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[ascl:1403.014] T(dust) as a function of sSFR

This IDL code returns the dust temperature of a galaxy from its redshift, SFR and stellar mass; it can also predict the observed monochromatic fluxes of the galaxy. These monochromatic fluxes correspond to those of a DH SED template with the appropriate dust temperature and the appropriate normalization. Dust temperatures and fluxes predictions are only valid and provided in the redshift, stellar mass, SSFR and wavelength ranges 0 < z < 2.5, Mstar> 10^10 Msun, 10^-11 < SSFR[yr-1]< 10^-7 and 30um < lambda_rest < 2mm.

Code site:
http://www.mpe.mpg.de/ir/Research/PEP/Tdust_sSFR
Described in:
http://adsabs.harvard.edu/abs/2014A%26A...561A..86M
Bibcode:
2014ascl.soft03014M

Views: 1587

ascl:1403.014
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