SpecDG¶
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class
pydirtygrid.SpecDG.SpecDG[source]¶ Read in the mapping file for all spectra
Returns: (self.)plan: Table
table containing the identification of each spectrum, as well as its parameters
- (self.)seds: list
empty list to save the spectra if you want to
Methods Summary
findFile(file_id)Returns the full filename for a given GID from the spectrum mapping. findGidFromParam(grain, geom, sf_type, ...)Returns the GID given a set of parameters findParamsFromGid(thisgid)Returns the parameter values for a given GID spec2Phot(trans_curve, trans_waves, wave0[, ...])Compute the new photometry specGet(filename)Save a spectrum from the filename specPlot([ind])Plot SEDs, either giving a specific index of which if more that Methods Documentation
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findFile(file_id)[source]¶ Returns the full filename for a given GID from the spectrum mapping.
Returns: filepath+filename: string
the absolute path and name of the .fits file
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findGidFromParam(grain, geom, sf_type, metal, age, sfr, tau)[source]¶ Returns the GID given a set of parameters (If you want to plot or something)
Parameters: grain: string
type of grain
geom: string
geometry
sf_type: string
star formation type
metal: float
metallicity
age: float
age of the stellar population
sfr: float
star formation rate
tau: float
optical depth
Returns: file_gid: string
identification number of the spectrum with the given set
of parameters
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findParamsFromGid(thisgid)[source]¶ Returns the parameter values for a given GID (Used later to update the cube)
Parameters: thisgid: string
identification number of the spectrum
Returns: thisgt, thisgm, thissf, thismt, thissa, thissr, thista: integers
indices of the parameter values for the given spectrum,
in the multidimensional photometry cube
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spec2Phot(trans_curve, trans_waves, wave0, energy=1)[source]¶ Compute the new photometry
Parameters: trans_curve: array
transmission curve of the new filter /!Alread read, as an array
trans_waves: array
wavelengths of the new filter
wave0: float
center/effective wavelength of the new filter
energy: integer (Optional)
specification for integration with energy(=1, default) or photons
Returns: newcube: array(3, 6, 2, 5, 50, 29, 25) (float)
new photometry cube