maria Celeste Artale, D. Bianchi, August Bliese, D. Brooks, R. Canning, Maria Candela Cerdosino, T. Claybaugh, A. Cuceu, A. de la Macorra, P. Doel, J. E. Forero-Romero, Eric Gawiser, E. Gaztañaga, S. Gontcho A Gontcho, Caryl Gronwall, Lucia Guaita, G. Gutierrez, H. K. Herrera-Alcantar, Ho Seong Hwang, Woong-Seob Jeong, R. Joyce, R. Kehoe, T. Kisner, A. Kremin, Ankit Kumar, O. Lahav, M. Landriau, Jaehyun Lee, Seong-Kook Lee, L. Le Guillou, M. Manera, A. Meisner, R. Miquel, Byeongha Moon, J. Moustakas, A. D. Myers, S. Nadathur, N. Palanque-Delabrouille, Changbom Park, W. J. Percival, I. Pérez-Ràfols, F. Prada, Eshwar Puvvada, G. Rossi, E. Sanchez, D. Schlegel, M. Schubnell, J. Silber, Hyunmi Song, D. Sprayberry, G. Tarlé, Paulina Troncoso Iribarren, Ana Sofía M. Uzsoy, B. A. Weaver, Yujin Yang, R. Zhou, H. Zou

Ashley Ortiz et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 10.

Histograms of ﹩{F}_{{\rm{Ly}}\alpha }^{{\rm{spec}}}﹩ for protocluster (filled) and field (hatched) samples at z ≈ 2.4 (top) and z ≈ 3.1 (bottom). The left (middle) panels show 3D (2D) protocluster member galaxies, while the right panels show galaxies identified as members by both 2D and 3D selection. Field galaxies are chosen to have local density δLAE,2D at the 50%-tile or below. Vertical solid (dashed) lines mark the median line fluxes of the protocluster (field) sample. The KS and AD test p-values, comparing the two distributions, are listed in the bottom right of each panel.

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