Free Access

Fig. 23.

image

Spectral energy distributions of AGS4 and IDCANDELS 8923. Aperture photometry allows the separation between the local galaxy detected by HST (blue, and indicated by a white arrow in Fig. 21, IDCANDELS 8923) and the distant galaxy detected by ALMA (orange). The top panel shows the photometric redshift probability distribution of AGS4. As the Balmer break is well established in the K-band, we consider that this redshift determination is robust, and we adopt the derived redshift and stellar mass (1011.45 ± 0.2M) values for AGS4.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.