Technosignature, previously known as SETI(search for extraterrestrial intelligence), is the scientic evidence of past or present extraterrestrial civilizations. Since NRAO's Project Ozma was performed in 1960, most of the noticeable technosignature searches have been done by radio telescopes, hoping to find strong and narrow bandwidth signals that cannot be explained by known natural processes. Recently, the Breakthrough Listen project has opened a new opportunity for technosignature by utilizing both optical telescopes, radio telescopes, and next-generation radio telescope arrays. In this review, mainly based on NASA Technosignatures Workshop (2018), we review the current trends of technosignature surveys, as well as other possible methods for detecting technosignature. Also, we suggest what the Korean community could contribute the technosignature research, including the new SETI project with Korea VLBI Network (KVN).

Since the farside of the moon is a place to avoid arti cial radio frequency interference (RFI) created byhuman civilization, it is a most suitable place for searching technosignature, which are signs of technolog-ical civilization in the universe, in the radio band. The RFI is a factor that makes the study of searchingtechnosignature quite complicated because it is di cult to distinguish between technological signals pro-duced by human and extraterrestrial civilizations. In this paper, we review why the farside of the moon isthe best place to detect technosignature and also introduce radio observatories on the farside of the moonthat have been proposed in radio astronomy. The SETI (Search for Extraterrestrial Intelligence) projecton the farside of the moon is expected to be one of the main candidates for international collaborationresearch topics on lunar surface observatory.

"Are we alone in the universe?" is the fundamental question of mankind. To search for the life signaturesin the universe, there have been a lot of researches and space explorations, especially in our solar system. In this review paper, we introduce the de nition and characteristics of the \biosignature". The currentsituations and future plans for searching for biosignatures in our solar system are reviewed, especially atVenus, Mars, and Ocean Worlds such as Europa and Enceladus where life signatures are more likely toexist than in other places in the solar system. Finally, we discuss the opportunities and strategies for theKorean scienti c society to participate in searching for biosignatures in the solar system.

본 연구에서는 식품섭취량 데이터를 활용하여, 한국인의 식습관을 분석하고 관리방향을 제안하였다. 국민건강영양 조사의 원시자료를 활용하고, 국내 대표적 식품 분류체계인 식품공전을 반영해서 품목수 839개(세부품목수 1,419개)를 대상으로 실시하였다. 일일 총 식품섭취량은 1,585.77 g/day 이고, 그 중 원재료식품은 858.96 g/day(54.2%), 가공식품은 726.81 g/day(45.8%)로 산출되었다. 식품군별 식품섭취량은, 곡류가 가장 높은 비율을 차지했고, 식품섭취량 상위15위 식품군 중 90% 이상의 대상자가 섭취하는 목록으로는 곡 류(99.06%), 근채류(95.80%)로 나타났다. 품목별 분석에 의하면 주요 다소비(일일식품섭취량 1%이상 섭취, 158.6 g/ day) 및 다빈도(일일평균 국민 25% 이상 섭취, 5,168명) 품목은 쌀, 배추김치, 사과, 무, 달걀, 고추, 양파, 밀, 두부, 감자, 오이, 돼지고기로 산출되었다. 섭취빈도 중심의 상위순위 목록은 주로 한식양념 재료들이 포함되었다. 김치류는 배추김치(64.89 g/day)의 섭취량 비율이 67%로 가장 높게 나타났다. 주류의 경우 섭취량 및 섭취빈도 모두 상위 5위 안에 포함되어 있으며, 세부적인 섭취량은 맥주 (63.53 g/day), 소주(39.11 g/day), 막걸리(19.70 g/day) 순으로 높았고, 섭취빈도는 소주(11.3%), 맥주(7.2%), 청주(6.6%) 순으로 높게 산출되었다. 2010년부터 2015년도 식품섭취 량 추이에서 곡류는 꾸준하게 감소하고, 음료류는 다소 증가하는 추세였다. 주류의 섭취빈도에서는 일부 종류인 막걸리, 와인, 청주, 복분자주에서 년도별로 감소하는 경향 이었고, 김치류도 감소하는 추세였다. 식품 섭취패턴은 체내노출과 직접적인 영향이 있으며, 식품섭취량이 높은 식품과 섭취빈도가 높은 식품 모두 관리가 중요하지만, 우 리나라 섭취 특성을 고려하여 국내에 적합한 안전관리 방안 마련이 필요하다. 식품 섭취로 인한 유해오염물질의 노출량 관리를 위해서 다소비 식품은 섭취용량과 관련이 높으므로 식품의 오염도 관리 중심으로 다빈도 식품은 섭취 기간과 관련이 높으므로 섭취시 장기노출로 인한 체내축적 중심으로 접근하는 것을 권장한다.

The DEEP-South (the Deep Ecliptic Patrol of the Southern Sky) photometric census of small Solar System bodies produces massive time-series data of variable, transient or moving objects as a by- product. To fully investigate unexplored variable phenomena, we present an application of multi-aperture photometry and FastBit indexing techniques for faster access to a portion of the DEEP-South year-one data. Our new pipeline is designed to perform automated point source detection, robust high-precision photometry and calibration of non-crowded fields which have overlap with previously surveyed areas. In this paper, we show some examples of catalog-based variability searches to find new variable stars and to recover targeted asteroids. We discover 21 new periodic variables with period ranging between 0.1 and 31 days, including four eclipsing binary systems (detached, over-contact, and ellipsoidal variables), one white dwarf/M dwarf pair candidate, and rotating variable stars. We also recover astrometry (< ±1–2 arcsec level accuracy) and photometry of two targeted near-earth asteroids, 2006 DZ169 and 1996 SK, along with the small- (0.12 mag) and relatively large-amplitude (0.5 mag) variations of their dominant rotational signals in R-band.