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[ascl:1803.008] FAST: Fitting and Assessment of Synthetic Templates

FAST (Fitting and Assessment of Synthetic Templates) fits stellar population synthesis templates to broadband photometry and/or spectra. FAST is compatible with the photometric redshift code EAzY (ascl:1010.052) when fitting broadband photometry; it uses the photometric redshifts derived by EAzY, and the input files (for examply, photometric catalog and master filter file) are the same. FAST fits spectra in combination with broadband photometric data points or simultaneously fits two components, allowing for an AGN contribution in addition to the host galaxy light. Depending on the input parameters, FAST outputs the best-fit redshift, age, dust content, star formation timescale, metallicity, stellar mass, star formation rate (SFR), and their confidence intervals. Though some of FAST's functions overlap with those of HYPERZ (ascl:1108.010), it differs by fitting fluxes instead of magnitudes, allows the user to completely define the grid of input stellar population parameters and easily input photometric redshifts and their confidence intervals, and calculates calibrated confidence intervals for all parameters. Note that FAST is not a photometric redshift code, though it can be used as one.

Code site:
https://github.com/jamesaird/FAST
Appears in:
http://adsabs.harvard.edu/abs/2009ApJ...700..221K http://adsabs.harvard.edu/abs/2017MNRAS.465.3390A http://adsabs.harvard.edu/abs/2018MNRAS.474.1225A
Bibcode:
2018ascl.soft03008K
Preferred citation method:

http://adsabs.harvard.edu/abs/2009ApJ...700..221K. Please also cite http://adsabs.harvard.edu/abs/2017MNRAS.465.3390A and/or http://adsabs.harvard.edu/abs/2018MNRAS.474.1225A if using the features described in those papers.


ascl:1803.008
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