Outputs (8)

Turbulence velocity profiling for high sensitivity and vertical-resolution atmospheric characterization with Stereo-SCIDAR (2016)
Journal Article
Osborn, 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

As telescopes become larger, into the era of ∼40 m Extremely Large Telescopes, the high-resolution vertical profile of the optical turbulence strength is critical for the validation, optimization and operation of optical systems. The velocity of atmo... Read More about Turbulence velocity profiling for high sensitivity and vertical-resolution atmospheric characterization with Stereo-SCIDAR.

Efficient photonic reformatting of celestial light for diffraction-limited spectroscopy (2016)
Journal Article
MacLachlan, D., Harris, R., Gris-Sánchez, I., Morris, T., Choudhury, D., Gendron, E., …Thomson, R. (2017). Efficient photonic reformatting of celestial light for diffraction-limited spectroscopy. Monthly Notices of the Royal Astronomical Society, 464(4), 4950-4957. https://doi.org/10.1093/mnras/stw2558

The spectral resolution of a dispersive astronomical spectrograph is limited by the trade-off between throughput and the width of the entrance slit. Photonic guided wave transitions have been proposed as a route to bypass this trade-off, by enabling... Read More about Efficient photonic reformatting of celestial light for diffraction-limited spectroscopy.

Monte-Carlo modelling of multi-object adaptive optics performance on the European Extremely Large Telescope (2016)
Journal Article
Basden, A., & Morris, T. (2016). Monte-Carlo modelling of multi-object adaptive optics performance on the European Extremely Large Telescope. Monthly Notices of the Royal Astronomical Society, 463(4), 4184-4193. https://doi.org/10.1093/mnras/stw2306

The performance of a wide-field adaptive optics system depends on input design parameters. Here we investigate the performance of a multi-object adaptive optics system design for the European Extremely Large Telescope, using an end-to-end Monte-Carlo... Read More about Monte-Carlo modelling of multi-object adaptive optics performance on the European Extremely Large Telescope.

The E-ELT first light spectrograph HARMONI: capabilities and modes (2016)
Presentation / Conference Contribution
Thatte, N. A., Clarke, F., Bryson, I., Shnetler, H., Tecza, M., Fusco, T., …Evans, C. J. (2016). The E-ELT first light spectrograph HARMONI: capabilities and modes. In L. Simard, H. Takami, & C. J. Evans (Eds.), Proceedings Volume 9908, Ground-based and Airborne Instrumentation for Astronomy VI. https://doi.org/10.1117/12.2230629

HARMONI is the E-ELT’s first light visible and near-infrared integral field spectrograph. It will provide four different spatial scales, ranging from coarse spaxels of 60 × 30 mas best suited for seeing limited observations, to 4 mas spaxels that Nyq... Read More about The E-ELT first light spectrograph HARMONI: capabilities and modes.

CHOUGH: implementation and performance of a high-order 4m AO demonstrator (2016)
Presentation / Conference Contribution
Bharmal, N. A., Basden, A. G., Bourgenot, C. J., Black, M., Dubbeldam, C. M., Henry, D. M., …Myers, R. M. (2016). CHOUGH: implementation and performance of a high-order 4m AO demonstrator. In E. Marchetti, L. M. Close, & J. Véran (Eds.), Adaptive Optics Systems V (990948-990948-7). https://doi.org/10.1117/12.2231721

CHOUGH is a small, fast project to provide an experimental on-sky high-order SCAO capability to the 4.2m WHT telescope. The basic goal has r0-sized sub- apertures with the aim of achieving high-Strehl ratios (> 0:5) in the visible (> 650 nm). It achi... Read More about CHOUGH: implementation and performance of a high-order 4m AO demonstrator.

Science requirements and trade-offs for the MOSAIC instrument for the European ELT (2016)
Presentation / Conference Contribution
Evans, C., Puech, M., Rodrigues, M., Barbuy, B., Cuby, J., Dalton, G., …Morris, T. (2016). Science requirements and trade-offs for the MOSAIC instrument for the European ELT. In C. J. Evans, L. Simard, & H. Takami (Eds.), Ground-based and Airborne Instrumentation for Astronomy VI (99089J-99089J-12). https://doi.org/10.1117/12.2231675

Building on the comprehensive White Paper on the scientific case for multi-object spectroscopy on the European ELT, we present the top-level instrument requirements that are being used in the Phase A design study of the MOSAIC concept. The assembled... Read More about Science requirements and trade-offs for the MOSAIC instrument for the European ELT.

Experience with wavefront sensor and deformable mirror interfaces for wide-field adaptive optics systems (2016)
Journal Article
Basden, A., Atkinson, D., Bharmal, N., Bitenc, U., Brangier, M., Buey, T., …Younger, E. (2016). Experience with wavefront sensor and deformable mirror interfaces for wide-field adaptive optics systems. Monthly Notices of the Royal Astronomical Society, 459(2), 1350-1359. https://doi.org/10.1093/mnras/stw730

Recent advances in adaptive optics (AO) have led to the implementation of wide field-of-view AO systems. A number of wide-field AO systems are also planned for the forthcoming Extremely Large Telescopes. Such systems have multiple wavefront sensors o... Read More about Experience with wavefront sensor and deformable mirror interfaces for wide-field adaptive optics systems.

A tomographic algorithm to determine tip-tilt information from laser guide stars (2016)
Journal Article
Reeves, A., Morris, T., Myers, R., Bharmal, N., & Osborn, J. (2016). A tomographic algorithm to determine tip-tilt information from laser guide stars. Monthly Notices of the Royal Astronomical Society, 459(1), 333-341. https://doi.org/10.1093/mnras/stw622

Laser Guide Stars (LGS) have greatly increased the sky-coverage of Adaptive Optics (AO) systems. Due to the up-link turbulence experienced by LGSs, a Natural Guide Star (NGS) is still required, preventing full sky-coverage. We present a method of obt... Read More about A tomographic algorithm to determine tip-tilt information from laser guide stars.