Dependency of halo concentration on mass, redshift and fossilness in Magneticum hydrodynamic simulations-Reference-Cited by-同舟云学术

Dependency of halo concentration on mass, redshift and fossilness in Magneticum hydrodynamic simulations

Author:

Ragagnin Antonio¹²³,Dolag Klaus³⁴,Moscardini Lauro⁵⁶⁷,Biviano Andrea⁸,D’Onofrio Mauro⁹^ORCID

Affiliation:

1. Leibniz-Rechenzentrum (LRZ), Boltzmannstrasse 1, D-85748 Garching, Germany

2. Excellence Cluster Universe, Boltzmannstrasse 2, D-85748 Garching, Germany

3. Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München, Scheinerstrasse 1, D-81679 München, Germany

4. Max-Planck-Institut für Astrophysik, Karl-Schwarzschild Strasse 1, D-85748 Garching bei München, Germany

5. Dipartimento di Fisica e Astronomia, Alma Mater Studiorum - Università di Bologna, via Piero Gobetti 93/2, I-40129 Bologna, Italy

6. INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, via Piero Gobetti 93/3, I-40129 Bologna, Italy

7. INFN, Sezione di Bologna, viale Berti Pichat 6/2, I-40127 Bologna, Italy

8. INAF - Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, I-34143 Trieste, Italy

9. Dipartimento di Fisica e Astronomia G. Galilei, Università di Padova, Vicolo Osservatorio 3, I-35122 Padova, Italy

Funder

Deutsche Forschungsgemeinschaft

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference89 articles.

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