cosmICweb: Cosmological Initial Conditions for Zoom-in Simulations in the Cloud

We present the online service cosmICweb ( COSM ological I nitial C onditions on the WEB ) - the first database and web interface to store, analyze, and disseminate initial conditions for zoom simulations of objects forming in cosmological simulations: from galaxy clusters to galaxies and more. Specifically, we store compressed information about the Lagrangian proto-halo patches for all objects in a typical simulation merger tree along with properties of the halo/galaxy across cosmic time. This enables a convenient web-based selection of the desired zoom region for an object fitting user-specified selection criteria. The information about the region can then be used with the MUSIC code to generate the zoom ICs for the simulation. In addition to some other simulations, we currently support all objects in the EAGLE simulation database, so that for example the Auriga simulations are easily reproduced, which we demonstrate explicitly. The framework is extensible to include other simulations through an API that can be added to an existing database structure and with which cosmICweb can then be interfaced. We make the web portal and database publicly available to the community.

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Publication Details

Journal
The Open Journal of Astrophysics
Published
2025-03-28
DOI
https://doi.org/10.33232/001c.133696
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
0.00
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article

cosmICweb: Cosmological Initial Conditions for Zoom-in Simulations in the Cloud

Oliver Hahn, John C Helly, Adrian Jenkins, Michael Buehlmann et al.
The Open Journal of Astrophysics
Solar and Space Plasma Dynamics
article

cosmICweb: Cosmological Initial Conditions for Zoom-in Simulations in the Cloud

Oliver Hahn, John C Helly, Adrian Jenkins, Michael Buehlmann, Lukas Winkler
article en

Abstract

We present the online service cosmICweb ( COSM ological I nitial C onditions on the WEB ) - the first database and web interface to store, analyze, and disseminate initial conditions for zoom simulations of objects forming in cosmological simulations: from galaxy clusters to galaxies and more. Specifically, we store compressed information about the Lagrangian proto-halo patches for all objects in a typical simulation merger tree along with properties of the halo/galaxy across cosmic time. This enables a convenient web-based selection of the desired zoom region for an object fitting user-specified selection criteria. The information about the region can then be used with the MUSIC code to generate the zoom ICs for the simulation. In addition to some other simulations, we currently support all objects in the EAGLE simulation database, so that for example the Auriga simulations are easily reproduced, which we demonstrate explicitly. The framework is extensible to include other simulations through an API that can be added to an existing database structure and with which cosmICweb can then be interfaced. We make the web portal and database publicly available to the community.

The Open Journal of AstrophysicsVol. 8
Argonne National Laboratory (US), University of Vienna (AT), Durham University (GB)
Openalex Percentile: Top 95%
Solar and Space Plasma Dynamics
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cosmICweb: Cosmological Initial Conditions for Zoom-in Simulations in the Cloud — Oliver Hahn, John C Helly, et al. · The Open Journal of Astrophysics (2025) | TGRS Research Map | TGRS