• Journal of Astronomy and Space Sciences
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• 제33권2호
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• pp.109-117
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• 2016

We explain the results of Yu et al. (2015b) of the novel sharpness angle measurement to a large number of spectra obtained from the Fermi gamma-ray burst monitor. The sharpness angle is compared to the values obtained from various representative emission models: blackbody, single-electron synchrotron, synchrotron emission from a Maxwellian or power-law electron distribution. It is found that more than 91% of the high temporally and spectrally resolved spectra are inconsistent with any kind of optically thin synchrotron emission model alone. It is also found that the limiting case, a single temperature Maxwellian synchrotron function, can only contribute up to 58⁺²³₋₁₈% of the peak flux. These results show that even the sharpest but non-realistic case, the single-electron synchrotron function, cannot explain a large fraction of the observed spectra. Since any combination of physically possible synchrotron spectra added together will always further broaden the spectrum, emission mechanisms other than optically thin synchrotron radiation are likely required in a full explanation of the spectral peaks or breaks of the GRB prompt emission phase.

• 천문학회지
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• 제47권1호
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• pp.15-39
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• 2014

Polarization is a basic property of light and is fundamentally linked to the internal geometry of a source of radiation. Polarimetry complements photometric, spectroscopic, and imaging analyses of sources of radiation and has made possible multiple astrophysical discoveries. In this article I review (i) the physical basics of polarization: electromagnetic waves, photons, and parameterizations; (ii) astrophysical sources of polarization: scattering, synchrotron radiation, active media, and the Zeeman, Goldreich-Kylafis, and Hanle effects, as well as interactions between polarization and matter (like birefringence, Faraday rotation, or the Chandrasekhar-Fermi effect); (iii) observational methodology: on-sky geometry, influence of atmosphere and instrumental polarization, polarization statistics, and observational techniques for radio, optical, and $X/{\gamma}$ wavelengths; and (iv) science cases for astronomical polarimetry: solar and stellar physics, planetary system bodies, interstellar matter, astrobiology, astronomical masers, pulsars, galactic magnetic fields, gamma-ray bursts, active galactic nuclei, and cosmic microwave background radiation.

• Journal of Radiation Protection and Research
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• 제36권4호
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• pp.190-194
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• 2011

After the first report that electrons with sub-ionization energy of DNA could cause single strand breaks or double strand breaks to DNA, there have been various studies to investigate the mechanisms of DNA damage by low-energy electrons. In this paper, we examined the possibility of using X-ray photoelectron spectroscopy (XPS) to analyze the dissociation patterns of the molecular bonds by electron irradiation on DNA thin films and tried to establish the method as a general tool for studying the radiation damage of biomolecules by low energ yelectrons. For the experiment, pBR322 plasmid DNA solution was formed into the films on tantalum plates by lyophilization and was irradiated by 5-eV electrons. Un-irradiated and irradiated DNA films were compared and analyzed using the XPS technique.

• 천문학회지
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• 제45권6호
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• pp.147-156
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• 2012

We present a test of the emission statistics of active galactic nuclei (AGN), probing the connection between the red-noise temporal power spectra and multi-modal flux distributions known from observations. We simulate AGN lightcurves under the assumption of uniform stochastic emission processes for different power-law indices of their respective power spectra. For sufficiently shallow slopes (power-law indices (${\beta}{\leq}1$), the flux distributions (histograms) of the resulting lightcurves are approximately Gaussian. For indices corresponding to steeper slopes (${\beta}{\geq}1$), the flux distributions become multi-modal. This finding disagrees systematically with results of recent mm/radio observations. Accordingly, we conclude that the emission from AGN does not necessarily originate from uniform stochastic processes even if their power spectra suggest otherwise. Possible mechanisms include transitions between different activity states and/or the presence of multiple, spatially disconnected, emission regions.

• Asian Pacific Journal of Cancer Prevention
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• 제15권16호
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• pp.6649-6655
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• 2014

Radiation therapy is an important treatment for head and neck squamous cell carcinoma (HNSCC). However, how to promote radiation sensitivity in HNSCC remains a challenge. This study aimed to investigate the radiosensitizing effects of fenofibrate on HNSCC and explore the underlying mechanisms. HNSCC cell lines CNE-2 and KB were subjected to ionizing radiation (IR), in the presence or absence of fenofibrate treatment. Cell growth and survival, apoptosis and cell cycle were evaluated. In addition, CNE-2 cells were xenografted into nude mice and subjected to IR and/or fenofibrate treatment. The expression of cyclinB and CDK1 was detected by Western blotting. Our results showed that fenofibrate efficiently radiosensitized HNSCC cells and xenografts in mice, and induced apoptosis and G2/M arrest via reducing the activity of the CDK1/cyclinB1 kinase complex. These data suggest that fenofibrate could be a promising radiosensitizer for HNSCC radiotherapy.

• 한국환경농학회지
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• 제17권1호
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• pp.76-83
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• 1998

Hormesis법칙의 주핵심은 유해작용을 가진 물질이 유해량 이하에서는 다량의 동일 작용물질이 보여주는 장해영향과는 정반대의 영향을 보여주는 것이다. 미량의 유해물질 투여는 생체에 미세 변화를 일으키고, 조절기능은 생체를 통상상태에서 예민상태와 회복태세로 바꾼다. 자극 받은 생체는 이전과는 다르게 환경 변화에 민감하게 반응하며, 통상기능은 지연되고 회복과 방어와 같은 기능에 에너지와 자원을 우선 이용하게 한다. 예민상태하의 생체는 영양분을 효과적으로 이용하고 성장을 빠르게 하며 방어 반응을 향상시키고 성숙도 빠르게하여 보다 효율적으로 번식시키며 질병이 감소되고 오래 살게된다. 저선량 전리 방사선 조사효과는 hormesis 일반 개념과 일치하였는데 방사선 종류에 상관없이 저선량으로 조사된 생물은 자극효과를 보여주었다. 식물에서는 발아, 출아, 생장, 발육, 개화, 결실촉진과 수량증대와 질병저항력 증가 및 저선량 조사 이후의 고선량 방사선에 대한 저항력 증가 등이 나타났다. 방사선 hormesis 작용은 대상식물, 종자상태, 환경 및 재배조건, 측정하는 생리적 기능, 선량율과 선량에 따라 다르고, 조절되지 않은 많은 변수 때문에 일관된 재현성이 적으나, 일반적 용선량은 환경방사선량의 약 100배($10{\sim}1,000$), 또는 확실한 유해작용이 있는 선량의 100($10{\sim}1,000$)분의 1정도로 생각되나 실험조건에 따라 변경될 것이다. 방사선 hormesis의 생화학적 작용기작은 아직 미확인 상태이나 회복기능의 과잉보상이 주요 작용기작의 하나로 제시되고 있다.

• 천문학회지
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• 제52권5호
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• pp.173-180
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• 2019

We present IR flux density measurements, models of the broadband SED, and results of SED modeling for the Pulsar Wind Nebula (PWN) 3C 58. We find that the Herschel flux density seems to be slightly lower than suggested by interpolation of previous measurements in nearby wavebands, implying that there may be multiple electron populations in 3C 58. We model the SED using a simple stationary one-zone and a more realistic time-evolving multi-zone scenario. The latter includes variations of flow properties in the PWN (injected energy, magnetic field, and bulk speed), radiative energy losses, adiabatic expansion, and diffusion, similar to previous PWN models. From the modeling, we find that a PWN age of 2900-5400 yrs is preferred and that there may be excess emission at ${\sim}10^{11}Hz$. The latter may imply multiple populations of electrons in the PWN.

• 한국식품영양과학회지
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• 제41권7호
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• pp.901-906
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• 2012

본 연구에서는 넓패 메탄올 추출물의 농도별 처리가 인체 자궁암 세포 HeLa의 세포사멸에 미치는 영향을 확인하기 위하여 세포독성 측정, Hoechst 33258 staining, flow cytometry 분석을 통하여 세포사멸을 확인하였다. 넓패 메탄올 추출물 처리 시 HeLa 세포에서 농도 의존적으로 세포의 증식을 억제하였으며, 또한 넓패 메탄올 추출물은 농도 의존적으로 핵을 응축하고 apoptotic bodies을 생성하였다. 유세포 분석을 통하여 apoptosis를 측정한 결과, 넓패 메탄올 추출물의 농도가 증가함에 따라 유의적으로 apoptotic 세포가 증가하였다. Western blot을 통해 PARP 단백질의 절단 현상을 분석한 결과, 넓패 메탄올 추출물의 처리 농도와 시간에 따라 PARP 단백질의 절단 현상이 증가하였다. 또한 넓패 메탄올 추출물은 caspase-8, caspase-9 및 caspase-3 활성을 농도와 시간에 따라 증가시켰으며, caspase 저해제인 z-VAD-fmk로 처리 시 넓패 메탄올 추출물에 의한 세포사멸이 유의적으로 감소되어 넓패 메탄올 추출물에 의한 HeLa 세포의 apoptosis 유도에 caspase가 중요한 역할을 하고 있음을 확인하였다. 따라서 넓패 메탄올 추출물은 HeLa 자궁암 세포의 apoptosis를 유도하는 것으로 나타나 넓패의 항암효과 가능성을 제시하였다.

• Asian Pacific Journal of Cancer Prevention
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• 제14권11호
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• pp.6197-6208
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• 2013

Cancers will continue to be a threat to health unless they can be controlled by combinations of treatment modalities. In this review, evaluate the role of resveratrol (RSV) as a radiosensitizing agent was evaluated and underlying mechanisms holistically explored in different cancer models focusing on therapeutic possibilities. The ability of RSV to modify the effect of radiation exposure in normal and cancer cells has indeed been shown quite convincingly, the combination of RSV and IR exhibiting synergistic effects on different cancer cells. This is relevant since controlled exposure to IR is one of the most frequently applied treatments in cancer patients. However, radiotherapy (XRT) treatment regimes are very often not effective in clinical practice as observed in patients with glioma, prostate cancer (PCa), melanoma, for example, largely due to tumour radioresistant properties. Sensitization of IR-induced apoptosis by natural products such as RSV is likely to be relevant in cancer control and treatment. However, all cancers do not respond to RSV+IR in a similar manner. Therefore, for those such as the radioresistant PCa or melanoma cells, the RSV+IR regime has to be very carefully chosen in order to achieve effective and desirable outcomes with minimum toxicity to normal cells. They are reports that the highest concentration of 100 ${\mu}M$ RSV and highest dose of 5 Gy IR are sufficient to kill cells by induction of apoptosis, indicating that RSV is effective in radiosensitizing otherwise radioresistant cells. In general, it has been shown in different cancer cells that RSV+XRT effectively act by enhancing expression of anti-proliferative and pro-apoptotic molecules, and inhibiting pro-proliferative and anti-apoptotic molecules, leading to induction of apoptosis through various pathways, and cell death. If RSV+XRT can suppress the signature of cancer stemness, enhance the radiosensitivity by either targeting the mitochondrial functionality or modulating the tumour necrosis factor-mediated or Fas-FasL-mediated pathways of apoptosis in different cancers, particularly in vivo, its therapeutic use in the control of cancers holds promise in the near future.

• 천문학회지
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• 제51권4호
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• pp.111-117
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• 2018

A numerical method is proposed to calculate the response of detectors measuring particle energies from incident isotropic fluxes of electrons and positive ions. The isotropic flux is generated by injecting particles moving radially inward on a hypothetical, spherical surface encompassing the detectors. A geometric projection of the field-of-view from the detectors onto the spherical surface allows for the identification of initial positions and momenta corresponding to the clear field-of-view of the detectors. The contamination of detector responses by particles penetrating through, or scattering off, the structure is also similarly identified by tracing the initial positions and momenta of the detected particles. The relative contribution from the contaminating particles is calculated using GEANT4 to obtain the geometric factor of the instrument as a function of the energy. This calculation clearly shows that the geometric factor is a strong function of incident particle energies. The current investigation provides a simple and decisive method to analyze the instrument geometric factor, which is a complicated function of contributions from the anticipated field-of-view particles, together with penetrating or scattered particles.