T(dust) as a function of sSFR

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T(dust) as a function of sSFR

Post by owlice » Tue Mar 18, 2014 3:51 am

T(dust) as a function of sSFR

Abstract: 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.

Credit: Magnelli, Benjamin

Site: https://www.mpe.mpg.de/ir/Research/PEP/Tdust_sSFR

Bibcode: 2014ascl.soft03014M

Preferred citation method: http://adsabs.harvard.edu/abs/2014A%26A...561A..86M

ID: ascl:1403.014
Last edited by Ada Coda on Sun Sep 06, 2020 7:45 pm, edited 1 time in total.
Reason: Updated code entry.
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