• 한국도서관정보학회지
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• 제26권
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• pp.131-168
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• 1997

The future of a country is influenced by the youth. Sound fostering of the youth is important for the country's future. Because of mechanization, industrialization and urbanization of our society, many social problems, such as confusion of the sense of value, dehumanization, money worshi n.0, ppings, juvenile delinquency are increasing. For the solution of problems of juvenile crime and dehumanization, bibliotherapy should be practiced in juvenile reformatories, schools and societies. The purpose of this study is to investigate the effectiveness and value of reading. And also the characteristics, brief history, principles and procedures of bibliotherapy are examined. In addition, the book catalog suitable for bibliotherapy is considered. The results of the study are as follows. (1) In order to solve the problem of dehumanization, and the confusion of the sense of value among young adults, we should enrich and cultivate the characters of young adults through the bibliotherapy. So, bibliotherapy for the treatment of human nature of juveniles should be practiced in the juvenile reformatories, schools and societies. (2) The values of reading in the past were inspiration, information and recreation. But, in recent times, the interest in therapeutic value of reading is increasing. (3) Bibliotherapy is a kind of psychotherapy using selected reading materials. A n.0, pplication scopes of bibliotherapy are very wides, including mental medicine, alcoholic poisoning, drug addiction, juvenile delinquency, counselling and education for school life, etc. (4) The principles of bibliotherapy consist of identification, catharsis, insight and it has self therapeutic principles through the reading. The procedures of bibliotherapy is similar to any other kind of psychotherapy: the participant's statement, diagnosis, treatment, continuous recognition of remedial value. (5) The well suited reading materials for bibliotherapy are literature and biography. Literature and biography are familiar to everyone, because they describe the mentalities, emotions and life styles of human beings. (6) The standard reading lists for bibliotherapy for the proper guidance of juvenile delinquency should be prepared for the solution of developmental tasks, such as, drinking, smoking, friendship, family, love, money, marriage, pregnancy, violence, etc. Finally, Bibliotherapy should be introduced to our school settings and corrections institutions for the proper guidance and prevention of the malpractice of the youths. In addition, we should be endeavor to develop the standard reading lists for bibliotherapy and case study.

• 천문학논총
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• 제27권4호
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• pp.265-270
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• 2012

Many observations have found evidence of the presence of a large number of heavily obscured Active Galactic Nuclei (AGNs). However, the nature of this population is only poorly understood because heavy obscuration by dust prevents one from finding them at optical wavelengths. Mid-infrared AGN searches can overcome this obstacle by penetrating through dust and by detecting direct emission from the dust torus. Thus, we can identify most of the AGN population, including type-2 and buried AGNs. Using the AKARI mid-infrared all-sky survey, we performed an AGN search in the nearby universe. Utilizing the 2MASS photometry, we selected mid-infrared-excess sources and carried out near-infrared spectroscopic observations in the AKARI Phase 3. During these follow-up observations, we have found three galaxies that show strong near-infrared red continuum from hot dust with a temperature of about 500 K, but do not show any AGN features in other wavelengths. The most suitable explanation of near-infrared continuum is the presence of central AGNs. Therefore, we conclude that they are AGNs obscured by dust. We performed X-ray observations of the two galaxies with SUZAKU. No detections in the 0.4-10 keV suggest that the column density may be much higher than $N_H=10^{23.5}cm^{-2}$. Comparing the masses of the host galaxies with those of the SDSS AGNs, we find that the host galaxies of the dusty AGNs discovered with AKARI are less massive populations than those of optically selected AGNs.

• 한국환경생태학회지
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• 제28권2호
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• pp.182-196
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• 2014

본 연구는 계방산 가문비나무 및 전나무 임분의 산림식생유형분류와 정량적 분석을 위하여 Z-M 식물사회학적 방법으로 식생구조의 유형분류를 실시한 결과, 군락단위에서 가문비나무군락, 전나무군락으로 분류되었으며 가문비나무군락은 군단위에서 흰인가목군과 부게꽃나무군으로 세분되었으며, 전나무군락은 복장나무군과 생강나무군으로 세분되었다. 분류된 식생단위를 기준으로 중요치를 산출한 결과, 가문비나무는 식생단위 1과 2의 교목층에서 각각 30.73%, 20.25%로 비교적 높게 나타나 당분간 가문비나무의 우점이 계속될 것이라 판단되었다. 또한 종다양도를 분석한 결과 식생단위 4의 종다양도 지수는 0.6976으로 가장 낮았으며, 식생단위 2의 종다양도 지수는 1.1256으로 가장 높게 나타났다. 군락간의 유사도는 식생단위 1과 4, 2와 4가 각각 0.2880과 0.3626으로 낮게 나타났으며 식생단위 1과 2, 3과 4의 군락유사성은 각각 0.5411과 0.5041로 나타나, 군락 간 구성종의 차이가 크지 않은 군락으로 판단되었다. 종간연관에 대한 Chi-square matrix와 성좌표를 각각 분석한 결과, 크게 2개의 유형으로 나뉘어졌는데 I유형의 식물 종들은 대부분 식물사회학적으로 분류된 가문비나무군락에서 주로 출현하는 식별종과 표징종이었으며, II유형의 식물종은 전나무군락에서 주로 출현하는 식물종으로, 비교적 습한 곳에 나타나는 종들로 나뉘어졌다. 이러한 결과는 각 수종들이 선호하는 생육환경이 비슷한 종들끼리는 정의 상관이 인정되고, 선호하는 환경이 다른 종들끼리는 부의 상관을 보이는 것으로 판단된다.

• 천문학회보
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• 제40권1호
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• pp.68.2-69
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• 2015

We present [Fe II] $1.644{\mu}m$ features around ultracompact H II regions (UCHIIs) found on a quest for the "footprint" outflow features of UCHIIs -the features produced by outflowing materials ejected during an earlier, active accretion phase of massive young stellar objects (MYSOs). We surveyed 237 UCHIIs in the first Galactic quadrant, employing the CORNISH UCHII catalog and UWIFE data, which is an imaging survey in [Fe II] $1.644{\mu}m$ performed with UKIRT-WFCAM under ~0.''8 seeing conditions. The [Fe II] features were found around five UCHIIs. We interpret the [Fe II] features to be shock-excited by outflows from YSOs and estimate the outflow mass-loss rates from the [Fe II] flux which are ${\sim}1{\times}10^{-6}-4{\times}10^{-5}M{\odot}yr^{-1}$. We propose that the [Fe II] features might be the "footprint" outflow features, but more studies are required to clarify whether or not this is the case. This is based on the morphological relation between the [Fe II] and 5 GHz radio features, the outflow mass-loss rate, the travel time of the [Fe II] features, and the existence of several YSO candidates near the UCHIIs.

• 한국도서관정보학회지
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• 제23권
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• pp.79-108
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• 1995

Government Publications are published to keep records of governmental activities and performances. In a rapidly changing information-oriented society, it is badly required for the operation system of government publications and a library to be effectively managed with government publications for satisfying 'right to know' of people and improving the obligation of government to 'let people know.' Accordingly, the purpose of this paper is to analyze such five research items as the situation of the publication and distribution of, government publications, the operation system of the publications in library, the number of publications regarding secondary information sources for the publications, and the legal deposit of the publications in the National Library, in order to proceed with a subject as to how much the government publication is satisfying 'right to know' of people. The research findings were suggested as follow : 1) Despite the fact that the publication of government publications has been gradually increased every year in numbers and kinds, it is unfortunately pointed out that the publications, distributions and sellings of them were not well organized and systematic. That is, the government publications had not been published more than 1.47% of all publications in number. Moreover, more than the half of the publications were non-periodically or annually published. To make the matter worse, it was not easy to get an access to the publications because of the publications not to be sold. 2) It a n.0, ppears that people could not use the publications efficiently because the library and administrative document office did not pay sufficient attention to public relations for all sorts of government publications. Not only that, there were not enough numbers of publications regarding such secondary information sources as bibliography, index and catalog. A speedy searching capacity for the information gave rise to another serious problem which the government publications could not be effectively used. 3) It is legally stated that all sorts of government publication should be deposited to the National Libraries. However, the law was not properly put into force because of lack of understanding of government agencies about the law.

• 천문학회보
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• 제41권1호
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• pp.54.1-54.1
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• 2016

Multi-wavelength variability is a staple of active galactic nuclei (AGN). Optical variability probes the nature of the central engine of AGN at smaller linear scales than conventional imaging and spectroscopic techniques. Previous studies have shown that optical variability is more prevalent at longer timescales and at shorter wavelengths. Intra-night variability can be explained through the damped random walk model but small samples and inhomogeneous data have made constraining this model hard. To understand the properties and physical mechanism of intra-night optical variability, we are performing the KMTNet Active Nuclei Variability Survey (KANVaS). Using KMTNet, we aim to study the intra-night variability of ~1000 AGN at a magnitude depth of ~19mag in R band over a total area of ${\sim}24deg^2$ on the sky. Test data in the COSMOS, XMM-LSS, and S82-2 fields was obtained over 4, 6, and 8 nights respectively during 2015, in B, V, R, and I bands. Each night was composed of 5-13 epoch with ~30 min cadence and 80-120 sec exposure times. As a pilot study, we analyzed data in the COSMOS field where we reach a magnitude depth of ~19.5 in R band (at S/N~100) with seeing varying between 1.5-2.0 arcsec. We used the Chandra-COSMOS catalog to identify 166 AGNs among 549 AGNs at B<23. We performed differential photometry between the selected AGN and nearby stars, achieving photometric uncertainty ~0.01mag. We employ various standard time-series analysis tools to identify variable AGN, including the chi-square test. Preliminarily results indicate that intra-night variability is found for ~17%, 17%, 8% and 7% of all X-ray selected AGN in the B, V, R, and I band, respectively. The majority of the identified variable AGN are classified as Type 1 AGN, with only a handful of Type 2 AGN showing evidence for variability. The work done so far confirms there are more variable AGN at shorter wavelengths and that intra-night variability most likely originates in the accretion disk of these objects. We will briefly discuss the quality of the data, challenges we encountered, solutions we employed for this work, and our updated future plans.

• Applied Biological Chemistry
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• 제19권1호
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• pp.1-23
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• 1976

약(約) 백만종(百萬種)이나 되는 레피도프테라족(族)(Lepidoptera)의 암나방이 갖는 성적유인물질(性的誘引物質)의 화학구조(化學構造)는 직쇄상의 불포화(不飽和) 알코홀이거나 에스텔이라고 알려져 있다. 본(本) 실험(實驗)에서는 곤충(昆蟲)의 성적유인물질(性的誘引物質)이 될수도 있는 $C_{16}$의 불포화(不飽和)에스텔 이성체(異性體)를 합성(合咸)하였다. 합성(合成)된 17개(個)의 에스텔을 분광분석(分光分析)하였으며 이 분석결과(分析結果)는 곧 자연산(自然産)의 유인물질(誘引物質)에 대(對)한 가스크로마토그래피 및 질량분석결과(質量分析結果)와 쉽게 비교(比較)할 수 있는 카탈로그가 될 것이다. 순도(純度)가 높은 시스와 트랜스 이성체합성(異性體合成)에는 각각(各各) 촉매적(觸媒約) 환원(還元)과 화학적(化學約) 환원법(遣元法)이 이용(利用)되었다. 합성(合成)에 필요(必要)한 출발물질(出發物質)로서 시판(市販)의 $CH_3(CH_2)mBr,\;HC{\equiv}C(CH_2)nOH,\; CH_3-(CH_2)mC{\equiv}CH$ 및 $HO(CH_2)nOH$이 사용(使用)되었다. 메틸렌기(基) 수(數)가 9이상(以上)인 1-알킨[$CH_3(CH_2)mC{\equiv}CH$]은 알킬디할리드(alkyldihalide)와 결합(結合)하지 않았다. 디올(Diol)[$HO(CH_2)nOH$]의 분자량(分子量)이 증가(增加)함에 따라 그 결합생성물(結合生成物)의 수량(收量)이 감소(減少)하였다. 아세틸렌(Acetylene)가스와 $BrCH_2CH_2OTHP$의 결합반응(結合反應)에 있어서 $BrCH_2CH_2OTHP$는 부반응(副反應)을 일으켰다. 장직쇄 알키노올(alkynol)의 테트라 히드로피라닐 에테르(tetrahydropyranyl ether)의 가수분해(加水分解)에 있어서 파라 톨루엔설폰산(p-toluenesulfonic acid)이 희류산(稀硫酸)보다도 더 우수(優秀)하였다.

• Journal of Astronomy and Space Sciences
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• 제22권4호
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• pp.393-408
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• 2005

YSTAR-NEOPAT 탐사프로그램에서는 관측된 영상으로부터 지구접근천체와 소행성 등의 이동천체 후보를 검출하기 위해 두 가지 자동검출 알고리즘을 개발하였다. 영상들의 측광자료를 이용하여 이동천체 후보를 검출하는 측광자료 비교방법과 영상들을 정렬시킨 후 영상간 차감 과정을 통해 이동천체 후보를 검출하는 영상차감방법이 그것이다. 두 가지 알고리즘의 이동천체 후보 자동검출효율을 시험, 비교하기 위하여, YSTAR-NEOPAT자동관측 루틴에 의해 관측된 영상들의 일부를 사용하였다. 시험 영상들의 지역좌표와 등급은 기준목록인 USNO-B1.0의 좌표와 등급에 비교되었으며, 이 과정에서 광시야망원경의 심각한 영상왜곡현상들이 1.5 초각 이상의 정밀도로 모두 보정되는 것을 검증하였다. 두 알고리즘을 시험 영상에 적용한 결과, 측광자료 비교방법을 적용한 경우 1차 후보군들이 과다 검출되었고, 이들로 인해 오검출되는 이동천체 최종후보가 다수 발생하였다. 반면, 영상차감방법을 적용한 경우에는 이동천체 후보의 오검출 비율이 측광자료비교방법을 적용했을 때보다 월등히 감소하였음을 확인하였다. 마지막으로 육안확인 과정을 거친 결과, 측광자료비교방법에 의해 검출된 이동천체 후보의 총개수는 검출문턱값에 따라 각각 60개$(2.0\sigma)$, 6개$(4.0\sigma)$이며, 육안확인에 의해 실제 이동천체로 분류된 것은 각각 27개와 6개이다. 반면, 영상차감방법에서 이동천체 후보는 모두 34개$(2.0\sigma)$와 12개$(4.0\sigma)$가 검출되었으며, 이 가운데 육안확인에 의해 실제 이동천체로 분류된 것은 각각 32개와 12개이다. 따라서 YSTAR-NEOPAT영상으로부터 이동천체 후보를 효율적으로 검출하기 위해서는 절대개수측면에서나 검출효율측면에서 측광자료비교방법보다 영상차감방법이 더 적합하다는 것을 확인할 수 있다.15\~20$배가량 높았다.과 립장이 부의 값이어서 소립의 형태를 보였으며 제2주성분은 립장, 립폭, 백립중 등이 정의 값을 나타내어 대립의 계통군들이 포함되며 경도와는 부의 상관을 보여 식미가 양호한 계통군으로 분류되었다. 6. 제1주성분과 제2주성분을 이용하여 군집분석을 한 결과 8개 자식계통군으로 구분할 수 있었으며 scatter diagram에서 제1주성분이 작아지고 제2주성분이 커지는 좌측 상단부에 분포한 VII, VIII군에 속한 계통들이 주로 식미가 높으며 조숙종보다는 중, 만숙종들이 대부분 이였다. 등과 정의 상관을 보였고 과피두께, 경도, 껌성, 씹힘성 등과는 부의 상관을 나타내었다. 이와 같은 결과를 바탕으로 품질기준을 설정해 보면 저식미 교잡종인 찰옥1호(100)를 표준으로 비교하였을 때 고식미 교잡계인 연농1호, 찰옥4호, 수원45호의 유리당 함량은 $6.2\~6.6\%(111\~l18)$, 립장 $8.8\~9.7(99\~109)$, 립폭 $9.8\~10.5mm(111\~l19)$, 백립중 $38.6\~41.9g(113\~123)$, 아밀로그램의 응집점도 $28.2\~30.6RVU(123\~133)$, 과피두께 $34\~41{\mu}m(42\~51)$, texture 분석의 경도 $460\~513(43\~48)$, 씹힘성 $125\~139(51\~57)$, 껌성 $130\~148(49\~56)$의 범위에 있었다.운 표면을 보이고, Unitek사의 경우 압흔과 함께 pitting 이 관찰되며, Ormco Stainless Steel의 경우 불규칙한 pitting이 다수 존재했다.수술 시행 시기별의 차이를 보이지 않고 고른 분포를 보였다. 10. 내원한 환자를 순구개열 종류와 Angle씨 분류법에

• 천문학회지
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• 제51권3호
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• pp.49-63
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• 2018

We carry out a study of Sub-Millimeter Galaxies (SMGs) in the AKARI NEP-Deep field using the James Clerk Maxwell Telescope (JCMT) SCUBA-2 $850{\mu}m$ source catalog, released as part of the SCUBA-2 Cosmology Legacy Survey (S2CLS) program. The SCUBA-2 $850{\mu}m$ map has a root mean square (rms) noise of $1.2mJy\;beam^{-1}$ and covers an area of $0.60degree^2$. We find four SMGs which have counterparts to Herschel sources with spectroscopic redshifts in the literature. In addition, three dust obscured galaxies (DOGs) detected in Herschel bands are selected as a comparison sample. We derive IR luminosities of SMGs using the CIGALE code, which are similar to those of high redshift SMGs from previous studies. The contribution of AGN to the total IR luminosity in SMGs (2%-11%) is smaller than the lower limit for the one in DOGs (19%-35%), which is consistent with the expectation from the evolutionary scenario of massive galaxies. We search for SMGs in overdense regions as protocluster candidates and investigate four regions, including candidates around three DOGs. Finally, we argue that follow-up spectroscopic observation for the NEP-Deep field will provide crucial information to understand the role of SMGs in the evolution of massive galaxies.

• Journal of Astronomy and Space Sciences
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• 제33권2호
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• pp.127-135
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• 2016

Inactive space objects are usually rotating and tumbling as a result of internal or external forces. KOREASAT 1 has been inactive since 2005, and its drift trajectory has been monitored with the optical wide-field patrol network (OWL-Net). However, a quantitative analysis of KOREASAT 1 in regard to the attitude evolution has never been performed. Here, two optical tracking systems were used to acquire raw measurements to analyze the rotation period of two inactive satellites. During the optical campaign in 2013, KOREASAT 1 was observed by a 0.6 m class optical telescope operated by the Korea Astronomy and Space Science Institute (KASI). The rotation period of KOREASAT 1 was analyzed with the light curves from the photometry results. The rotation periods of the low Earth orbit (LEO) satellite ASTRO-H after break-up were detected by OWL-Net on April 7, 2016. We analyzed the magnitude variation of each satellite by differential photometry and made comparisons with the star catalog. The illumination effect caused by the phase angle between the Sun and the target satellite was corrected with the system tool kit (STK) and two line element (TLE) technique. Finally, we determined the rotation period of two inactive satellites on LEO and geostationary Earth orbit (GEO) with light curves from the photometry. The main rotation periods were determined to be 5.2 sec for ASTRO-H and 74 sec for KOREASAT 1.