Open Access

Fig. 2.

image

Download original image

IR combined SED built from the ALMA-detected objects from the ALPINE sample, from Burgarella et al. (2020), and with the two stacks from Bethermin et al. (2020) and the associated uncertainty regions. We note that the four left-most points for the stacks are upper limits, as shown by the error bars reaching the bottom of the figure. The SEDs corresponding to optically thin modified black bodies are superimposed to the observed SEDs. Qualitatively, we can see that the IR-combined SED seems to be in agreement with greenish modified blackbody SEDs, that is Tdust ∼ 50–60 K. A qualitative analysis is performed later in this paper.

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.