The thesan project: public data release of radiation-hydrodynamic simulations matching reionization-era JWST observations

Author:

Garaldi Enrico12ORCID,Kannan Rahul3ORCID,Smith Aaron4ORCID,Borrow Josh5ORCID,Vogelsberger Mark56ORCID,Pakmor Rüdiger1ORCID,Springel Volker1ORCID,Hernquist Lars7,Galárraga-Espinosa Daniela1ORCID,Yeh Jessica Y -C8,Shen Xuejian59ORCID,Xu Clara5ORCID,Neyer Meredith5ORCID,Spina Benedetta10ORCID,Almualla Mouza7ORCID,Zhao Yu11ORCID

Affiliation:

1. Max Planck Institute for Astrophysics , Karl-Schwarzschild-Str. 1, D-85741 Garching , Germany

2. Institute for Fundamental Physics of the Universe , via Beirut 2, I-34151 Trieste , Italy

3. Department of Physics and Astronomy, York University , 4700 Keele Street, Toronto, ON M3J 1P3 , Canada

4. Department of Physics, The University of Texas at Dallas , 800 W Campbell Rd, Richardson, TX 75080 , USA

5. Department of Physics & Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology , Cambridge, MA 02139 , USA

6. The NSF AI Institute for Artificial Intelligence and Fundamental Interactions, Massachusetts Institute of Technology , Cambridge, MA 02139 , USA

7. Center for Astrophysics | Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138 , USA

8. Department of Physics, Stanford University , 382 Via Pueblo Mall, Stanford, CA 94305 , USA

9. TAPIR, California Institute of Technology , Pasadena, CA 91125 , USA

10. Argelander Institut für Astronomie , Auf dem Hügel 71, D-53121 Bonn , Germany

11. Department of Physics and Astronomy, University of Southern California , Los Angeles, CA 90007 , USA

Abstract

ABSTRACT Cosmological simulations serve as invaluable tools for understanding the Universe. However, the technical complexity and substantial computational resources required to generate such simulations often limit their accessibility within the broader research community. Notable exceptions exist, but most are not suited for simultaneously studying the physics of galaxy formation and cosmic reionization during the first billion years of cosmic history. This is especially relevant now that a fleet of advanced observatories (e.g. James Webb Space Telescope, Nancy Grace Roman Space Telescope, SPHEREx, ELT, SKA) will soon provide an holistic picture of this defining epoch. To bridge this gap, we publicly release all simulation outputs and post-processing products generated within the thesan simulation project at www.thesan-project.com. This project focuses on the z ≥ 5.5 Universe, combining a radiation-hydrodynamics solver (arepo-rt), a well-tested galaxy formation model (IllustrisTNG) and cosmic dust physics to provide a comprehensive view of the Epoch of Reionization. The thesan suite includes 16 distinct simulations, each varying in volume, resolution, and underlying physical models. This paper outlines the unique features of these new simulations, the production and detailed format of the wide range of derived data products, and the process for data retrieval. Finally, as a case study, we compare our simulation data with a number of recent observations from the James Webb Space Telescope, affirming the accuracy and applicability of thesan. The examples also serve as prototypes for how to utilize the released data set to perform comparisons between predictions and observations.

Funder

NASA

NSF

Publisher

Oxford University Press (OUP)

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