• 천문학회보
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• 제40권2호
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• pp.41.1-41.1
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• 2015

허블우주망원경에 장착된 ACS/WFC로 획득한 Anderson 등과 Sarajedini 등의 깊고 균질한 VI 측광 목록을 이용하여 우리은하 구상성단 M13(NGC 6205)과 M22(NGC 6656)의 뜨겁고 밝은 백색왜성 탐사를 수행하였다. 허블우주망원경 VI 측광 목록으로부터 M13과 M22의 V 대 V-I 색-등급도를 작성하였고 여기에서 많은 항성으로 잘못 검출된 대상(spurious detection)을 측광 질매개변수 qfit(V)와 qfit(I)에 따라서 제거하였다. 그리고 M13의 경우에는 중심의 높은 밀집도에 기인한 높은 측광오차를 가진 중심영역 별을 제거하기 위하여 성단 중심으로부터의 추가적인 반경 제한을 실시하였다. 이렇게 도출한 M13과 M22의 각각의 V 대 V-I 색-등급도에서 십여개 정도의 백색왜성 후보를 동정하였다. 이들은 동반되어 제공되는 ACS/WFC 각각의 영상에서 항성체로 동정되었으며, M13과 M22의 성단 중심부 영역에 임의적으로 분포하고 있으며, 색-등급도상의 위치가 DA 백색왜성 냉각계열의 밝은 부분에 위치하고 있어서 이들이 M13과 M22의 진짜 백색왜성임을 나타내고 있다. 이들에 대해 추가적으로 분광학적인 관측 연구를 수행한다면 이들의 백색왜성 진위 여부와 다양한 물리량을 밝혀낼 것이다. 또한 가까운 구상성단에 대해서 같은 방법으로 조사를 수행하면 더 많은 구상성단에서 갓 태어난 뜨겁고 밝은 백색왜성을 찾아낼 것으로 기대한다.

• Current Optics and Photonics
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• 제1권1호
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• pp.12-16
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• 2017

Color sensor systems based on M13 bacteriophage are being considerably researched. Although many studies on M13 bacteriophage-based chemical sensing of TNT, endocrine disrupting chemicals, and antibiotics have been undertaken, the fundamental physical and chemical properties of M13 bacteriophage-based nanostructures require further research. A simple M13 bacteriophage-based colorimetric sensor was fabricated by a simple pulling technique, and M13 bacteriophage was genetically engineered using a phage display technique to exhibit a negatively charged surface. Arrays of structurally and genetically modified M13 bacteriophage that can determine the polarity indexes of various alcohols were found. In this research, an M13 bacteriophage-based color sensor was used to detect various types of alcohols, including methanol, ethanol, and methanol/butanol mixtures, in order to investigate the polarity-related property of the sensor. Studies of the fundamental chemical sensing properties of M13 bacteriophage-based nanostructures should result in wider applications of M13 bacteriophage-based colorimetric sensors.

• Nuclear Medicine and Molecular Imaging
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• 제42권5호
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• pp.354-361
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• 2008

목적: 암모니아의 심근섭취는 심근의 관류나 생존능 및 대사에 관계되어 있으며, N-13 암모니아 PET은 심근의 허혈을 진단하는 데에 유용한 것으로 알려져 있다. 그러나, 아데노신을 이용한 약물부하 심근관류 검사로 N-13 암모니아 PET/CT와 Tc-99m 세스타미비 SPECT 검사를 비교한 연구는 없었다. 이 연구에서는 관상동맥질환이 의심되는 환자에게서 아데노신 약물부하로 N-13 암모니아 PET/CT와 Tc-99m 세스타미비 SPECT를 시행하여 두 검사의 차이를 비교분석하여 N-13 암모니아 PET/CT의 임상 유용성을 알아보았다. 대상 및 방법: 관상동맥질환이 의심되는 환자 중 Tc-99m 세스타미비 SPECT와 N-13 암모니아 PET/CT를 동시에 시행할 수 있었고, 검사 1주일 이내 관상동맥조영술을 시행하였던 17명의 환자(남자:13명, 평균연령 $63{\pm}11$세)를 대상으로 하였다. 아데노신약물 부하 후 N-13 암모니아 PET/CT와 Tc-99m 세스타미비를 검사하여 육안 분석과 정량분석을 실시하였다. 결과: 관상동맥조영술에서 50% 이상의 협착이 확인된 관상동맥의 진단에 대한 민감도와 특이도는 N-13 암모니아 PET/CT는 91%와 89%로, Tc-99m세스타미비 SPECT는 65%와 82%로 각각 나타났다. 또한 N-13 암모니아 PET/CT와 Tc-99m 세스타미비 SPECT는 전체에 238분절 중 65%인 154분절에서 동일한 결과를 보였으며, N-13 암모니아 PET/CT는 Tc-99m 세스타미비 SPECT에서 비가역적인 관류결손을 보였던 병변 중 54%에 대하여 가역적인 관류결손을 나타내었다. 협착혈관이 관장하는 심근부위에 해당하는 110개의 분절에 대하여 부하기와 휴식기의 계수를 N-13 암모니아 PET/CT와 Tc-99m세스타미비 SPECT에서 각각 비교하였을 때, 부하기의 비교에서는, 두 검사간에 유의한 차이를 보이지 않았으나, 휴식기에서는 N-13 암모니아 PET/CT의 계수가 Tc-99m세스타미비 SPECT의 계수보다 높았으며 (p<0.01), 휴식기와 부하기의 계수의 차이도 N-13 암모니아 PET/CT가 Tc-99m 세스타미비 SPECT보다 큰 것으로 나타났다(p<0.01). 결론: N-13 암모니아 PET/CT는 Tc-99m 세스타미비 SPECT보다 관상동맥질환의 진단이 정확하고, 가역적인 관류결손을 보인 분절의 수가 많으며, 휴식-부하 관류차이도 현저하여, 관상동맥질환의 정확한 진단과 함께 심근의 허혈이나 생존능을 더욱 잘 반영하는 것으로 사료된다.

• Genomics & Informatics
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• 제7권3호
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• pp.152-158
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• 2009

Although the genetic basis for bone mineral density (BMD) has been studied by many groups so far, genes responsible for this complex trait has not been completely revealed. In order to localize quantitative trait loci (QTLs) for BMD variation in Asian population, the study was designed using a group of Mongolian population, a genetically closed population with a homogeneous lifestyle. BMD was measured at the left and right wrists and ankles using DEXA in 1,082 participants from 142 families. Genotyping of 13 polymorphic microsatellite markers on chromosome 13 (average spacing 8-9 cM) and two-point and multipoint linkage analysis were performed. In two-point linkage analysis, we identified two markers, D13S175 (6.03 cM) and D13S265 (68.73 cM) that had LOD scores greater than 1 for left ankle (LOD=2.09, LOD=1.49, respectively). We also found a marker D13S175 (6.03 cM) with a high LOD for left wrist (LOD=1.49) and the markers D13S265 (68.73 cM) and D13S217 (17.21 cM) for the right wrist (LOD= 1.82, LOD= 1.62, respectively). Among these significant marker regions, only two regions at 17 cM (13p11) and 65 cM (13q21) for the right wrist overlapped with major QTLs reported in following multipoint linkage analysis (LOD= 1.7549, LOD=1.4462, respectively). This study provides the possible evidence of the presence of QTLs affecting right wrist BMD in Mongolian populations on 13p11 and 13q21. Modest evidence was also found for genes affecting left ankle and left wrist BMD on 13p13.

• 천문학논총
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• 제13권1호
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• pp.111-122
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• 1998

Among the sample of red giant stars in the globular clusters M3 and M13 whose CN bands $(3883{\AA})$ have been measured by various authors, the stars on the red giant evolutionary state are selected to have their CN band distributions. It is found that all stars brighter than Mv = 0, are CN-strong in M3, while all stars except IV-29 are CN-strong in M13. It hints that the onset of meridional mixing is related with the RGB bumps of the clusters.

• IMMUNE NETWORK
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• 제2권4호
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• pp.202-207
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• 2002

Background: Kawasaki disease is an acute febrile illness with systemic vasculitis which primarily affects children, We examined the production of leptin in plasma and gene expressions of CXC chemokines in peripheral blood mononuclear cells from patients with Kawasaki disease. Methods: Consecutive 39 samples from 13 patients according to the different clinical stages (acute, subacute, convalescent) of Kawasaki disease were collected. The plasma leptin levels according to clinical stages of Kawasaki disease were examined by ELISA and the expression of IP-10, Mig and IL-8 mRNAs in 39 samples (13 samples of each stage) from 13 cases were examined by RT-PCR. Results: There were not significant changes of plasma leptin levels according to the clinical stages of Kawasaki disease. The mean values of plasma leptin concentrations during each of the stages (n=13, p>0.05, pg/ml) were $335.8{\pm}549.0$ in acute, $358{\pm}347.6$ in subacute, and $443.6{\pm}645.9$ in convalescent stage. The mRNAs of IP-10, Mig, and IL-8 were expressed in 13/13 (100%), 2/13 (15%), 9/13 (69%) during acute stage, 13/13 (100%), 6/13 (46%), 13/13 (100%) during subacute stage, and 13/13 (100%), 4/13 (31%), 10/13 (77%) during the convalescent stage, respectively. In three patients, the production of leptin and expression of IP-10 mRNA were dramatically decreased according to the process of the clinical stages. In five patients with prominent cervical lymphadenopathy, the expression of IL-8 mRNA during the subacute stage was more elevated than the acute and convalescent stages. Conclusion: This data suggests that the production of leptin and the gene expressions of IP-10, Mig and IL-8 seem to have no significant correlation to the clinical stages of Kawasaki disease. However, expression patterns of IP-10, Mig and IL-8 mRNA may be related to the specific clinical manifestations, and the expression of IP-10 may also be correlated to leptin levels with pericardial involvement.

• 천문학논총
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• 제30권2호
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• pp.265-266
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• 2015

A search for luminous white dwarfs (WDs) in several nearby Galactic globular clusters (GCs) was carried out using the deep and homogeneous photometric catalog of Galactic GCs taken with the ACS/WFC aboard the Hubble Space Telescope (HST) by Sarajedini et al. and Anderson et al- It resulted in the identification of luminous WD candidates in the GCs M13 (NGC 6205) and M22 (NGC 6656). The purpose of the present study is to identify luminous WDs in the deep and homogeneous V versus V - I color-magnitude diagrams (CMDs) of several nearby Galactic GCs taken with the ACS/WFC aboard the HST. Using photometric data for the GCs M13 and M22 that are now in the public domain, the V versus V - I CMDs of the GCs M13 and M22 were constructed. Many spurious detections in the CMDs were removed using the photometric quality parameters qfit(V) and qfit(I), and a radial restriction was applied to the CMDs to remove the central stars with higher photometric errors due to central crowding. From each resultant V versus V - I CMD of the GCs M13 and M22, a dozen or so luminous WD candidates were identified. They were confirmed as stellar objects in the accompanying ACS/WFC images and their positions in the CMDs were in the bright part of the DA WD cooling curve. Therefore, the luminous WD candidates in the GCs M13 and M22 seem to be true luminous WDs, and spectroscopic observations are needed to confirm their true identity.

• 미생물학회지
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• 제26권3호
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• pp.162-166
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• 1988

Bacteriophage M13 DNAs carrying the wild type or base substituted SV40 DNA replication origins were used for replication assay. In vivo and in vitro assay with African green monkey cell line COS-1 showed that the replication of M13-SV40 recombinant DNAs was restricted like a pBR322 SV40 recombinant DNA(Lusky and Botchan, 1981). Furthermore, recombinant phage DNAs isolated from the transfected siminan cells subsequently show a reduced ability to retransform E. coli. But pATSV-W(Kim et al., 1988) was replicated in COS-1 cells normally. We think that a poison sequence may exist on bacteriophage M13 DNA like pBR322.

• Journal of Plant Biology
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• 제24권4호
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• pp.171-179
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• 1981

옥수수 뿌리로부터 분리한 13,000g pellet과 13,000~80,000g pellet 내에 있는 membrane-bound ATPases의 특성을 구명하였다. 13,000g pellet과 13,000~80,000g pellet의 membrane-bound ATPases의 최적 pH는 5와 9였다. Discontinuous sucrose gradient centrifugation에 의한 13,000g pellet의 분획중 Fraction C는 pH 5에서, Fraction D, E 및 F는 pH 5에서보다 pH 9에서 더높은 활성을 나타냈다. 13,000~80,000g pellet의 분획에서 보면, Fraction A, C는 pH 9보다 pH 5에서, Fraction B, D, E 및 F는 pH 5보다 pH 9에서 더 높은 활성을 가겠다. pH 5와 pH 9에서 membrane-bound ATPases의 기질포화 농도는 3~5 mM이며 ATP에 대한 Km 값은 모두 0.25 mM이였다. Vmax 값은 8.0~55.6 $\mu$M Pi/mg membrane protein/hr의 범위에 있었다. Membrane-bound ATPase의 활성은 $K^+$ 이온에 의해 증가되었다.

• 천문학회지
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• 제48권6호
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• pp.333-341
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• 2015

A search for hot and bright white dwarfs (WDs) in the Milky Way globular clusters M13 (NGC 6205) and M22 (NGC 6656) is carried out using the deep and homogeneous V I photometric catalog of Anderson et al. and and Sarajedini et al., based on data taken with the ACS/WFC aboard the Hubble Space Telescope (HST). V versus V − I color-magnitude diagrams (CMDs) of M13 and M22 are constructed and numerous spurious detections are rejected according to their photometric quality parameters qfit(V ) and qfit(I). In the case of M13, further radial restriction is applied to reject central stars with higher photometric errors due to central crowding. From each resultant V versus V −I CMD, sixteen and thirteen WD candidates are identified in M13 and M22, respectively. They are identified as stellar objects in the accompanying ACS/WFC images and are found to be randomly distributed across the central regions of M13 and M22. Their positions in the CMDs are in the bright part of the DA WD cooling sequences indicating that they are true WDs. In order to confirm their nature, follow-up spectroscopic observations are needed.