mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
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Wrapper for a native array to pass to levmarInterface, with Airy details.
Definition at line 220 of file fitAiry.hpp.
#include <math/fit/fitAiry.hpp>
Public Attributes | |
realT * | data { nullptr } |
Pointer to the array. | |
size_t | nx { 0 } |
X dimension of the array. | |
size_t | ny { 0 } |
Y dimension of the array. | |
realT | cenObs { 0 } |
is the ratio of the circular central obscuration diameter to the diameter. | |
realT | ps { 0 } |
the platescale in \( (\lambda/D)/pixel \) | |
realT mx::math::fit::array2FitAiry< realT >::cenObs { 0 } |
is the ratio of the circular central obscuration diameter to the diameter.
Definition at line 226 of file fitAiry.hpp.
realT* mx::math::fit::array2FitAiry< realT >::data { nullptr } |
Pointer to the array.
Definition at line 222 of file fitAiry.hpp.
size_t mx::math::fit::array2FitAiry< realT >::nx { 0 } |
X dimension of the array.
Definition at line 223 of file fitAiry.hpp.
size_t mx::math::fit::array2FitAiry< realT >::ny { 0 } |
Y dimension of the array.
Definition at line 224 of file fitAiry.hpp.
realT mx::math::fit::array2FitAiry< realT >::ps { 0 } |
the platescale in \( (\lambda/D)/pixel \)
Definition at line 227 of file fitAiry.hpp.