Weak Evolution of Cosmic HI Abundance in the Past 4.5 Billion Years

Zenodo (CERN European Organization for Nuclear Research) 2026 Open access

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Authors: Chuan-Peng Zhang, Hong Guo, Yizhou Gu, A. Saintonge, Xiaohu Yang, D. Scholte, Ming Zhu, Peng Jiang, Hu Zou, Manasvee Saraf, Wenlin Ma, Yirong Wang
+38 more Zheng Zheng, Z. Ding, J. Aguilar, Steven P. Ahlen, D. Bianchi, D. Brooks, Todd Claybaugh, Axel de la Macorra, P. Doel, ENRIQUE GAZTAÑAGA, Gaston Gutierrez, Mustapha Ishak, R. R. Joyce, Stéphanie Juneau, R. Kehoe, David P. Kirkby, Anthony Kremin, O. Lahav, C. Lamman, Martin Landriau, Laurent Le Guillou, Marc Manera, Aaron Meisner, R. Miquel, John Moustakas, S. Nadathur, Will J. Percival, Francisco Prada, Ignasi Pérez-Ràfols, Graziano Rossi, Eusebio Sanchez, David J. Schlegel, Michael S. Schubnell, Hee‐Jong Seo, Joseph Harry Silber, David Sprayberry, Gregory Tarlé, B A Weaver
DOI: 10.5281/zenodo.17790393
Cited by: 0

Abstract

Supplementary material to DESI+FASHI's publication "Inefficient Gas Conversion Drives the Decline in Cosmic Star Formation".

Fields of Study & Subjects

Galaxies: Formation Evolution Phenomena Cosmology and Gravitation Theories Astrophysics and Star Formation Studies

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
1 January 2026