This paper describes wave-optics Monte Carlo simulation results to asses the impact of laser guide star wavefront sensor nonlinearity with elongated sodium beacons on the residual wavefront error for the Thirty Meter Telescope Narrow Field InfraRed Adaptive Optics System, which is a laser guide star multi-conjugate adaptive optics system intended to provide near-diffraction limited performance in the near infrared over a 30 arcsec diameter field of view
Adaptive optics (AO) is essential for many elements of the science case for the Thirty Meter Telesco...
The Thirty Meter Telescope (TMT) will utilize adaptive optics to achieve near diffraction-limited im...
Sodium laser guide stars (LGSs) allow, in theory, Adaptive Optics (AO) systems to reach a full sky c...
This paper describes wave-optics Monte Carlo simulation results to asses the impact of laser guide s...
This paper describes modeling and simulation results for the Thirty Meter Telescope on the degradati...
This paper describes the modeling efforts undertaken in the past couple of years to derive wavefront...
We recently introduced matched filtering in the context of astronomical Shack-Hartmann wavefront sen...
This paper discusses point spread function reconstruction (PSFR) simulations for laser guide star (L...
Adaptive optics (AO) is essential for many elements of the science case for the Thirty Meter Telesco...
We describe modeling and simulation results for the Thirty Meter Telescope on the degradation of sod...
A Monte Carlo sky coverage model for laser guide star adaptive optics systems was proposed by Clare ...
For Extremely Large Telescope (ELT) adaptive optics (AO) systems, multiple Sodium Laser Guide Star (...
The very high-order multi-conjugate adaptive optics (MCAO) systems proposed for future giant telesco...
Laser tomography and multiconjugate adaptive optics are under development for ground-based extremely...
When using a laser guide star (LGS) adaptive optics (AO) system, quasi-static aberrations are observ...
Adaptive optics (AO) is essential for many elements of the science case for the Thirty Meter Telesco...
The Thirty Meter Telescope (TMT) will utilize adaptive optics to achieve near diffraction-limited im...
Sodium laser guide stars (LGSs) allow, in theory, Adaptive Optics (AO) systems to reach a full sky c...
This paper describes wave-optics Monte Carlo simulation results to asses the impact of laser guide s...
This paper describes modeling and simulation results for the Thirty Meter Telescope on the degradati...
This paper describes the modeling efforts undertaken in the past couple of years to derive wavefront...
We recently introduced matched filtering in the context of astronomical Shack-Hartmann wavefront sen...
This paper discusses point spread function reconstruction (PSFR) simulations for laser guide star (L...
Adaptive optics (AO) is essential for many elements of the science case for the Thirty Meter Telesco...
We describe modeling and simulation results for the Thirty Meter Telescope on the degradation of sod...
A Monte Carlo sky coverage model for laser guide star adaptive optics systems was proposed by Clare ...
For Extremely Large Telescope (ELT) adaptive optics (AO) systems, multiple Sodium Laser Guide Star (...
The very high-order multi-conjugate adaptive optics (MCAO) systems proposed for future giant telesco...
Laser tomography and multiconjugate adaptive optics are under development for ground-based extremely...
When using a laser guide star (LGS) adaptive optics (AO) system, quasi-static aberrations are observ...
Adaptive optics (AO) is essential for many elements of the science case for the Thirty Meter Telesco...
The Thirty Meter Telescope (TMT) will utilize adaptive optics to achieve near diffraction-limited im...
Sodium laser guide stars (LGSs) allow, in theory, Adaptive Optics (AO) systems to reach a full sky c...