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We present the characteristics and the performance of the new CCD camerasystem, SNUCAM-II (Seoul National University CAMera system II) that wasinstalled on the Lee Sang Gak Telescope (LSGT) at the Siding Spring Observatoryin 2016. SNUCAM-II consists of a deep depletion chip covering a wide wavelengthfrom 0.3 {\mu}m to 1.1 {\mu}m with high sensitivity (QE at > 80% over 0.4 to0.9 {\mu}m). It is equipped with the SDSS ugriz filters and 13 medium bandwidth (50 nm) filters, enabling us to study spectral energy distributions(SEDs) of diverse objects from extragalactic sources to solar system objects.On LSGT, SNUCAM-II offers 15.7 {\times} 15.7 arcmin field-of-view (FOV) at apixel scale of 0.92 arcsec and a limiting magnitude of g = 19.91 AB mag andz=18.20 AB mag at 5{\sigma} with 180 sec exposure time for point sourcedetection.

Seoul National University Camera II (SNUCAM-II): The New SED Camera for the Lee Sang Gak Telescope (LSGT)