Lee Sang Gak Telescope (LSGT)

  • Im, Myungshin (CEOU/Astronomy Program, Dept. of Physics & Astronomy, Seoul National University) ;
  • Choi, Changsu (CEOU/Astronomy Program, Dept. of Physics & Astronomy, Seoul National University) ;
  • Kim, Kihyun (CEOU/Astronomy Program, Dept. of Physics & Astronomy, Seoul National University)
  • Published : 2015.04.10

Abstract

In this talk, we introduce the Lee Sang Gak Telescope (LSGT), a 0.43m telescope that can be operated remotely. This telescope was installed at the Siding Spring Observatory in 2015 October, and since then, it has been operated through a robotic reservation system, remotely from Korea. This telescope is now being used for educational and research activities of SNU Astronomy program. By placing the telescope at a place with an excellent astro-climate in Australia, the observation class activity can include objects in the southern hemisphere to the magnitude limit of V=20 mag at an exposure time of a few minutes. For example, Cepheid stars in Magellanic clouds can be observed during a class activity for constructing the classical Cepheid light curves that has been a key distance measure technique. Research activities such as transient observation and monitoring observation of AGN are possible, and we are currently running a high cadence supernovae search program by monitoring nearby galaxies intensively (see a presentation by C. Choi). The installation of the telescope was made possible from a support from the Seoul.

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