D. Gavel, S. Severson, Brian Jeffrey Bauman, D. Dillon, M. Reinig, C. Lockwood, D. Palmer, K. Morzinski, S. Ammons, E. Gates, B. Grigsby
{"title":"村落:利用MEMS变形镜进行天空可见波长天文AO实验","authors":"D. Gavel, S. Severson, Brian Jeffrey Bauman, D. Dillon, M. Reinig, C. Lockwood, D. Palmer, K. Morzinski, S. Ammons, E. Gates, B. Grigsby","doi":"10.1117/12.772406","DOIUrl":null,"url":null,"abstract":"The MEMS-AO/Villages project consists of a series of on-sky experiments that will demonstrate key new technologies for the next generation of adaptive optics systems for large telescopes. One of our first goals is to demonstrate the use of a micro-electro-mechanical systems (MEMS) deformable mirror as the wavefront correcting element. The system is mounted the 1-meter Nickel Telescope at the UCO/Lick Observatory on Mount Hamilton. It uses a 140 element (10 subapertures across) MEMS deformable mirror and is designed to produce diffraction-limited images at wavelengths from 0.5 to 1.0 microns. The system had first light on the telescope in October 2007. Here we report on the results of initial on-sky tests.","PeriodicalId":130723,"journal":{"name":"SPIE MOEMS-MEMS","volume":"30 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-02-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"24","resultStr":"{\"title\":\"Villages: an on-sky visible wavelength astronomy AO experiment using a MEMS deformable mirror\",\"authors\":\"D. Gavel, S. Severson, Brian Jeffrey Bauman, D. Dillon, M. Reinig, C. Lockwood, D. Palmer, K. Morzinski, S. Ammons, E. Gates, B. Grigsby\",\"doi\":\"10.1117/12.772406\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The MEMS-AO/Villages project consists of a series of on-sky experiments that will demonstrate key new technologies for the next generation of adaptive optics systems for large telescopes. One of our first goals is to demonstrate the use of a micro-electro-mechanical systems (MEMS) deformable mirror as the wavefront correcting element. The system is mounted the 1-meter Nickel Telescope at the UCO/Lick Observatory on Mount Hamilton. It uses a 140 element (10 subapertures across) MEMS deformable mirror and is designed to produce diffraction-limited images at wavelengths from 0.5 to 1.0 microns. The system had first light on the telescope in October 2007. Here we report on the results of initial on-sky tests.\",\"PeriodicalId\":130723,\"journal\":{\"name\":\"SPIE MOEMS-MEMS\",\"volume\":\"30 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2008-02-07\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"24\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"SPIE MOEMS-MEMS\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1117/12.772406\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"SPIE MOEMS-MEMS","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.772406","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Villages: an on-sky visible wavelength astronomy AO experiment using a MEMS deformable mirror
The MEMS-AO/Villages project consists of a series of on-sky experiments that will demonstrate key new technologies for the next generation of adaptive optics systems for large telescopes. One of our first goals is to demonstrate the use of a micro-electro-mechanical systems (MEMS) deformable mirror as the wavefront correcting element. The system is mounted the 1-meter Nickel Telescope at the UCO/Lick Observatory on Mount Hamilton. It uses a 140 element (10 subapertures across) MEMS deformable mirror and is designed to produce diffraction-limited images at wavelengths from 0.5 to 1.0 microns. The system had first light on the telescope in October 2007. Here we report on the results of initial on-sky tests.