Standard Calibration for Broadband and Narrowband Filters of KHAO 0.4 m Telescope

  • Ahn, Hojae (School of Space Research, Kyung Hee Univeristy) ;
  • Jeong, Inhwan (Department of Space Science, Kyung Hee University) ;
  • Paek, Gregory S.H. (SNU Astronomy Research Center, Department of Physics and Astronomy, Seoul National University) ;
  • Lee, Sumin (Department of Space Science, Kyung Hee University) ;
  • Kim, Changgon (School of Space Research, Kyung Hee Univeristy) ;
  • Pak, Soojong (School of Space Research, Kyung Hee Univeristy) ;
  • Shim, Hyunjin (Department of Earth Science Education, Kyungpook University) ;
  • Im, Myungshin (SNU Astronomy Research Center, Department of Physics and Astronomy, Seoul National University)
  • Published : 2021.10.13

Abstract

Maemi Dual Field Telescope System (MDFTS) is a dual telescope system located at Kyung Hee University. The system consists of 0.4 m telescope and 0.1 m telescope for wide-field observation. The 0.4 m telescope provides photometric observation which covers a field of view of 21'×16'. It has been used for various purposes with Johnson-Cousins UBVRI broadband filter system, e.g., SomangNet and Intensive Monitoring Survey of Nearby Galaxies. In this poster, we present the standard calibration result for our broadband filter system. Also, we suggest a new usage of the KHAO 0.4m telescope which is narrowband photometry by demonstrating the standard calibration of H-alpha filter. For flux calibration, not only R filter but also V filter is used for compensating the central wavelength discrepancy between R filter and H-alpha filter.

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