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Far-infrared emission from dust was examined in detail through the spectral energy distribution (SED) of galaxies detected by AKARI in order to derive average SEDs as a function of infrared luminosity (Małek et al., this issue).
Fig. 2. A typical spectral energy distributions (SED) of starburst galaxies consists of two major components: an optical component (peaking at ~0.4 μm) due to photoionized gas and an infrared component (peaking at ~100 μm) due to dust.
MPSAHC system delivered specific energy demand (SED) of 11.51 kWh kg−1 while the maximum thermal collector and daily average transient collector efficiencies of 72.59% and 36.38% were achieved, respectively.
It was found that with MnOX catalyst, the toluene removal efficiency was nearly two times than that of without catalyst, but the HO* yield in gas streams was only one eighth of that without catalyst at a specific energy density (SED) of 50 Wh/m3.
To check the observability of a sublimation ring in the spectral energy distribution (SED) of thermal emission expected from a disk around Vega located at the distance of 7.6 pc from the earth, we take our formulae with M*. = 2.1M⊙ and L* = 59 L⊙ for compact spherical olivine particles.
The SED of both substrates after 24 hours were further enhanced at elevated pH 5.5.
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Not anywhere near as fiddly as the 4in iPhone SE of course.
Odds ratio SE of Coef.
Values are Mean ± SE of four experiments.
Values are Mean ± SE of 4 replicates.
Data are means ± SE of three replicates.
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