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Euclid preparation. LVII. Observational expectations for redshift z < 7 active galactic nuclei in the Euclid Wide and Deep surveys
M. Selwood*, S. Fotopoulou, M. N. Bremer, L. Bisigello, H. Landt, E. Bañados, G. Zamorani, F. Shankar, D. Stern, E. Lusso, L. Spinoglio, V. Allevato, F. Ricci, A. Feltre, F. Mannucci, M. Salvato, R. A.A. Bowler, M. Mignoli, D. Vergani, F. La Franca
*Corresponding author for this work
- University of Bristol
- Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
- University of Padova
- Durham University
- Max Planck Institute for Astronomy
- University of Southampton
- California Institute of Technology
- INAF - Osservatorio Astrofisico di Arcetri
- University of Florence
- National Institute for Astrophysics (INAF)
- Osservatorio Astronomico di Capodimonte
- Roma Tre University
- Osservatorio Astronomico di Roma
- Max Planck Institute for Extraterrestrial Physics
- University of Manchester
- University of Surrey
- Osservatorio Astronomico di Brera
- Universitá di Bologna
- National Institute for Nuclear Physics
- Ludwig Maximilian University of Munich
- University of Genoa
- University of Naples Federico II
- University of Porto
- University of Turin
- Istituto Nazionale di Astrofisica (INAF)
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas - CIEMAT
- Port d'Informació Científica
- RWTH Aachen University
- University of Edinburgh
- ESRIN - ESA Centre for Earth Observation
- Urbanización Villafranca Del Castillo
- Université Claude Bernard Lyon 1
- European Space Research and Technology Centre
- University of Bonn
- University of Helsinki
- Niels Bohr Institute
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