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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 2.

Left: NB497 and NB503 filters of G20, shown in comparison to the ODIN N501 filter. The three filters have significant overlap. Right: the offset between spectroscopic and tomographic redshifts, Δz = zspec − ztomo, is plotted together with the N501 transmission. The median value of the offset is 0, and its standard deviation is 0.005, an order of magnitude smaller than the FWHM of the N501 filter.

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