| Issue |
A&A
Volume 567, July 2014
|
|
|---|---|---|
| Article Number | A76 | |
| Number of page(s) | 32 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201423906 | |
| Published online | 14 July 2014 | |
Online material
Appendix A: Radio maps, host identifications and SEDs
In this Appendix we include Tables A.1 and A.2, which present the final magnitudes and fluxes of the multiband counterparts of the radio sources of the sample. Figures A.1−A.3 show the VLA-COSMOS radio maps and the optical/IR images of the sources, for which we easily can identify the host, for the FR IIs that lack of a clear point-like emission from the radio core and for the sources that we fail in the host identification, respectively. Figure A.4 collects the modeled SEDs of the radio galaxies selected in this work.
COSMOS multiwavelength counterparts of the sample.
COSMOS GALEX and Spitzer counterparts of the sample.
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Fig. A.1
Images of the radio sources selected in the COSMOS field associated with a host galaxy with I> 21 (see Table 1). The left image for each source is from the VLA-COSMOS survey; the right image shows radio contours and the host identification in the band labelled on top. The image size in arcsec is marked on the bottom of each panel. When necessary, we mark the identified host galaxy with a white circle. |
| Open with DEXTER | |
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Fig. A.1
continued. |
| Open with DEXTER | |
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Fig. A.1
continued. |
| Open with DEXTER | |
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Fig. A.1
continued. |
| Open with DEXTER | |
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Fig. A.2
Host identification for FR IIs that lack of a clear point-like emission from the radio core. The labels and marks are as in Fig. A.1. |
| Open with DEXTER | |
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Fig. A.3
Images of the failed host identification. The labels and marks are as in Fig. A.1. |
| Open with DEXTER | |
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Fig. A.4
SEDs of the objects of the sample. The model is the green line, which includes the YSP (blue), the OSP (red), and the dust component(s) (cyan). The wavelengths on top of the plots correspond to observed wavelengths, while those on bottom are at rest frame. For the two spectroscopically confirmed quasars (objects 29 and 37) we only show the photometric points. |
| Open with DEXTER | |
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Fig. A.4
continued. |
| Open with DEXTER | |
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Fig. A.4
continued. |
| Open with DEXTER | |
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Fig. A.4
continued. |
| Open with DEXTER | |
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Fig. A.4
continued. |
| Open with DEXTER | |
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Fig. A.4
continued. |
| Open with DEXTER | |
© ESO, 2014
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