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The cosmic evolution of C IV absorbers at 1.4 < z < 4.5: insights from 100,000 systems in DESI quasars
Abhijeet Anand*, J. Aguilar, S. Ahlen, D. Bianchi, A. Brodzeller, D. Brooks, R. Canning, T. Claybaugh, A. Cuceu, A. de la Macorra, P. Doel, S. Ferraro, A. Font-Ribera, J. E. Forero-Romero, E. Gaztañaga, S. Gontcho A Gontcho, G. Gutierrez, J. Guy, H. K. Herrera-Alcantar, M. Ishak
*Corresponding author for this work
- Lawrence Berkeley National Laboratory
- Boston University
- University of Milan
- Osservatorio Astronomico di Brera
- University College London
- Universidad Nacional Autónoma de México
- University of California at Berkeley
- Institute for High Energy Physics
- Universidad de los Andes Colombia
- Institute of Space Studies of Catalonia
- CSIC - Instituto de Ciencias del Espacio (ICE)
- Fermi National Accelerator Laboratory
- Institut d 'Astrophysique de Paris
- Université Paris-Saclay
- University of Texas at Dallas
- NSF’s National Optical-Infrared Astronomy Research Laboratory
- Southern Methodist University
- Sorbonne Université
- Departament de Física
- Autonomous University of Barcelona
- ICREA
- Sienna College
- University of Wyoming
- Polytechnic University of Catalonia
- Sejong University
- CIEMAT
- University of Michigan, Ann Arbor
- Durham University
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