Vibrations in MagAO: frequency-based analysis of on-sky data, resonance sources identification, and future challenges in vibrations mitigation
Close, Laird M.
Males, Jared R.
Morzinski, Katie M.
AffiliationUniv Arizona, Dept Astron, CAAO
Univ Arizona, Steward Observ
MetadataShow full item record
PublisherSPIE-INT SOC OPTICAL ENGINEERING
CitationSebastián Zúñiga ; Javier Garcés ; Laird M. Close ; Jared R. Males ; Katie M. Morzinski ; Pedro Escárate ; Mario Castro ; José Marchioni and Diego Zagals " Vibrations in MagAO: frequency-based analysis of on-sky data, resonance sources identification, and future challenges in vibrations mitigation ", Proc. SPIE 9909, Adaptive Optics Systems V, 99093L (July 27, 2016); doi:10.1117/12.2232676; http://dx.doi.org/10.1117/12.2232676
JournalADAPTIVE OPTICS SYSTEMS V
Rights© 2016 SPIE
Collection InformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at firstname.lastname@example.org.
AbstractFrequency-based analysis and comparisons of tip-tilt on-sky data registered with 6.5 Magellan Telescope Adaptive Optics (MagAO) system on April and Oct 2014 was performed. Twelve tests are conducted under different operation conditions in order to observe the influence of system instrumentation (such as fans, pumps and louvers). Vibration peaks can be detected, power spectral densities (PSDs) are presented to reveal their presence. Instrumentation-induced resonances, close-loop gain and future challenges in vibrations mitigation techniques are discussed.
VersionFinal published version