Free Access

Fig. 16

thumbnail

a) Dependence of the luminosity L(WISE) integrated over all WISE bands in the wavelength range 3.4 μm−22 μm on the total extinction-corrected luminosity L(total) in the wavelength range 0.1 μm−22 μm. Galaxies with EW(Hβ) ≥ 50 Å and EW(Hβ) < 50 Å are shown by red and blue symbols, respectively. Galaxies with m(3.4 μm)−m(4.6 μm) ≥1.5 mag are shown by large black filled circles. Solid line is the line of equal values; dotted and dashed lines are maximum likelihood fits to the sample galaxies with EW(Hβ) ≥ 50 Å and EW(Hβ) < 50 Å, respectively. Error bars are average dispersions of the data around the fits. b) Dependence of the luminosity L(WISE) on the luminosity L(absorbed) of the absorbed emission in the wavelength range 0.1 μm−3 μm. The meaning of lines and symbols is the same as in a).

This figure is made of several images, please see below:

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.