J. Molenda–Żakowicz, T. Arentoft, H. Kjeldsen, M. Vaňko
{"title":"用开普勒观测类太阳振荡","authors":"J. Molenda–Żakowicz, T. Arentoft, H. Kjeldsen, M. Vaňko","doi":"10.1553/CIA150S143","DOIUrl":null,"url":null,"abstract":"We describe our program of ground-based spectroscopic and photometric observations of stars selected to be scientific targets in the Kepler Asteroseismic Program.","PeriodicalId":151133,"journal":{"name":"Third Coast","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2007-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Solar-like Oscillations with Kepler\",\"authors\":\"J. Molenda–Żakowicz, T. Arentoft, H. Kjeldsen, M. Vaňko\",\"doi\":\"10.1553/CIA150S143\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We describe our program of ground-based spectroscopic and photometric observations of stars selected to be scientific targets in the Kepler Asteroseismic Program.\",\"PeriodicalId\":151133,\"journal\":{\"name\":\"Third Coast\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2007-06-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Third Coast\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1553/CIA150S143\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Third Coast","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1553/CIA150S143","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
We describe our program of ground-based spectroscopic and photometric observations of stars selected to be scientific targets in the Kepler Asteroseismic Program.