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\begin_body

\begin_layout Title
PySEDFit
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\begin_layout Date
January, 2016
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\begin_layout Section
Introduction
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\begin_layout Section
makeBBsed
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\begin_layout Subsection
makeBBsed parameters
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Parameter Name
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Values
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Description
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['galaxev']
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Specifies the format of the input model file containing rest frame spectrum
 information.
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If galaxev input files are used, dotsed specifies the .sed filename 
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If galaxev input files are used, fotfourcolour specifies the filename of
 the .4color file which contains parameter information about the models in
 the .sed file
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filter_dir
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Specifies the path to the folder where filter transmission curve files are
 located
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filter_names
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[string,string]
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Specifies the filenames of filter FTCs to be convolved with each processed
 spectrum.
 Each FTC file is assumed to have the format described SOMEWHERE
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redshifts
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['range', startValue, stopValue, stepValue] or ['values', value1, value2,
 ...
 , valueN]
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Specifies the redshifts to which each rest frame input spectrum will be
 shifted, if the range option is invoked, NumPy's arange function is used
 to create an array of redshifts, if the value option is used, an array
 is created from the specified values
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['madau', 'inoue']
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Secifies the IGM attenation law to be applied to each redshifted spectrum.
 Madau (1998) and Inoue (2010) are currently supported
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Specifies the IGM opacities of the specified attenuation law to be applied
 to each redshifted spectrum
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dust_law
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['calzetti1997', 'calzetti2000', 'lmc', 'smc', 'mw', 'dor30']
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ebvs
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cosmology
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models
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makeBBsed parameter descriptions
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fitSED
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Libraries
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\start_of_appendix
Appendices
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Sample Calculations
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Here, we'll want to see examples of all the non-trivial calculations you
 made during the lab and derivations used to propagate uncertainties.
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