• 천문학회지
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• 제37권5호
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• pp.361-369
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• 2004

Galaxy clusters as the densest and most prominent regions within the large-scale structure can be used as well characterizable laboratories to study astrophysical processes on the largest scales. X-ray observations provide currently the best way to determine the physical properties of galaxy clusters and the environmental parameters that describe them as laboratories. We illustrate this use of galaxy clusters and the precision of our understanding of them as laboratory environments with several examples. Their application to determine the matter composition of the Universe shows good agreement with results from other methods and is therefore a good test of our understanding. We test the reliability of mass measurements and illustrate the use of X-ray diagnostics to study the dynamical state of clusters. We discuss further studies on turbulence in the cluster ICM, the interaction of central AGN with the radiatively cooling plasma in cluster cooling cores and the lessons learned from the ICM enrichment by heavy elements.

• 천문학회보
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• 제44권1호
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• pp.74.1-74.1
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• 2019

We present an ongoing imaging survey of the host galaxies of hard X-ray-selected active galactic nuclei (AGNs) observed with the Hubble Space Telescope (HST). The snapshot images are taken with the Advanced Camera for Surveys through an HST gap-filler program. The sample, selected from the 70-month Swift-BAT X-ray source catalog, represents an unbiased and uniform AGN population, which will enable us to test the AGN unification model and explore the physical connection between host galaxies and central supermassive black holes. We also plan to investigate the AGN triggering mechanism by examining merger signatures and searching for dual nuclei. We present the pipeline for imaging analysis and the current status of the survey.

• 천문학논총
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• 제30권2호
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• pp.605-607
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• 2015

The development of time-frequency analysis techniques allow astronomers to successfully deal with the non-stationary time series that originate from unstable physical mechanisms. We applied a recently developed time-frequency analysis method, the Hilbert-Huang transform (HHT), to two non-stationary phenomena: the superorbital modulation in the high-mass X-ray binary SMC X-1 and the quasi-periodic oscillation (QPO) of the AGN RE J1034+396. From the analysis of SMC X-1, we obtained a Hilbert spectrum that shows more detailed information in both the time and frequency domains. Then, a phase-resolved analysis of both the spectra and the orbital profiles was presented. From the spectral analysis, we noticed that the iron line production is dominated by different regions of this binary system in different superorbital phases. Furthermore, a pre-eclipse dip lying at orbital phase ~0:6-0:85 was discovered during the superorbital transition state. We further applied the HHT to analyze the QPO of RE J1034+396. From the Hilbert spectrum and the O-C analysis results, we suggest that it is better to divide the evolution of the QPO into three epochs according to their different periodicities. The correlations between the QPO periods and corresponding fluxes were also different in these three epochs. The change in periodicity and the relationships could be interpreted as the change in oscillation mode based on the diskoseismology model.

• 천문학회보
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• 제36권2호
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• pp.147.2-147.2
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• 2011

We have initiated a long-term identification campaign of supernova remnant candidates in X-ray regime. In the short-listed unidentified sources from the ROSAT All Sky Survey, we have chosen the brightest candidate, G308.3-1.4, as our pilot target for a dedicated investigation with Chandra X-ray Observatory. Our observation has revealed an incomplete shell-like X-ray structure which well-correlated with the radio feature. Together with the spectral properties of a shocked heated plasma, we confirm that G308.3-1.4 is indeed a supernova remnant. A bright X-ray point source which locates close to the remnant center is also uncovered in this observation. Its spectral behavior conform with those observed in a rare class of neutron stars. The properties of its optical/infrared counterpart suggests the evidence for a late-type companion star. Interestingly, possible excesses in B-band and H-alpha have been found which indicate this can be an accretion-powered system. With the further support from the putative periodicity of ~1.4 hrs, this source can possibly provide the direct evidence of a binary system survived in a supernova explosion for the first time.

• Journal of Biosystems Engineering
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• 제27권4호
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• pp.341-348
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• 2002

Quality evaluation of red ginsengs is determined by outer shape and inner qualities. Especially, the inner qualities are main grading criteria. Currently, red ginsengs are classified into 3-grades; heaven, earth and good. The best heaven grade must not include inner holes and sponge tissues. This study was conducted to develop a red ginseng sorting system using x-ray image processing technique. Because of lens characteristic, gray values of the central region in the x-ray image are higher and gradually decreased towards the edge regions. This difference of gray values gives trouble in segmentation and detection of inner holes in red ginseng image, so preprocessing technique is necessary. The preprocessing was done by subtracting source image from an empty background image. But, simple subtraction was not quite appropriate because of too small contrast between inner holes and sound part. Scaled subtraction images were obtained by multiplying all gray values by some numbers. However this method could not help to set threshold value because the gray values of root part are generally lower than body part when red ginseng is exposed to the x-ray. To determine threshold value for detecting inner holes, an algorithm was developed by increasing overall gray values of less clear images.

• 한국광물학회지
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• 제23권4호
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• pp.305-313
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• 2010

콩고민주공화국의 중앙아프리카 구리광화대에서 수입하는 Cu-Co 광석의 광물학적 특성을 X-선 회절 분석, 2차원 X-선 회절 분석과 전자현미분석에 의하여 연구하였다. 검은색 광석은 코발트 광석광물인 헤테로제나이트와 구리 광석광물인 공작석, 초록색 광석은 공작석으로 주로 구성된다. 헤테로제나이트는 반사 현미경 하에서 매우 밝은 흰색을 나타내며 X-선 회절 분석에서는 $4.39{\AA}$과 $2.316{\AA}$ 피크를 가지는 3R 다형으로 확인된다. 그러나 전형적인 3R형에 비하여 낮은 NiO와 $Fe_20_3$의 함량으로 미루어 보아, 3R 다형 이외에 2H 다형도 일부 존재하는 것으로 판단된다. 공작석은 반사 현미경하에서 밝은 회색을 나타내며, 화학식은 $Cu_{1.97}Co_{0.02}Fe^{2+}{_{0.01}}CO_3(OH)_2$이다. 헤테로제나이트와 공작석은 중앙아프리카 구리광화대의 광화작용 중 최후기인 표성부화기에 형성되었으며, 코발트는 일차 광석보다는 표성작용에 의하여 형성된 (산)수산화 광석에 더 많이 부화되었을 것으로 추정된다.

• 천문학회지
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• 제37권5호
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• pp.381-385
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• 2004

Similarly to other cluster of galaxies previously classified as cooling flow systems, the Chandra observation of MKW 3s reveals that this object has a complex X-ray structure hosting both a X-ray cavity and a X-ray filament. Unlike the other clusters, however, the temperature map of the core of MKW 3s shows the presence of extended regions of gas heated above the radially averaged gas temperature at any radius. As the cluster does not show evidences for ongoing major mergers Mazzotta et al. suggest a connection between the heated gas and the activity of the central AGN. Nevertheless, due to the lack of high quality radio maps, this interpretation was controversial. In this paper we present the results of two new radio observations of MKW 3s at 1.28 GHz and 604 MHz obtained at the GMRT. Together with the Chandra observation and a separate VLA observation at 327 MHz from Young, we show unequivocal evidences for a close connection between the heated gas region and the AGN activity and we briefly summarize possible implications.

• 대한방사선기술학회지:방사선기술과학
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• 제16권1호
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• pp.101-106
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• 1993

In order to assure safety of both patient and operator, and to provide uniform quality radiographs, it is necessary to perform periodic calibration of diagnostic X-ray equipment. A basic parameter of diagnostic equipment's and its image sharpness is the size(and shape the energy distribution) of the focal spot as viewed along the central X-ray beam. This size determines the resolution possible with the equipment and also determines the heat characteristics of an anode. A fine focus tube gives high resolution but causes high local heating of target. In past, the pin-hole and star pattern image measurement for evaluation of resolution have been widely used, but it produced blurring and inaccuracy of image. So newly inverted Ug-meter has advantage in more convenient measurement method and less out-put bias than other image measurement. The authors intended to compare measured focal size between Ug-meter and focal spot test tool, changed state from setting to now of units.

• Journal of Radiation Protection and Research
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• 제12권1호
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• pp.1-11
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• 1987

X-선 target 으로 부터 water phantom($30{\times}30{\times}30cm^3$) 표면까지 1m이고 이 지점에서 비임 크기가 $5cm{\phi},\;10cm{\phi},\;15cm{\phi}$인 경우 phantom 표면으로 부터 X-선 중심축을 따라 깊이 2.5cm의 기준점으로 부터깊이 20cm까지 2.5cm 간격으로 깊이-선량 백분율, P(%)을 추정하였다. 사용된 X-선 인가전압 및 전류는 $150{\sim}250kV$ 및 5 mA 이었고 물속 흡수선량률, $\dot{D}_w$은 NE 2571 공동전리함의 조사선량 교정인자 $N_x$로부터 구한 공기 kerma 고정인자 $N_k$를 이용하여 결정하였다. 기준조사선량룰 $\dot{X}_c$은 Exradin A-2공동 전리함을 일본 ETL로부터 교정하여 X-선 선질을 ETL 교정선질과 같도록 반가층을 결정한 후에 측정되었다. 한편, 흡수선량 및 깊이-선량 백분율 측정의 정확도를 검증하기 위해 phantom 속 깊이 5 cm되는 교정점에서 물속흡수선량률, $\dot{D}_w$을 $N_k$로부터 산출한 값과 Burlin의 일반화된 공동이론을 이용하여 계산한 값을 비교해 보았으며, $N_k$로부터 결정된 깊이-선량 백분율 P(%)을 BJR Suppl. 로부터 구한 값과 비교해 본 결과는 좋은 일치를 보였다.

• Imaging Science in Dentistry
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• 제44권2호
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• pp.161-164
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• 2014

Mucoepidermoid carcinomas (MECs) arising within the jaws as primary central bony lesions are termed central MECs. Central MECs are extremely rare, comprising 2-3% of all mucoepidermoid carcinomas. We herein report a rare case of central MEC of the maxilla in a 52-year-old male whose plain radiographs showed a "ground glass" pattern and computed tomographic images, a hypodense mass with numerous calcifications. To the best of our knowledge, this is the first report of central MEC showing a "ground glass" appearance.