• 천문학회보
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• 제35권2호
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• pp.78.2-78.2
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• 2010

We report the detection of a low-amplitude 380.8-day radial velocity (RV) variations in oscillating K2 III star ${\alpha}$ Ari (HD 12929). We do not found the correlation between RV variations and equivalent widths of chromospheric activity indicators ($H{\alpha}$ and CaII 8662 ${\AA}line$). The bisector analysis shows that bisector velocity span (BVS) and RV variations are not strongly correlated with each other. These result suggest that the RV variations could have been produced either by planetary companion or by the surface spots. If this RV variation is indeed caused by a planetary companion, an orbital solution with a period of P = 381 days, a semi-amplitude of K = 41 m/s, and an eccentricity of e = 0.25 fits the data best. Assuming a possible stellar mass of $M_{\bigstar} = 1.4-5.6 M\odot$, we estimate the minimum mass for the companion of m sini = 1.8-4.5 $M_{Jup}$ with an orbital semi-major axis of 1.2-1.9 AU. If confirmed, our finding gives a support to search for exoplanets around giant stars with multi-periodic oscillations.

• 천문학회보
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• 제42권1호
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• pp.42.4-43
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• 2017

We investigate the long-period radial velocity (RV) variations for M giant HD 18438 and K giant HD 158996 using the high-resolution Bohyunsan Observatory Echelle Spectrograph at the 1.8m telescope of Bohyunsan Optical Astronomy Observatory in Korea. These two target stars are important because HD 18438 is the largest star and HD 158996 is the brightest star for exoplantary system candidate so we can understarnd how evolved stars affect planets by researching these stars. We calculated precise RV measurements of 38 and 24 spectra from November 2010 to January 2017 and June 2010 to January 2017, respectively. We dreived the RV variation period for 719.0 days of HD 18438, 775.6 days for HD 158996. We conclude that the RV variation of HD 158996 is caused by planetary companion which has the mass of 14.7 MJup, semi-major axis of 2.2 AU, and eccentricity of 0.27 assuming the stellar mass of $2.34M{\odot}$. On the other hand, the origin of RV variation of HD 18438 with period of 719.0 days is still uncertain. It might be caused by stellar chromospheric activity or planetary companion, so more observations and tests are required.

• 천문학회보
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• 제36권2호
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• pp.140.2-140.2
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• 2011

We present high-resolution radial velocity (RV) measurements of K2 giant HD 66141 from December 2003 to January 2011 using the fiber-fed Bohyunsan Observatory Echelle Spectrograph (BOES) at Bohyunsan Optical Astronomy Observatory (BOAO). We find that the RV measurements for HD 66141 exhibit a periodic variation of 480 days with a semi-amplitude of 146 m/s. We do not find the correlation between RV variations and a chromospheric activity indicator (H line). The Hipparcos photometry as well as bisector velocity span (BVS) also do not show any obvious correlations with RV variations. Thus, Keplerian motion is the most likely explanation, which suggests that the RV variations arise from an orbital motion. Assuming a possible stellar mass of 1.5 $M{\odot}$, for HD 66141, we obtain a minimum mass for the planetary companion of 7.4 MJup with an orbital semi-major axis of 1.4 AU, and an eccentricity of 0.07. We support that planet occurrence rate around evolved stars is more than 10 % (Dollinger et al. 2009) as well as more massive stars do form significantly more massive planetary companions (Johnson et al. 2007; Lovis & Mayor 2007; Dollinger et al. 2009).

• 천문학회지
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• 제47권2호
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• pp.69-76
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• 2014

We report the detection of an exoplanet candidate in orbit around ${\sigma}$ Persei from a radial velocity (RV) survey. The system exhibits periodic RV variations of $579.8{\pm}2.4$ days. The purpose of the survey is to search for low-amplitude and long-period RV variations in giants and examine the origin of the variations using the fiber-fed Bohyunsan Observatory Echelle Spectrograph installed at the 1.8-m telescope of Bohyunsan Optical Astronomy Observatory in Korea. We present high-accuracy RV measurements of ${\sigma}$ Per made from December 2003 to January 2014. We argue that the RV variations are not related to the surface inhomogeneities but instead a Keplerian motion of the planetary companion is the most likely explanation. Assuming a stellar mass of $2.25{\pm}0.5$ $M_{\odot}$, we obtain a minimum planetary companion mass of $6.5{\pm}1.0$ $M_{Jup}$, with an orbital semi-major axis of $1.8{\pm}0.1$ AU, and an eccentricity of $0.3{\pm}0.1$ around ${\sigma}$ Per.

• Journal of Microbiology and Biotechnology
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• 제31권8호
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• pp.1175-1182
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• 2021

We investigated the effect of bovine lactoferricin (Lfcin-B), a peptide derived from bovine lactoferrin, on activation of intestinal epithelial cells in IEC-6 intestinal cell, and protection against in vivo rotavirus (RV) infection. Treatment with Lfcin-B significantly enhanced the growth of IEC-6 cells and increased their capacity for attachment and spreading in culture plates. Also, Lfcin-B synergistically augmented the binding of IEC-6 cells to laminin, a component of the extracellular matrix (ECM). In the analysis of the intracellular mechanism related to Lfcin-B-induced activation of IEC-6 cells, this peptide upregulated tyrosine-dependent phosphorylation of focal adhesion kinase (FAK) and paxillin, which are intracellular proteins associated with cell adhesion, spreading, and signal transduction during cell activation. An experiment using synthetic peptides with various sequences of amino acids revealed that a sequence of 9 amino acids (FKCRRWQWR) corresponding to 17-25 of the N-terminus of Lfcin-B is responsible for the epithelial cell activation. In an in vivo experiment, treatment with Lfcin-B one day before RV infection effectively prevented RV-induced diarrhea and significantly reduced RV titers in the bowels of infected mice. These results suggest that Lfcin-B plays meaningful roles in the maintenance and repair of intestinal mucosal tissues, as well as in protecting against intestinal infection by RV. Collectively, Lfcin-B is a promising candidate with potential applications in drugs or functional foods beneficial for intestinal health and mucosal immunity.

• Nuclear Engineering and Technology
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• 제53권12호
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• pp.4003-4013
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• 2021

During the long-term cooling (LTC) phase of a loss-of-coolant accident (LOCA) in a pressurized water reactor (PWR), water is supplied from the containment sump to the reactor coolant system (RCS) by the flooded sump water to the Reactor Vessel (RV) through the broken pipes. As part of the technical efforts for resolving GSI-191 [( Reid and Crytzer, May. 2007) 1, consideration is needed for the consequences of debris penetrating the sump screen and propagating downstream into the RV. Injection of debris (fiberglass) into the RV during the LTC recirculation phase needs special attention to assure that reactor core cooling is maintained. The point of concern is the potential for debris to adversely affect the reactor core flow paths or heat transfer [2]. However, all the experiments for proving the coolability of RV have been done with the assumption of the most of debris would be transferred to the RV and the bottom nozzle of the FAs. The purpose of the tests is to quantify the amount of the debris that would be accumulated at the lower plenum and the debris that passes through the FAs since non-conservatism of other researches assumptions that have been used in the past experimental or analytical programs.

• 반도체디스플레이기술학회지
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• 제23권2호
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• pp.76-81
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• 2024

UC Berkeley developed RISC-V, which is an open-source Instruction Set Architecture. This paper proposes a 32-bit 6-stage pipeline architecture based on the RV32I RSIC-V. The performance of the proposed 6-stage pipeline architecture is compared with the existing 32-bit 5-stage pipeline architecture also based on the RV32I processor ISA to determine the impact of the number of pipeline stages on performance. The RISC-V processor is designed in Verilog-HDL and implemented using Quartus Prime 20.1. To compare performance the Dhrystone benchmark is used. Subsequently, peripherals such as GPIO, TIMER, and UART are connected to verify operation through an FPGA. The maximum clock frequency for the 5-stage pipeline processor is 42.02 MHz, while for the 6-stage pipeline processor, it was 49.9MHz, representing an 18.75% increase.

• Clinical and Experimental Pediatrics
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• 제53권3호
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• pp.373-379
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• 2010

목 적 : 급성 하기도 감염으로 입원하는 소아에서 최근 알려진 hRV C 및 hBoV를 포함하여 13종 호흡기 바이러스의 임상 양상 및 역학을 알아보고자 하였다. 방 법 : 2008년 5월부터 2009년 4월까지 충북대학교병원 소아과에 급성 하기도 감염으로 입원한 소아 중 325명을 대상으로 비인두 흡인물에서 multiplex RT-PCR법을 이용하여 총 13종의 바이러스를 검출하였으며, 대상 소아의 의무기록을 검토하였다. 결 과 : 대상 소아 중 270례(83.1%)에서 호흡기 바이러스가 검출되었으며, 혼합 감염은 71례(26.3%)에서 관찰되었다. 바이러스 검출 빈도는 RSV 108례(33.2%), hRV 62례(19.1%), Flu A 55례(16.9%), hMPV 50례(15.4%), PIV 27례(8.3%), hBoV 26례(8.0%), ADV 19례(5.8%), hCoV 7례(2.2%)였다. 임상진단은 세기관지염 37.5%, 폐렴 34.5%, 급성 천식 악화 20.9%, 크룹 7.1%이었으며, 세기관지염과 폐렴으로 진단된 소아에서 가장 높은 빈도로 검출된 호흡기 바이러스는 RSV, hRV, hMPV, Flu A였다. Flu A와 hRV는 3세 이상의 천식 악화로 진단된 소아에서 가장 높은 빈도로 검출되었다. hRV A와 hRV C는 각각 48명(14.8%)와 14명(4.3%)에서 검출되었으며, hRV C가 검출된 소아의 평균 연령은 $4.1{\pm}3.5$세로 hRV A가 검출된 소아에서의 $1.7{\pm}2.3$세에 비해 유의하게 높았다(P =0.009). hBoV는 세기관지염 또는 폐렴으로 진단된 소아에서 주로 검출되었고, 이들의 평균 연령은 $2.3{\pm}3.4$세였다. 결 론 : 본 연구에서는 한국 소아에서 13종의 바이러스에 의한 하기도 감염의 양상을 관찰하였다. 소아 하기도 감염에서 새로 알려진 바이러스들의 역할을 명확히 알기 위해서는 향후 지속적인 연구가 필요하다.

• 대한전기학회:학술대회논문집
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• 대한전기학회 2009년도 제40회 하계학술대회
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• pp.171_172
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• 2009

본 논문에서는 EMTP-RV를 이용하여 초전도 케이블과 보호기기를 모델링 하였고, 고장 발생 시 케이블에 발생하는 ��치 현상을 분석하였다. 그리고 계통 적용 시 초전도 케이블을 모선으로 사용하고 보호협조를 분석하였다.

• 대한전기학회:학술대회논문집
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• 대한전기학회 2008년도 추계학술대회 논문집 전력기술부문
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• pp.157-159
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• 2008

This paper describes modeling and analysis of magnetic inrush for a 765kV transformer using EMTP-RV. EMTP-RV generates the core flux and thus helps show the behavior of the core, i.e. hysteresis characteristics. The results of three kinds of the magnetic inrush such as initial inrush, sympathetic inrush, and recovery inrush are included. This modelling can help the design of a protection relay for a transformer.