Jedoguk and Jaesiljaesanjeongriguk were the offices related to the reorganization of the royal finance during the Residency-General period and surveyed royal facilities. Jedoguk surveyed palaces, offices and royal ritual facilities in the manner of traditional survey. However, Jaesiljaesajeongriguk which is the successor office to Jedoguk surveyed royal facilities using the modern surveying techniques and figured out the value of royal facilities. In 1908, most of the royal facilities were nationalized and were managed as government property by Takjibu. These nationalized royal facilities were used new modern facilities under the rule of Japanese.

The Herschel Space Observatory is the European Space Agency's state of the art infrared space telescope launched into space on 14 May 2009, covering the wavelength range from 70-700 microns with 3 instruments SPIRE, PACS and HIFI. Large area surveys are being carried out by Herschel in the AKARI legacy fields at the North and South Ecliptic Poles and the AKARI All-Sky Survey provides additional synergy with the largest survey with Herschel, H-ATLAS, covering more than 500 square degrees. This paper reports on some of the early results of these synergies between Herschel and AKARI including the first comparison of the AKARI All-Sky Survey number counts with the deeper Herschel surveys.

A sample of nearby galaxies was built from the AKARI/FIS all sky survey cross-correlated with the SDSS and GALEX surveys. The spectral energy distributions from 0.15 to 160 microns of these galaxies are analysed to study dust attenuation and star formation properties. The calibrations of the amount of dust attenuation as a function of the IR-to-UV flux ratio and the FUV-NUV colour are re-investigated: the former one is confirmed to be robust and accurate whereas the use of the FUV-NUV colour to measure dust attenuation is found highly uncertain. The current star formation rate given by the SED fitting process is compared to that directly obtained from the UV and total IR luminosities. It leads to an accurate estimate of dust heating by old stars. We emphasize the importance of such a sample as a reference for IR selected star forming galaxies in the nearby universe.

We combine data from two all-sky surveys, the Swift/Burst Alert Telescope 22 Month Source Catalog and the AKARI Point Source Catalogue, in order to study the connection between the hard X-ray (> 10 keV) and infrared (IR) properties of local active galactic nuclei (AGN). We find two photometric diagnostics are useful for source classification: one is the X-ray luminosity vs. IR color diagram, in which type 1 radio-loud AGN are well isolated from other AGN. The second one uses the X-ray vs. IR color-color diagram as a redshift-independent indicator for identifying Compton-thick (CT) AGN. Importantly, CT AGN and starburst galaxies in composite systems can also be separated in this plane based upon their hard X-ray fluxes and dust temperatures. This diagram may be useful as a new indicator to classify objects in new surveys such as with WISE and NuSTAR.

We present the method of star/galaxy separation based on the support vector machines (SVM) in the data from the AKARI North Ecliptic Pole (NEP) Deep survey collected through nine AKARI / IRC bands from 2 to 24 μm , with a classification accuracy of 93 %.

We present the results of Spectral Energy Distribution (SED) fitting of far-infrared galaxies detected in the AKARI Deep Field-South (ADF-S) Survey and discuss their physical properties. Additionally, we perform a comparison between photometric redshifts estimated using only optical and both optical and infrared data. We conclude that our sample consists mostly of nearby galaxies rich in dust and young stars. We observe an improvement in the estimation of photometric redshifts when the IR data are included, comparing to a standard approach based mainly on the optical to UV photometry.

Far-infrared observations provide crucial data for the investigation and characterisation of the properties of dusty material in the Interstellar Medium (ISM), since most of its energy is emitted between ~ 100 and 200 μm . We present the first all-sky image from a sensitive all-sky survey using the Japanese AKARI satellite, in the wavelength range 50 − 180 μm . Covering > 99% of the sky in four photometric bands with four filters centred at 65 μm , 90 μm , 140 μm , and 160 μ m wavelengths, this achieved spatial resolutions from 1 to 2 arcmin and a detection limit of < 10 MJy s r − 1 , with absolute and relative photometric accuracies of < 20%. All-sky images of the Galactic dust continuum emission enable astronomers to map the large-scale distribution of the diffuse ISM cirrus, to study its thermal dust temperature, emissivity and column density, and to measure the interaction of the Galactic radiation field and embedded objects with the surrounding ISM. In addition to the point source population of stars, protostars, star-forming regions, and galaxies, the high Galactic latitude sky is shown to be covered with a diffuse filamentary-web of dusty emission that traces the potential sites of high latitude star formation. We show that the temperature of dust particles in thermal equilibrium with the ambient interstellar radiation field can be estimated by using 90 μm , 140 μm , and 160 μm data. The FIR AKARI full-sky maps provide a rich new data set within which astronomers can investigate the distribution of interstellar matter throughout our Galaxy, and beyond.

Korea is recognized home and abroad as a country where various religions exist without conflict or enmity which is rare in the world. However, it's certain that Korea is one of the country where social conflict can happen caused by religious conflict or enmity at any time. The conflict and enmity among religions are already deep and it can’t be solved by temporary measure. It will be difficult to overcome this problem without continuous and honest conversations among religions. This study was done with this issue and I aim at finding the new way for conversation and collaboration to reach peace among religions. In Korea, the portion of protestantism and buddhism is biggest and these two religions have the most serious conflict between them. In this situation, I analyzed two survey results. One is ‘the survey for social credit to Korean churches’ done by ‘Christian Ethics Movement of Korea’ with the aim of “evaluating the social credit of Korean churches and finding a way to enhance it.” The other is ‘social culture in Korea and survey of people about religion’ done by ‘Buddhism Society Institute,’ affiliated by Jogye Order of Korean Buddhist with the aim of “finding a indicator for religions in Korea including buddhism and to utilize as a fundamental data on social culture and religion in Korea.” The result of the study shows that the future of Korea churches will be pessimistic if they continue church individualism and aggressive evangelism for the growth of church. It is an urgent task to reform such a image. The way to reach the harmony and co-existence for the peace among religions may be different but being different does not mean wrong. I believe that we can reach harmony with the spirit of ‘Hwa-i-bu-dong’(peace in difference) which is admitting and respecting others. In this era, community spirit is required for rebuilding of community. Religion is not an exception of it. Furthermore, religion has more responsibility and duty compared to other sectors in the society to enhance community spirit and social spirit. Like this, it can be the way to reach the ultimate goal or original function of the religion. For conversation and collaboration among religions, the authenticity from the deep inside of people’s heart is required absolutely.

In this study, 3,301 domestic and foreign patents, established from 1980 to June, 2007, were reviewed in order to examine the technological trends in treating or preventing liver disease. Primary focus was placed on countries such as Korea, Japan, and the United States - the leading nations with regard to liver function research. This paper explores the systematic search that utilized a research-focused database and research analysts. Since the year 2000, Korea has demonstrated increased developments in the area of diet and liver disease, as shown by an increase in relevant patent caseloads and submissions especially for medicinal preparations containing compounds or reaction products with undetermined constitutions. In addition, there was up to a 29% increase in themarket share and the frequency of patent submissionshad increased. Japan has shown a similar trend to Korea with an increase in research, but has focused more on medical preparations containing active organic ingredients. In the United States, an increase in the number of patents was shown after the year 2000.

A technological trend of treating or preventing the cardiovascular diseases has reviewed on 381 domestic and foreign patents from the year 1980 to June, 2007. Primarily focused upon countries such as Korea, Japan and the United States; the leading nations concerning cardiovascular disease, this paper delved into a systematic research of the cardiovascular disease utilizing research focused database and research analysts. Korea was showing increased development in the diet and cardiovascular related areas as shown by increase in related patent caseloads and submission since the 2000. Especially within the area of food production, there had been an increase of market share by up to 50% and the frequency of patent submission had also increased. Japan was showing similar trend as Korea with its increase in research, but the only difference was that Japan was focused more upon medical supplies. With the United States, there was no real consistency with the number of patents, therefore harder to make an accurate assessment.

We present measurements of interstellar H2 absorption lines in the continuum spectra of 54 early-type stars in the Galactic disk and halo and 3 stars in the Magellanic Clouds. The data were obtained with the Berkeley Extreme and Far-Ultraviolet Spectrometer (BEFS), part of the ORFEUS telescope, which flew on the ORFEUS-SPAS I and II space-shuttle missions in 1993 and 1996, respectively. The spectra extend from the interstellar cutoff at 912＼AA to about 1200＼AA with a spectral resolution of ∼3000 and statistical signal-to-noise ratios between 10 and 65. Assuming a velocity profile derived from optical observations (when available), we model the column densities N(J) of the rotational levels J = 0 through 5 for each line of sight. Our data reproduce the relationships among molecular and total hydrogen column density, fractional molecular abundance, and reddening first seen in Copernicusobservations of nearby stars (Savage et al. 1977). The results show that most of these molecular clouds have H2 total column densities between 1015cm−2 and 1021cm−2, and kinetic temperatures from 21 K to 232 K, with average of 89 K, consistent with the result of Copernicus (Savage et al. 1977).

On behalf of the IRSF/SIRIUS group, I introduce some recent results from our deep near-infrared surveys (J, Hand Ks bands, limiting magnitude of Ks=17) toward star forming regions in the Milky Way Galaxy (MWG) and Large Magellanic Cloud (LMC) with the near-infrared camera SIRIUS. We discovered a rich population of low-mass young stellar objects associated with the W3 and NGC 7538 regions in the MWG based on the near-infrared colors arid magnitudes. The high sensitivity of our survey enables us to detect intermediate-mass pre-main sequence stars, i.e. HAEBE stars, even in the LMC. We detected many HAEBE candidate stars in the N159/N160 complex star forming region in the LMC with the IRSF 1.4-m telescope. Spatial distributions of the young stellar objects indicate the sequential cluster formation in each star forming region in the complex and large scale (a few X 100 pc) sequential cluster formation over the entire complex.

1978년에 규모 5.0의 지진이 발생한 홍성지역에 발달한 단층대의 전기, 전자적 특성을 조사하였다. 전기, 전자 탐사는 최근 토목공사현장에서 단층대 및 파쇄대 등의 연약지반을 확인하기 위한 수단으로 널리 쓰이고 있으며 이들 탐사로부터 얻어지는 전기비저항 구조는 연약대의 공간적 분포를 효과적으로 파악할 수 있는 정보를 제공한다. 홍성지역에 위치한 단층대를 가로질러 쌍극자배열 전기비저항탐사와 MT (Magnetotelluric) 탐사를 실시하였으며 역산을 통해 단층대의 전기비저항의 분포를 추정하였다. MT 탐사는 주단층대를 가로지르는 2.9 km의 측선상의 18측점에서 실시하였으며, 자기쌍극자를 인공 송신원으로 사용하였다 전기탐사는 단층대를 측선의 중앙으로 하여 전극간격이 50 m인 쌍극자배열전기비저항 탐사를 실시하였다. 두 탐사 결과는 예상단층선을 따라 좌우지역의 전기비저항이 서로 다른 양상으로 발달하고 있음을 보여주고 있으며, 특히 예상단층선을 따라서는 뚜렷한 저비저항대가 깊게 발달해 있음을 보여주고 있다. 홍성지역의 단층대에서 낮은 전기비저항분포를 보이는 부분이 수직으로 잘 발달해 있다는 것은 최근에 두 차례의 지진이 발생한 것처럼 이 지역 단층이 활동 중인 단층이라는 사실과 일치하는 결과를 보여주는 것이다. 본 연구 성과는 앞으로 홍성단층 뿐만이 아니라 우리나라에서 발생하는 지진들에 대한 연구에 기초 자료를 제공할 것이라 기대된다.