mxlib
c++ tools for analyzing astronomical data and other tasks by Jared R. Males. [git repo]
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The shack hartmann wavefront sensor sensitivity function.
Provides the \( \beta_p \) parameter of Guyon, 2005 [9] for the shack hartmann WFS.
realT | is the floating point type used for calculations |
iosT | is an output stream type with operator << defined (default is std::ostream) |
#include <ao/analysis/aoWFS.hpp>
Public Member Functions | |
virtual realT | beta_p (int m, int n, realT D, realT d, realT r0) |
Get the photon noise sensitivity at a spatial frequency. More... | |
virtual realT | beta_r (int m, int n, realT D, realT d, realT r0) |
Get the read noise sensitivity at a spatial frequency. More... | |
Public Member Functions inherited from mx::AO::analysis::wfs< realT, std::ostream > | |
wfs () | |
Constructor. More... | |
virtual | ~wfs () |
Destructor. More... | |
virtual std::ostream & | dumpWFS (std::ostream &ios) |
Dump the details of the WFS to an io stream. More... | |
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inlinevirtual |
Get the photon noise sensitivity at a spatial frequency.
The photon noise sensitivity of the shack hartmann WFS
[in] | m | the spatial frequency index for u |
[in] | n | the spatial frequency index for v |
[in] | D | the telescope diameter |
[in] | d | the sub-ap spacing |
[in] | r0 | Fried's parameter |
Reimplemented from mx::AO::analysis::wfs< realT, std::ostream >.
Definition at line 242 of file aoWFS.hpp.
References mx::astro::constants::k().
Referenced by mx::AO::analysis::shwfs< realT, iosT >::beta_r().
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inlinevirtual |
Get the read noise sensitivity at a spatial frequency.
Here we assume beta_r = beta_p
[in] | m | the spatial frequency index for u |
[in] | n | the spatial frequency index for v |
[in] | D | the telescope diameter |
[in] | d | the sub-ap spacing |
[in] | r0 | Fried's parameter |
Reimplemented from mx::AO::analysis::wfs< realT, std::ostream >.
Definition at line 260 of file aoWFS.hpp.
References mx::AO::analysis::shwfs< realT, iosT >::beta_p().