alphabooalphabooalphaboo/* DOCUMENT lpb_limb_power(ufreq, vfreq, flux_weight, x, y, diameter, power)
Returns the Fourier transform, at spatial frequencies (UFREQ,VFREQ), of
a center-to-limb darkened disk of diameter DIAMETER, centered at coordinates (X,Y).
The brightness distribution o, if expressed versus mu, which is the cosine
of the azimuth of a surface element of the star, follows
a law of power POWER, and is normalized for mu = 1 (center of the star).
o(mu) = mu^POWER.
POWER equal to zero makes the function equivalent to lpb_disk.
FLUX_WEIGHT is the intensity coefficient.
NB: also works if DIAMETER=0 or abs(ufreq,vfreq)=0.
SEE ALSO: lpb_functions
*/
1.00.0truemas0.0truemas0.0true0.00.01.0falsefalsealphaboo/* DOCUMENT lpb_limb_power(ufreq, vfreq, flux_weight, x, y, diameter, power)
Returns the Fourier transform, at spatial frequencies (UFREQ,VFREQ), of
a center-to-limb darkened disk of diameter DIAMETER, centered at coordinates (X,Y).
The brightness distribution o, if expressed versus mu, which is the cosine
of the azimuth of a surface element of the star, follows
a law of power POWER, and is normalized for mu = 1 (center of the star).
o(mu) = mu^POWER.
POWER equal to zero makes the function equivalent to lpb_disk.
FLUX_WEIGHT is the intensity coefficient.
NB: also works if DIAMETER=0 or abs(ufreq,vfreq)=0.
SEE ALSO: lpb_functions
*/
1.00.0truemas0.0truemas0.0true0.00.01.0falsefalsemas10.01.030.0falsestandardTuturial settings file for the example 2 :
Sharing parameters