EDP Sciences
Free Access
Issue
A&A
Volume 580, August 2015
Article Number A91
Number of page(s) 23
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361/201525728
Published online 07 August 2015

Online material

Table 4

Best fit SED parameters, model A.

Table 5

Best fit SED parameters, model B.

Table 6

Best fit SED parameters, model C.

Appendix A: Postage stamps of all candidate LAEs

We here show the postage stamps for all of our candidates in Fig. A.

thumbnail Fig. A.1

Postage stamps for all of our candidate LAEs. The field of view of all stamps is 10 × 10 arcsec. The large RGB picture shows an HST bvi colour composite made with the scale in each colour channel related to the true total intensity, with an arcsinh intensity scaling relation. This colouring scheme is similar to that described in Lupton et al. (2004). The white circle has a one arcsec radius – typically twice the size of the ground-based seeing disk.

Open with DEXTER


© ESO, 2015

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