activity
20172023
most citedDemonstrating 24-hour continuous vertical monitoring of atmospheric optical turbulence

34 citations · 82 across the 5 of their papers we have counts for

collaborators
Showing 2018 · astro-ph.IMShow all

5 papers · 2 filters

astro-ph.IM2018

Representative optical turbulence profiles for ESO Paranal by hierarchical clustering

O. J. D. Farley, J. Osborn, T. Morris +5

Knowledge of the optical turbulence profile is important in adaptive optics (AO) systems, particularly tomographic AO systems such as those to be employed by the next generation of…

astro-ph.IM2018

Generating Artificial Reference Images for Open Loop Correlation Wavefront Sensors

M. J. Townson, G. D Love, C. D. Saunter

Shack-Hartmann wavefront sensors for both solar and laser guide star adaptive optics (with elongated spots) need to observe extended objects. Correlation techniques have been succe…

astro-ph.IM2018

Optimizing astrophotonic spatial reformatters using simulated on-sky performance

Theodoros Anagnos, Robert J. Harris, Mark K. Corrigan +7

One of the most useful techniques in astronomical instrumentation is image slicing. It enables a spectrograph to have a more compact angular slit, whilst retaining throughput and i…

astro-ph.IM2018

Optical turbulence profiling with Stereo-SCIDAR for VLT and ELT

J. Osborn, R. W. Wilson, M. Sarazin +11

Knowledge of the Earth's atmospheric optical turbulence is critical for astronomical instrumentation. Not only does it enable performance verification and optimisation of existing…

astro-ph.IM2018

Simulation and Optimization of an Astrophotonic Reformatter

Th. Anagnos, R. J. Harris, M. K. Corrigan +7

Image slicing is a powerful technique in astronomy. It allows the instrument designer to reduce the slit width of the spectrograph, increasing spectral resolving power whilst retai…