Modeling a MEMS deformable mirror using non-parametric estimation techniques
(2010)
Journal Article
Guzman, D., de Cos Juez, F. J., Myers, R., Guesalaga, A., & Sanchez Lasheras, F. (2010). Modeling a MEMS deformable mirror using non-parametric estimation techniques. Optics Express, 18(20), 21356-21369. https://doi.org/10.1364/oe.18.021356
Richard Myers' Outputs (40)
Durham adaptive optics real-time controller (2010)
Journal Article
Basden, A., Geng, D., Myers, R., & Younger, E. (2010). Durham adaptive optics real-time controller. Applied optics, 49(32), 6354-6363. https://doi.org/10.1364/ao.49.006354The Durham adaptive optics (AO) real-time controller was initially a proof of concept design for a generic AO control system. It has since been developed into a modern and powerful central-processing-unit-based real-time control system, capable of us... Read More about Durham adaptive optics real-time controller.
Considerations for EAGLE from Monte Carlo adaptive optics simulation (2010)
Journal Article
Basden, A., Myers, R., & Butterley, T. (2010). Considerations for EAGLE from Monte Carlo adaptive optics simulation. Applied optics, 49(31), G1-G8. https://doi.org/10.1364/ao.49.0000g1The EAGLE instrument for the European Extremely Large Telescope is a multi-object integral field unit spectrograph that uses a multi-object adaptive optics (AO) system for wavefront correction of interesting lines of sight. We present a Monte Carlo A... Read More about Considerations for EAGLE from Monte Carlo adaptive optics simulation.
PSF halo reduction in adaptive optics using dynamic pupil masking (2009)
Journal Article
Osborn, J., Myers, R. M., & Love, G. D. (2009). PSF halo reduction in adaptive optics using dynamic pupil masking. Optics Express, 17(20), 17279-17292. https://doi.org/10.1364/oe.17.017279
Durham extremely large telescope adaptive optics simulation platform (2007)
Journal Article
Basden, A., Butterley, T., Myers, R., & Wilson, R. (2007). Durham extremely large telescope adaptive optics simulation platform. Applied optics, 46(7), 1089-1098. https://doi.org/10.1364/ao.46.001089Adaptive optics systems are essential on all large telescopes for which image quality is important. These are complex systems with many design parameters requiring optimization before good performance can be achieved. The simulation of adaptive optic... Read More about Durham extremely large telescope adaptive optics simulation platform.
Performance modeling of a wide-field ground-layer adaptive optics system (2006)
Journal Article
Andersen, D., Stoesz, J., Morris, S., Lloyd-Hart, M., Crampton, D., Butterley, T., …Wilson, R. (2006). Performance modeling of a wide-field ground-layer adaptive optics system. Publications of the Astronomical Society of the Pacific, 118(849), 1574-1590. https://doi.org/10.1086/509266Using five independent analytic and Monte Carlo simulation codes, we have studied the performance of wide-field ground-layer adaptive optics (GLAO), which can use a single, relatively low order deformable mirror to correct the wave-front errors from... Read More about Performance modeling of a wide-field ground-layer adaptive optics system.
WIde-field adaptive optics correction using a single rotating laser guide star (2006)
Journal Article
Morris, T., & Myers, R. (2006). WIde-field adaptive optics correction using a single rotating laser guide star. Monthly Notices of the Royal Astronomical Society, 370(4), 1783-1789. https://doi.org/10.1111/j.1365-2966.2006.10588.xThe problem of providing Adaptive Optics (AO) correction over a wide field of view is one that can be alleviated by using multiple conjugate AO (MCAO), or a low-altitude Laser Guide Star (LGS) that is projected to an altitude below any high layer tur... Read More about WIde-field adaptive optics correction using a single rotating laser guide star.
A Shack-Hartmann wavefront sensor projected on to the sky with reduced focal anisoplanatism (2006)
Journal Article
Butterley, T., Love, G., Wilson, R., Myers, R., & Morris, T. (2006). A Shack-Hartmann wavefront sensor projected on to the sky with reduced focal anisoplanatism. Monthly Notices of the Royal Astronomical Society, 368(2), 837-843. https://doi.org/10.1111/j.1365-2966.2006.10160.xA method for producing a laser guide star wavefront sensor for adaptive optics with reduced focal anisoplanatism is presented. A theoretical analysis and numerical simulations have been carried out and the results are presented. The technique, named... Read More about A Shack-Hartmann wavefront sensor projected on to the sky with reduced focal anisoplanatism.
Results from the adaptive optics coronagraph at the William Herschel Telescope (2005)
Journal Article
Thompson, S., Doel, A., Bingham, R., Charalambous, A., Myers, R., Bissonauth, N., …Talbot, G. (2005). Results from the adaptive optics coronagraph at the William Herschel Telescope. Monthly Notices of the Royal Astronomical Society, 364(4), 1203-1210. https://doi.org/10.1111/j.1365-2966.2005.09628.xDescribed here is the design and commissioning of a coronagraph facility for the 4.2-m William Herschel Telescope (WHT) and its Nasmyth Adaptive Optics for Multi-purpose Instrumentation (NAOMI). The use of the NAOMI system gives an improved image res... Read More about Results from the adaptive optics coronagraph at the William Herschel Telescope.
Multiconjugate adaptive optics: laboratory experience (2004)
Journal Article
Langlois, M., Saunter, C., Dunlop, C., Myers, R., & Love, G. (2004). Multiconjugate adaptive optics: laboratory experience. Optics Express, 12(8), 1689-1699
Laser beacon wave-front sensing without focal anisoplanatism (2002)
Journal Article
Buscher, D., Love, G., & Myers, R. (2002). Laser beacon wave-front sensing without focal anisoplanatism. Optics Letters, 27(3), 149-151. https://doi.org/10.1364/ol.27.000149Wave-front sensing from artificial beacons is normally performed by formation of a focused spot in the atmosphere and sensing of the wave-front distortions produced during the beam's return passage. We propose an alternative method that senses the di... Read More about Laser beacon wave-front sensing without focal anisoplanatism.
Recent developments in spectroscopy (2001)
Journal Article
Sharples, R., Allington-Smith, J., Buscher, D., Content, R., Haynes, R., & Myers, R. (2001). Recent developments in spectroscopy. New Astronomy Reviews, 45, 77-81. https://doi.org/10.1016/s1387-6473%2800%2900133-0
Wavefront correction using a self-referencing phase conjugation system based on a Zernike cell (2001)
Journal Article
Dale, S., Love, G., Myers, R., & Naumov, A. (2001). Wavefront correction using a self-referencing phase conjugation system based on a Zernike cell. Optics Communications, 191(1-2), 31-38. https://doi.org/10.1016/s0030-4018%2801%2901116-6A wavefront correction system was produced using a phase conjugating method based on a point diffraction interferometer, or Zernike cell. This has the main advantage that no separate reference beam is required. The PDI was constructed using an optica... Read More about Wavefront correction using a self-referencing phase conjugation system based on a Zernike cell.
The MARTINI adaptive optics instrument (2000)
Journal Article
Doel, A., Dunlop, C., Buscher, D., Myers, R., Sharples, R., & Major, J. (2000). The MARTINI adaptive optics instrument. New Astronomy, 5, 223-233
Dual-conjugate wavefront generation for adaptive optics (2000)
Journal Article
Kelly, T., Buscher, D., Clark, P., Dunlop, C., Love, G., Myers, R., …Zadrozny, A. (2000). Dual-conjugate wavefront generation for adaptive optics. Optics Express, 7(11), 368-374. https://doi.org/10.1364/oe.7.000368We present results of the isoplanatic performance of an astronomical adaptive optics system in the laboratory, by using a dual layer turbulence simulator. We describe how the performance of adaptive correction degrades with off-axis angle. These expe... Read More about Dual-conjugate wavefront generation for adaptive optics.
Binary adaptive optics: atmospheric wave-front correction with a half-wave phase shifter (1995)
Journal Article
Love, G. D., Andrews, N., Birch, P., Buscher, D., Doel, P., Dunlop, C., …Glindemann, A. (1995). Binary adaptive optics: atmospheric wave-front correction with a half-wave phase shifter. Applied Optics, 34, 6058-
High resolution imaging of Virgo galaxies. (1993)
Journal Article
Shanks, T., Major, J., Doel, A., Dunlop, C., Myers, R., Ratcliffe, A., & Tanvir, N. (1993). High resolution imaging of Virgo galaxies
High-resolution imaging of Virgo cluster galaxies. II - Detection of the brightest stars in NGC 4523 (1992)
Journal Article
Shanks, T., Tanvir, N., Major, J., Doel, A., Dunlop, C., & Myers, R. (1992). High-resolution imaging of Virgo cluster galaxies. II - Detection of the brightest stars in NGC 4523. Monthly Notices of the Royal Astronomical Society, 256, 29P-32P
High-resolution imaging of Virgo cluster galaxies. I - Observational techniques and first results (1991)
Journal Article
Tanvir, N., Shanks, T., Major, J., Doel, A., Dunlop, C., Myers, R., …Devaney, M. (1991). High-resolution imaging of Virgo cluster galaxies. I - Observational techniques and first results. Monthly Notices of the Royal Astronomical Society, 253, 21P-24P. https://doi.org/10.1093/mnras/253.1.21p
Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV (1983)
Journal Article
Ayre, C., Myers, R., Thompson, M., Bhat, P., Ma, ,., & Q., Y. (1983). Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV. Monthly Notices of the Royal Astronomical Society, 205, 285-295. https://doi.org/10.1093/mnras/205.2.285