Fig. 7
Environment of the radio galaxy MRC1138. SPIRE 250 μm is shown in greyscale. The black contours are the (extended) LABOCA emission of the radio galaxy, indicating levels at 2.0, 4.0 and 6.0 mJy/beam. The circles with a diameter of 16′′ (the FWHM of SCUBA) indicate SCUBA emission (Stevens et al. 2003). The red contours show the location of the CO(1–0) emission (Emonts et al. 2013) associated to the spectroscopically confirmed Hα emitter # 229 at z = 2.15 (Kurk et al. 2004b). The CO levels are 0.134 and 0.168 mJy/beam.
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.