CHARA array adaptive optics II: Non-common-path correction and downstream optics
| dc.contributor.author | Brummelaar, Theo ten | en_AU |
| dc.contributor.author | Che, X | en_AU |
| dc.contributor.author | McAlister, H | en_AU |
| dc.contributor.author | Monnier, J. D. | en_AU |
| dc.contributor.author | Mourard, D. | en_AU |
| dc.contributor.author | Ridgway, Stephen T | en_AU |
| dc.contributor.author | Sturmann, Judit | en_AU |
| dc.contributor.author | Sturmann, Laszlo | en_AU |
| dc.contributor.author | Turner, Nils | en_AU |
| dc.contributor.author | Tuthill, Peter G | en_AU |
| dc.contributor.author | Ireland, Michael | en_AU |
| dc.coverage.spatial | Montreal, Canada | |
| dc.date.accessioned | 2015-12-10T23:17:52Z | |
| dc.date.created | June 22-27 2014 | |
| dc.date.issued | 2014 | |
| dc.date.updated | 2015-12-10T10:01:59Z | |
| dc.description.abstract | We describe a back-end Adaptive Optics system for the CHARA Array called Lab-AO intended to compensate for non-common path errors between the AO system at the telescopes and the final beam combining area some hundreds of meters away. The system is an on-axis, very small field of view, low order system that will work on star light if enough is present, or will make use of a blue light beacon sent from the telescope towards the laboratory if not enough star light is available. The first of six of these system has been installed and has recently been tested on the sky. Another five will be built for the remaining telescopes later this year. | |
| dc.identifier.isbn | 9780819496164 | |
| dc.identifier.uri | http://hdl.handle.net/1885/65380 | |
| dc.publisher | SPIE | |
| dc.relation.ispartofseries | Adaptive Optics Systems IV | |
| dc.rights | Author/s retain copyright | en_AU |
| dc.source | Proceedings of SPIE - The International Society for Optical Engineering, vol 9148 | |
| dc.title | CHARA array adaptive optics II: Non-common-path correction and downstream optics | |
| dc.type | Conference paper | |
| dcterms.accessRights | Open Access | en_AU |
| local.contributor.affiliation | Brummelaar, Theo ten, The CHARA Array | |
| local.contributor.affiliation | Che, X, University of Michigan | |
| local.contributor.affiliation | McAlister, H, Georgia State University | |
| local.contributor.affiliation | Ireland, Michael, College of Physical and Mathematical Sciences, ANU | |
| local.contributor.affiliation | Monnier, J. D. , University of Michigan | |
| local.contributor.affiliation | Mourard, D., Université de Nice Sophia-Antipolis | |
| local.contributor.affiliation | Ridgway, Stephen T, National Optical Astronomy Observatories | |
| local.contributor.affiliation | Sturmann, Judit, The CHARA Array | |
| local.contributor.affiliation | Sturmann, Laszlo, The CHARA Array | |
| local.contributor.affiliation | Turner, Nils, The CHARA Array | |
| local.contributor.affiliation | Tuthill, Peter G, University of Sydney | |
| local.contributor.authoruid | Ireland, Michael, u5544212 | |
| local.description.notes | Imported from ARIES | |
| local.description.refereed | Yes | |
| local.identifier.absfor | 020110 - Stellar Astronomy and Planetary Systems | |
| local.identifier.absfor | 020104 - Galactic Astronomy | |
| local.identifier.absfor | 020102 - Astronomical and Space Instrumentation | |
| local.identifier.ariespublication | a383154xPUB1097 | |
| local.identifier.doi | 10.1117/12.2056662 | |
| local.identifier.scopusID | 2-s2.0-84922711968 | |
| local.type.status | Published Version |
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