On-sky vibration environment for the Gemini Planet Imager and mitigation effort
العنوان: | On-sky vibration environment for the Gemini Planet Imager and mitigation effort |
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المؤلفون: | Gaston Gausachs, Pascale Hibon, Ramon Galvez, Andrew Cardwell, Daren Dillon, Markus Hartung, Les Saddlemyer, Lisa Poyneer, Andrés Guesalaga, Stephen J. Goodsell, Andrew Serio, Chas Cavedoni, Kent Wallace, Myung Cho, Fredrik T. Rantakyrö, Naru Sadakuni, James E. Larkin, Jeffrey Chilcote, Dmitry Savransky, Paul Collins, Bruce Macintosh, Dave Palmer, Thomas L. Hayward |
بيانات النشر: | arXiv, 2014. |
سنة النشر: | 2014 |
مصطلحات موضوعية: | High contrast imaging, FOS: Physical sciences, Specific frequencies, law.invention, Telescope, Vibration absorber, law, Gemini Planet Imager, Adaptive optics, Coronagraph, LQG, Instrumentation and Methods for Astrophysics (astro-ph.IM), Remote sensing, Wavefront, Physics, Instrument Data, Vibration environment, Telescope structures, Exoplanet, Tilt (optics), Extreme adaptive optics, Integral field spectrograph, Astrophysics - Instrumentation and Methods for Astrophysics, Kalman filters, Telescopes |
الوصف: | The Gemini Planet Imager (GPI) entered on-sky commissioning and had its first-light at the Gemini South (GS) telescope in November 2013. GPI is an extreme adaptive optics (XAO), high-contrast imager and integral-field spectrograph dedicated to the direct detection of hot exo-planets down to a Jupiter mass. The performance of the apodized pupil Lyot coronagraph depends critically upon the residual wavefront error (design goal of 60nmRMS with Adaptive Optics Systems IV, June 22-27, 2014 Series: Proceedings of SPIE; no. 9148 |
DOI: | 10.48550/arxiv.1407.7893 |
URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d39e6763a9b6509526b526cc4db69299 |
Rights: | OPEN |
رقم الانضمام: | edsair.doi.dedup.....d39e6763a9b6509526b526cc4db69299 |
قاعدة البيانات: | OpenAIRE |
DOI: | 10.48550/arxiv.1407.7893 |
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