| Issue |
A&A
Volume 603, July 2017
|
|
|---|---|---|
| Article Number | C3 | |
| Number of page(s) | 6 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201629857e | |
| Published online | 20 July 2017 | |
Stellar content of extremely red quiescent galaxies at z > 2 (Corrigendum)
1 Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain
e-mail: martinlc@iac.es
2 Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
3 GRANTECAN S. A., 38712, Breña Baja, La Palma, Spain
Key words: galaxies: evolution / galaxies: high-redshift / cosmology: observations / errata, addenda
The calculation of the luminosities Lλ,rest(λrest) for all 20 galaxies in the sample from the original paper was underestimated by a factor (1 + z)4. This implies that the vertical axis of Figs. 5, 6 and A.1 in the paper should be multiplied by that factor. Here we include corrected figures. The conclusions of the paper are not affected by this correction.
 |
Fig. 5 Spectrum and photometry at rest corresponding to the best fits with two SSPs of E-MILES model (see Table 2) of spectroscopy or photometry for galaxies #40812 and #78891, indicating the decomposition of the young and the old component. |
 |
Fig. 6 Spectrum and photometry at rest corresponding to the best fits with two SSPs of BC03 model (see Table 2) of spectroscopy or photometry for galaxies #40812 and #78891, indicating the decomposition of the young and the old component. |
 |
Fig. A.1 Photometry at rest corresponding to the best fits with two SSPs of BC03 model (see Table 3) for the CL12 galaxies, except #40812 and #78891. |
 |
Fig. A.1 continued. |
 |
Fig. A.1 continued. |
© ESO, 2017
All Figures
|
Fig. 5 Spectrum and photometry at rest corresponding to the best fits with two SSPs of E-MILES model (see Table 2) of spectroscopy or photometry for galaxies #40812 and #78891, indicating the decomposition of the young and the old component. |
| In the text | |
|
Fig. 6 Spectrum and photometry at rest corresponding to the best fits with two SSPs of BC03 model (see Table 2) of spectroscopy or photometry for galaxies #40812 and #78891, indicating the decomposition of the young and the old component. |
| In the text | |
|
Fig. A.1 Photometry at rest corresponding to the best fits with two SSPs of BC03 model (see Table 3) for the CL12 galaxies, except #40812 and #78891. |
| In the text | |
|
Fig. A.1 continued. |
| In the text | |
|
Fig. A.1 continued. |
| In the text | |
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