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[ascl:1611.020] CMCIRSED: Far-infrared spectral energy distribution fitting for galaxies near and far

The Caitlin M. Casey Infra Red Spectral Energy Distribution model (CMCIRSED) provides a simple SED fitting technique suitable for a wide range of IR data, from sources which have only three IR photometric points to sources with >10 photometric points. These SED fits produce accurate estimates to a source's integrated IR luminosity, dust temperature and dust mass. CMCIRSED is based on a single dust temperature greybody fit linked to a MIR power law, fitted simultaneously to data across ∼5–2000 μm.

Code site:
http://www.as.utexas.edu/~cmcasey/cmcirsed.html
Appears in:
http://adsabs.harvard.edu/abs/2012MNRAS.425.3094C http://adsabs.harvard.edu/abs/2016arXiv161107410M
Bibcode:
2016ascl.soft11020C

ascl:1611.020
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