| Issue |
A&A
Volume 561, January 2014
|
|
|---|---|---|
| Article Number | A33 | |
| Number of page(s) | 30 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201322338 | |
| Published online | 20 December 2013 | |
Online material
Observed parameters of the galaxies.
Derived parameters of the galaxies.
 |
Fig. 10
20′′ × 20′′ SDSS composite g,r,i images of galaxies with m(3.4 μm)−m(4.6 μm) ≥ 2 mag. |
| Open with DEXTER | |
 |
Fig. 11
20′′ × 20′′ SDSS composite g,r,i images of galaxies with 2 mag >m(3.4 μm)−m(4.6 μm) ≥ 1.5 mag. |
| Open with DEXTER | |
 |
Fig. 11
continued. |
| Open with DEXTER | |
 |
Fig. 11
continued. |
| Open with DEXTER | |
 |
Fig. 12
20′′ × 20′′ SDSS composite g,r,i images of ten representative galaxies with m(3.4 μm)−m(4.6 μm) < 0.5 mag. |
| Open with DEXTER | |
 |
Fig. 13
Spectral energy distributions galaxies with m(3.4 μm)−m(4.6 μm) ≥ 2 mag. Observed SDSS optical spectra are shown by black solid lines; observed GALEX, SDSS and WISE monochromatic fluxes are shown by filled red circles. The WISE data are connected by a red solid line. The modelled SED shown by the blue line is a sum of stellar emission (green line) and ionised gas emission (magenta line). |
| Open with DEXTER | |
 |
Fig. 13
continued. |
| Open with DEXTER | |
 |
Fig. 14
Same as in Fig. 13 but for galaxies with 2 mag >m(3.4 μm)−m(4.6 μm) ≥ 1.5 mag. |
| Open with DEXTER | |
 |
Fig. 14
continued. |
| Open with DEXTER | |
 |
Fig. 14
continued. |
| Open with DEXTER | |
 |
Fig. 14
continued. |
| Open with DEXTER | |
 |
Fig. 14
continued. |
| Open with DEXTER | |
 |
Fig. 14
continued. |
| Open with DEXTER | |
 |
Fig. 14
continued. |
| Open with DEXTER | |
 |
Fig. 15
Same as in Fig. 13 but for galaxies with m(3.4 μm)−m(4.6 μm) < 0.5 mag. |
| Open with DEXTER | |
© ESO, 2013
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