File:Comparison of the resolutions and box sizes of the FLAMINGO runs with cosmological, hydrodynamical simulations from the literature.jpg
Size of this preview: 600 × 600 pixels. Other resolutions: 240 × 240 pixels | 480 × 480 pixels | 768 × 768 pixels | 1,024 × 1,024 pixels | 1,351 × 1,351 pixels.
Original file (1,351 × 1,351 pixels, file size: 200 KB, MIME type: image/jpeg)
File information
Structured data
Captions
Summary
editDescriptionComparison of the resolutions and box sizes of the FLAMINGO runs with cosmological, hydrodynamical simulations from the literature.jpg |
English: "Second, the simulations use very large numbers of particles, up to 3 × 1011, which is the largest number of resolution elements for any existing cosmological hydrodynamical simulation run to z = 0. See Fig. 2 for a comparison with simulations from the literature."
"Comparison of the resolutions (baryonic particle mass or target cell mass; resolution increases along the y-axis) and box sizes of the FLAMINGO runs (filled red circles) with cosmological, hydrodynamical simulations from the literature that include radiative cooling, use a box size of at least (100 Mpc)3, and were run down to z = 0. The grey diagonal lines indicate the total number of baryonic resolution elements. The simulations from the literature shown are BAHAMAS (McCarthy et al. 2017), cosmo-OWLS (Le Brun et al. 2014), EAGLE (Schaye et al. 2015), Horizon-AGN (Dubois et al. 2014), IllustrisTNG (Springel et al. 2018), Magneticum (Dolag et al. 2016), MassiveBlack-II (Khandai et al. 2015), MillenniumTNG (Pakmor et al. 2022), OWLS (Schaye et al. 2010), SIMBA (Davé et al. 2019), and SLOW (Dolag et al. 2023)." |
Date | |
Source | https://academic.oup.com/mnras/article/526/4/4978/7246074 |
Author | Authors of the study: Schaye, Joop ; Kugel, Roi ; Schaller, Matthieu ; Helly, John C. ; Braspenning, Joey ; Elbers, Willem ; McCarthy, Ian G. ; van Daalen, Marcel P. ; Vandenbroucke, Bert ; Frenk, Carlos S. ; Kwan, Juliana ; Salcido, Jaime ; Bahé, Yannick M. ; Borrow, Josh ; Chaikin, Evgenii ; Hahn, Oliver ; Huško, Filip ; Jenkins, Adrian ; Lacey, Cedric G. ; Nobels, Folkert S. J. |
Licensing
editThis file is licensed under the Creative Commons Attribution 4.0 International license.
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 17:16, 22 December 2023 | 1,351 × 1,351 (200 KB) | Prototyperspective (talk | contribs) | Uploaded a work by Authors of the study: Schaye, Joop ; Kugel, Roi ; Schaller, Matthieu ; Helly, John C. ; Braspenning, Joey ; Elbers, Willem ; McCarthy, Ian G. ; van Daalen, Marcel P. ; Vandenbroucke, Bert ; Frenk, Carlos S. ; Kwan, Juliana ; Salcido, Jaime ; Bahé, Yannick M. ; Borrow, Josh ; Chaikin, Evgenii ; Hahn, Oliver ; Huško, Filip ; Jenkins, Adrian ; Lacey, Cedric G. ; Nobels, Folkert S. J. from https://academic.oup.com/mnras/article/526/4/4978/7246074 with UploadWizard |
You cannot overwrite this file.
File usage on Commons
There are no pages that use this file.