A new approach for extrapolating star flux using cross-matching multiple catalogues
Received:October 14, 2018  Revised:May 24, 2019  download
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Author NameAffiliationE-mail
WANG Yu-Du Key Laboratory of Intelligent Infrared Perception , Chinese Academy of Sciences, Shanghai 200083
Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China
University of Chinese Academy of Sciences, Beijing 100049, China 
wangyudu@gmai.com 
SUN Xiao-Jin Key Laboratory of Intelligent Infrared Perception , Chinese Academy of Sciences, Shanghai 200083
Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China 
 
ZHANG Heng Key Laboratory of Intelligent Infrared Perception , Chinese Academy of Sciences, Shanghai 200083
Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China 
 
CHEN Fan-Sheng Key Laboratory of Intelligent Infrared Perception , Chinese Academy of Sciences, Shanghai 200083
Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China 
cfs@mail.sitp.ac.cn 
Abstract:This paper presents a model for extrapolating flux from cross-matching multiple catalogues combining the data of IRAS, WISE and 2MASS, which used the Planck’s law to extrapolate flux to every band. The model simplifies the extrapolation process, and improves the extrapolation efficiency with a high precision of 3% for 70% of the stars. Our finding is in agreement with the independent long-term observation of the Vega and Sirius star reported by Cohen et al. According to the extrapolation results, more suitable multiple data of stars could be selected for star calibration.
keywords:star calibration  flux extrapolation  star catalogues  Planck’s law
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Copyright:《Journal of Infrared And Millimeter Waves》