CCD Observations of Some Variable Stars

Using 1024x1024 pixels CCD camera of ChungBuk National University Observatory (CBNUO), 62 photometric observations were made on January 11-12, 1993. A time of minimum lights of U Cep was determined as JD Hel 2448999.2274 from our data. On October 21-22 in 1993, CCD photometry in V and R for GW Cephe...

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Bibliographic Details
Main Authors: J. H. Jeong, Y.-S. Lee, C. U. Lee, K.-C. Leung
Format: Article
Language:English
Published: The Korean Space Science Society 1994-12-01
Series:Journal of Astronomy and Space Sciences
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1994/v11n2/OJOOBS_1994_v11n2_185.pdf
Description
Summary:Using 1024x1024 pixels CCD camera of ChungBuk National University Observatory (CBNUO), 62 photometric observations were made on January 11-12, 1993. A time of minimum lights of U Cep was determined as JD Hel 2448999.2274 from our data. On October 21-22 in 1993, CCD photometry in V and R for GW Cephei and V700 Cygni was carried out with 309 x 584 pixels cooled CCD system of Behlen Observatory, University of Nebraska-Lincoln(BOUNL) and 168 observations were obtained. From the data time of minimum lights JD Hel 2449282.8485 for GW Cep and JD Hel 2449282.7979 were determined. To develop a new CCD system of CBNUO, the CCD photometry method using at CBNUO is compared with at BOUNL.
ISSN:2093-5587
2093-1409