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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 7.

Similar to Figure 3 but for XMM-z2.4-B. In the top-left, bottom-left, and bottom-right panels, green dashed contours mark the LATIS Lyα absorption isosurface at δF/σmap = −2 (see Footnote  for the definition of this quantity), reported by A. B. Newman et al. (2025a). These contours trace regions of enhanced H I absorption around the highest-significance LATIS peaks identified in their analysis, in three redshift slices corresponding to D1-00, D1-01, and D1-05, respectively, whose centers are indicated by green crosses. In the bottom-right panel, the field center is shifted by ≈0.5 deg eastward to show D1-05. Yellow dotted contours mark the projected LATIS LBG overdensity contour at δLBG/σ = 2, and yellow diamonds indicate individual LBG/QSO positions at these redshift slices from LATIS. The background gray scale is the 2D LAE surface density map. The downward triangles in the two left panels mark spectroscopic sources overlapping with D1-00; while these sources are not formally part of XMM-z2.4-B in our 3D detection, they reside in a 2D-selected protocluster whose angular extent overlaps significantly with D1-00 (see text for more discussion).

An interactive version of this figure is available in the online article.

An interactive version of this figure is available.

An interactive version of this figure is available in the online journal.

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