Staff profile
Overview
https://apps.dur.ac.uk/biography/image/1093
Affiliation | Telephone |
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Associate Professor in the Department of Physics | +44 (0) 191 33 43663 |
Biography
Research Interests
Effects of optical turbulence in astronomy; astronomical site characterisation; high resolution imaging methods - adaptive optics; stellar interferometry; time-resolved photometry - scintillation correction, transiting exoplanets; robotic telescope systems.
Publications
Conference Paper
- The 24hSHIMM: a continuous day and night turbulence monitor for optical communicationsGriffiths, R., Osborn, J., Farley, O., Butterley, T., Townson, M., & Wilson, R. (2023). The 24hSHIMM: a continuous day and night turbulence monitor for optical communications. In H. Hemmati & B. S. Robinson (Eds.), Proceedings Volume 12413, Free-Space Laser Communications XXXV. SPIE. https://doi.org/10.1117/12.2648789
- Correction of photometric scintillation noise via tomographic wavefront sensing: simulation and on-sky demonstrationHartley, K., Farley, O., Townson, M. J., Osborn, J., & Wilson, R. W. (2022). Correction of photometric scintillation noise via tomographic wavefront sensing: simulation and on-sky demonstration. In D. Schmidt, L. Schreiber, & E. Vernet (Eds.), Proceedings Volume 12185, Adaptive Optics Systems VIII (p. 326). SPIE. https://doi.org/10.1117/12.2628703
- United Kingdom adaptive optics programsGilmore, G., Longmore, A., Myers, R., & Wilson, R. (1996). United Kingdom adaptive optics programs. In Adaptive Optics (p. 9-).
- Novel adaptive optics with the Durham University ELECTRA systemBuscher, D., Doel, A., Andrews, N., Dunlop, C., Morris, P., Myers, R., Sharples, R., Vick, A., Zadrozny, A., Haniff, C., & Wilson, R. (1996). Novel adaptive optics with the Durham University ELECTRA system. In Adaptive Optics (p. 63-).
- Aspects of the theoretical performance of modal adaptive opticsWilson, R., & Jenkins, C. (1994). Aspects of the theoretical performance of modal adaptive optics. In IAU Symp. 158: Very High Angular Resolution Imaging (p. 305-).
- N.R.M. Imaging of M Giant Stars at the William Herschel TelescopeWilson, R., Baldwin, J., Warner, P., & Buscher, D. (1992). N.R.M. Imaging of M Giant Stars at the William Herschel Telescope. In High-Resolution Imaging by Interferometry (p. 381-).
Journal Article
- Exploring atmospheric optical turbulence: observations across zenith anglesBeesley, L. F., Osborn, J., Wilson, R., Farley, O. J. D., Griffiths, R., & Love, G. D. (2024). Exploring atmospheric optical turbulence: observations across zenith angles. Applied Optics, 63(16), E48. https://doi.org/10.1364/ao.519063
- A comparison of next-generation turbulence profiling instruments at ParanalGriffiths, R., Bardou, L., Butterley, T., Osborn, J., Wilson, R., Bustos, E., Tokovinin, A., Le Louarn, M., & Otarola, A. (2024). A comparison of next-generation turbulence profiling instruments at Paranal. Monthly Notices of the Royal Astronomical Society, 529(1), 320-330. https://doi.org/10.1093/mnras/stae434
- Optimized temporal binning of comparison star measurements for differential photometryHartley, K. E., & Wilson, R. W. (2023). Optimized temporal binning of comparison star measurements for differential photometry. Monthly Notices of the Royal Astronomical Society, 526(3), 3482-3494. https://doi.org/10.1093/mnras/stad2964
- Optical sparse telescope arrays and scintillation noiseHartley, K. E., Farley, O. J. D., Townson, M. J., Osborn, J., & Wilson, R. W. (2023). Optical sparse telescope arrays and scintillation noise. Monthly Notices of the Royal Astronomical Society, 526(1), 1235-1245. https://doi.org/10.1093/mnras/stad2835
- Continuous daytime and nighttime forecast of atmospheric optical turbulence from numerical weather prediction modelsQuatresooz, F., Griffiths, R., Bardou, L., Wilson, R., Osborn, J., Vanhoenacker-Janvier, D., & Oestges, C. (2023). Continuous daytime and nighttime forecast of atmospheric optical turbulence from numerical weather prediction models. Optics Express, 31(21), 33850-33872. https://doi.org/10.1364/oe.500090
- First On-Sky Demonstration of a Scintillation Correction technique using Tomographic Wavefront SensingHartley, K. E., Farley, O. J., Townson, M. J., Osborn, J., & Wilson, R. (2023). First On-Sky Demonstration of a Scintillation Correction technique using Tomographic Wavefront Sensing. Monthly Notices of the Royal Astronomical Society, 520(3), 4134-4146. https://doi.org/10.1093/mnras/stad420
- SHIMM: a versatile seeing monitor for astronomyPerera, S., Wilson, R. W., Butterley, T., Osborn, J., Farley, O. J., & Laidlaw, D. J. (2023). SHIMM: a versatile seeing monitor for astronomy. Monthly Notices of the Royal Astronomical Society, 520(4), 5475-5486. https://doi.org/10.1093/mnras/stad339
- Demonstrating 24-hour continuous vertical monitoring of atmospheric optical turbulenceGriffiths, R., Osborn, J., Farley, O., Butterley, T., Townson, M. J., & Wilson, R. (2023). Demonstrating 24-hour continuous vertical monitoring of atmospheric optical turbulence. Optics Express, 31(4), 6730-6740. https://doi.org/10.1364/oe.479544
- FASS: a turbulence profiler based on a fast, low-noise cameraGuesalaga, A., Ayancán, B., Sarazin, M., Wilson, R., Perera, S., & Le Louarn, M. (2021). FASS: a turbulence profiler based on a fast, low-noise camera. Monthly Notices of the Royal Astronomical Society, 501(2), 3030-3045. https://doi.org/10.1093/mnras/staa3823
- Automated wind velocity profiling from adaptive optics telemetryLaidlaw, D. J., Osborn, J., Morris, T. J., Basden, A. G., Gendron, E., Rousset, G., Townson, M. J., & Wilson, R. W. (2020). Automated wind velocity profiling from adaptive optics telemetry. Monthly Notices of the Royal Astronomical Society, 491(1), 1287-1294. https://doi.org/10.1093/mnras/stz3062
- The Pre-He White Dwarf in the Post-mass Transfer Binary EL CVnWang, L., Gies, D. R., Lester, K. V., Guo, Z., Matson, R. A., Peters, G. J., Dhillon, V. S., Butterley, T., Littlefair, S. P., Wilson, R. W., & Maxted, P. F. (2020). The Pre-He White Dwarf in the Post-mass Transfer Binary EL CVn. Astronomical Journal, 159(1), Article 4. https://doi.org/10.3847/1538-3881/ab52fa
- Atmospheric scintillation noise in ground-based exoplanet photometryFöhring, D., Wilson, R., Osborn, J., & Dhillon, V. (2019). Atmospheric scintillation noise in ground-based exoplanet photometry. Monthly Notices of the Royal Astronomical Society, 489(4), 5098-5108. https://doi.org/10.1093/mnras/stz2444
- Identifying optical turbulence profiles for realistic tomographic error in adaptive opticsFarley, O., Osborn, J., Morris, T., Fusco, T., Neichel, B., Correia, C., & Wilson, R. (2019). Identifying optical turbulence profiles for realistic tomographic error in adaptive optics. Monthly Notices of the Royal Astronomical Society, 488(1), 213-221. https://doi.org/10.1093/mnras/stz1669
- The PDS 110 observing campaign – photometric and spectroscopic observations reveal eclipses are aperiodicOsborn, H., Kenworthy, M., Rodriguez, J., de Mooij, E., Kennedy, G., Relles, H., Gomez, E., Hippke, M., Banfi, M., Barbieri, L., Becker, I., Benni, P., Berlind, P., Bieryla, A., Bonnoli, G., Boussier, H., Brincat, S., Briol, J., Burleigh, M., … Zhou, G. (2019). The PDS 110 observing campaign – photometric and spectroscopic observations reveal eclipses are aperiodic. Monthly Notices of the Royal Astronomical Society, 485(2), 1614-1625. https://doi.org/10.1093/mnras/stz283
- Representative optical turbulence profiles for ESO Paranal by hierarchical clusteringFarley, O., Osborn, J., Morris, T., Sarazin, M., Butterley, T., Townson, M., Jia, P., & Wilson, R. (2018). Representative optical turbulence profiles for ESO Paranal by hierarchical clustering. Monthly Notices of the Royal Astronomical Society, 481(3), 4030-4037. https://doi.org/10.1093/mnras/sty2536
- Optimizing the accuracy and efficiency of optical turbulence profiling using adaptive optics telemetry for extremely large telescopesLaidlaw, D. J., Osborn, J., Morris, T. J., Basden, A. G., Beltramo-Martin, O., Butterley, T., Gendron, E., Reeves, A. P., Rousset, G., Townson, M. J., & Wilson, R. W. (2018). Optimizing the accuracy and efficiency of optical turbulence profiling using adaptive optics telemetry for extremely large telescopes. Monthly Notices of the Royal Astronomical Society, 483(4), 4341-4353. https://doi.org/10.1093/mnras/sty3285
- Optical turbulence profiling with Stereo-SCIDAR for VLT and ELTOsborn, J., Wilson, R., Sarazin, M., Butterley, T., Chacon, A., Derie, F., Farley, O., Haubois, X., Laidlaw, D., LeLouarn, M., Masciadri, E., Milli, J., Navarrete, J., & Townson, M. (2018). Optical turbulence profiling with Stereo-SCIDAR for VLT and ELT. Monthly Notices of the Royal Astronomical Society, 478(1), 825-834. https://doi.org/10.1093/mnras/sty1070
- SS Cancri: the shortest modulation-period Blazhko RR LyraeCafolla, C., Mathew, R., Edge, A., Swinbank, A., Lansbury, G., Wilson, R., Butterley, T., Lucey, J., Hardy, L., Littlefair, S., & Dhillon, V. (2017). SS Cancri: the shortest modulation-period Blazhko RR Lyrae. Information Bulletin on Variable Stars, 63, Article 6213. https://doi.org/10.22444/ibvs.6213
- Hunting for eclipses: high-speed observations of cataclysmic variablesHardy, L., McAllister, M., Dhillon, V., Littlefair, S., Bours, M., Breedt, E., Butterley, T., Chakpor, A., Irawati, P., Kerry, P., Marsh, T., Parsons, S., Savoury, C., Wilson, R., & Woudt, P. (2017). Hunting for eclipses: high-speed observations of cataclysmic variables. Monthly Notices of the Royal Astronomical Society, 465(4), 4968-4984. https://doi.org/10.1093/mnras/stw3051
- Turbulence velocity profiling for high sensitivity and vertical-resolution atmospheric characterization with Stereo-SCIDAROsborn, J., Butterley, T., Townson, M., Reeves, A., Morris, T., & Wilson, R. (2017). Turbulence velocity profiling for high sensitivity and vertical-resolution atmospheric characterization with Stereo-SCIDAR. Monthly Notices of the Royal Astronomical Society, 464(4), 3998-4007. https://doi.org/10.1093/mnras/stw2685
- pt5m – a 0.5 m robotic telescope on La PalmaHardy, L., Butterley, T., Dhillon, V., Littlefair, S., & Wilson, R. (2015). pt5m – a 0.5 m robotic telescope on La Palma. Monthly Notices of the Royal Astronomical Society, 454(4), 4316-4325. https://doi.org/10.1093/mnras/stv2279
- Atmospheric scintillation in astronomical photometryOsborn, J., Föhring, D., Dhillon, V., & Wilson, R. (2015). Atmospheric scintillation in astronomical photometry. Monthly Notices of the Royal Astronomical Society, 452(2), 1707-1716. https://doi.org/10.1093/mnras/stv1400
- Stereo-SCIDAR: optical turbulence profiling with high sensitivity using a modified SCIDAR instrumentShepherd, H., Osborn, J., Wilson, R., Butterley, T., Avila, R., Dhillon, V., & Morris, T. (2014). Stereo-SCIDAR: optical turbulence profiling with high sensitivity using a modified SCIDAR instrument. Monthly Notices of the Royal Astronomical Society, 437(4), 3568-3577. https://doi.org/10.1093/mnras/stt2150
- ULTRACAM z′-band detection of the secondary eclipse of WASP-12bFöhring, D., Dhillon, V., Madhusudhan, N., Marsh, T., Copperwheat, C., Littlefair, S., & Wilson, R. (2013). ULTRACAM z′-band detection of the secondary eclipse of WASP-12b. Monthly Notices of the Royal Astronomical Society, 435(3), 2268-2273. https://doi.org/10.1093/mnras/stt1443
- Conjugate-plane photometry: reducing scintillation in ground-based photometryOsborn, J., Wilson, R. W., Dhillon, V., Avila, R., & Love, G. D. (2011). Conjugate-plane photometry: reducing scintillation in ground-based photometry. Monthly Notices of the Royal Astronomical Society, 411(2), 1223-1230. https://doi.org/10.1111/j.1365-2966.2010.17759.x
- Profiling the surface layer of optical turbulence with SLODAROsborn, J., Wilson, R., Butterley, T., Shepherd, H., & Sarazin, M. (2010). Profiling the surface layer of optical turbulence with SLODAR. Monthly Notices of the Royal Astronomical Society, 406(2), 1405-1408. https://doi.org/10.1111/j.1365-2966.2010.16795.x
- Mauna Kea ground-layer characterization campaignChun, M., Wilson, R., Avila, R., Butterley, T., Aviles, J., Wier, D., & Begnini, S. (2009). Mauna Kea ground-layer characterization campaign. Monthly Notices of the Royal Astronomical Society, 394(3), 1121-1230. https://doi.org/10.1111/j.1365-2966.2008.14346.x
- The Durham/ESO SLODAR optical turbulence profilerWilson, R., Butterley, T., & Sarazin, M. (2009). The Durham/ESO SLODAR optical turbulence profiler. Monthly Notices of the Royal Astronomical Society, 399(4), 2129-2138. https://doi.org/10.1111/j.1365-2966.2009.15409.x
- LOLAS: an optical turbulence profiler in the atmospheric boundary layer with extreme altitude resolutionAvila, R., Aviles, J., Wilson, R., Chun, M., Butterley, T., & Carrasco, E. (2008). LOLAS: an optical turbulence profiler in the atmospheric boundary layer with extreme altitude resolution. Monthly Notices of the Royal Astronomical Society, 387(4), 1511-1516. https://doi.org/10.1111/j.1365-2966.2008.13386.x
- Durham extremely large telescope adaptive optics simulation platformBasden, 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.46.001089
- Method of estimating time scales of atmospheric piston and its application at Dome C (Antarctica)Kellerer, A., Sarazin, M., Butterley, T., & WIlson, R. (2007). Method of estimating time scales of atmospheric piston and its application at Dome C (Antarctica). Applied Optics, 46(21), 4754-4762. https://doi.org/10.1364/ao.46.004754
- Determination of the profile of atmospheric optical turbulence strength from SLODAR dataButterley, T., Wilson, R., & Sarazin, M. (2006). Determination of the profile of atmospheric optical turbulence strength from SLODAR data. Monthly Notices of the Royal Astronomical Society, 369(2), 835-845. https://doi.org/10.1111/j.1365-2966.2006.10337.x
- Method for simulating infinitely long and non stationary phase screens with optimized memory storageAssemat, F., Wilson, R., & Gendron, E. (2006). Method for simulating infinitely long and non stationary phase screens with optimized memory storage. Optics Express, 14(3). https://doi.org/10.1364/oe.14.000988
- Acceleration of adaptive optics simulations using programmable logicBasden, A., Assemat, F., Butterley, T., Geng, D., Saunter, C., & Wilson, R. (2005). Acceleration of adaptive optics simulations using programmable logic. Monthly Notices of the Royal Astronomical Society, 364(4), 1413-1418. https://doi.org/10.1111/j.1365-2966.2005.09670.x
- Estimation of anisoplanatism in adaptive optics by generalized SCIDAR profilingWilson, R., Wooder, N., Rigal, F., & Dainty, J. (2003). Estimation of anisoplanatism in adaptive optics by generalized SCIDAR profiling. Monthly Notices of the Royal Astronomical Society, 339(2), 491-494. https://doi.org/10.1046/j.1365-8711.2003.06198.x
- SLODAR: measuring optical turbulence altitude with a Shack-Hartmann wavefront sensorWilson, R. (2002). SLODAR: measuring optical turbulence altitude with a Shack-Hartmann wavefront sensor. Monthly Notices of the Royal Astronomical Society, 337(1), 103-108. https://doi.org/10.1046/j.1365-8711.2002.05847.x
- Characterization of the mesospheric sodium layer at La PalmaMichaille, L., Clifford, J., Dainty, J., Gregory, T., Quartel, J., Reavell, F., Wilson, R., & Wooder, N. (2001). Characterization of the mesospheric sodium layer at La Palma. Monthly Notices of the Royal Astronomical Society, 328(4), 993-1000. https://doi.org/10.1046/j.1365-8711.2001.04703.x
- Diffraction-limited 800 nm imaging with the 2.56 m Nordic optical telescopeBaldwin, J., Tubbs, R., Cox, G., Mackay, C., Wilson, R., & Andersen, M. (2001). Diffraction-limited 800 nm imaging with the 2.56 m Nordic optical telescope. Astronomy and Astrophysics., 368(1), L1-L4. https://doi.org/10.1051/0004-6361%3A20010118
- New views of Betelgeuse: multi-wavelength surface imaging and implications for models of hotspot generationYoung, J., Baldwin, J., Boysen, R., Haniff, C., Lawson, P., Mackay, C., Pearson, D., Rogers, J., St.-Jacques, D., Warner, P., Wilson, D., & Wilson, R. (2000). New views of Betelgeuse: multi-wavelength surface imaging and implications for models of hotspot generation. Monthly Notices of the Royal Astronomical Society, 315, 635-645.
- A laser beacon for monitoring the mesospheric sodium layer at La PalmaMichaille, L., Cañas, A., Dainty, J., Maxwell, J., Gregory, T., Quartel, J., Reavell, F., Wilson, R., & Wooder, N. (2000). A laser beacon for monitoring the mesospheric sodium layer at La Palma. Monthly Notices of the Royal Astronomical Society, 318, 139-144.
- The seeing at the William Herschel TelescopeWilson, R., O’Mahony, N., Packham, C., & Azzaro, M. (1999). The seeing at the William Herschel Telescope. Monthly Notices of the Royal Astronomical Society, 309, 379-387.
- Results of the JOSE site evaluation project for adaptive optics at the William Herschel TelescopeWilson, R. (1998). Results of the JOSE site evaluation project for adaptive optics at the William Herschel Telescope. New Astronomy Review, 42, 465-469.
- Recent developments in the Half Arcsecond ProgrammePackham, C., O’Mahony, N., & Wilson, R. (1998). Recent developments in the Half Arcsecond Programme. New Astronomy Reviews, 42, 431-433.
- The JOSE atmospheric seeing monitor at the William Herschel TelescopeSt-Jacques, D., Cox, G., Baldwin, J., Mackay, C., Waldram, E., & Wilson, R. (1997). The JOSE atmospheric seeing monitor at the William Herschel Telescope. Monthly Notices of the Royal Astronomical Society, 290, 66-74.
- The changing face of BetelgeuseWilson, R., Dhillon, V., & Haniff, C. (1997). The changing face of Betelgeuse. Monthly Notices of the Royal Astronomical Society, 291, 819-.
- Adaptive optics for astronomy: theoretical performance and limitationsWilson, R., & Jenkins, C. (1996). Adaptive optics for astronomy: theoretical performance and limitations. Monthly Notices of the Royal Astronomical Society, 278, 39-61.
- The first images from an optical aperture synthesis array: mapping of Capella with COAST at two epochs.Baldwin, J., Beckett, M., Boysen, R., Burns, D., Buscher, D., Cox, G., Haniff, C., Mackay, C., Nightingale, N., Rogers, J., Scheuer, P., Scott, T., Tuthill, P., Warner, P., Wilson, D., & Wilson, R. (1996). The first images from an optical aperture synthesis array: mapping of Capella with COAST at two epochs. Astronomy and Astrophysics., 306, L13-.
- High-resolution imaging of Betelgeuse and MiraWilson, R., Baldwin, J., Buscher, D., & Warner, P. (1992). High-resolution imaging of Betelgeuse and Mira. Monthly Notices of the Royal Astronomical Society, 257, 369-376.
Other (Digital/Visual Media)
- SLODAR: Profiling Atmospheric Turbulence at the WHTWilson, R., & Saunter, C. (2003). SLODAR: Profiling Atmospheric Turbulence at the WHT [7].
- The Half Arcsecond Programme (I)Packham, C., Wilson, R., Azzaro, M., O’Mahony, N., Fine, S., Gray, D., Reyes, V., & Martín, C. (2000). The Half Arcsecond Programme (I) [2].
- First Sodium Laser Beacon at La PalmaMichaille, L., Quartel, J., Dainty, J., Wooder, N., Wilson, R., & Gregory, T. (2000). First Sodium Laser Beacon at La Palma [2].
- The changing surface of Betelgeuse.Wilson, R., Baldwin, J., Warner, P., & Buscher, D. (1991). The changing surface of Betelgeuse [34].
Supervision students
Declan Morbey
PGR Student
Jaya Chand
PGR Student
Rose Blyth
PGR Student