• 제목/요약/키워드: Korean origin

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돼지, 닭 및 소유래 Staphylococcus hyicus에 대한 swine phage와 chicken phage의 용균능 비교 (A comparison of lytic activity of swine and chicken phages with Staphylococcus hyicus of swine, chicken and cattle origin)

  • 박청규;장한내;권영삼
    • 대한수의학회지
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    • 제43권1호
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    • pp.87-94
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    • 2003
  • The lytic activity of the set of swine and chicken phages which were derived from lysogenic Staphylococcus hyicus strains of swine and chicken origin was compared by means of S. hyicus isolated from swine, chicken and cattle. Of the 80 strains each from swine and chicken, 71 (88.8%) of strains from swine and all the strains of chicken origin were found to be lysogenic. Swine phages showed wider range of lytic activity to the examined strains than that of chicken phages. Using chicken phages at $100{\times}routine$ test dilution (RTD), 25.0%, 85.6% and 50.0% of swine, chicken and bovine strains were lysed, respectively. However, when the set of swine phages was used at $100{\times}RTD$, higher frequency of the typable strains was found in strains of swine and chicken origin (73.8% and 90.2%). Phage F12 and L16 from chicken set were found to be highly active with chicken and bovine strains. On the contrary, all the swine strains were completely resistant to lysis by the two phages at $100{\times}RTD$. Thirteen (12.5%) of 104 S. aureus strains, 1 (1.8%) of 55 S. simudance strains, 31 (58.5%) of 53 S. chromo genes strains, and none of 31 strains of other coagulase-negative Staphylococcus species isolated from bovine mastitis were typable with the set of swine phages.

Do Galaxy Mergers Enhance Star Formation Rate in Nearby Galaxies?

  • 임구;임명신;최창수;윤용민
    • 천문학회보
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    • 제42권1호
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    • pp.50.1-50.1
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    • 2017
  • We present our study of the correlation between star formation rate(SFR) and merging activities of nearby galaxies(d<150Mpc). Our study uses 265 UV-selected galaxies which are not classified as AGN. The UV selection is made using the GALEX Atlas of Galaxies (Gil de Paz+07) and the updated UV catalog of nearby galaxies (Bai+15). We use deep R band optical images reaching to $1{\sigma}$ surface brightness detection limit ${\sim}27mag/arcsec^2$ to classify merger features by visual inspection. We also estimated unobscured SFR($SFR_{NUV}$) and obscured SFR($SFR_{W4}$) using Near-UV continuum and 22 micron Mid-IR luminosity respectively as a indicator of star forming activity. The fraction of galaxies with merger features in each SFR bin is obtained to see if how the fraction of galaxies with merging features($F_m$) changes as a function of SFR. As a result, for 203 late type galaxies(LTGs), we found that merger fraction increases from ~8% up to 50% with $SFR_{W4}$, while for 229 LTGs $SFR_{NUV}$ shows relatively consistent fraction(~18%) of merger fraction. For early type galaxies(ETGs), we could also find no significant correlation between $F_m$ and SFR(both $SFR_{NUV}$ and $SFR_{W4}$). This result suggests that a main driver of star forming activity of UV bright galaxies, especially for obscured late types, is mergers.

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Software Architecture of KHU Automatic Observing Software for McDonald 30-inch telescope (KAOS30)

  • Ji, Tae-Geun;Byeon, Seoyeon;Lee, Hye-In;Park, Woojin;Lee, Sang-Yun;Hwang, Sungyong;Choi, Changsu;Gibson, Coyne A.;Kuehne, John W.;Prochaska, Travis;Marshall, Jennifer;Im, Myungshin;Pak, Soojong
    • 천문학회보
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    • 제43권1호
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    • pp.69.4-70
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    • 2018
  • KAOS30 is an automatic observing software for the wide-field 10-inch telescope as a piggyback system on the 30-inch telescope at the McDonald Observatory in Texas, US. The software has four packages in terms of functionality and is divided into communication with Telescope Control System (TCS), controlling of CCD camera and filter wheel, controlling of focuser, and script for automation observing. Each interconnect of those are based on exe-exe communication. The advantage of this distinction is that each package can be independently maintained for further updates. KAOS30 has an integrated control library that combines function library connecting each device and package. This ensures that the software can extensible interface because all packages are access to the control devices independently. Also, the library includes the ASCOM driver platform. ASCOM is a standard general purpose library that supports Application Programming Interface (API) of astronomical devices. We present the software architecture of KAOS30, and structure of interfacing between hardware and package or package and package.

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A Morphometric Aspect of the Brachial Plexus in the Periclavicular Region

  • Lee, Jung-Pyo;Chang, Jae-Chil;Cho, Sung-Jin;Park, Hyung-Ki;Choi, Soon-Kwan;Bae, Hack-Gun
    • Journal of Korean Neurosurgical Society
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    • 제46권2호
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    • pp.130-135
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    • 2009
  • Objective: The purpose of this study was to determine the normal morphometric landmarks of the uniting and dividing points of the brachial plexus (BP) in the periclavicular region to provide useful guidance in surgery of BP injuries. Methods: A total of 20 brachial plexuses were obtained from 10 adult, formalin-fixed cadavers. Distances were measured on the basis of the Chassaignac tubercle (CT), and the most lateral margin of the BP (LMBP) crossing the superior and inferior edge of the clavicle. Results: LMBP was located within 25 mm medially from the midpoint in all subjects. In the supraclavicular region, the upper trunk uniting at 21$\pm$7 mm from the CT, separating into divisions at 42$\pm$5 mm from the CT, and dividing at 19$\pm$4 mm from the LMBP crossing the superior edge of the clavicle. In the infraclavicular region, the distance from the inferior edge of the clavicle to the musculocutaneous nerve (MCN) origin was 49$\pm$12 mm, to the median nerve origin 57$\pm$7 mm, and the ulnar nerve origin 48$\pm$6 mm. From the lateral margin of the pectoralis minor to the MCN origin the distance averaged 3.3$\pm$10 mm. Mean diameter of the MCN was 4.3$\pm$1.1 mm (range, 2.5-6.0) in males (n = 6), and 3.1$\pm$1.5 mm (range, 1.6-4.0) in females (n = 4). Conclusion: We hope these data will aid in understanding the anatomy of the BP and in planning surgical treatment in BP injuries.

$B_t$ Band의 형성 과정 (Origin of Banded $B_t$ Horizons in Sandy Deposits)

  • 오경섭
    • 한국제4기학회지
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    • 제3권1호
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    • pp.35-45
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    • 1989
  • 한국과 서부 유럽의 사질층에 발달해 있는 $B_t$ band의 성인은 퇴적학적인 현상과는 무관하다. 그렇다고 토양학적인 사고만으로도 설명될 수 없다. 본 연구 결과 $B_t$ band는 사질층이 형성된 후 시기를 달리하여 다음과 같이 두 부류의 물질이 서로 다른 메카니즘에 의해 이동.집적되어 형성되었다. 1)먼저 silt중심의 heterometric fine grains과 운모류들이 결빙과 관련된 cryophoresis에 의해 이동되어 이들이 사질층 단면에서 밴드 형태로 집적되었고 2)다음에 철분을 함유한 점토가 토양수에 의해 이미 형성된 맨드에 집적되어 결국 적색의 $B_t$ band가 형성되었다. 이 두 과정에서 전자는 토양의 결빙이 지표에서 3m 정도 이상까지 진전될 정도로 한랭하고 습윤한 환경과, 후자는 podzolization이 진행되는 정도의 냉량.습윤한 환경과 관련된다. 오늘날 갈색토화작용(brunification)이 진전되는 우리나라와 서부 유럽의 경우, $B_t$ band의 polygenetic한 성인과 관련된 한랭.습윤한 환경들은 제4기 근자(주로 Wurm빙기 이래)의 고환경으로 추정된다.

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인산비옥도(燐酸肥沃度)가 상이(相異)한 답토양(畓土壤)에서 환원용출(還元溶出)되는 인산형태(燐酸形態)의 추정(推定) (Estimation of Chemical Forms of Phosphate Released from the Paddy Soils with Different Effect of Phosphate Application)

  • 홍정국
    • 한국토양비료학회지
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    • 제15권2호
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    • pp.89-94
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    • 1982
  • 1. 벼수량(收量)에 미치는 인산시용효과(燐酸施用効果)가 현저(顯著)하지 않은 화강암유래(花崗岩由來) 보통답(普通畓)과 시용효과(施用効果)가 현저(顯著)한 현무암유래중점질답(玄武岩由來重粘質畓)에 있어서 담수(湛水)에 따라 용출(溶出)되는 인산염(燐酸塩)을 추정(推定)하기 위해 solubility diagram법(法)을 사용(使用)했다. 2. 토양용액중(土壤溶液中) 인산농도(燐酸濃度), 양(陽)이온농도(濃度), pH치(値)의 담수(湛水)에 따른 변화(変化)를 측정(測定)했다. 그 변화양상(変化樣相)은 어느 토양(土壤)에서도 비슷했다. 보통답(普通畓)의 인산시용구(燐酸施用区), 무시용구(無施用区)의 값은 비슷했으나 중점질답(中粘質畓)에서는 차이(差異)가 보였다. 3. 보통답(普通畓), 중점질답(重粘質畓) 공(共)히 담수(湛水)에 따라 용출(溶出)되는 인산농도(燐酸濃度)는 담수후(湛水後) 얼마동안은 시용인산(施用燐酸)과 토양중(土壤中)알루미늄인산(燐酸)에 의해 지배(支配)되고, 그후 환원발달(還元発達)에 따라 토양중(土壤中) vivianite계(系) 인산(燐酸)에 의해 지배(支配)되는 것으로 추정(推定)되었다.

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Morphological Characteristics of the Thalamoperforating Arteries

  • Park, Sukh-Que;Bae, Hack-Gun;Yoon, Seok-Mann;Shim, Jai-Joon;Yun, Il-Gyu;Choi, Soon-Kwan
    • Journal of Korean Neurosurgical Society
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    • 제47권1호
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    • pp.36-41
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    • 2010
  • Objective: The aim of this study was to investigate the morphological characteristics of the thalamoperforating arteries that arise from the P1 segment of the posterior cerebral artery. Methods: Thalamoperforating arteries located in the interpeduncular fossa were dissected in 26 formalin-fixed human cadaver brains. We investigated the origin site of thalamoperforating arteries from the P1 segment, number and diameter. and variations in their origin. Results: Thalamoperforating arteries arose from the superior, posterior or posterosuperior surfaces of the P1 segment at the mean 1.93 mm (range, 0.41-4.71 mm) distance from the basilar apex and entered the brain through the posterior perforated substance. The average number was 3.6 (range 1-8) and mean diameter was 0.70 mm (range 0.24-1.18 mm). Thalamoperforating arteries could be classified into five different types according to their origin at the P1 segment: Type I (bilateral multiple), 38.5%; Type II (unilateral single, unilateral multiple), 26.9%; Type III (bilateral single), 19.2%; Type IV (unilateral single), 11.5%; Type V (unilateral multiple), 3.8%. In 15.4% of all specimens. thalamoperforating arteries arose from the only one side of P1 segment and were not noted in the other side. In such cases, the branches arising from the one side of P1 segment supplied the opposite side. Conclusion: Variations in the origin of the thalamoperforating arteries should be keep in mind to perform the surgical clipping, endovascular treatment or operation involving the interpeduncular fossa. In particular, unilateral single branch seems to be very risky and significant for surgical technique or endovascular treatment.

HIGH REDSHIFT GALAXY CLUSTERS IN ELIAS-N1/N2 FIELDS WITH A NEW COLOR SELECTION TECHNIQUE

  • HYUN, MINHEE;IM, MYUNGSHIN;KIM, JAE-WOO;LEE, SEONG-KOOK
    • 천문학논총
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    • 제30권2호
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    • pp.409-411
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    • 2015
  • Galaxy clusters, the largest gravitationally bound systems, are an important subject of study to place constraints on cosmological models. Moreover, they are excellent places to test galaxy evolution models in connection to their environments. To date, massive clusters have been found unexpectedly (Kang & Im 2009; Gonzales et al. 2012) and the evolution of galaxies in clusters is still controversial (Elbaz et al. 2007; Faloon et al. 2013). Finding galaxy cluster candidates at z > 1 in a wide, deep imaging survey data will enable us to solve such issues of modern extragalactic astronomy. We report new candidate galaxy clusters in one of the wide and deep survey fields, the European Large Area ISO Survey North1 (ELAIS-N1) and North2 (ELAIS-N2) fields, covering a sky area of $8.75deg^2$ and $4.85deg^2$ each. We also suggest a new useful color selection technique to separate z > 1 galaxies from low - z galaxies by combining multi-wavelength data.

레이저로 조사된 이축연신 폴리프로필렌 필름의 열자격 전류특성에 관한 연구 (A study on the properties of TSC in oriented polypropylene film irradiated by laser)

  • 노영배;홍진웅;김재환;이준웅
    • 한국전기전자재료학회:학술대회논문집
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    • 한국전기전자재료학회 1990년도 추계학술대회 논문집
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    • pp.98-101
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    • 1990
  • In order to investigate the laser effects resulted from the behaviors of carriers for BOPP film, experiment of TSC were carried out on the specimen with 15[$\mu\textrm{m}$] thick irradiated by He-Ne laser. The TSC spectras were observed in the temperature range of -100[$^{\circ}C$] to 130[$^{\circ}C$] with the electric field of 20∼60[MV/m], had show four of the distinguished peak such as ${\alpha}$$_1$, ${\alpha}$$_2$, ${\beta}$ and ${\gamma}$, which appeared at 115, 80, 17 and -30[$^{\circ}C$] respectively. Specially, ${\alpha}$$_1$ was observed and anomalous TSC flowing in the same direction as the charging current on the high-electric field such as 50∼60[MV/m]. In according on the consequences obtained from the studies, the origin of ${\alpha}$$_1$peak was attributed to the detrapping process form trap with 2.88[eV] deep of injected space charge from the chathode in the crystaline regions. The origin of ${\alpha}$$_2$ peak was regarded as the detrapping process of ions trapped with 0.9[eV] deep originated from impurity-ion remained in the specimen during production process of the material, in the crystalline regions. The origin of ${\beta}$ peak was concluded to be due to the depolarization process of "C=0"dipole with the activation energy of 0.75[eV] in the amorphous regions. The origin of ${\gamma}$ peak was responsible to the process combined with the depolarization of "CH$_3$", chain segment, with the activation energy of carriers from the shallow trap with 0.4[eV], in he amorphous regions.

Differential Parental Transmission of Markers in BCL3 among Korean Cleft Case-parent Trios

  • Park, Beyoung-Yun;Sull, Jae-Woong;Park, Jung-Yong;Jee, Sun-Ha;Beaty, Terri H.
    • Journal of Preventive Medicine and Public Health
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    • 제42권1호
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    • pp.1-4
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    • 2009
  • Objectives : Isolated cleft lip with or without cleft palate(CL/P) is among the most common human birth defects, with a prevalence of approximately 1 in 700 live births. The B-Cell Leukemia/lymphoma 3(BCL3) gene has been suggested as a candidate gene for CL/P based on association and linkage studies in some populations. This study tests for an association between markers in BCL3 and isolated, non-syndromic CL/P using a case-parent trio design, while considering parent-of-origin effects. Methods : Forty case-parent trios were genotyped for two single nucleotide polymorphisms(SNPs) in the BCL3 gene. We performed a transmission disequilibrium test(TDT) on individual SNPs, and the FAMHAP package was used to estimate haplotype frequencies and to test for excess transmission of multi-SNP haplotypes. Results : The odds ratio for transmission of the minor allele, OR(transmission), was significant for SNP rs8100239(OR=3.50, p=0.004) and rs2965169(OR=2.08, p=0.027) when parent-of-origin was not considered. Parentspecific TDT revealed that SNP rs8100239 showed excess maternal transmission. Analysis of haplotypes of rs2965169 and rs8100239 also suggested excess maternal transmission. Conclusions : BCL3 appears to influence risk of CL/P through a parent-of-origin effect with excess maternal transmission.