• Tuberculosis and Respiratory Diseases
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• 제62권6호
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• pp.549-553
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• 2007

유육종증은 다발성 비건락성 육아종 형성을 특징으로 하는 원인 미상의 전신 질환으로 주로 폐, 피부, 림프절 등의 장기를 침범하며, 신경계 침범은 상대적으로 드문 것으로 알려져 있다. 저자들은 다른 신경학적 증상 없이 단기 기억장애만을 특징으로 하는 신경유육종증이 병발한 폐유육종증 1예를 경험하였기에 문헌고찰과 함께 보고하는 바이다.

• Asian Pacific Journal of Cancer Prevention
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• 제15권8호
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• pp.3525-3531
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• 2014

Objective: Fluorine-18-fluorodeoxyglucose positron emission tomography (18F-FDG-PET) is a new technique for identifying different malignant tumors using different uptake values between tumor cells and normal tissues. Here we assessed the diagnostic accuracy of 18F-FDG-PET in patients with testicular cancer by pooling data of existing trials in a meta-analysis. Methods: PubMed/MEDLINE, Embase and Cochrane Central Trials databases were searched and studies published in English relating to the diagnostic value of FDG-PET for testicular cancer were collected. The summary receiver operating characteristic (SROC) curve was used to examine the FDG-PET accuracy. Results: A total of 16 studies which included 957 examinations in 807 patients (median age, 31.1 years) were analyzed. A meta-analysis was performed to combine the sensitivity and specificity and their 95% confidence intervals (CIs), from diagnostic odds ratio (DOR), positive likelihood ratios (PLR), negative likelihood ratio (NLR). SROC were derived to demonstrate the diagnostic accuracy of FDG-PET for testicular cancer. The pooled sensitivity and specificity were 0.75 (95% confidence interval (CI), 0.70-0.80) and 0.87 (95% CI, 0.84-0.89), respectively. The pooled DOR was 35.6 (95% CI, 12.9-98.3). The area under the curve (AUC) was 0.88. The pooled PLR and pooled NLR were 7.80 (95% CI, 3.73-16.3) and 0.31 (95% CI, 0.23-0.43), respectively. Conclusion: In patients with testicular cancer, 18F-FDG-PET demonstrated a high SROC area, and could be a potentially useful tool if combined with other imaging methods such as MRI and CT. Nevertheless, the literature focusing on the use of 18F-FDG-PET in this setting still remains limited.

• Asian Pacific Journal of Cancer Prevention
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• 제13권5호
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• pp.1887-1893
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• 2012

The aim of this study was to detail characteristics of mammary Paget's disease (PD) representing the whole population in China. A total of 4211 female breast cancer inpatients at seven tertiary hospitals from seven representative geographical regions of China were collected randomly during 1999 to 2008. Data for demography, risk factors, diagnostic imaging test, physical examination and pathologic characters were surveyed and biomarker status was tested by immunohistochemistry. The differences of demography and risk factors between PD with breast cancer and other lesions were compared using Chi-square test or t-test, with attention to physical examination and pathological characters. The percentage of PD was 1.6% (68/4211) in all breast cancers. The mean age at diagnosis was 48.1, and 63.2% (43/68) patients were premenopausal. There is no difference in demography and risk factors between PD with breast cancer and other breast cancer (P > 0.05). The main pattern of PD in physical exam and pathologic pattern were patients presenting with a palpable mass in breast (65/68, 95.6%) and PD with underlying invasive cancer (82.4%, 56/68) respectively. The rate of multifocal disease was 7.4% (5/68). PD with invasive breast cancer showed larger tumor size, more multifocal disease, lower ER and PR expression and higher HER2 overexpression than those in other invasive breast cancer (P < 0.05). These results suggested that PD in China is a concomitant disease of breast cancer, and that PD with underlying invasive cancer has more multiple foci and more aggressive behavior compared with other breast invasive cancer. We address the urgent needs for establishing diagnostic and therapeutic guidelines for mammary PD in China.

• Clinical and Experimental Pediatrics
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• 제53권2호
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• pp.262-266
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• 2010

$TNF-{\alpha}$ 는 소아기 류마티스모양 관절염의 병태생리학에 관여하는 주요 cytokine 이다. Etanercept 는 $TNF-{\alpha}$ 억제제 중 하나로 소아기 류마티스모양 관절염에 효과적인 약물로 각광받고 있다. Etanercept의 주요 부작용은 면역력 저하에 의한 감염으로, 대게 중등도의 상기도 감염이 대부분으로 알려져 있으나, 최근 중증의 감염도 보고되고 있다. 저자들은 소아기 류마티스모양 관절염 환자가 etanercept를 14개월간 투약 후 발생한 뇌염 1예를 경험하였기에 보고하는 바이다.

• 대한의용생체공학회:의공학회지
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• 제39권1호
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• pp.48-54
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• 2018

In this study, We developed a Ancillary device for child radiography for X-ray of children under 5 years old and verified its effectiveness. Chest X-rays of children younger than 5 years of age were performed by Supine method at the position of Table detector, Short - Source to Image Receptor Distance(SID). Existing Supine and Short -SID imaging methods cause many problems, such as errors in image reading and excessive radiation exposure dose to patients, but the use of an Ancillary device for child radiography(ADCR) solves these problems. A total of 160 children were divided into the Upright group using ADCR and Supine group without ADCR. The chest X-ray image was visually evaluated by two radiologists with reference to the European Commission's List of Quality Criteria for Diagnostic Radiographic Images in Pediatrics. The total score of the qualitative evaluation was 5.15% higher in the chest upright method using ADCR than in the chest supine method without ADCR, and the chest upright method score was higher than that of the chest supine method in items 1 to 7. whether infants have deep inspiration or not, 4.87% higher for item 1, whether infants rotate or not and the degree of tilting, 0% higher for the item 2, the reproduction of image from just above apices of lungs to T12/L1, 0% for the item 3, reproduction of the vascular pattern in central 2/3 of the lungs, 6.92% higher for the item 4, reproduction of the trachea and the proximal bronchi, 12.9% higher for the item 5, visually sharp reproduction of the diaphragm and costo-phrenic angles, 10% higher for the item 6, reproduction of the spine and paraspinal structures and visualisation of the retrocardiac lung and the mediastinum, and 3.65% higher for the item 7. Items 2 and 3 showed no statistically significant differences(P > 0.05), and items 1, 4, 5, 6, and 7 showed statistically significant differences(P < 0.05). In conclusion, Upright method using ADCR in pediatric chest X-ray is considered as a good alternative to existing Supine method.

• 대한소아치과학회지
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• 제42권3호
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• pp.218-225
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• 2015

본 연구의 목적은 건전 법랑질과 우식 병소의 형광 차이를 증진시켜 QLF의 영상학적인 진단강도를 높이고, QLF로 촬영한 이미지 상에서 착색과 우식병소를 감별하기 위해 형광 염색제인 플루오레세인나트륨을 접목하여 사람 치아의 법랑질 표면에 유발된 초기 우식병소를 평가하는데 있다. 치아우식증이나 균열이 없는 최근 발거된 소구치 및 제3대구치를 대상으로 하여 치아의 평활면을 $6mm{\times}3mm{\times}3mm$ 크기로 절단한 후 아크릴 주형에 매몰하였고, 시편 표면적의 1/2에 nail varnish를 도포하여 대조군으로 설정하였다. 시편은 무작위로 15개씩 총 6개 탈회그룹(6, 12, 24, 48, 72, 96시간)으로 나누었다. 시편을 각 시간에 맞게 탈회시키고 생리 식염수로 세척한 후 QLF-D를 이용하여 탈회 정도(${\Delta}F$)를 측정하고 0.075% 플루오레세인나트륨을 적용한 후 세척하고 ${\Delta}F$ 값을 측정하여 그 값을 비교하였다. 시편의 중앙 부위를 삭제하고 연마하여 주사전자현미경 상으로 영상을 저장한 후 병소 깊이를 측정하였다. QLF를 이용하여 관찰한 우식병소는 건전 법랑질보다 어둡게, 플루오레세인나트륨을 도포한 후 QLF로 관찰한 우식병소는 건전 법랑질보다 밝게 관찰되었으며 탈회시간이 증가함에 따라 형광염료는 더 많이 침투하였다. 플루오레세인나트륨을 적용한 후 측정한 ${\Delta}F$ 값은 염색 전과 비교하여 모두 증가하였다(p < 0.05). QLF 수치와 병소 깊이는 높은 상관관계를 보였고 회귀분석을 통해 선형 방정식을 추출하였다. 따라서 플루오레세인나트륨을 접목시킨 QLF 측정은 임상적으로 초기우식을 감지하고 분류하는데 기여할 수 있을 것이며, QLF로 촬영한 이미지에서 우식병소와 착색을 감별하는데 도움을 줄 것이다.

• 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.

• Investigative Magnetic Resonance Imaging
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• 제2권1호
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• pp.83-88
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• 1998

목적 : 저자는 생체의 방추형 동맥류를 단순화 시킨 비박동성 방추형 유체 모형을 이용하여 방추형 유체의 자기공명 혈과조영술의 신호강도를 분석하고 컴퓨터를 이용한 유체의 모의 실험과 비교하여 임상적으로 방추형 동맥류의 자기공명 혈관조영술의 신호강도의 해석에 도움이 되는 자료를 얻고자 하였다. 대상 및 방법 : 증류수를 유체로 이용한 비박동성 방추형 동맥류 유체 모형에서 3D TOF MRA를 촬영하여 영상을 얻고 각 영상에서 유체의 평균 신호강도를 측정하였으며, 컴퓨터에서 동일 형태의 방추형 유체를 모의 실험하여 유속의 분포, 방향을 얻어 비교 분석하였다. 결과 : 자기공명 혈관조영술에서 방추형 유체의 유입부와 유출부의 신호강도는 균질한 신호 강도를 보였으나, 팽대부에서는 비균질한 신호강도를 보였으며, 유출부로의 이행부위에서는 중심부 저신호강도, 주변부 고신호강도의 과녁 모야으로 보였다. 방추형 유체의 평균 신호강도는 팽대부에서 서서히 감소하다가 유출부로의 이행 부위에서 급속히 감소하였다가 회복되어 유출부에서는 유입부와 같은 정도의 신호강도를 보였다. 컴퓨터를 이용한 모의실험에서 유입부와 유출부에서는 층류의 소견이었으며, 유입부 이행부위 빛 팽대부에서는 유속의 감소와 주변부로의 방향변화가 있었다. 유출부로의 이행부위에서는 유속이 급속히 회복되었고, 중심부분으로의 방향 변화가 현저하였다. 결론 : 방추형 유체는 자기공명 혈관조영술에서 유출부로의 이행부위에서 신호소실과 과녁모양을 보이며, 이는 급격한 유속증가 및 방향 변화에 따른 위상 전위 때문이다.

• 천문학회지
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• 제36권3호
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• pp.81-87
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• 2003

It is suggested that a flying-by star in a hot accretion disk may cool the hot accretion disk by the Comptonization of the stellar emission. Such a stellar cooling can be observed in the radio frequency regime since synchrotron luminosity depends strongly on the electron temperature of the accretion flow. If a bright star orbiting around the supermassive black hole cools the hot disk, one should expect a quasi-periodic modulation in radio, or even possible an anti-correlation of luminosities in radio and X-rays. Recently, the unprecedentedly accurate infrared imaging of the Sagittarius A$\ast$ for about ten years enables us to resolve stars around it and thus determine orbital parameters of the currently closest star S2. We explore the possibility of using such kind of observation to distinguish two quite different physical models for the central engine of the Sagittarius A$\ast$, that is, a hot accretion disk model and a jet model. We have attempted to estimate the observables using the observed parameters of the star S2. The relative difference in the electron temperature is a few parts of a thousand at the epoch when the star S2 is near at the pericenter. The relative radio luminosity difference with and without the stellar cooling is also small of order $10^{-4}$, particularly even when the star S2 is near at the pericenter. On the basis of our findings we tentatively conclude that even the currently closest pass of the star S2 is insufficiently close enough to meaningfully constrain the nature of the Sagittarius A$\ast$ and distinguish two competing models. This implies that even though Bower et al. (2002)have found no periodic radio flux variations in their data set from 1981 to 1998, which is naturally expected from the presence of a hot disk, a hot disk model cannot be conclusively ruled out. This is simply because the energy bands they have studied are too high to observe the effect of the star S2 even if it indeed interacts with the hot disk. In other words, even if there is a hot accretion disk the star like S2 has imprints in the frequency range at v $\le$ 100 MHz.

• 한국광학회지
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• 제6권3호
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• pp.188-200
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• 1995

파장 13nm의 연 X-선을 사용하여 초고밀도 반도체 칩을 네작할 수 있는 고분해능의 투사 결상용 2-반사경계(배율=1)을 설계하였다. 등배율(1:1)의 광학계는 holosymmetric system으로 구성하였을 때 코마와 왜곡수차가 완전히 제거되는 이점을 갖는다. 2-반사경 holosymmetric system에서 추가적으로 구면수차를 제거하기 위해 두 반사경을 동일한 포물면으로 만들고 두 반사경 사이 거리를 조절하여 비점수차와 Petzval 합이 상쇄되게 함으로써 상면만곡 수차를 보정하였다. 이렇게 구한 aplanat flat-field 포물면 2-반사경 holosymmetric system은 크기가 작고 광축회전대칭의 간단한 구조를 가지면 중앙부 차폐가 아주 작다는 특징을 갖고 있다. 이 반사경계에 대해 잔류 수차, spot diagrams, 회절효과가 고려된 NTF의 분석 등을 통해 연 X-선 리소그라피용 투사 광학계로서의 성능이 조사된 결과, $0.25\mum$및. $0.18\mum$의 해상도가 얻어지는 상의 최대 크기가 각각 4.0mm, 2.5mm로 구해졌고 초점심도는 각각 $2.5.\mu$m, $2.4.\mum$로 얻어졌다. 그러므로 이 반사경계는 256Mega DRAM 및 1Giga DRAM의 반도체 칩 제작의 연구에 응용될 수 있다.