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The environmental dependence of the structure of outer galactic discs in STAGES spiral galaxies

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Academic year: 2021

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Figure 3. The distribution of Hubble-type morphologies for the final field (light grey) and cluster (dark grey) spiral galaxy samples
Figure 4. Example profile fit. Left-hand column: ACS image (top) and bad pixel mask (bottom) showing the visually determined stellar disc limit a disc lim
Table 2. Determination of the ± 1 σ sky error from observed dark patches of sky in the STAGES ACS V-band imaging.
Figure 5. The distribution of break surface brightness μ brk . The surface brightness at the break radius μ brk for field (top row) and cluster (bottom row) galaxies as determined by DTM (left-hand column), AAS (centre column) and MEG (right-hand column)
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