ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

ASCL Code Record

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

Views: 4219

ascl:1403.014
Add this shield to your page
Copy the above HTML to add this shield to your code's website.