본 논문은 예수회 선교사들이 16-18세기에 서양 원근법 관련 저서를 중국에 들여오게 된 과정과 맥락을 페어하렌의 『북당 도서관 목록』을 중심으로 고찰해 보았다. 『북당 도서관 목록』에는 예수회 선교 사들이 서양 서적을 매개로 중국의 황제나 사대부층과 대화하려는 접촉점을 마련하려 했던 역사와 노력이 반영되어 있다. 또한, 이 목록에 있는 원근법 저서의 저자와 내용을 살펴보면, 예수회 선교사들이 서양 의 예술 분야의 책뿐만 아니라, 광학, 수학, 천문학 분야의 최신 서적을 통해 중국 지식인들의 관심을 끌어서 하나님의 창조질서나 본성에 관심을 가지게 하려는 선교적 의도가 반영되어 있다. 한편 명말 청초의 중국 지식인층은 서양의 천문학이나 지리학, 수학, 기하학, 예술기법으 로서의 원근법에 커다란 관심을 가졌고, 원근법 책을 번역하는 작업에 도 관심을 가졌다. 물론 서양 선교사들이 중국 지식층에게 서양 학문을매개로 하나님을 알아가게 했던 노력은 의도한 만큼 큰 효과를 거두지는 못했다. 하지만 이러한 문서선교를 통해서 중국의 지식인 계층이 서양 의 학문과 기독교를 좀 더 주체적으로 번역하고 확산할 수 있는 기초작업 을 했다고 본다.

서평

In the 1930s, The Architectural Association of Joseon run the ‘Architectural Material Display’ on the 2nd floor of the Japan Life Insurance Building in Hwanggumjeong(currently Euljiro street). The purpose of this place was to introduce new architectural materials to builders. And they issued a 『建築資料型錄(Architectural Material Catalog)』and distributed it free of charge so that people in districts at long distances can make use of it. This catalog contains descriptions, photographs and drawings of various architectural materials that were common at the time, and the overseas branch address of the store is stated. The purpose of this research is to investigate the type and characteristics of architectural materials distributed in Northeast Asia around the 1930s, the region of sale, affiliated companies by closely analyzing the 『建築資料型錄』.

On the early stage of Emperor Qianlong period, Qianlong ordered the ministers to sort out interior cultural relics. Therefore ministers successively compiled four antiques catalogue, they are "Midian Zhulin Buddhism and Taoism paintings appreciation", "Shiqu Baoji paintings appreciation", "Ancient bronze vessels collection appreciation in Qing Dynasty" and "Tianlu Linlang official books collection catalogue appreciation" respectively. The stylistic rules and layout of the first two was borrowed from Gao Shiqi "Jiang Cun Xiao Xia Lu". The stylistic rules and layout of the record of "Ancient bronze vessels collection appreciation in Qing Dynasty" was borrowed from Wang Fu "Bo Gu Picture" and Lv Dalin "The Archaeological Picture". To a great extent, the stylistic rules and layout of "Tianlu Linlang official books collection catalogue appreciation" was inherited from the connoisseur ideology of "Shiqu Baoji paintings appreciation" and "Ancient bronze vessels collection appreciation in Qing Dynasty", which was the evolutionary adaptation of style reference and actual situation of books identification and collection. As the classic examples of official connoisseur catalogue, "Tianlu Linlang official books collection catalogue appreciation" had a significant impact on Qing dynasty bibliography. As the development of textology in Qing Dynasty, the connoisseur gradually flourished in society. Under its inspiration and influence, the edition bibliography of Qing dynasty continued to develop.

The family Thyrididae was known as a small group comprising 760 species in the world. Among them, about 30% of the species in the family was unnamed(Choi, 2005). The typical characteristics of the family Thyrididae is a window-like transparent pattern of wings. In this study, the preliminary catalogue of the family Thyrididae was presented with two newly recorded species, Striglina sp. and Rhodoneura sp., for the first time from Korea. All the available information including host plants, distributional ranges and synonymic list were provided for the further study.

We have identified 22 quasars in the AKARI far-infrared all-sky Bright Source Catalogue, using a matching radius of < 10", and excluding matches which are close to foreground extended sources or cirrus. We have confirmed a relation between quasar optical luminosity and far-infrared luminosity which was found in an earlier study. In addition, we have found that the 11 sources which are at redshift z > 1 are magnified with respect to the predicted far-infrared luminosity, and consider this may be due to gravitational lensing. If confirmed, this would provide a new way to identify lenses; if not, we may have identied an interesting new population of extreme starbursting quasars.

The point sources in the Bright Source Catalogue of the AKARI Far-Infrared Surveyor (FIS) were classied based on their FIR and mid-IR uxes and colours into young stellar object (YSO) and ex- tragalactic source types using a Quadratic Discriminant Analysis method (QDA) and Support Vector Machines (SVM). The reliability of the selection of YSO candidates is high, and the number of known YSO candidates were increased signicantly, that we demonstrate in the case of the nearby open cluster IC348. Our results show that we can separate galactic and extragalactic AKARI point sources in the multidimensioal space of FIR uxes and colours with high reliability, however, dierentiating among the extragalactic sub-types needs further information.

We plan to produce a faint source catalogue from the AKARI mid-infrared (IR) all-sky diffuse maps. In the publicly-available AKARI mid-IR point source catalogue (PSC), sources were extracted from single- scan images, and conrmed by using the other scan images. By stacking multiple scan images, we can detect fainter sources which are not listed in the PSC. We optimized the source extraction process using a 6◦  6◦ area around the star-forming region, Cepheus B. Then, we divided the all-sky data into three seasonal images, and checked the positions and the uxes of the detected sources on the images. As a result, our new source extraction method works well; 90% of the sources are also identied in the WISE catalogue. In this method, we obtain the detection limit twice deeper than that of the PSC. The number of sources increases by a factor of 2, as compared with the PSC.

We use light-curve fitting models (MLCS2k2, SALT2, and SNooPy) as implemented in SNANA to make the YOnsei Nearby Supernova Evolution Investigation (YONSEI) Supernova Catalogue. The catalogue consists of several hundred Type Ia supernovae (SNe Ia) in the redshift range from 0.01 to 1.35, and provides distance moduli, light-curve shape parameters, and color or extinction values for each supernova. This data set will be used to study the dependence of SNe Ia luminosities on the host galaxy morphologies. In this paper, we present the YONSEI Supernova Catalogue and preliminary systematic tests for the catalogue.

We performed a BVR photometric survey for the entire Small Magellanic Cloud (~26 deg 2 ) with a mosaic system, Wide Field Imager (WFI), covering three seasons: September and October 2001 and November 2002. Through the usual data reduction procedures, we present ~0.73 million catalogue stars brighter than 19 magnitude in B amongst a total of ~1.3 million and compare them with published astrometry and photometry results. We found that the average differences between our and the published data are ~0.7 arcsec in astrometry and 0.065, 0.054, and 0.163 in B, V, and R, respectively, in photometry. In addition, using the 2dF spectroscopic data from Evans et al. (2004), we determined the color excesses in (B-V) and (V-R) to be 0.086±0.156, and 0.065±0.112, respectively, while for the distance modulus, we obtained 18.55±1.05.

The current status of the AKARI-FIS Point Source Catalogue is reported. The first version of the Bright Source Catalogue has been in public since March 2010 and used extensively in the various fields in astronomy. The second version of the Bright Source Catalogue and the first version of the Faint Source Catalogue are currently under development. The revised Bright Source Catalogue is expected to have improved completeness, reliability, and accuracy compared to the current version. The Faint Source Catalogue will have a scan-density dependent detection limit and will enable much deeper exploration of the sky especially in the high-ecliptic latitude regions. Both catalogues will be available in a year time scale.