CONCERTO: Simulating the CO, [CII], and [CI] line emission of galaxies in a 117 deg2 field and the impact of field-to-field variance

Open Access

Fig. 18.

Level of relative uncertainty of the clustering component (the standard deviation of P(k)_clust divided by the average) of the [CII] power spectra (top panel) and the CO (bottom panel) for various LIM experiments (see Table 5). The different line styles correspond to different number of averaged channels (Δν).

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.