Optimizing the accuracy and efficiency of optical turbulence profiling using adaptive optics telemetry for extremely large telescopes

Douglas Laidlaw; James Osborn; Timothy Morris; Alastair Basden; Olivier Beltramo-Martin; Timothy Butterley; Eric Gendron; Andrew Reeves; Gérard Rousset; Matthew Townson; Richard Wilson

doi:10.1093/mnras/sty3285

Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2019

Optimizing the accuracy and efficiency of optical turbulence profiling using adaptive optics telemetry for extremely large telescopes

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1

Douglas Laidlaw

Function : Author

James Osborn

Function : Author

Timothy Morris

Function : Author

Alastair Basden

Function : Author

Olivier Beltramo-Martin

Function : Author

Timothy Butterley

Function : Author

Eric Gendron

Function : Author

Laboratoire d'études spatiales et d'instrumentation en astrophysique

Andrew Reeves

Function : Author
PersonId : 786322
ORCID : 0000-0003-2618-6408

Gérard Rousset

Function : Author

Laboratoire d'études spatiales et d'instrumentation en astrophysique

Matthew Townson

Function : Author

Richard Wilson

Function : Author

Domains

Physics [physics] Astrophysics [astro-ph]

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https://hal.science/hal-03111719

Submitted on : Thursday, June 1, 2023-1:33:38 PM

Last modification on : Thursday, June 1, 2023-1:33:44 PM

Long-term archiving on: Saturday, September 2, 2023-6:49:36 PM

Dates and versions

hal-03111719 , version 1 (01-06-2023)

Identifiers

HAL Id : hal-03111719 , version 1
ARXIV : 1901.05860
BIBCODE : 2019MNRAS.483.4341L
DOI : 10.1093/mnras/sty3285

Cite

Douglas Laidlaw, James Osborn, Timothy Morris, Alastair Basden, Olivier Beltramo-Martin, et al.. Optimizing the accuracy and efficiency of optical turbulence profiling using adaptive optics telemetry for extremely large telescopes. Monthly Notices of the Royal Astronomical Society, 2019, 483 (4), pp.4341-4353. ⟨10.1093/mnras/sty3285⟩. ⟨hal-03111719⟩

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Optimizing the accuracy and efficiency of optical turbulence profiling using adaptive optics telemetry for extremely large telescopes

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