HIGHLIGHTS
SUMMARY
For Iν (250 µm)/Iν (500 µm) > 5, the authors see the same trends as for ν (250 µm) in all the Herschel bands, with the emissivity SED being systematically lower than model predictions (compare the black and purple lines for the same Iν (250 µm)/Iν (500 µm) value in Fig 7). For λ ≥ 160 µm the THEMIS model could match the average SEDs if scaled by a factor 1/1.4 for the Iν (250 µm)/Iν (500 µm)=5.5 bin and 1/1.9 for the Iν (250 µm)/Iν (500 µm . . .
If you want to have access to all the content you need to log in!
Thanks :)
If you don't have an account, you can create one here.