| Issue |
A&A
Volume 572, December 2014
|
|
|---|---|---|
| Article Number | L4 | |
| Number of page(s) | 12 | |
| Section | Letters | |
| DOI | https://doi.org/10.1051/0004-6361/201424607 | |
| Published online | 25 November 2014 | |
Online material
Appendix A: Additional plots and tables
Summary of stacked properties when stacking as a function of the UV continuum slope.
Summary of stacked properties when stacking as a function of stellar mass.
 |
Fig. A.1
Radial profiles and associated stacked images when stacking as a function of the UV continuum slope. Redshift and UV continuum bins are indicated in each case. Orange curves are the best-fit Gaussian to the radial profile, while red dashed curves represent the shape of the PACS-160 μm PSF. |
| Open with DEXTER | |
 |
Fig. A.1
continued. |
| Open with DEXTER | |
 |
Fig. A.1
continued. |
| Open with DEXTER | |
 |
Fig. A.2
Radial profiles and associated stacked images when stacking as a function of the stellar mass. Redshift and stellar mass bins are indicated in each case. Orange curves are the best-fitted Gaussian to the radial profile, while red dashed curves represent the shape of the PACS-160 μm PSF. |
| Open with DEXTER | |
 |
Fig. A.2
continued. |
| Open with DEXTER | |
 |
Fig. A.2
continued. |
| Open with DEXTER | |
© ESO, 2014
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