Gallery

2.8 Gpc intermediate resolution

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Dark matter surface density, zooming in on a massive cluster in the centre. The video uses a logarithmic colour scale to better bring out faint objects.

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Combined gas surface density and temperature, zooming in on a massive cluster in the centre. Both the surface density and the temperature use a logarithmic colour scale. The temperature varies from blue to red, while the surface density determines the brightness.

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Stellar surface density, zooming in on a massive cluster in the centre. The brightness scales logarithmically with the stellar surface density.

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X-ray luminosity in the ROSAT band, zooming in on a massive cluster in the centre. The colour map scales logarithmically with the X-ray luminosity.

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Dark matter surface density evolution of a 20Mpc slice through the entire box. The video uses a fixed logarithmic colour scale to better bring out faint objects.

text

Combined gas surface density and temperature evolution of a 20Mpc slice through the entire box. Both quantities use a logarithmic colour scale. Temperature varies from blue to red, while the surface density determines the brightness.

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Stellar surface density evolution of a 20Mpc slice through the entire box. The video uses a fixed logarithmic colour scale to better bring out faint objects.

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Evolution of the X-ray luminosity in the ROSAT band in a 20Mpc slice through the entire box. The video uses a fixed logarithmic colour scale to better bring out faint objects.

1 Gpc high resolution

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Dark matter surface density, zooming in on a massive cluster in the centre. The video uses a logarithmic colour scale to better bring out faint objects.

text

Combined gas surface density and temperature, zooming in on a massive cluster in the centre. Both the surface density and the temperature use a logarithmic colour scale. The temperature varies from blue to red, while the surface density determines the brightness.

text

Stellar surface density, zooming in on a massive cluster in the centre. The brightness scales logarithmically with the stellar surface density.

text

X-ray luminosity in the ROSAT band, zooming in on a massive cluster in the centre. The colour map scales logarithmically with the X-ray luminosity.

text

Dark matter surface density evolution of a 20Mpc slice through the entire box. The video uses a fixed logarithmic colour scale to better bring out faint objects.

text

Combined gas surface density and temperature evolution of a 20Mpc slice through the entire box. Both quantities use a logarithmic colour scale. Temperature varies from blue to red, while the surface density determines the brightness.

text

Stellar surface density evolution of a 20Mpc slice through the entire box. The video uses a fixed logarithmic colour scale to better bring out faint objects.

text

Evolution of the X-ray luminosity in the ROSAT band in a 20Mpc slice through the entire box. The video uses a fixed logarithmic colour scale to better bring out faint objects.