• 천문학회보
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• 제44권2호
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• pp.37.3-37.3
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• 2019

We study the stellar populations of the brightest group galaxies (BGGs) in groups whose halos have different dynamical states, using observational data from the GAMA survey. The two independent indicators to probe the dynamical state of the halo are the magnitude gap between two most luminous galaxies (∆M12) and offset between BGG and the luminosity center (Doffset) of the group. Such indicators complement each other in identifying relaxed and unrelaxed galaxy groups in our samples. We find that the BGGs of unrelaxed groups have significantly bluer NUV-r colours than in relaxed groups. This is also true at fixed sersic index. We find the bluer colours cannot be explained away by differing dust fraction, suggesting there are real differences in their stellar populations. SFRs derived from SED-fitting tend to be higher in unrelaxed systems. This could be partly because there is a greater fraction of BGGs with non-elliptical morphology, but also because unrelaxed systems are expected to have larger numbers of mergers, some of which may bring fuel for star formation. The SED-fitted stellar metallicities of BGGs in unrelaxed systems also tend to be higher, perhaps because the building blocks of the unrelaxed systems were more massive and had more time to enrich themselves. We find that the ∆M12 parameter is the most important parameter behind the observed differences in the relaxed/unrelaxed groups. We also find that groups selected to be unrelaxed using our criteria tend to have higher velocity offsets between the BGG and their group.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2009년도 하계학술대회 논문집
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• pp.113-114
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• 2009

Silicon carbide is one of the most attractive and promising wide band-gap semiconductor material with excellent physical properties and huge potential for electronic applications. Up to now, the most successful method for growth of large SiC crystals with high quality is the physical vapor transport (PVT) method [1, 2]. Since further reduction of defect densities in larger crystal are needed for the true implementation of SiC devices, many researchers are focusing to improve the quality of SiC single crystal through the process modifications for SiC bulk growth or new material implementations [3, 4]. It is well known that for getting high quality SiC crystal, source materials with high purity must be used in PVT method. Among various source materials in PVT method, a SiC powder is considered to take an important role because it would influence on crystal quality of SiC crystal as well as optimum temperature of single crystal growth, the growth rate and doping characteristics. In reality, the effect of powder on SiC crystal could definitely exhibit the complicated correlation. Therefore, the present research was focused to investigate the quality difference of SiC crystal grown by conventional PVT method with using various SiC powders. As shown in Fig. 1, we used three SiC powders with different particles size. The 6H-SiC crystals were grown by conventional PVT process and the SiC seeds and the high purity SiC source materials are placed on opposite side in a sealed graphite crucible which is surrounded by graphite insulation[5, 6]. The bulk SiC crystal was grown at $2300^{\circ}C$ of the growth temperature and 50mbar of an argon pressure. The axial thermal gradient across the SiC crystal during the growth is estimated in the range of $15\sim20^{\circ}C/cm$. The chemical etch in molten KOH maintained at $450^{\circ}C$ for 10 min was used for defect observation with a polarizing microscope in Nomarski mode. Electrical properties of bulk SiC materials were measured by Hall effect using van der Pauw geometry and a UV/VIS spectrophotometer. Fig. 2 shows optical photographs of SiC crystal ingot grown by PVT method and Table 1 shows electrical properties of SiC crystals. The electrical properties as well as crystal quality of SiC crystals were systematically investigated.

• 구강회복응용과학지
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• 제20권2호
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• pp.121-134
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• 2004

진단과 치료과정을 통해서 후천적으로 습득된 부정교합을 가진 부분무치악자 성인에게서, 교합고경을 회복해 줌으로써 3급 부정교합 안모에서 정상교합상태의 안모와 기능을 부여할 수 있었다. 대부분의 부분무치악자에서 치조골의 위축, 그리고 감소된 교합고경 인해 이루어진 부정교합자에게서 교합고경의 수복은 매우 어려운 작업이다. 적절한 안모의 심미는 대체로 interlabial gap이 약 0-2mm일 때 얻어진다. 이것과 함께, 제한된 입술 지지도(lip competence)가 교합고경 수복과 적절한 안모의 심미를 위한 지표로 사용될 수 있다. 소개된 증례의 경우는, 7년 이상의 계속 관찰 결과, 성공적인 치료였다고 판단된다. 교합고경을 증가시킨 경우이긴 하지만, 사실은 원래의 정상 교합고경으로 회복 시켜주었다고 하는 것이 더욱 옳은 표현일 것 같다. 교합고경을 증가시키는 작업은 안모의 수복, 절치부의 외상성 교합을 수정하고 하악을 후퇴시키는데 매우 어렵고도 중요한 일이다. 최종적으로, 3급 부정교합이 수정되고, 적절한 교합고경을 가지게 되었으며, 위축된 구치 무치악부가 rigid support 개념으로 제작된 가철성 의치로 수복되었다. 부분 무치악부를 가진 후천적 부정교합자의 치료의 결과로 획득한 치아 및 안모의 심미와 이것의 장기간 안정성은 다음의 관계를 잘 고려함으로써 지속될 수 있을 것으로 사료된다: 1) 이상적인 교합고경에서의 교합수복, 2) 상,하악골 관계에서 기능적으로 유도되는 최종 교합의 허용, 3) lip competence (입술 적응) 한계 내에서 기능적으로 유도되는 최종교합.

• 한국항공우주학회지
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• 제48권5호
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• pp.355-361
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• 2020

인공위성 중 군사적 성격을 띠는 저궤도 소형 인공위성의 경우 다표적 관측을 필요로 하고 고해상도의 사진 및 영상의 수요가 증가하는 추세이다. 고해상도 영상과 다표적 관측을 위해 인공위성의 기동성이 가장 큰 변수로 작용한다. 소형 인공위성의 경우 고기동성을 갖게 되면 빠르게 자세기동을 할 수 있지만 자세 기동을 완료 후 다음 자세 기동을 할 때 잔류진동이 발생하게 된다. 이에 본 연구에서 자세 기동 후 발생하는 평판의 진동 특성을 검증하기 위하여 자세기동을 모사하기 위한 실험 치구를 제작하고 실험을 수행하였다. 추가로 이러한 진동을 저감시키기 위해 영구자석을 이용한 수동형 감쇠방법으로 와전류 브레이크 시스템을 응용한 와전류 감쇠기를 제시하였다. 와전류 감쇠기를 적용하기 위하여 수학적 모델을 정립하였으며 영구자석의 자속밀도와 공극거리에 따라 이를 실험적으로 구현하였으며, 4개의 태양전지판(평판) 중 1개 평판을 특정하여 와전류감쇠기를 적용유무에 따라 자세 기동 후 발생하는 잔류진동에 대한 저감 성능을 실험적으로 검증하였다.

• Restorative Dentistry and Endodontics
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• 제21권1호
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• pp.321-338
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• 1996

The purpose of this study was to evaluate the effect of moistening and air-drying of acid conditioned dentin and enamel on the marginal microleakage. In this study, Class V cavity were prepared on both buccal and lingual surface of sixty extracted human premolars with cementum margin. These specimens were randomly devided into three groups and three dentin adhesives(Scotchbond Multi-Purpose, All bond 2, Prisma Universal Bond 3) were applied to each group. The specimens in each group were subdevided into four groups (Wet/primed, Dry/primed, Wet/not primed, Dry/not primed) and the etched dentin and enamel surface were treated these four surface treatments prior to the placement of a bonding agent or adhesive. Wet/primed group was simply blot-dried with a damp facial tissue before primer placement ; Dry/primed group was air dried for 30 seconds before the placement of a primer ; Wet/not primed group and Dry/not primed group were not primed after blot dried and air dried for 30 seconds each group. The bonding agent and composite resin were applied for each group. All specimens were exposed to 500 cycle of thermal stress. Specimens were placed in a silver nitrate solution and then sectioned buccolingually through the center of the restoration. The dye penetrations of the specimens were observed with a stereo microscope. The statistical test were applied to the results using a one way analysis variance (ANOVA) and Duncan's multiple range test. The aspects of silver ion penetration into the resin/dentin interface were examined under scanning electron microscopy. The results were as follows. 1. In all groups, the enamel margin showed significantly lower leakage value than the cementum margin (p<0.05). 2. Regardless of various surface treatment and dentin adhesives, there was no significant difference at the enamel margins (p>0.05). 3. At the dentin margins, the leakage values of Dry/not primed group showed significantly higher than that of the other groups (p<0.05). The leakage values of Wet/primed group showed significantly lower than that of the other groups, but, there was no significant difference between Wet group and Dry group. 4. There was no significantly difference between the dentin adhesives regarding the surface treatments in all groups(p>0.05). 5. On the backscatterd scanning electron microscopy observation, the penetration of the silver ion occured at the bonding resin/dentin interface. In the Wet/primed group, resindentin hybrid zone and resin penetration into the dentin was observed. The resin tags were compactively formed to a thickness of $3\sim4{\mu}m$ at the upper part of dentinal tubules. In the Dry/primed group, the thickness of the hybrid zone and the diameter, depth of the resin tags diminished. In the Non-primed groups, the hybrid zone was not identified and few resin tag was observed. There was the gap formation in the resin/dentin interface.

• 한국도서관정보학회지
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• 제19권
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• pp.145-209
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• 1992

This study, that is made by an on-the-spot survey and a library survey, is aimed at finding some problems in the recognition regarding public library users and suggesting the clue to solve the problems revealed in the way of having compared with 'Book-Room' and Public Library. Poor material was always a troublemaker in this study. Especially the part of 'Book-Room' phenomenon is wholly dependent upon a field survey, that is, interview with a 'book-room' clerks, gathering the advertising leaflets, a close observation on 'Book-Room', etc. There are little printed materials, much less precedent research theses. In the other parts of this paper, there are needed good statistical materials, but the nortion presented in the public library user statistics-for example pupil, students, housewives, old men, the generality of people, etc.- is so vague that it is insufficient and unhelpful for this study. In my judgment, with all these limitations, this article gets some results as follows : 1. 'Book-Room' is the cultural organization which is being operated by, for, of the community inhabitants and it takes on the character of movement - labor movement, cultural movement, and community movement. 2. The pioneer of the Book-Room is 'Yangso Hyupdong chohap' (which means good book- cooperative association) lasted from 1978 to the next year. 3. 'Arom'(means learning) Book-Room is the first real Book-Room at Seomyon district in Pusan established in 1987. 4. Book-Room can be classified by its character as 'Labor BookRoom' and 'Cultural Book-Room'. There are 10 Labor BookRooms and 4 Cultural Book-Rooms in Pusan. 5. Labor Book-Rooms organized themselves to 'Labor Book-Room conference'. 6. Book-Rooms have done their best to extort the needs and interests of the community inhabitants, but relatively public libraries do not, hence the majority of residents are neglected from the public library service. This is at Book-Rooms' back to have been spread so quickly. 7. There is a very large gap between the component ratio of community inhabitants by class and that of public library users by same criterion, that is, in the case of the former, the labor class goes beyond a half point, in the latter, the majority of public library user is composed of students and housewives. 8. Researchers and librarians have concentrated their attention and effort not upon whole residents in community but upon existing users at present time. They do not try to develope potential users. So, researchers' and librarians' recognition regarding the public library users needs to be changed. 9. The concept of 'core-user' may be the key to solve the problems related with public library users. For the purpose of ensuring the 'core-user', it is necessary to study the community and inhabitants.

• 한국콘텐츠학회논문지
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• 제9권8호
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• pp.360-366
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• 2009

본 연구는 하체 비만 해소를 위한 효과적인 방법을 모색하고자 실시하였다. 여대생을 대상으로 아로마에센셜 오일을 이용한 경락마사지를 한 후 그 결과를 살펴보고자 하였다. 연구 대상은 본 연구에 참여를 희망하는 여대생을 중심으로 선발하였으며, 기간은 2008년 4월부터 6월까지로 8주였다. 선발군은 체성분 분석기로 체지방량과 체중을 측정하고 그 평균을 측정치로 이용하였으며, 표준과 과체중 각 4명씩, 비만 8명으로 분류하고 비만을 실험군으로, 표준과 과체증을 대조군으로 삼았다. 각 군은 아로마 에센션 오일 중 비만 해소에 효과가 있다고 선행연구에서 밝혀진 쥬니퍼 베리, 사이프러스, 파출리를 1:1:0.8의 비율(5방울(약 1ml),5방울, 4방울)로 혼합한 후 베이스오일로 30ml의 호호바 오일과 혼합하여 사용하였으며 선발군에 에센셜 오일 테스트를 거친 후 30분씩 하체 부위에 경락마사지를 실시하는 실험을 하였다. 실험을 통해 실험군과 대조군 모두 체중, 허벅지와 종아리 치수, 체지방률이 줄어드는 결과를 얻었다. 체지방률에서는 실험군과 대조군 모두 체지방률이 감소하였다. 다만 대조군과 실험군에서 각각 한 명씩이 체지방률이 약간 증가하였다. 혈액측정을 통한 연구 결과는 실험군과 대조군 모두 총콜레스테롤, LDL, 중성지방, 혈당 수치가 감소하였으나, HDL은 수치가 증가하는 결과를 얻었다. 이를 통해 여대생들의 잘못된 비만 관리가 이상 수치를 일으킬 수 있음을 발견할 수 있었으며 실험자의 각오와 인내심에 따라 결과치가 다름을 알 수 있었다.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2008년도 추계학술대회 논문집 Vol.21
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• pp.50-50
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• 2008

ZnO has been extensively studied for optoelectronic applications such as blue and ultraviolet (UV) light emitters and detectors, because it has a wide band gap (3.37 eV) anda large exciton binding energy of ~60 meV over GaN (~26 meV). However, the fabrication of the light emitting devices using ZnO homojunctions is suffered from the lack of reproducibility of the p-type ZnO with high hall concentration and mobility. Thus, the ZnO-based p-n heterojunction light emitting diode (LED) using p-Si and p-GaN would be expected to exhibit stable device performance compared to the homojunction LED. The n-ZnO/p-GaN heterostructure is a good candidate for ZnO-based heterojunction LEDs because of their similar physical properties and the reproducibleavailability of p-type GaN. Especially, the reduced lattice mismatch (~1.8 %) and similar crystal structure result in the advantage of acquiring high performance LED devices with low defect density. However, the electroluminescence (EL) of the device using n-ZnO/p-GaN heterojunctions shows the blue and greenish emissions, which are attributed to the emission from the p-GaN and deep-level defects. In this work, the n-ZnO:Ga/p-GaN:Mg heterojunction light emitting diodes (LEDs) were fabricated at different growth temperatures and carrier concentrations in the n-type region. The effects of the growth temperature and carrier concentration on the electrical and emission properties were investigated. The I-V and the EL results showed that the device performance of the heterostructure LEDs, such as turn-on voltage and true ultraviolet emission, developed through the insertion of a thin intrinsic layer between n-ZnO:Ga and p-GaN:Mg. This observation was attributed to a lowering of the energy barriers for the supply of electrons and holes into intrinsic ZnO, and recombination in the intrinsic ZnO with the absence of deep level emission.

• 천문학회지
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• 제49권1호
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• pp.25-35
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• 2016

Multiple color selection techniques are successful in identifying quasars from wide-field broadband imaging survey data. Among the quasars that have been discovered so far, however, there is a redshift gap at 5 ≲ z ≲ 5.7 due to the limitations of filter sets in previous studies. In this work, we present a new selection technique of high redshift quasars using a sequence of medium-band filters: nine filters with central wavelengths from 625 to 1025 nm and bandwidths of 50 nm. Photometry with these medium-bands traces the spectral energy distribution (SED) of a source, similar to spectroscopy with resolution R ~ 15. By conducting medium-band observations of high redshift quasars at 4.7 ≤ z ≤ 6.0 and brown dwarfs (the main contaminants in high redshift quasar selection) using the SED camera for QUasars in EArly uNiverse (SQUEAN) on the 2.1-m telescope at the McDonald Observatory, we show that these medium-band filters are superior to multi-color broad-band color section in separating high redshift quasars from brown dwarfs. In addition, we show that redshifts of high redshift quasars can be determined to an accuracy of Δz/(1 + z) = 0.002 - 0.026. The selection technique can be extended to z ~ 7, suggesting that the medium-band observation can be powerful in identifying quasars even at the re-ionization epoch.

• 천문학회보
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• 제37권1호
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• pp.42-42
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• 2012

The First stars (Pop.III stars) in the universe are expected to be formed between the recombination era at z - 1100 and the most distant quasar (z - 8). They have never been directly detected due to its faintness so far, but can be observed as a background radiation at around 1${\mu}m$ which is called the Cosmic Near-Infrared Background (CNB). Main part of the CNB is thought to be redshifted Lyman-alpha from gas clouds surrounding the Pop.III stars. Until now, the COBE (COsmic Background Explorer) and the IRTS (Infrared Telescope in Space) observed excess emission over the background due to galaxies. To confirm the COBE and the IRTS results and pursue more observational evidences, we carried out the sounding rocket experiment named the Cosmic Infrared Background ExpeRiment (CIBER). The CIBER is successfully launched on July 10, 2010 at White Sands Missile Range, New Mexico, USA. It consists of three kinds of instruments. We report the results obtained by LRS (Low Resolution Spectrometer) which is developed to fill the uncovered spectrum around 1${\mu}m$. LRS is a refractive telescope of 5.5 cm aperture with spectral resolution of 20 - 30 and wavelength coverage of 0.7 to 2.0${\mu}m$. After subtracting foreground components (zodiacal light, integrated star light and diffuse galactic light) from the sky brightness of observed five fields, there remained significant residual emission (even for the lower limit case) consistent with the IRTS and the COBE results. In addition, there exists a clear gap at 0.7 - 0.8${\mu}m$ in the CNB spectrum over the background due to galaxies according to recent results (Matsuoka et al. 2011; Mattila et al. 2011). The origin of the excess emission could be ascribed to the Pop.III stars with its active era of z = 7 - 10.