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Stacked Average Far infrared Spectrum of Dusty Star forming Galaxies from the Herschel/SPIRE Fourier Transform Spectrometer

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Figure

Figure 1. Top:Total infrared luminosities (rest-frame 8 Distribution of redshifts for sources included in each of the five redshift bins: (a) 115 sources with 0.005 < z < 0.05, (b)34 sources with 0.05 < z < 0.2, (c) 12 sources with 0.2 < z < 0.5, (d) 8 sour
Figure 2. Top:The horizontal dashed line indicates Sand the water lines within the frequency (wavelength) range covered in this stack from 50toas a qualitative representation of the average spectrum of all of thedataset is split into redshift and luminosit
Figure 3. TopSignal-to-noise ratio. The horizontal dashed line indicates Sand dashed vertical lines showing the locations of main molecular emission lines
Figure 4.Same as Figure(wavelength) covered by the stack from 480 GHz to 1760 GHz (170[C I](2 3, but for the redshift range 0.05 < z < 0.2
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