# Straylight analysis for preliminary filter and baffle design for New Generation GOCI

• Oh, Eun-Song (Space Optics Laboratory, Dept. of Astronomy, Yonsei University) ;
• Ahn, Ki-Beom (Space Optics Laboratory, Dept. of Astronomy, Yonsei University) ;
• Jung, Kil-Jae (Space Optics Laboratory, Dept. of Astronomy, Yonsei University) ;
• Ryu, Dong-Ok (Space Optics Laboratory, Dept. of Astronomy, Yonsei University) ;
• Kim, Sug-Whan (Space Optics Laboratory, Dept. of Astronomy, Yonsei University)
• Published : 2010.04.15

#### Abstract

We present a three-mirror anastigmat(TMA) optical system for New Generation GOCI. In order to reduce the ghost optimized filter and baffle. By using carefully chosen antireflective coating and tilted filter angle, we fulfilled the design SNR requirement of 1500. We then designed a new entrance baffle and an internal baffle capable of producing the ghost ratio better than 0.01% of the nominal signal. The entrance baffle limits FOV to $0.75^{\circ}$ (E/W) $\times$ $0.60^{\circ}$ (S/N), and prevents the system from strong sun illumination, and the internal baffle prevents stray and scattered ray from entering into the telescope cavity. From these filter and baffle design, we confirmed that the instrument signal to noise ratio can be met with the current conceptual opto-mechanical design.