PSF Data Sources

Sources of necessary data for PSF fitting

blurreddata.blur(mu, variance)

The gaussian weights used in the convolution.

class blurreddata.BlurredData(spectra, sigma, measurement_sigma=0.0)

Class defining the Solar Spectrum and useful functions.

class blurreddata.SAO2010(sigma=array([0.35, 0.36, 0.37, 0.38, 0.39, 0.4, 0.41, 0.42, 0.43, 0.44, 0.45, 0.46, 0.47, 0.48, 0.49, 0.5, 0.51, 0.52, 0.53, 0.54, 0.55, 0.56, 0.57, 0.58, 0.59, 0.6]))

Implements the Solar Spectrum Class with the SAO2010 data.

class blurreddata.O3BDM(sigma=array([0.35, 0.36, 0.37, 0.38, 0.39, 0.4, 0.41, 0.42, 0.43, 0.44, 0.45, 0.46, 0.47, 0.48, 0.49, 0.5, 0.51, 0.52, 0.53, 0.54, 0.55, 0.56, 0.57, 0.58, 0.59, 0.6]), temperature=243)

Implements the Brion–Daumont–Malicet (BDM) O3 Cross Section.