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Archetype-based Redshift Estimation for the Dark Energy Spectroscopic Instrument Survey
Abhijeet Anand*, Julien Guy, Stephen Bailey, John Moustakas, J. Aguilar, S. Ahlen, A. S. Bolton, A. Brodzeller, D. Brooks, T. Claybaugh, S. Cole, A. de la Macorra, Biprateep Dey, K. Fanning, J. E. Forero-Romero, E. Gaztañaga, S. Gontcho A. Gontcho, G. Gutierrez, K. Honscheid, C. Howlett
*Corresponding author for this work
- Lawrence Berkeley National Laboratory
- Sienna College
- Boston University
- NSF’s National Optical-Infrared Astronomy Research Laboratory
- University of Utah
- University College London
- Durham University
- Universidad Nacional Autónoma de México
- University of Pittsburgh
- Stanford University
- SLAC National Accelerator Laboratory
- Universidad de los Andes Colombia
- Institute of Space Studies of Catalonia
- CSIC - Instituto de Ciencias del Espacio (ICE)
- Fermi National Accelerator Laboratory
- Ohio State University
- School of Mathematics and Physics
- University of Queensland
- University of California at Irvine
- Sorbonne Université
- Departament de Física
- Autonomous University of Barcelona
- Institute for High Energy Physics
- ICREA
- University of Sussex
- Universidad de Guanajuato
- Instituto Avanzado de Cosmología A. C.
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- Department of Physics and Astronomy
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- Perimeter Institute for Theoretical Physics
- University of California at Berkeley
- Instituto de Astrofísica de Andalucía - CSIC
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- CIEMAT
- Space Telescope Science Institute
- University of Michigan, Ann Arbor
- University of Florida
- CAS - National Astronomical Observatories
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