We are proud that we are launching “Have 4,000 Students sign a Jeju 4.3 Petition to the U.S. Capitol” for enactment of “the Korea Jeju 4.3 Human Rights Act 2022” in 2022, which was result of various visits to offices of U.S. Congressman Mark Takano and Congresswoman Judy Chu on May 1, 2019. It was historic sentence for Jeju 4.3 Survivors, Mr. Dong-Soo Park of Sogil Village, Mr. Wonhue Boo of Hwabuk village, Ms. Hee-Chun Oh of Harye village dismissed all charges against the accused on January 17, 2019 by Presiding Judge Jaegal, Chang, Chung, Seung-jin and Seo, Youngwoo at the Korea Jeju Distict Court. “South Korean victims who were wrongfully charged with insurrection during an anti-communist crackdown from 1948 to 1949 and thrown in jail for defying violent paramilitary and military forces, are to receive more that $4 million in compensation for wrongful imprisonment following the Jeju 4.3 massacre, “South Korea Jeju Massacre victims awarded $ 4M in damages,” by Elizabeth Shim: UPI, August 21, 2019).

We submit a proposal ‘Jeju 6+1 Forum in France : World Environment University in Korea and its Sister University in Strasbourg in 2022’ for a private meeting for the IUCN World Conservation Congress 2020 at Parc Chanot in Marseille to 7 to 15 January 2021. The purpose of this study is not only to practice both Jeju Environment or bio diplomacy utilizing UNESCO Environmental Assets but also actualize Jeju peace island cultural and educational diplomacy making use of peace-promoting image of Jeju Special Self-Governing Province through institutionalization of 6+1 Wonsan Culture Forum, Jeju Peace Concert, Global Youth Peace Documentary Film contest by people to people democracy at grassroots level

본 논문은 시진핑정부가 이슬람교정책에서 기존의 온건노선을 버리고 강경노선으로 전환 하게 된 배경을 살펴보고, 이슬람교중국화 5개년규획문건을 중심으로 중국의 이슬람교중국화 정책의 주요 내용과 특징을 살펴보았다. 중국정부는 아랍과는 차별화된 ‘중국식 이슬람교’라는 프레임을 만들어 내고, 이슬람교중국화 정책을 시행하였다. 본 논문은 정부의 정책에 따라 이슬람교협회가 작성한 ｢堅持我國伊斯蘭教中國化方向五年工作規劃綱要(2018—2022)｣을 주요 분석대상으로 삼아, 이슬람교중국화정책의 주요 범위와 내용을 짚어보았다. 그리고 이와 더불어 이슬람교중국화 정책의 시행에 따른 무슬림사회의 현실과 그 정책적 한계도 함께 살펴보았다.

본고에서는 ｢中国道教协会章程｣과 ｢道教五年工作规划纲要(2019-2023)｣를 통해 도교중국화의 구체적인 양상을 조명하기로 한다. 도교의 중국화에 대한 주요한 정책 방안의 구체적인 내용을 검토하고 이러한 정책이 실제 도교 교단을 중심으로 궁관 등에서 어느 정도로 관철되고 있는지 살펴보고자 하는 것이다. 특히 도교는 중국의 토착종교로서 중국정부가 인정하는 5대종교 중에서 다른 종교들과는 현격한 입장의 차이가 있다. 중화인민공화민국 건립 이후 정부의 종교정책에 따라 가장 큰 타격을 입은 도교는 실상 교단의 조직적 체계와 종교적 위상이 다른 종교 단체에 비하여 취약하다. 그럼으로 도교 중국화 과정에서 궁관의 복구와 교단의 활성화, 교리의 개발과 인재 양성, 문화사업과 해외교류를 통한 도교의 위상을 끌어 올리는 것이 시급한 과제이다. 그럼 점에서 도교중국화 과정을 통한 도교 교단의 자율성 회복 은 도교가 대중적 신앙으로 부활하는 갈림길에 서 있다고 하겠다.

We report the detection of exoplanet candidates in orbits around HD 60292 and HD 112640 from a radial velocity (RV) survey. The stars exhibit RV variations with periods of 4953 days and 6136 days, respectively. These detections are part of the Search for Exoplanets around Northern Circumpolar Stars (SENS) survey using the ber-fed Bohyunsan Observatory Echelle Spectrograph installed at the 1.8-m telescope of the Bohyunsan Optical Astronomy Observatory in Korea. The aim of the survey is to search for planetary or substellar companions. We argue that the periodic RV variations are not related to surface inhomogeneities; rather, Keplerian motions of planetary companions are the most likely interpretation. Assuming stellar masses of 1:7  0:2M⊙ (HD 60292) and 1:8  0:2M⊙ (HD 112640), we obtain minimum planetary companion masses of 6:5  1:0MJup and 5:0  1:0MJup, and periods of 495:4  3:0 days and 613:2  5:8 days, respectively.

At q = 1.81 ± 0.20 × 10-5, KMT-2018-BLG-0029Lb has the lowest planet-host mass ratio q of any microlensing planet to date by more than a factor of two. Hence, it is the first planet that probes below the apparent "pile-up" at q = 5-10 ×10-5. The event was observed by Spitzer, yielding a microlens-parallax πE measurement. Combined with a measurement of the Einstein radius θE from finite-source effects during the caustic crossings, these measurements imply masses of the host Mhost = 1.14+0.10-0.12 M⊙ and planet Mplanet = 7.59+0.75-0.69 M⊕, system distance DL = 3.38+0.22-0.26 kpc and projected separation a⊥ = 4.27+0.21-0.23 AU. The blended light, which is substantially brighter than the microlensed source, is plausibly due to the lens and could be observed at high resolution immediately.