| Flux Calibration of the BATC Survey and Its Application for Checking the Consistency of the Oke—Gunn Standards |
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| 引用本文： | XuZhou,Zhao－JiJiang,等.Flux Calibration of the BATC Survey and Its Application for Checking the Consistency of the Oke—Gunn Standards[J].中国天文和天体物理学报,2001,1(4):372-382. |
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| 作者姓名： | XuZhou Zhao－JiJiang 等 |
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| 作者单位： | [1]CAS－PekingUniversityJointBeijingAstrophysicalCenter,Beijing100871 [2]NationalAstronomicalObservatories, |
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| 摘 要： | 1 INTRODUCTIONThe B eij lug- Ahs ona~ TaiP ei- C onnect lout Color S urvey of t he S by (Hereaft er B AT C ) ut driesthe 15 intermediate band filters to make CCD forage photometric ohs~ion. The BATCphotometric system ties its maghtude zero P~Oint to the spectro-photometric AB maghtudesystem. The AB system is a monochro~ic fi system fort introduced by Oke in 1969 with aprovisional calibration designated AB69.The AB system selects F subdwarfs around visual magnitude 9 as standa…
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| 关 键 词： | 光度测量 分类 CCD观测 光度计 |
Flux Calibration of the BATC Survey and Its Application for Checking the Consistency of the Oke-Gunn Standards |
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| Xu Zhou,Zhao-Ji Jiang,Sui-Jian Xue,Hong Wu,Jun Ma and Jian-Sheng Chen.Flux Calibration of the BATC Survey and Its Application for Checking the Consistency of the Oke-Gunn Standards[J].Chinese Journal of Astronomy and Astrophysics,2001,1(4):372-382. |
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| Authors: | Xu Zhou Zhao-Ji Jiang Sui-Jian Xue Hong Wu Jun Ma and Jian-Sheng Chen |
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| Abstract: | Four Oke-Gunn(OG) standards, HD 19445,HD 84937,BD 26 2606 and BD 17 4708 are used as standard stars for flux calibration in the BATC project. They are also widely used in the visual wavelength region in many other photometric projects. Over the years we have observed on 58 good photometric nights, and the data obtained are used for flux calibration.Normally two or three OG standards are observed in every photometric night. The data are used for getting the atmospheric extinction coefficients and instrumental magnitude zero point. We also use these data to make inter-comparisons among the magnitudes of these standard stars. As a result,we found the magnitudes of HD 19445,HD 84937 and BD 17 4708 to agree well with those estimated in previous work to within 0.03 magnitude. How-ever,BD 26 2606 shows a larger deviation especially at short wavebands.Possible reasons are analyzed and the revised magnitudes are obtained for these standards. It is shown that the quality of flux calibration of the BATC fields is significantly improved by applying the new magnitudes. |
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| Keywords: | techniques: photometric: calibration |
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