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Euclid preparation. XXXIX. The effect of baryons on the halo mass function
T. Castro*, S. Borgani, M. Costanzi, J. Dakin, K. Dolag, A. Fumagalli, A. Ragagnin, A. Saro, A. M.C. Le Brun, N. Aghanim, A. Amara, S. Andreon, N. Auricchio, M. Baldi, S. Bardelli, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann
*Corresponding author for this work
- Osservatorio Astronomico di Trieste
- National Institute for Nuclear Physics
- University of Trieste
- University of Zurich
- Ludwig Maximilian University of Munich
- Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
- Universitá di Bologna
- Observatoire de Paris
- Université Paris-Saclay
- University of Portsmouth
- Osservatorio Astronomico di Brera
- Max Planck Institute for Extraterrestrial Physics
- National Institute for Astrophysics (INAF)
- University of Genoa
- University of Naples Federico II
- Osservatorio Astronomico di Capodimonte
- Universidade do Porto
- University of Turin
- Istituto Nazionale di Astrofisica (INAF)
- Institute for High Energy Physics
- Port d'Informació Científica
- RWTH Aachen University
- Osservatorio Astronomico di Roma
- University of Edinburgh
- University of Manchester
- Urbanización Villafranca Del Castillo
- Université Claude Bernard Lyon 1
- Swiss Federal Institute of Technology Lausanne
- Institut national de physique nucléaire et de physique des particules
- University College London
- University of Lisbon
- University of Geneva
- University of Oxford
- European Space Research and Technology Centre
- University of Bonn
- California Institute of Technology
- ESRIN - ESA Centre for Earth Observation
Research output: Contribution to journal › Article › Scientific › peer-review
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