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Euclid preparation. LV. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
H. Böhringer*, G. Chon, O. Cucciati, H. Dannerbauer, M. Bolzonella, G. De Lucia, A. Cappi, L. Moscardini, C. Giocoli, G. Castignani, N. A. Hatch, S. Andreon, E. Bañados, S. Ettori, F. Fontanot, H. Gully, M. Hirschmann, M. Maturi, S. Mei, L. Pozzetti
*Corresponding author for this work
- Max Planck Institute for Extraterrestrial Physics
- Ludwig Maximilian University of Munich
- Max Planck Institute for Physics
- Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
- University of La Laguna
- Osservatorio Astronomico di Trieste
- Université Côte d'Azur
- Universitá di Bologna
- National Institute for Nuclear Physics
- University of Nottingham
- Osservatorio Astronomico di Brera
- Max Planck Institute for Astronomy
- University of Trieste
- Swiss Federal Institute of Technology Lausanne
- Heidelberg University
- Université Paris Diderot - Paris 7
- University of the Western Cape
- Université Paris-Saclay
- Urbanización Villafranca Del Castillo
- International School for Advanced Studies
- National Institute for Astrophysics (INAF)
- University of Genoa
- University of Naples Federico II
- Osservatorio Astronomico di Capodimonte
- 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
- CSIC - Institute of Space Sciences
- Institute of Space Studies of Catalonia
- Osservatorio Astronomico di Roma
- European Space Research and Technology Centre
- University of Bonn
- California Institute of Technology
- Astronomical Observatory of the Autonomous Region of the Aosta Valley (OAVdA)
- University of Helsinki
- University of Edinburgh
- Niels Bohr Institute
Research output: Contribution to journal › Article › Scientific › peer-review
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